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antares (), known during early development as taurus ii, is an expendable launch system developed by orbital sciences corporation (now part of northrop grumman) and the pivdenne design bureau to launch the cygnus spacecraft to the international space station as part of nasa's cots and crs programs.able to launch payloads heavier than 8,000 kg (18,000 lb) into low earth orbit, antares is currently the largest rocket operated by northrop grumman.antares launches from the mid-atlantic regional spaceport and made its inaugural flight on april 21, 2013.nasa awarded orbital a commercial orbital transportation services (cots) space act agreement (saa) in 2008 to demonstrate delivery of cargo to the international space station.for these cots missions orbital intends to use antares to launch its cygnus spacecraft.in addition, antares will compete for small-to-medium missions.originally designated the taurus ii, orbital sciences renamed the vehicle antares, after the star of the same name, on december 12, 2011.out of 17 total launches, antares has suffered one failure.during the fifth launch on october 28, 2014, the rocket failed catastrophically, and the vehicle and payload were destroyed.the rocket's first-stage engines were identified as the cause for the failure.a different engine was chosen for subsequent launches, and the rocket had a successful return to flight on october 17, 2016.the antares has flown two major design iterations, the 100 series and 200 series.both series have used a castor 30xl as an upper stage but have differed on the first stage.the 100 series used two kerolox powered aj26 engine in the first stage and launched successfully four times.the 100 series was retired following a launch failure in 2014.the 200 series which first flew in 2016 also featured a kerolox first stage but instead used two rd-181 engine along with other minor upgrades.the 200 series future became uncertain following the russian invasion of ukraine.due to the first stage being produced in ukraine and the engines in russia, future production of the rocket was unable to be continued.as a result northrop grumman entered into an agreement with firefly aerospace to build the first stage of the antares 300 series.northrop also contracted with spacex for 3 falcon 9 launches.a commercial resupply service contract of $1.9 billion for eight flights was awarded in 2008.as of april 2012, development costs were estimated at $472 million.in june 2008, it was announced that the mid-atlantic regional spaceport, formerly part of the wallops flight facility, in virginia, would be the primary launch site for the rocket.launch pad 0a (lp-0a), previously used for the failed conestoga rocket, would be modified to handle antares.wallops allows launches which reach the international space station's orbit as effectively as those from cape canaveral, florida, while being less crowded.the first antares flight launched a cygnus mass simulator.on december 10, 2009, alliant techsystems inc. (atk) test-fired their castor 30 motor for use on the second stage of the antares rocket.in march 2010, orbital sciences and aerojet completed test firings of the aj-26 engines.on february 22, 2013, a hot fire test was successfully performed, the entire first stage being erected on the pad and held down while the engines fired for 29 seconds.as orbital had little experience with large liquid stages and lox propellant, the first stage core was designed and is manufactured in ukraine by kb pivdenne and pivdenmash and includes propellant tanks, pressurization tanks, valves, sensors, feed lines, tubing, wiring and other associated hardware.like the zenit—also manufactured by yuzhmash—the antares vehicle has a diameter of 3.9 m (150 in) with a matching 3.9 m payload fairing. | azoxazole | reinsert | rampikes <tsp> azoxazole | whores | callant | no related information |
(66063) 1998 ro1 is a stony near-earth object of the aten group on a highly-eccentric orbit.the synchronous binary system measures approximately 800 meters (0.50 miles) in diameter.it was discovered by astronomers of the lincoln near-earth asteroid research at the lincoln laboratory's experimental test site near socorro, new mexico, on 14 september 1998.its minor-planet moon, provisionally designated s/2001 (66063) 1, was discovered in september 2003.it has an orbital period of 14.53 hours and measures approximately 48% of its primary, or 380 meters.it is one of seven known aten binaries as of 2017.it has an orbital period of 360.29 days (0.99 years) and makes close approaches to earth.but 1998 ro1 makes closer approaches to other inner planets, especially mars.its closest approach to a planet between 1950–2200 was to mars, as it passed 0.00898 au (1,343,000 km) from mars on 18 march 1964, and will pass 0.0054 au (810,000 km) from mars on 12 october 2065.this moon was discovered from lightcurve observations going from 13 to 28 september 2013, and was confirmed by radar observations from the arecibo observatory one year later.it is in a very close orbit to 1998 ro1, with a semi-major axis of 800 m (2,600 ft) and an eccentricity of 0.06, giving it a periapsis of 752 m (2,467 ft) and an apoapsis of 848 m (2,782 ft).s/2001 (66063) 1 takes 14.54 hours to complete one orbit around 1998 ro1.from the surface of 1998 ro1, s/2001 (66063) 1 would have an apparent diameter of roughly 41°.for comparison, the sun appears to be 0.5° from earth.the secondary orbits its primary in a manner very similar to the adjunct image, where the red cross is the center of mass.as of 2018, it has not been named. | umping | axmaster | convoker <tsp> umping | hero | wounder | no related information |
san sebastián de los reyes (colloquially called 'sanse') is a municipality in the community of madrid, spain.founded in 1492, it is located 20 kilometres (12 mi) north of madrid.this line buses, along with urban ones, are the following: urban line 2: alcobendas - la moraleja (by paseo de alcobendas) (interbús) urban line 4: sports center - moscatelares (interbús) urban line 5: san sebastián de los reyes - alcobendas - el soto de la moraleja (interbús) urban line 7: alcobendas train station - polígonos - alcobendas train station (interbús) urban line 8: alcobendas (train station) - alcobendas (arroyo de la vega) (interbús) 151: madrid (plaza de castilla) - alcobendas (interbús) 152c: madrid (plaza de castilla) - san sebastián de los reyes (dehesa vieja) (interbús) 153: madrid (plaza de castilla) - alcobendas - rosa luxemburgo (interbús) 154: madrid (chamartín) - san sebastián de los reyes (circular by fuencarral) (interbús) 154c: madrid (plaza de castilla) - san sebastián de los reyes (quiñones avenue) (interbús) 156: madrid (plaza de castilla) - san sebastián de los reyes (polígono industrial moscatelares) (interbús) 158: madrid (pinar de chamartín) - alcobendas-san sebastián de los reyes (tempranales) (interbús) 161: madrid (plaza de castilla) - fuente del fresno urbanization (interbús) 166: san sebastián de los reyes-urbanización valdelagua (interbús) 180: alcobendas - algete (interbús) 171: madrid (plaza de castilla) - santo domingo urbanization (alsa) 191: madrid (plaza de castilla) - buitrago del lozoya (alsa) 193: madrid (plaza de castilla) - el vellón (alsa) 194: madrid (plaza de castilla) - rascafría (alsa) 195: madrid (plaza de castilla) - braojos (alsa) 196: madrid (plaza de castilla) - la acebeda (alsa) 197: madrid (plaza de castilla) - uceda (alsa) 210: san sebastián de los reyes - paracuellos de jarama (alsa) 827: madrid (canillejas) - tres cantos (doroteo casado montes) 827a: alcobendas - san sebastián de los reyes - university (doroteo casado montes) night bus line 102: madrid (plaza de castilla) - san sebastián de los reyes (interbús) night bus line 103: madrid (plaza de castilla) - algete (interbús) night bus line 104: madrid (plaza de castilla) - san agustín del guadalix (alsa)san sebastián de los reyes also shares a railway station with the neighboring municipality of alcobendas.from this station you can go to the city of madrid and to many other places such as getafe or parla.game developer mercurysteam is based here.a women's soccer team, madrid cff, plays in the primera división (women) but it has not gone well for them there.they are from madrid, but their stadium is in san sebastián. | san sebastián de los reyes | ispartof | community of madrid <tsp> adolfo suárez madrid–barajas airport | elevationabovethesealevel in metres | 6100 <tsp> adolfo suárez madrid–barajas airport | runwaylength | 35000 <tsp> adolfo suárez madrid–barajas airport | location | san sebastián de los reyes <tsp> san sebastián de los reyes | country | spain | san sebastián de los reyes (colloquially called 'sanse') is a municipality in the community of madrid, spain.this line buses, along with urban ones, are the following: urban line 2: alcobendas - la moraleja (by paseo de alcobendas) (interbús) urban line 4: sports center - moscatelares (interbús) urban line 5: san sebastián de los reyes - alcobendas - el soto de la moraleja (interbús) urban line 7: alcobendas train station - polígonos - alcobendas train station (interbús) urban line 8: alcobendas (train station) - alcobendas (arroyo de la vega) (interbús) 151: madrid (plaza de castilla) - alcobendas (interbús) 152c: madrid (plaza de castilla) - san sebastián de los reyes (dehesa vieja) (interbús) 153: madrid (plaza de castilla) - alcobendas - rosa luxemburgo (interbús) 154: madrid (chamartín) - san sebastián de los reyes (circular by fuencarral) (interbús) 154c: madrid (plaza de castilla) - san sebastián de los reyes (quiñones avenue) (interbús) 156: madrid (plaza de castilla) - san sebastián de los reyes (polígono industrial moscatelares) (interbús) 158: madrid (pinar de chamartín) - alcobendas-san sebastián de los reyes (tempranales) (interbús) 161: madrid (plaza de castilla) - fuente del fresno urbanization (interbús) 166: san sebastián de los reyes-urbanización valdelagua (interbús) 180: alcobendas - algete (interbús) 171: madrid (plaza de castilla) - santo domingo urbanization (alsa) 191: madrid (plaza de castilla) - buitrago del lozoya (alsa) 193: madrid (plaza de castilla) - el vellón (alsa) 194: madrid (plaza de castilla) - rascafría (alsa) 195: madrid (plaza de castilla) - braojos (alsa) 196: madrid (plaza de castilla) - la acebeda (alsa) 197: madrid (plaza de castilla) - uceda (alsa) 210: san sebastián de los reyes - paracuellos de jarama (alsa) 827: madrid (canillejas) - tres cantos (doroteo casado montes) 827a: alcobendas - san sebastián de los reyes - university (doroteo casado montes) night bus line 102: madrid (plaza de castilla) - san sebastián de los reyes (interbús) night bus line 103: madrid (plaza de castilla) - algete (interbús) night bus line 104: madrid (plaza de castilla) - san agustín del guadalix (alsa)san sebastián de los reyes also shares a railway station with the neighboring municipality of alcobendas.they are from madrid, but their stadium is in san sebastián. |
antares (), known during early development as taurus ii, is an expendable launch system developed by orbital sciences corporation (now part of northrop grumman) and the pivdenne design bureau to launch the cygnus spacecraft to the international space station as part of nasa's cots and crs programs.able to launch payloads heavier than 8,000 kg (18,000 lb) into low earth orbit, antares is currently the largest rocket operated by northrop grumman.antares launches from the mid-atlantic regional spaceport and made its inaugural flight on april 21, 2013.nasa awarded orbital a commercial orbital transportation services (cots) space act agreement (saa) in 2008 to demonstrate delivery of cargo to the international space station.for these cots missions orbital intends to use antares to launch its cygnus spacecraft.in addition, antares will compete for small-to-medium missions.originally designated the taurus ii, orbital sciences renamed the vehicle antares, after the star of the same name, on december 12, 2011.out of 17 total launches, antares has suffered one failure.during the fifth launch on october 28, 2014, the rocket failed catastrophically, and the vehicle and payload were destroyed.the rocket's first-stage engines were identified as the cause for the failure.a different engine was chosen for subsequent launches, and the rocket had a successful return to flight on october 17, 2016.the antares has flown two major design iterations, the 100 series and 200 series.both series have used a castor 30xl as an upper stage but have differed on the first stage.the 100 series used two kerolox powered aj26 engine in the first stage and launched successfully four times.the 100 series was retired following a launch failure in 2014.the 200 series which first flew in 2016 also featured a kerolox first stage but instead used two rd-181 engine along with other minor upgrades.the 200 series future became uncertain following the russian invasion of ukraine.due to the first stage being produced in ukraine and the engines in russia, future production of the rocket was unable to be continued.as a result northrop grumman entered into an agreement with firefly aerospace to build the first stage of the antares 300 series.northrop also contracted with spacex for 3 falcon 9 launches.a commercial resupply service contract of $1.9 billion for eight flights was awarded in 2008.as of april 2012, development costs were estimated at $472 million.in june 2008, it was announced that the mid-atlantic regional spaceport, formerly part of the wallops flight facility, in virginia, would be the primary launch site for the rocket.launch pad 0a (lp-0a), previously used for the failed conestoga rocket, would be modified to handle antares.wallops allows launches which reach the international space station's orbit as effectively as those from cape canaveral, florida, while being less crowded.the first antares flight launched a cygnus mass simulator.on december 10, 2009, alliant techsystems inc. (atk) test-fired their castor 30 motor for use on the second stage of the antares rocket.in march 2010, orbital sciences and aerojet completed test firings of the aj-26 engines.on february 22, 2013, a hot fire test was successfully performed, the entire first stage being erected on the pad and held down while the engines fired for 29 seconds.as orbital had little experience with large liquid stages and lox propellant, the first stage core was designed and is manufactured in ukraine by kb pivdenne and pivdenmash and includes propellant tanks, pressurization tanks, valves, sensors, feed lines, tubing, wiring and other associated hardware.like the zenit—also manufactured by yuzhmash—the antares vehicle has a diameter of 3.9 m (150 in) with a matching 3.9 m payload fairing. | antares rocket | launchsite | mid-atlantic regional spaceport <tsp> antares rocket | comparable | delta ii <tsp> antares rocket | manufacturer | yuzhnoye design office <tsp> delta ii | countryorigin | united states <tsp> antares rocket | launchsite | mid-atlantic regional spaceport launch pad 0 | antares (), known during early development as taurus ii, is an expendable launch system developed by orbital sciences corporation (now part of northrop grumman) and the pivdenne design bureau to launch the cygnus spacecraft to the international space station as part of nasa's cots and crs programs.able to launch payloads heavier than 8,000 kg (18,000 lb) into low earth orbit, antares is currently the largest rocket operated by northrop grumman.antares launches from the mid-atlantic regional spaceport and made its inaugural flight on april 21, 2013.nasa awarded orbital a commercial orbital transportation services (cots) space act agreement (saa) in 2008 to demonstrate delivery of cargo to the international space station.for these cots missions orbital intends to use antares to launch its cygnus spacecraft.originally designated the taurus ii, orbital sciences renamed the vehicle antares, after the star of the same name, on december 12, 2011.out of 17 total launches, antares has suffered one failure.the antares has flown two major design iterations, the 100 series and 200 series.launch pad 0a (lp-0a), previously used for the failed conestoga rocket, would be modified to handle antares.the first antares flight launched a cygnus mass simulator.on december 10, 2009, alliant techsystems inc. (atk) test-fired their castor 30 motor for use on the second stage of the antares rocket. |
