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hera (minor planet designation: 103 hera) is a moderately large main-belt asteroid with an orbital period of 4.44 years.it was discovered by canadian-american astronomer james craig watson on september 7, 1868, and named after hera, queen and fifth in power of the olympian gods in greek mythology.this is a stony s-type asteroid with a silicate surface composition.photometric observations made in 2010 at the organ mesa observatory at las cruces, new mexico, and the hunters hill observatory at ngunnawal, australian capital territory, give a synodic rotation period of 23.740±0.001 h. the bimodal light curve shows a maximum brightness variation of 0.45 ± 0.03 in magnitude.measurements made with the iras observatory give a diameter of 91.58±4.14 km and a geometric albedo of 0.19±0.02.by comparison, the mips photometer on the spitzer space telescope gives a diameter of 88.30±8.51 km and a geometric albedo of 0.20±0.04.when the asteroid was observed occulting a star, the chords showed a diameter of 89.1±1.1 km. | leptostracous | azotous | detecter | no related information |
aaron turner (born november 5, 1977) is an american musician, singer, graphic artist, and founder of label hydra head records.he is most widely known for his role as guitarist and vocalist for the post-metal bands sumac and isis, while also participating in several other bands and projects such as old man gloom, lotus eaters and split cranium, a collaboration with jussi lehtisalo of finnish band circle who toured with isis in 2009.raised in new mexico, turner moved to the boston area, where he attended art school and formed isis and hydra head.in june 2003, turner moved operations of both the band and label to los angeles, california.turner now resides in vashon, wa which is also the base of operations for hydra head and his various other activities.in partnership with his wife faith coloccia, turner founded another record label, sige, in march 2011.it has gone on to release material from his musical collaboration with coloccia, mamiffer.sige is distributed by the business.at an early age, his family moved to new mexico, where he was raised.his mother was a teacher 'who taught a progressive curriculum' and his father an author, 'mainly [of] non-fiction'.turner describes his upbringing, surrounded by his parents' writer, artist and photographer friends, as 'creatively nurturing'.at age 17, he started a company that sold rare punk rock records via mail-order.he later moved to boston to attend art school at the school of the museum of fine arts, and in 1995 began releasing music.by 1997, the hydra head label was becoming a respectable small record label.turner describes his early industriousness as being motivated in part by boredom: i grew up in new mexico, and there wasn't a whole lot as far as youth culture is concerned.especially when i started to get interested in straight edge and wasn't doing drugs anymore, there was really nothing for me to do.so that was like a big reason for me, i suppose, to become really productive.also, i've never been a really social person.so there's not a lot of time taken up by my social life.and music has always been a very very big part of my life.i guess just a combination of those factors is why everything got started so early.around 1997–99, turner was living with future isis bassist and co-founder jeff caxide; until this point, he had been a member of the bands union suit and hollomen.isis was formed in 1997 out of a dissatisfaction with said bands' musical direction and turner and caxide's respective degrees of creative control.in mid-2009, turner moved from los angeles, where both isis and hydra head records were based at the time, to seattle with his then-girlfriend, faith coloccia; they went on to wed in september of the same year.he has also acquired a custom guitar from the electrical guitar company (as did fellow isis guitarist michael gallagher).in the past, turner has also used a gibson les paul standard, prs ce24, and has played through sunn, mesa boogie, and mackie amplifiers.when playing with isis, turner and his fellow guitarists usually tuned their instruments (low to high) b-f#-b-e-g#-b, to achieve a heavier sound.they also used other tunings, though less frequently, such as f# (octave below)-f#-b-e-g#-b.in 2016, turner described the live rig he used with sumac as consisting of two custom-built guitars from the electrical guitar company.both have lucite bodies and aluminum necks, and custom-wound wide frequency range pickups.the newer of the two—a prototype for a signature model—has a slightly flatter fingerboard radius than the older instrument. | aaron turner | associatedband/associatedmusicalartist | twilight band <tsp> aaron turner | associatedband/associatedmusicalartist | greymachine <tsp> aaron turner | genre | black metal <tsp> aaron turner | origin | united states <tsp> aaron turner | activeyearsstartyear | 1995 | no related information |
the aston martin v8 is a grand tourer manufactured by aston martin in the united kingdom from 1969 to 1989.as with all traditional aston martins, it was entirely handbuilt – with each car requiring 1,200 man-hours to finish.aston martin were looking to replace the db6 model and had designed a larger, more modern looking car.the engine was not ready, however, so in 1967 the company released the dbs with the straight-six vantage engine from the db6.two years later, tadek marek's v8 was ready, and aston released the dbs v8.with the demise of the straight-six vantage in 1973, the dbs v8, now restyled and called simply the aston martin v8, became the company's mainstream car for nearly two decades.it was eventually retired in favour of the virage in 1989.though the body and name was shared with the six-cylinder dbs, the v8 sold for much more.the body was a modern reinterpretation of the traditional aston martin look, with a squared-off grille and four headlights (william towns admitted that the rear quarters were 'borrowed' from the early ford mustang).distinguishing features of the v8 model are the larger front air dam, 225/70vr15 tyres and lack of wire wheels, though some six-cylinder dbs cars also used the v8's alloy wheels.the tail lights were taken from the hillman hunter.a road test report of the time noted that the car had gained 250 lb (113 kg) in weight with the fitting of the v8 in place of the previously used six-cylinder unit, despite the manufacturer's assurance that the engine weighed only 30 lb (14 kg) more than the older straight-six.other contributions to the weight gain included heavier ventilated brake discs, air conditioning, fatter tyres, a new and stronger zf gearbox as well as some extra bodywork beneath the front bumper.marek's v8 engine displaced 5,340 cc (5.3 l; 325.9 cu in) and used bosch fuel injection.output was not officially released, but estimates center around 315 hp (235 kw).the dbs v8 could reach 100 km/h (62 mph) in 7.1 seconds and had a top speed of 242 km/h (150 mph).402 dbs v8s were built.a dbs v8 was planned to be used by roger moore's character brett sinclair in the television show, the persuaders!but no v8 car was available at that time so a six-cylinder dbs was modified to look like a v8 model for use in the show.it is based on a dbs v8 and two cars were commissioned by the tobacco company w.o.wills to promote their new premium brand of cigarettes: one show car with chassis number dbsv8/10380/r and one road going car with chassis number dbsv8/10381/rc.a third 'replica' car was commissioned by a private party.visual differences included twin quartz-halogen headlights and a mesh grille, a front design which was to last until the end of production in 1989.am v8 cars, produced from may 1972 through july 1973, used a similar engine to the dbs v8, albeit with bosch fuel injection rather than the earlier carburetors.just 288 series 2 cars were built.although david brown had left the company, he had overseen development of this model.the first 34 cars still carried leftover 'dbs v8' badging.these cars are distinguished by a taller hood scoop to accommodate four twin-choke (two-barrel) weber carbs.the car produced 310 hp (231 kw; 314 ps) and could reach 60 mph (97 km/h) in 6.1 seconds with an automatic transmission or 5.7 with a manual.performance suffered with emissions regulations, falling to 288 hp (215 kw; 292 ps) in 1976.the next year, a more powerful 'stage 1' engine with new camshafts and exhaust brought it up to 305 hp (227 kw; 309 ps).these cars either fitted 225/70vr15 avon turbospeed or 235/70vr15 turbospeed rolls-royce tyre on the auto models or the 255/60r15 pirelli cinturato cn12 off the vantage. | underfrequencies | gabs | vulgarizations | no related information |
hera (minor planet designation: 103 hera) is a moderately large main-belt asteroid with an orbital period of 4.44 years.it was discovered by canadian-american astronomer james craig watson on september 7, 1868, and named after hera, queen and fifth in power of the olympian gods in greek mythology.this is a stony s-type asteroid with a silicate surface composition.photometric observations made in 2010 at the organ mesa observatory at las cruces, new mexico, and the hunters hill observatory at ngunnawal, australian capital territory, give a synodic rotation period of 23.740±0.001 h. the bimodal light curve shows a maximum brightness variation of 0.45 ± 0.03 in magnitude.measurements made with the iras observatory give a diameter of 91.58±4.14 km and a geometric albedo of 0.19±0.02.by comparison, the mips photometer on the spitzer space telescope gives a diameter of 88.30±8.51 km and a geometric albedo of 0.20±0.04.when the asteroid was observed occulting a star, the chords showed a diameter of 89.1±1.1 km. | 103 hera | discoverer | james craig watson <tsp> james craig watson | almamater | university of michigan <tsp> 103 hera | absolutemagnitude | 766 <tsp> james craig watson | nationality | canada <tsp> james craig watson | deathplace | madison wisconsin | it was discovered by canadian-american astronomer james craig watson on september 7, 1868, and named after hera, queen and fifth in power of the olympian gods in greek mythology. |
the aston martin virage is an automobile produced by british luxury automobile manufacturer aston martin as a replacement for its v8 models.introduced at the birmingham motor show in 1988, it was joined by the high-performance vantage in 1993, and then the name of the base model was changed to v8 coupe in 1996.the v8-powered model was intended as the company's flagship model, with the 6-cylinder db7, introduced in 1994, positioned below it as an entry-level model.although the db7 became available with a v12 engine and claimed a performance advantage, the virage remained the exclusive, expensive and hand-built flagship of the aston martin range.it was replaced in 2000 with the vanquish.by the end of the 2000 model year, 1,050 cars in total had been produced.the v8 vantage name reappeared on a new entry-level model in 2005.a new virage model was introduced at the 2011 geneva motor show, to fit into the middle of aston martin's then current lineup but was discontinued in 2012 due to many similarities between the brand's other models.the virage was more similar in design language to the lagonda than the v8 it replaced.indeed, the chassis was an evolution of the lagonda's, with a de dion tube rear suspension, located by triangulated radius rods and a watts linkage, and a double wishbone unit at the front.to cut costs, many of the less-important pieces came from other companies, as had been the case for aston martin automobiles of the past.the sleek headlights and taillights were sourced from the audi 200 and the volkswagen scirocco respectively, while general motors, jaguar, citroën and ford provided the steering column, climate control panel, wing mirrors and dash switches.in fact, ford had purchased aston martin and jaguar shortly before the virage debuted and it became the first model to be introduced under the new ownership.the virage was a large, heavy car in spite of its all-aluminium body, but the 32-valve 5.3 l (5,340 cc) v8 engine's 494 n⋅m (364 lb⋅ft) torque elevated its performance to near sports car levels.'acceleration just never seems to run out', claimed sports car international during a first test.they also praised the 'eager and quicker revving' nature of the 330 hp (246 kw; 335 ps) engine with its callaway-designed heads and weber-marelli fuel injection.'nothing sounds quite like an aston v8,' they concluded.the 1,790 kg (3,946 lb) car could attain a top-speed of 254 km/h (158 mph).the automatic variant could accelerate to 97 km/h (60 mph) from a standing start in about 6.5 seconds (7.4 seconds for the manual version).an engine power upgrade to 350 hp (261 kw; 355 ps) was announced at the 1996 geneva motor show.english actor rowan atkinson owned virage coupé chassis 50010 which featured on the front cover of car may 1990.in the article he commented how the modern climate control system provided heating efficiency beyond the veteran aston martin driver's dreams and could not believe warm air would emanate from the footwell within 90 seconds of start up.this car also appeared in the beginning of his 1991 tv series the driven man.other celebrity owners included lennox lewis, elton john and chris eubank.the five-speed zf friedrichshafen manual was fitted to about forty percent of the cars produced.the more popular automatic option was the chrysler three-speed torqueflite transmission.for the 1993 model year, the three-speed unit was replaced by a four-speed automatic unit.the six-speed manual from the vantage also became optional at the end of the virage's production run.as the name implies, the centerpiece of the conversion was a bored and stroked 6.3 l (6,347 cc) v8 derived from the amr1 racing car. | aston martin virage | relatedmeanoftransportation | aston martin dbs <tsp> aston martin v8 | assembly | newport pagnell <tsp> aston martin v8 | engine | 53 litres <tsp> aston martin v8 | successor | aston martin virage <tsp> aston martin dbs | manufacturer | aston martin | the aston martin virage is an automobile produced by british luxury automobile manufacturer aston martin as a replacement for its v8 models.although the db7 became available with a v12 engine and claimed a performance advantage, the virage remained the exclusive, expensive and hand-built flagship of the aston martin range.a new virage model was introduced at the 2011 geneva motor show, to fit into the middle of aston martin's then current lineup but was discontinued in 2012 due to many similarities between the brand's other models.to cut costs, many of the less-important pieces came from other companies, as had been the case for aston martin automobiles of the past.in fact, ford had purchased aston martin and jaguar shortly before the virage debuted and it became the first model to be introduced under the new ownership.'nothing sounds quite like an aston v8,' they concluded.in the article he commented how the modern climate control system provided heating efficiency beyond the veteran aston martin driver's dreams and could not believe warm air would emanate from the footwell within 90 seconds of start up. |
aaron turner (born november 5, 1977) is an american musician, singer, graphic artist, and founder of label hydra head records.he is most widely known for his role as guitarist and vocalist for the post-metal bands sumac and isis, while also participating in several other bands and projects such as old man gloom, lotus eaters and split cranium, a collaboration with jussi lehtisalo of finnish band circle who toured with isis in 2009.raised in new mexico, turner moved to the boston area, where he attended art school and formed isis and hydra head.in june 2003, turner moved operations of both the band and label to los angeles, california.turner now resides in vashon, wa which is also the base of operations for hydra head and his various other activities.in partnership with his wife faith coloccia, turner founded another record label, sige, in march 2011.it has gone on to release material from his musical collaboration with coloccia, mamiffer.sige is distributed by the business.at an early age, his family moved to new mexico, where he was raised.his mother was a teacher 'who taught a progressive curriculum' and his father an author, 'mainly [of] non-fiction'.turner describes his upbringing, surrounded by his parents' writer, artist and photographer friends, as 'creatively nurturing'.at age 17, he started a company that sold rare punk rock records via mail-order.he later moved to boston to attend art school at the school of the museum of fine arts, and in 1995 began releasing music.by 1997, the hydra head label was becoming a respectable small record label.turner describes his early industriousness as being motivated in part by boredom: i grew up in new mexico, and there wasn't a whole lot as far as youth culture is concerned.especially when i started to get interested in straight edge and wasn't doing drugs anymore, there was really nothing for me to do.so that was like a big reason for me, i suppose, to become really productive.also, i've never been a really social person.so there's not a lot of time taken up by my social life.and music has always been a very very big part of my life.i guess just a combination of those factors is why everything got started so early.around 1997–99, turner was living with future isis bassist and co-founder jeff caxide; until this point, he had been a member of the bands union suit and hollomen.isis was formed in 1997 out of a dissatisfaction with said bands' musical direction and turner and caxide's respective degrees of creative control.in mid-2009, turner moved from los angeles, where both isis and hydra head records were based at the time, to seattle with his then-girlfriend, faith coloccia; they went on to wed in september of the same year.he has also acquired a custom guitar from the electrical guitar company (as did fellow isis guitarist michael gallagher).in the past, turner has also used a gibson les paul standard, prs ce24, and has played through sunn, mesa boogie, and mackie amplifiers.when playing with isis, turner and his fellow guitarists usually tuned their instruments (low to high) b-f#-b-e-g#-b, to achieve a heavier sound.they also used other tunings, though less frequently, such as f# (octave below)-f#-b-e-g#-b.in 2016, turner described the live rig he used with sumac as consisting of two custom-built guitars from the electrical guitar company.both have lucite bodies and aluminum necks, and custom-wound wide frequency range pickups.the newer of the two—a prototype for a signature model—has a slightly flatter fingerboard radius than the older instrument. | aaron turner | associatedband/associatedmusicalartist | twilight band <tsp> aaron turner | associatedband/associatedmusicalartist | greymachine <tsp> aaron turner | genre | black metal <tsp> aaron turner | origin | united states <tsp> aaron turner | activeyearsstartyear | 1995 | no related information |
hera (minor planet designation: 103 hera) is a moderately large main-belt asteroid with an orbital period of 4.44 years.it was discovered by canadian-american astronomer james craig watson on september 7, 1868, and named after hera, queen and fifth in power of the olympian gods in greek mythology.this is a stony s-type asteroid with a silicate surface composition.photometric observations made in 2010 at the organ mesa observatory at las cruces, new mexico, and the hunters hill observatory at ngunnawal, australian capital territory, give a synodic rotation period of 23.740±0.001 h. the bimodal light curve shows a maximum brightness variation of 0.45 ± 0.03 in magnitude.measurements made with the iras observatory give a diameter of 91.58±4.14 km and a geometric albedo of 0.19±0.02.by comparison, the mips photometer on the spitzer space telescope gives a diameter of 88.30±8.51 km and a geometric albedo of 0.20±0.04.when the asteroid was observed occulting a star, the chords showed a diameter of 89.1±1.1 km. | 103 hera | discoverer | james craig watson <tsp> james craig watson | almamater | university of michigan <tsp> 103 hera | epoch | 2011-08-27 <tsp> james craig watson | nationality | canada <tsp> james craig watson | deathplace | madison wisconsin | it was discovered by canadian-american astronomer james craig watson on september 7, 1868, and named after hera, queen and fifth in power of the olympian gods in greek mythology. |
aaron turner (born november 5, 1977) is an american musician, singer, graphic artist, and founder of label hydra head records.he is most widely known for his role as guitarist and vocalist for the post-metal bands sumac and isis, while also participating in several other bands and projects such as old man gloom, lotus eaters and split cranium, a collaboration with jussi lehtisalo of finnish band circle who toured with isis in 2009.raised in new mexico, turner moved to the boston area, where he attended art school and formed isis and hydra head.in june 2003, turner moved operations of both the band and label to los angeles, california.turner now resides in vashon, wa which is also the base of operations for hydra head and his various other activities.in partnership with his wife faith coloccia, turner founded another record label, sige, in march 2011.it has gone on to release material from his musical collaboration with coloccia, mamiffer.sige is distributed by the business.at an early age, his family moved to new mexico, where he was raised.his mother was a teacher 'who taught a progressive curriculum' and his father an author, 'mainly [of] non-fiction'.turner describes his upbringing, surrounded by his parents' writer, artist and photographer friends, as 'creatively nurturing'.at age 17, he started a company that sold rare punk rock records via mail-order.he later moved to boston to attend art school at the school of the museum of fine arts, and in 1995 began releasing music.by 1997, the hydra head label was becoming a respectable small record label.turner describes his early industriousness as being motivated in part by boredom: i grew up in new mexico, and there wasn't a whole lot as far as youth culture is concerned.especially when i started to get interested in straight edge and wasn't doing drugs anymore, there was really nothing for me to do.so that was like a big reason for me, i suppose, to become really productive.also, i've never been a really social person.so there's not a lot of time taken up by my social life.and music has always been a very very big part of my life.i guess just a combination of those factors is why everything got started so early.around 1997–99, turner was living with future isis bassist and co-founder jeff caxide; until this point, he had been a member of the bands union suit and hollomen.isis was formed in 1997 out of a dissatisfaction with said bands' musical direction and turner and caxide's respective degrees of creative control.in mid-2009, turner moved from los angeles, where both isis and hydra head records were based at the time, to seattle with his then-girlfriend, faith coloccia; they went on to wed in september of the same year.he has also acquired a custom guitar from the electrical guitar company (as did fellow isis guitarist michael gallagher).in the past, turner has also used a gibson les paul standard, prs ce24, and has played through sunn, mesa boogie, and mackie amplifiers.when playing with isis, turner and his fellow guitarists usually tuned their instruments (low to high) b-f#-b-e-g#-b, to achieve a heavier sound.they also used other tunings, though less frequently, such as f# (octave below)-f#-b-e-g#-b.in 2016, turner described the live rig he used with sumac as consisting of two custom-built guitars from the electrical guitar company.both have lucite bodies and aluminum necks, and custom-wound wide frequency range pickups.the newer of the two—a prototype for a signature model—has a slightly flatter fingerboard radius than the older instrument. | aaron turner | associatedband/associatedmusicalartist | twilight band <tsp> aaron turner | associatedband/associatedmusicalartist | lotus eaters band <tsp> aaron turner | genre | black metal <tsp> aaron turner | instrument | singing <tsp> black metal | musicfusiongenre | death metal | he is most widely known for his role as guitarist and vocalist for the post-metal bands sumac and isis, while also participating in several other bands and projects such as old man gloom, lotus eaters and split cranium, a collaboration with jussi lehtisalo of finnish band circle who toured with isis in 2009. |
hera (minor planet designation: 103 hera) is a moderately large main-belt asteroid with an orbital period of 4.44 years.it was discovered by canadian-american astronomer james craig watson on september 7, 1868, and named after hera, queen and fifth in power of the olympian gods in greek mythology.this is a stony s-type asteroid with a silicate surface composition.photometric observations made in 2010 at the organ mesa observatory at las cruces, new mexico, and the hunters hill observatory at ngunnawal, australian capital territory, give a synodic rotation period of 23.740±0.001 h. the bimodal light curve shows a maximum brightness variation of 0.45 ± 0.03 in magnitude.measurements made with the iras observatory give a diameter of 91.58±4.14 km and a geometric albedo of 0.19±0.02.by comparison, the mips photometer on the spitzer space telescope gives a diameter of 88.30±8.51 km and a geometric albedo of 0.20±0.04.when the asteroid was observed occulting a star, the chords showed a diameter of 89.1±1.1 km. | 103 hera | discoverer | james craig watson <tsp> james craig watson | almamater | university of michigan <tsp> 103 hera | epoch | 2011-08-27 <tsp> james craig watson | nationality | canada <tsp> james craig watson | deathplace | madison wisconsin | it was discovered by canadian-american astronomer james craig watson on september 7, 1868, and named after hera, queen and fifth in power of the olympian gods in greek mythology. |
the aston martin virage is an automobile produced by british luxury automobile manufacturer aston martin as a replacement for its v8 models.introduced at the birmingham motor show in 1988, it was joined by the high-performance vantage in 1993, and then the name of the base model was changed to v8 coupe in 1996.the v8-powered model was intended as the company's flagship model, with the 6-cylinder db7, introduced in 1994, positioned below it as an entry-level model.although the db7 became available with a v12 engine and claimed a performance advantage, the virage remained the exclusive, expensive and hand-built flagship of the aston martin range.it was replaced in 2000 with the vanquish.by the end of the 2000 model year, 1,050 cars in total had been produced.the v8 vantage name reappeared on a new entry-level model in 2005.a new virage model was introduced at the 2011 geneva motor show, to fit into the middle of aston martin's then current lineup but was discontinued in 2012 due to many similarities between the brand's other models.the virage was more similar in design language to the lagonda than the v8 it replaced.indeed, the chassis was an evolution of the lagonda's, with a de dion tube rear suspension, located by triangulated radius rods and a watts linkage, and a double wishbone unit at the front.to cut costs, many of the less-important pieces came from other companies, as had been the case for aston martin automobiles of the past.the sleek headlights and taillights were sourced from the audi 200 and the volkswagen scirocco respectively, while general motors, jaguar, citroën and ford provided the steering column, climate control panel, wing mirrors and dash switches.in fact, ford had purchased aston martin and jaguar shortly before the virage debuted and it became the first model to be introduced under the new ownership.the virage was a large, heavy car in spite of its all-aluminium body, but the 32-valve 5.3 l (5,340 cc) v8 engine's 494 n⋅m (364 lb⋅ft) torque elevated its performance to near sports car levels.'acceleration just never seems to run out', claimed sports car international during a first test.they also praised the 'eager and quicker revving' nature of the 330 hp (246 kw; 335 ps) engine with its callaway-designed heads and weber-marelli fuel injection.'nothing sounds quite like an aston v8,' they concluded.the 1,790 kg (3,946 lb) car could attain a top-speed of 254 km/h (158 mph).the automatic variant could accelerate to 97 km/h (60 mph) from a standing start in about 6.5 seconds (7.4 seconds for the manual version).an engine power upgrade to 350 hp (261 kw; 355 ps) was announced at the 1996 geneva motor show.english actor rowan atkinson owned virage coupé chassis 50010 which featured on the front cover of car may 1990.in the article he commented how the modern climate control system provided heating efficiency beyond the veteran aston martin driver's dreams and could not believe warm air would emanate from the footwell within 90 seconds of start up.this car also appeared in the beginning of his 1991 tv series the driven man.other celebrity owners included lennox lewis, elton john and chris eubank.the five-speed zf friedrichshafen manual was fitted to about forty percent of the cars produced.the more popular automatic option was the chrysler three-speed torqueflite transmission.for the 1993 model year, the three-speed unit was replaced by a four-speed automatic unit.the six-speed manual from the vantage also became optional at the end of the virage's production run.as the name implies, the centerpiece of the conversion was a bored and stroked 6.3 l (6,347 cc) v8 derived from the amr1 racing car. | santon | isotria | proliferates <tsp> santon | racahout | syphiliphobia | no related information |
aaron turner (born november 5, 1977) is an american musician, singer, graphic artist, and founder of label hydra head records.he is most widely known for his role as guitarist and vocalist for the post-metal bands sumac and isis, while also participating in several other bands and projects such as old man gloom, lotus eaters and split cranium, a collaboration with jussi lehtisalo of finnish band circle who toured with isis in 2009.raised in new mexico, turner moved to the boston area, where he attended art school and formed isis and hydra head.in june 2003, turner moved operations of both the band and label to los angeles, california.turner now resides in vashon, wa which is also the base of operations for hydra head and his various other activities.in partnership with his wife faith coloccia, turner founded another record label, sige, in march 2011.it has gone on to release material from his musical collaboration with coloccia, mamiffer.sige is distributed by the business.at an early age, his family moved to new mexico, where he was raised.his mother was a teacher 'who taught a progressive curriculum' and his father an author, 'mainly [of] non-fiction'.turner describes his upbringing, surrounded by his parents' writer, artist and photographer friends, as 'creatively nurturing'.at age 17, he started a company that sold rare punk rock records via mail-order.he later moved to boston to attend art school at the school of the museum of fine arts, and in 1995 began releasing music.by 1997, the hydra head label was becoming a respectable small record label.turner describes his early industriousness as being motivated in part by boredom: i grew up in new mexico, and there wasn't a whole lot as far as youth culture is concerned.especially when i started to get interested in straight edge and wasn't doing drugs anymore, there was really nothing for me to do.so that was like a big reason for me, i suppose, to become really productive.also, i've never been a really social person.so there's not a lot of time taken up by my social life.and music has always been a very very big part of my life.i guess just a combination of those factors is why everything got started so early.around 1997–99, turner was living with future isis bassist and co-founder jeff caxide; until this point, he had been a member of the bands union suit and hollomen.isis was formed in 1997 out of a dissatisfaction with said bands' musical direction and turner and caxide's respective degrees of creative control.in mid-2009, turner moved from los angeles, where both isis and hydra head records were based at the time, to seattle with his then-girlfriend, faith coloccia; they went on to wed in september of the same year.he has also acquired a custom guitar from the electrical guitar company (as did fellow isis guitarist michael gallagher).in the past, turner has also used a gibson les paul standard, prs ce24, and has played through sunn, mesa boogie, and mackie amplifiers.when playing with isis, turner and his fellow guitarists usually tuned their instruments (low to high) b-f#-b-e-g#-b, to achieve a heavier sound.they also used other tunings, though less frequently, such as f# (octave below)-f#-b-e-g#-b.in 2016, turner described the live rig he used with sumac as consisting of two custom-built guitars from the electrical guitar company.both have lucite bodies and aluminum necks, and custom-wound wide frequency range pickups.the newer of the two—a prototype for a signature model—has a slightly flatter fingerboard radius than the older instrument. | dimout | rovingly | giggit | no related information |
the aston martin virage is an automobile produced by british luxury automobile manufacturer aston martin as a replacement for its v8 models.introduced at the birmingham motor show in 1988, it was joined by the high-performance vantage in 1993, and then the name of the base model was changed to v8 coupe in 1996.the v8-powered model was intended as the company's flagship model, with the 6-cylinder db7, introduced in 1994, positioned below it as an entry-level model.although the db7 became available with a v12 engine and claimed a performance advantage, the virage remained the exclusive, expensive and hand-built flagship of the aston martin range.it was replaced in 2000 with the vanquish.by the end of the 2000 model year, 1,050 cars in total had been produced.the v8 vantage name reappeared on a new entry-level model in 2005.a new virage model was introduced at the 2011 geneva motor show, to fit into the middle of aston martin's then current lineup but was discontinued in 2012 due to many similarities between the brand's other models.the virage was more similar in design language to the lagonda than the v8 it replaced.indeed, the chassis was an evolution of the lagonda's, with a de dion tube rear suspension, located by triangulated radius rods and a watts linkage, and a double wishbone unit at the front.to cut costs, many of the less-important pieces came from other companies, as had been the case for aston martin automobiles of the past.the sleek headlights and taillights were sourced from the audi 200 and the volkswagen scirocco respectively, while general motors, jaguar, citroën and ford provided the steering column, climate control panel, wing mirrors and dash switches.in fact, ford had purchased aston martin and jaguar shortly before the virage debuted and it became the first model to be introduced under the new ownership.the virage was a large, heavy car in spite of its all-aluminium body, but the 32-valve 5.3 l (5,340 cc) v8 engine's 494 n⋅m (364 lb⋅ft) torque elevated its performance to near sports car levels.'acceleration just never seems to run out', claimed sports car international during a first test.they also praised the 'eager and quicker revving' nature of the 330 hp (246 kw; 335 ps) engine with its callaway-designed heads and weber-marelli fuel injection.'nothing sounds quite like an aston v8,' they concluded.the 1,790 kg (3,946 lb) car could attain a top-speed of 254 km/h (158 mph).the automatic variant could accelerate to 97 km/h (60 mph) from a standing start in about 6.5 seconds (7.4 seconds for the manual version).an engine power upgrade to 350 hp (261 kw; 355 ps) was announced at the 1996 geneva motor show.english actor rowan atkinson owned virage coupé chassis 50010 which featured on the front cover of car may 1990.in the article he commented how the modern climate control system provided heating efficiency beyond the veteran aston martin driver's dreams and could not believe warm air would emanate from the footwell within 90 seconds of start up.this car also appeared in the beginning of his 1991 tv series the driven man.other celebrity owners included lennox lewis, elton john and chris eubank.the five-speed zf friedrichshafen manual was fitted to about forty percent of the cars produced.the more popular automatic option was the chrysler three-speed torqueflite transmission.for the 1993 model year, the three-speed unit was replaced by a four-speed automatic unit.the six-speed manual from the vantage also became optional at the end of the virage's production run.as the name implies, the centerpiece of the conversion was a bored and stroked 6.3 l (6,347 cc) v8 derived from the amr1 racing car. | aston martin virage | relatedmeanoftransportation | aston martin dbs <tsp> aston martin v8 | assembly | newport pagnell <tsp> aston martin v8 | engine | 53 litres <tsp> aston martin v8 | successor | aston martin virage <tsp> aston martin dbs | manufacturer | aston martin | the aston martin virage is an automobile produced by british luxury automobile manufacturer aston martin as a replacement for its v8 models.although the db7 became available with a v12 engine and claimed a performance advantage, the virage remained the exclusive, expensive and hand-built flagship of the aston martin range.a new virage model was introduced at the 2011 geneva motor show, to fit into the middle of aston martin's then current lineup but was discontinued in 2012 due to many similarities between the brand's other models.to cut costs, many of the less-important pieces came from other companies, as had been the case for aston martin automobiles of the past.in fact, ford had purchased aston martin and jaguar shortly before the virage debuted and it became the first model to be introduced under the new ownership.'nothing sounds quite like an aston v8,' they concluded.in the article he commented how the modern climate control system provided heating efficiency beyond the veteran aston martin driver's dreams and could not believe warm air would emanate from the footwell within 90 seconds of start up. |
hera (minor planet designation: 103 hera) is a moderately large main-belt asteroid with an orbital period of 4.44 years.it was discovered by canadian-american astronomer james craig watson on september 7, 1868, and named after hera, queen and fifth in power of the olympian gods in greek mythology.this is a stony s-type asteroid with a silicate surface composition.photometric observations made in 2010 at the organ mesa observatory at las cruces, new mexico, and the hunters hill observatory at ngunnawal, australian capital territory, give a synodic rotation period of 23.740±0.001 h. the bimodal light curve shows a maximum brightness variation of 0.45 ± 0.03 in magnitude.measurements made with the iras observatory give a diameter of 91.58±4.14 km and a geometric albedo of 0.19±0.02.by comparison, the mips photometer on the spitzer space telescope gives a diameter of 88.30±8.51 km and a geometric albedo of 0.20±0.04.when the asteroid was observed occulting a star, the chords showed a diameter of 89.1±1.1 km. | spencerianism | facto | trefoillike <tsp> spencerianism | baresma | scenic | no related information |
aaron turner (born november 5, 1977) is an american musician, singer, graphic artist, and founder of label hydra head records.he is most widely known for his role as guitarist and vocalist for the post-metal bands sumac and isis, while also participating in several other bands and projects such as old man gloom, lotus eaters and split cranium, a collaboration with jussi lehtisalo of finnish band circle who toured with isis in 2009.raised in new mexico, turner moved to the boston area, where he attended art school and formed isis and hydra head.in june 2003, turner moved operations of both the band and label to los angeles, california.turner now resides in vashon, wa which is also the base of operations for hydra head and his various other activities.in partnership with his wife faith coloccia, turner founded another record label, sige, in march 2011.it has gone on to release material from his musical collaboration with coloccia, mamiffer.sige is distributed by the business.at an early age, his family moved to new mexico, where he was raised.his mother was a teacher 'who taught a progressive curriculum' and his father an author, 'mainly [of] non-fiction'.turner describes his upbringing, surrounded by his parents' writer, artist and photographer friends, as 'creatively nurturing'.at age 17, he started a company that sold rare punk rock records via mail-order.he later moved to boston to attend art school at the school of the museum of fine arts, and in 1995 began releasing music.by 1997, the hydra head label was becoming a respectable small record label.turner describes his early industriousness as being motivated in part by boredom: i grew up in new mexico, and there wasn't a whole lot as far as youth culture is concerned.especially when i started to get interested in straight edge and wasn't doing drugs anymore, there was really nothing for me to do.so that was like a big reason for me, i suppose, to become really productive.also, i've never been a really social person.so there's not a lot of time taken up by my social life.and music has always been a very very big part of my life.i guess just a combination of those factors is why everything got started so early.around 1997–99, turner was living with future isis bassist and co-founder jeff caxide; until this point, he had been a member of the bands union suit and hollomen.isis was formed in 1997 out of a dissatisfaction with said bands' musical direction and turner and caxide's respective degrees of creative control.in mid-2009, turner moved from los angeles, where both isis and hydra head records were based at the time, to seattle with his then-girlfriend, faith coloccia; they went on to wed in september of the same year.he has also acquired a custom guitar from the electrical guitar company (as did fellow isis guitarist michael gallagher).in the past, turner has also used a gibson les paul standard, prs ce24, and has played through sunn, mesa boogie, and mackie amplifiers.when playing with isis, turner and his fellow guitarists usually tuned their instruments (low to high) b-f#-b-e-g#-b, to achieve a heavier sound.they also used other tunings, though less frequently, such as f# (octave below)-f#-b-e-g#-b.in 2016, turner described the live rig he used with sumac as consisting of two custom-built guitars from the electrical guitar company.both have lucite bodies and aluminum necks, and custom-wound wide frequency range pickups.the newer of the two—a prototype for a signature model—has a slightly flatter fingerboard radius than the older instrument. | rechauffe | remainder | judgement | no related information |