(66063) 1998 ro1 is a stony near-earth object of the aten group on a highly-eccentric orbit.the synchronous binary system measures approximately 800 meters (0.50 miles) in diameter.it was discovered by astronomers of the lincoln near-earth asteroid research at the lincoln laboratory's experimental test site near socorro, new mexico, on 14 september 1998.its minor-planet moon, provisionally designated s/2001 (66063) 1, was discovered in september 2003.it has an orbital period of 14.53 hours and measures approximately 48% of its primary, or 380 meters.it is one of seven known aten binaries as of 2017.it has an orbital period of 360.29 days (0.99 years) and makes close approaches to earth.but 1998 ro1 makes closer approaches to other inner planets, especially mars.its closest approach to a planet between 1950–2200 was to mars, as it passed 0.00898 au (1,343,000 km) from mars on 18 march 1964, and will pass 0.0054 au (810,000 km) from mars on 12 october 2065.this moon was discovered from lightcurve observations going from 13 to 28 september 2013, and was confirmed by radar observations from the arecibo observatory one year later.it is in a very close orbit to 1998 ro1, with a semi-major axis of 800 m (2,600 ft) and an eccentricity of 0.06, giving it a periapsis of 752 m (2,467 ft) and an apoapsis of 848 m (2,782 ft).s/2001 (66063) 1 takes 14.54 hours to complete one orbit around 1998 ro1.from the surface of 1998 ro1, s/2001 (66063) 1 would have an apparent diameter of roughly 41°.for comparison, the sun appears to be 0.5° from earth.the secondary orbits its primary in a manner very similar to the adjunct image, where the red cross is the center of mass.as of 2018, it has not been named. | capriccios | championing | pappy | no related information |
san sebastián de los reyes (colloquially called 'sanse') is a municipality in the community of madrid, spain.founded in 1492, it is located 20 kilometres (12 mi) north of madrid.this line buses, along with urban ones, are the following: urban line 2: alcobendas - la moraleja (by paseo de alcobendas) (interbús) urban line 4: sports center - moscatelares (interbús) urban line 5: san sebastián de los reyes - alcobendas - el soto de la moraleja (interbús) urban line 7: alcobendas train station - polígonos - alcobendas train station (interbús) urban line 8: alcobendas (train station) - alcobendas (arroyo de la vega) (interbús) 151: madrid (plaza de castilla) - alcobendas (interbús) 152c: madrid (plaza de castilla) - san sebastián de los reyes (dehesa vieja) (interbús) 153: madrid (plaza de castilla) - alcobendas - rosa luxemburgo (interbús) 154: madrid (chamartín) - san sebastián de los reyes (circular by fuencarral) (interbús) 154c: madrid (plaza de castilla) - san sebastián de los reyes (quiñones avenue) (interbús) 156: madrid (plaza de castilla) - san sebastián de los reyes (polígono industrial moscatelares) (interbús) 158: madrid (pinar de chamartín) - alcobendas-san sebastián de los reyes (tempranales) (interbús) 161: madrid (plaza de castilla) - fuente del fresno urbanization (interbús) 166: san sebastián de los reyes-urbanización valdelagua (interbús) 180: alcobendas - algete (interbús) 171: madrid (plaza de castilla) - santo domingo urbanization (alsa) 191: madrid (plaza de castilla) - buitrago del lozoya (alsa) 193: madrid (plaza de castilla) - el vellón (alsa) 194: madrid (plaza de castilla) - rascafría (alsa) 195: madrid (plaza de castilla) - braojos (alsa) 196: madrid (plaza de castilla) - la acebeda (alsa) 197: madrid (plaza de castilla) - uceda (alsa) 210: san sebastián de los reyes - paracuellos de jarama (alsa) 827: madrid (canillejas) - tres cantos (doroteo casado montes) 827a: alcobendas - san sebastián de los reyes - university (doroteo casado montes) night bus line 102: madrid (plaza de castilla) - san sebastián de los reyes (interbús) night bus line 103: madrid (plaza de castilla) - algete (interbús) night bus line 104: madrid (plaza de castilla) - san agustín del guadalix (alsa)san sebastián de los reyes also shares a railway station with the neighboring municipality of alcobendas.from this station you can go to the city of madrid and to many other places such as getafe or parla.game developer mercurysteam is based here.a women's soccer team, madrid cff, plays in the primera división (women) but it has not gone well for them there.they are from madrid, but their stadium is in san sebastián. | san sebastián de los reyes | ispartof | community of madrid <tsp> adolfo suárez madrid–barajas airport | elevationabovethesealevel in metres | 6100 <tsp> adolfo suárez madrid–barajas airport | runwaylength | 35000 <tsp> adolfo suárez madrid–barajas airport | location | san sebastián de los reyes <tsp> san sebastián de los reyes | country | spain | san sebastián de los reyes (colloquially called 'sanse') is a municipality in the community of madrid, spain.this line buses, along with urban ones, are the following: urban line 2: alcobendas - la moraleja (by paseo de alcobendas) (interbús) urban line 4: sports center - moscatelares (interbús) urban line 5: san sebastián de los reyes - alcobendas - el soto de la moraleja (interbús) urban line 7: alcobendas train station - polígonos - alcobendas train station (interbús) urban line 8: alcobendas (train station) - alcobendas (arroyo de la vega) (interbús) 151: madrid (plaza de castilla) - alcobendas (interbús) 152c: madrid (plaza de castilla) - san sebastián de los reyes (dehesa vieja) (interbús) 153: madrid (plaza de castilla) - alcobendas - rosa luxemburgo (interbús) 154: madrid (chamartín) - san sebastián de los reyes (circular by fuencarral) (interbús) 154c: madrid (plaza de castilla) - san sebastián de los reyes (quiñones avenue) (interbús) 156: madrid (plaza de castilla) - san sebastián de los reyes (polígono industrial moscatelares) (interbús) 158: madrid (pinar de chamartín) - alcobendas-san sebastián de los reyes (tempranales) (interbús) 161: madrid (plaza de castilla) - fuente del fresno urbanization (interbús) 166: san sebastián de los reyes-urbanización valdelagua (interbús) 180: alcobendas - algete (interbús) 171: madrid (plaza de castilla) - santo domingo urbanization (alsa) 191: madrid (plaza de castilla) - buitrago del lozoya (alsa) 193: madrid (plaza de castilla) - el vellón (alsa) 194: madrid (plaza de castilla) - rascafría (alsa) 195: madrid (plaza de castilla) - braojos (alsa) 196: madrid (plaza de castilla) - la acebeda (alsa) 197: madrid (plaza de castilla) - uceda (alsa) 210: san sebastián de los reyes - paracuellos de jarama (alsa) 827: madrid (canillejas) - tres cantos (doroteo casado montes) 827a: alcobendas - san sebastián de los reyes - university (doroteo casado montes) night bus line 102: madrid (plaza de castilla) - san sebastián de los reyes (interbús) night bus line 103: madrid (plaza de castilla) - algete (interbús) night bus line 104: madrid (plaza de castilla) - san agustín del guadalix (alsa)san sebastián de los reyes also shares a railway station with the neighboring municipality of alcobendas.they are from madrid, but their stadium is in san sebastián. |
(66063) 1998 ro1 is a stony near-earth object of the aten group on a highly-eccentric orbit.the synchronous binary system measures approximately 800 meters (0.50 miles) in diameter.it was discovered by astronomers of the lincoln near-earth asteroid research at the lincoln laboratory's experimental test site near socorro, new mexico, on 14 september 1998.its minor-planet moon, provisionally designated s/2001 (66063) 1, was discovered in september 2003.it has an orbital period of 14.53 hours and measures approximately 48% of its primary, or 380 meters.it is one of seven known aten binaries as of 2017.it has an orbital period of 360.29 days (0.99 years) and makes close approaches to earth.but 1998 ro1 makes closer approaches to other inner planets, especially mars.its closest approach to a planet between 1950–2200 was to mars, as it passed 0.00898 au (1,343,000 km) from mars on 18 march 1964, and will pass 0.0054 au (810,000 km) from mars on 12 october 2065.this moon was discovered from lightcurve observations going from 13 to 28 september 2013, and was confirmed by radar observations from the arecibo observatory one year later.it is in a very close orbit to 1998 ro1, with a semi-major axis of 800 m (2,600 ft) and an eccentricity of 0.06, giving it a periapsis of 752 m (2,467 ft) and an apoapsis of 848 m (2,782 ft).s/2001 (66063) 1 takes 14.54 hours to complete one orbit around 1998 ro1.from the surface of 1998 ro1, s/2001 (66063) 1 would have an apparent diameter of roughly 41°.for comparison, the sun appears to be 0.5° from earth.the secondary orbits its primary in a manner very similar to the adjunct image, where the red cross is the center of mass.as of 2018, it has not been named. | 66063 1998 ro1 | formername | 1999 sn5 <tsp> 66063 1998 ro1 | orbitalperiod | 36029 days <tsp> 66063 1998 ro1 | periapsis | 414984000000 <tsp> 66063 1998 ro1 | epoch | 2013-11-04 <tsp> 66063 1998 ro1 | escapevelocity | 00999 kilometreperseconds | no related information |
san sebastián de los reyes (colloquially called 'sanse') is a municipality in the community of madrid, spain.founded in 1492, it is located 20 kilometres (12 mi) north of madrid.this line buses, along with urban ones, are the following: urban line 2: alcobendas - la moraleja (by paseo de alcobendas) (interbús) urban line 4: sports center - moscatelares (interbús) urban line 5: san sebastián de los reyes - alcobendas - el soto de la moraleja (interbús) urban line 7: alcobendas train station - polígonos - alcobendas train station (interbús) urban line 8: alcobendas (train station) - alcobendas (arroyo de la vega) (interbús) 151: madrid (plaza de castilla) - alcobendas (interbús) 152c: madrid (plaza de castilla) - san sebastián de los reyes (dehesa vieja) (interbús) 153: madrid (plaza de castilla) - alcobendas - rosa luxemburgo (interbús) 154: madrid (chamartín) - san sebastián de los reyes (circular by fuencarral) (interbús) 154c: madrid (plaza de castilla) - san sebastián de los reyes (quiñones avenue) (interbús) 156: madrid (plaza de castilla) - san sebastián de los reyes (polígono industrial moscatelares) (interbús) 158: madrid (pinar de chamartín) - alcobendas-san sebastián de los reyes (tempranales) (interbús) 161: madrid (plaza de castilla) - fuente del fresno urbanization (interbús) 166: san sebastián de los reyes-urbanización valdelagua (interbús) 180: alcobendas - algete (interbús) 171: madrid (plaza de castilla) - santo domingo urbanization (alsa) 191: madrid (plaza de castilla) - buitrago del lozoya (alsa) 193: madrid (plaza de castilla) - el vellón (alsa) 194: madrid (plaza de castilla) - rascafría (alsa) 195: madrid (plaza de castilla) - braojos (alsa) 196: madrid (plaza de castilla) - la acebeda (alsa) 197: madrid (plaza de castilla) - uceda (alsa) 210: san sebastián de los reyes - paracuellos de jarama (alsa) 827: madrid (canillejas) - tres cantos (doroteo casado montes) 827a: alcobendas - san sebastián de los reyes - university (doroteo casado montes) night bus line 102: madrid (plaza de castilla) - san sebastián de los reyes (interbús) night bus line 103: madrid (plaza de castilla) - algete (interbús) night bus line 104: madrid (plaza de castilla) - san agustín del guadalix (alsa)san sebastián de los reyes also shares a railway station with the neighboring municipality of alcobendas.from this station you can go to the city of madrid and to many other places such as getafe or parla.game developer mercurysteam is based here.a women's soccer team, madrid cff, plays in the primera división (women) but it has not gone well for them there.they are from madrid, but their stadium is in san sebastián. | san sebastián de los reyes | ispartof | community of madrid <tsp> adolfo suárez madrid–barajas airport | elevationabovethesealevel in metres | 6100 <tsp> adolfo suárez madrid–barajas airport | runwaylength | 35000 <tsp> adolfo suárez madrid–barajas airport | location | san sebastián de los reyes <tsp> san sebastián de los reyes | country | spain | san sebastián de los reyes (colloquially called 'sanse') is a municipality in the community of madrid, spain.this line buses, along with urban ones, are the following: urban line 2: alcobendas - la moraleja (by paseo de alcobendas) (interbús) urban line 4: sports center - moscatelares (interbús) urban line 5: san sebastián de los reyes - alcobendas - el soto de la moraleja (interbús) urban line 7: alcobendas train station - polígonos - alcobendas train station (interbús) urban line 8: alcobendas (train station) - alcobendas (arroyo de la vega) (interbús) 151: madrid (plaza de castilla) - alcobendas (interbús) 152c: madrid (plaza de castilla) - san sebastián de los reyes (dehesa vieja) (interbús) 153: madrid (plaza de castilla) - alcobendas - rosa luxemburgo (interbús) 154: madrid (chamartín) - san sebastián de los reyes (circular by fuencarral) (interbús) 154c: madrid (plaza de castilla) - san sebastián de los reyes (quiñones avenue) (interbús) 156: madrid (plaza de castilla) - san sebastián de los reyes (polígono industrial moscatelares) (interbús) 158: madrid (pinar de chamartín) - alcobendas-san sebastián de los reyes (tempranales) (interbús) 161: madrid (plaza de castilla) - fuente del fresno urbanization (interbús) 166: san sebastián de los reyes-urbanización valdelagua (interbús) 180: alcobendas - algete (interbús) 171: madrid (plaza de castilla) - santo domingo urbanization (alsa) 191: madrid (plaza de castilla) - buitrago del lozoya (alsa) 193: madrid (plaza de castilla) - el vellón (alsa) 194: madrid (plaza de castilla) - rascafría (alsa) 195: madrid (plaza de castilla) - braojos (alsa) 196: madrid (plaza de castilla) - la acebeda (alsa) 197: madrid (plaza de castilla) - uceda (alsa) 210: san sebastián de los reyes - paracuellos de jarama (alsa) 827: madrid (canillejas) - tres cantos (doroteo casado montes) 827a: alcobendas - san sebastián de los reyes - university (doroteo casado montes) night bus line 102: madrid (plaza de castilla) - san sebastián de los reyes (interbús) night bus line 103: madrid (plaza de castilla) - algete (interbús) night bus line 104: madrid (plaza de castilla) - san agustín del guadalix (alsa)san sebastián de los reyes also shares a railway station with the neighboring municipality of alcobendas.they are from madrid, but their stadium is in san sebastián. |
antares (), known during early development as taurus ii, is an expendable launch system developed by orbital sciences corporation (now part of northrop grumman) and the pivdenne design bureau to launch the cygnus spacecraft to the international space station as part of nasa's cots and crs programs.able to launch payloads heavier than 8,000 kg (18,000 lb) into low earth orbit, antares is currently the largest rocket operated by northrop grumman.antares launches from the mid-atlantic regional spaceport and made its inaugural flight on april 21, 2013.nasa awarded orbital a commercial orbital transportation services (cots) space act agreement (saa) in 2008 to demonstrate delivery of cargo to the international space station.for these cots missions orbital intends to use antares to launch its cygnus spacecraft.in addition, antares will compete for small-to-medium missions.originally designated the taurus ii, orbital sciences renamed the vehicle antares, after the star of the same name, on december 12, 2011.out of 17 total launches, antares has suffered one failure.during the fifth launch on october 28, 2014, the rocket failed catastrophically, and the vehicle and payload were destroyed.the rocket's first-stage engines were identified as the cause for the failure.a different engine was chosen for subsequent launches, and the rocket had a successful return to flight on october 17, 2016.the antares has flown two major design iterations, the 100 series and 200 series.both series have used a castor 30xl as an upper stage but have differed on the first stage.the 100 series used two kerolox powered aj26 engine in the first stage and launched successfully four times.the 100 series was retired following a launch failure in 2014.the 200 series which first flew in 2016 also featured a kerolox first stage but instead used two rd-181 engine along with other minor upgrades.the 200 series future became uncertain following the russian invasion of ukraine.due to the first stage being produced in ukraine and the engines in russia, future production of the rocket was unable to be continued.as a result northrop grumman entered into an agreement with firefly aerospace to build the first stage of the antares 300 series.northrop also contracted with spacex for 3 falcon 9 launches.a commercial resupply service contract of $1.9 billion for eight flights was awarded in 2008.as of april 2012, development costs were estimated at $472 million.in june 2008, it was announced that the mid-atlantic regional spaceport, formerly part of the wallops flight facility, in virginia, would be the primary launch site for the rocket.launch pad 0a (lp-0a), previously used for the failed conestoga rocket, would be modified to handle antares.wallops allows launches which reach the international space station's orbit as effectively as those from cape canaveral, florida, while being less crowded.the first antares flight launched a cygnus mass simulator.on december 10, 2009, alliant techsystems inc. (atk) test-fired their castor 30 motor for use on the second stage of the antares rocket.in march 2010, orbital sciences and aerojet completed test firings of the aj-26 engines.on february 22, 2013, a hot fire test was successfully performed, the entire first stage being erected on the pad and held down while the engines fired for 29 seconds.as orbital had little experience with large liquid stages and lox propellant, the first stage core was designed and is manufactured in ukraine by kb pivdenne and pivdenmash and includes propellant tanks, pressurization tanks, valves, sensors, feed lines, tubing, wiring and other associated hardware.like the zenit—also manufactured by yuzhmash—the antares vehicle has a diameter of 3.9 m (150 in) with a matching 3.9 m payload fairing. | antares rocket | launchsite | mid-atlantic regional spaceport <tsp> antares rocket | comparable | delta ii <tsp> antares rocket | manufacturer | yuzhnoye design office <tsp> delta ii | countryorigin | united states <tsp> antares rocket | launchsite | mid-atlantic regional spaceport launch pad 0 | antares (), known during early development as taurus ii, is an expendable launch system developed by orbital sciences corporation (now part of northrop grumman) and the pivdenne design bureau to launch the cygnus spacecraft to the international space station as part of nasa's cots and crs programs.able to launch payloads heavier than 8,000 kg (18,000 lb) into low earth orbit, antares is currently the largest rocket operated by northrop grumman.antares launches from the mid-atlantic regional spaceport and made its inaugural flight on april 21, 2013.nasa awarded orbital a commercial orbital transportation services (cots) space act agreement (saa) in 2008 to demonstrate delivery of cargo to the international space station.for these cots missions orbital intends to use antares to launch its cygnus spacecraft.originally designated the taurus ii, orbital sciences renamed the vehicle antares, after the star of the same name, on december 12, 2011.out of 17 total launches, antares has suffered one failure.the antares has flown two major design iterations, the 100 series and 200 series.launch pad 0a (lp-0a), previously used for the failed conestoga rocket, would be modified to handle antares.the first antares flight launched a cygnus mass simulator.on december 10, 2009, alliant techsystems inc. (atk) test-fired their castor 30 motor for use on the second stage of the antares rocket. |
(66063) 1998 ro1 is a stony near-earth object of the aten group on a highly-eccentric orbit.the synchronous binary system measures approximately 800 meters (0.50 miles) in diameter.it was discovered by astronomers of the lincoln near-earth asteroid research at the lincoln laboratory's experimental test site near socorro, new mexico, on 14 september 1998.its minor-planet moon, provisionally designated s/2001 (66063) 1, was discovered in september 2003.it has an orbital period of 14.53 hours and measures approximately 48% of its primary, or 380 meters.it is one of seven known aten binaries as of 2017.it has an orbital period of 360.29 days (0.99 years) and makes close approaches to earth.but 1998 ro1 makes closer approaches to other inner planets, especially mars.its closest approach to a planet between 1950–2200 was to mars, as it passed 0.00898 au (1,343,000 km) from mars on 18 march 1964, and will pass 0.0054 au (810,000 km) from mars on 12 october 2065.this moon was discovered from lightcurve observations going from 13 to 28 september 2013, and was confirmed by radar observations from the arecibo observatory one year later.it is in a very close orbit to 1998 ro1, with a semi-major axis of 800 m (2,600 ft) and an eccentricity of 0.06, giving it a periapsis of 752 m (2,467 ft) and an apoapsis of 848 m (2,782 ft).s/2001 (66063) 1 takes 14.54 hours to complete one orbit around 1998 ro1.from the surface of 1998 ro1, s/2001 (66063) 1 would have an apparent diameter of roughly 41°.for comparison, the sun appears to be 0.5° from earth.the secondary orbits its primary in a manner very similar to the adjunct image, where the red cross is the center of mass.as of 2018, it has not been named. | 66063 1998 ro1 | meantemperature | 2650 kelvins <tsp> 66063 1998 ro1 | apoapsis | 25498957060815 kilometres <tsp> 66063 1998 ro1 | epoch | 2013-11-04 <tsp> 66063 1998 ro1 | orbitalperiod | 36029 days <tsp> 66063 1998 ro1 | periapsis | 414984000000 | no related information |
san sebastián de los reyes (colloquially called 'sanse') is a municipality in the community of madrid, spain.founded in 1492, it is located 20 kilometres (12 mi) north of madrid.this line buses, along with urban ones, are the following: urban line 2: alcobendas - la moraleja (by paseo de alcobendas) (interbús) urban line 4: sports center - moscatelares (interbús) urban line 5: san sebastián de los reyes - alcobendas - el soto de la moraleja (interbús) urban line 7: alcobendas train station - polígonos - alcobendas train station (interbús) urban line 8: alcobendas (train station) - alcobendas (arroyo de la vega) (interbús) 151: madrid (plaza de castilla) - alcobendas (interbús) 152c: madrid (plaza de castilla) - san sebastián de los reyes (dehesa vieja) (interbús) 153: madrid (plaza de castilla) - alcobendas - rosa luxemburgo (interbús) 154: madrid (chamartín) - san sebastián de los reyes (circular by fuencarral) (interbús) 154c: madrid (plaza de castilla) - san sebastián de los reyes (quiñones avenue) (interbús) 156: madrid (plaza de castilla) - san sebastián de los reyes (polígono industrial moscatelares) (interbús) 158: madrid (pinar de chamartín) - alcobendas-san sebastián de los reyes (tempranales) (interbús) 161: madrid (plaza de castilla) - fuente del fresno urbanization (interbús) 166: san sebastián de los reyes-urbanización valdelagua (interbús) 180: alcobendas - algete (interbús) 171: madrid (plaza de castilla) - santo domingo urbanization (alsa) 191: madrid (plaza de castilla) - buitrago del lozoya (alsa) 193: madrid (plaza de castilla) - el vellón (alsa) 194: madrid (plaza de castilla) - rascafría (alsa) 195: madrid (plaza de castilla) - braojos (alsa) 196: madrid (plaza de castilla) - la acebeda (alsa) 197: madrid (plaza de castilla) - uceda (alsa) 210: san sebastián de los reyes - paracuellos de jarama (alsa) 827: madrid (canillejas) - tres cantos (doroteo casado montes) 827a: alcobendas - san sebastián de los reyes - university (doroteo casado montes) night bus line 102: madrid (plaza de castilla) - san sebastián de los reyes (interbús) night bus line 103: madrid (plaza de castilla) - algete (interbús) night bus line 104: madrid (plaza de castilla) - san agustín del guadalix (alsa)san sebastián de los reyes also shares a railway station with the neighboring municipality of alcobendas.from this station you can go to the city of madrid and to many other places such as getafe or parla.game developer mercurysteam is based here.a women's soccer team, madrid cff, plays in the primera división (women) but it has not gone well for them there.they are from madrid, but their stadium is in san sebastián. | san sebastián de los reyes | ispartof | community of madrid <tsp> enaire | locationcity | madrid <tsp> adolfo suárez madrid–barajas airport | location | san sebastián de los reyes <tsp> san sebastián de los reyes | country | spain <tsp> adolfo suárez madrid–barajas airport | operatingorganisation | enaire | san sebastián de los reyes (colloquially called 'sanse') is a municipality in the community of madrid, spain.this line buses, along with urban ones, are the following: urban line 2: alcobendas - la moraleja (by paseo de alcobendas) (interbús) urban line 4: sports center - moscatelares (interbús) urban line 5: san sebastián de los reyes - alcobendas - el soto de la moraleja (interbús) urban line 7: alcobendas train station - polígonos - alcobendas train station (interbús) urban line 8: alcobendas (train station) - alcobendas (arroyo de la vega) (interbús) 151: madrid (plaza de castilla) - alcobendas (interbús) 152c: madrid (plaza de castilla) - san sebastián de los reyes (dehesa vieja) (interbús) 153: madrid (plaza de castilla) - alcobendas - rosa luxemburgo (interbús) 154: madrid (chamartín) - san sebastián de los reyes (circular by fuencarral) (interbús) 154c: madrid (plaza de castilla) - san sebastián de los reyes (quiñones avenue) (interbús) 156: madrid (plaza de castilla) - san sebastián de los reyes (polígono industrial moscatelares) (interbús) 158: madrid (pinar de chamartín) - alcobendas-san sebastián de los reyes (tempranales) (interbús) 161: madrid (plaza de castilla) - fuente del fresno urbanization (interbús) 166: san sebastián de los reyes-urbanización valdelagua (interbús) 180: alcobendas - algete (interbús) 171: madrid (plaza de castilla) - santo domingo urbanization (alsa) 191: madrid (plaza de castilla) - buitrago del lozoya (alsa) 193: madrid (plaza de castilla) - el vellón (alsa) 194: madrid (plaza de castilla) - rascafría (alsa) 195: madrid (plaza de castilla) - braojos (alsa) 196: madrid (plaza de castilla) - la acebeda (alsa) 197: madrid (plaza de castilla) - uceda (alsa) 210: san sebastián de los reyes - paracuellos de jarama (alsa) 827: madrid (canillejas) - tres cantos (doroteo casado montes) 827a: alcobendas - san sebastián de los reyes - university (doroteo casado montes) night bus line 102: madrid (plaza de castilla) - san sebastián de los reyes (interbús) night bus line 103: madrid (plaza de castilla) - algete (interbús) night bus line 104: madrid (plaza de castilla) - san agustín del guadalix (alsa)san sebastián de los reyes also shares a railway station with the neighboring municipality of alcobendas.they are from madrid, but their stadium is in san sebastián. |
antares (), known during early development as taurus ii, is an expendable launch system developed by orbital sciences corporation (now part of northrop grumman) and the pivdenne design bureau to launch the cygnus spacecraft to the international space station as part of nasa's cots and crs programs.able to launch payloads heavier than 8,000 kg (18,000 lb) into low earth orbit, antares is currently the largest rocket operated by northrop grumman.antares launches from the mid-atlantic regional spaceport and made its inaugural flight on april 21, 2013.nasa awarded orbital a commercial orbital transportation services (cots) space act agreement (saa) in 2008 to demonstrate delivery of cargo to the international space station.for these cots missions orbital intends to use antares to launch its cygnus spacecraft.in addition, antares will compete for small-to-medium missions.originally designated the taurus ii, orbital sciences renamed the vehicle antares, after the star of the same name, on december 12, 2011.out of 17 total launches, antares has suffered one failure.during the fifth launch on october 28, 2014, the rocket failed catastrophically, and the vehicle and payload were destroyed.the rocket's first-stage engines were identified as the cause for the failure.a different engine was chosen for subsequent launches, and the rocket had a successful return to flight on october 17, 2016.the antares has flown two major design iterations, the 100 series and 200 series.both series have used a castor 30xl as an upper stage but have differed on the first stage.the 100 series used two kerolox powered aj26 engine in the first stage and launched successfully four times.the 100 series was retired following a launch failure in 2014.the 200 series which first flew in 2016 also featured a kerolox first stage but instead used two rd-181 engine along with other minor upgrades.the 200 series future became uncertain following the russian invasion of ukraine.due to the first stage being produced in ukraine and the engines in russia, future production of the rocket was unable to be continued.as a result northrop grumman entered into an agreement with firefly aerospace to build the first stage of the antares 300 series.northrop also contracted with spacex for 3 falcon 9 launches.a commercial resupply service contract of $1.9 billion for eight flights was awarded in 2008.as of april 2012, development costs were estimated at $472 million.in june 2008, it was announced that the mid-atlantic regional spaceport, formerly part of the wallops flight facility, in virginia, would be the primary launch site for the rocket.launch pad 0a (lp-0a), previously used for the failed conestoga rocket, would be modified to handle antares.wallops allows launches which reach the international space station's orbit as effectively as those from cape canaveral, florida, while being less crowded.the first antares flight launched a cygnus mass simulator.on december 10, 2009, alliant techsystems inc. (atk) test-fired their castor 30 motor for use on the second stage of the antares rocket.in march 2010, orbital sciences and aerojet completed test firings of the aj-26 engines.on february 22, 2013, a hot fire test was successfully performed, the entire first stage being erected on the pad and held down while the engines fired for 29 seconds.as orbital had little experience with large liquid stages and lox propellant, the first stage core was designed and is manufactured in ukraine by kb pivdenne and pivdenmash and includes propellant tanks, pressurization tanks, valves, sensors, feed lines, tubing, wiring and other associated hardware.like the zenit—also manufactured by yuzhmash—the antares vehicle has a diameter of 3.9 m (150 in) with a matching 3.9 m payload fairing. | antares rocket | launchsite | mid-atlantic regional spaceport <tsp> antares rocket | manufacturer | orbital atk <tsp> antares rocket | comparable | delta ii <tsp> delta ii | countryorigin | united states <tsp> antares rocket | launchsite | mid-atlantic regional spaceport launch pad 0 | antares (), known during early development as taurus ii, is an expendable launch system developed by orbital sciences corporation (now part of northrop grumman) and the pivdenne design bureau to launch the cygnus spacecraft to the international space station as part of nasa's cots and crs programs.able to launch payloads heavier than 8,000 kg (18,000 lb) into low earth orbit, antares is currently the largest rocket operated by northrop grumman.antares launches from the mid-atlantic regional spaceport and made its inaugural flight on april 21, 2013.nasa awarded orbital a commercial orbital transportation services (cots) space act agreement (saa) in 2008 to demonstrate delivery of cargo to the international space station.for these cots missions orbital intends to use antares to launch its cygnus spacecraft.originally designated the taurus ii, orbital sciences renamed the vehicle antares, after the star of the same name, on december 12, 2011.out of 17 total launches, antares has suffered one failure.launch pad 0a (lp-0a), previously used for the failed conestoga rocket, would be modified to handle antares.the first antares flight launched a cygnus mass simulator.on december 10, 2009, alliant techsystems inc. (atk) test-fired their castor 30 motor for use on the second stage of the antares rocket. |