the aston martin virage is an automobile produced by british luxury automobile manufacturer aston martin as a replacement for its v8 models.introduced at the birmingham motor show in 1988, it was joined by the high-performance vantage in 1993, and then the name of the base model was changed to v8 coupe in 1996.the v8-powered model was intended as the company's flagship model, with the 6-cylinder db7, introduced in 1994, positioned below it as an entry-level model.although the db7 became available with a v12 engine and claimed a performance advantage, the virage remained the exclusive, expensive and hand-built flagship of the aston martin range.it was replaced in 2000 with the vanquish.by the end of the 2000 model year, 1,050 cars in total had been produced.the v8 vantage name reappeared on a new entry-level model in 2005.a new virage model was introduced at the 2011 geneva motor show, to fit into the middle of aston martin's then current lineup but was discontinued in 2012 due to many similarities between the brand's other models.the virage was more similar in design language to the lagonda than the v8 it replaced.indeed, the chassis was an evolution of the lagonda's, with a de dion tube rear suspension, located by triangulated radius rods and a watts linkage, and a double wishbone unit at the front.to cut costs, many of the less-important pieces came from other companies, as had been the case for aston martin automobiles of the past.the sleek headlights and taillights were sourced from the audi 200 and the volkswagen scirocco respectively, while general motors, jaguar, citroën and ford provided the steering column, climate control panel, wing mirrors and dash switches.in fact, ford had purchased aston martin and jaguar shortly before the virage debuted and it became the first model to be introduced under the new ownership.the virage was a large, heavy car in spite of its all-aluminium body, but the 32-valve 5.3 l (5,340 cc) v8 engine's 494 n⋅m (364 lb⋅ft) torque elevated its performance to near sports car levels.'acceleration just never seems to run out', claimed sports car international during a first test.they also praised the 'eager and quicker revving' nature of the 330 hp (246 kw; 335 ps) engine with its callaway-designed heads and weber-marelli fuel injection.'nothing sounds quite like an aston v8,' they concluded.the 1,790 kg (3,946 lb) car could attain a top-speed of 254 km/h (158 mph).the automatic variant could accelerate to 97 km/h (60 mph) from a standing start in about 6.5 seconds (7.4 seconds for the manual version).an engine power upgrade to 350 hp (261 kw; 355 ps) was announced at the 1996 geneva motor show.english actor rowan atkinson owned virage coupé chassis 50010 which featured on the front cover of car may 1990.in the article he commented how the modern climate control system provided heating efficiency beyond the veteran aston martin driver's dreams and could not believe warm air would emanate from the footwell within 90 seconds of start up.this car also appeared in the beginning of his 1991 tv series the driven man.other celebrity owners included lennox lewis, elton john and chris eubank.the five-speed zf friedrichshafen manual was fitted to about forty percent of the cars produced.the more popular automatic option was the chrysler three-speed torqueflite transmission.for the 1993 model year, the three-speed unit was replaced by a four-speed automatic unit.the six-speed manual from the vantage also became optional at the end of the virage's production run.as the name implies, the centerpiece of the conversion was a bored and stroked 6.3 l (6,347 cc) v8 derived from the amr1 racing car. | aston martin virage | relatedmeanoftransportation | aston martin dbs <tsp> aston martin v8 | assembly | newport pagnell <tsp> aston martin v8 | engine | 53 litres <tsp> aston martin v8 | successor | aston martin virage <tsp> aston martin virage | manufacturer | aston martin | the aston martin virage is an automobile produced by british luxury automobile manufacturer aston martin as a replacement for its v8 models.although the db7 became available with a v12 engine and claimed a performance advantage, the virage remained the exclusive, expensive and hand-built flagship of the aston martin range.a new virage model was introduced at the 2011 geneva motor show, to fit into the middle of aston martin's then current lineup but was discontinued in 2012 due to many similarities between the brand's other models.to cut costs, many of the less-important pieces came from other companies, as had been the case for aston martin automobiles of the past.in fact, ford had purchased aston martin and jaguar shortly before the virage debuted and it became the first model to be introduced under the new ownership.'nothing sounds quite like an aston v8,' they concluded.in the article he commented how the modern climate control system provided heating efficiency beyond the veteran aston martin driver's dreams and could not believe warm air would emanate from the footwell within 90 seconds of start up. |
hera (minor planet designation: 103 hera) is a moderately large main-belt asteroid with an orbital period of 4.44 years.it was discovered by canadian-american astronomer james craig watson on september 7, 1868, and named after hera, queen and fifth in power of the olympian gods in greek mythology.this is a stony s-type asteroid with a silicate surface composition.photometric observations made in 2010 at the organ mesa observatory at las cruces, new mexico, and the hunters hill observatory at ngunnawal, australian capital territory, give a synodic rotation period of 23.740±0.001 h. the bimodal light curve shows a maximum brightness variation of 0.45 ± 0.03 in magnitude.measurements made with the iras observatory give a diameter of 91.58±4.14 km and a geometric albedo of 0.19±0.02.by comparison, the mips photometer on the spitzer space telescope gives a diameter of 88.30±8.51 km and a geometric albedo of 0.20±0.04.when the asteroid was observed occulting a star, the chords showed a diameter of 89.1±1.1 km. | 103 hera | discoverer | james craig watson <tsp> james craig watson | almamater | university of michigan <tsp> james craig watson | nationality | canada <tsp> james craig watson | deathplace | madison wisconsin <tsp> 103 hera | apoapsis | 4371700000 kilometres | it was discovered by canadian-american astronomer james craig watson on september 7, 1868, and named after hera, queen and fifth in power of the olympian gods in greek mythology. |
the aston martin virage is an automobile produced by british luxury automobile manufacturer aston martin as a replacement for its v8 models.introduced at the birmingham motor show in 1988, it was joined by the high-performance vantage in 1993, and then the name of the base model was changed to v8 coupe in 1996.the v8-powered model was intended as the company's flagship model, with the 6-cylinder db7, introduced in 1994, positioned below it as an entry-level model.although the db7 became available with a v12 engine and claimed a performance advantage, the virage remained the exclusive, expensive and hand-built flagship of the aston martin range.it was replaced in 2000 with the vanquish.by the end of the 2000 model year, 1,050 cars in total had been produced.the v8 vantage name reappeared on a new entry-level model in 2005.a new virage model was introduced at the 2011 geneva motor show, to fit into the middle of aston martin's then current lineup but was discontinued in 2012 due to many similarities between the brand's other models.the virage was more similar in design language to the lagonda than the v8 it replaced.indeed, the chassis was an evolution of the lagonda's, with a de dion tube rear suspension, located by triangulated radius rods and a watts linkage, and a double wishbone unit at the front.to cut costs, many of the less-important pieces came from other companies, as had been the case for aston martin automobiles of the past.the sleek headlights and taillights were sourced from the audi 200 and the volkswagen scirocco respectively, while general motors, jaguar, citroën and ford provided the steering column, climate control panel, wing mirrors and dash switches.in fact, ford had purchased aston martin and jaguar shortly before the virage debuted and it became the first model to be introduced under the new ownership.the virage was a large, heavy car in spite of its all-aluminium body, but the 32-valve 5.3 l (5,340 cc) v8 engine's 494 n⋅m (364 lb⋅ft) torque elevated its performance to near sports car levels.'acceleration just never seems to run out', claimed sports car international during a first test.they also praised the 'eager and quicker revving' nature of the 330 hp (246 kw; 335 ps) engine with its callaway-designed heads and weber-marelli fuel injection.'nothing sounds quite like an aston v8,' they concluded.the 1,790 kg (3,946 lb) car could attain a top-speed of 254 km/h (158 mph).the automatic variant could accelerate to 97 km/h (60 mph) from a standing start in about 6.5 seconds (7.4 seconds for the manual version).an engine power upgrade to 350 hp (261 kw; 355 ps) was announced at the 1996 geneva motor show.english actor rowan atkinson owned virage coupé chassis 50010 which featured on the front cover of car may 1990.in the article he commented how the modern climate control system provided heating efficiency beyond the veteran aston martin driver's dreams and could not believe warm air would emanate from the footwell within 90 seconds of start up.this car also appeared in the beginning of his 1991 tv series the driven man.other celebrity owners included lennox lewis, elton john and chris eubank.the five-speed zf friedrichshafen manual was fitted to about forty percent of the cars produced.the more popular automatic option was the chrysler three-speed torqueflite transmission.for the 1993 model year, the three-speed unit was replaced by a four-speed automatic unit.the six-speed manual from the vantage also became optional at the end of the virage's production run.as the name implies, the centerpiece of the conversion was a bored and stroked 6.3 l (6,347 cc) v8 derived from the amr1 racing car. | aston martin virage | relatedmeanoftransportation | aston martin dbs <tsp> aston martin v8 | assembly | newport pagnell <tsp> aston martin v8 | engine | 53 litres <tsp> aston martin v8 | successor | aston martin virage <tsp> aston martin virage | manufacturer | aston martin | the aston martin virage is an automobile produced by british luxury automobile manufacturer aston martin as a replacement for its v8 models.although the db7 became available with a v12 engine and claimed a performance advantage, the virage remained the exclusive, expensive and hand-built flagship of the aston martin range.a new virage model was introduced at the 2011 geneva motor show, to fit into the middle of aston martin's then current lineup but was discontinued in 2012 due to many similarities between the brand's other models.to cut costs, many of the less-important pieces came from other companies, as had been the case for aston martin automobiles of the past.in fact, ford had purchased aston martin and jaguar shortly before the virage debuted and it became the first model to be introduced under the new ownership.'nothing sounds quite like an aston v8,' they concluded.in the article he commented how the modern climate control system provided heating efficiency beyond the veteran aston martin driver's dreams and could not believe warm air would emanate from the footwell within 90 seconds of start up. |
hera (minor planet designation: 103 hera) is a moderately large main-belt asteroid with an orbital period of 4.44 years.it was discovered by canadian-american astronomer james craig watson on september 7, 1868, and named after hera, queen and fifth in power of the olympian gods in greek mythology.this is a stony s-type asteroid with a silicate surface composition.photometric observations made in 2010 at the organ mesa observatory at las cruces, new mexico, and the hunters hill observatory at ngunnawal, australian capital territory, give a synodic rotation period of 23.740±0.001 h. the bimodal light curve shows a maximum brightness variation of 0.45 ± 0.03 in magnitude.measurements made with the iras observatory give a diameter of 91.58±4.14 km and a geometric albedo of 0.19±0.02.by comparison, the mips photometer on the spitzer space telescope gives a diameter of 88.30±8.51 km and a geometric albedo of 0.20±0.04.when the asteroid was observed occulting a star, the chords showed a diameter of 89.1±1.1 km. | risposta | charango | unendamaged <tsp> risposta | valvular | ungutturalness | no related information |
aaron turner (born november 5, 1977) is an american musician, singer, graphic artist, and founder of label hydra head records.he is most widely known for his role as guitarist and vocalist for the post-metal bands sumac and isis, while also participating in several other bands and projects such as old man gloom, lotus eaters and split cranium, a collaboration with jussi lehtisalo of finnish band circle who toured with isis in 2009.raised in new mexico, turner moved to the boston area, where he attended art school and formed isis and hydra head.in june 2003, turner moved operations of both the band and label to los angeles, california.turner now resides in vashon, wa which is also the base of operations for hydra head and his various other activities.in partnership with his wife faith coloccia, turner founded another record label, sige, in march 2011.it has gone on to release material from his musical collaboration with coloccia, mamiffer.sige is distributed by the business.at an early age, his family moved to new mexico, where he was raised.his mother was a teacher 'who taught a progressive curriculum' and his father an author, 'mainly [of] non-fiction'.turner describes his upbringing, surrounded by his parents' writer, artist and photographer friends, as 'creatively nurturing'.at age 17, he started a company that sold rare punk rock records via mail-order.he later moved to boston to attend art school at the school of the museum of fine arts, and in 1995 began releasing music.by 1997, the hydra head label was becoming a respectable small record label.turner describes his early industriousness as being motivated in part by boredom: i grew up in new mexico, and there wasn't a whole lot as far as youth culture is concerned.especially when i started to get interested in straight edge and wasn't doing drugs anymore, there was really nothing for me to do.so that was like a big reason for me, i suppose, to become really productive.also, i've never been a really social person.so there's not a lot of time taken up by my social life.and music has always been a very very big part of my life.i guess just a combination of those factors is why everything got started so early.around 1997–99, turner was living with future isis bassist and co-founder jeff caxide; until this point, he had been a member of the bands union suit and hollomen.isis was formed in 1997 out of a dissatisfaction with said bands' musical direction and turner and caxide's respective degrees of creative control.in mid-2009, turner moved from los angeles, where both isis and hydra head records were based at the time, to seattle with his then-girlfriend, faith coloccia; they went on to wed in september of the same year.he has also acquired a custom guitar from the electrical guitar company (as did fellow isis guitarist michael gallagher).in the past, turner has also used a gibson les paul standard, prs ce24, and has played through sunn, mesa boogie, and mackie amplifiers.when playing with isis, turner and his fellow guitarists usually tuned their instruments (low to high) b-f#-b-e-g#-b, to achieve a heavier sound.they also used other tunings, though less frequently, such as f# (octave below)-f#-b-e-g#-b.in 2016, turner described the live rig he used with sumac as consisting of two custom-built guitars from the electrical guitar company.both have lucite bodies and aluminum necks, and custom-wound wide frequency range pickups.the newer of the two—a prototype for a signature model—has a slightly flatter fingerboard radius than the older instrument. | umstroke | profusion | vintener <tsp> umstroke | algorithms | byee | no related information |
the aston martin virage is an automobile produced by british luxury automobile manufacturer aston martin as a replacement for its v8 models.introduced at the birmingham motor show in 1988, it was joined by the high-performance vantage in 1993, and then the name of the base model was changed to v8 coupe in 1996.the v8-powered model was intended as the company's flagship model, with the 6-cylinder db7, introduced in 1994, positioned below it as an entry-level model.although the db7 became available with a v12 engine and claimed a performance advantage, the virage remained the exclusive, expensive and hand-built flagship of the aston martin range.it was replaced in 2000 with the vanquish.by the end of the 2000 model year, 1,050 cars in total had been produced.the v8 vantage name reappeared on a new entry-level model in 2005.a new virage model was introduced at the 2011 geneva motor show, to fit into the middle of aston martin's then current lineup but was discontinued in 2012 due to many similarities between the brand's other models.the virage was more similar in design language to the lagonda than the v8 it replaced.indeed, the chassis was an evolution of the lagonda's, with a de dion tube rear suspension, located by triangulated radius rods and a watts linkage, and a double wishbone unit at the front.to cut costs, many of the less-important pieces came from other companies, as had been the case for aston martin automobiles of the past.the sleek headlights and taillights were sourced from the audi 200 and the volkswagen scirocco respectively, while general motors, jaguar, citroën and ford provided the steering column, climate control panel, wing mirrors and dash switches.in fact, ford had purchased aston martin and jaguar shortly before the virage debuted and it became the first model to be introduced under the new ownership.the virage was a large, heavy car in spite of its all-aluminium body, but the 32-valve 5.3 l (5,340 cc) v8 engine's 494 n⋅m (364 lb⋅ft) torque elevated its performance to near sports car levels.'acceleration just never seems to run out', claimed sports car international during a first test.they also praised the 'eager and quicker revving' nature of the 330 hp (246 kw; 335 ps) engine with its callaway-designed heads and weber-marelli fuel injection.'nothing sounds quite like an aston v8,' they concluded.the 1,790 kg (3,946 lb) car could attain a top-speed of 254 km/h (158 mph).the automatic variant could accelerate to 97 km/h (60 mph) from a standing start in about 6.5 seconds (7.4 seconds for the manual version).an engine power upgrade to 350 hp (261 kw; 355 ps) was announced at the 1996 geneva motor show.english actor rowan atkinson owned virage coupé chassis 50010 which featured on the front cover of car may 1990.in the article he commented how the modern climate control system provided heating efficiency beyond the veteran aston martin driver's dreams and could not believe warm air would emanate from the footwell within 90 seconds of start up.this car also appeared in the beginning of his 1991 tv series the driven man.other celebrity owners included lennox lewis, elton john and chris eubank.the five-speed zf friedrichshafen manual was fitted to about forty percent of the cars produced.the more popular automatic option was the chrysler three-speed torqueflite transmission.for the 1993 model year, the three-speed unit was replaced by a four-speed automatic unit.the six-speed manual from the vantage also became optional at the end of the virage's production run.as the name implies, the centerpiece of the conversion was a bored and stroked 6.3 l (6,347 cc) v8 derived from the amr1 racing car. | churchless | lengthways | outwaved | no related information |
hera (minor planet designation: 103 hera) is a moderately large main-belt asteroid with an orbital period of 4.44 years.it was discovered by canadian-american astronomer james craig watson on september 7, 1868, and named after hera, queen and fifth in power of the olympian gods in greek mythology.this is a stony s-type asteroid with a silicate surface composition.photometric observations made in 2010 at the organ mesa observatory at las cruces, new mexico, and the hunters hill observatory at ngunnawal, australian capital territory, give a synodic rotation period of 23.740±0.001 h. the bimodal light curve shows a maximum brightness variation of 0.45 ± 0.03 in magnitude.measurements made with the iras observatory give a diameter of 91.58±4.14 km and a geometric albedo of 0.19±0.02.by comparison, the mips photometer on the spitzer space telescope gives a diameter of 88.30±8.51 km and a geometric albedo of 0.20±0.04.when the asteroid was observed occulting a star, the chords showed a diameter of 89.1±1.1 km. | 103 hera | discoverer | james craig watson <tsp> james craig watson | almamater | university of michigan <tsp> james craig watson | nationality | canada <tsp> james craig watson | deathplace | madison wisconsin <tsp> 103 hera | orbitalperiod | 1622213 days | it was discovered by canadian-american astronomer james craig watson on september 7, 1868, and named after hera, queen and fifth in power of the olympian gods in greek mythology. |
aaron turner (born november 5, 1977) is an american musician, singer, graphic artist, and founder of label hydra head records.he is most widely known for his role as guitarist and vocalist for the post-metal bands sumac and isis, while also participating in several other bands and projects such as old man gloom, lotus eaters and split cranium, a collaboration with jussi lehtisalo of finnish band circle who toured with isis in 2009.raised in new mexico, turner moved to the boston area, where he attended art school and formed isis and hydra head.in june 2003, turner moved operations of both the band and label to los angeles, california.turner now resides in vashon, wa which is also the base of operations for hydra head and his various other activities.in partnership with his wife faith coloccia, turner founded another record label, sige, in march 2011.it has gone on to release material from his musical collaboration with coloccia, mamiffer.sige is distributed by the business.at an early age, his family moved to new mexico, where he was raised.his mother was a teacher 'who taught a progressive curriculum' and his father an author, 'mainly [of] non-fiction'.turner describes his upbringing, surrounded by his parents' writer, artist and photographer friends, as 'creatively nurturing'.at age 17, he started a company that sold rare punk rock records via mail-order.he later moved to boston to attend art school at the school of the museum of fine arts, and in 1995 began releasing music.by 1997, the hydra head label was becoming a respectable small record label.turner describes his early industriousness as being motivated in part by boredom: i grew up in new mexico, and there wasn't a whole lot as far as youth culture is concerned.especially when i started to get interested in straight edge and wasn't doing drugs anymore, there was really nothing for me to do.so that was like a big reason for me, i suppose, to become really productive.also, i've never been a really social person.so there's not a lot of time taken up by my social life.and music has always been a very very big part of my life.i guess just a combination of those factors is why everything got started so early.around 1997–99, turner was living with future isis bassist and co-founder jeff caxide; until this point, he had been a member of the bands union suit and hollomen.isis was formed in 1997 out of a dissatisfaction with said bands' musical direction and turner and caxide's respective degrees of creative control.in mid-2009, turner moved from los angeles, where both isis and hydra head records were based at the time, to seattle with his then-girlfriend, faith coloccia; they went on to wed in september of the same year.he has also acquired a custom guitar from the electrical guitar company (as did fellow isis guitarist michael gallagher).in the past, turner has also used a gibson les paul standard, prs ce24, and has played through sunn, mesa boogie, and mackie amplifiers.when playing with isis, turner and his fellow guitarists usually tuned their instruments (low to high) b-f#-b-e-g#-b, to achieve a heavier sound.they also used other tunings, though less frequently, such as f# (octave below)-f#-b-e-g#-b.in 2016, turner described the live rig he used with sumac as consisting of two custom-built guitars from the electrical guitar company.both have lucite bodies and aluminum necks, and custom-wound wide frequency range pickups.the newer of the two—a prototype for a signature model—has a slightly flatter fingerboard radius than the older instrument. | aaron turner | associatedband/associatedmusicalartist | twilight band <tsp> aaron turner | associatedband/associatedmusicalartist | lotus eaters band <tsp> aaron turner | genre | black metal <tsp> aaron turner | origin | boston <tsp> aaron turner | activeyearsstartyear | 1995 | raised in new mexico, turner moved to the boston area, where he attended art school and formed isis and hydra head. |
atlas ii was a member of the atlas family of launch vehicles, which evolved from the successful atlas missile program of the 1950s.the atlas ii was a direct evolution of the atlas i, featuring longer first stage tanks, higher-performing engines, and the option for strap-on solid rocket boosters.it was designed to launch payloads into low earth orbit, geosynchronous transfer orbit or geosynchronous orbit.sixty-three launches of the atlas ii, iia and iias models were carried out between 1991 and 2004; all sixty-three launches were successes, making the atlas ii a highly reliable space launch system.the atlas line was continued by the atlas iii, used between 2000 and 2005, and the atlas v which is still in use.additional commercial and u.s. government sales resulted in production increases leading to greater than 60 vehicles being produced and launched.atlas ii was developed from the atlas i and featured numerous upgrades over that vehicle.atlas ii was launched from launch complex 36 at cape canaveral space force station in florida as well as space launch complex 3e at vandenberg space force base in california.all launches were successful.the increased thrust, engine efficiency, and propellant capacity enabled the vehicle to lift payloads of 6,100 pounds (2,767 kg) into geostationary transfer orbit (gto), or more on later atlas ii variants.atlas ii also featured lower-cost electronics, an improved flight computer, and longer propellant tanks than its predecessor, atlas i.the stage was powered by 3 rs-56 rocket engines (derived from the rs-27 main engine of the delta ii rocket) burning 156 t (344,000 lb) of rp-1 and liquid oxygen.the two booster engines were the rs-56-oba variants (the complete assembly of both engines and the aft skirt was referred to as the ma-5a), with high thrust but moderate efficiency.the sustainer (center) engine was the rs-56-osa variant, featuring much less thrust but higher efficiency at high altitudes than the booster engines.the vernier engines used on the first stage of the atlas i (and all previous atlas models) were replaced by a hydrazine-fueled roll control system on atlas ii.this system, mounted on the interstage between the first and second stages, utilized small thrusters to control the vehicle's roll.compared to atlas i, the atlas ii first stage was 2.7 m (8 ft 10 in) taller.the atlas ii was the last atlas rocket to use the 'stage-and-a-half' technique, where it ignited all 3 rs-56 engines at liftoff and then jettisoned the 2 rs-56-oba side engines and their support structure during ascent.the two rs-56-oba engines were integrated into a single unit called the ma-5a and shared a common gas generator.they burned for approximately 164 seconds before being jettisoned, when acceleration reached approximately 5.0-5.5 g. the central sustainer engine on the first stage, an rs-56-osa, would burn for an additional 125 seconds after their jettison.it featured better efficiency at high altitudes than the rs-56-obas.the first stage also had the option to be fitted with 4 castor 4a solid rocket boosters as part of the iias version, each providing an additional 478.3 kn (107,500 lbf) of thrust for 56 seconds.the first two boosters were ignited at liftoff, and the other two were ignited after the first two burnt out.both pairs of boosters were jettisoned shortly after their respective burns.centaur ii featured 2 rl-10a-3-3a engines, burning liquid hydrogen and liquid oxygen.it featured propellant tanks 0.9 meters longer than its predecessor, centaur i, giving the stage more propellant and therefore higher performance.due to the super cold propellants inside centaur, foam insulation was installed onto the outer metal skin on the stage to help mitigate propellant boiloff inside the tank. | venditate | kittenless | interprater | no related information |
hera (minor planet designation: 103 hera) is a moderately large main-belt asteroid with an orbital period of 4.44 years.it was discovered by canadian-american astronomer james craig watson on september 7, 1868, and named after hera, queen and fifth in power of the olympian gods in greek mythology.this is a stony s-type asteroid with a silicate surface composition.photometric observations made in 2010 at the organ mesa observatory at las cruces, new mexico, and the hunters hill observatory at ngunnawal, australian capital territory, give a synodic rotation period of 23.740±0.001 h. the bimodal light curve shows a maximum brightness variation of 0.45 ± 0.03 in magnitude.measurements made with the iras observatory give a diameter of 91.58±4.14 km and a geometric albedo of 0.19±0.02.by comparison, the mips photometer on the spitzer space telescope gives a diameter of 88.30±8.51 km and a geometric albedo of 0.20±0.04.when the asteroid was observed occulting a star, the chords showed a diameter of 89.1±1.1 km. | 103 hera | discoverer | james craig watson <tsp> james craig watson | almamater | university of michigan <tsp> james craig watson | nationality | canada <tsp> james craig watson | deathplace | madison wisconsin <tsp> 103 hera | orbitalperiod | 1622213 days | it was discovered by canadian-american astronomer james craig watson on september 7, 1868, and named after hera, queen and fifth in power of the olympian gods in greek mythology. |
aaron turner (born november 5, 1977) is an american musician, singer, graphic artist, and founder of label hydra head records.he is most widely known for his role as guitarist and vocalist for the post-metal bands sumac and isis, while also participating in several other bands and projects such as old man gloom, lotus eaters and split cranium, a collaboration with jussi lehtisalo of finnish band circle who toured with isis in 2009.raised in new mexico, turner moved to the boston area, where he attended art school and formed isis and hydra head.in june 2003, turner moved operations of both the band and label to los angeles, california.turner now resides in vashon, wa which is also the base of operations for hydra head and his various other activities.in partnership with his wife faith coloccia, turner founded another record label, sige, in march 2011.it has gone on to release material from his musical collaboration with coloccia, mamiffer.sige is distributed by the business.at an early age, his family moved to new mexico, where he was raised.his mother was a teacher 'who taught a progressive curriculum' and his father an author, 'mainly [of] non-fiction'.turner describes his upbringing, surrounded by his parents' writer, artist and photographer friends, as 'creatively nurturing'.at age 17, he started a company that sold rare punk rock records via mail-order.he later moved to boston to attend art school at the school of the museum of fine arts, and in 1995 began releasing music.by 1997, the hydra head label was becoming a respectable small record label.turner describes his early industriousness as being motivated in part by boredom: i grew up in new mexico, and there wasn't a whole lot as far as youth culture is concerned.especially when i started to get interested in straight edge and wasn't doing drugs anymore, there was really nothing for me to do.so that was like a big reason for me, i suppose, to become really productive.also, i've never been a really social person.so there's not a lot of time taken up by my social life.and music has always been a very very big part of my life.i guess just a combination of those factors is why everything got started so early.around 1997–99, turner was living with future isis bassist and co-founder jeff caxide; until this point, he had been a member of the bands union suit and hollomen.isis was formed in 1997 out of a dissatisfaction with said bands' musical direction and turner and caxide's respective degrees of creative control.in mid-2009, turner moved from los angeles, where both isis and hydra head records were based at the time, to seattle with his then-girlfriend, faith coloccia; they went on to wed in september of the same year.he has also acquired a custom guitar from the electrical guitar company (as did fellow isis guitarist michael gallagher).in the past, turner has also used a gibson les paul standard, prs ce24, and has played through sunn, mesa boogie, and mackie amplifiers.when playing with isis, turner and his fellow guitarists usually tuned their instruments (low to high) b-f#-b-e-g#-b, to achieve a heavier sound.they also used other tunings, though less frequently, such as f# (octave below)-f#-b-e-g#-b.in 2016, turner described the live rig he used with sumac as consisting of two custom-built guitars from the electrical guitar company.both have lucite bodies and aluminum necks, and custom-wound wide frequency range pickups.the newer of the two—a prototype for a signature model—has a slightly flatter fingerboard radius than the older instrument. | palaeoniscoid | delabialized | undercarried | no related information |
hera (minor planet designation: 103 hera) is a moderately large main-belt asteroid with an orbital period of 4.44 years.it was discovered by canadian-american astronomer james craig watson on september 7, 1868, and named after hera, queen and fifth in power of the olympian gods in greek mythology.this is a stony s-type asteroid with a silicate surface composition.photometric observations made in 2010 at the organ mesa observatory at las cruces, new mexico, and the hunters hill observatory at ngunnawal, australian capital territory, give a synodic rotation period of 23.740±0.001 h. the bimodal light curve shows a maximum brightness variation of 0.45 ± 0.03 in magnitude.measurements made with the iras observatory give a diameter of 91.58±4.14 km and a geometric albedo of 0.19±0.02.by comparison, the mips photometer on the spitzer space telescope gives a diameter of 88.30±8.51 km and a geometric albedo of 0.20±0.04.when the asteroid was observed occulting a star, the chords showed a diameter of 89.1±1.1 km. | waterbank | hypothecal | wanier | no related information |
atlas ii was a member of the atlas family of launch vehicles, which evolved from the successful atlas missile program of the 1950s.the atlas ii was a direct evolution of the atlas i, featuring longer first stage tanks, higher-performing engines, and the option for strap-on solid rocket boosters.it was designed to launch payloads into low earth orbit, geosynchronous transfer orbit or geosynchronous orbit.sixty-three launches of the atlas ii, iia and iias models were carried out between 1991 and 2004; all sixty-three launches were successes, making the atlas ii a highly reliable space launch system.the atlas line was continued by the atlas iii, used between 2000 and 2005, and the atlas v which is still in use.additional commercial and u.s. government sales resulted in production increases leading to greater than 60 vehicles being produced and launched.atlas ii was developed from the atlas i and featured numerous upgrades over that vehicle.atlas ii was launched from launch complex 36 at cape canaveral space force station in florida as well as space launch complex 3e at vandenberg space force base in california.all launches were successful.the increased thrust, engine efficiency, and propellant capacity enabled the vehicle to lift payloads of 6,100 pounds (2,767 kg) into geostationary transfer orbit (gto), or more on later atlas ii variants.atlas ii also featured lower-cost electronics, an improved flight computer, and longer propellant tanks than its predecessor, atlas i.the stage was powered by 3 rs-56 rocket engines (derived from the rs-27 main engine of the delta ii rocket) burning 156 t (344,000 lb) of rp-1 and liquid oxygen.the two booster engines were the rs-56-oba variants (the complete assembly of both engines and the aft skirt was referred to as the ma-5a), with high thrust but moderate efficiency.the sustainer (center) engine was the rs-56-osa variant, featuring much less thrust but higher efficiency at high altitudes than the booster engines.the vernier engines used on the first stage of the atlas i (and all previous atlas models) were replaced by a hydrazine-fueled roll control system on atlas ii.this system, mounted on the interstage between the first and second stages, utilized small thrusters to control the vehicle's roll.compared to atlas i, the atlas ii first stage was 2.7 m (8 ft 10 in) taller.the atlas ii was the last atlas rocket to use the 'stage-and-a-half' technique, where it ignited all 3 rs-56 engines at liftoff and then jettisoned the 2 rs-56-oba side engines and their support structure during ascent.the two rs-56-oba engines were integrated into a single unit called the ma-5a and shared a common gas generator.they burned for approximately 164 seconds before being jettisoned, when acceleration reached approximately 5.0-5.5 g. the central sustainer engine on the first stage, an rs-56-osa, would burn for an additional 125 seconds after their jettison.it featured better efficiency at high altitudes than the rs-56-obas.the first stage also had the option to be fitted with 4 castor 4a solid rocket boosters as part of the iias version, each providing an additional 478.3 kn (107,500 lbf) of thrust for 56 seconds.the first two boosters were ignited at liftoff, and the other two were ignited after the first two burnt out.both pairs of boosters were jettisoned shortly after their respective burns.centaur ii featured 2 rl-10a-3-3a engines, burning liquid hydrogen and liquid oxygen.it featured propellant tanks 0.9 meters longer than its predecessor, centaur i, giving the stage more propellant and therefore higher performance.due to the super cold propellants inside centaur, foam insulation was installed onto the outer metal skin on the stage to help mitigate propellant boiloff inside the tank. | mangers | noncombatant | appalled | no related information |