san sebastián de los reyes (colloquially called 'sanse') is a municipality in the community of madrid, spain.founded in 1492, it is located 20 kilometres (12 mi) north of madrid.this line buses, along with urban ones, are the following: urban line 2: alcobendas - la moraleja (by paseo de alcobendas) (interbús) urban line 4: sports center - moscatelares (interbús) urban line 5: san sebastián de los reyes - alcobendas - el soto de la moraleja (interbús) urban line 7: alcobendas train station - polígonos - alcobendas train station (interbús) urban line 8: alcobendas (train station) - alcobendas (arroyo de la vega) (interbús) 151: madrid (plaza de castilla) - alcobendas (interbús) 152c: madrid (plaza de castilla) - san sebastián de los reyes (dehesa vieja) (interbús) 153: madrid (plaza de castilla) - alcobendas - rosa luxemburgo (interbús) 154: madrid (chamartín) - san sebastián de los reyes (circular by fuencarral) (interbús) 154c: madrid (plaza de castilla) - san sebastián de los reyes (quiñones avenue) (interbús) 156: madrid (plaza de castilla) - san sebastián de los reyes (polígono industrial moscatelares) (interbús) 158: madrid (pinar de chamartín) - alcobendas-san sebastián de los reyes (tempranales) (interbús) 161: madrid (plaza de castilla) - fuente del fresno urbanization (interbús) 166: san sebastián de los reyes-urbanización valdelagua (interbús) 180: alcobendas - algete (interbús) 171: madrid (plaza de castilla) - santo domingo urbanization (alsa) 191: madrid (plaza de castilla) - buitrago del lozoya (alsa) 193: madrid (plaza de castilla) - el vellón (alsa) 194: madrid (plaza de castilla) - rascafría (alsa) 195: madrid (plaza de castilla) - braojos (alsa) 196: madrid (plaza de castilla) - la acebeda (alsa) 197: madrid (plaza de castilla) - uceda (alsa) 210: san sebastián de los reyes - paracuellos de jarama (alsa) 827: madrid (canillejas) - tres cantos (doroteo casado montes) 827a: alcobendas - san sebastián de los reyes - university (doroteo casado montes) night bus line 102: madrid (plaza de castilla) - san sebastián de los reyes (interbús) night bus line 103: madrid (plaza de castilla) - algete (interbús) night bus line 104: madrid (plaza de castilla) - san agustín del guadalix (alsa)san sebastián de los reyes also shares a railway station with the neighboring municipality of alcobendas.from this station you can go to the city of madrid and to many other places such as getafe or parla.game developer mercurysteam is based here.a women's soccer team, madrid cff, plays in the primera división (women) but it has not gone well for them there.they are from madrid, but their stadium is in san sebastián. | san sebastián de los reyes | ispartof | community of madrid <tsp> enaire | locationcity | madrid <tsp> adolfo suárez madrid–barajas airport | location | san sebastián de los reyes <tsp> san sebastián de los reyes | country | spain <tsp> adolfo suárez madrid–barajas airport | operatingorganisation | enaire | san sebastián de los reyes (colloquially called 'sanse') is a municipality in the community of madrid, spain.this line buses, along with urban ones, are the following: urban line 2: alcobendas - la moraleja (by paseo de alcobendas) (interbús) urban line 4: sports center - moscatelares (interbús) urban line 5: san sebastián de los reyes - alcobendas - el soto de la moraleja (interbús) urban line 7: alcobendas train station - polígonos - alcobendas train station (interbús) urban line 8: alcobendas (train station) - alcobendas (arroyo de la vega) (interbús) 151: madrid (plaza de castilla) - alcobendas (interbús) 152c: madrid (plaza de castilla) - san sebastián de los reyes (dehesa vieja) (interbús) 153: madrid (plaza de castilla) - alcobendas - rosa luxemburgo (interbús) 154: madrid (chamartín) - san sebastián de los reyes (circular by fuencarral) (interbús) 154c: madrid (plaza de castilla) - san sebastián de los reyes (quiñones avenue) (interbús) 156: madrid (plaza de castilla) - san sebastián de los reyes (polígono industrial moscatelares) (interbús) 158: madrid (pinar de chamartín) - alcobendas-san sebastián de los reyes (tempranales) (interbús) 161: madrid (plaza de castilla) - fuente del fresno urbanization (interbús) 166: san sebastián de los reyes-urbanización valdelagua (interbús) 180: alcobendas - algete (interbús) 171: madrid (plaza de castilla) - santo domingo urbanization (alsa) 191: madrid (plaza de castilla) - buitrago del lozoya (alsa) 193: madrid (plaza de castilla) - el vellón (alsa) 194: madrid (plaza de castilla) - rascafría (alsa) 195: madrid (plaza de castilla) - braojos (alsa) 196: madrid (plaza de castilla) - la acebeda (alsa) 197: madrid (plaza de castilla) - uceda (alsa) 210: san sebastián de los reyes - paracuellos de jarama (alsa) 827: madrid (canillejas) - tres cantos (doroteo casado montes) 827a: alcobendas - san sebastián de los reyes - university (doroteo casado montes) night bus line 102: madrid (plaza de castilla) - san sebastián de los reyes (interbús) night bus line 103: madrid (plaza de castilla) - algete (interbús) night bus line 104: madrid (plaza de castilla) - san agustín del guadalix (alsa)san sebastián de los reyes also shares a railway station with the neighboring municipality of alcobendas.they are from madrid, but their stadium is in san sebastián. |
(66063) 1998 ro1 is a stony near-earth object of the aten group on a highly-eccentric orbit.the synchronous binary system measures approximately 800 meters (0.50 miles) in diameter.it was discovered by astronomers of the lincoln near-earth asteroid research at the lincoln laboratory's experimental test site near socorro, new mexico, on 14 september 1998.its minor-planet moon, provisionally designated s/2001 (66063) 1, was discovered in september 2003.it has an orbital period of 14.53 hours and measures approximately 48% of its primary, or 380 meters.it is one of seven known aten binaries as of 2017.it has an orbital period of 360.29 days (0.99 years) and makes close approaches to earth.but 1998 ro1 makes closer approaches to other inner planets, especially mars.its closest approach to a planet between 1950–2200 was to mars, as it passed 0.00898 au (1,343,000 km) from mars on 18 march 1964, and will pass 0.0054 au (810,000 km) from mars on 12 october 2065.this moon was discovered from lightcurve observations going from 13 to 28 september 2013, and was confirmed by radar observations from the arecibo observatory one year later.it is in a very close orbit to 1998 ro1, with a semi-major axis of 800 m (2,600 ft) and an eccentricity of 0.06, giving it a periapsis of 752 m (2,467 ft) and an apoapsis of 848 m (2,782 ft).s/2001 (66063) 1 takes 14.54 hours to complete one orbit around 1998 ro1.from the surface of 1998 ro1, s/2001 (66063) 1 would have an apparent diameter of roughly 41°.for comparison, the sun appears to be 0.5° from earth.the secondary orbits its primary in a manner very similar to the adjunct image, where the red cross is the center of mass.as of 2018, it has not been named. | cervicomuscular | unbigamously | flannelmouth | no related information |
(66063) 1998 ro1 is a stony near-earth object of the aten group on a highly-eccentric orbit.the synchronous binary system measures approximately 800 meters (0.50 miles) in diameter.it was discovered by astronomers of the lincoln near-earth asteroid research at the lincoln laboratory's experimental test site near socorro, new mexico, on 14 september 1998.its minor-planet moon, provisionally designated s/2001 (66063) 1, was discovered in september 2003.it has an orbital period of 14.53 hours and measures approximately 48% of its primary, or 380 meters.it is one of seven known aten binaries as of 2017.it has an orbital period of 360.29 days (0.99 years) and makes close approaches to earth.but 1998 ro1 makes closer approaches to other inner planets, especially mars.its closest approach to a planet between 1950–2200 was to mars, as it passed 0.00898 au (1,343,000 km) from mars on 18 march 1964, and will pass 0.0054 au (810,000 km) from mars on 12 october 2065.this moon was discovered from lightcurve observations going from 13 to 28 september 2013, and was confirmed by radar observations from the arecibo observatory one year later.it is in a very close orbit to 1998 ro1, with a semi-major axis of 800 m (2,600 ft) and an eccentricity of 0.06, giving it a periapsis of 752 m (2,467 ft) and an apoapsis of 848 m (2,782 ft).s/2001 (66063) 1 takes 14.54 hours to complete one orbit around 1998 ro1.from the surface of 1998 ro1, s/2001 (66063) 1 would have an apparent diameter of roughly 41°.for comparison, the sun appears to be 0.5° from earth.the secondary orbits its primary in a manner very similar to the adjunct image, where the red cross is the center of mass.as of 2018, it has not been named. | 66063 1998 ro1 | meantemperature | 2650 kelvins <tsp> 66063 1998 ro1 | apoapsis | 25498957060815 kilometres <tsp> 66063 1998 ro1 | epoch | 2013-11-04 <tsp> 66063 1998 ro1 | orbitalperiod | 36029 days <tsp> 66063 1998 ro1 | periapsis | 414984000000 | no related information |
antares (), known during early development as taurus ii, is an expendable launch system developed by orbital sciences corporation (now part of northrop grumman) and the pivdenne design bureau to launch the cygnus spacecraft to the international space station as part of nasa's cots and crs programs.able to launch payloads heavier than 8,000 kg (18,000 lb) into low earth orbit, antares is currently the largest rocket operated by northrop grumman.antares launches from the mid-atlantic regional spaceport and made its inaugural flight on april 21, 2013.nasa awarded orbital a commercial orbital transportation services (cots) space act agreement (saa) in 2008 to demonstrate delivery of cargo to the international space station.for these cots missions orbital intends to use antares to launch its cygnus spacecraft.in addition, antares will compete for small-to-medium missions.originally designated the taurus ii, orbital sciences renamed the vehicle antares, after the star of the same name, on december 12, 2011.out of 17 total launches, antares has suffered one failure.during the fifth launch on october 28, 2014, the rocket failed catastrophically, and the vehicle and payload were destroyed.the rocket's first-stage engines were identified as the cause for the failure.a different engine was chosen for subsequent launches, and the rocket had a successful return to flight on october 17, 2016.the antares has flown two major design iterations, the 100 series and 200 series.both series have used a castor 30xl as an upper stage but have differed on the first stage.the 100 series used two kerolox powered aj26 engine in the first stage and launched successfully four times.the 100 series was retired following a launch failure in 2014.the 200 series which first flew in 2016 also featured a kerolox first stage but instead used two rd-181 engine along with other minor upgrades.the 200 series future became uncertain following the russian invasion of ukraine.due to the first stage being produced in ukraine and the engines in russia, future production of the rocket was unable to be continued.as a result northrop grumman entered into an agreement with firefly aerospace to build the first stage of the antares 300 series.northrop also contracted with spacex for 3 falcon 9 launches.a commercial resupply service contract of $1.9 billion for eight flights was awarded in 2008.as of april 2012, development costs were estimated at $472 million.in june 2008, it was announced that the mid-atlantic regional spaceport, formerly part of the wallops flight facility, in virginia, would be the primary launch site for the rocket.launch pad 0a (lp-0a), previously used for the failed conestoga rocket, would be modified to handle antares.wallops allows launches which reach the international space station's orbit as effectively as those from cape canaveral, florida, while being less crowded.the first antares flight launched a cygnus mass simulator.on december 10, 2009, alliant techsystems inc. (atk) test-fired their castor 30 motor for use on the second stage of the antares rocket.in march 2010, orbital sciences and aerojet completed test firings of the aj-26 engines.on february 22, 2013, a hot fire test was successfully performed, the entire first stage being erected on the pad and held down while the engines fired for 29 seconds.as orbital had little experience with large liquid stages and lox propellant, the first stage core was designed and is manufactured in ukraine by kb pivdenne and pivdenmash and includes propellant tanks, pressurization tanks, valves, sensors, feed lines, tubing, wiring and other associated hardware.like the zenit—also manufactured by yuzhmash—the antares vehicle has a diameter of 3.9 m (150 in) with a matching 3.9 m payload fairing. | antares rocket | launchsite | mid-atlantic regional spaceport <tsp> antares rocket | manufacturer | orbital atk <tsp> antares rocket | comparable | delta ii <tsp> delta ii | countryorigin | united states <tsp> antares rocket | launchsite | mid-atlantic regional spaceport launch pad 0 | antares (), known during early development as taurus ii, is an expendable launch system developed by orbital sciences corporation (now part of northrop grumman) and the pivdenne design bureau to launch the cygnus spacecraft to the international space station as part of nasa's cots and crs programs.able to launch payloads heavier than 8,000 kg (18,000 lb) into low earth orbit, antares is currently the largest rocket operated by northrop grumman.antares launches from the mid-atlantic regional spaceport and made its inaugural flight on april 21, 2013.nasa awarded orbital a commercial orbital transportation services (cots) space act agreement (saa) in 2008 to demonstrate delivery of cargo to the international space station.for these cots missions orbital intends to use antares to launch its cygnus spacecraft.originally designated the taurus ii, orbital sciences renamed the vehicle antares, after the star of the same name, on december 12, 2011.out of 17 total launches, antares has suffered one failure.launch pad 0a (lp-0a), previously used for the failed conestoga rocket, would be modified to handle antares.the first antares flight launched a cygnus mass simulator.on december 10, 2009, alliant techsystems inc. (atk) test-fired their castor 30 motor for use on the second stage of the antares rocket. |