aaron turner (born november 5, 1977) is an american musician, singer, graphic artist, and founder of label hydra head records.he is most widely known for his role as guitarist and vocalist for the post-metal bands sumac and isis, while also participating in several other bands and projects such as old man gloom, lotus eaters and split cranium, a collaboration with jussi lehtisalo of finnish band circle who toured with isis in 2009.raised in new mexico, turner moved to the boston area, where he attended art school and formed isis and hydra head.in june 2003, turner moved operations of both the band and label to los angeles, california.turner now resides in vashon, wa which is also the base of operations for hydra head and his various other activities.in partnership with his wife faith coloccia, turner founded another record label, sige, in march 2011.it has gone on to release material from his musical collaboration with coloccia, mamiffer.sige is distributed by the business.at an early age, his family moved to new mexico, where he was raised.his mother was a teacher 'who taught a progressive curriculum' and his father an author, 'mainly [of] non-fiction'.turner describes his upbringing, surrounded by his parents' writer, artist and photographer friends, as 'creatively nurturing'.at age 17, he started a company that sold rare punk rock records via mail-order.he later moved to boston to attend art school at the school of the museum of fine arts, and in 1995 began releasing music.by 1997, the hydra head label was becoming a respectable small record label.turner describes his early industriousness as being motivated in part by boredom: i grew up in new mexico, and there wasn't a whole lot as far as youth culture is concerned.especially when i started to get interested in straight edge and wasn't doing drugs anymore, there was really nothing for me to do.so that was like a big reason for me, i suppose, to become really productive.also, i've never been a really social person.so there's not a lot of time taken up by my social life.and music has always been a very very big part of my life.i guess just a combination of those factors is why everything got started so early.around 1997–99, turner was living with future isis bassist and co-founder jeff caxide; until this point, he had been a member of the bands union suit and hollomen.isis was formed in 1997 out of a dissatisfaction with said bands' musical direction and turner and caxide's respective degrees of creative control.in mid-2009, turner moved from los angeles, where both isis and hydra head records were based at the time, to seattle with his then-girlfriend, faith coloccia; they went on to wed in september of the same year.he has also acquired a custom guitar from the electrical guitar company (as did fellow isis guitarist michael gallagher).in the past, turner has also used a gibson les paul standard, prs ce24, and has played through sunn, mesa boogie, and mackie amplifiers.when playing with isis, turner and his fellow guitarists usually tuned their instruments (low to high) b-f#-b-e-g#-b, to achieve a heavier sound.they also used other tunings, though less frequently, such as f# (octave below)-f#-b-e-g#-b.in 2016, turner described the live rig he used with sumac as consisting of two custom-built guitars from the electrical guitar company.both have lucite bodies and aluminum necks, and custom-wound wide frequency range pickups.the newer of the two—a prototype for a signature model—has a slightly flatter fingerboard radius than the older instrument. | rectococcygeal | exconjugant | kuvaszok | no related information |
atlas ii was a member of the atlas family of launch vehicles, which evolved from the successful atlas missile program of the 1950s.the atlas ii was a direct evolution of the atlas i, featuring longer first stage tanks, higher-performing engines, and the option for strap-on solid rocket boosters.it was designed to launch payloads into low earth orbit, geosynchronous transfer orbit or geosynchronous orbit.sixty-three launches of the atlas ii, iia and iias models were carried out between 1991 and 2004; all sixty-three launches were successes, making the atlas ii a highly reliable space launch system.the atlas line was continued by the atlas iii, used between 2000 and 2005, and the atlas v which is still in use.additional commercial and u.s. government sales resulted in production increases leading to greater than 60 vehicles being produced and launched.atlas ii was developed from the atlas i and featured numerous upgrades over that vehicle.atlas ii was launched from launch complex 36 at cape canaveral space force station in florida as well as space launch complex 3e at vandenberg space force base in california.all launches were successful.the increased thrust, engine efficiency, and propellant capacity enabled the vehicle to lift payloads of 6,100 pounds (2,767 kg) into geostationary transfer orbit (gto), or more on later atlas ii variants.atlas ii also featured lower-cost electronics, an improved flight computer, and longer propellant tanks than its predecessor, atlas i.the stage was powered by 3 rs-56 rocket engines (derived from the rs-27 main engine of the delta ii rocket) burning 156 t (344,000 lb) of rp-1 and liquid oxygen.the two booster engines were the rs-56-oba variants (the complete assembly of both engines and the aft skirt was referred to as the ma-5a), with high thrust but moderate efficiency.the sustainer (center) engine was the rs-56-osa variant, featuring much less thrust but higher efficiency at high altitudes than the booster engines.the vernier engines used on the first stage of the atlas i (and all previous atlas models) were replaced by a hydrazine-fueled roll control system on atlas ii.this system, mounted on the interstage between the first and second stages, utilized small thrusters to control the vehicle's roll.compared to atlas i, the atlas ii first stage was 2.7 m (8 ft 10 in) taller.the atlas ii was the last atlas rocket to use the 'stage-and-a-half' technique, where it ignited all 3 rs-56 engines at liftoff and then jettisoned the 2 rs-56-oba side engines and their support structure during ascent.the two rs-56-oba engines were integrated into a single unit called the ma-5a and shared a common gas generator.they burned for approximately 164 seconds before being jettisoned, when acceleration reached approximately 5.0-5.5 g. the central sustainer engine on the first stage, an rs-56-osa, would burn for an additional 125 seconds after their jettison.it featured better efficiency at high altitudes than the rs-56-obas.the first stage also had the option to be fitted with 4 castor 4a solid rocket boosters as part of the iias version, each providing an additional 478.3 kn (107,500 lbf) of thrust for 56 seconds.the first two boosters were ignited at liftoff, and the other two were ignited after the first two burnt out.both pairs of boosters were jettisoned shortly after their respective burns.centaur ii featured 2 rl-10a-3-3a engines, burning liquid hydrogen and liquid oxygen.it featured propellant tanks 0.9 meters longer than its predecessor, centaur i, giving the stage more propellant and therefore higher performance.due to the super cold propellants inside centaur, foam insulation was installed onto the outer metal skin on the stage to help mitigate propellant boiloff inside the tank. | atlas ii | countryorigin | united states <tsp> atlas ii | finalflight | 1998-03-16 <tsp> atlas ii | launchsite | vandenberg air force base <tsp> atlas ii | diameter | 304 m <tsp> atlas ii | launchsite | cape canaveral air force station | atlas ii was developed from the atlas i and featured numerous upgrades over that vehicle.atlas ii was launched from launch complex 36 at cape canaveral space force station in florida as well as space launch complex 3e at vandenberg space force base in california.the increased thrust, engine efficiency, and propellant capacity enabled the vehicle to lift payloads of 6,100 pounds (2,767 kg) into geostationary transfer orbit (gto), or more on later atlas ii variants.atlas ii also featured lower-cost electronics, an improved flight computer, and longer propellant tanks than its predecessor, atlas i. |
hera (minor planet designation: 103 hera) is a moderately large main-belt asteroid with an orbital period of 4.44 years.it was discovered by canadian-american astronomer james craig watson on september 7, 1868, and named after hera, queen and fifth in power of the olympian gods in greek mythology.this is a stony s-type asteroid with a silicate surface composition.photometric observations made in 2010 at the organ mesa observatory at las cruces, new mexico, and the hunters hill observatory at ngunnawal, australian capital territory, give a synodic rotation period of 23.740±0.001 h. the bimodal light curve shows a maximum brightness variation of 0.45 ± 0.03 in magnitude.measurements made with the iras observatory give a diameter of 91.58±4.14 km and a geometric albedo of 0.19±0.02.by comparison, the mips photometer on the spitzer space telescope gives a diameter of 88.30±8.51 km and a geometric albedo of 0.20±0.04.when the asteroid was observed occulting a star, the chords showed a diameter of 89.1±1.1 km. | 103 hera | discoverer | james craig watson <tsp> james craig watson | almamater | university of michigan <tsp> james craig watson | nationality | canada <tsp> james craig watson | deathplace | madison wisconsin <tsp> james craig watson | deathcause | peritonitis | it was discovered by canadian-american astronomer james craig watson on september 7, 1868, and named after hera, queen and fifth in power of the olympian gods in greek mythology. |
aaron turner (born november 5, 1977) is an american musician, singer, graphic artist, and founder of label hydra head records.he is most widely known for his role as guitarist and vocalist for the post-metal bands sumac and isis, while also participating in several other bands and projects such as old man gloom, lotus eaters and split cranium, a collaboration with jussi lehtisalo of finnish band circle who toured with isis in 2009.raised in new mexico, turner moved to the boston area, where he attended art school and formed isis and hydra head.in june 2003, turner moved operations of both the band and label to los angeles, california.turner now resides in vashon, wa which is also the base of operations for hydra head and his various other activities.in partnership with his wife faith coloccia, turner founded another record label, sige, in march 2011.it has gone on to release material from his musical collaboration with coloccia, mamiffer.sige is distributed by the business.at an early age, his family moved to new mexico, where he was raised.his mother was a teacher 'who taught a progressive curriculum' and his father an author, 'mainly [of] non-fiction'.turner describes his upbringing, surrounded by his parents' writer, artist and photographer friends, as 'creatively nurturing'.at age 17, he started a company that sold rare punk rock records via mail-order.he later moved to boston to attend art school at the school of the museum of fine arts, and in 1995 began releasing music.by 1997, the hydra head label was becoming a respectable small record label.turner describes his early industriousness as being motivated in part by boredom: i grew up in new mexico, and there wasn't a whole lot as far as youth culture is concerned.especially when i started to get interested in straight edge and wasn't doing drugs anymore, there was really nothing for me to do.so that was like a big reason for me, i suppose, to become really productive.also, i've never been a really social person.so there's not a lot of time taken up by my social life.and music has always been a very very big part of my life.i guess just a combination of those factors is why everything got started so early.around 1997–99, turner was living with future isis bassist and co-founder jeff caxide; until this point, he had been a member of the bands union suit and hollomen.isis was formed in 1997 out of a dissatisfaction with said bands' musical direction and turner and caxide's respective degrees of creative control.in mid-2009, turner moved from los angeles, where both isis and hydra head records were based at the time, to seattle with his then-girlfriend, faith coloccia; they went on to wed in september of the same year.he has also acquired a custom guitar from the electrical guitar company (as did fellow isis guitarist michael gallagher).in the past, turner has also used a gibson les paul standard, prs ce24, and has played through sunn, mesa boogie, and mackie amplifiers.when playing with isis, turner and his fellow guitarists usually tuned their instruments (low to high) b-f#-b-e-g#-b, to achieve a heavier sound.they also used other tunings, though less frequently, such as f# (octave below)-f#-b-e-g#-b.in 2016, turner described the live rig he used with sumac as consisting of two custom-built guitars from the electrical guitar company.both have lucite bodies and aluminum necks, and custom-wound wide frequency range pickups.the newer of the two—a prototype for a signature model—has a slightly flatter fingerboard radius than the older instrument. | aaron turner | associatedband/associatedmusicalartist | twilight band <tsp> aaron turner | associatedband/associatedmusicalartist | lotus eaters band <tsp> aaron turner | genre | black metal <tsp> aaron turner | origin | massachusetts <tsp> aaron turner | activeyearsstartyear | 1995 | no related information |
atlas ii was a member of the atlas family of launch vehicles, which evolved from the successful atlas missile program of the 1950s.the atlas ii was a direct evolution of the atlas i, featuring longer first stage tanks, higher-performing engines, and the option for strap-on solid rocket boosters.it was designed to launch payloads into low earth orbit, geosynchronous transfer orbit or geosynchronous orbit.sixty-three launches of the atlas ii, iia and iias models were carried out between 1991 and 2004; all sixty-three launches were successes, making the atlas ii a highly reliable space launch system.the atlas line was continued by the atlas iii, used between 2000 and 2005, and the atlas v which is still in use.additional commercial and u.s. government sales resulted in production increases leading to greater than 60 vehicles being produced and launched.atlas ii was developed from the atlas i and featured numerous upgrades over that vehicle.atlas ii was launched from launch complex 36 at cape canaveral space force station in florida as well as space launch complex 3e at vandenberg space force base in california.all launches were successful.the increased thrust, engine efficiency, and propellant capacity enabled the vehicle to lift payloads of 6,100 pounds (2,767 kg) into geostationary transfer orbit (gto), or more on later atlas ii variants.atlas ii also featured lower-cost electronics, an improved flight computer, and longer propellant tanks than its predecessor, atlas i.the stage was powered by 3 rs-56 rocket engines (derived from the rs-27 main engine of the delta ii rocket) burning 156 t (344,000 lb) of rp-1 and liquid oxygen.the two booster engines were the rs-56-oba variants (the complete assembly of both engines and the aft skirt was referred to as the ma-5a), with high thrust but moderate efficiency.the sustainer (center) engine was the rs-56-osa variant, featuring much less thrust but higher efficiency at high altitudes than the booster engines.the vernier engines used on the first stage of the atlas i (and all previous atlas models) were replaced by a hydrazine-fueled roll control system on atlas ii.this system, mounted on the interstage between the first and second stages, utilized small thrusters to control the vehicle's roll.compared to atlas i, the atlas ii first stage was 2.7 m (8 ft 10 in) taller.the atlas ii was the last atlas rocket to use the 'stage-and-a-half' technique, where it ignited all 3 rs-56 engines at liftoff and then jettisoned the 2 rs-56-oba side engines and their support structure during ascent.the two rs-56-oba engines were integrated into a single unit called the ma-5a and shared a common gas generator.they burned for approximately 164 seconds before being jettisoned, when acceleration reached approximately 5.0-5.5 g. the central sustainer engine on the first stage, an rs-56-osa, would burn for an additional 125 seconds after their jettison.it featured better efficiency at high altitudes than the rs-56-obas.the first stage also had the option to be fitted with 4 castor 4a solid rocket boosters as part of the iias version, each providing an additional 478.3 kn (107,500 lbf) of thrust for 56 seconds.the first two boosters were ignited at liftoff, and the other two were ignited after the first two burnt out.both pairs of boosters were jettisoned shortly after their respective burns.centaur ii featured 2 rl-10a-3-3a engines, burning liquid hydrogen and liquid oxygen.it featured propellant tanks 0.9 meters longer than its predecessor, centaur i, giving the stage more propellant and therefore higher performance.due to the super cold propellants inside centaur, foam insulation was installed onto the outer metal skin on the stage to help mitigate propellant boiloff inside the tank. | atlas ii | countryorigin | united states <tsp> atlas ii | finalflight | 2002-12-05 <tsp> atlas ii | launchsite | vandenberg air force base <tsp> atlas ii | diameter | 304 m <tsp> atlas ii | launchsite | cape canaveral air force station | atlas ii was developed from the atlas i and featured numerous upgrades over that vehicle.atlas ii was launched from launch complex 36 at cape canaveral space force station in florida as well as space launch complex 3e at vandenberg space force base in california.the increased thrust, engine efficiency, and propellant capacity enabled the vehicle to lift payloads of 6,100 pounds (2,767 kg) into geostationary transfer orbit (gto), or more on later atlas ii variants.atlas ii also featured lower-cost electronics, an improved flight computer, and longer propellant tanks than its predecessor, atlas i. |
hera (minor planet designation: 103 hera) is a moderately large main-belt asteroid with an orbital period of 4.44 years.it was discovered by canadian-american astronomer james craig watson on september 7, 1868, and named after hera, queen and fifth in power of the olympian gods in greek mythology.this is a stony s-type asteroid with a silicate surface composition.photometric observations made in 2010 at the organ mesa observatory at las cruces, new mexico, and the hunters hill observatory at ngunnawal, australian capital territory, give a synodic rotation period of 23.740±0.001 h. the bimodal light curve shows a maximum brightness variation of 0.45 ± 0.03 in magnitude.measurements made with the iras observatory give a diameter of 91.58±4.14 km and a geometric albedo of 0.19±0.02.by comparison, the mips photometer on the spitzer space telescope gives a diameter of 88.30±8.51 km and a geometric albedo of 0.20±0.04.when the asteroid was observed occulting a star, the chords showed a diameter of 89.1±1.1 km. | 103 hera | discoverer | james craig watson <tsp> james craig watson | almamater | university of michigan <tsp> james craig watson | nationality | canada <tsp> james craig watson | deathplace | madison wisconsin <tsp> james craig watson | deathcause | peritonitis | it was discovered by canadian-american astronomer james craig watson on september 7, 1868, and named after hera, queen and fifth in power of the olympian gods in greek mythology. |
hera (minor planet designation: 103 hera) is a moderately large main-belt asteroid with an orbital period of 4.44 years.it was discovered by canadian-american astronomer james craig watson on september 7, 1868, and named after hera, queen and fifth in power of the olympian gods in greek mythology.this is a stony s-type asteroid with a silicate surface composition.photometric observations made in 2010 at the organ mesa observatory at las cruces, new mexico, and the hunters hill observatory at ngunnawal, australian capital territory, give a synodic rotation period of 23.740±0.001 h. the bimodal light curve shows a maximum brightness variation of 0.45 ± 0.03 in magnitude.measurements made with the iras observatory give a diameter of 91.58±4.14 km and a geometric albedo of 0.19±0.02.by comparison, the mips photometer on the spitzer space telescope gives a diameter of 88.30±8.51 km and a geometric albedo of 0.20±0.04.when the asteroid was observed occulting a star, the chords showed a diameter of 89.1±1.1 km. | 103 hera | discoverer | james craig watson <tsp> james craig watson | almamater | university of michigan <tsp> james craig watson | nationality | canada <tsp> james craig watson | deathplace | madison wisconsin <tsp> james craig watson | deathcause | peritonitis | it was discovered by canadian-american astronomer james craig watson on september 7, 1868, and named after hera, queen and fifth in power of the olympian gods in greek mythology. |
atlas ii was a member of the atlas family of launch vehicles, which evolved from the successful atlas missile program of the 1950s.the atlas ii was a direct evolution of the atlas i, featuring longer first stage tanks, higher-performing engines, and the option for strap-on solid rocket boosters.it was designed to launch payloads into low earth orbit, geosynchronous transfer orbit or geosynchronous orbit.sixty-three launches of the atlas ii, iia and iias models were carried out between 1991 and 2004; all sixty-three launches were successes, making the atlas ii a highly reliable space launch system.the atlas line was continued by the atlas iii, used between 2000 and 2005, and the atlas v which is still in use.additional commercial and u.s. government sales resulted in production increases leading to greater than 60 vehicles being produced and launched.atlas ii was developed from the atlas i and featured numerous upgrades over that vehicle.atlas ii was launched from launch complex 36 at cape canaveral space force station in florida as well as space launch complex 3e at vandenberg space force base in california.all launches were successful.the increased thrust, engine efficiency, and propellant capacity enabled the vehicle to lift payloads of 6,100 pounds (2,767 kg) into geostationary transfer orbit (gto), or more on later atlas ii variants.atlas ii also featured lower-cost electronics, an improved flight computer, and longer propellant tanks than its predecessor, atlas i.the stage was powered by 3 rs-56 rocket engines (derived from the rs-27 main engine of the delta ii rocket) burning 156 t (344,000 lb) of rp-1 and liquid oxygen.the two booster engines were the rs-56-oba variants (the complete assembly of both engines and the aft skirt was referred to as the ma-5a), with high thrust but moderate efficiency.the sustainer (center) engine was the rs-56-osa variant, featuring much less thrust but higher efficiency at high altitudes than the booster engines.the vernier engines used on the first stage of the atlas i (and all previous atlas models) were replaced by a hydrazine-fueled roll control system on atlas ii.this system, mounted on the interstage between the first and second stages, utilized small thrusters to control the vehicle's roll.compared to atlas i, the atlas ii first stage was 2.7 m (8 ft 10 in) taller.the atlas ii was the last atlas rocket to use the 'stage-and-a-half' technique, where it ignited all 3 rs-56 engines at liftoff and then jettisoned the 2 rs-56-oba side engines and their support structure during ascent.the two rs-56-oba engines were integrated into a single unit called the ma-5a and shared a common gas generator.they burned for approximately 164 seconds before being jettisoned, when acceleration reached approximately 5.0-5.5 g. the central sustainer engine on the first stage, an rs-56-osa, would burn for an additional 125 seconds after their jettison.it featured better efficiency at high altitudes than the rs-56-obas.the first stage also had the option to be fitted with 4 castor 4a solid rocket boosters as part of the iias version, each providing an additional 478.3 kn (107,500 lbf) of thrust for 56 seconds.the first two boosters were ignited at liftoff, and the other two were ignited after the first two burnt out.both pairs of boosters were jettisoned shortly after their respective burns.centaur ii featured 2 rl-10a-3-3a engines, burning liquid hydrogen and liquid oxygen.it featured propellant tanks 0.9 meters longer than its predecessor, centaur i, giving the stage more propellant and therefore higher performance.due to the super cold propellants inside centaur, foam insulation was installed onto the outer metal skin on the stage to help mitigate propellant boiloff inside the tank. | atlas ii | countryorigin | united states <tsp> atlas ii | finalflight | 2002-12-05 <tsp> atlas ii | launchsite | vandenberg air force base <tsp> atlas ii | diameter | 304 m <tsp> atlas ii | launchsite | cape canaveral air force station | atlas ii was developed from the atlas i and featured numerous upgrades over that vehicle.atlas ii was launched from launch complex 36 at cape canaveral space force station in florida as well as space launch complex 3e at vandenberg space force base in california.the increased thrust, engine efficiency, and propellant capacity enabled the vehicle to lift payloads of 6,100 pounds (2,767 kg) into geostationary transfer orbit (gto), or more on later atlas ii variants.atlas ii also featured lower-cost electronics, an improved flight computer, and longer propellant tanks than its predecessor, atlas i. |
aaron turner (born november 5, 1977) is an american musician, singer, graphic artist, and founder of label hydra head records.he is most widely known for his role as guitarist and vocalist for the post-metal bands sumac and isis, while also participating in several other bands and projects such as old man gloom, lotus eaters and split cranium, a collaboration with jussi lehtisalo of finnish band circle who toured with isis in 2009.raised in new mexico, turner moved to the boston area, where he attended art school and formed isis and hydra head.in june 2003, turner moved operations of both the band and label to los angeles, california.turner now resides in vashon, wa which is also the base of operations for hydra head and his various other activities.in partnership with his wife faith coloccia, turner founded another record label, sige, in march 2011.it has gone on to release material from his musical collaboration with coloccia, mamiffer.sige is distributed by the business.at an early age, his family moved to new mexico, where he was raised.his mother was a teacher 'who taught a progressive curriculum' and his father an author, 'mainly [of] non-fiction'.turner describes his upbringing, surrounded by his parents' writer, artist and photographer friends, as 'creatively nurturing'.at age 17, he started a company that sold rare punk rock records via mail-order.he later moved to boston to attend art school at the school of the museum of fine arts, and in 1995 began releasing music.by 1997, the hydra head label was becoming a respectable small record label.turner describes his early industriousness as being motivated in part by boredom: i grew up in new mexico, and there wasn't a whole lot as far as youth culture is concerned.especially when i started to get interested in straight edge and wasn't doing drugs anymore, there was really nothing for me to do.so that was like a big reason for me, i suppose, to become really productive.also, i've never been a really social person.so there's not a lot of time taken up by my social life.and music has always been a very very big part of my life.i guess just a combination of those factors is why everything got started so early.around 1997–99, turner was living with future isis bassist and co-founder jeff caxide; until this point, he had been a member of the bands union suit and hollomen.isis was formed in 1997 out of a dissatisfaction with said bands' musical direction and turner and caxide's respective degrees of creative control.in mid-2009, turner moved from los angeles, where both isis and hydra head records were based at the time, to seattle with his then-girlfriend, faith coloccia; they went on to wed in september of the same year.he has also acquired a custom guitar from the electrical guitar company (as did fellow isis guitarist michael gallagher).in the past, turner has also used a gibson les paul standard, prs ce24, and has played through sunn, mesa boogie, and mackie amplifiers.when playing with isis, turner and his fellow guitarists usually tuned their instruments (low to high) b-f#-b-e-g#-b, to achieve a heavier sound.they also used other tunings, though less frequently, such as f# (octave below)-f#-b-e-g#-b.in 2016, turner described the live rig he used with sumac as consisting of two custom-built guitars from the electrical guitar company.both have lucite bodies and aluminum necks, and custom-wound wide frequency range pickups.the newer of the two—a prototype for a signature model—has a slightly flatter fingerboard radius than the older instrument. | femininism | unmarbled | navette | no related information |
hera (minor planet designation: 103 hera) is a moderately large main-belt asteroid with an orbital period of 4.44 years.it was discovered by canadian-american astronomer james craig watson on september 7, 1868, and named after hera, queen and fifth in power of the olympian gods in greek mythology.this is a stony s-type asteroid with a silicate surface composition.photometric observations made in 2010 at the organ mesa observatory at las cruces, new mexico, and the hunters hill observatory at ngunnawal, australian capital territory, give a synodic rotation period of 23.740±0.001 h. the bimodal light curve shows a maximum brightness variation of 0.45 ± 0.03 in magnitude.measurements made with the iras observatory give a diameter of 91.58±4.14 km and a geometric albedo of 0.19±0.02.by comparison, the mips photometer on the spitzer space telescope gives a diameter of 88.30±8.51 km and a geometric albedo of 0.20±0.04.when the asteroid was observed occulting a star, the chords showed a diameter of 89.1±1.1 km. | 103 hera | discoverer | james craig watson <tsp> james craig watson | almamater | university of michigan <tsp> james craig watson | stateoforigin | canada <tsp> james craig watson | deathplace | madison wisconsin <tsp> james craig watson | deathcause | peritonitis | it was discovered by canadian-american astronomer james craig watson on september 7, 1868, and named after hera, queen and fifth in power of the olympian gods in greek mythology. |
atlas ii was a member of the atlas family of launch vehicles, which evolved from the successful atlas missile program of the 1950s.the atlas ii was a direct evolution of the atlas i, featuring longer first stage tanks, higher-performing engines, and the option for strap-on solid rocket boosters.it was designed to launch payloads into low earth orbit, geosynchronous transfer orbit or geosynchronous orbit.sixty-three launches of the atlas ii, iia and iias models were carried out between 1991 and 2004; all sixty-three launches were successes, making the atlas ii a highly reliable space launch system.the atlas line was continued by the atlas iii, used between 2000 and 2005, and the atlas v which is still in use.additional commercial and u.s. government sales resulted in production increases leading to greater than 60 vehicles being produced and launched.atlas ii was developed from the atlas i and featured numerous upgrades over that vehicle.atlas ii was launched from launch complex 36 at cape canaveral space force station in florida as well as space launch complex 3e at vandenberg space force base in california.all launches were successful.the increased thrust, engine efficiency, and propellant capacity enabled the vehicle to lift payloads of 6,100 pounds (2,767 kg) into geostationary transfer orbit (gto), or more on later atlas ii variants.atlas ii also featured lower-cost electronics, an improved flight computer, and longer propellant tanks than its predecessor, atlas i.the stage was powered by 3 rs-56 rocket engines (derived from the rs-27 main engine of the delta ii rocket) burning 156 t (344,000 lb) of rp-1 and liquid oxygen.the two booster engines were the rs-56-oba variants (the complete assembly of both engines and the aft skirt was referred to as the ma-5a), with high thrust but moderate efficiency.the sustainer (center) engine was the rs-56-osa variant, featuring much less thrust but higher efficiency at high altitudes than the booster engines.the vernier engines used on the first stage of the atlas i (and all previous atlas models) were replaced by a hydrazine-fueled roll control system on atlas ii.this system, mounted on the interstage between the first and second stages, utilized small thrusters to control the vehicle's roll.compared to atlas i, the atlas ii first stage was 2.7 m (8 ft 10 in) taller.the atlas ii was the last atlas rocket to use the 'stage-and-a-half' technique, where it ignited all 3 rs-56 engines at liftoff and then jettisoned the 2 rs-56-oba side engines and their support structure during ascent.the two rs-56-oba engines were integrated into a single unit called the ma-5a and shared a common gas generator.they burned for approximately 164 seconds before being jettisoned, when acceleration reached approximately 5.0-5.5 g. the central sustainer engine on the first stage, an rs-56-osa, would burn for an additional 125 seconds after their jettison.it featured better efficiency at high altitudes than the rs-56-obas.the first stage also had the option to be fitted with 4 castor 4a solid rocket boosters as part of the iias version, each providing an additional 478.3 kn (107,500 lbf) of thrust for 56 seconds.the first two boosters were ignited at liftoff, and the other two were ignited after the first two burnt out.both pairs of boosters were jettisoned shortly after their respective burns.centaur ii featured 2 rl-10a-3-3a engines, burning liquid hydrogen and liquid oxygen.it featured propellant tanks 0.9 meters longer than its predecessor, centaur i, giving the stage more propellant and therefore higher performance.due to the super cold propellants inside centaur, foam insulation was installed onto the outer metal skin on the stage to help mitigate propellant boiloff inside the tank. | atlas ii | countryorigin | united states <tsp> atlas ii | finalflight | 2002-12-05 <tsp> atlas ii | launchsite | vandenberg air force base <tsp> atlas ii | diameter | 304 m <tsp> atlas ii | launchsite | cape canaveral air force station | atlas ii was developed from the atlas i and featured numerous upgrades over that vehicle.atlas ii was launched from launch complex 36 at cape canaveral space force station in florida as well as space launch complex 3e at vandenberg space force base in california.the increased thrust, engine efficiency, and propellant capacity enabled the vehicle to lift payloads of 6,100 pounds (2,767 kg) into geostationary transfer orbit (gto), or more on later atlas ii variants.atlas ii also featured lower-cost electronics, an improved flight computer, and longer propellant tanks than its predecessor, atlas i. |
hera (minor planet designation: 103 hera) is a moderately large main-belt asteroid with an orbital period of 4.44 years.it was discovered by canadian-american astronomer james craig watson on september 7, 1868, and named after hera, queen and fifth in power of the olympian gods in greek mythology.this is a stony s-type asteroid with a silicate surface composition.photometric observations made in 2010 at the organ mesa observatory at las cruces, new mexico, and the hunters hill observatory at ngunnawal, australian capital territory, give a synodic rotation period of 23.740±0.001 h. the bimodal light curve shows a maximum brightness variation of 0.45 ± 0.03 in magnitude.measurements made with the iras observatory give a diameter of 91.58±4.14 km and a geometric albedo of 0.19±0.02.by comparison, the mips photometer on the spitzer space telescope gives a diameter of 88.30±8.51 km and a geometric albedo of 0.20±0.04.when the asteroid was observed occulting a star, the chords showed a diameter of 89.1±1.1 km. | 103 hera | discoverer | james craig watson <tsp> james craig watson | almamater | university of michigan <tsp> james craig watson | stateoforigin | canada <tsp> james craig watson | deathplace | madison wisconsin <tsp> james craig watson | deathcause | peritonitis | it was discovered by canadian-american astronomer james craig watson on september 7, 1868, and named after hera, queen and fifth in power of the olympian gods in greek mythology. |
atlas ii was a member of the atlas family of launch vehicles, which evolved from the successful atlas missile program of the 1950s.the atlas ii was a direct evolution of the atlas i, featuring longer first stage tanks, higher-performing engines, and the option for strap-on solid rocket boosters.it was designed to launch payloads into low earth orbit, geosynchronous transfer orbit or geosynchronous orbit.sixty-three launches of the atlas ii, iia and iias models were carried out between 1991 and 2004; all sixty-three launches were successes, making the atlas ii a highly reliable space launch system.the atlas line was continued by the atlas iii, used between 2000 and 2005, and the atlas v which is still in use.additional commercial and u.s. government sales resulted in production increases leading to greater than 60 vehicles being produced and launched.atlas ii was developed from the atlas i and featured numerous upgrades over that vehicle.atlas ii was launched from launch complex 36 at cape canaveral space force station in florida as well as space launch complex 3e at vandenberg space force base in california.all launches were successful.the increased thrust, engine efficiency, and propellant capacity enabled the vehicle to lift payloads of 6,100 pounds (2,767 kg) into geostationary transfer orbit (gto), or more on later atlas ii variants.atlas ii also featured lower-cost electronics, an improved flight computer, and longer propellant tanks than its predecessor, atlas i.the stage was powered by 3 rs-56 rocket engines (derived from the rs-27 main engine of the delta ii rocket) burning 156 t (344,000 lb) of rp-1 and liquid oxygen.the two booster engines were the rs-56-oba variants (the complete assembly of both engines and the aft skirt was referred to as the ma-5a), with high thrust but moderate efficiency.the sustainer (center) engine was the rs-56-osa variant, featuring much less thrust but higher efficiency at high altitudes than the booster engines.the vernier engines used on the first stage of the atlas i (and all previous atlas models) were replaced by a hydrazine-fueled roll control system on atlas ii.this system, mounted on the interstage between the first and second stages, utilized small thrusters to control the vehicle's roll.compared to atlas i, the atlas ii first stage was 2.7 m (8 ft 10 in) taller.the atlas ii was the last atlas rocket to use the 'stage-and-a-half' technique, where it ignited all 3 rs-56 engines at liftoff and then jettisoned the 2 rs-56-oba side engines and their support structure during ascent.the two rs-56-oba engines were integrated into a single unit called the ma-5a and shared a common gas generator.they burned for approximately 164 seconds before being jettisoned, when acceleration reached approximately 5.0-5.5 g. the central sustainer engine on the first stage, an rs-56-osa, would burn for an additional 125 seconds after their jettison.it featured better efficiency at high altitudes than the rs-56-obas.the first stage also had the option to be fitted with 4 castor 4a solid rocket boosters as part of the iias version, each providing an additional 478.3 kn (107,500 lbf) of thrust for 56 seconds.the first two boosters were ignited at liftoff, and the other two were ignited after the first two burnt out.both pairs of boosters were jettisoned shortly after their respective burns.centaur ii featured 2 rl-10a-3-3a engines, burning liquid hydrogen and liquid oxygen.it featured propellant tanks 0.9 meters longer than its predecessor, centaur i, giving the stage more propellant and therefore higher performance.due to the super cold propellants inside centaur, foam insulation was installed onto the outer metal skin on the stage to help mitigate propellant boiloff inside the tank. | atlas ii | countryorigin | united states <tsp> atlas ii | finalflight | 2004-08-31 <tsp> atlas ii | launchsite | vandenberg air force base <tsp> atlas ii | diameter | 304 m <tsp> atlas ii | launchsite | cape canaveral air force station | atlas ii was developed from the atlas i and featured numerous upgrades over that vehicle.atlas ii was launched from launch complex 36 at cape canaveral space force station in florida as well as space launch complex 3e at vandenberg space force base in california.the increased thrust, engine efficiency, and propellant capacity enabled the vehicle to lift payloads of 6,100 pounds (2,767 kg) into geostationary transfer orbit (gto), or more on later atlas ii variants.atlas ii also featured lower-cost electronics, an improved flight computer, and longer propellant tanks than its predecessor, atlas i. |
aaron turner (born november 5, 1977) is an american musician, singer, graphic artist, and founder of label hydra head records.he is most widely known for his role as guitarist and vocalist for the post-metal bands sumac and isis, while also participating in several other bands and projects such as old man gloom, lotus eaters and split cranium, a collaboration with jussi lehtisalo of finnish band circle who toured with isis in 2009.raised in new mexico, turner moved to the boston area, where he attended art school and formed isis and hydra head.in june 2003, turner moved operations of both the band and label to los angeles, california.turner now resides in vashon, wa which is also the base of operations for hydra head and his various other activities.in partnership with his wife faith coloccia, turner founded another record label, sige, in march 2011.it has gone on to release material from his musical collaboration with coloccia, mamiffer.sige is distributed by the business.at an early age, his family moved to new mexico, where he was raised.his mother was a teacher 'who taught a progressive curriculum' and his father an author, 'mainly [of] non-fiction'.turner describes his upbringing, surrounded by his parents' writer, artist and photographer friends, as 'creatively nurturing'.at age 17, he started a company that sold rare punk rock records via mail-order.he later moved to boston to attend art school at the school of the museum of fine arts, and in 1995 began releasing music.by 1997, the hydra head label was becoming a respectable small record label.turner describes his early industriousness as being motivated in part by boredom: i grew up in new mexico, and there wasn't a whole lot as far as youth culture is concerned.especially when i started to get interested in straight edge and wasn't doing drugs anymore, there was really nothing for me to do.so that was like a big reason for me, i suppose, to become really productive.also, i've never been a really social person.so there's not a lot of time taken up by my social life.and music has always been a very very big part of my life.i guess just a combination of those factors is why everything got started so early.around 1997–99, turner was living with future isis bassist and co-founder jeff caxide; until this point, he had been a member of the bands union suit and hollomen.isis was formed in 1997 out of a dissatisfaction with said bands' musical direction and turner and caxide's respective degrees of creative control.in mid-2009, turner moved from los angeles, where both isis and hydra head records were based at the time, to seattle with his then-girlfriend, faith coloccia; they went on to wed in september of the same year.he has also acquired a custom guitar from the electrical guitar company (as did fellow isis guitarist michael gallagher).in the past, turner has also used a gibson les paul standard, prs ce24, and has played through sunn, mesa boogie, and mackie amplifiers.when playing with isis, turner and his fellow guitarists usually tuned their instruments (low to high) b-f#-b-e-g#-b, to achieve a heavier sound.they also used other tunings, though less frequently, such as f# (octave below)-f#-b-e-g#-b.in 2016, turner described the live rig he used with sumac as consisting of two custom-built guitars from the electrical guitar company.both have lucite bodies and aluminum necks, and custom-wound wide frequency range pickups.the newer of the two—a prototype for a signature model—has a slightly flatter fingerboard radius than the older instrument. | quotable | sculptitory | chesterfieldian <tsp> quotable | centas | urosomite | no related information |
atlas ii was a member of the atlas family of launch vehicles, which evolved from the successful atlas missile program of the 1950s.the atlas ii was a direct evolution of the atlas i, featuring longer first stage tanks, higher-performing engines, and the option for strap-on solid rocket boosters.it was designed to launch payloads into low earth orbit, geosynchronous transfer orbit or geosynchronous orbit.sixty-three launches of the atlas ii, iia and iias models were carried out between 1991 and 2004; all sixty-three launches were successes, making the atlas ii a highly reliable space launch system.the atlas line was continued by the atlas iii, used between 2000 and 2005, and the atlas v which is still in use.additional commercial and u.s. government sales resulted in production increases leading to greater than 60 vehicles being produced and launched.atlas ii was developed from the atlas i and featured numerous upgrades over that vehicle.atlas ii was launched from launch complex 36 at cape canaveral space force station in florida as well as space launch complex 3e at vandenberg space force base in california.all launches were successful.the increased thrust, engine efficiency, and propellant capacity enabled the vehicle to lift payloads of 6,100 pounds (2,767 kg) into geostationary transfer orbit (gto), or more on later atlas ii variants.atlas ii also featured lower-cost electronics, an improved flight computer, and longer propellant tanks than its predecessor, atlas i.the stage was powered by 3 rs-56 rocket engines (derived from the rs-27 main engine of the delta ii rocket) burning 156 t (344,000 lb) of rp-1 and liquid oxygen.the two booster engines were the rs-56-oba variants (the complete assembly of both engines and the aft skirt was referred to as the ma-5a), with high thrust but moderate efficiency.the sustainer (center) engine was the rs-56-osa variant, featuring much less thrust but higher efficiency at high altitudes than the booster engines.the vernier engines used on the first stage of the atlas i (and all previous atlas models) were replaced by a hydrazine-fueled roll control system on atlas ii.this system, mounted on the interstage between the first and second stages, utilized small thrusters to control the vehicle's roll.compared to atlas i, the atlas ii first stage was 2.7 m (8 ft 10 in) taller.the atlas ii was the last atlas rocket to use the 'stage-and-a-half' technique, where it ignited all 3 rs-56 engines at liftoff and then jettisoned the 2 rs-56-oba side engines and their support structure during ascent.the two rs-56-oba engines were integrated into a single unit called the ma-5a and shared a common gas generator.they burned for approximately 164 seconds before being jettisoned, when acceleration reached approximately 5.0-5.5 g. the central sustainer engine on the first stage, an rs-56-osa, would burn for an additional 125 seconds after their jettison.it featured better efficiency at high altitudes than the rs-56-obas.the first stage also had the option to be fitted with 4 castor 4a solid rocket boosters as part of the iias version, each providing an additional 478.3 kn (107,500 lbf) of thrust for 56 seconds.the first two boosters were ignited at liftoff, and the other two were ignited after the first two burnt out.both pairs of boosters were jettisoned shortly after their respective burns.centaur ii featured 2 rl-10a-3-3a engines, burning liquid hydrogen and liquid oxygen.it featured propellant tanks 0.9 meters longer than its predecessor, centaur i, giving the stage more propellant and therefore higher performance.due to the super cold propellants inside centaur, foam insulation was installed onto the outer metal skin on the stage to help mitigate propellant boiloff inside the tank. | atlas ii | countryorigin | united states <tsp> atlas ii | finalflight | 2004-08-31 <tsp> atlas ii | launchsite | vandenberg air force base <tsp> atlas ii | diameter | 304 m <tsp> atlas ii | launchsite | cape canaveral air force station | atlas ii was developed from the atlas i and featured numerous upgrades over that vehicle.atlas ii was launched from launch complex 36 at cape canaveral space force station in florida as well as space launch complex 3e at vandenberg space force base in california.the increased thrust, engine efficiency, and propellant capacity enabled the vehicle to lift payloads of 6,100 pounds (2,767 kg) into geostationary transfer orbit (gto), or more on later atlas ii variants.atlas ii also featured lower-cost electronics, an improved flight computer, and longer propellant tanks than its predecessor, atlas i. |
aaron turner (born november 5, 1977) is an american musician, singer, graphic artist, and founder of label hydra head records.he is most widely known for his role as guitarist and vocalist for the post-metal bands sumac and isis, while also participating in several other bands and projects such as old man gloom, lotus eaters and split cranium, a collaboration with jussi lehtisalo of finnish band circle who toured with isis in 2009.raised in new mexico, turner moved to the boston area, where he attended art school and formed isis and hydra head.in june 2003, turner moved operations of both the band and label to los angeles, california.turner now resides in vashon, wa which is also the base of operations for hydra head and his various other activities.in partnership with his wife faith coloccia, turner founded another record label, sige, in march 2011.it has gone on to release material from his musical collaboration with coloccia, mamiffer.sige is distributed by the business.at an early age, his family moved to new mexico, where he was raised.his mother was a teacher 'who taught a progressive curriculum' and his father an author, 'mainly [of] non-fiction'.turner describes his upbringing, surrounded by his parents' writer, artist and photographer friends, as 'creatively nurturing'.at age 17, he started a company that sold rare punk rock records via mail-order.he later moved to boston to attend art school at the school of the museum of fine arts, and in 1995 began releasing music.by 1997, the hydra head label was becoming a respectable small record label.turner describes his early industriousness as being motivated in part by boredom: i grew up in new mexico, and there wasn't a whole lot as far as youth culture is concerned.especially when i started to get interested in straight edge and wasn't doing drugs anymore, there was really nothing for me to do.so that was like a big reason for me, i suppose, to become really productive.also, i've never been a really social person.so there's not a lot of time taken up by my social life.and music has always been a very very big part of my life.i guess just a combination of those factors is why everything got started so early.around 1997–99, turner was living with future isis bassist and co-founder jeff caxide; until this point, he had been a member of the bands union suit and hollomen.isis was formed in 1997 out of a dissatisfaction with said bands' musical direction and turner and caxide's respective degrees of creative control.in mid-2009, turner moved from los angeles, where both isis and hydra head records were based at the time, to seattle with his then-girlfriend, faith coloccia; they went on to wed in september of the same year.he has also acquired a custom guitar from the electrical guitar company (as did fellow isis guitarist michael gallagher).in the past, turner has also used a gibson les paul standard, prs ce24, and has played through sunn, mesa boogie, and mackie amplifiers.when playing with isis, turner and his fellow guitarists usually tuned their instruments (low to high) b-f#-b-e-g#-b, to achieve a heavier sound.they also used other tunings, though less frequently, such as f# (octave below)-f#-b-e-g#-b.in 2016, turner described the live rig he used with sumac as consisting of two custom-built guitars from the electrical guitar company.both have lucite bodies and aluminum necks, and custom-wound wide frequency range pickups.the newer of the two—a prototype for a signature model—has a slightly flatter fingerboard radius than the older instrument. | straddlebug | passenger | adenoses | no related information |
hera (minor planet designation: 103 hera) is a moderately large main-belt asteroid with an orbital period of 4.44 years.it was discovered by canadian-american astronomer james craig watson on september 7, 1868, and named after hera, queen and fifth in power of the olympian gods in greek mythology.this is a stony s-type asteroid with a silicate surface composition.photometric observations made in 2010 at the organ mesa observatory at las cruces, new mexico, and the hunters hill observatory at ngunnawal, australian capital territory, give a synodic rotation period of 23.740±0.001 h. the bimodal light curve shows a maximum brightness variation of 0.45 ± 0.03 in magnitude.measurements made with the iras observatory give a diameter of 91.58±4.14 km and a geometric albedo of 0.19±0.02.by comparison, the mips photometer on the spitzer space telescope gives a diameter of 88.30±8.51 km and a geometric albedo of 0.20±0.04.when the asteroid was observed occulting a star, the chords showed a diameter of 89.1±1.1 km. | vitiligoid | consumating | ryots <tsp> vitiligoid | interester | ranid | no related information |
atlas ii was a member of the atlas family of launch vehicles, which evolved from the successful atlas missile program of the 1950s.the atlas ii was a direct evolution of the atlas i, featuring longer first stage tanks, higher-performing engines, and the option for strap-on solid rocket boosters.it was designed to launch payloads into low earth orbit, geosynchronous transfer orbit or geosynchronous orbit.sixty-three launches of the atlas ii, iia and iias models were carried out between 1991 and 2004; all sixty-three launches were successes, making the atlas ii a highly reliable space launch system.the atlas line was continued by the atlas iii, used between 2000 and 2005, and the atlas v which is still in use.additional commercial and u.s. government sales resulted in production increases leading to greater than 60 vehicles being produced and launched.atlas ii was developed from the atlas i and featured numerous upgrades over that vehicle.atlas ii was launched from launch complex 36 at cape canaveral space force station in florida as well as space launch complex 3e at vandenberg space force base in california.all launches were successful.the increased thrust, engine efficiency, and propellant capacity enabled the vehicle to lift payloads of 6,100 pounds (2,767 kg) into geostationary transfer orbit (gto), or more on later atlas ii variants.atlas ii also featured lower-cost electronics, an improved flight computer, and longer propellant tanks than its predecessor, atlas i.the stage was powered by 3 rs-56 rocket engines (derived from the rs-27 main engine of the delta ii rocket) burning 156 t (344,000 lb) of rp-1 and liquid oxygen.the two booster engines were the rs-56-oba variants (the complete assembly of both engines and the aft skirt was referred to as the ma-5a), with high thrust but moderate efficiency.the sustainer (center) engine was the rs-56-osa variant, featuring much less thrust but higher efficiency at high altitudes than the booster engines.the vernier engines used on the first stage of the atlas i (and all previous atlas models) were replaced by a hydrazine-fueled roll control system on atlas ii.this system, mounted on the interstage between the first and second stages, utilized small thrusters to control the vehicle's roll.compared to atlas i, the atlas ii first stage was 2.7 m (8 ft 10 in) taller.the atlas ii was the last atlas rocket to use the 'stage-and-a-half' technique, where it ignited all 3 rs-56 engines at liftoff and then jettisoned the 2 rs-56-oba side engines and their support structure during ascent.the two rs-56-oba engines were integrated into a single unit called the ma-5a and shared a common gas generator.they burned for approximately 164 seconds before being jettisoned, when acceleration reached approximately 5.0-5.5 g. the central sustainer engine on the first stage, an rs-56-osa, would burn for an additional 125 seconds after their jettison.it featured better efficiency at high altitudes than the rs-56-obas.the first stage also had the option to be fitted with 4 castor 4a solid rocket boosters as part of the iias version, each providing an additional 478.3 kn (107,500 lbf) of thrust for 56 seconds.the first two boosters were ignited at liftoff, and the other two were ignited after the first two burnt out.both pairs of boosters were jettisoned shortly after their respective burns.centaur ii featured 2 rl-10a-3-3a engines, burning liquid hydrogen and liquid oxygen.it featured propellant tanks 0.9 meters longer than its predecessor, centaur i, giving the stage more propellant and therefore higher performance.due to the super cold propellants inside centaur, foam insulation was installed onto the outer metal skin on the stage to help mitigate propellant boiloff inside the tank. | unrebuked | heptatomic | mopehawk | no related information |
aaron turner (born november 5, 1977) is an american musician, singer, graphic artist, and founder of label hydra head records.he is most widely known for his role as guitarist and vocalist for the post-metal bands sumac and isis, while also participating in several other bands and projects such as old man gloom, lotus eaters and split cranium, a collaboration with jussi lehtisalo of finnish band circle who toured with isis in 2009.raised in new mexico, turner moved to the boston area, where he attended art school and formed isis and hydra head.in june 2003, turner moved operations of both the band and label to los angeles, california.turner now resides in vashon, wa which is also the base of operations for hydra head and his various other activities.in partnership with his wife faith coloccia, turner founded another record label, sige, in march 2011.it has gone on to release material from his musical collaboration with coloccia, mamiffer.sige is distributed by the business.at an early age, his family moved to new mexico, where he was raised.his mother was a teacher 'who taught a progressive curriculum' and his father an author, 'mainly [of] non-fiction'.turner describes his upbringing, surrounded by his parents' writer, artist and photographer friends, as 'creatively nurturing'.at age 17, he started a company that sold rare punk rock records via mail-order.he later moved to boston to attend art school at the school of the museum of fine arts, and in 1995 began releasing music.by 1997, the hydra head label was becoming a respectable small record label.turner describes his early industriousness as being motivated in part by boredom: i grew up in new mexico, and there wasn't a whole lot as far as youth culture is concerned.especially when i started to get interested in straight edge and wasn't doing drugs anymore, there was really nothing for me to do.so that was like a big reason for me, i suppose, to become really productive.also, i've never been a really social person.so there's not a lot of time taken up by my social life.and music has always been a very very big part of my life.i guess just a combination of those factors is why everything got started so early.around 1997–99, turner was living with future isis bassist and co-founder jeff caxide; until this point, he had been a member of the bands union suit and hollomen.isis was formed in 1997 out of a dissatisfaction with said bands' musical direction and turner and caxide's respective degrees of creative control.in mid-2009, turner moved from los angeles, where both isis and hydra head records were based at the time, to seattle with his then-girlfriend, faith coloccia; they went on to wed in september of the same year.he has also acquired a custom guitar from the electrical guitar company (as did fellow isis guitarist michael gallagher).in the past, turner has also used a gibson les paul standard, prs ce24, and has played through sunn, mesa boogie, and mackie amplifiers.when playing with isis, turner and his fellow guitarists usually tuned their instruments (low to high) b-f#-b-e-g#-b, to achieve a heavier sound.they also used other tunings, though less frequently, such as f# (octave below)-f#-b-e-g#-b.in 2016, turner described the live rig he used with sumac as consisting of two custom-built guitars from the electrical guitar company.both have lucite bodies and aluminum necks, and custom-wound wide frequency range pickups.the newer of the two—a prototype for a signature model—has a slightly flatter fingerboard radius than the older instrument. | unjogged | currane | sicklies <tsp> unjogged | accusatively | redwares | no related information |
atlas ii was a member of the atlas family of launch vehicles, which evolved from the successful atlas missile program of the 1950s.the atlas ii was a direct evolution of the atlas i, featuring longer first stage tanks, higher-performing engines, and the option for strap-on solid rocket boosters.it was designed to launch payloads into low earth orbit, geosynchronous transfer orbit or geosynchronous orbit.sixty-three launches of the atlas ii, iia and iias models were carried out between 1991 and 2004; all sixty-three launches were successes, making the atlas ii a highly reliable space launch system.the atlas line was continued by the atlas iii, used between 2000 and 2005, and the atlas v which is still in use.additional commercial and u.s. government sales resulted in production increases leading to greater than 60 vehicles being produced and launched.atlas ii was developed from the atlas i and featured numerous upgrades over that vehicle.atlas ii was launched from launch complex 36 at cape canaveral space force station in florida as well as space launch complex 3e at vandenberg space force base in california.all launches were successful.the increased thrust, engine efficiency, and propellant capacity enabled the vehicle to lift payloads of 6,100 pounds (2,767 kg) into geostationary transfer orbit (gto), or more on later atlas ii variants.atlas ii also featured lower-cost electronics, an improved flight computer, and longer propellant tanks than its predecessor, atlas i.the stage was powered by 3 rs-56 rocket engines (derived from the rs-27 main engine of the delta ii rocket) burning 156 t (344,000 lb) of rp-1 and liquid oxygen.the two booster engines were the rs-56-oba variants (the complete assembly of both engines and the aft skirt was referred to as the ma-5a), with high thrust but moderate efficiency.the sustainer (center) engine was the rs-56-osa variant, featuring much less thrust but higher efficiency at high altitudes than the booster engines.the vernier engines used on the first stage of the atlas i (and all previous atlas models) were replaced by a hydrazine-fueled roll control system on atlas ii.this system, mounted on the interstage between the first and second stages, utilized small thrusters to control the vehicle's roll.compared to atlas i, the atlas ii first stage was 2.7 m (8 ft 10 in) taller.the atlas ii was the last atlas rocket to use the 'stage-and-a-half' technique, where it ignited all 3 rs-56 engines at liftoff and then jettisoned the 2 rs-56-oba side engines and their support structure during ascent.the two rs-56-oba engines were integrated into a single unit called the ma-5a and shared a common gas generator.they burned for approximately 164 seconds before being jettisoned, when acceleration reached approximately 5.0-5.5 g. the central sustainer engine on the first stage, an rs-56-osa, would burn for an additional 125 seconds after their jettison.it featured better efficiency at high altitudes than the rs-56-obas.the first stage also had the option to be fitted with 4 castor 4a solid rocket boosters as part of the iias version, each providing an additional 478.3 kn (107,500 lbf) of thrust for 56 seconds.the first two boosters were ignited at liftoff, and the other two were ignited after the first two burnt out.both pairs of boosters were jettisoned shortly after their respective burns.centaur ii featured 2 rl-10a-3-3a engines, burning liquid hydrogen and liquid oxygen.it featured propellant tanks 0.9 meters longer than its predecessor, centaur i, giving the stage more propellant and therefore higher performance.due to the super cold propellants inside centaur, foam insulation was installed onto the outer metal skin on the stage to help mitigate propellant boiloff inside the tank. | stion | resoluble | cowwheat | no related information |
hera (minor planet designation: 103 hera) is a moderately large main-belt asteroid with an orbital period of 4.44 years.it was discovered by canadian-american astronomer james craig watson on september 7, 1868, and named after hera, queen and fifth in power of the olympian gods in greek mythology.this is a stony s-type asteroid with a silicate surface composition.photometric observations made in 2010 at the organ mesa observatory at las cruces, new mexico, and the hunters hill observatory at ngunnawal, australian capital territory, give a synodic rotation period of 23.740±0.001 h. the bimodal light curve shows a maximum brightness variation of 0.45 ± 0.03 in magnitude.measurements made with the iras observatory give a diameter of 91.58±4.14 km and a geometric albedo of 0.19±0.02.by comparison, the mips photometer on the spitzer space telescope gives a diameter of 88.30±8.51 km and a geometric albedo of 0.20±0.04.when the asteroid was observed occulting a star, the chords showed a diameter of 89.1±1.1 km. | mesoarial | contraorbitally | tricephalic <tsp> mesoarial | spiritualizing | sickling | no related information |
aaron turner (born november 5, 1977) is an american musician, singer, graphic artist, and founder of label hydra head records.he is most widely known for his role as guitarist and vocalist for the post-metal bands sumac and isis, while also participating in several other bands and projects such as old man gloom, lotus eaters and split cranium, a collaboration with jussi lehtisalo of finnish band circle who toured with isis in 2009.raised in new mexico, turner moved to the boston area, where he attended art school and formed isis and hydra head.in june 2003, turner moved operations of both the band and label to los angeles, california.turner now resides in vashon, wa which is also the base of operations for hydra head and his various other activities.in partnership with his wife faith coloccia, turner founded another record label, sige, in march 2011.it has gone on to release material from his musical collaboration with coloccia, mamiffer.sige is distributed by the business.at an early age, his family moved to new mexico, where he was raised.his mother was a teacher 'who taught a progressive curriculum' and his father an author, 'mainly [of] non-fiction'.turner describes his upbringing, surrounded by his parents' writer, artist and photographer friends, as 'creatively nurturing'.at age 17, he started a company that sold rare punk rock records via mail-order.he later moved to boston to attend art school at the school of the museum of fine arts, and in 1995 began releasing music.by 1997, the hydra head label was becoming a respectable small record label.turner describes his early industriousness as being motivated in part by boredom: i grew up in new mexico, and there wasn't a whole lot as far as youth culture is concerned.especially when i started to get interested in straight edge and wasn't doing drugs anymore, there was really nothing for me to do.so that was like a big reason for me, i suppose, to become really productive.also, i've never been a really social person.so there's not a lot of time taken up by my social life.and music has always been a very very big part of my life.i guess just a combination of those factors is why everything got started so early.around 1997–99, turner was living with future isis bassist and co-founder jeff caxide; until this point, he had been a member of the bands union suit and hollomen.isis was formed in 1997 out of a dissatisfaction with said bands' musical direction and turner and caxide's respective degrees of creative control.in mid-2009, turner moved from los angeles, where both isis and hydra head records were based at the time, to seattle with his then-girlfriend, faith coloccia; they went on to wed in september of the same year.he has also acquired a custom guitar from the electrical guitar company (as did fellow isis guitarist michael gallagher).in the past, turner has also used a gibson les paul standard, prs ce24, and has played through sunn, mesa boogie, and mackie amplifiers.when playing with isis, turner and his fellow guitarists usually tuned their instruments (low to high) b-f#-b-e-g#-b, to achieve a heavier sound.they also used other tunings, though less frequently, such as f# (octave below)-f#-b-e-g#-b.in 2016, turner described the live rig he used with sumac as consisting of two custom-built guitars from the electrical guitar company.both have lucite bodies and aluminum necks, and custom-wound wide frequency range pickups.the newer of the two—a prototype for a signature model—has a slightly flatter fingerboard radius than the older instrument. | aaron turner | associatedband/associatedmusicalartist | twilight band <tsp> aaron turner | associatedband/associatedmusicalartist | lotus eaters band <tsp> aaron turner | genre | progressive metal <tsp> aaron turner | origin | massachusetts <tsp> aaron turner | activeyearsstartyear | 1995 | no related information |
hera (minor planet designation: 103 hera) is a moderately large main-belt asteroid with an orbital period of 4.44 years.it was discovered by canadian-american astronomer james craig watson on september 7, 1868, and named after hera, queen and fifth in power of the olympian gods in greek mythology.this is a stony s-type asteroid with a silicate surface composition.photometric observations made in 2010 at the organ mesa observatory at las cruces, new mexico, and the hunters hill observatory at ngunnawal, australian capital territory, give a synodic rotation period of 23.740±0.001 h. the bimodal light curve shows a maximum brightness variation of 0.45 ± 0.03 in magnitude.measurements made with the iras observatory give a diameter of 91.58±4.14 km and a geometric albedo of 0.19±0.02.by comparison, the mips photometer on the spitzer space telescope gives a diameter of 88.30±8.51 km and a geometric albedo of 0.20±0.04.when the asteroid was observed occulting a star, the chords showed a diameter of 89.1±1.1 km. | itll | whensomever | cushlamochree | no related information |
atlas ii was a member of the atlas family of launch vehicles, which evolved from the successful atlas missile program of the 1950s.the atlas ii was a direct evolution of the atlas i, featuring longer first stage tanks, higher-performing engines, and the option for strap-on solid rocket boosters.it was designed to launch payloads into low earth orbit, geosynchronous transfer orbit or geosynchronous orbit.sixty-three launches of the atlas ii, iia and iias models were carried out between 1991 and 2004; all sixty-three launches were successes, making the atlas ii a highly reliable space launch system.the atlas line was continued by the atlas iii, used between 2000 and 2005, and the atlas v which is still in use.additional commercial and u.s. government sales resulted in production increases leading to greater than 60 vehicles being produced and launched.atlas ii was developed from the atlas i and featured numerous upgrades over that vehicle.atlas ii was launched from launch complex 36 at cape canaveral space force station in florida as well as space launch complex 3e at vandenberg space force base in california.all launches were successful.the increased thrust, engine efficiency, and propellant capacity enabled the vehicle to lift payloads of 6,100 pounds (2,767 kg) into geostationary transfer orbit (gto), or more on later atlas ii variants.atlas ii also featured lower-cost electronics, an improved flight computer, and longer propellant tanks than its predecessor, atlas i.the stage was powered by 3 rs-56 rocket engines (derived from the rs-27 main engine of the delta ii rocket) burning 156 t (344,000 lb) of rp-1 and liquid oxygen.the two booster engines were the rs-56-oba variants (the complete assembly of both engines and the aft skirt was referred to as the ma-5a), with high thrust but moderate efficiency.the sustainer (center) engine was the rs-56-osa variant, featuring much less thrust but higher efficiency at high altitudes than the booster engines.the vernier engines used on the first stage of the atlas i (and all previous atlas models) were replaced by a hydrazine-fueled roll control system on atlas ii.this system, mounted on the interstage between the first and second stages, utilized small thrusters to control the vehicle's roll.compared to atlas i, the atlas ii first stage was 2.7 m (8 ft 10 in) taller.the atlas ii was the last atlas rocket to use the 'stage-and-a-half' technique, where it ignited all 3 rs-56 engines at liftoff and then jettisoned the 2 rs-56-oba side engines and their support structure during ascent.the two rs-56-oba engines were integrated into a single unit called the ma-5a and shared a common gas generator.they burned for approximately 164 seconds before being jettisoned, when acceleration reached approximately 5.0-5.5 g. the central sustainer engine on the first stage, an rs-56-osa, would burn for an additional 125 seconds after their jettison.it featured better efficiency at high altitudes than the rs-56-obas.the first stage also had the option to be fitted with 4 castor 4a solid rocket boosters as part of the iias version, each providing an additional 478.3 kn (107,500 lbf) of thrust for 56 seconds.the first two boosters were ignited at liftoff, and the other two were ignited after the first two burnt out.both pairs of boosters were jettisoned shortly after their respective burns.centaur ii featured 2 rl-10a-3-3a engines, burning liquid hydrogen and liquid oxygen.it featured propellant tanks 0.9 meters longer than its predecessor, centaur i, giving the stage more propellant and therefore higher performance.due to the super cold propellants inside centaur, foam insulation was installed onto the outer metal skin on the stage to help mitigate propellant boiloff inside the tank. | adagial | idoist | polysyllabism <tsp> adagial | shpt | araucarian | no related information |
hera (minor planet designation: 103 hera) is a moderately large main-belt asteroid with an orbital period of 4.44 years.it was discovered by canadian-american astronomer james craig watson on september 7, 1868, and named after hera, queen and fifth in power of the olympian gods in greek mythology.this is a stony s-type asteroid with a silicate surface composition.photometric observations made in 2010 at the organ mesa observatory at las cruces, new mexico, and the hunters hill observatory at ngunnawal, australian capital territory, give a synodic rotation period of 23.740±0.001 h. the bimodal light curve shows a maximum brightness variation of 0.45 ± 0.03 in magnitude.measurements made with the iras observatory give a diameter of 91.58±4.14 km and a geometric albedo of 0.19±0.02.by comparison, the mips photometer on the spitzer space telescope gives a diameter of 88.30±8.51 km and a geometric albedo of 0.20±0.04.when the asteroid was observed occulting a star, the chords showed a diameter of 89.1±1.1 km. | 103 hera | epoch | 2011-08-27 <tsp> 103 hera | mass | 79 kilograms <tsp> 103 hera | orbitalperiod | 1622213 days <tsp> 103 hera | periapsis | 3712400000 kilometres <tsp> 103 hera | apoapsis | 4371700000 kilometres | no related information |
aaron turner (born november 5, 1977) is an american musician, singer, graphic artist, and founder of label hydra head records.he is most widely known for his role as guitarist and vocalist for the post-metal bands sumac and isis, while also participating in several other bands and projects such as old man gloom, lotus eaters and split cranium, a collaboration with jussi lehtisalo of finnish band circle who toured with isis in 2009.raised in new mexico, turner moved to the boston area, where he attended art school and formed isis and hydra head.in june 2003, turner moved operations of both the band and label to los angeles, california.turner now resides in vashon, wa which is also the base of operations for hydra head and his various other activities.in partnership with his wife faith coloccia, turner founded another record label, sige, in march 2011.it has gone on to release material from his musical collaboration with coloccia, mamiffer.sige is distributed by the business.at an early age, his family moved to new mexico, where he was raised.his mother was a teacher 'who taught a progressive curriculum' and his father an author, 'mainly [of] non-fiction'.turner describes his upbringing, surrounded by his parents' writer, artist and photographer friends, as 'creatively nurturing'.at age 17, he started a company that sold rare punk rock records via mail-order.he later moved to boston to attend art school at the school of the museum of fine arts, and in 1995 began releasing music.by 1997, the hydra head label was becoming a respectable small record label.turner describes his early industriousness as being motivated in part by boredom: i grew up in new mexico, and there wasn't a whole lot as far as youth culture is concerned.especially when i started to get interested in straight edge and wasn't doing drugs anymore, there was really nothing for me to do.so that was like a big reason for me, i suppose, to become really productive.also, i've never been a really social person.so there's not a lot of time taken up by my social life.and music has always been a very very big part of my life.i guess just a combination of those factors is why everything got started so early.around 1997–99, turner was living with future isis bassist and co-founder jeff caxide; until this point, he had been a member of the bands union suit and hollomen.isis was formed in 1997 out of a dissatisfaction with said bands' musical direction and turner and caxide's respective degrees of creative control.in mid-2009, turner moved from los angeles, where both isis and hydra head records were based at the time, to seattle with his then-girlfriend, faith coloccia; they went on to wed in september of the same year.he has also acquired a custom guitar from the electrical guitar company (as did fellow isis guitarist michael gallagher).in the past, turner has also used a gibson les paul standard, prs ce24, and has played through sunn, mesa boogie, and mackie amplifiers.when playing with isis, turner and his fellow guitarists usually tuned their instruments (low to high) b-f#-b-e-g#-b, to achieve a heavier sound.they also used other tunings, though less frequently, such as f# (octave below)-f#-b-e-g#-b.in 2016, turner described the live rig he used with sumac as consisting of two custom-built guitars from the electrical guitar company.both have lucite bodies and aluminum necks, and custom-wound wide frequency range pickups.the newer of the two—a prototype for a signature model—has a slightly flatter fingerboard radius than the older instrument. | dink | reinaugurating | spiritedness <tsp> dink | bakership | summonsed | no related information |
atlas ii was a member of the atlas family of launch vehicles, which evolved from the successful atlas missile program of the 1950s.the atlas ii was a direct evolution of the atlas i, featuring longer first stage tanks, higher-performing engines, and the option for strap-on solid rocket boosters.it was designed to launch payloads into low earth orbit, geosynchronous transfer orbit or geosynchronous orbit.sixty-three launches of the atlas ii, iia and iias models were carried out between 1991 and 2004; all sixty-three launches were successes, making the atlas ii a highly reliable space launch system.the atlas line was continued by the atlas iii, used between 2000 and 2005, and the atlas v which is still in use.additional commercial and u.s. government sales resulted in production increases leading to greater than 60 vehicles being produced and launched.atlas ii was developed from the atlas i and featured numerous upgrades over that vehicle.atlas ii was launched from launch complex 36 at cape canaveral space force station in florida as well as space launch complex 3e at vandenberg space force base in california.all launches were successful.the increased thrust, engine efficiency, and propellant capacity enabled the vehicle to lift payloads of 6,100 pounds (2,767 kg) into geostationary transfer orbit (gto), or more on later atlas ii variants.atlas ii also featured lower-cost electronics, an improved flight computer, and longer propellant tanks than its predecessor, atlas i.the stage was powered by 3 rs-56 rocket engines (derived from the rs-27 main engine of the delta ii rocket) burning 156 t (344,000 lb) of rp-1 and liquid oxygen.the two booster engines were the rs-56-oba variants (the complete assembly of both engines and the aft skirt was referred to as the ma-5a), with high thrust but moderate efficiency.the sustainer (center) engine was the rs-56-osa variant, featuring much less thrust but higher efficiency at high altitudes than the booster engines.the vernier engines used on the first stage of the atlas i (and all previous atlas models) were replaced by a hydrazine-fueled roll control system on atlas ii.this system, mounted on the interstage between the first and second stages, utilized small thrusters to control the vehicle's roll.compared to atlas i, the atlas ii first stage was 2.7 m (8 ft 10 in) taller.the atlas ii was the last atlas rocket to use the 'stage-and-a-half' technique, where it ignited all 3 rs-56 engines at liftoff and then jettisoned the 2 rs-56-oba side engines and their support structure during ascent.the two rs-56-oba engines were integrated into a single unit called the ma-5a and shared a common gas generator.they burned for approximately 164 seconds before being jettisoned, when acceleration reached approximately 5.0-5.5 g. the central sustainer engine on the first stage, an rs-56-osa, would burn for an additional 125 seconds after their jettison.it featured better efficiency at high altitudes than the rs-56-obas.the first stage also had the option to be fitted with 4 castor 4a solid rocket boosters as part of the iias version, each providing an additional 478.3 kn (107,500 lbf) of thrust for 56 seconds.the first two boosters were ignited at liftoff, and the other two were ignited after the first two burnt out.both pairs of boosters were jettisoned shortly after their respective burns.centaur ii featured 2 rl-10a-3-3a engines, burning liquid hydrogen and liquid oxygen.it featured propellant tanks 0.9 meters longer than its predecessor, centaur i, giving the stage more propellant and therefore higher performance.due to the super cold propellants inside centaur, foam insulation was installed onto the outer metal skin on the stage to help mitigate propellant boiloff inside the tank. | palenesses | naturalesque | sprangly | no related information |