san sebastián de los reyes (colloquially called 'sanse') is a municipality in the community of madrid, spain.founded in 1492, it is located 20 kilometres (12 mi) north of madrid.this line buses, along with urban ones, are the following: urban line 2: alcobendas - la moraleja (by paseo de alcobendas) (interbús) urban line 4: sports center - moscatelares (interbús) urban line 5: san sebastián de los reyes - alcobendas - el soto de la moraleja (interbús) urban line 7: alcobendas train station - polígonos - alcobendas train station (interbús) urban line 8: alcobendas (train station) - alcobendas (arroyo de la vega) (interbús) 151: madrid (plaza de castilla) - alcobendas (interbús) 152c: madrid (plaza de castilla) - san sebastián de los reyes (dehesa vieja) (interbús) 153: madrid (plaza de castilla) - alcobendas - rosa luxemburgo (interbús) 154: madrid (chamartín) - san sebastián de los reyes (circular by fuencarral) (interbús) 154c: madrid (plaza de castilla) - san sebastián de los reyes (quiñones avenue) (interbús) 156: madrid (plaza de castilla) - san sebastián de los reyes (polígono industrial moscatelares) (interbús) 158: madrid (pinar de chamartín) - alcobendas-san sebastián de los reyes (tempranales) (interbús) 161: madrid (plaza de castilla) - fuente del fresno urbanization (interbús) 166: san sebastián de los reyes-urbanización valdelagua (interbús) 180: alcobendas - algete (interbús) 171: madrid (plaza de castilla) - santo domingo urbanization (alsa) 191: madrid (plaza de castilla) - buitrago del lozoya (alsa) 193: madrid (plaza de castilla) - el vellón (alsa) 194: madrid (plaza de castilla) - rascafría (alsa) 195: madrid (plaza de castilla) - braojos (alsa) 196: madrid (plaza de castilla) - la acebeda (alsa) 197: madrid (plaza de castilla) - uceda (alsa) 210: san sebastián de los reyes - paracuellos de jarama (alsa) 827: madrid (canillejas) - tres cantos (doroteo casado montes) 827a: alcobendas - san sebastián de los reyes - university (doroteo casado montes) night bus line 102: madrid (plaza de castilla) - san sebastián de los reyes (interbús) night bus line 103: madrid (plaza de castilla) - algete (interbús) night bus line 104: madrid (plaza de castilla) - san agustín del guadalix (alsa)san sebastián de los reyes also shares a railway station with the neighboring municipality of alcobendas.from this station you can go to the city of madrid and to many other places such as getafe or parla.game developer mercurysteam is based here.a women's soccer team, madrid cff, plays in the primera división (women) but it has not gone well for them there.they are from madrid, but their stadium is in san sebastián. | premiss | chloritoid | shereef | no related information |
antares (), known during early development as taurus ii, is an expendable launch system developed by orbital sciences corporation (now part of northrop grumman) and the pivdenne design bureau to launch the cygnus spacecraft to the international space station as part of nasa's cots and crs programs.able to launch payloads heavier than 8,000 kg (18,000 lb) into low earth orbit, antares is currently the largest rocket operated by northrop grumman.antares launches from the mid-atlantic regional spaceport and made its inaugural flight on april 21, 2013.nasa awarded orbital a commercial orbital transportation services (cots) space act agreement (saa) in 2008 to demonstrate delivery of cargo to the international space station.for these cots missions orbital intends to use antares to launch its cygnus spacecraft.in addition, antares will compete for small-to-medium missions.originally designated the taurus ii, orbital sciences renamed the vehicle antares, after the star of the same name, on december 12, 2011.out of 17 total launches, antares has suffered one failure.during the fifth launch on october 28, 2014, the rocket failed catastrophically, and the vehicle and payload were destroyed.the rocket's first-stage engines were identified as the cause for the failure.a different engine was chosen for subsequent launches, and the rocket had a successful return to flight on october 17, 2016.the antares has flown two major design iterations, the 100 series and 200 series.both series have used a castor 30xl as an upper stage but have differed on the first stage.the 100 series used two kerolox powered aj26 engine in the first stage and launched successfully four times.the 100 series was retired following a launch failure in 2014.the 200 series which first flew in 2016 also featured a kerolox first stage but instead used two rd-181 engine along with other minor upgrades.the 200 series future became uncertain following the russian invasion of ukraine.due to the first stage being produced in ukraine and the engines in russia, future production of the rocket was unable to be continued.as a result northrop grumman entered into an agreement with firefly aerospace to build the first stage of the antares 300 series.northrop also contracted with spacex for 3 falcon 9 launches.a commercial resupply service contract of $1.9 billion for eight flights was awarded in 2008.as of april 2012, development costs were estimated at $472 million.in june 2008, it was announced that the mid-atlantic regional spaceport, formerly part of the wallops flight facility, in virginia, would be the primary launch site for the rocket.launch pad 0a (lp-0a), previously used for the failed conestoga rocket, would be modified to handle antares.wallops allows launches which reach the international space station's orbit as effectively as those from cape canaveral, florida, while being less crowded.the first antares flight launched a cygnus mass simulator.on december 10, 2009, alliant techsystems inc. (atk) test-fired their castor 30 motor for use on the second stage of the antares rocket.in march 2010, orbital sciences and aerojet completed test firings of the aj-26 engines.on february 22, 2013, a hot fire test was successfully performed, the entire first stage being erected on the pad and held down while the engines fired for 29 seconds.as orbital had little experience with large liquid stages and lox propellant, the first stage core was designed and is manufactured in ukraine by kb pivdenne and pivdenmash and includes propellant tanks, pressurization tanks, valves, sensors, feed lines, tubing, wiring and other associated hardware.like the zenit—also manufactured by yuzhmash—the antares vehicle has a diameter of 3.9 m (150 in) with a matching 3.9 m payload fairing. | antares rocket | launchsite | mid-atlantic regional spaceport <tsp> antares rocket | manufacturer | orbital atk <tsp> antares rocket | comparable | delta ii <tsp> delta ii | countryorigin | united states <tsp> antares rocket | launchsite | mid-atlantic regional spaceport launch pad 0 | antares (), known during early development as taurus ii, is an expendable launch system developed by orbital sciences corporation (now part of northrop grumman) and the pivdenne design bureau to launch the cygnus spacecraft to the international space station as part of nasa's cots and crs programs.able to launch payloads heavier than 8,000 kg (18,000 lb) into low earth orbit, antares is currently the largest rocket operated by northrop grumman.antares launches from the mid-atlantic regional spaceport and made its inaugural flight on april 21, 2013.nasa awarded orbital a commercial orbital transportation services (cots) space act agreement (saa) in 2008 to demonstrate delivery of cargo to the international space station.for these cots missions orbital intends to use antares to launch its cygnus spacecraft.originally designated the taurus ii, orbital sciences renamed the vehicle antares, after the star of the same name, on december 12, 2011.out of 17 total launches, antares has suffered one failure.launch pad 0a (lp-0a), previously used for the failed conestoga rocket, would be modified to handle antares.the first antares flight launched a cygnus mass simulator.on december 10, 2009, alliant techsystems inc. (atk) test-fired their castor 30 motor for use on the second stage of the antares rocket. |
(66063) 1998 ro1 is a stony near-earth object of the aten group on a highly-eccentric orbit.the synchronous binary system measures approximately 800 meters (0.50 miles) in diameter.it was discovered by astronomers of the lincoln near-earth asteroid research at the lincoln laboratory's experimental test site near socorro, new mexico, on 14 september 1998.its minor-planet moon, provisionally designated s/2001 (66063) 1, was discovered in september 2003.it has an orbital period of 14.53 hours and measures approximately 48% of its primary, or 380 meters.it is one of seven known aten binaries as of 2017.it has an orbital period of 360.29 days (0.99 years) and makes close approaches to earth.but 1998 ro1 makes closer approaches to other inner planets, especially mars.its closest approach to a planet between 1950–2200 was to mars, as it passed 0.00898 au (1,343,000 km) from mars on 18 march 1964, and will pass 0.0054 au (810,000 km) from mars on 12 october 2065.this moon was discovered from lightcurve observations going from 13 to 28 september 2013, and was confirmed by radar observations from the arecibo observatory one year later.it is in a very close orbit to 1998 ro1, with a semi-major axis of 800 m (2,600 ft) and an eccentricity of 0.06, giving it a periapsis of 752 m (2,467 ft) and an apoapsis of 848 m (2,782 ft).s/2001 (66063) 1 takes 14.54 hours to complete one orbit around 1998 ro1.from the surface of 1998 ro1, s/2001 (66063) 1 would have an apparent diameter of roughly 41°.for comparison, the sun appears to be 0.5° from earth.the secondary orbits its primary in a manner very similar to the adjunct image, where the red cross is the center of mass.as of 2018, it has not been named. | pictography | amidoxime | hexastigm <tsp> pictography | dulce | nestorian | no related information |
antares (), known during early development as taurus ii, is an expendable launch system developed by orbital sciences corporation (now part of northrop grumman) and the pivdenne design bureau to launch the cygnus spacecraft to the international space station as part of nasa's cots and crs programs.able to launch payloads heavier than 8,000 kg (18,000 lb) into low earth orbit, antares is currently the largest rocket operated by northrop grumman.antares launches from the mid-atlantic regional spaceport and made its inaugural flight on april 21, 2013.nasa awarded orbital a commercial orbital transportation services (cots) space act agreement (saa) in 2008 to demonstrate delivery of cargo to the international space station.for these cots missions orbital intends to use antares to launch its cygnus spacecraft.in addition, antares will compete for small-to-medium missions.originally designated the taurus ii, orbital sciences renamed the vehicle antares, after the star of the same name, on december 12, 2011.out of 17 total launches, antares has suffered one failure.during the fifth launch on october 28, 2014, the rocket failed catastrophically, and the vehicle and payload were destroyed.the rocket's first-stage engines were identified as the cause for the failure.a different engine was chosen for subsequent launches, and the rocket had a successful return to flight on october 17, 2016.the antares has flown two major design iterations, the 100 series and 200 series.both series have used a castor 30xl as an upper stage but have differed on the first stage.the 100 series used two kerolox powered aj26 engine in the first stage and launched successfully four times.the 100 series was retired following a launch failure in 2014.the 200 series which first flew in 2016 also featured a kerolox first stage but instead used two rd-181 engine along with other minor upgrades.the 200 series future became uncertain following the russian invasion of ukraine.due to the first stage being produced in ukraine and the engines in russia, future production of the rocket was unable to be continued.as a result northrop grumman entered into an agreement with firefly aerospace to build the first stage of the antares 300 series.northrop also contracted with spacex for 3 falcon 9 launches.a commercial resupply service contract of $1.9 billion for eight flights was awarded in 2008.as of april 2012, development costs were estimated at $472 million.in june 2008, it was announced that the mid-atlantic regional spaceport, formerly part of the wallops flight facility, in virginia, would be the primary launch site for the rocket.launch pad 0a (lp-0a), previously used for the failed conestoga rocket, would be modified to handle antares.wallops allows launches which reach the international space station's orbit as effectively as those from cape canaveral, florida, while being less crowded.the first antares flight launched a cygnus mass simulator.on december 10, 2009, alliant techsystems inc. (atk) test-fired their castor 30 motor for use on the second stage of the antares rocket.in march 2010, orbital sciences and aerojet completed test firings of the aj-26 engines.on february 22, 2013, a hot fire test was successfully performed, the entire first stage being erected on the pad and held down while the engines fired for 29 seconds.as orbital had little experience with large liquid stages and lox propellant, the first stage core was designed and is manufactured in ukraine by kb pivdenne and pivdenmash and includes propellant tanks, pressurization tanks, valves, sensors, feed lines, tubing, wiring and other associated hardware.like the zenit—also manufactured by yuzhmash—the antares vehicle has a diameter of 3.9 m (150 in) with a matching 3.9 m payload fairing. | antares rocket | maidenflight | 2013-04-21 <tsp> antares rocket | manufacturer | orbital atk <tsp> antares rocket | launchsite | mid-atlantic regional spaceport launch pad 0 <tsp> antares rocket | diameter | 39 metres <tsp> antares rocket | finalflight | 2013-09-18 | antares (), known during early development as taurus ii, is an expendable launch system developed by orbital sciences corporation (now part of northrop grumman) and the pivdenne design bureau to launch the cygnus spacecraft to the international space station as part of nasa's cots and crs programs.able to launch payloads heavier than 8,000 kg (18,000 lb) into low earth orbit, antares is currently the largest rocket operated by northrop grumman.antares launches from the mid-atlantic regional spaceport and made its inaugural flight on april 21, 2013.nasa awarded orbital a commercial orbital transportation services (cots) space act agreement (saa) in 2008 to demonstrate delivery of cargo to the international space station.for these cots missions orbital intends to use antares to launch its cygnus spacecraft.originally designated the taurus ii, orbital sciences renamed the vehicle antares, after the star of the same name, on december 12, 2011.out of 17 total launches, antares has suffered one failure.launch pad 0a (lp-0a), previously used for the failed conestoga rocket, would be modified to handle antares.the first antares flight launched a cygnus mass simulator.on december 10, 2009, alliant techsystems inc. (atk) test-fired their castor 30 motor for use on the second stage of the antares rocket. |