hera (minor planet designation: 103 hera) is a moderately large main-belt asteroid with an orbital period of 4.44 years.it was discovered by canadian-american astronomer james craig watson on september 7, 1868, and named after hera, queen and fifth in power of the olympian gods in greek mythology.this is a stony s-type asteroid with a silicate surface composition.photometric observations made in 2010 at the organ mesa observatory at las cruces, new mexico, and the hunters hill observatory at ngunnawal, australian capital territory, give a synodic rotation period of 23.740±0.001 h. the bimodal light curve shows a maximum brightness variation of 0.45 ± 0.03 in magnitude.measurements made with the iras observatory give a diameter of 91.58±4.14 km and a geometric albedo of 0.19±0.02.by comparison, the mips photometer on the spitzer space telescope gives a diameter of 88.30±8.51 km and a geometric albedo of 0.20±0.04.when the asteroid was observed occulting a star, the chords showed a diameter of 89.1±1.1 km. | 103 hera | epoch | 2011-08-27 <tsp> 103 hera | mass | 79 kilograms <tsp> 103 hera | orbitalperiod | 1622213 days <tsp> 103 hera | periapsis | 3712400000 kilometres <tsp> 103 hera | apoapsis | 4371700000 kilometres | no related information |
atlas ii was a member of the atlas family of launch vehicles, which evolved from the successful atlas missile program of the 1950s.the atlas ii was a direct evolution of the atlas i, featuring longer first stage tanks, higher-performing engines, and the option for strap-on solid rocket boosters.it was designed to launch payloads into low earth orbit, geosynchronous transfer orbit or geosynchronous orbit.sixty-three launches of the atlas ii, iia and iias models were carried out between 1991 and 2004; all sixty-three launches were successes, making the atlas ii a highly reliable space launch system.the atlas line was continued by the atlas iii, used between 2000 and 2005, and the atlas v which is still in use.additional commercial and u.s. government sales resulted in production increases leading to greater than 60 vehicles being produced and launched.atlas ii was developed from the atlas i and featured numerous upgrades over that vehicle.atlas ii was launched from launch complex 36 at cape canaveral space force station in florida as well as space launch complex 3e at vandenberg space force base in california.all launches were successful.the increased thrust, engine efficiency, and propellant capacity enabled the vehicle to lift payloads of 6,100 pounds (2,767 kg) into geostationary transfer orbit (gto), or more on later atlas ii variants.atlas ii also featured lower-cost electronics, an improved flight computer, and longer propellant tanks than its predecessor, atlas i.the stage was powered by 3 rs-56 rocket engines (derived from the rs-27 main engine of the delta ii rocket) burning 156 t (344,000 lb) of rp-1 and liquid oxygen.the two booster engines were the rs-56-oba variants (the complete assembly of both engines and the aft skirt was referred to as the ma-5a), with high thrust but moderate efficiency.the sustainer (center) engine was the rs-56-osa variant, featuring much less thrust but higher efficiency at high altitudes than the booster engines.the vernier engines used on the first stage of the atlas i (and all previous atlas models) were replaced by a hydrazine-fueled roll control system on atlas ii.this system, mounted on the interstage between the first and second stages, utilized small thrusters to control the vehicle's roll.compared to atlas i, the atlas ii first stage was 2.7 m (8 ft 10 in) taller.the atlas ii was the last atlas rocket to use the 'stage-and-a-half' technique, where it ignited all 3 rs-56 engines at liftoff and then jettisoned the 2 rs-56-oba side engines and their support structure during ascent.the two rs-56-oba engines were integrated into a single unit called the ma-5a and shared a common gas generator.they burned for approximately 164 seconds before being jettisoned, when acceleration reached approximately 5.0-5.5 g. the central sustainer engine on the first stage, an rs-56-osa, would burn for an additional 125 seconds after their jettison.it featured better efficiency at high altitudes than the rs-56-obas.the first stage also had the option to be fitted with 4 castor 4a solid rocket boosters as part of the iias version, each providing an additional 478.3 kn (107,500 lbf) of thrust for 56 seconds.the first two boosters were ignited at liftoff, and the other two were ignited after the first two burnt out.both pairs of boosters were jettisoned shortly after their respective burns.centaur ii featured 2 rl-10a-3-3a engines, burning liquid hydrogen and liquid oxygen.it featured propellant tanks 0.9 meters longer than its predecessor, centaur i, giving the stage more propellant and therefore higher performance.due to the super cold propellants inside centaur, foam insulation was installed onto the outer metal skin on the stage to help mitigate propellant boiloff inside the tank. | atlas ii | launchsite | cape canaveral air force station <tsp> atlas ii | countryorigin | united states <tsp> atlas ii | finalflight | 1998-03-16 <tsp> atlas ii | diameter | 304 m <tsp> atlas ii | launchsite | spaceport florida launch complex 36 | atlas ii was a member of the atlas family of launch vehicles, which evolved from the successful atlas missile program of the 1950s.sixty-three launches of the atlas ii, iia and iias models were carried out between 1991 and 2004; all sixty-three launches were successes, making the atlas ii a highly reliable space launch system.atlas ii was developed from the atlas i and featured numerous upgrades over that vehicle.atlas ii was launched from launch complex 36 at cape canaveral space force station in florida as well as space launch complex 3e at vandenberg space force base in california.the increased thrust, engine efficiency, and propellant capacity enabled the vehicle to lift payloads of 6,100 pounds (2,767 kg) into geostationary transfer orbit (gto), or more on later atlas ii variants.atlas ii also featured lower-cost electronics, an improved flight computer, and longer propellant tanks than its predecessor, atlas i. |
hera (minor planet designation: 103 hera) is a moderately large main-belt asteroid with an orbital period of 4.44 years.it was discovered by canadian-american astronomer james craig watson on september 7, 1868, and named after hera, queen and fifth in power of the olympian gods in greek mythology.this is a stony s-type asteroid with a silicate surface composition.photometric observations made in 2010 at the organ mesa observatory at las cruces, new mexico, and the hunters hill observatory at ngunnawal, australian capital territory, give a synodic rotation period of 23.740±0.001 h. the bimodal light curve shows a maximum brightness variation of 0.45 ± 0.03 in magnitude.measurements made with the iras observatory give a diameter of 91.58±4.14 km and a geometric albedo of 0.19±0.02.by comparison, the mips photometer on the spitzer space telescope gives a diameter of 88.30±8.51 km and a geometric albedo of 0.20±0.04.when the asteroid was observed occulting a star, the chords showed a diameter of 89.1±1.1 km. | 103 hera | epoch | 2011-08-27 <tsp> 103 hera | mass | 79 kilograms <tsp> 103 hera | orbitalperiod | 1622213 days <tsp> 103 hera | periapsis | 3712400000 kilometres <tsp> 103 hera | apoapsis | 4371700000 kilometres | no related information |
aaron turner (born november 5, 1977) is an american musician, singer, graphic artist, and founder of label hydra head records.he is most widely known for his role as guitarist and vocalist for the post-metal bands sumac and isis, while also participating in several other bands and projects such as old man gloom, lotus eaters and split cranium, a collaboration with jussi lehtisalo of finnish band circle who toured with isis in 2009.raised in new mexico, turner moved to the boston area, where he attended art school and formed isis and hydra head.in june 2003, turner moved operations of both the band and label to los angeles, california.turner now resides in vashon, wa which is also the base of operations for hydra head and his various other activities.in partnership with his wife faith coloccia, turner founded another record label, sige, in march 2011.it has gone on to release material from his musical collaboration with coloccia, mamiffer.sige is distributed by the business.at an early age, his family moved to new mexico, where he was raised.his mother was a teacher 'who taught a progressive curriculum' and his father an author, 'mainly [of] non-fiction'.turner describes his upbringing, surrounded by his parents' writer, artist and photographer friends, as 'creatively nurturing'.at age 17, he started a company that sold rare punk rock records via mail-order.he later moved to boston to attend art school at the school of the museum of fine arts, and in 1995 began releasing music.by 1997, the hydra head label was becoming a respectable small record label.turner describes his early industriousness as being motivated in part by boredom: i grew up in new mexico, and there wasn't a whole lot as far as youth culture is concerned.especially when i started to get interested in straight edge and wasn't doing drugs anymore, there was really nothing for me to do.so that was like a big reason for me, i suppose, to become really productive.also, i've never been a really social person.so there's not a lot of time taken up by my social life.and music has always been a very very big part of my life.i guess just a combination of those factors is why everything got started so early.around 1997–99, turner was living with future isis bassist and co-founder jeff caxide; until this point, he had been a member of the bands union suit and hollomen.isis was formed in 1997 out of a dissatisfaction with said bands' musical direction and turner and caxide's respective degrees of creative control.in mid-2009, turner moved from los angeles, where both isis and hydra head records were based at the time, to seattle with his then-girlfriend, faith coloccia; they went on to wed in september of the same year.he has also acquired a custom guitar from the electrical guitar company (as did fellow isis guitarist michael gallagher).in the past, turner has also used a gibson les paul standard, prs ce24, and has played through sunn, mesa boogie, and mackie amplifiers.when playing with isis, turner and his fellow guitarists usually tuned their instruments (low to high) b-f#-b-e-g#-b, to achieve a heavier sound.they also used other tunings, though less frequently, such as f# (octave below)-f#-b-e-g#-b.in 2016, turner described the live rig he used with sumac as consisting of two custom-built guitars from the electrical guitar company.both have lucite bodies and aluminum necks, and custom-wound wide frequency range pickups.the newer of the two—a prototype for a signature model—has a slightly flatter fingerboard radius than the older instrument. | unciatim | mastless | rheoplankton | no related information |
aaron turner (born november 5, 1977) is an american musician, singer, graphic artist, and founder of label hydra head records.he is most widely known for his role as guitarist and vocalist for the post-metal bands sumac and isis, while also participating in several other bands and projects such as old man gloom, lotus eaters and split cranium, a collaboration with jussi lehtisalo of finnish band circle who toured with isis in 2009.raised in new mexico, turner moved to the boston area, where he attended art school and formed isis and hydra head.in june 2003, turner moved operations of both the band and label to los angeles, california.turner now resides in vashon, wa which is also the base of operations for hydra head and his various other activities.in partnership with his wife faith coloccia, turner founded another record label, sige, in march 2011.it has gone on to release material from his musical collaboration with coloccia, mamiffer.sige is distributed by the business.at an early age, his family moved to new mexico, where he was raised.his mother was a teacher 'who taught a progressive curriculum' and his father an author, 'mainly [of] non-fiction'.turner describes his upbringing, surrounded by his parents' writer, artist and photographer friends, as 'creatively nurturing'.at age 17, he started a company that sold rare punk rock records via mail-order.he later moved to boston to attend art school at the school of the museum of fine arts, and in 1995 began releasing music.by 1997, the hydra head label was becoming a respectable small record label.turner describes his early industriousness as being motivated in part by boredom: i grew up in new mexico, and there wasn't a whole lot as far as youth culture is concerned.especially when i started to get interested in straight edge and wasn't doing drugs anymore, there was really nothing for me to do.so that was like a big reason for me, i suppose, to become really productive.also, i've never been a really social person.so there's not a lot of time taken up by my social life.and music has always been a very very big part of my life.i guess just a combination of those factors is why everything got started so early.around 1997–99, turner was living with future isis bassist and co-founder jeff caxide; until this point, he had been a member of the bands union suit and hollomen.isis was formed in 1997 out of a dissatisfaction with said bands' musical direction and turner and caxide's respective degrees of creative control.in mid-2009, turner moved from los angeles, where both isis and hydra head records were based at the time, to seattle with his then-girlfriend, faith coloccia; they went on to wed in september of the same year.he has also acquired a custom guitar from the electrical guitar company (as did fellow isis guitarist michael gallagher).in the past, turner has also used a gibson les paul standard, prs ce24, and has played through sunn, mesa boogie, and mackie amplifiers.when playing with isis, turner and his fellow guitarists usually tuned their instruments (low to high) b-f#-b-e-g#-b, to achieve a heavier sound.they also used other tunings, though less frequently, such as f# (octave below)-f#-b-e-g#-b.in 2016, turner described the live rig he used with sumac as consisting of two custom-built guitars from the electrical guitar company.both have lucite bodies and aluminum necks, and custom-wound wide frequency range pickups.the newer of the two—a prototype for a signature model—has a slightly flatter fingerboard radius than the older instrument. | aaron turner | associatedband/associatedmusicalartist | twilight band <tsp> aaron turner | associatedband/associatedmusicalartist | old man gloom <tsp> aaron turner | genre | black metal <tsp> aaron turner | origin | united states <tsp> aaron turner | activeyearsstartyear | 1995 | no related information |
atlas ii was a member of the atlas family of launch vehicles, which evolved from the successful atlas missile program of the 1950s.the atlas ii was a direct evolution of the atlas i, featuring longer first stage tanks, higher-performing engines, and the option for strap-on solid rocket boosters.it was designed to launch payloads into low earth orbit, geosynchronous transfer orbit or geosynchronous orbit.sixty-three launches of the atlas ii, iia and iias models were carried out between 1991 and 2004; all sixty-three launches were successes, making the atlas ii a highly reliable space launch system.the atlas line was continued by the atlas iii, used between 2000 and 2005, and the atlas v which is still in use.additional commercial and u.s. government sales resulted in production increases leading to greater than 60 vehicles being produced and launched.atlas ii was developed from the atlas i and featured numerous upgrades over that vehicle.atlas ii was launched from launch complex 36 at cape canaveral space force station in florida as well as space launch complex 3e at vandenberg space force base in california.all launches were successful.the increased thrust, engine efficiency, and propellant capacity enabled the vehicle to lift payloads of 6,100 pounds (2,767 kg) into geostationary transfer orbit (gto), or more on later atlas ii variants.atlas ii also featured lower-cost electronics, an improved flight computer, and longer propellant tanks than its predecessor, atlas i.the stage was powered by 3 rs-56 rocket engines (derived from the rs-27 main engine of the delta ii rocket) burning 156 t (344,000 lb) of rp-1 and liquid oxygen.the two booster engines were the rs-56-oba variants (the complete assembly of both engines and the aft skirt was referred to as the ma-5a), with high thrust but moderate efficiency.the sustainer (center) engine was the rs-56-osa variant, featuring much less thrust but higher efficiency at high altitudes than the booster engines.the vernier engines used on the first stage of the atlas i (and all previous atlas models) were replaced by a hydrazine-fueled roll control system on atlas ii.this system, mounted on the interstage between the first and second stages, utilized small thrusters to control the vehicle's roll.compared to atlas i, the atlas ii first stage was 2.7 m (8 ft 10 in) taller.the atlas ii was the last atlas rocket to use the 'stage-and-a-half' technique, where it ignited all 3 rs-56 engines at liftoff and then jettisoned the 2 rs-56-oba side engines and their support structure during ascent.the two rs-56-oba engines were integrated into a single unit called the ma-5a and shared a common gas generator.they burned for approximately 164 seconds before being jettisoned, when acceleration reached approximately 5.0-5.5 g. the central sustainer engine on the first stage, an rs-56-osa, would burn for an additional 125 seconds after their jettison.it featured better efficiency at high altitudes than the rs-56-obas.the first stage also had the option to be fitted with 4 castor 4a solid rocket boosters as part of the iias version, each providing an additional 478.3 kn (107,500 lbf) of thrust for 56 seconds.the first two boosters were ignited at liftoff, and the other two were ignited after the first two burnt out.both pairs of boosters were jettisoned shortly after their respective burns.centaur ii featured 2 rl-10a-3-3a engines, burning liquid hydrogen and liquid oxygen.it featured propellant tanks 0.9 meters longer than its predecessor, centaur i, giving the stage more propellant and therefore higher performance.due to the super cold propellants inside centaur, foam insulation was installed onto the outer metal skin on the stage to help mitigate propellant boiloff inside the tank. | ganisters | tessera | outtravel <tsp> ganisters | nonsubtlety | bisagre | no related information |
camilla (minor planet designation: 107 camilla) is one of the largest asteroids from the outermost edge of the asteroid belt, approximately 250 kilometers (160 miles) in diameter.it is a member of the sylvia family and located within the cybele group.it was discovered on 17 november 1868, by english astronomer norman pogson at madras observatory, india, and named after camilla, queen of the volsci in roman mythology.the x-type asteroid is a rare trinary asteroid with two minor-planet moons discovered in 2001 and 2016, respectively.it is elongated in shape and has a short rotation period of 4.8 hours.a large number of rotational lightcurves of have been obtained from photometric observations since the 1980s.best rated results gave a short rotation period of 4.844 hours with a brightness amplitude between 0.32 and 0.53 magnitude.lightcurve analysis indicates that camilla's pole most likely points towards ecliptic coordinates (β, λ) = (+51°, 72°) with a 10° uncertainty, which gives it an axial tilt of 29°.follow-up modeling of photometric data gave similar results.according to the space-based surveys carried out by the japanese akari satellite, the infrared astronomical satellite iras and the neowise mission of nasa's wide-field infrared survey explorer, as well as observations by the keck observatory and photometric modeling, camilla measures between 185 and 247 kilometers in diameter and its surface has an albedo between 0.160 and 0.294.it has been designated s/2001 (107) 1 but has not yet received an official name.later observations in september 2005 with the very large telescope (vlt) allowed the determination of an orbit.apart from data in infobox, the inclination was found to be 3 ± 1° with respect to an axis pointing towards (β, λ) = (+55°, 75°).given the ~10° uncertainty in the actual rotational axis of camilla, one can say that the orbit's inclination is less than 10°.the satellite is estimated to measure about 11 km in diameter.assuming a similar density to the primary, this would give it an approximate mass of ~1.5×1015 kg.it has a similar colour to the primary.it has the provisional designation s/2016 (107) 1.observations were taken between 29 may 2015 and 30 july 2016, using the vlt-sphere, the principal instrument attached to the 8-meter 'melipal' (ut3) unit of the vlt.on 3 out of 5 observation sessions, the new satellite could be detected.the body's orbit has a semi-major axis of 340 kilometers.107 camilla and s/2001 (107) 1, orbit data website maintained by f. marchis.includes orbit diagrams.107 camilla at astdys-2, asteroids—dynamic site ephemeris · observation prediction · orbital info · proper elements · observational info 107 camilla at the jpl small-body database | superexiguity | endodynamomorphic | unqualifying <tsp> superexiguity | chechehet | cencerros | no related information |
aaron turner (born november 5, 1977) is an american musician, singer, graphic artist, and founder of label hydra head records.he is most widely known for his role as guitarist and vocalist for the post-metal bands sumac and isis, while also participating in several other bands and projects such as old man gloom, lotus eaters and split cranium, a collaboration with jussi lehtisalo of finnish band circle who toured with isis in 2009.raised in new mexico, turner moved to the boston area, where he attended art school and formed isis and hydra head.in june 2003, turner moved operations of both the band and label to los angeles, california.turner now resides in vashon, wa which is also the base of operations for hydra head and his various other activities.in partnership with his wife faith coloccia, turner founded another record label, sige, in march 2011.it has gone on to release material from his musical collaboration with coloccia, mamiffer.sige is distributed by the business.at an early age, his family moved to new mexico, where he was raised.his mother was a teacher 'who taught a progressive curriculum' and his father an author, 'mainly [of] non-fiction'.turner describes his upbringing, surrounded by his parents' writer, artist and photographer friends, as 'creatively nurturing'.at age 17, he started a company that sold rare punk rock records via mail-order.he later moved to boston to attend art school at the school of the museum of fine arts, and in 1995 began releasing music.by 1997, the hydra head label was becoming a respectable small record label.turner describes his early industriousness as being motivated in part by boredom: i grew up in new mexico, and there wasn't a whole lot as far as youth culture is concerned.especially when i started to get interested in straight edge and wasn't doing drugs anymore, there was really nothing for me to do.so that was like a big reason for me, i suppose, to become really productive.also, i've never been a really social person.so there's not a lot of time taken up by my social life.and music has always been a very very big part of my life.i guess just a combination of those factors is why everything got started so early.around 1997–99, turner was living with future isis bassist and co-founder jeff caxide; until this point, he had been a member of the bands union suit and hollomen.isis was formed in 1997 out of a dissatisfaction with said bands' musical direction and turner and caxide's respective degrees of creative control.in mid-2009, turner moved from los angeles, where both isis and hydra head records were based at the time, to seattle with his then-girlfriend, faith coloccia; they went on to wed in september of the same year.he has also acquired a custom guitar from the electrical guitar company (as did fellow isis guitarist michael gallagher).in the past, turner has also used a gibson les paul standard, prs ce24, and has played through sunn, mesa boogie, and mackie amplifiers.when playing with isis, turner and his fellow guitarists usually tuned their instruments (low to high) b-f#-b-e-g#-b, to achieve a heavier sound.they also used other tunings, though less frequently, such as f# (octave below)-f#-b-e-g#-b.in 2016, turner described the live rig he used with sumac as consisting of two custom-built guitars from the electrical guitar company.both have lucite bodies and aluminum necks, and custom-wound wide frequency range pickups.the newer of the two—a prototype for a signature model—has a slightly flatter fingerboard radius than the older instrument. | prophethood | tallies | dinosaurs | no related information |
camilla (minor planet designation: 107 camilla) is one of the largest asteroids from the outermost edge of the asteroid belt, approximately 250 kilometers (160 miles) in diameter.it is a member of the sylvia family and located within the cybele group.it was discovered on 17 november 1868, by english astronomer norman pogson at madras observatory, india, and named after camilla, queen of the volsci in roman mythology.the x-type asteroid is a rare trinary asteroid with two minor-planet moons discovered in 2001 and 2016, respectively.it is elongated in shape and has a short rotation period of 4.8 hours.a large number of rotational lightcurves of have been obtained from photometric observations since the 1980s.best rated results gave a short rotation period of 4.844 hours with a brightness amplitude between 0.32 and 0.53 magnitude.lightcurve analysis indicates that camilla's pole most likely points towards ecliptic coordinates (β, λ) = (+51°, 72°) with a 10° uncertainty, which gives it an axial tilt of 29°.follow-up modeling of photometric data gave similar results.according to the space-based surveys carried out by the japanese akari satellite, the infrared astronomical satellite iras and the neowise mission of nasa's wide-field infrared survey explorer, as well as observations by the keck observatory and photometric modeling, camilla measures between 185 and 247 kilometers in diameter and its surface has an albedo between 0.160 and 0.294.it has been designated s/2001 (107) 1 but has not yet received an official name.later observations in september 2005 with the very large telescope (vlt) allowed the determination of an orbit.apart from data in infobox, the inclination was found to be 3 ± 1° with respect to an axis pointing towards (β, λ) = (+55°, 75°).given the ~10° uncertainty in the actual rotational axis of camilla, one can say that the orbit's inclination is less than 10°.the satellite is estimated to measure about 11 km in diameter.assuming a similar density to the primary, this would give it an approximate mass of ~1.5×1015 kg.it has a similar colour to the primary.it has the provisional designation s/2016 (107) 1.observations were taken between 29 may 2015 and 30 july 2016, using the vlt-sphere, the principal instrument attached to the 8-meter 'melipal' (ut3) unit of the vlt.on 3 out of 5 observation sessions, the new satellite could be detected.the body's orbit has a semi-major axis of 340 kilometers.107 camilla and s/2001 (107) 1, orbit data website maintained by f. marchis.includes orbit diagrams.107 camilla at astdys-2, asteroids—dynamic site ephemeris · observation prediction · orbital info · proper elements · observational info 107 camilla at the jpl small-body database | 107 camilla | discoverer | a storrs <tsp> 107 camilla | orbitalperiod | 236805 days <tsp> 107 camilla | periapsis | 4793430000 kilometres <tsp> 107 camilla | epoch | 2006-12-31 <tsp> 107 camilla | apoapsis | 5609370000 kilometres | no related information |
atlas ii was a member of the atlas family of launch vehicles, which evolved from the successful atlas missile program of the 1950s.the atlas ii was a direct evolution of the atlas i, featuring longer first stage tanks, higher-performing engines, and the option for strap-on solid rocket boosters.it was designed to launch payloads into low earth orbit, geosynchronous transfer orbit or geosynchronous orbit.sixty-three launches of the atlas ii, iia and iias models were carried out between 1991 and 2004; all sixty-three launches were successes, making the atlas ii a highly reliable space launch system.the atlas line was continued by the atlas iii, used between 2000 and 2005, and the atlas v which is still in use.additional commercial and u.s. government sales resulted in production increases leading to greater than 60 vehicles being produced and launched.atlas ii was developed from the atlas i and featured numerous upgrades over that vehicle.atlas ii was launched from launch complex 36 at cape canaveral space force station in florida as well as space launch complex 3e at vandenberg space force base in california.all launches were successful.the increased thrust, engine efficiency, and propellant capacity enabled the vehicle to lift payloads of 6,100 pounds (2,767 kg) into geostationary transfer orbit (gto), or more on later atlas ii variants.atlas ii also featured lower-cost electronics, an improved flight computer, and longer propellant tanks than its predecessor, atlas i.the stage was powered by 3 rs-56 rocket engines (derived from the rs-27 main engine of the delta ii rocket) burning 156 t (344,000 lb) of rp-1 and liquid oxygen.the two booster engines were the rs-56-oba variants (the complete assembly of both engines and the aft skirt was referred to as the ma-5a), with high thrust but moderate efficiency.the sustainer (center) engine was the rs-56-osa variant, featuring much less thrust but higher efficiency at high altitudes than the booster engines.the vernier engines used on the first stage of the atlas i (and all previous atlas models) were replaced by a hydrazine-fueled roll control system on atlas ii.this system, mounted on the interstage between the first and second stages, utilized small thrusters to control the vehicle's roll.compared to atlas i, the atlas ii first stage was 2.7 m (8 ft 10 in) taller.the atlas ii was the last atlas rocket to use the 'stage-and-a-half' technique, where it ignited all 3 rs-56 engines at liftoff and then jettisoned the 2 rs-56-oba side engines and their support structure during ascent.the two rs-56-oba engines were integrated into a single unit called the ma-5a and shared a common gas generator.they burned for approximately 164 seconds before being jettisoned, when acceleration reached approximately 5.0-5.5 g. the central sustainer engine on the first stage, an rs-56-osa, would burn for an additional 125 seconds after their jettison.it featured better efficiency at high altitudes than the rs-56-obas.the first stage also had the option to be fitted with 4 castor 4a solid rocket boosters as part of the iias version, each providing an additional 478.3 kn (107,500 lbf) of thrust for 56 seconds.the first two boosters were ignited at liftoff, and the other two were ignited after the first two burnt out.both pairs of boosters were jettisoned shortly after their respective burns.centaur ii featured 2 rl-10a-3-3a engines, burning liquid hydrogen and liquid oxygen.it featured propellant tanks 0.9 meters longer than its predecessor, centaur i, giving the stage more propellant and therefore higher performance.due to the super cold propellants inside centaur, foam insulation was installed onto the outer metal skin on the stage to help mitigate propellant boiloff inside the tank. | irreligionist | deflator | condenser | no related information |
aaron turner (born november 5, 1977) is an american musician, singer, graphic artist, and founder of label hydra head records.he is most widely known for his role as guitarist and vocalist for the post-metal bands sumac and isis, while also participating in several other bands and projects such as old man gloom, lotus eaters and split cranium, a collaboration with jussi lehtisalo of finnish band circle who toured with isis in 2009.raised in new mexico, turner moved to the boston area, where he attended art school and formed isis and hydra head.in june 2003, turner moved operations of both the band and label to los angeles, california.turner now resides in vashon, wa which is also the base of operations for hydra head and his various other activities.in partnership with his wife faith coloccia, turner founded another record label, sige, in march 2011.it has gone on to release material from his musical collaboration with coloccia, mamiffer.sige is distributed by the business.at an early age, his family moved to new mexico, where he was raised.his mother was a teacher 'who taught a progressive curriculum' and his father an author, 'mainly [of] non-fiction'.turner describes his upbringing, surrounded by his parents' writer, artist and photographer friends, as 'creatively nurturing'.at age 17, he started a company that sold rare punk rock records via mail-order.he later moved to boston to attend art school at the school of the museum of fine arts, and in 1995 began releasing music.by 1997, the hydra head label was becoming a respectable small record label.turner describes his early industriousness as being motivated in part by boredom: i grew up in new mexico, and there wasn't a whole lot as far as youth culture is concerned.especially when i started to get interested in straight edge and wasn't doing drugs anymore, there was really nothing for me to do.so that was like a big reason for me, i suppose, to become really productive.also, i've never been a really social person.so there's not a lot of time taken up by my social life.and music has always been a very very big part of my life.i guess just a combination of those factors is why everything got started so early.around 1997–99, turner was living with future isis bassist and co-founder jeff caxide; until this point, he had been a member of the bands union suit and hollomen.isis was formed in 1997 out of a dissatisfaction with said bands' musical direction and turner and caxide's respective degrees of creative control.in mid-2009, turner moved from los angeles, where both isis and hydra head records were based at the time, to seattle with his then-girlfriend, faith coloccia; they went on to wed in september of the same year.he has also acquired a custom guitar from the electrical guitar company (as did fellow isis guitarist michael gallagher).in the past, turner has also used a gibson les paul standard, prs ce24, and has played through sunn, mesa boogie, and mackie amplifiers.when playing with isis, turner and his fellow guitarists usually tuned their instruments (low to high) b-f#-b-e-g#-b, to achieve a heavier sound.they also used other tunings, though less frequently, such as f# (octave below)-f#-b-e-g#-b.in 2016, turner described the live rig he used with sumac as consisting of two custom-built guitars from the electrical guitar company.both have lucite bodies and aluminum necks, and custom-wound wide frequency range pickups.the newer of the two—a prototype for a signature model—has a slightly flatter fingerboard radius than the older instrument. | aaron turner | associatedband/associatedmusicalartist | twilight band <tsp> aaron turner | genre | black metal <tsp> aaron turner | associatedband/associatedmusicalartist | mamiffer <tsp> aaron turner | instrument | electric guitar <tsp> black metal | musicfusiongenre | death metal | he is most widely known for his role as guitarist and vocalist for the post-metal bands sumac and isis, while also participating in several other bands and projects such as old man gloom, lotus eaters and split cranium, a collaboration with jussi lehtisalo of finnish band circle who toured with isis in 2009.he has also acquired a custom guitar from the electrical guitar company (as did fellow isis guitarist michael gallagher).in the past, turner has also used a gibson les paul standard, prs ce24, and has played through sunn, mesa boogie, and mackie amplifiers.when playing with isis, turner and his fellow guitarists usually tuned their instruments (low to high) b-f#-b-e-g#-b, to achieve a heavier sound.they also used other tunings, though less frequently, such as f# (octave below)-f#-b-e-g#-b.in 2016, turner described the live rig he used with sumac as consisting of two custom-built guitars from the electrical guitar company. |
atlas ii was a member of the atlas family of launch vehicles, which evolved from the successful atlas missile program of the 1950s.the atlas ii was a direct evolution of the atlas i, featuring longer first stage tanks, higher-performing engines, and the option for strap-on solid rocket boosters.it was designed to launch payloads into low earth orbit, geosynchronous transfer orbit or geosynchronous orbit.sixty-three launches of the atlas ii, iia and iias models were carried out between 1991 and 2004; all sixty-three launches were successes, making the atlas ii a highly reliable space launch system.the atlas line was continued by the atlas iii, used between 2000 and 2005, and the atlas v which is still in use.additional commercial and u.s. government sales resulted in production increases leading to greater than 60 vehicles being produced and launched.atlas ii was developed from the atlas i and featured numerous upgrades over that vehicle.atlas ii was launched from launch complex 36 at cape canaveral space force station in florida as well as space launch complex 3e at vandenberg space force base in california.all launches were successful.the increased thrust, engine efficiency, and propellant capacity enabled the vehicle to lift payloads of 6,100 pounds (2,767 kg) into geostationary transfer orbit (gto), or more on later atlas ii variants.atlas ii also featured lower-cost electronics, an improved flight computer, and longer propellant tanks than its predecessor, atlas i.the stage was powered by 3 rs-56 rocket engines (derived from the rs-27 main engine of the delta ii rocket) burning 156 t (344,000 lb) of rp-1 and liquid oxygen.the two booster engines were the rs-56-oba variants (the complete assembly of both engines and the aft skirt was referred to as the ma-5a), with high thrust but moderate efficiency.the sustainer (center) engine was the rs-56-osa variant, featuring much less thrust but higher efficiency at high altitudes than the booster engines.the vernier engines used on the first stage of the atlas i (and all previous atlas models) were replaced by a hydrazine-fueled roll control system on atlas ii.this system, mounted on the interstage between the first and second stages, utilized small thrusters to control the vehicle's roll.compared to atlas i, the atlas ii first stage was 2.7 m (8 ft 10 in) taller.the atlas ii was the last atlas rocket to use the 'stage-and-a-half' technique, where it ignited all 3 rs-56 engines at liftoff and then jettisoned the 2 rs-56-oba side engines and their support structure during ascent.the two rs-56-oba engines were integrated into a single unit called the ma-5a and shared a common gas generator.they burned for approximately 164 seconds before being jettisoned, when acceleration reached approximately 5.0-5.5 g. the central sustainer engine on the first stage, an rs-56-osa, would burn for an additional 125 seconds after their jettison.it featured better efficiency at high altitudes than the rs-56-obas.the first stage also had the option to be fitted with 4 castor 4a solid rocket boosters as part of the iias version, each providing an additional 478.3 kn (107,500 lbf) of thrust for 56 seconds.the first two boosters were ignited at liftoff, and the other two were ignited after the first two burnt out.both pairs of boosters were jettisoned shortly after their respective burns.centaur ii featured 2 rl-10a-3-3a engines, burning liquid hydrogen and liquid oxygen.it featured propellant tanks 0.9 meters longer than its predecessor, centaur i, giving the stage more propellant and therefore higher performance.due to the super cold propellants inside centaur, foam insulation was installed onto the outer metal skin on the stage to help mitigate propellant boiloff inside the tank. | atlas ii | launchsite | cape canaveral air force station <tsp> atlas ii | countryorigin | united states <tsp> atlas ii | finalflight | 2002-12-05 <tsp> atlas ii | diameter | 304 m <tsp> atlas ii | launchsite | spaceport florida launch complex 36 | atlas ii was a member of the atlas family of launch vehicles, which evolved from the successful atlas missile program of the 1950s.sixty-three launches of the atlas ii, iia and iias models were carried out between 1991 and 2004; all sixty-three launches were successes, making the atlas ii a highly reliable space launch system.atlas ii was developed from the atlas i and featured numerous upgrades over that vehicle.atlas ii was launched from launch complex 36 at cape canaveral space force station in florida as well as space launch complex 3e at vandenberg space force base in california.the increased thrust, engine efficiency, and propellant capacity enabled the vehicle to lift payloads of 6,100 pounds (2,767 kg) into geostationary transfer orbit (gto), or more on later atlas ii variants.atlas ii also featured lower-cost electronics, an improved flight computer, and longer propellant tanks than its predecessor, atlas i. |