(66063) 1998 ro1 is a stony near-earth object of the aten group on a highly-eccentric orbit.the synchronous binary system measures approximately 800 meters (0.50 miles) in diameter.it was discovered by astronomers of the lincoln near-earth asteroid research at the lincoln laboratory's experimental test site near socorro, new mexico, on 14 september 1998.its minor-planet moon, provisionally designated s/2001 (66063) 1, was discovered in september 2003.it has an orbital period of 14.53 hours and measures approximately 48% of its primary, or 380 meters.it is one of seven known aten binaries as of 2017.it has an orbital period of 360.29 days (0.99 years) and makes close approaches to earth.but 1998 ro1 makes closer approaches to other inner planets, especially mars.its closest approach to a planet between 1950–2200 was to mars, as it passed 0.00898 au (1,343,000 km) from mars on 18 march 1964, and will pass 0.0054 au (810,000 km) from mars on 12 october 2065.this moon was discovered from lightcurve observations going from 13 to 28 september 2013, and was confirmed by radar observations from the arecibo observatory one year later.it is in a very close orbit to 1998 ro1, with a semi-major axis of 800 m (2,600 ft) and an eccentricity of 0.06, giving it a periapsis of 752 m (2,467 ft) and an apoapsis of 848 m (2,782 ft).s/2001 (66063) 1 takes 14.54 hours to complete one orbit around 1998 ro1.from the surface of 1998 ro1, s/2001 (66063) 1 would have an apparent diameter of roughly 41°.for comparison, the sun appears to be 0.5° from earth.the secondary orbits its primary in a manner very similar to the adjunct image, where the red cross is the center of mass.as of 2018, it has not been named. | dorlach | precorrespond | rochet | no related information |
antares (), known during early development as taurus ii, is an expendable launch system developed by orbital sciences corporation (now part of northrop grumman) and the pivdenne design bureau to launch the cygnus spacecraft to the international space station as part of nasa's cots and crs programs.able to launch payloads heavier than 8,000 kg (18,000 lb) into low earth orbit, antares is currently the largest rocket operated by northrop grumman.antares launches from the mid-atlantic regional spaceport and made its inaugural flight on april 21, 2013.nasa awarded orbital a commercial orbital transportation services (cots) space act agreement (saa) in 2008 to demonstrate delivery of cargo to the international space station.for these cots missions orbital intends to use antares to launch its cygnus spacecraft.in addition, antares will compete for small-to-medium missions.originally designated the taurus ii, orbital sciences renamed the vehicle antares, after the star of the same name, on december 12, 2011.out of 17 total launches, antares has suffered one failure.during the fifth launch on october 28, 2014, the rocket failed catastrophically, and the vehicle and payload were destroyed.the rocket's first-stage engines were identified as the cause for the failure.a different engine was chosen for subsequent launches, and the rocket had a successful return to flight on october 17, 2016.the antares has flown two major design iterations, the 100 series and 200 series.both series have used a castor 30xl as an upper stage but have differed on the first stage.the 100 series used two kerolox powered aj26 engine in the first stage and launched successfully four times.the 100 series was retired following a launch failure in 2014.the 200 series which first flew in 2016 also featured a kerolox first stage but instead used two rd-181 engine along with other minor upgrades.the 200 series future became uncertain following the russian invasion of ukraine.due to the first stage being produced in ukraine and the engines in russia, future production of the rocket was unable to be continued.as a result northrop grumman entered into an agreement with firefly aerospace to build the first stage of the antares 300 series.northrop also contracted with spacex for 3 falcon 9 launches.a commercial resupply service contract of $1.9 billion for eight flights was awarded in 2008.as of april 2012, development costs were estimated at $472 million.in june 2008, it was announced that the mid-atlantic regional spaceport, formerly part of the wallops flight facility, in virginia, would be the primary launch site for the rocket.launch pad 0a (lp-0a), previously used for the failed conestoga rocket, would be modified to handle antares.wallops allows launches which reach the international space station's orbit as effectively as those from cape canaveral, florida, while being less crowded.the first antares flight launched a cygnus mass simulator.on december 10, 2009, alliant techsystems inc. (atk) test-fired their castor 30 motor for use on the second stage of the antares rocket.in march 2010, orbital sciences and aerojet completed test firings of the aj-26 engines.on february 22, 2013, a hot fire test was successfully performed, the entire first stage being erected on the pad and held down while the engines fired for 29 seconds.as orbital had little experience with large liquid stages and lox propellant, the first stage core was designed and is manufactured in ukraine by kb pivdenne and pivdenmash and includes propellant tanks, pressurization tanks, valves, sensors, feed lines, tubing, wiring and other associated hardware.like the zenit—also manufactured by yuzhmash—the antares vehicle has a diameter of 3.9 m (150 in) with a matching 3.9 m payload fairing. | antares rocket | maidenflight | 2013-04-21 <tsp> antares rocket | manufacturer | orbital atk <tsp> antares rocket | launchsite | mid-atlantic regional spaceport launch pad 0 <tsp> antares rocket | diameter | 39 metres <tsp> antares rocket | finalflight | 2013-09-18 | antares (), known during early development as taurus ii, is an expendable launch system developed by orbital sciences corporation (now part of northrop grumman) and the pivdenne design bureau to launch the cygnus spacecraft to the international space station as part of nasa's cots and crs programs.able to launch payloads heavier than 8,000 kg (18,000 lb) into low earth orbit, antares is currently the largest rocket operated by northrop grumman.antares launches from the mid-atlantic regional spaceport and made its inaugural flight on april 21, 2013.nasa awarded orbital a commercial orbital transportation services (cots) space act agreement (saa) in 2008 to demonstrate delivery of cargo to the international space station.for these cots missions orbital intends to use antares to launch its cygnus spacecraft.originally designated the taurus ii, orbital sciences renamed the vehicle antares, after the star of the same name, on december 12, 2011.out of 17 total launches, antares has suffered one failure.launch pad 0a (lp-0a), previously used for the failed conestoga rocket, would be modified to handle antares.the first antares flight launched a cygnus mass simulator.on december 10, 2009, alliant techsystems inc. (atk) test-fired their castor 30 motor for use on the second stage of the antares rocket. |
66391 moshup , provisional designation 1999 kw4, is a binary asteroid, classified as a near-earth object and potentially hazardous asteroid of the aten group, approximately 1.3 kilometers in diameter.it was discovered on 20 may 1999, by lincoln near-earth asteroid research (linear) at the lincoln laboratory's experimental test site in socorro, new mexico, united states.it is a mercury-crosser that comes extremely close to the sun at a perihelion of 0.2 au.its orbit has an eccentricity of 0.69 and an inclination of 39° with respect to the ecliptic.a first precovery was taken by 2mass at the fred lawrence whipple observatory in 1998, extending the body's observation arc by one year prior to its official discovery observation at socorro.as a potentially hazardous asteroid, it has an earth minimum orbital intersection distance of 0.0138 au (2,060,000 km) which corresponds to 5.4 lunar distances.on 25 may 2036, it will pass 0.0155 au (2,320,000 km) from earth.it was named from mohegan legend, after moshup, a giant who lived in the coastal areas of new england.the asteroid's companion is named squannit, after the wife of moshup and a medicine woman of the makiawisug (little people).the official naming citation was published by the minor planet center on 27 august 2019 (m.p.c.115894).the moon, named squannit and designated s/2001 (66391) 1, is approximately 360 metres in diameter, and orbits its primary in every 16 hours at a mean-distance of 2.6 kilometers.the presence of a companion was suggested by photometric observations made by pravec and šarounová and was confirmed by radar observations from arecibo observations and announced on 23 may 2001 (also see below).based on radar imaging, squannit's dimensions are estimated to be 595 × 450 × 343 meters.the observations were taken from may 21–23, 2001, by lance a. m. benner, steven j. ostro, jon d. giorgini, raymond f. jurgens, jean-luc margot and michael c. nolan.the collaborative asteroid lightcurve link adopts a diameter of 1.3 kilometers and derives an albedo 0.26 with an absolute magnitude of 16.5.the shapes of the two bodies and their dynamics are complex.with a dimension of approximately 1.42 × 1.36 × 1.18 kilometers for a simple triaxial ellipsoid, the asteroid has an oblate shape, which is dominated by an equatorial ridge at the body's potential-energy minimum.this bizarre property of the equatorial region means that it is close to breakup: raising a particle a meter above the surface would put it into orbit.as seen in the image at above right, the gravitational effects between the moon and the asteroid create a gigantic mountain extending in the equatorial plane around the entire asteroid.it was the first asteroid to be described as 'muffin-shaped', which is now understood to be a very common shape for asteroids in critical rotation, including 101955 bennu and 162173 ryugu.lightcurve analysis gave a rotation period of 2.7650 hours with a brightness variation of 0.12 magnitude (u=3). | 66391 1999 kw4 | epoch | 2004-07-14 <tsp> 66391 1999 kw4 | escapevelocity | 0 <tsp> 66391 1999 kw4 | orbitalperiod | 162447000 <tsp> 66391 1999 kw4 | periapsis | 299196000000 <tsp> 66391 1999 kw4 | density | 20 grampercubiccentimetres | no related information |
66391 moshup , provisional designation 1999 kw4, is a binary asteroid, classified as a near-earth object and potentially hazardous asteroid of the aten group, approximately 1.3 kilometers in diameter.it was discovered on 20 may 1999, by lincoln near-earth asteroid research (linear) at the lincoln laboratory's experimental test site in socorro, new mexico, united states.it is a mercury-crosser that comes extremely close to the sun at a perihelion of 0.2 au.its orbit has an eccentricity of 0.69 and an inclination of 39° with respect to the ecliptic.a first precovery was taken by 2mass at the fred lawrence whipple observatory in 1998, extending the body's observation arc by one year prior to its official discovery observation at socorro.as a potentially hazardous asteroid, it has an earth minimum orbital intersection distance of 0.0138 au (2,060,000 km) which corresponds to 5.4 lunar distances.on 25 may 2036, it will pass 0.0155 au (2,320,000 km) from earth.it was named from mohegan legend, after moshup, a giant who lived in the coastal areas of new england.the asteroid's companion is named squannit, after the wife of moshup and a medicine woman of the makiawisug (little people).the official naming citation was published by the minor planet center on 27 august 2019 (m.p.c.115894).the moon, named squannit and designated s/2001 (66391) 1, is approximately 360 metres in diameter, and orbits its primary in every 16 hours at a mean-distance of 2.6 kilometers.the presence of a companion was suggested by photometric observations made by pravec and šarounová and was confirmed by radar observations from arecibo observations and announced on 23 may 2001 (also see below).based on radar imaging, squannit's dimensions are estimated to be 595 × 450 × 343 meters.the observations were taken from may 21–23, 2001, by lance a. m. benner, steven j. ostro, jon d. giorgini, raymond f. jurgens, jean-luc margot and michael c. nolan.the collaborative asteroid lightcurve link adopts a diameter of 1.3 kilometers and derives an albedo 0.26 with an absolute magnitude of 16.5.the shapes of the two bodies and their dynamics are complex.with a dimension of approximately 1.42 × 1.36 × 1.18 kilometers for a simple triaxial ellipsoid, the asteroid has an oblate shape, which is dominated by an equatorial ridge at the body's potential-energy minimum.this bizarre property of the equatorial region means that it is close to breakup: raising a particle a meter above the surface would put it into orbit.as seen in the image at above right, the gravitational effects between the moon and the asteroid create a gigantic mountain extending in the equatorial plane around the entire asteroid.it was the first asteroid to be described as 'muffin-shaped', which is now understood to be a very common shape for asteroids in critical rotation, including 101955 bennu and 162173 ryugu.lightcurve analysis gave a rotation period of 2.7650 hours with a brightness variation of 0.12 magnitude (u=3). | 66391 1999 kw4 | epoch | 2004-07-14 <tsp> 66391 1999 kw4 | escapevelocity | 0 <tsp> 66391 1999 kw4 | orbitalperiod | 162447000 <tsp> 66391 1999 kw4 | periapsis | 299196000000 <tsp> 66391 1999 kw4 | density | 20 grampercubiccentimetres | no related information |
antares (), known during early development as taurus ii, is an expendable launch system developed by orbital sciences corporation (now part of northrop grumman) and the pivdenne design bureau to launch the cygnus spacecraft to the international space station as part of nasa's cots and crs programs.able to launch payloads heavier than 8,000 kg (18,000 lb) into low earth orbit, antares is currently the largest rocket operated by northrop grumman.antares launches from the mid-atlantic regional spaceport and made its inaugural flight on april 21, 2013.nasa awarded orbital a commercial orbital transportation services (cots) space act agreement (saa) in 2008 to demonstrate delivery of cargo to the international space station.for these cots missions orbital intends to use antares to launch its cygnus spacecraft.in addition, antares will compete for small-to-medium missions.originally designated the taurus ii, orbital sciences renamed the vehicle antares, after the star of the same name, on december 12, 2011.out of 17 total launches, antares has suffered one failure.during the fifth launch on october 28, 2014, the rocket failed catastrophically, and the vehicle and payload were destroyed.the rocket's first-stage engines were identified as the cause for the failure.a different engine was chosen for subsequent launches, and the rocket had a successful return to flight on october 17, 2016.the antares has flown two major design iterations, the 100 series and 200 series.both series have used a castor 30xl as an upper stage but have differed on the first stage.the 100 series used two kerolox powered aj26 engine in the first stage and launched successfully four times.the 100 series was retired following a launch failure in 2014.the 200 series which first flew in 2016 also featured a kerolox first stage but instead used two rd-181 engine along with other minor upgrades.the 200 series future became uncertain following the russian invasion of ukraine.due to the first stage being produced in ukraine and the engines in russia, future production of the rocket was unable to be continued.as a result northrop grumman entered into an agreement with firefly aerospace to build the first stage of the antares 300 series.northrop also contracted with spacex for 3 falcon 9 launches.a commercial resupply service contract of $1.9 billion for eight flights was awarded in 2008.as of april 2012, development costs were estimated at $472 million.in june 2008, it was announced that the mid-atlantic regional spaceport, formerly part of the wallops flight facility, in virginia, would be the primary launch site for the rocket.launch pad 0a (lp-0a), previously used for the failed conestoga rocket, would be modified to handle antares.wallops allows launches which reach the international space station's orbit as effectively as those from cape canaveral, florida, while being less crowded.the first antares flight launched a cygnus mass simulator.on december 10, 2009, alliant techsystems inc. (atk) test-fired their castor 30 motor for use on the second stage of the antares rocket.in march 2010, orbital sciences and aerojet completed test firings of the aj-26 engines.on february 22, 2013, a hot fire test was successfully performed, the entire first stage being erected on the pad and held down while the engines fired for 29 seconds.as orbital had little experience with large liquid stages and lox propellant, the first stage core was designed and is manufactured in ukraine by kb pivdenne and pivdenmash and includes propellant tanks, pressurization tanks, valves, sensors, feed lines, tubing, wiring and other associated hardware.like the zenit—also manufactured by yuzhmash—the antares vehicle has a diameter of 3.9 m (150 in) with a matching 3.9 m payload fairing. | antares rocket | maidenflight | 2013-04-21 <tsp> antares rocket | manufacturer | orbital atk <tsp> antares rocket | launchsite | mid-atlantic regional spaceport launch pad 0 <tsp> antares rocket | diameter | 39 metres <tsp> antares rocket | finalflight | 2013-09-18 | antares (), known during early development as taurus ii, is an expendable launch system developed by orbital sciences corporation (now part of northrop grumman) and the pivdenne design bureau to launch the cygnus spacecraft to the international space station as part of nasa's cots and crs programs.able to launch payloads heavier than 8,000 kg (18,000 lb) into low earth orbit, antares is currently the largest rocket operated by northrop grumman.antares launches from the mid-atlantic regional spaceport and made its inaugural flight on april 21, 2013.nasa awarded orbital a commercial orbital transportation services (cots) space act agreement (saa) in 2008 to demonstrate delivery of cargo to the international space station.for these cots missions orbital intends to use antares to launch its cygnus spacecraft.originally designated the taurus ii, orbital sciences renamed the vehicle antares, after the star of the same name, on december 12, 2011.out of 17 total launches, antares has suffered one failure.launch pad 0a (lp-0a), previously used for the failed conestoga rocket, would be modified to handle antares.the first antares flight launched a cygnus mass simulator.on december 10, 2009, alliant techsystems inc. (atk) test-fired their castor 30 motor for use on the second stage of the antares rocket. |
66391 moshup , provisional designation 1999 kw4, is a binary asteroid, classified as a near-earth object and potentially hazardous asteroid of the aten group, approximately 1.3 kilometers in diameter.it was discovered on 20 may 1999, by lincoln near-earth asteroid research (linear) at the lincoln laboratory's experimental test site in socorro, new mexico, united states.it is a mercury-crosser that comes extremely close to the sun at a perihelion of 0.2 au.its orbit has an eccentricity of 0.69 and an inclination of 39° with respect to the ecliptic.a first precovery was taken by 2mass at the fred lawrence whipple observatory in 1998, extending the body's observation arc by one year prior to its official discovery observation at socorro.as a potentially hazardous asteroid, it has an earth minimum orbital intersection distance of 0.0138 au (2,060,000 km) which corresponds to 5.4 lunar distances.on 25 may 2036, it will pass 0.0155 au (2,320,000 km) from earth.it was named from mohegan legend, after moshup, a giant who lived in the coastal areas of new england.the asteroid's companion is named squannit, after the wife of moshup and a medicine woman of the makiawisug (little people).the official naming citation was published by the minor planet center on 27 august 2019 (m.p.c.115894).the moon, named squannit and designated s/2001 (66391) 1, is approximately 360 metres in diameter, and orbits its primary in every 16 hours at a mean-distance of 2.6 kilometers.the presence of a companion was suggested by photometric observations made by pravec and šarounová and was confirmed by radar observations from arecibo observations and announced on 23 may 2001 (also see below).based on radar imaging, squannit's dimensions are estimated to be 595 × 450 × 343 meters.the observations were taken from may 21–23, 2001, by lance a. m. benner, steven j. ostro, jon d. giorgini, raymond f. jurgens, jean-luc margot and michael c. nolan.the collaborative asteroid lightcurve link adopts a diameter of 1.3 kilometers and derives an albedo 0.26 with an absolute magnitude of 16.5.the shapes of the two bodies and their dynamics are complex.with a dimension of approximately 1.42 × 1.36 × 1.18 kilometers for a simple triaxial ellipsoid, the asteroid has an oblate shape, which is dominated by an equatorial ridge at the body's potential-energy minimum.this bizarre property of the equatorial region means that it is close to breakup: raising a particle a meter above the surface would put it into orbit.as seen in the image at above right, the gravitational effects between the moon and the asteroid create a gigantic mountain extending in the equatorial plane around the entire asteroid.it was the first asteroid to be described as 'muffin-shaped', which is now understood to be a very common shape for asteroids in critical rotation, including 101955 bennu and 162173 ryugu.lightcurve analysis gave a rotation period of 2.7650 hours with a brightness variation of 0.12 magnitude (u=3). | 66391 1999 kw4 | epoch | 2004-07-14 <tsp> 66391 1999 kw4 | escapevelocity | 0 <tsp> 66391 1999 kw4 | orbitalperiod | 162447000 <tsp> 66391 1999 kw4 | periapsis | 299196000000 <tsp> 66391 1999 kw4 | density | 20 grampercubiccentimetres | no related information |
antares (), known during early development as taurus ii, is an expendable launch system developed by orbital sciences corporation (now part of northrop grumman) and the pivdenne design bureau to launch the cygnus spacecraft to the international space station as part of nasa's cots and crs programs.able to launch payloads heavier than 8,000 kg (18,000 lb) into low earth orbit, antares is currently the largest rocket operated by northrop grumman.antares launches from the mid-atlantic regional spaceport and made its inaugural flight on april 21, 2013.nasa awarded orbital a commercial orbital transportation services (cots) space act agreement (saa) in 2008 to demonstrate delivery of cargo to the international space station.for these cots missions orbital intends to use antares to launch its cygnus spacecraft.in addition, antares will compete for small-to-medium missions.originally designated the taurus ii, orbital sciences renamed the vehicle antares, after the star of the same name, on december 12, 2011.out of 17 total launches, antares has suffered one failure.during the fifth launch on october 28, 2014, the rocket failed catastrophically, and the vehicle and payload were destroyed.the rocket's first-stage engines were identified as the cause for the failure.a different engine was chosen for subsequent launches, and the rocket had a successful return to flight on october 17, 2016.the antares has flown two major design iterations, the 100 series and 200 series.both series have used a castor 30xl as an upper stage but have differed on the first stage.the 100 series used two kerolox powered aj26 engine in the first stage and launched successfully four times.the 100 series was retired following a launch failure in 2014.the 200 series which first flew in 2016 also featured a kerolox first stage but instead used two rd-181 engine along with other minor upgrades.the 200 series future became uncertain following the russian invasion of ukraine.due to the first stage being produced in ukraine and the engines in russia, future production of the rocket was unable to be continued.as a result northrop grumman entered into an agreement with firefly aerospace to build the first stage of the antares 300 series.northrop also contracted with spacex for 3 falcon 9 launches.a commercial resupply service contract of $1.9 billion for eight flights was awarded in 2008.as of april 2012, development costs were estimated at $472 million.in june 2008, it was announced that the mid-atlantic regional spaceport, formerly part of the wallops flight facility, in virginia, would be the primary launch site for the rocket.launch pad 0a (lp-0a), previously used for the failed conestoga rocket, would be modified to handle antares.wallops allows launches which reach the international space station's orbit as effectively as those from cape canaveral, florida, while being less crowded.the first antares flight launched a cygnus mass simulator.on december 10, 2009, alliant techsystems inc. (atk) test-fired their castor 30 motor for use on the second stage of the antares rocket.in march 2010, orbital sciences and aerojet completed test firings of the aj-26 engines.on february 22, 2013, a hot fire test was successfully performed, the entire first stage being erected on the pad and held down while the engines fired for 29 seconds.as orbital had little experience with large liquid stages and lox propellant, the first stage core was designed and is manufactured in ukraine by kb pivdenne and pivdenmash and includes propellant tanks, pressurization tanks, valves, sensors, feed lines, tubing, wiring and other associated hardware.like the zenit—also manufactured by yuzhmash—the antares vehicle has a diameter of 3.9 m (150 in) with a matching 3.9 m payload fairing. | antares rocket | manufacturer | yuzhnoye design office <tsp> antares rocket | finalflight | 2014-07-13 <tsp> antares rocket | maidenflight | 2013-04-21 <tsp> antares rocket | launchsite | mid-atlantic regional spaceport launch pad 0 <tsp> antares rocket | diameter | 39 metres | antares (), known during early development as taurus ii, is an expendable launch system developed by orbital sciences corporation (now part of northrop grumman) and the pivdenne design bureau to launch the cygnus spacecraft to the international space station as part of nasa's cots and crs programs.able to launch payloads heavier than 8,000 kg (18,000 lb) into low earth orbit, antares is currently the largest rocket operated by northrop grumman.antares launches from the mid-atlantic regional spaceport and made its inaugural flight on april 21, 2013.nasa awarded orbital a commercial orbital transportation services (cots) space act agreement (saa) in 2008 to demonstrate delivery of cargo to the international space station.for these cots missions orbital intends to use antares to launch its cygnus spacecraft.originally designated the taurus ii, orbital sciences renamed the vehicle antares, after the star of the same name, on december 12, 2011.out of 17 total launches, antares has suffered one failure.the antares has flown two major design iterations, the 100 series and 200 series.launch pad 0a (lp-0a), previously used for the failed conestoga rocket, would be modified to handle antares.the first antares flight launched a cygnus mass simulator.on december 10, 2009, alliant techsystems inc. (atk) test-fired their castor 30 motor for use on the second stage of the antares rocket. |
66391 moshup , provisional designation 1999 kw4, is a binary asteroid, classified as a near-earth object and potentially hazardous asteroid of the aten group, approximately 1.3 kilometers in diameter.it was discovered on 20 may 1999, by lincoln near-earth asteroid research (linear) at the lincoln laboratory's experimental test site in socorro, new mexico, united states.it is a mercury-crosser that comes extremely close to the sun at a perihelion of 0.2 au.its orbit has an eccentricity of 0.69 and an inclination of 39° with respect to the ecliptic.a first precovery was taken by 2mass at the fred lawrence whipple observatory in 1998, extending the body's observation arc by one year prior to its official discovery observation at socorro.as a potentially hazardous asteroid, it has an earth minimum orbital intersection distance of 0.0138 au (2,060,000 km) which corresponds to 5.4 lunar distances.on 25 may 2036, it will pass 0.0155 au (2,320,000 km) from earth.it was named from mohegan legend, after moshup, a giant who lived in the coastal areas of new england.the asteroid's companion is named squannit, after the wife of moshup and a medicine woman of the makiawisug (little people).the official naming citation was published by the minor planet center on 27 august 2019 (m.p.c.115894).the moon, named squannit and designated s/2001 (66391) 1, is approximately 360 metres in diameter, and orbits its primary in every 16 hours at a mean-distance of 2.6 kilometers.the presence of a companion was suggested by photometric observations made by pravec and šarounová and was confirmed by radar observations from arecibo observations and announced on 23 may 2001 (also see below).based on radar imaging, squannit's dimensions are estimated to be 595 × 450 × 343 meters.the observations were taken from may 21–23, 2001, by lance a. m. benner, steven j. ostro, jon d. giorgini, raymond f. jurgens, jean-luc margot and michael c. nolan.the collaborative asteroid lightcurve link adopts a diameter of 1.3 kilometers and derives an albedo 0.26 with an absolute magnitude of 16.5.the shapes of the two bodies and their dynamics are complex.with a dimension of approximately 1.42 × 1.36 × 1.18 kilometers for a simple triaxial ellipsoid, the asteroid has an oblate shape, which is dominated by an equatorial ridge at the body's potential-energy minimum.this bizarre property of the equatorial region means that it is close to breakup: raising a particle a meter above the surface would put it into orbit.as seen in the image at above right, the gravitational effects between the moon and the asteroid create a gigantic mountain extending in the equatorial plane around the entire asteroid.it was the first asteroid to be described as 'muffin-shaped', which is now understood to be a very common shape for asteroids in critical rotation, including 101955 bennu and 162173 ryugu.lightcurve analysis gave a rotation period of 2.7650 hours with a brightness variation of 0.12 magnitude (u=3). | 66391 1999 kw4 | epoch | 2004-07-14 <tsp> 66391 1999 kw4 | orbitalperiod | 162447000 <tsp> 66391 1999 kw4 | periapsis | 299196000000 <tsp> 66391 1999 kw4 | escapevelocity | 0 <tsp> 66391 1999 kw4 | apoapsis | 1621640918388 kilometres | no related information |