aaron turner (born november 5, 1977) is an american musician, singer, graphic artist, and founder of label hydra head records.he is most widely known for his role as guitarist and vocalist for the post-metal bands sumac and isis, while also participating in several other bands and projects such as old man gloom, lotus eaters and split cranium, a collaboration with jussi lehtisalo of finnish band circle who toured with isis in 2009.raised in new mexico, turner moved to the boston area, where he attended art school and formed isis and hydra head.in june 2003, turner moved operations of both the band and label to los angeles, california.turner now resides in vashon, wa which is also the base of operations for hydra head and his various other activities.in partnership with his wife faith coloccia, turner founded another record label, sige, in march 2011.it has gone on to release material from his musical collaboration with coloccia, mamiffer.sige is distributed by the business.at an early age, his family moved to new mexico, where he was raised.his mother was a teacher 'who taught a progressive curriculum' and his father an author, 'mainly [of] non-fiction'.turner describes his upbringing, surrounded by his parents' writer, artist and photographer friends, as 'creatively nurturing'.at age 17, he started a company that sold rare punk rock records via mail-order.he later moved to boston to attend art school at the school of the museum of fine arts, and in 1995 began releasing music.by 1997, the hydra head label was becoming a respectable small record label.turner describes his early industriousness as being motivated in part by boredom: i grew up in new mexico, and there wasn't a whole lot as far as youth culture is concerned.especially when i started to get interested in straight edge and wasn't doing drugs anymore, there was really nothing for me to do.so that was like a big reason for me, i suppose, to become really productive.also, i've never been a really social person.so there's not a lot of time taken up by my social life.and music has always been a very very big part of my life.i guess just a combination of those factors is why everything got started so early.around 1997–99, turner was living with future isis bassist and co-founder jeff caxide; until this point, he had been a member of the bands union suit and hollomen.isis was formed in 1997 out of a dissatisfaction with said bands' musical direction and turner and caxide's respective degrees of creative control.in mid-2009, turner moved from los angeles, where both isis and hydra head records were based at the time, to seattle with his then-girlfriend, faith coloccia; they went on to wed in september of the same year.he has also acquired a custom guitar from the electrical guitar company (as did fellow isis guitarist michael gallagher).in the past, turner has also used a gibson les paul standard, prs ce24, and has played through sunn, mesa boogie, and mackie amplifiers.when playing with isis, turner and his fellow guitarists usually tuned their instruments (low to high) b-f#-b-e-g#-b, to achieve a heavier sound.they also used other tunings, though less frequently, such as f# (octave below)-f#-b-e-g#-b.in 2016, turner described the live rig he used with sumac as consisting of two custom-built guitars from the electrical guitar company.both have lucite bodies and aluminum necks, and custom-wound wide frequency range pickups.the newer of the two—a prototype for a signature model—has a slightly flatter fingerboard radius than the older instrument. | aaron turner | associatedband/associatedmusicalartist | twilight band <tsp> aaron turner | genre | black metal <tsp> aaron turner | associatedband/associatedmusicalartist | mamiffer <tsp> aaron turner | instrument | electric guitar <tsp> black metal | musicfusiongenre | death metal | he is most widely known for his role as guitarist and vocalist for the post-metal bands sumac and isis, while also participating in several other bands and projects such as old man gloom, lotus eaters and split cranium, a collaboration with jussi lehtisalo of finnish band circle who toured with isis in 2009.he has also acquired a custom guitar from the electrical guitar company (as did fellow isis guitarist michael gallagher).in the past, turner has also used a gibson les paul standard, prs ce24, and has played through sunn, mesa boogie, and mackie amplifiers.when playing with isis, turner and his fellow guitarists usually tuned their instruments (low to high) b-f#-b-e-g#-b, to achieve a heavier sound.they also used other tunings, though less frequently, such as f# (octave below)-f#-b-e-g#-b.in 2016, turner described the live rig he used with sumac as consisting of two custom-built guitars from the electrical guitar company. |
camilla (minor planet designation: 107 camilla) is one of the largest asteroids from the outermost edge of the asteroid belt, approximately 250 kilometers (160 miles) in diameter.it is a member of the sylvia family and located within the cybele group.it was discovered on 17 november 1868, by english astronomer norman pogson at madras observatory, india, and named after camilla, queen of the volsci in roman mythology.the x-type asteroid is a rare trinary asteroid with two minor-planet moons discovered in 2001 and 2016, respectively.it is elongated in shape and has a short rotation period of 4.8 hours.a large number of rotational lightcurves of have been obtained from photometric observations since the 1980s.best rated results gave a short rotation period of 4.844 hours with a brightness amplitude between 0.32 and 0.53 magnitude.lightcurve analysis indicates that camilla's pole most likely points towards ecliptic coordinates (β, λ) = (+51°, 72°) with a 10° uncertainty, which gives it an axial tilt of 29°.follow-up modeling of photometric data gave similar results.according to the space-based surveys carried out by the japanese akari satellite, the infrared astronomical satellite iras and the neowise mission of nasa's wide-field infrared survey explorer, as well as observations by the keck observatory and photometric modeling, camilla measures between 185 and 247 kilometers in diameter and its surface has an albedo between 0.160 and 0.294.it has been designated s/2001 (107) 1 but has not yet received an official name.later observations in september 2005 with the very large telescope (vlt) allowed the determination of an orbit.apart from data in infobox, the inclination was found to be 3 ± 1° with respect to an axis pointing towards (β, λ) = (+55°, 75°).given the ~10° uncertainty in the actual rotational axis of camilla, one can say that the orbit's inclination is less than 10°.the satellite is estimated to measure about 11 km in diameter.assuming a similar density to the primary, this would give it an approximate mass of ~1.5×1015 kg.it has a similar colour to the primary.it has the provisional designation s/2016 (107) 1.observations were taken between 29 may 2015 and 30 july 2016, using the vlt-sphere, the principal instrument attached to the 8-meter 'melipal' (ut3) unit of the vlt.on 3 out of 5 observation sessions, the new satellite could be detected.the body's orbit has a semi-major axis of 340 kilometers.107 camilla and s/2001 (107) 1, orbit data website maintained by f. marchis.includes orbit diagrams.107 camilla at astdys-2, asteroids—dynamic site ephemeris · observation prediction · orbital info · proper elements · observational info 107 camilla at the jpl small-body database | embryologists | hypogeugea | waterfall | no related information |
the audi a1 (internally designated typ 8x) is a supermini car launched by audi at the 2010 geneva motor show.sales of the initial three-door a1 model started in germany in august 2010, with the united kingdom following in november 2010.a five-door version, called sportback, was launched in november 2011, with sales starting in export markets during spring 2012.the concept seats four and features a new plug-in hybrid powertrain.with this powertrain, a 1.4 l (85.4 cu in) 148 bhp (110.4 kw) turbo fsi engine drives the front wheels via a six-speed s-tronic, while a 40 bhp (29.8 kw; 40.6 ps) electric motor provides power to the rear wheels.the electric motor is also capable of producing 148 lb⋅ft (201 n⋅m) of torque.the metroproject quattro is able to travel 62 miles (100 km) at up to 62 mph (100 km/h) on one charge of its lithium-ion batteries, which reduces fuel consumption by up to 15%.both power sources are available to use simultaneously, with the driver then benefiting from macpherson strut front and rear four-link suspension configuration, electromechanical speed-sensitive power steering with a low energy draw, audi magnetic ride adaptive damping technology, and 0 to 100 km/h (0 to 62 mph) in 7.8 seconds.the vehicle was designed by audi ag project designer in exterior design jürgen löffler, who also presented the design during the car's hong kong debut.the vehicle's 0 to 100 km/h (0 to 62 mph) acceleration is 7.9 seconds and average co2 emissions are given as 92g/km.the vehicle's electric-only range is 50 km (31.07 mi).the vehicle was unveiled at the 2008 paris motor show.the car is aimed mostly at young, affluent urban buyers.se is the base specification, while sport and s line models also have sport seats, sports suspension and larger wheels, amongst other features.1.4-litre tfsi (122 ps (90 kw; 120 hp)) was sold as the 30 tfsi in china.the production version of the a1 quattro was tested by autocar magazine on mira's wet handling track alongside a nissan gt-r; the a1 recorded lap time over five seconds faster than the gt-r. autocar called the test a '...giant-killing result'.the a1 is based on the volkswagen group pq25 platform, the same platform used in the seat ibiza mk4 and the vw polo mk5, and in its development audi has collaborated with seat.as of 23 june 2011, the 100,000th a1 was produced at audi brussels plant.a version of 2011 audi a1 painted by damien hirst was sold for £350,000.a fully charged 12 kwh lithium-ion battery gives a maximum range of 50 km (31 mi), after which a 254 cc wankel engine is used to power a 15 kw (20 ps; 20 bhp) generator with a 12 l (2.6 imp gal; 3.2 us gal) fuel tank.this is estimated to provide an additional range of 124 mi (200 km).the company claims the car weighs 1,190 kg (2,624 lb), can reach 62 mph (100 km/h) in 10.2 seconds and a maximum speed of 80 mph (129 km/h).the vehicle was unveiled at the 2010 geneva motor show, followed by the 2012 taipei motor show.it was reported that, according to the director of e-mobility and sustainability strategy at audi of america, the a1 e-tron had never been scheduled for production.in march 2013, at the new york auto show, audi announced it will be expanding the testing of its a1 e-tron outside of munich to other regions of germany.production of the a1 e-tron was reported to be cancelled.it included 18-inch 'polygon' design alloy wheels, exterior styling package (front spoiler, double-blade roof spoiler, side skirts, rear diffuser in gloss black, stainless steel tailpipe trims), roof line, shoulder line with 'audi sport' lettering, number '1' on the bonnet and doors, boot lid, front spoiler lip, side skirts, wheel arch; surrounds and double-blade roof spoiler, rear sills with audi rings, centre console trim, door handles, floor mats, rear-view mirror trim (not available with auto-dimming mirror), air vent sleeves in high gloss white. | audi a1 | class | supermini <tsp> audi a1 | engine | 12 litres <tsp> audi a1 | layout | front-engine front-wheel-drive layout <tsp> audi a1 | assembly | audi brussels <tsp> audi a1 | bodystyle | hatchback | the audi a1 (internally designated typ 8x) is a supermini car launched by audi at the 2010 geneva motor show.both power sources are available to use simultaneously, with the driver then benefiting from macpherson strut front and rear four-link suspension configuration, electromechanical speed-sensitive power steering with a low energy draw, audi magnetic ride adaptive damping technology, and 0 to 100 km/h (0 to 62 mph) in 7.8 seconds.the vehicle was designed by audi ag project designer in exterior design jürgen löffler, who also presented the design during the car's hong kong debut.the a1 is based on the volkswagen group pq25 platform, the same platform used in the seat ibiza mk4 and the vw polo mk5, and in its development audi has collaborated with seat.as of 23 june 2011, the 100,000th a1 was produced at audi brussels plant.a version of 2011 audi a1 painted by damien hirst was sold for £350,000.it was reported that, according to the director of e-mobility and sustainability strategy at audi of america, the a1 e-tron had never been scheduled for production.in march 2013, at the new york auto show, audi announced it will be expanding the testing of its a1 e-tron outside of munich to other regions of germany.production of the a1 e-tron was reported to be cancelled.it included 18-inch 'polygon' design alloy wheels, exterior styling package (front spoiler, double-blade roof spoiler, side skirts, rear diffuser in gloss black, stainless steel tailpipe trims), roof line, shoulder line with 'audi sport' lettering, number '1' on the bonnet and doors, boot lid, front spoiler lip, side skirts, wheel arch; surrounds and double-blade roof spoiler, rear sills with audi rings, centre console trim, door handles, floor mats, rear-view mirror trim (not available with auto-dimming mirror), air vent sleeves in high gloss white. |
camilla (minor planet designation: 107 camilla) is one of the largest asteroids from the outermost edge of the asteroid belt, approximately 250 kilometers (160 miles) in diameter.it is a member of the sylvia family and located within the cybele group.it was discovered on 17 november 1868, by english astronomer norman pogson at madras observatory, india, and named after camilla, queen of the volsci in roman mythology.the x-type asteroid is a rare trinary asteroid with two minor-planet moons discovered in 2001 and 2016, respectively.it is elongated in shape and has a short rotation period of 4.8 hours.a large number of rotational lightcurves of have been obtained from photometric observations since the 1980s.best rated results gave a short rotation period of 4.844 hours with a brightness amplitude between 0.32 and 0.53 magnitude.lightcurve analysis indicates that camilla's pole most likely points towards ecliptic coordinates (β, λ) = (+51°, 72°) with a 10° uncertainty, which gives it an axial tilt of 29°.follow-up modeling of photometric data gave similar results.according to the space-based surveys carried out by the japanese akari satellite, the infrared astronomical satellite iras and the neowise mission of nasa's wide-field infrared survey explorer, as well as observations by the keck observatory and photometric modeling, camilla measures between 185 and 247 kilometers in diameter and its surface has an albedo between 0.160 and 0.294.it has been designated s/2001 (107) 1 but has not yet received an official name.later observations in september 2005 with the very large telescope (vlt) allowed the determination of an orbit.apart from data in infobox, the inclination was found to be 3 ± 1° with respect to an axis pointing towards (β, λ) = (+55°, 75°).given the ~10° uncertainty in the actual rotational axis of camilla, one can say that the orbit's inclination is less than 10°.the satellite is estimated to measure about 11 km in diameter.assuming a similar density to the primary, this would give it an approximate mass of ~1.5×1015 kg.it has a similar colour to the primary.it has the provisional designation s/2016 (107) 1.observations were taken between 29 may 2015 and 30 july 2016, using the vlt-sphere, the principal instrument attached to the 8-meter 'melipal' (ut3) unit of the vlt.on 3 out of 5 observation sessions, the new satellite could be detected.the body's orbit has a semi-major axis of 340 kilometers.107 camilla and s/2001 (107) 1, orbit data website maintained by f. marchis.includes orbit diagrams.107 camilla at astdys-2, asteroids—dynamic site ephemeris · observation prediction · orbital info · proper elements · observational info 107 camilla at the jpl small-body database | 107 camilla | discoverer | e wells <tsp> 107 camilla | orbitalperiod | 236805 days <tsp> 107 camilla | periapsis | 4793430000 kilometres <tsp> 107 camilla | epoch | 2006-12-31 <tsp> 107 camilla | apoapsis | 5609370000 kilometres | no related information |
aaron turner (born november 5, 1977) is an american musician, singer, graphic artist, and founder of label hydra head records.he is most widely known for his role as guitarist and vocalist for the post-metal bands sumac and isis, while also participating in several other bands and projects such as old man gloom, lotus eaters and split cranium, a collaboration with jussi lehtisalo of finnish band circle who toured with isis in 2009.raised in new mexico, turner moved to the boston area, where he attended art school and formed isis and hydra head.in june 2003, turner moved operations of both the band and label to los angeles, california.turner now resides in vashon, wa which is also the base of operations for hydra head and his various other activities.in partnership with his wife faith coloccia, turner founded another record label, sige, in march 2011.it has gone on to release material from his musical collaboration with coloccia, mamiffer.sige is distributed by the business.at an early age, his family moved to new mexico, where he was raised.his mother was a teacher 'who taught a progressive curriculum' and his father an author, 'mainly [of] non-fiction'.turner describes his upbringing, surrounded by his parents' writer, artist and photographer friends, as 'creatively nurturing'.at age 17, he started a company that sold rare punk rock records via mail-order.he later moved to boston to attend art school at the school of the museum of fine arts, and in 1995 began releasing music.by 1997, the hydra head label was becoming a respectable small record label.turner describes his early industriousness as being motivated in part by boredom: i grew up in new mexico, and there wasn't a whole lot as far as youth culture is concerned.especially when i started to get interested in straight edge and wasn't doing drugs anymore, there was really nothing for me to do.so that was like a big reason for me, i suppose, to become really productive.also, i've never been a really social person.so there's not a lot of time taken up by my social life.and music has always been a very very big part of my life.i guess just a combination of those factors is why everything got started so early.around 1997–99, turner was living with future isis bassist and co-founder jeff caxide; until this point, he had been a member of the bands union suit and hollomen.isis was formed in 1997 out of a dissatisfaction with said bands' musical direction and turner and caxide's respective degrees of creative control.in mid-2009, turner moved from los angeles, where both isis and hydra head records were based at the time, to seattle with his then-girlfriend, faith coloccia; they went on to wed in september of the same year.he has also acquired a custom guitar from the electrical guitar company (as did fellow isis guitarist michael gallagher).in the past, turner has also used a gibson les paul standard, prs ce24, and has played through sunn, mesa boogie, and mackie amplifiers.when playing with isis, turner and his fellow guitarists usually tuned their instruments (low to high) b-f#-b-e-g#-b, to achieve a heavier sound.they also used other tunings, though less frequently, such as f# (octave below)-f#-b-e-g#-b.in 2016, turner described the live rig he used with sumac as consisting of two custom-built guitars from the electrical guitar company.both have lucite bodies and aluminum necks, and custom-wound wide frequency range pickups.the newer of the two—a prototype for a signature model—has a slightly flatter fingerboard radius than the older instrument. | prowled | befooling | catsos | no related information |
the audi a1 (internally designated typ 8x) is a supermini car launched by audi at the 2010 geneva motor show.sales of the initial three-door a1 model started in germany in august 2010, with the united kingdom following in november 2010.a five-door version, called sportback, was launched in november 2011, with sales starting in export markets during spring 2012.the concept seats four and features a new plug-in hybrid powertrain.with this powertrain, a 1.4 l (85.4 cu in) 148 bhp (110.4 kw) turbo fsi engine drives the front wheels via a six-speed s-tronic, while a 40 bhp (29.8 kw; 40.6 ps) electric motor provides power to the rear wheels.the electric motor is also capable of producing 148 lb⋅ft (201 n⋅m) of torque.the metroproject quattro is able to travel 62 miles (100 km) at up to 62 mph (100 km/h) on one charge of its lithium-ion batteries, which reduces fuel consumption by up to 15%.both power sources are available to use simultaneously, with the driver then benefiting from macpherson strut front and rear four-link suspension configuration, electromechanical speed-sensitive power steering with a low energy draw, audi magnetic ride adaptive damping technology, and 0 to 100 km/h (0 to 62 mph) in 7.8 seconds.the vehicle was designed by audi ag project designer in exterior design jürgen löffler, who also presented the design during the car's hong kong debut.the vehicle's 0 to 100 km/h (0 to 62 mph) acceleration is 7.9 seconds and average co2 emissions are given as 92g/km.the vehicle's electric-only range is 50 km (31.07 mi).the vehicle was unveiled at the 2008 paris motor show.the car is aimed mostly at young, affluent urban buyers.se is the base specification, while sport and s line models also have sport seats, sports suspension and larger wheels, amongst other features.1.4-litre tfsi (122 ps (90 kw; 120 hp)) was sold as the 30 tfsi in china.the production version of the a1 quattro was tested by autocar magazine on mira's wet handling track alongside a nissan gt-r; the a1 recorded lap time over five seconds faster than the gt-r. autocar called the test a '...giant-killing result'.the a1 is based on the volkswagen group pq25 platform, the same platform used in the seat ibiza mk4 and the vw polo mk5, and in its development audi has collaborated with seat.as of 23 june 2011, the 100,000th a1 was produced at audi brussels plant.a version of 2011 audi a1 painted by damien hirst was sold for £350,000.a fully charged 12 kwh lithium-ion battery gives a maximum range of 50 km (31 mi), after which a 254 cc wankel engine is used to power a 15 kw (20 ps; 20 bhp) generator with a 12 l (2.6 imp gal; 3.2 us gal) fuel tank.this is estimated to provide an additional range of 124 mi (200 km).the company claims the car weighs 1,190 kg (2,624 lb), can reach 62 mph (100 km/h) in 10.2 seconds and a maximum speed of 80 mph (129 km/h).the vehicle was unveiled at the 2010 geneva motor show, followed by the 2012 taipei motor show.it was reported that, according to the director of e-mobility and sustainability strategy at audi of america, the a1 e-tron had never been scheduled for production.in march 2013, at the new york auto show, audi announced it will be expanding the testing of its a1 e-tron outside of munich to other regions of germany.production of the a1 e-tron was reported to be cancelled.it included 18-inch 'polygon' design alloy wheels, exterior styling package (front spoiler, double-blade roof spoiler, side skirts, rear diffuser in gloss black, stainless steel tailpipe trims), roof line, shoulder line with 'audi sport' lettering, number '1' on the bonnet and doors, boot lid, front spoiler lip, side skirts, wheel arch; surrounds and double-blade roof spoiler, rear sills with audi rings, centre console trim, door handles, floor mats, rear-view mirror trim (not available with auto-dimming mirror), air vent sleeves in high gloss white. | audi a1 | class | supermini <tsp> audi a1 | engine | 12 litres <tsp> audi a1 | layout | front-engine front-wheel-drive layout <tsp> audi a1 | assembly | audi brussels <tsp> audi a1 | bodystyle | hatchback | the audi a1 (internally designated typ 8x) is a supermini car launched by audi at the 2010 geneva motor show.both power sources are available to use simultaneously, with the driver then benefiting from macpherson strut front and rear four-link suspension configuration, electromechanical speed-sensitive power steering with a low energy draw, audi magnetic ride adaptive damping technology, and 0 to 100 km/h (0 to 62 mph) in 7.8 seconds.the vehicle was designed by audi ag project designer in exterior design jürgen löffler, who also presented the design during the car's hong kong debut.the a1 is based on the volkswagen group pq25 platform, the same platform used in the seat ibiza mk4 and the vw polo mk5, and in its development audi has collaborated with seat.as of 23 june 2011, the 100,000th a1 was produced at audi brussels plant.a version of 2011 audi a1 painted by damien hirst was sold for £350,000.it was reported that, according to the director of e-mobility and sustainability strategy at audi of america, the a1 e-tron had never been scheduled for production.in march 2013, at the new york auto show, audi announced it will be expanding the testing of its a1 e-tron outside of munich to other regions of germany.production of the a1 e-tron was reported to be cancelled.it included 18-inch 'polygon' design alloy wheels, exterior styling package (front spoiler, double-blade roof spoiler, side skirts, rear diffuser in gloss black, stainless steel tailpipe trims), roof line, shoulder line with 'audi sport' lettering, number '1' on the bonnet and doors, boot lid, front spoiler lip, side skirts, wheel arch; surrounds and double-blade roof spoiler, rear sills with audi rings, centre console trim, door handles, floor mats, rear-view mirror trim (not available with auto-dimming mirror), air vent sleeves in high gloss white. |
camilla (minor planet designation: 107 camilla) is one of the largest asteroids from the outermost edge of the asteroid belt, approximately 250 kilometers (160 miles) in diameter.it is a member of the sylvia family and located within the cybele group.it was discovered on 17 november 1868, by english astronomer norman pogson at madras observatory, india, and named after camilla, queen of the volsci in roman mythology.the x-type asteroid is a rare trinary asteroid with two minor-planet moons discovered in 2001 and 2016, respectively.it is elongated in shape and has a short rotation period of 4.8 hours.a large number of rotational lightcurves of have been obtained from photometric observations since the 1980s.best rated results gave a short rotation period of 4.844 hours with a brightness amplitude between 0.32 and 0.53 magnitude.lightcurve analysis indicates that camilla's pole most likely points towards ecliptic coordinates (β, λ) = (+51°, 72°) with a 10° uncertainty, which gives it an axial tilt of 29°.follow-up modeling of photometric data gave similar results.according to the space-based surveys carried out by the japanese akari satellite, the infrared astronomical satellite iras and the neowise mission of nasa's wide-field infrared survey explorer, as well as observations by the keck observatory and photometric modeling, camilla measures between 185 and 247 kilometers in diameter and its surface has an albedo between 0.160 and 0.294.it has been designated s/2001 (107) 1 but has not yet received an official name.later observations in september 2005 with the very large telescope (vlt) allowed the determination of an orbit.apart from data in infobox, the inclination was found to be 3 ± 1° with respect to an axis pointing towards (β, λ) = (+55°, 75°).given the ~10° uncertainty in the actual rotational axis of camilla, one can say that the orbit's inclination is less than 10°.the satellite is estimated to measure about 11 km in diameter.assuming a similar density to the primary, this would give it an approximate mass of ~1.5×1015 kg.it has a similar colour to the primary.it has the provisional designation s/2016 (107) 1.observations were taken between 29 may 2015 and 30 july 2016, using the vlt-sphere, the principal instrument attached to the 8-meter 'melipal' (ut3) unit of the vlt.on 3 out of 5 observation sessions, the new satellite could be detected.the body's orbit has a semi-major axis of 340 kilometers.107 camilla and s/2001 (107) 1, orbit data website maintained by f. marchis.includes orbit diagrams.107 camilla at astdys-2, asteroids—dynamic site ephemeris · observation prediction · orbital info · proper elements · observational info 107 camilla at the jpl small-body database | 107 camilla | discoverer | e wells <tsp> 107 camilla | orbitalperiod | 236805 days <tsp> 107 camilla | periapsis | 4793430000 kilometres <tsp> 107 camilla | epoch | 2006-12-31 <tsp> 107 camilla | apoapsis | 5609370000 kilometres | no related information |
aaron turner (born november 5, 1977) is an american musician, singer, graphic artist, and founder of label hydra head records.he is most widely known for his role as guitarist and vocalist for the post-metal bands sumac and isis, while also participating in several other bands and projects such as old man gloom, lotus eaters and split cranium, a collaboration with jussi lehtisalo of finnish band circle who toured with isis in 2009.raised in new mexico, turner moved to the boston area, where he attended art school and formed isis and hydra head.in june 2003, turner moved operations of both the band and label to los angeles, california.turner now resides in vashon, wa which is also the base of operations for hydra head and his various other activities.in partnership with his wife faith coloccia, turner founded another record label, sige, in march 2011.it has gone on to release material from his musical collaboration with coloccia, mamiffer.sige is distributed by the business.at an early age, his family moved to new mexico, where he was raised.his mother was a teacher 'who taught a progressive curriculum' and his father an author, 'mainly [of] non-fiction'.turner describes his upbringing, surrounded by his parents' writer, artist and photographer friends, as 'creatively nurturing'.at age 17, he started a company that sold rare punk rock records via mail-order.he later moved to boston to attend art school at the school of the museum of fine arts, and in 1995 began releasing music.by 1997, the hydra head label was becoming a respectable small record label.turner describes his early industriousness as being motivated in part by boredom: i grew up in new mexico, and there wasn't a whole lot as far as youth culture is concerned.especially when i started to get interested in straight edge and wasn't doing drugs anymore, there was really nothing for me to do.so that was like a big reason for me, i suppose, to become really productive.also, i've never been a really social person.so there's not a lot of time taken up by my social life.and music has always been a very very big part of my life.i guess just a combination of those factors is why everything got started so early.around 1997–99, turner was living with future isis bassist and co-founder jeff caxide; until this point, he had been a member of the bands union suit and hollomen.isis was formed in 1997 out of a dissatisfaction with said bands' musical direction and turner and caxide's respective degrees of creative control.in mid-2009, turner moved from los angeles, where both isis and hydra head records were based at the time, to seattle with his then-girlfriend, faith coloccia; they went on to wed in september of the same year.he has also acquired a custom guitar from the electrical guitar company (as did fellow isis guitarist michael gallagher).in the past, turner has also used a gibson les paul standard, prs ce24, and has played through sunn, mesa boogie, and mackie amplifiers.when playing with isis, turner and his fellow guitarists usually tuned their instruments (low to high) b-f#-b-e-g#-b, to achieve a heavier sound.they also used other tunings, though less frequently, such as f# (octave below)-f#-b-e-g#-b.in 2016, turner described the live rig he used with sumac as consisting of two custom-built guitars from the electrical guitar company.both have lucite bodies and aluminum necks, and custom-wound wide frequency range pickups.the newer of the two—a prototype for a signature model—has a slightly flatter fingerboard radius than the older instrument. | aaron turner | associatedband/associatedmusicalartist | twilight band <tsp> twilight band | genre | black metal <tsp> aaron turner | associatedband/associatedmusicalartist | greymachine <tsp> aaron turner | instrument | electric guitar <tsp> black metal | musicfusiongenre | death metal | he is most widely known for his role as guitarist and vocalist for the post-metal bands sumac and isis, while also participating in several other bands and projects such as old man gloom, lotus eaters and split cranium, a collaboration with jussi lehtisalo of finnish band circle who toured with isis in 2009.he has also acquired a custom guitar from the electrical guitar company (as did fellow isis guitarist michael gallagher).in the past, turner has also used a gibson les paul standard, prs ce24, and has played through sunn, mesa boogie, and mackie amplifiers.when playing with isis, turner and his fellow guitarists usually tuned their instruments (low to high) b-f#-b-e-g#-b, to achieve a heavier sound.they also used other tunings, though less frequently, such as f# (octave below)-f#-b-e-g#-b.in 2016, turner described the live rig he used with sumac as consisting of two custom-built guitars from the electrical guitar company. |
the audi a1 (internally designated typ 8x) is a supermini car launched by audi at the 2010 geneva motor show.sales of the initial three-door a1 model started in germany in august 2010, with the united kingdom following in november 2010.a five-door version, called sportback, was launched in november 2011, with sales starting in export markets during spring 2012.the concept seats four and features a new plug-in hybrid powertrain.with this powertrain, a 1.4 l (85.4 cu in) 148 bhp (110.4 kw) turbo fsi engine drives the front wheels via a six-speed s-tronic, while a 40 bhp (29.8 kw; 40.6 ps) electric motor provides power to the rear wheels.the electric motor is also capable of producing 148 lb⋅ft (201 n⋅m) of torque.the metroproject quattro is able to travel 62 miles (100 km) at up to 62 mph (100 km/h) on one charge of its lithium-ion batteries, which reduces fuel consumption by up to 15%.both power sources are available to use simultaneously, with the driver then benefiting from macpherson strut front and rear four-link suspension configuration, electromechanical speed-sensitive power steering with a low energy draw, audi magnetic ride adaptive damping technology, and 0 to 100 km/h (0 to 62 mph) in 7.8 seconds.the vehicle was designed by audi ag project designer in exterior design jürgen löffler, who also presented the design during the car's hong kong debut.the vehicle's 0 to 100 km/h (0 to 62 mph) acceleration is 7.9 seconds and average co2 emissions are given as 92g/km.the vehicle's electric-only range is 50 km (31.07 mi).the vehicle was unveiled at the 2008 paris motor show.the car is aimed mostly at young, affluent urban buyers.se is the base specification, while sport and s line models also have sport seats, sports suspension and larger wheels, amongst other features.1.4-litre tfsi (122 ps (90 kw; 120 hp)) was sold as the 30 tfsi in china.the production version of the a1 quattro was tested by autocar magazine on mira's wet handling track alongside a nissan gt-r; the a1 recorded lap time over five seconds faster than the gt-r. autocar called the test a '...giant-killing result'.the a1 is based on the volkswagen group pq25 platform, the same platform used in the seat ibiza mk4 and the vw polo mk5, and in its development audi has collaborated with seat.as of 23 june 2011, the 100,000th a1 was produced at audi brussels plant.a version of 2011 audi a1 painted by damien hirst was sold for £350,000.a fully charged 12 kwh lithium-ion battery gives a maximum range of 50 km (31 mi), after which a 254 cc wankel engine is used to power a 15 kw (20 ps; 20 bhp) generator with a 12 l (2.6 imp gal; 3.2 us gal) fuel tank.this is estimated to provide an additional range of 124 mi (200 km).the company claims the car weighs 1,190 kg (2,624 lb), can reach 62 mph (100 km/h) in 10.2 seconds and a maximum speed of 80 mph (129 km/h).the vehicle was unveiled at the 2010 geneva motor show, followed by the 2012 taipei motor show.it was reported that, according to the director of e-mobility and sustainability strategy at audi of america, the a1 e-tron had never been scheduled for production.in march 2013, at the new york auto show, audi announced it will be expanding the testing of its a1 e-tron outside of munich to other regions of germany.production of the a1 e-tron was reported to be cancelled.it included 18-inch 'polygon' design alloy wheels, exterior styling package (front spoiler, double-blade roof spoiler, side skirts, rear diffuser in gloss black, stainless steel tailpipe trims), roof line, shoulder line with 'audi sport' lettering, number '1' on the bonnet and doors, boot lid, front spoiler lip, side skirts, wheel arch; surrounds and double-blade roof spoiler, rear sills with audi rings, centre console trim, door handles, floor mats, rear-view mirror trim (not available with auto-dimming mirror), air vent sleeves in high gloss white. | sermonically | ballsiest | agrimotor <tsp> sermonically | graffiti | immeshes | no related information |
aaron turner (born november 5, 1977) is an american musician, singer, graphic artist, and founder of label hydra head records.he is most widely known for his role as guitarist and vocalist for the post-metal bands sumac and isis, while also participating in several other bands and projects such as old man gloom, lotus eaters and split cranium, a collaboration with jussi lehtisalo of finnish band circle who toured with isis in 2009.raised in new mexico, turner moved to the boston area, where he attended art school and formed isis and hydra head.in june 2003, turner moved operations of both the band and label to los angeles, california.turner now resides in vashon, wa which is also the base of operations for hydra head and his various other activities.in partnership with his wife faith coloccia, turner founded another record label, sige, in march 2011.it has gone on to release material from his musical collaboration with coloccia, mamiffer.sige is distributed by the business.at an early age, his family moved to new mexico, where he was raised.his mother was a teacher 'who taught a progressive curriculum' and his father an author, 'mainly [of] non-fiction'.turner describes his upbringing, surrounded by his parents' writer, artist and photographer friends, as 'creatively nurturing'.at age 17, he started a company that sold rare punk rock records via mail-order.he later moved to boston to attend art school at the school of the museum of fine arts, and in 1995 began releasing music.by 1997, the hydra head label was becoming a respectable small record label.turner describes his early industriousness as being motivated in part by boredom: i grew up in new mexico, and there wasn't a whole lot as far as youth culture is concerned.especially when i started to get interested in straight edge and wasn't doing drugs anymore, there was really nothing for me to do.so that was like a big reason for me, i suppose, to become really productive.also, i've never been a really social person.so there's not a lot of time taken up by my social life.and music has always been a very very big part of my life.i guess just a combination of those factors is why everything got started so early.around 1997–99, turner was living with future isis bassist and co-founder jeff caxide; until this point, he had been a member of the bands union suit and hollomen.isis was formed in 1997 out of a dissatisfaction with said bands' musical direction and turner and caxide's respective degrees of creative control.in mid-2009, turner moved from los angeles, where both isis and hydra head records were based at the time, to seattle with his then-girlfriend, faith coloccia; they went on to wed in september of the same year.he has also acquired a custom guitar from the electrical guitar company (as did fellow isis guitarist michael gallagher).in the past, turner has also used a gibson les paul standard, prs ce24, and has played through sunn, mesa boogie, and mackie amplifiers.when playing with isis, turner and his fellow guitarists usually tuned their instruments (low to high) b-f#-b-e-g#-b, to achieve a heavier sound.they also used other tunings, though less frequently, such as f# (octave below)-f#-b-e-g#-b.in 2016, turner described the live rig he used with sumac as consisting of two custom-built guitars from the electrical guitar company.both have lucite bodies and aluminum necks, and custom-wound wide frequency range pickups.the newer of the two—a prototype for a signature model—has a slightly flatter fingerboard radius than the older instrument. | aaron turner | associatedband/associatedmusicalartist | twilight band <tsp> twilight band | genre | black metal <tsp> aaron turner | associatedband/associatedmusicalartist | greymachine <tsp> aaron turner | instrument | electric guitar <tsp> black metal | musicfusiongenre | death metal | he is most widely known for his role as guitarist and vocalist for the post-metal bands sumac and isis, while also participating in several other bands and projects such as old man gloom, lotus eaters and split cranium, a collaboration with jussi lehtisalo of finnish band circle who toured with isis in 2009.he has also acquired a custom guitar from the electrical guitar company (as did fellow isis guitarist michael gallagher).in the past, turner has also used a gibson les paul standard, prs ce24, and has played through sunn, mesa boogie, and mackie amplifiers.when playing with isis, turner and his fellow guitarists usually tuned their instruments (low to high) b-f#-b-e-g#-b, to achieve a heavier sound.they also used other tunings, though less frequently, such as f# (octave below)-f#-b-e-g#-b.in 2016, turner described the live rig he used with sumac as consisting of two custom-built guitars from the electrical guitar company. |
camilla (minor planet designation: 107 camilla) is one of the largest asteroids from the outermost edge of the asteroid belt, approximately 250 kilometers (160 miles) in diameter.it is a member of the sylvia family and located within the cybele group.it was discovered on 17 november 1868, by english astronomer norman pogson at madras observatory, india, and named after camilla, queen of the volsci in roman mythology.the x-type asteroid is a rare trinary asteroid with two minor-planet moons discovered in 2001 and 2016, respectively.it is elongated in shape and has a short rotation period of 4.8 hours.a large number of rotational lightcurves of have been obtained from photometric observations since the 1980s.best rated results gave a short rotation period of 4.844 hours with a brightness amplitude between 0.32 and 0.53 magnitude.lightcurve analysis indicates that camilla's pole most likely points towards ecliptic coordinates (β, λ) = (+51°, 72°) with a 10° uncertainty, which gives it an axial tilt of 29°.follow-up modeling of photometric data gave similar results.according to the space-based surveys carried out by the japanese akari satellite, the infrared astronomical satellite iras and the neowise mission of nasa's wide-field infrared survey explorer, as well as observations by the keck observatory and photometric modeling, camilla measures between 185 and 247 kilometers in diameter and its surface has an albedo between 0.160 and 0.294.it has been designated s/2001 (107) 1 but has not yet received an official name.later observations in september 2005 with the very large telescope (vlt) allowed the determination of an orbit.apart from data in infobox, the inclination was found to be 3 ± 1° with respect to an axis pointing towards (β, λ) = (+55°, 75°).given the ~10° uncertainty in the actual rotational axis of camilla, one can say that the orbit's inclination is less than 10°.the satellite is estimated to measure about 11 km in diameter.assuming a similar density to the primary, this would give it an approximate mass of ~1.5×1015 kg.it has a similar colour to the primary.it has the provisional designation s/2016 (107) 1.observations were taken between 29 may 2015 and 30 july 2016, using the vlt-sphere, the principal instrument attached to the 8-meter 'melipal' (ut3) unit of the vlt.on 3 out of 5 observation sessions, the new satellite could be detected.the body's orbit has a semi-major axis of 340 kilometers.107 camilla and s/2001 (107) 1, orbit data website maintained by f. marchis.includes orbit diagrams.107 camilla at astdys-2, asteroids—dynamic site ephemeris · observation prediction · orbital info · proper elements · observational info 107 camilla at the jpl small-body database | outsubtle | mimodrama | mousetraps <tsp> outsubtle | thornen | manubrium | no related information |
the audi a1 (internally designated typ 8x) is a supermini car launched by audi at the 2010 geneva motor show.sales of the initial three-door a1 model started in germany in august 2010, with the united kingdom following in november 2010.a five-door version, called sportback, was launched in november 2011, with sales starting in export markets during spring 2012.the concept seats four and features a new plug-in hybrid powertrain.with this powertrain, a 1.4 l (85.4 cu in) 148 bhp (110.4 kw) turbo fsi engine drives the front wheels via a six-speed s-tronic, while a 40 bhp (29.8 kw; 40.6 ps) electric motor provides power to the rear wheels.the electric motor is also capable of producing 148 lb⋅ft (201 n⋅m) of torque.the metroproject quattro is able to travel 62 miles (100 km) at up to 62 mph (100 km/h) on one charge of its lithium-ion batteries, which reduces fuel consumption by up to 15%.both power sources are available to use simultaneously, with the driver then benefiting from macpherson strut front and rear four-link suspension configuration, electromechanical speed-sensitive power steering with a low energy draw, audi magnetic ride adaptive damping technology, and 0 to 100 km/h (0 to 62 mph) in 7.8 seconds.the vehicle was designed by audi ag project designer in exterior design jürgen löffler, who also presented the design during the car's hong kong debut.the vehicle's 0 to 100 km/h (0 to 62 mph) acceleration is 7.9 seconds and average co2 emissions are given as 92g/km.the vehicle's electric-only range is 50 km (31.07 mi).the vehicle was unveiled at the 2008 paris motor show.the car is aimed mostly at young, affluent urban buyers.se is the base specification, while sport and s line models also have sport seats, sports suspension and larger wheels, amongst other features.1.4-litre tfsi (122 ps (90 kw; 120 hp)) was sold as the 30 tfsi in china.the production version of the a1 quattro was tested by autocar magazine on mira's wet handling track alongside a nissan gt-r; the a1 recorded lap time over five seconds faster than the gt-r. autocar called the test a '...giant-killing result'.the a1 is based on the volkswagen group pq25 platform, the same platform used in the seat ibiza mk4 and the vw polo mk5, and in its development audi has collaborated with seat.as of 23 june 2011, the 100,000th a1 was produced at audi brussels plant.a version of 2011 audi a1 painted by damien hirst was sold for £350,000.a fully charged 12 kwh lithium-ion battery gives a maximum range of 50 km (31 mi), after which a 254 cc wankel engine is used to power a 15 kw (20 ps; 20 bhp) generator with a 12 l (2.6 imp gal; 3.2 us gal) fuel tank.this is estimated to provide an additional range of 124 mi (200 km).the company claims the car weighs 1,190 kg (2,624 lb), can reach 62 mph (100 km/h) in 10.2 seconds and a maximum speed of 80 mph (129 km/h).the vehicle was unveiled at the 2010 geneva motor show, followed by the 2012 taipei motor show.it was reported that, according to the director of e-mobility and sustainability strategy at audi of america, the a1 e-tron had never been scheduled for production.in march 2013, at the new york auto show, audi announced it will be expanding the testing of its a1 e-tron outside of munich to other regions of germany.production of the a1 e-tron was reported to be cancelled.it included 18-inch 'polygon' design alloy wheels, exterior styling package (front spoiler, double-blade roof spoiler, side skirts, rear diffuser in gloss black, stainless steel tailpipe trims), roof line, shoulder line with 'audi sport' lettering, number '1' on the bonnet and doors, boot lid, front spoiler lip, side skirts, wheel arch; surrounds and double-blade roof spoiler, rear sills with audi rings, centre console trim, door handles, floor mats, rear-view mirror trim (not available with auto-dimming mirror), air vent sleeves in high gloss white. | audi a1 | manufacturer | audi <tsp> audi | foundedby | august horch <tsp> audi | division | audi e-tron <tsp> audi | subsidiary | quattro gmbh <tsp> audi | subsidiary | lamborghini | the audi a1 (internally designated typ 8x) is a supermini car launched by audi at the 2010 geneva motor show.both power sources are available to use simultaneously, with the driver then benefiting from macpherson strut front and rear four-link suspension configuration, electromechanical speed-sensitive power steering with a low energy draw, audi magnetic ride adaptive damping technology, and 0 to 100 km/h (0 to 62 mph) in 7.8 seconds.the vehicle was designed by audi ag project designer in exterior design jürgen löffler, who also presented the design during the car's hong kong debut.the a1 is based on the volkswagen group pq25 platform, the same platform used in the seat ibiza mk4 and the vw polo mk5, and in its development audi has collaborated with seat.as of 23 june 2011, the 100,000th a1 was produced at audi brussels plant.a version of 2011 audi a1 painted by damien hirst was sold for £350,000.it was reported that, according to the director of e-mobility and sustainability strategy at audi of america, the a1 e-tron had never been scheduled for production.in march 2013, at the new york auto show, audi announced it will be expanding the testing of its a1 e-tron outside of munich to other regions of germany.production of the a1 e-tron was reported to be cancelled.it included 18-inch 'polygon' design alloy wheels, exterior styling package (front spoiler, double-blade roof spoiler, side skirts, rear diffuser in gloss black, stainless steel tailpipe trims), roof line, shoulder line with 'audi sport' lettering, number '1' on the bonnet and doors, boot lid, front spoiler lip, side skirts, wheel arch; surrounds and double-blade roof spoiler, rear sills with audi rings, centre console trim, door handles, floor mats, rear-view mirror trim (not available with auto-dimming mirror), air vent sleeves in high gloss white. |
aaron turner (born november 5, 1977) is an american musician, singer, graphic artist, and founder of label hydra head records.he is most widely known for his role as guitarist and vocalist for the post-metal bands sumac and isis, while also participating in several other bands and projects such as old man gloom, lotus eaters and split cranium, a collaboration with jussi lehtisalo of finnish band circle who toured with isis in 2009.raised in new mexico, turner moved to the boston area, where he attended art school and formed isis and hydra head.in june 2003, turner moved operations of both the band and label to los angeles, california.turner now resides in vashon, wa which is also the base of operations for hydra head and his various other activities.in partnership with his wife faith coloccia, turner founded another record label, sige, in march 2011.it has gone on to release material from his musical collaboration with coloccia, mamiffer.sige is distributed by the business.at an early age, his family moved to new mexico, where he was raised.his mother was a teacher 'who taught a progressive curriculum' and his father an author, 'mainly [of] non-fiction'.turner describes his upbringing, surrounded by his parents' writer, artist and photographer friends, as 'creatively nurturing'.at age 17, he started a company that sold rare punk rock records via mail-order.he later moved to boston to attend art school at the school of the museum of fine arts, and in 1995 began releasing music.by 1997, the hydra head label was becoming a respectable small record label.turner describes his early industriousness as being motivated in part by boredom: i grew up in new mexico, and there wasn't a whole lot as far as youth culture is concerned.especially when i started to get interested in straight edge and wasn't doing drugs anymore, there was really nothing for me to do.so that was like a big reason for me, i suppose, to become really productive.also, i've never been a really social person.so there's not a lot of time taken up by my social life.and music has always been a very very big part of my life.i guess just a combination of those factors is why everything got started so early.around 1997–99, turner was living with future isis bassist and co-founder jeff caxide; until this point, he had been a member of the bands union suit and hollomen.isis was formed in 1997 out of a dissatisfaction with said bands' musical direction and turner and caxide's respective degrees of creative control.in mid-2009, turner moved from los angeles, where both isis and hydra head records were based at the time, to seattle with his then-girlfriend, faith coloccia; they went on to wed in september of the same year.he has also acquired a custom guitar from the electrical guitar company (as did fellow isis guitarist michael gallagher).in the past, turner has also used a gibson les paul standard, prs ce24, and has played through sunn, mesa boogie, and mackie amplifiers.when playing with isis, turner and his fellow guitarists usually tuned their instruments (low to high) b-f#-b-e-g#-b, to achieve a heavier sound.they also used other tunings, though less frequently, such as f# (octave below)-f#-b-e-g#-b.in 2016, turner described the live rig he used with sumac as consisting of two custom-built guitars from the electrical guitar company.both have lucite bodies and aluminum necks, and custom-wound wide frequency range pickups.the newer of the two—a prototype for a signature model—has a slightly flatter fingerboard radius than the older instrument. | aaron turner | associatedband/associatedmusicalartist | twilight band <tsp> twilight band | genre | black metal <tsp> aaron turner | associatedband/associatedmusicalartist | greymachine <tsp> aaron turner | instrument | electric guitar <tsp> black metal | musicfusiongenre | death metal | he is most widely known for his role as guitarist and vocalist for the post-metal bands sumac and isis, while also participating in several other bands and projects such as old man gloom, lotus eaters and split cranium, a collaboration with jussi lehtisalo of finnish band circle who toured with isis in 2009.he has also acquired a custom guitar from the electrical guitar company (as did fellow isis guitarist michael gallagher).in the past, turner has also used a gibson les paul standard, prs ce24, and has played through sunn, mesa boogie, and mackie amplifiers.when playing with isis, turner and his fellow guitarists usually tuned their instruments (low to high) b-f#-b-e-g#-b, to achieve a heavier sound.they also used other tunings, though less frequently, such as f# (octave below)-f#-b-e-g#-b.in 2016, turner described the live rig he used with sumac as consisting of two custom-built guitars from the electrical guitar company. |
camilla (minor planet designation: 107 camilla) is one of the largest asteroids from the outermost edge of the asteroid belt, approximately 250 kilometers (160 miles) in diameter.it is a member of the sylvia family and located within the cybele group.it was discovered on 17 november 1868, by english astronomer norman pogson at madras observatory, india, and named after camilla, queen of the volsci in roman mythology.the x-type asteroid is a rare trinary asteroid with two minor-planet moons discovered in 2001 and 2016, respectively.it is elongated in shape and has a short rotation period of 4.8 hours.a large number of rotational lightcurves of have been obtained from photometric observations since the 1980s.best rated results gave a short rotation period of 4.844 hours with a brightness amplitude between 0.32 and 0.53 magnitude.lightcurve analysis indicates that camilla's pole most likely points towards ecliptic coordinates (β, λ) = (+51°, 72°) with a 10° uncertainty, which gives it an axial tilt of 29°.follow-up modeling of photometric data gave similar results.according to the space-based surveys carried out by the japanese akari satellite, the infrared astronomical satellite iras and the neowise mission of nasa's wide-field infrared survey explorer, as well as observations by the keck observatory and photometric modeling, camilla measures between 185 and 247 kilometers in diameter and its surface has an albedo between 0.160 and 0.294.it has been designated s/2001 (107) 1 but has not yet received an official name.later observations in september 2005 with the very large telescope (vlt) allowed the determination of an orbit.apart from data in infobox, the inclination was found to be 3 ± 1° with respect to an axis pointing towards (β, λ) = (+55°, 75°).given the ~10° uncertainty in the actual rotational axis of camilla, one can say that the orbit's inclination is less than 10°.the satellite is estimated to measure about 11 km in diameter.assuming a similar density to the primary, this would give it an approximate mass of ~1.5×1015 kg.it has a similar colour to the primary.it has the provisional designation s/2016 (107) 1.observations were taken between 29 may 2015 and 30 july 2016, using the vlt-sphere, the principal instrument attached to the 8-meter 'melipal' (ut3) unit of the vlt.on 3 out of 5 observation sessions, the new satellite could be detected.the body's orbit has a semi-major axis of 340 kilometers.107 camilla and s/2001 (107) 1, orbit data website maintained by f. marchis.includes orbit diagrams.107 camilla at astdys-2, asteroids—dynamic site ephemeris · observation prediction · orbital info · proper elements · observational info 107 camilla at the jpl small-body database | 107 camilla | discoverer | n r pogson <tsp> n r pogson | deathplace | chennai <tsp> 107 camilla | orbitalperiod | 236805 days <tsp> n r pogson | birthplace | nottingham <tsp> n r pogson | nationality | england | it was discovered on 17 november 1868, by english astronomer norman pogson at madras observatory, india, and named after camilla, queen of the volsci in roman mythology. |
camilla (minor planet designation: 107 camilla) is one of the largest asteroids from the outermost edge of the asteroid belt, approximately 250 kilometers (160 miles) in diameter.it is a member of the sylvia family and located within the cybele group.it was discovered on 17 november 1868, by english astronomer norman pogson at madras observatory, india, and named after camilla, queen of the volsci in roman mythology.the x-type asteroid is a rare trinary asteroid with two minor-planet moons discovered in 2001 and 2016, respectively.it is elongated in shape and has a short rotation period of 4.8 hours.a large number of rotational lightcurves of have been obtained from photometric observations since the 1980s.best rated results gave a short rotation period of 4.844 hours with a brightness amplitude between 0.32 and 0.53 magnitude.lightcurve analysis indicates that camilla's pole most likely points towards ecliptic coordinates (β, λ) = (+51°, 72°) with a 10° uncertainty, which gives it an axial tilt of 29°.follow-up modeling of photometric data gave similar results.according to the space-based surveys carried out by the japanese akari satellite, the infrared astronomical satellite iras and the neowise mission of nasa's wide-field infrared survey explorer, as well as observations by the keck observatory and photometric modeling, camilla measures between 185 and 247 kilometers in diameter and its surface has an albedo between 0.160 and 0.294.it has been designated s/2001 (107) 1 but has not yet received an official name.later observations in september 2005 with the very large telescope (vlt) allowed the determination of an orbit.apart from data in infobox, the inclination was found to be 3 ± 1° with respect to an axis pointing towards (β, λ) = (+55°, 75°).given the ~10° uncertainty in the actual rotational axis of camilla, one can say that the orbit's inclination is less than 10°.the satellite is estimated to measure about 11 km in diameter.assuming a similar density to the primary, this would give it an approximate mass of ~1.5×1015 kg.it has a similar colour to the primary.it has the provisional designation s/2016 (107) 1.observations were taken between 29 may 2015 and 30 july 2016, using the vlt-sphere, the principal instrument attached to the 8-meter 'melipal' (ut3) unit of the vlt.on 3 out of 5 observation sessions, the new satellite could be detected.the body's orbit has a semi-major axis of 340 kilometers.107 camilla and s/2001 (107) 1, orbit data website maintained by f. marchis.includes orbit diagrams.107 camilla at astdys-2, asteroids—dynamic site ephemeris · observation prediction · orbital info · proper elements · observational info 107 camilla at the jpl small-body database | 107 camilla | discoverer | n r pogson <tsp> n r pogson | deathplace | chennai <tsp> 107 camilla | orbitalperiod | 236805 days <tsp> n r pogson | birthplace | nottingham <tsp> n r pogson | nationality | england | it was discovered on 17 november 1868, by english astronomer norman pogson at madras observatory, india, and named after camilla, queen of the volsci in roman mythology. |
aaron turner (born november 5, 1977) is an american musician, singer, graphic artist, and founder of label hydra head records.he is most widely known for his role as guitarist and vocalist for the post-metal bands sumac and isis, while also participating in several other bands and projects such as old man gloom, lotus eaters and split cranium, a collaboration with jussi lehtisalo of finnish band circle who toured with isis in 2009.raised in new mexico, turner moved to the boston area, where he attended art school and formed isis and hydra head.in june 2003, turner moved operations of both the band and label to los angeles, california.turner now resides in vashon, wa which is also the base of operations for hydra head and his various other activities.in partnership with his wife faith coloccia, turner founded another record label, sige, in march 2011.it has gone on to release material from his musical collaboration with coloccia, mamiffer.sige is distributed by the business.at an early age, his family moved to new mexico, where he was raised.his mother was a teacher 'who taught a progressive curriculum' and his father an author, 'mainly [of] non-fiction'.turner describes his upbringing, surrounded by his parents' writer, artist and photographer friends, as 'creatively nurturing'.at age 17, he started a company that sold rare punk rock records via mail-order.he later moved to boston to attend art school at the school of the museum of fine arts, and in 1995 began releasing music.by 1997, the hydra head label was becoming a respectable small record label.turner describes his early industriousness as being motivated in part by boredom: i grew up in new mexico, and there wasn't a whole lot as far as youth culture is concerned.especially when i started to get interested in straight edge and wasn't doing drugs anymore, there was really nothing for me to do.so that was like a big reason for me, i suppose, to become really productive.also, i've never been a really social person.so there's not a lot of time taken up by my social life.and music has always been a very very big part of my life.i guess just a combination of those factors is why everything got started so early.around 1997–99, turner was living with future isis bassist and co-founder jeff caxide; until this point, he had been a member of the bands union suit and hollomen.isis was formed in 1997 out of a dissatisfaction with said bands' musical direction and turner and caxide's respective degrees of creative control.in mid-2009, turner moved from los angeles, where both isis and hydra head records were based at the time, to seattle with his then-girlfriend, faith coloccia; they went on to wed in september of the same year.he has also acquired a custom guitar from the electrical guitar company (as did fellow isis guitarist michael gallagher).in the past, turner has also used a gibson les paul standard, prs ce24, and has played through sunn, mesa boogie, and mackie amplifiers.when playing with isis, turner and his fellow guitarists usually tuned their instruments (low to high) b-f#-b-e-g#-b, to achieve a heavier sound.they also used other tunings, though less frequently, such as f# (octave below)-f#-b-e-g#-b.in 2016, turner described the live rig he used with sumac as consisting of two custom-built guitars from the electrical guitar company.both have lucite bodies and aluminum necks, and custom-wound wide frequency range pickups.the newer of the two—a prototype for a signature model—has a slightly flatter fingerboard radius than the older instrument. | pneumatosic | neuralgia | nuque | no related information |
the audi a1 (internally designated typ 8x) is a supermini car launched by audi at the 2010 geneva motor show.sales of the initial three-door a1 model started in germany in august 2010, with the united kingdom following in november 2010.a five-door version, called sportback, was launched in november 2011, with sales starting in export markets during spring 2012.the concept seats four and features a new plug-in hybrid powertrain.with this powertrain, a 1.4 l (85.4 cu in) 148 bhp (110.4 kw) turbo fsi engine drives the front wheels via a six-speed s-tronic, while a 40 bhp (29.8 kw; 40.6 ps) electric motor provides power to the rear wheels.the electric motor is also capable of producing 148 lb⋅ft (201 n⋅m) of torque.the metroproject quattro is able to travel 62 miles (100 km) at up to 62 mph (100 km/h) on one charge of its lithium-ion batteries, which reduces fuel consumption by up to 15%.both power sources are available to use simultaneously, with the driver then benefiting from macpherson strut front and rear four-link suspension configuration, electromechanical speed-sensitive power steering with a low energy draw, audi magnetic ride adaptive damping technology, and 0 to 100 km/h (0 to 62 mph) in 7.8 seconds.the vehicle was designed by audi ag project designer in exterior design jürgen löffler, who also presented the design during the car's hong kong debut.the vehicle's 0 to 100 km/h (0 to 62 mph) acceleration is 7.9 seconds and average co2 emissions are given as 92g/km.the vehicle's electric-only range is 50 km (31.07 mi).the vehicle was unveiled at the 2008 paris motor show.the car is aimed mostly at young, affluent urban buyers.se is the base specification, while sport and s line models also have sport seats, sports suspension and larger wheels, amongst other features.1.4-litre tfsi (122 ps (90 kw; 120 hp)) was sold as the 30 tfsi in china.the production version of the a1 quattro was tested by autocar magazine on mira's wet handling track alongside a nissan gt-r; the a1 recorded lap time over five seconds faster than the gt-r. autocar called the test a '...giant-killing result'.the a1 is based on the volkswagen group pq25 platform, the same platform used in the seat ibiza mk4 and the vw polo mk5, and in its development audi has collaborated with seat.as of 23 june 2011, the 100,000th a1 was produced at audi brussels plant.a version of 2011 audi a1 painted by damien hirst was sold for £350,000.a fully charged 12 kwh lithium-ion battery gives a maximum range of 50 km (31 mi), after which a 254 cc wankel engine is used to power a 15 kw (20 ps; 20 bhp) generator with a 12 l (2.6 imp gal; 3.2 us gal) fuel tank.this is estimated to provide an additional range of 124 mi (200 km).the company claims the car weighs 1,190 kg (2,624 lb), can reach 62 mph (100 km/h) in 10.2 seconds and a maximum speed of 80 mph (129 km/h).the vehicle was unveiled at the 2010 geneva motor show, followed by the 2012 taipei motor show.it was reported that, according to the director of e-mobility and sustainability strategy at audi of america, the a1 e-tron had never been scheduled for production.in march 2013, at the new york auto show, audi announced it will be expanding the testing of its a1 e-tron outside of munich to other regions of germany.production of the a1 e-tron was reported to be cancelled.it included 18-inch 'polygon' design alloy wheels, exterior styling package (front spoiler, double-blade roof spoiler, side skirts, rear diffuser in gloss black, stainless steel tailpipe trims), roof line, shoulder line with 'audi sport' lettering, number '1' on the bonnet and doors, boot lid, front spoiler lip, side skirts, wheel arch; surrounds and double-blade roof spoiler, rear sills with audi rings, centre console trim, door handles, floor mats, rear-view mirror trim (not available with auto-dimming mirror), air vent sleeves in high gloss white. | opposability | kanaima | geneses <tsp> opposability | appellations | chocard | no related information |
aaron turner (born november 5, 1977) is an american musician, singer, graphic artist, and founder of label hydra head records.he is most widely known for his role as guitarist and vocalist for the post-metal bands sumac and isis, while also participating in several other bands and projects such as old man gloom, lotus eaters and split cranium, a collaboration with jussi lehtisalo of finnish band circle who toured with isis in 2009.raised in new mexico, turner moved to the boston area, where he attended art school and formed isis and hydra head.in june 2003, turner moved operations of both the band and label to los angeles, california.turner now resides in vashon, wa which is also the base of operations for hydra head and his various other activities.in partnership with his wife faith coloccia, turner founded another record label, sige, in march 2011.it has gone on to release material from his musical collaboration with coloccia, mamiffer.sige is distributed by the business.at an early age, his family moved to new mexico, where he was raised.his mother was a teacher 'who taught a progressive curriculum' and his father an author, 'mainly [of] non-fiction'.turner describes his upbringing, surrounded by his parents' writer, artist and photographer friends, as 'creatively nurturing'.at age 17, he started a company that sold rare punk rock records via mail-order.he later moved to boston to attend art school at the school of the museum of fine arts, and in 1995 began releasing music.by 1997, the hydra head label was becoming a respectable small record label.turner describes his early industriousness as being motivated in part by boredom: i grew up in new mexico, and there wasn't a whole lot as far as youth culture is concerned.especially when i started to get interested in straight edge and wasn't doing drugs anymore, there was really nothing for me to do.so that was like a big reason for me, i suppose, to become really productive.also, i've never been a really social person.so there's not a lot of time taken up by my social life.and music has always been a very very big part of my life.i guess just a combination of those factors is why everything got started so early.around 1997–99, turner was living with future isis bassist and co-founder jeff caxide; until this point, he had been a member of the bands union suit and hollomen.isis was formed in 1997 out of a dissatisfaction with said bands' musical direction and turner and caxide's respective degrees of creative control.in mid-2009, turner moved from los angeles, where both isis and hydra head records were based at the time, to seattle with his then-girlfriend, faith coloccia; they went on to wed in september of the same year.he has also acquired a custom guitar from the electrical guitar company (as did fellow isis guitarist michael gallagher).in the past, turner has also used a gibson les paul standard, prs ce24, and has played through sunn, mesa boogie, and mackie amplifiers.when playing with isis, turner and his fellow guitarists usually tuned their instruments (low to high) b-f#-b-e-g#-b, to achieve a heavier sound.they also used other tunings, though less frequently, such as f# (octave below)-f#-b-e-g#-b.in 2016, turner described the live rig he used with sumac as consisting of two custom-built guitars from the electrical guitar company.both have lucite bodies and aluminum necks, and custom-wound wide frequency range pickups.the newer of the two—a prototype for a signature model—has a slightly flatter fingerboard radius than the older instrument. | aaron turner | associatedband/associatedmusicalartist | twilight band <tsp> twilight band | genre | black metal <tsp> aaron turner | associatedband/associatedmusicalartist | mamiffer <tsp> aaron turner | instrument | singing <tsp> black metal | musicfusiongenre | death metal | he is most widely known for his role as guitarist and vocalist for the post-metal bands sumac and isis, while also participating in several other bands and projects such as old man gloom, lotus eaters and split cranium, a collaboration with jussi lehtisalo of finnish band circle who toured with isis in 2009. |
camilla (minor planet designation: 107 camilla) is one of the largest asteroids from the outermost edge of the asteroid belt, approximately 250 kilometers (160 miles) in diameter.it is a member of the sylvia family and located within the cybele group.it was discovered on 17 november 1868, by english astronomer norman pogson at madras observatory, india, and named after camilla, queen of the volsci in roman mythology.the x-type asteroid is a rare trinary asteroid with two minor-planet moons discovered in 2001 and 2016, respectively.it is elongated in shape and has a short rotation period of 4.8 hours.a large number of rotational lightcurves of have been obtained from photometric observations since the 1980s.best rated results gave a short rotation period of 4.844 hours with a brightness amplitude between 0.32 and 0.53 magnitude.lightcurve analysis indicates that camilla's pole most likely points towards ecliptic coordinates (β, λ) = (+51°, 72°) with a 10° uncertainty, which gives it an axial tilt of 29°.follow-up modeling of photometric data gave similar results.according to the space-based surveys carried out by the japanese akari satellite, the infrared astronomical satellite iras and the neowise mission of nasa's wide-field infrared survey explorer, as well as observations by the keck observatory and photometric modeling, camilla measures between 185 and 247 kilometers in diameter and its surface has an albedo between 0.160 and 0.294.it has been designated s/2001 (107) 1 but has not yet received an official name.later observations in september 2005 with the very large telescope (vlt) allowed the determination of an orbit.apart from data in infobox, the inclination was found to be 3 ± 1° with respect to an axis pointing towards (β, λ) = (+55°, 75°).given the ~10° uncertainty in the actual rotational axis of camilla, one can say that the orbit's inclination is less than 10°.the satellite is estimated to measure about 11 km in diameter.assuming a similar density to the primary, this would give it an approximate mass of ~1.5×1015 kg.it has a similar colour to the primary.it has the provisional designation s/2016 (107) 1.observations were taken between 29 may 2015 and 30 july 2016, using the vlt-sphere, the principal instrument attached to the 8-meter 'melipal' (ut3) unit of the vlt.on 3 out of 5 observation sessions, the new satellite could be detected.the body's orbit has a semi-major axis of 340 kilometers.107 camilla and s/2001 (107) 1, orbit data website maintained by f. marchis.includes orbit diagrams.107 camilla at astdys-2, asteroids—dynamic site ephemeris · observation prediction · orbital info · proper elements · observational info 107 camilla at the jpl small-body database | reimprint | grace | subjee <tsp> reimprint | rook | caffeic | no related information |
the audi a1 (internally designated typ 8x) is a supermini car launched by audi at the 2010 geneva motor show.sales of the initial three-door a1 model started in germany in august 2010, with the united kingdom following in november 2010.a five-door version, called sportback, was launched in november 2011, with sales starting in export markets during spring 2012.the concept seats four and features a new plug-in hybrid powertrain.with this powertrain, a 1.4 l (85.4 cu in) 148 bhp (110.4 kw) turbo fsi engine drives the front wheels via a six-speed s-tronic, while a 40 bhp (29.8 kw; 40.6 ps) electric motor provides power to the rear wheels.the electric motor is also capable of producing 148 lb⋅ft (201 n⋅m) of torque.the metroproject quattro is able to travel 62 miles (100 km) at up to 62 mph (100 km/h) on one charge of its lithium-ion batteries, which reduces fuel consumption by up to 15%.both power sources are available to use simultaneously, with the driver then benefiting from macpherson strut front and rear four-link suspension configuration, electromechanical speed-sensitive power steering with a low energy draw, audi magnetic ride adaptive damping technology, and 0 to 100 km/h (0 to 62 mph) in 7.8 seconds.the vehicle was designed by audi ag project designer in exterior design jürgen löffler, who also presented the design during the car's hong kong debut.the vehicle's 0 to 100 km/h (0 to 62 mph) acceleration is 7.9 seconds and average co2 emissions are given as 92g/km.the vehicle's electric-only range is 50 km (31.07 mi).the vehicle was unveiled at the 2008 paris motor show.the car is aimed mostly at young, affluent urban buyers.se is the base specification, while sport and s line models also have sport seats, sports suspension and larger wheels, amongst other features.1.4-litre tfsi (122 ps (90 kw; 120 hp)) was sold as the 30 tfsi in china.the production version of the a1 quattro was tested by autocar magazine on mira's wet handling track alongside a nissan gt-r; the a1 recorded lap time over five seconds faster than the gt-r. autocar called the test a '...giant-killing result'.the a1 is based on the volkswagen group pq25 platform, the same platform used in the seat ibiza mk4 and the vw polo mk5, and in its development audi has collaborated with seat.as of 23 june 2011, the 100,000th a1 was produced at audi brussels plant.a version of 2011 audi a1 painted by damien hirst was sold for £350,000.a fully charged 12 kwh lithium-ion battery gives a maximum range of 50 km (31 mi), after which a 254 cc wankel engine is used to power a 15 kw (20 ps; 20 bhp) generator with a 12 l (2.6 imp gal; 3.2 us gal) fuel tank.this is estimated to provide an additional range of 124 mi (200 km).the company claims the car weighs 1,190 kg (2,624 lb), can reach 62 mph (100 km/h) in 10.2 seconds and a maximum speed of 80 mph (129 km/h).the vehicle was unveiled at the 2010 geneva motor show, followed by the 2012 taipei motor show.it was reported that, according to the director of e-mobility and sustainability strategy at audi of america, the a1 e-tron had never been scheduled for production.in march 2013, at the new york auto show, audi announced it will be expanding the testing of its a1 e-tron outside of munich to other regions of germany.production of the a1 e-tron was reported to be cancelled.it included 18-inch 'polygon' design alloy wheels, exterior styling package (front spoiler, double-blade roof spoiler, side skirts, rear diffuser in gloss black, stainless steel tailpipe trims), roof line, shoulder line with 'audi sport' lettering, number '1' on the bonnet and doors, boot lid, front spoiler lip, side skirts, wheel arch; surrounds and double-blade roof spoiler, rear sills with audi rings, centre console trim, door handles, floor mats, rear-view mirror trim (not available with auto-dimming mirror), air vent sleeves in high gloss white. | audi a1 | manufacturer | audi <tsp> audi | foundedby | august horch <tsp> audi | subsidiary | ducati <tsp> audi | division | audi e-tron <tsp> audi | subsidiary | quattro gmbh | the audi a1 (internally designated typ 8x) is a supermini car launched by audi at the 2010 geneva motor show.both power sources are available to use simultaneously, with the driver then benefiting from macpherson strut front and rear four-link suspension configuration, electromechanical speed-sensitive power steering with a low energy draw, audi magnetic ride adaptive damping technology, and 0 to 100 km/h (0 to 62 mph) in 7.8 seconds.the vehicle was designed by audi ag project designer in exterior design jürgen löffler, who also presented the design during the car's hong kong debut.the a1 is based on the volkswagen group pq25 platform, the same platform used in the seat ibiza mk4 and the vw polo mk5, and in its development audi has collaborated with seat.as of 23 june 2011, the 100,000th a1 was produced at audi brussels plant.a version of 2011 audi a1 painted by damien hirst was sold for £350,000.it was reported that, according to the director of e-mobility and sustainability strategy at audi of america, the a1 e-tron had never been scheduled for production.in march 2013, at the new york auto show, audi announced it will be expanding the testing of its a1 e-tron outside of munich to other regions of germany.production of the a1 e-tron was reported to be cancelled.it included 18-inch 'polygon' design alloy wheels, exterior styling package (front spoiler, double-blade roof spoiler, side skirts, rear diffuser in gloss black, stainless steel tailpipe trims), roof line, shoulder line with 'audi sport' lettering, number '1' on the bonnet and doors, boot lid, front spoiler lip, side skirts, wheel arch; surrounds and double-blade roof spoiler, rear sills with audi rings, centre console trim, door handles, floor mats, rear-view mirror trim (not available with auto-dimming mirror), air vent sleeves in high gloss white. |
camilla (minor planet designation: 107 camilla) is one of the largest asteroids from the outermost edge of the asteroid belt, approximately 250 kilometers (160 miles) in diameter.it is a member of the sylvia family and located within the cybele group.it was discovered on 17 november 1868, by english astronomer norman pogson at madras observatory, india, and named after camilla, queen of the volsci in roman mythology.the x-type asteroid is a rare trinary asteroid with two minor-planet moons discovered in 2001 and 2016, respectively.it is elongated in shape and has a short rotation period of 4.8 hours.a large number of rotational lightcurves of have been obtained from photometric observations since the 1980s.best rated results gave a short rotation period of 4.844 hours with a brightness amplitude between 0.32 and 0.53 magnitude.lightcurve analysis indicates that camilla's pole most likely points towards ecliptic coordinates (β, λ) = (+51°, 72°) with a 10° uncertainty, which gives it an axial tilt of 29°.follow-up modeling of photometric data gave similar results.according to the space-based surveys carried out by the japanese akari satellite, the infrared astronomical satellite iras and the neowise mission of nasa's wide-field infrared survey explorer, as well as observations by the keck observatory and photometric modeling, camilla measures between 185 and 247 kilometers in diameter and its surface has an albedo between 0.160 and 0.294.it has been designated s/2001 (107) 1 but has not yet received an official name.later observations in september 2005 with the very large telescope (vlt) allowed the determination of an orbit.apart from data in infobox, the inclination was found to be 3 ± 1° with respect to an axis pointing towards (β, λ) = (+55°, 75°).given the ~10° uncertainty in the actual rotational axis of camilla, one can say that the orbit's inclination is less than 10°.the satellite is estimated to measure about 11 km in diameter.assuming a similar density to the primary, this would give it an approximate mass of ~1.5×1015 kg.it has a similar colour to the primary.it has the provisional designation s/2016 (107) 1.observations were taken between 29 may 2015 and 30 july 2016, using the vlt-sphere, the principal instrument attached to the 8-meter 'melipal' (ut3) unit of the vlt.on 3 out of 5 observation sessions, the new satellite could be detected.the body's orbit has a semi-major axis of 340 kilometers.107 camilla and s/2001 (107) 1, orbit data website maintained by f. marchis.includes orbit diagrams.107 camilla at astdys-2, asteroids—dynamic site ephemeris · observation prediction · orbital info · proper elements · observational info 107 camilla at the jpl small-body database | 107 camilla | discoverer | n r pogson <tsp> n r pogson | deathplace | chennai <tsp> 107 camilla | periapsis | 4793430000 kilometres <tsp> n r pogson | birthplace | nottingham <tsp> n r pogson | nationality | england | it was discovered on 17 november 1868, by english astronomer norman pogson at madras observatory, india, and named after camilla, queen of the volsci in roman mythology. |
aaron turner (born november 5, 1977) is an american musician, singer, graphic artist, and founder of label hydra head records.he is most widely known for his role as guitarist and vocalist for the post-metal bands sumac and isis, while also participating in several other bands and projects such as old man gloom, lotus eaters and split cranium, a collaboration with jussi lehtisalo of finnish band circle who toured with isis in 2009.raised in new mexico, turner moved to the boston area, where he attended art school and formed isis and hydra head.in june 2003, turner moved operations of both the band and label to los angeles, california.turner now resides in vashon, wa which is also the base of operations for hydra head and his various other activities.in partnership with his wife faith coloccia, turner founded another record label, sige, in march 2011.it has gone on to release material from his musical collaboration with coloccia, mamiffer.sige is distributed by the business.at an early age, his family moved to new mexico, where he was raised.his mother was a teacher 'who taught a progressive curriculum' and his father an author, 'mainly [of] non-fiction'.turner describes his upbringing, surrounded by his parents' writer, artist and photographer friends, as 'creatively nurturing'.at age 17, he started a company that sold rare punk rock records via mail-order.he later moved to boston to attend art school at the school of the museum of fine arts, and in 1995 began releasing music.by 1997, the hydra head label was becoming a respectable small record label.turner describes his early industriousness as being motivated in part by boredom: i grew up in new mexico, and there wasn't a whole lot as far as youth culture is concerned.especially when i started to get interested in straight edge and wasn't doing drugs anymore, there was really nothing for me to do.so that was like a big reason for me, i suppose, to become really productive.also, i've never been a really social person.so there's not a lot of time taken up by my social life.and music has always been a very very big part of my life.i guess just a combination of those factors is why everything got started so early.around 1997–99, turner was living with future isis bassist and co-founder jeff caxide; until this point, he had been a member of the bands union suit and hollomen.isis was formed in 1997 out of a dissatisfaction with said bands' musical direction and turner and caxide's respective degrees of creative control.in mid-2009, turner moved from los angeles, where both isis and hydra head records were based at the time, to seattle with his then-girlfriend, faith coloccia; they went on to wed in september of the same year.he has also acquired a custom guitar from the electrical guitar company (as did fellow isis guitarist michael gallagher).in the past, turner has also used a gibson les paul standard, prs ce24, and has played through sunn, mesa boogie, and mackie amplifiers.when playing with isis, turner and his fellow guitarists usually tuned their instruments (low to high) b-f#-b-e-g#-b, to achieve a heavier sound.they also used other tunings, though less frequently, such as f# (octave below)-f#-b-e-g#-b.in 2016, turner described the live rig he used with sumac as consisting of two custom-built guitars from the electrical guitar company.both have lucite bodies and aluminum necks, and custom-wound wide frequency range pickups.the newer of the two—a prototype for a signature model—has a slightly flatter fingerboard radius than the older instrument. | boskiest | ripraps | emender <tsp> boskiest | accus | trochisk | no related information |
the audi a1 (internally designated typ 8x) is a supermini car launched by audi at the 2010 geneva motor show.sales of the initial three-door a1 model started in germany in august 2010, with the united kingdom following in november 2010.a five-door version, called sportback, was launched in november 2011, with sales starting in export markets during spring 2012.the concept seats four and features a new plug-in hybrid powertrain.with this powertrain, a 1.4 l (85.4 cu in) 148 bhp (110.4 kw) turbo fsi engine drives the front wheels via a six-speed s-tronic, while a 40 bhp (29.8 kw; 40.6 ps) electric motor provides power to the rear wheels.the electric motor is also capable of producing 148 lb⋅ft (201 n⋅m) of torque.the metroproject quattro is able to travel 62 miles (100 km) at up to 62 mph (100 km/h) on one charge of its lithium-ion batteries, which reduces fuel consumption by up to 15%.both power sources are available to use simultaneously, with the driver then benefiting from macpherson strut front and rear four-link suspension configuration, electromechanical speed-sensitive power steering with a low energy draw, audi magnetic ride adaptive damping technology, and 0 to 100 km/h (0 to 62 mph) in 7.8 seconds.the vehicle was designed by audi ag project designer in exterior design jürgen löffler, who also presented the design during the car's hong kong debut.the vehicle's 0 to 100 km/h (0 to 62 mph) acceleration is 7.9 seconds and average co2 emissions are given as 92g/km.the vehicle's electric-only range is 50 km (31.07 mi).the vehicle was unveiled at the 2008 paris motor show.the car is aimed mostly at young, affluent urban buyers.se is the base specification, while sport and s line models also have sport seats, sports suspension and larger wheels, amongst other features.1.4-litre tfsi (122 ps (90 kw; 120 hp)) was sold as the 30 tfsi in china.the production version of the a1 quattro was tested by autocar magazine on mira's wet handling track alongside a nissan gt-r; the a1 recorded lap time over five seconds faster than the gt-r. autocar called the test a '...giant-killing result'.the a1 is based on the volkswagen group pq25 platform, the same platform used in the seat ibiza mk4 and the vw polo mk5, and in its development audi has collaborated with seat.as of 23 june 2011, the 100,000th a1 was produced at audi brussels plant.a version of 2011 audi a1 painted by damien hirst was sold for £350,000.a fully charged 12 kwh lithium-ion battery gives a maximum range of 50 km (31 mi), after which a 254 cc wankel engine is used to power a 15 kw (20 ps; 20 bhp) generator with a 12 l (2.6 imp gal; 3.2 us gal) fuel tank.this is estimated to provide an additional range of 124 mi (200 km).the company claims the car weighs 1,190 kg (2,624 lb), can reach 62 mph (100 km/h) in 10.2 seconds and a maximum speed of 80 mph (129 km/h).the vehicle was unveiled at the 2010 geneva motor show, followed by the 2012 taipei motor show.it was reported that, according to the director of e-mobility and sustainability strategy at audi of america, the a1 e-tron had never been scheduled for production.in march 2013, at the new york auto show, audi announced it will be expanding the testing of its a1 e-tron outside of munich to other regions of germany.production of the a1 e-tron was reported to be cancelled.it included 18-inch 'polygon' design alloy wheels, exterior styling package (front spoiler, double-blade roof spoiler, side skirts, rear diffuser in gloss black, stainless steel tailpipe trims), roof line, shoulder line with 'audi sport' lettering, number '1' on the bonnet and doors, boot lid, front spoiler lip, side skirts, wheel arch; surrounds and double-blade roof spoiler, rear sills with audi rings, centre console trim, door handles, floor mats, rear-view mirror trim (not available with auto-dimming mirror), air vent sleeves in high gloss white. | callboys | aplacophora | fastest <tsp> callboys | coarticulate | diaculum | no related information |
camilla (minor planet designation: 107 camilla) is one of the largest asteroids from the outermost edge of the asteroid belt, approximately 250 kilometers (160 miles) in diameter.it is a member of the sylvia family and located within the cybele group.it was discovered on 17 november 1868, by english astronomer norman pogson at madras observatory, india, and named after camilla, queen of the volsci in roman mythology.the x-type asteroid is a rare trinary asteroid with two minor-planet moons discovered in 2001 and 2016, respectively.it is elongated in shape and has a short rotation period of 4.8 hours.a large number of rotational lightcurves of have been obtained from photometric observations since the 1980s.best rated results gave a short rotation period of 4.844 hours with a brightness amplitude between 0.32 and 0.53 magnitude.lightcurve analysis indicates that camilla's pole most likely points towards ecliptic coordinates (β, λ) = (+51°, 72°) with a 10° uncertainty, which gives it an axial tilt of 29°.follow-up modeling of photometric data gave similar results.according to the space-based surveys carried out by the japanese akari satellite, the infrared astronomical satellite iras and the neowise mission of nasa's wide-field infrared survey explorer, as well as observations by the keck observatory and photometric modeling, camilla measures between 185 and 247 kilometers in diameter and its surface has an albedo between 0.160 and 0.294.it has been designated s/2001 (107) 1 but has not yet received an official name.later observations in september 2005 with the very large telescope (vlt) allowed the determination of an orbit.apart from data in infobox, the inclination was found to be 3 ± 1° with respect to an axis pointing towards (β, λ) = (+55°, 75°).given the ~10° uncertainty in the actual rotational axis of camilla, one can say that the orbit's inclination is less than 10°.the satellite is estimated to measure about 11 km in diameter.assuming a similar density to the primary, this would give it an approximate mass of ~1.5×1015 kg.it has a similar colour to the primary.it has the provisional designation s/2016 (107) 1.observations were taken between 29 may 2015 and 30 july 2016, using the vlt-sphere, the principal instrument attached to the 8-meter 'melipal' (ut3) unit of the vlt.on 3 out of 5 observation sessions, the new satellite could be detected.the body's orbit has a semi-major axis of 340 kilometers.107 camilla and s/2001 (107) 1, orbit data website maintained by f. marchis.includes orbit diagrams.107 camilla at astdys-2, asteroids—dynamic site ephemeris · observation prediction · orbital info · proper elements · observational info 107 camilla at the jpl small-body database | prosecutors | shahaptian | ruralizes <tsp> prosecutors | sarrow | currishness | no related information |
marcin 'abradab' marten (born 12 november 1978 in katowice) is a polish rapper and music producer.marten is a founding member of polish hip-hop group kaliber 44 and, since 2002, a solo artist.he is a member of polish society of the phonographic industry (związek producentów audio video, zpav).marten is a winner of two fryderyk awards.in 2011, machina magazine placed marten at no.17 on the list of 30 best polish rappers.he has also collaborated with artists like piotr banach, bosski roman, maciej maleńczuk, wojciech waglewski, grubson, l.u.c and o.s.t.r.the group was joined by piotr łuszcz performing under pseudonym mag magik i.in 1995, kaliber 44 was signed to s. p. records, and a year later their debut album księga tajemnicza.prolog was released.in 1998, after the group recorded its second album w 63 minuty dookoła świata, piotr 'magik' łuszcz left the band and formed paktofonika.kaliber 44's third album 3:44 was released in 2000.on 6 june 2004, he released his first solo album czerwony album through s. p. records.the album charted at no.21 on olis.the album featured a popular song titled 'rapowe ziarno 2 (szyderap)', for which a music video was released.the album won fryderyk award in the 'album of the year - hip-hop/r&b' category, while 'rapowe ziarno 2 (szyderap)' received a nomination in the 'video of the year' category.abradab's second album emisja spalin was released on 1 december 2005 and featured guest appearances by rapper numer raz and abradab's brother joka.the album peak at no.38 on olis.emisja spalin was followed by ostatni poziom kontroli, which was released on 3 october 2008 and featured grubson, reggae singer marika and igs.the album peaked at no.42 on olis.both albums received nominations for fryderyk award.on 4 october 2010, the fourth solo record by abradab was released.the album, titled abradabing and produced by rapper o.s.t.r., received a fryderyk award for hip-hop/r&b album of the year.marten's fifth studio album, extravertik, was released on 21 april 2012 through abradab's record label inna-my-twórnia. | phylactolaema | frats | assaulting | no related information |
the audi a1 (internally designated typ 8x) is a supermini car launched by audi at the 2010 geneva motor show.sales of the initial three-door a1 model started in germany in august 2010, with the united kingdom following in november 2010.a five-door version, called sportback, was launched in november 2011, with sales starting in export markets during spring 2012.the concept seats four and features a new plug-in hybrid powertrain.with this powertrain, a 1.4 l (85.4 cu in) 148 bhp (110.4 kw) turbo fsi engine drives the front wheels via a six-speed s-tronic, while a 40 bhp (29.8 kw; 40.6 ps) electric motor provides power to the rear wheels.the electric motor is also capable of producing 148 lb⋅ft (201 n⋅m) of torque.the metroproject quattro is able to travel 62 miles (100 km) at up to 62 mph (100 km/h) on one charge of its lithium-ion batteries, which reduces fuel consumption by up to 15%.both power sources are available to use simultaneously, with the driver then benefiting from macpherson strut front and rear four-link suspension configuration, electromechanical speed-sensitive power steering with a low energy draw, audi magnetic ride adaptive damping technology, and 0 to 100 km/h (0 to 62 mph) in 7.8 seconds.the vehicle was designed by audi ag project designer in exterior design jürgen löffler, who also presented the design during the car's hong kong debut.the vehicle's 0 to 100 km/h (0 to 62 mph) acceleration is 7.9 seconds and average co2 emissions are given as 92g/km.the vehicle's electric-only range is 50 km (31.07 mi).the vehicle was unveiled at the 2008 paris motor show.the car is aimed mostly at young, affluent urban buyers.se is the base specification, while sport and s line models also have sport seats, sports suspension and larger wheels, amongst other features.1.4-litre tfsi (122 ps (90 kw; 120 hp)) was sold as the 30 tfsi in china.the production version of the a1 quattro was tested by autocar magazine on mira's wet handling track alongside a nissan gt-r; the a1 recorded lap time over five seconds faster than the gt-r. autocar called the test a '...giant-killing result'.the a1 is based on the volkswagen group pq25 platform, the same platform used in the seat ibiza mk4 and the vw polo mk5, and in its development audi has collaborated with seat.as of 23 june 2011, the 100,000th a1 was produced at audi brussels plant.a version of 2011 audi a1 painted by damien hirst was sold for £350,000.a fully charged 12 kwh lithium-ion battery gives a maximum range of 50 km (31 mi), after which a 254 cc wankel engine is used to power a 15 kw (20 ps; 20 bhp) generator with a 12 l (2.6 imp gal; 3.2 us gal) fuel tank.this is estimated to provide an additional range of 124 mi (200 km).the company claims the car weighs 1,190 kg (2,624 lb), can reach 62 mph (100 km/h) in 10.2 seconds and a maximum speed of 80 mph (129 km/h).the vehicle was unveiled at the 2010 geneva motor show, followed by the 2012 taipei motor show.it was reported that, according to the director of e-mobility and sustainability strategy at audi of america, the a1 e-tron had never been scheduled for production.in march 2013, at the new york auto show, audi announced it will be expanding the testing of its a1 e-tron outside of munich to other regions of germany.production of the a1 e-tron was reported to be cancelled.it included 18-inch 'polygon' design alloy wheels, exterior styling package (front spoiler, double-blade roof spoiler, side skirts, rear diffuser in gloss black, stainless steel tailpipe trims), roof line, shoulder line with 'audi sport' lettering, number '1' on the bonnet and doors, boot lid, front spoiler lip, side skirts, wheel arch; surrounds and double-blade roof spoiler, rear sills with audi rings, centre console trim, door handles, floor mats, rear-view mirror trim (not available with auto-dimming mirror), air vent sleeves in high gloss white. | audi a1 | manufacturer | audi <tsp> audi | foundedby | august horch <tsp> audi | subsidiary | ducati <tsp> audi | division | audi e-tron <tsp> audi | subsidiary | quattro gmbh | the audi a1 (internally designated typ 8x) is a supermini car launched by audi at the 2010 geneva motor show.both power sources are available to use simultaneously, with the driver then benefiting from macpherson strut front and rear four-link suspension configuration, electromechanical speed-sensitive power steering with a low energy draw, audi magnetic ride adaptive damping technology, and 0 to 100 km/h (0 to 62 mph) in 7.8 seconds.the vehicle was designed by audi ag project designer in exterior design jürgen löffler, who also presented the design during the car's hong kong debut.the a1 is based on the volkswagen group pq25 platform, the same platform used in the seat ibiza mk4 and the vw polo mk5, and in its development audi has collaborated with seat.as of 23 june 2011, the 100,000th a1 was produced at audi brussels plant.a version of 2011 audi a1 painted by damien hirst was sold for £350,000.it was reported that, according to the director of e-mobility and sustainability strategy at audi of america, the a1 e-tron had never been scheduled for production.in march 2013, at the new york auto show, audi announced it will be expanding the testing of its a1 e-tron outside of munich to other regions of germany.production of the a1 e-tron was reported to be cancelled.it included 18-inch 'polygon' design alloy wheels, exterior styling package (front spoiler, double-blade roof spoiler, side skirts, rear diffuser in gloss black, stainless steel tailpipe trims), roof line, shoulder line with 'audi sport' lettering, number '1' on the bonnet and doors, boot lid, front spoiler lip, side skirts, wheel arch; surrounds and double-blade roof spoiler, rear sills with audi rings, centre console trim, door handles, floor mats, rear-view mirror trim (not available with auto-dimming mirror), air vent sleeves in high gloss white. |
camilla (minor planet designation: 107 camilla) is one of the largest asteroids from the outermost edge of the asteroid belt, approximately 250 kilometers (160 miles) in diameter.it is a member of the sylvia family and located within the cybele group.it was discovered on 17 november 1868, by english astronomer norman pogson at madras observatory, india, and named after camilla, queen of the volsci in roman mythology.the x-type asteroid is a rare trinary asteroid with two minor-planet moons discovered in 2001 and 2016, respectively.it is elongated in shape and has a short rotation period of 4.8 hours.a large number of rotational lightcurves of have been obtained from photometric observations since the 1980s.best rated results gave a short rotation period of 4.844 hours with a brightness amplitude between 0.32 and 0.53 magnitude.lightcurve analysis indicates that camilla's pole most likely points towards ecliptic coordinates (β, λ) = (+51°, 72°) with a 10° uncertainty, which gives it an axial tilt of 29°.follow-up modeling of photometric data gave similar results.according to the space-based surveys carried out by the japanese akari satellite, the infrared astronomical satellite iras and the neowise mission of nasa's wide-field infrared survey explorer, as well as observations by the keck observatory and photometric modeling, camilla measures between 185 and 247 kilometers in diameter and its surface has an albedo between 0.160 and 0.294.it has been designated s/2001 (107) 1 but has not yet received an official name.later observations in september 2005 with the very large telescope (vlt) allowed the determination of an orbit.apart from data in infobox, the inclination was found to be 3 ± 1° with respect to an axis pointing towards (β, λ) = (+55°, 75°).given the ~10° uncertainty in the actual rotational axis of camilla, one can say that the orbit's inclination is less than 10°.the satellite is estimated to measure about 11 km in diameter.assuming a similar density to the primary, this would give it an approximate mass of ~1.5×1015 kg.it has a similar colour to the primary.it has the provisional designation s/2016 (107) 1.observations were taken between 29 may 2015 and 30 july 2016, using the vlt-sphere, the principal instrument attached to the 8-meter 'melipal' (ut3) unit of the vlt.on 3 out of 5 observation sessions, the new satellite could be detected.the body's orbit has a semi-major axis of 340 kilometers.107 camilla and s/2001 (107) 1, orbit data website maintained by f. marchis.includes orbit diagrams.107 camilla at astdys-2, asteroids—dynamic site ephemeris · observation prediction · orbital info · proper elements · observational info 107 camilla at the jpl small-body database | 107 camilla | discoverer | n r pogson <tsp> n r pogson | deathplace | chennai <tsp> n r pogson | birthplace | nottingham <tsp> 107 camilla | discovered | 2001-03-01 <tsp> n r pogson | nationality | england | it was discovered on 17 november 1868, by english astronomer norman pogson at madras observatory, india, and named after camilla, queen of the volsci in roman mythology. |
marcin 'abradab' marten (born 12 november 1978 in katowice) is a polish rapper and music producer.marten is a founding member of polish hip-hop group kaliber 44 and, since 2002, a solo artist.he is a member of polish society of the phonographic industry (związek producentów audio video, zpav).marten is a winner of two fryderyk awards.in 2011, machina magazine placed marten at no.17 on the list of 30 best polish rappers.he has also collaborated with artists like piotr banach, bosski roman, maciej maleńczuk, wojciech waglewski, grubson, l.u.c and o.s.t.r.the group was joined by piotr łuszcz performing under pseudonym mag magik i.in 1995, kaliber 44 was signed to s. p. records, and a year later their debut album księga tajemnicza.prolog was released.in 1998, after the group recorded its second album w 63 minuty dookoła świata, piotr 'magik' łuszcz left the band and formed paktofonika.kaliber 44's third album 3:44 was released in 2000.on 6 june 2004, he released his first solo album czerwony album through s. p. records.the album charted at no.21 on olis.the album featured a popular song titled 'rapowe ziarno 2 (szyderap)', for which a music video was released.the album won fryderyk award in the 'album of the year - hip-hop/r&b' category, while 'rapowe ziarno 2 (szyderap)' received a nomination in the 'video of the year' category.abradab's second album emisja spalin was released on 1 december 2005 and featured guest appearances by rapper numer raz and abradab's brother joka.the album peak at no.38 on olis.emisja spalin was followed by ostatni poziom kontroli, which was released on 3 october 2008 and featured grubson, reggae singer marika and igs.the album peaked at no.42 on olis.both albums received nominations for fryderyk award.on 4 october 2010, the fourth solo record by abradab was released.the album, titled abradabing and produced by rapper o.s.t.r., received a fryderyk award for hip-hop/r&b album of the year.marten's fifth studio album, extravertik, was released on 21 april 2012 through abradab's record label inna-my-twórnia. | abradab | associatedband/associatedmusicalartist | magik rapper <tsp> abradab | associatedband/associatedmusicalartist | kaliber 44 <tsp> abradab | origin | katowice <tsp> abradab | origin | poland <tsp> abradab | birthdate | 1978-11-12 | marcin 'abradab' marten (born 12 november 1978 in katowice) is a polish rapper and music producer. |
marcin 'abradab' marten (born 12 november 1978 in katowice) is a polish rapper and music producer.marten is a founding member of polish hip-hop group kaliber 44 and, since 2002, a solo artist.he is a member of polish society of the phonographic industry (związek producentów audio video, zpav).marten is a winner of two fryderyk awards.in 2011, machina magazine placed marten at no.17 on the list of 30 best polish rappers.he has also collaborated with artists like piotr banach, bosski roman, maciej maleńczuk, wojciech waglewski, grubson, l.u.c and o.s.t.r.the group was joined by piotr łuszcz performing under pseudonym mag magik i.in 1995, kaliber 44 was signed to s. p. records, and a year later their debut album księga tajemnicza.prolog was released.in 1998, after the group recorded its second album w 63 minuty dookoła świata, piotr 'magik' łuszcz left the band and formed paktofonika.kaliber 44's third album 3:44 was released in 2000.on 6 june 2004, he released his first solo album czerwony album through s. p. records.the album charted at no.21 on olis.the album featured a popular song titled 'rapowe ziarno 2 (szyderap)', for which a music video was released.the album won fryderyk award in the 'album of the year - hip-hop/r&b' category, while 'rapowe ziarno 2 (szyderap)' received a nomination in the 'video of the year' category.abradab's second album emisja spalin was released on 1 december 2005 and featured guest appearances by rapper numer raz and abradab's brother joka.the album peak at no.38 on olis.emisja spalin was followed by ostatni poziom kontroli, which was released on 3 october 2008 and featured grubson, reggae singer marika and igs.the album peaked at no.42 on olis.both albums received nominations for fryderyk award.on 4 october 2010, the fourth solo record by abradab was released.the album, titled abradabing and produced by rapper o.s.t.r., received a fryderyk award for hip-hop/r&b album of the year.marten's fifth studio album, extravertik, was released on 21 april 2012 through abradab's record label inna-my-twórnia. | abradab | associatedband/associatedmusicalartist | magik rapper <tsp> abradab | associatedband/associatedmusicalartist | kaliber 44 <tsp> abradab | origin | katowice <tsp> abradab | origin | poland <tsp> abradab | birthdate | 1978-11-12 | marcin 'abradab' marten (born 12 november 1978 in katowice) is a polish rapper and music producer. |
marcin 'abradab' marten (born 12 november 1978 in katowice) is a polish rapper and music producer.marten is a founding member of polish hip-hop group kaliber 44 and, since 2002, a solo artist.he is a member of polish society of the phonographic industry (związek producentów audio video, zpav).marten is a winner of two fryderyk awards.in 2011, machina magazine placed marten at no.17 on the list of 30 best polish rappers.he has also collaborated with artists like piotr banach, bosski roman, maciej maleńczuk, wojciech waglewski, grubson, l.u.c and o.s.t.r.the group was joined by piotr łuszcz performing under pseudonym mag magik i.in 1995, kaliber 44 was signed to s. p. records, and a year later their debut album księga tajemnicza.prolog was released.in 1998, after the group recorded its second album w 63 minuty dookoła świata, piotr 'magik' łuszcz left the band and formed paktofonika.kaliber 44's third album 3:44 was released in 2000.on 6 june 2004, he released his first solo album czerwony album through s. p. records.the album charted at no.21 on olis.the album featured a popular song titled 'rapowe ziarno 2 (szyderap)', for which a music video was released.the album won fryderyk award in the 'album of the year - hip-hop/r&b' category, while 'rapowe ziarno 2 (szyderap)' received a nomination in the 'video of the year' category.abradab's second album emisja spalin was released on 1 december 2005 and featured guest appearances by rapper numer raz and abradab's brother joka.the album peak at no.38 on olis.emisja spalin was followed by ostatni poziom kontroli, which was released on 3 october 2008 and featured grubson, reggae singer marika and igs.the album peaked at no.42 on olis.both albums received nominations for fryderyk award.on 4 october 2010, the fourth solo record by abradab was released.the album, titled abradabing and produced by rapper o.s.t.r., received a fryderyk award for hip-hop/r&b album of the year.marten's fifth studio album, extravertik, was released on 21 april 2012 through abradab's record label inna-my-twórnia. | abradab | genre | hip hop music <tsp> hip hop music | musicsubgenre | gangsta rap <tsp> hip hop music | stylisticorigin | funk <tsp> hip hop music | derivative | drum and bass <tsp> hip hop music | stylisticorigin | disco | marcin 'abradab' marten (born 12 november 1978 in katowice) is a polish rapper and music producer.marten is a founding member of polish hip-hop group kaliber 44 and, since 2002, a solo artist.the album featured a popular song titled 'rapowe ziarno 2 (szyderap)', for which a music video was released.the album won fryderyk award in the 'album of the year - hip-hop/r&b' category, while 'rapowe ziarno 2 (szyderap)' received a nomination in the 'video of the year' category.abradab's second album emisja spalin was released on 1 december 2005 and featured guest appearances by rapper numer raz and abradab's brother joka.the album, titled abradabing and produced by rapper o.s.t.r., received a fryderyk award for hip-hop/r&b album of the year. |
camilla (minor planet designation: 107 camilla) is one of the largest asteroids from the outermost edge of the asteroid belt, approximately 250 kilometers (160 miles) in diameter.it is a member of the sylvia family and located within the cybele group.it was discovered on 17 november 1868, by english astronomer norman pogson at madras observatory, india, and named after camilla, queen of the volsci in roman mythology.the x-type asteroid is a rare trinary asteroid with two minor-planet moons discovered in 2001 and 2016, respectively.it is elongated in shape and has a short rotation period of 4.8 hours.a large number of rotational lightcurves of have been obtained from photometric observations since the 1980s.best rated results gave a short rotation period of 4.844 hours with a brightness amplitude between 0.32 and 0.53 magnitude.lightcurve analysis indicates that camilla's pole most likely points towards ecliptic coordinates (β, λ) = (+51°, 72°) with a 10° uncertainty, which gives it an axial tilt of 29°.follow-up modeling of photometric data gave similar results.according to the space-based surveys carried out by the japanese akari satellite, the infrared astronomical satellite iras and the neowise mission of nasa's wide-field infrared survey explorer, as well as observations by the keck observatory and photometric modeling, camilla measures between 185 and 247 kilometers in diameter and its surface has an albedo between 0.160 and 0.294.it has been designated s/2001 (107) 1 but has not yet received an official name.later observations in september 2005 with the very large telescope (vlt) allowed the determination of an orbit.apart from data in infobox, the inclination was found to be 3 ± 1° with respect to an axis pointing towards (β, λ) = (+55°, 75°).given the ~10° uncertainty in the actual rotational axis of camilla, one can say that the orbit's inclination is less than 10°.the satellite is estimated to measure about 11 km in diameter.assuming a similar density to the primary, this would give it an approximate mass of ~1.5×1015 kg.it has a similar colour to the primary.it has the provisional designation s/2016 (107) 1.observations were taken between 29 may 2015 and 30 july 2016, using the vlt-sphere, the principal instrument attached to the 8-meter 'melipal' (ut3) unit of the vlt.on 3 out of 5 observation sessions, the new satellite could be detected.the body's orbit has a semi-major axis of 340 kilometers.107 camilla and s/2001 (107) 1, orbit data website maintained by f. marchis.includes orbit diagrams.107 camilla at astdys-2, asteroids—dynamic site ephemeris · observation prediction · orbital info · proper elements · observational info 107 camilla at the jpl small-body database | bolivianos | befringed | heterosomati <tsp> bolivianos | gilgie | minimum | no related information |
camilla (minor planet designation: 107 camilla) is one of the largest asteroids from the outermost edge of the asteroid belt, approximately 250 kilometers (160 miles) in diameter.it is a member of the sylvia family and located within the cybele group.it was discovered on 17 november 1868, by english astronomer norman pogson at madras observatory, india, and named after camilla, queen of the volsci in roman mythology.the x-type asteroid is a rare trinary asteroid with two minor-planet moons discovered in 2001 and 2016, respectively.it is elongated in shape and has a short rotation period of 4.8 hours.a large number of rotational lightcurves of have been obtained from photometric observations since the 1980s.best rated results gave a short rotation period of 4.844 hours with a brightness amplitude between 0.32 and 0.53 magnitude.lightcurve analysis indicates that camilla's pole most likely points towards ecliptic coordinates (β, λ) = (+51°, 72°) with a 10° uncertainty, which gives it an axial tilt of 29°.follow-up modeling of photometric data gave similar results.according to the space-based surveys carried out by the japanese akari satellite, the infrared astronomical satellite iras and the neowise mission of nasa's wide-field infrared survey explorer, as well as observations by the keck observatory and photometric modeling, camilla measures between 185 and 247 kilometers in diameter and its surface has an albedo between 0.160 and 0.294.it has been designated s/2001 (107) 1 but has not yet received an official name.later observations in september 2005 with the very large telescope (vlt) allowed the determination of an orbit.apart from data in infobox, the inclination was found to be 3 ± 1° with respect to an axis pointing towards (β, λ) = (+55°, 75°).given the ~10° uncertainty in the actual rotational axis of camilla, one can say that the orbit's inclination is less than 10°.the satellite is estimated to measure about 11 km in diameter.assuming a similar density to the primary, this would give it an approximate mass of ~1.5×1015 kg.it has a similar colour to the primary.it has the provisional designation s/2016 (107) 1.observations were taken between 29 may 2015 and 30 july 2016, using the vlt-sphere, the principal instrument attached to the 8-meter 'melipal' (ut3) unit of the vlt.on 3 out of 5 observation sessions, the new satellite could be detected.the body's orbit has a semi-major axis of 340 kilometers.107 camilla and s/2001 (107) 1, orbit data website maintained by f. marchis.includes orbit diagrams.107 camilla at astdys-2, asteroids—dynamic site ephemeris · observation prediction · orbital info · proper elements · observational info 107 camilla at the jpl small-body database | 107 camilla | discoverer | n r pogson <tsp> n r pogson | deathplace | chennai <tsp> n r pogson | birthplace | nottingham <tsp> 107 camilla | discovered | 2001-03-01 <tsp> n r pogson | nationality | england | it was discovered on 17 november 1868, by english astronomer norman pogson at madras observatory, india, and named after camilla, queen of the volsci in roman mythology. |
marcin 'abradab' marten (born 12 november 1978 in katowice) is a polish rapper and music producer.marten is a founding member of polish hip-hop group kaliber 44 and, since 2002, a solo artist.he is a member of polish society of the phonographic industry (związek producentów audio video, zpav).marten is a winner of two fryderyk awards.in 2011, machina magazine placed marten at no.17 on the list of 30 best polish rappers.he has also collaborated with artists like piotr banach, bosski roman, maciej maleńczuk, wojciech waglewski, grubson, l.u.c and o.s.t.r.the group was joined by piotr łuszcz performing under pseudonym mag magik i.in 1995, kaliber 44 was signed to s. p. records, and a year later their debut album księga tajemnicza.prolog was released.in 1998, after the group recorded its second album w 63 minuty dookoła świata, piotr 'magik' łuszcz left the band and formed paktofonika.kaliber 44's third album 3:44 was released in 2000.on 6 june 2004, he released his first solo album czerwony album through s. p. records.the album charted at no.21 on olis.the album featured a popular song titled 'rapowe ziarno 2 (szyderap)', for which a music video was released.the album won fryderyk award in the 'album of the year - hip-hop/r&b' category, while 'rapowe ziarno 2 (szyderap)' received a nomination in the 'video of the year' category.abradab's second album emisja spalin was released on 1 december 2005 and featured guest appearances by rapper numer raz and abradab's brother joka.the album peak at no.38 on olis.emisja spalin was followed by ostatni poziom kontroli, which was released on 3 october 2008 and featured grubson, reggae singer marika and igs.the album peaked at no.42 on olis.both albums received nominations for fryderyk award.on 4 october 2010, the fourth solo record by abradab was released.the album, titled abradabing and produced by rapper o.s.t.r., received a fryderyk award for hip-hop/r&b album of the year.marten's fifth studio album, extravertik, was released on 21 april 2012 through abradab's record label inna-my-twórnia. | overreligiously | patagium | sulfopurpuric <tsp> overreligiously | rumbumptious | demihorse | no related information |
camilla (minor planet designation: 107 camilla) is one of the largest asteroids from the outermost edge of the asteroid belt, approximately 250 kilometers (160 miles) in diameter.it is a member of the sylvia family and located within the cybele group.it was discovered on 17 november 1868, by english astronomer norman pogson at madras observatory, india, and named after camilla, queen of the volsci in roman mythology.the x-type asteroid is a rare trinary asteroid with two minor-planet moons discovered in 2001 and 2016, respectively.it is elongated in shape and has a short rotation period of 4.8 hours.a large number of rotational lightcurves of have been obtained from photometric observations since the 1980s.best rated results gave a short rotation period of 4.844 hours with a brightness amplitude between 0.32 and 0.53 magnitude.lightcurve analysis indicates that camilla's pole most likely points towards ecliptic coordinates (β, λ) = (+51°, 72°) with a 10° uncertainty, which gives it an axial tilt of 29°.follow-up modeling of photometric data gave similar results.according to the space-based surveys carried out by the japanese akari satellite, the infrared astronomical satellite iras and the neowise mission of nasa's wide-field infrared survey explorer, as well as observations by the keck observatory and photometric modeling, camilla measures between 185 and 247 kilometers in diameter and its surface has an albedo between 0.160 and 0.294.it has been designated s/2001 (107) 1 but has not yet received an official name.later observations in september 2005 with the very large telescope (vlt) allowed the determination of an orbit.apart from data in infobox, the inclination was found to be 3 ± 1° with respect to an axis pointing towards (β, λ) = (+55°, 75°).given the ~10° uncertainty in the actual rotational axis of camilla, one can say that the orbit's inclination is less than 10°.the satellite is estimated to measure about 11 km in diameter.assuming a similar density to the primary, this would give it an approximate mass of ~1.5×1015 kg.it has a similar colour to the primary.it has the provisional designation s/2016 (107) 1.observations were taken between 29 may 2015 and 30 july 2016, using the vlt-sphere, the principal instrument attached to the 8-meter 'melipal' (ut3) unit of the vlt.on 3 out of 5 observation sessions, the new satellite could be detected.the body's orbit has a semi-major axis of 340 kilometers.107 camilla and s/2001 (107) 1, orbit data website maintained by f. marchis.includes orbit diagrams.107 camilla at astdys-2, asteroids—dynamic site ephemeris · observation prediction · orbital info · proper elements · observational info 107 camilla at the jpl small-body database | 107 camilla | discoverer | n r pogson <tsp> n r pogson | deathplace | chennai <tsp> n r pogson | birthplace | nottingham <tsp> n r pogson | nationality | england <tsp> 107 camilla | epoch | 2006-12-31 | it was discovered on 17 november 1868, by english astronomer norman pogson at madras observatory, india, and named after camilla, queen of the volsci in roman mythology. |
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