aaron bertram (born april 3, 1981, in lubbock, texas) is a trumpet player for third wave ska band suburban legends, and member of the children's music group kids imagine nation.in the past he has taught music and movement to preschool students in orange county, ca.his music program was called little rockstars.he launched an online streaming service for children's entertainment and arts education called kintv in march of 2020, where he currently performs and teaches music.he was a trumpet player for the third-wave ska band suburban legends from the band's origin in 1998 to may 2005, when he left to start his company, kids imagine with wife, rachel charest.he was known for doing a lot of backing vocals in the band and originated the idea of the band's signature choreography.aaron returned for a final performance with the band on november 29, 2005, at huntington beach high school for a benefit show for the ryan dallas cook memorial fund.since the summer of 2009, aaron has been performing with suburban legends at local shows.as of november 2010, he is listed as an official member of the band.in addition to playing trumpet for suburban legends, he also performed vocals for the band's cover of the gummi bears theme song, the band's cover of rose tint my world and the song powerful game on the album rump shaker.aaron is currently writing children's music under the name kids imagine nation with rachel charest and vince walker. | aaron bertram | associatedband/associatedmusicalartist | suburban legends <tsp> aaron bertram | birthdate | 1981-04-03 <tsp> aaron bertram | genre | ska punk <tsp> aaron bertram | activeyearsstartyear | 1998 <tsp> aaron bertram | associatedband/associatedmusicalartist | kids imagine nation | aaron bertram (born april 3, 1981, in lubbock, texas) is a trumpet player for third wave ska band suburban legends, and member of the children's music group kids imagine nation.since the summer of 2009, aaron has been performing with suburban legends at local shows.aaron is currently writing children's music under the name kids imagine nation with rachel charest and vince walker. |
66391 moshup , provisional designation 1999 kw4, is a binary asteroid, classified as a near-earth object and potentially hazardous asteroid of the aten group, approximately 1.3 kilometers in diameter.it was discovered on 20 may 1999, by lincoln near-earth asteroid research (linear) at the lincoln laboratory's experimental test site in socorro, new mexico, united states.it is a mercury-crosser that comes extremely close to the sun at a perihelion of 0.2 au.its orbit has an eccentricity of 0.69 and an inclination of 39° with respect to the ecliptic.a first precovery was taken by 2mass at the fred lawrence whipple observatory in 1998, extending the body's observation arc by one year prior to its official discovery observation at socorro.as a potentially hazardous asteroid, it has an earth minimum orbital intersection distance of 0.0138 au (2,060,000 km) which corresponds to 5.4 lunar distances.on 25 may 2036, it will pass 0.0155 au (2,320,000 km) from earth.it was named from mohegan legend, after moshup, a giant who lived in the coastal areas of new england.the asteroid's companion is named squannit, after the wife of moshup and a medicine woman of the makiawisug (little people).the official naming citation was published by the minor planet center on 27 august 2019 (m.p.c.115894).the moon, named squannit and designated s/2001 (66391) 1, is approximately 360 metres in diameter, and orbits its primary in every 16 hours at a mean-distance of 2.6 kilometers.the presence of a companion was suggested by photometric observations made by pravec and šarounová and was confirmed by radar observations from arecibo observations and announced on 23 may 2001 (also see below).based on radar imaging, squannit's dimensions are estimated to be 595 × 450 × 343 meters.the observations were taken from may 21–23, 2001, by lance a. m. benner, steven j. ostro, jon d. giorgini, raymond f. jurgens, jean-luc margot and michael c. nolan.the collaborative asteroid lightcurve link adopts a diameter of 1.3 kilometers and derives an albedo 0.26 with an absolute magnitude of 16.5.the shapes of the two bodies and their dynamics are complex.with a dimension of approximately 1.42 × 1.36 × 1.18 kilometers for a simple triaxial ellipsoid, the asteroid has an oblate shape, which is dominated by an equatorial ridge at the body's potential-energy minimum.this bizarre property of the equatorial region means that it is close to breakup: raising a particle a meter above the surface would put it into orbit.as seen in the image at above right, the gravitational effects between the moon and the asteroid create a gigantic mountain extending in the equatorial plane around the entire asteroid.it was the first asteroid to be described as 'muffin-shaped', which is now understood to be a very common shape for asteroids in critical rotation, including 101955 bennu and 162173 ryugu.lightcurve analysis gave a rotation period of 2.7650 hours with a brightness variation of 0.12 magnitude (u=3). | 66391 1999 kw4 | epoch | 2004-07-14 <tsp> 66391 1999 kw4 | orbitalperiod | 162447000 <tsp> 66391 1999 kw4 | periapsis | 299196000000 <tsp> 66391 1999 kw4 | escapevelocity | 0 <tsp> 66391 1999 kw4 | apoapsis | 1621640918388 kilometres | no related information |
aaron bertram (born april 3, 1981, in lubbock, texas) is a trumpet player for third wave ska band suburban legends, and member of the children's music group kids imagine nation.in the past he has taught music and movement to preschool students in orange county, ca.his music program was called little rockstars.he launched an online streaming service for children's entertainment and arts education called kintv in march of 2020, where he currently performs and teaches music.he was a trumpet player for the third-wave ska band suburban legends from the band's origin in 1998 to may 2005, when he left to start his company, kids imagine with wife, rachel charest.he was known for doing a lot of backing vocals in the band and originated the idea of the band's signature choreography.aaron returned for a final performance with the band on november 29, 2005, at huntington beach high school for a benefit show for the ryan dallas cook memorial fund.since the summer of 2009, aaron has been performing with suburban legends at local shows.as of november 2010, he is listed as an official member of the band.in addition to playing trumpet for suburban legends, he also performed vocals for the band's cover of the gummi bears theme song, the band's cover of rose tint my world and the song powerful game on the album rump shaker.aaron is currently writing children's music under the name kids imagine nation with rachel charest and vince walker. | aaron bertram | associatedband/associatedmusicalartist | suburban legends <tsp> aaron bertram | birthdate | 1981-04-03 <tsp> aaron bertram | genre | ska punk <tsp> aaron bertram | activeyearsstartyear | 1998 <tsp> aaron bertram | associatedband/associatedmusicalartist | kids imagine nation | aaron bertram (born april 3, 1981, in lubbock, texas) is a trumpet player for third wave ska band suburban legends, and member of the children's music group kids imagine nation.since the summer of 2009, aaron has been performing with suburban legends at local shows.aaron is currently writing children's music under the name kids imagine nation with rachel charest and vince walker. |
antares (), known during early development as taurus ii, is an expendable launch system developed by orbital sciences corporation (now part of northrop grumman) and the pivdenne design bureau to launch the cygnus spacecraft to the international space station as part of nasa's cots and crs programs.able to launch payloads heavier than 8,000 kg (18,000 lb) into low earth orbit, antares is currently the largest rocket operated by northrop grumman.antares launches from the mid-atlantic regional spaceport and made its inaugural flight on april 21, 2013.nasa awarded orbital a commercial orbital transportation services (cots) space act agreement (saa) in 2008 to demonstrate delivery of cargo to the international space station.for these cots missions orbital intends to use antares to launch its cygnus spacecraft.in addition, antares will compete for small-to-medium missions.originally designated the taurus ii, orbital sciences renamed the vehicle antares, after the star of the same name, on december 12, 2011.out of 17 total launches, antares has suffered one failure.during the fifth launch on october 28, 2014, the rocket failed catastrophically, and the vehicle and payload were destroyed.the rocket's first-stage engines were identified as the cause for the failure.a different engine was chosen for subsequent launches, and the rocket had a successful return to flight on october 17, 2016.the antares has flown two major design iterations, the 100 series and 200 series.both series have used a castor 30xl as an upper stage but have differed on the first stage.the 100 series used two kerolox powered aj26 engine in the first stage and launched successfully four times.the 100 series was retired following a launch failure in 2014.the 200 series which first flew in 2016 also featured a kerolox first stage but instead used two rd-181 engine along with other minor upgrades.the 200 series future became uncertain following the russian invasion of ukraine.due to the first stage being produced in ukraine and the engines in russia, future production of the rocket was unable to be continued.as a result northrop grumman entered into an agreement with firefly aerospace to build the first stage of the antares 300 series.northrop also contracted with spacex for 3 falcon 9 launches.a commercial resupply service contract of $1.9 billion for eight flights was awarded in 2008.as of april 2012, development costs were estimated at $472 million.in june 2008, it was announced that the mid-atlantic regional spaceport, formerly part of the wallops flight facility, in virginia, would be the primary launch site for the rocket.launch pad 0a (lp-0a), previously used for the failed conestoga rocket, would be modified to handle antares.wallops allows launches which reach the international space station's orbit as effectively as those from cape canaveral, florida, while being less crowded.the first antares flight launched a cygnus mass simulator.on december 10, 2009, alliant techsystems inc. (atk) test-fired their castor 30 motor for use on the second stage of the antares rocket.in march 2010, orbital sciences and aerojet completed test firings of the aj-26 engines.on february 22, 2013, a hot fire test was successfully performed, the entire first stage being erected on the pad and held down while the engines fired for 29 seconds.as orbital had little experience with large liquid stages and lox propellant, the first stage core was designed and is manufactured in ukraine by kb pivdenne and pivdenmash and includes propellant tanks, pressurization tanks, valves, sensors, feed lines, tubing, wiring and other associated hardware.like the zenit—also manufactured by yuzhmash—the antares vehicle has a diameter of 3.9 m (150 in) with a matching 3.9 m payload fairing. | antares rocket | manufacturer | yuzhnoye design office <tsp> antares rocket | finalflight | 2014-07-13 <tsp> antares rocket | maidenflight | 2013-04-21 <tsp> antares rocket | launchsite | mid-atlantic regional spaceport launch pad 0 <tsp> antares rocket | diameter | 39 metres | antares (), known during early development as taurus ii, is an expendable launch system developed by orbital sciences corporation (now part of northrop grumman) and the pivdenne design bureau to launch the cygnus spacecraft to the international space station as part of nasa's cots and crs programs.able to launch payloads heavier than 8,000 kg (18,000 lb) into low earth orbit, antares is currently the largest rocket operated by northrop grumman.antares launches from the mid-atlantic regional spaceport and made its inaugural flight on april 21, 2013.nasa awarded orbital a commercial orbital transportation services (cots) space act agreement (saa) in 2008 to demonstrate delivery of cargo to the international space station.for these cots missions orbital intends to use antares to launch its cygnus spacecraft.originally designated the taurus ii, orbital sciences renamed the vehicle antares, after the star of the same name, on december 12, 2011.out of 17 total launches, antares has suffered one failure.the antares has flown two major design iterations, the 100 series and 200 series.launch pad 0a (lp-0a), previously used for the failed conestoga rocket, would be modified to handle antares.the first antares flight launched a cygnus mass simulator.on december 10, 2009, alliant techsystems inc. (atk) test-fired their castor 30 motor for use on the second stage of the antares rocket. |
66391 moshup , provisional designation 1999 kw4, is a binary asteroid, classified as a near-earth object and potentially hazardous asteroid of the aten group, approximately 1.3 kilometers in diameter.it was discovered on 20 may 1999, by lincoln near-earth asteroid research (linear) at the lincoln laboratory's experimental test site in socorro, new mexico, united states.it is a mercury-crosser that comes extremely close to the sun at a perihelion of 0.2 au.its orbit has an eccentricity of 0.69 and an inclination of 39° with respect to the ecliptic.a first precovery was taken by 2mass at the fred lawrence whipple observatory in 1998, extending the body's observation arc by one year prior to its official discovery observation at socorro.as a potentially hazardous asteroid, it has an earth minimum orbital intersection distance of 0.0138 au (2,060,000 km) which corresponds to 5.4 lunar distances.on 25 may 2036, it will pass 0.0155 au (2,320,000 km) from earth.it was named from mohegan legend, after moshup, a giant who lived in the coastal areas of new england.the asteroid's companion is named squannit, after the wife of moshup and a medicine woman of the makiawisug (little people).the official naming citation was published by the minor planet center on 27 august 2019 (m.p.c.115894).the moon, named squannit and designated s/2001 (66391) 1, is approximately 360 metres in diameter, and orbits its primary in every 16 hours at a mean-distance of 2.6 kilometers.the presence of a companion was suggested by photometric observations made by pravec and šarounová and was confirmed by radar observations from arecibo observations and announced on 23 may 2001 (also see below).based on radar imaging, squannit's dimensions are estimated to be 595 × 450 × 343 meters.the observations were taken from may 21–23, 2001, by lance a. m. benner, steven j. ostro, jon d. giorgini, raymond f. jurgens, jean-luc margot and michael c. nolan.the collaborative asteroid lightcurve link adopts a diameter of 1.3 kilometers and derives an albedo 0.26 with an absolute magnitude of 16.5.the shapes of the two bodies and their dynamics are complex.with a dimension of approximately 1.42 × 1.36 × 1.18 kilometers for a simple triaxial ellipsoid, the asteroid has an oblate shape, which is dominated by an equatorial ridge at the body's potential-energy minimum.this bizarre property of the equatorial region means that it is close to breakup: raising a particle a meter above the surface would put it into orbit.as seen in the image at above right, the gravitational effects between the moon and the asteroid create a gigantic mountain extending in the equatorial plane around the entire asteroid.it was the first asteroid to be described as 'muffin-shaped', which is now understood to be a very common shape for asteroids in critical rotation, including 101955 bennu and 162173 ryugu.lightcurve analysis gave a rotation period of 2.7650 hours with a brightness variation of 0.12 magnitude (u=3). | 66391 1999 kw4 | epoch | 2004-07-14 <tsp> 66391 1999 kw4 | orbitalperiod | 162447000 <tsp> 66391 1999 kw4 | periapsis | 299196000000 <tsp> 66391 1999 kw4 | escapevelocity | 0 <tsp> 66391 1999 kw4 | apoapsis | 1621640918388 kilometres | no related information |
aaron bertram (born april 3, 1981, in lubbock, texas) is a trumpet player for third wave ska band suburban legends, and member of the children's music group kids imagine nation.in the past he has taught music and movement to preschool students in orange county, ca.his music program was called little rockstars.he launched an online streaming service for children's entertainment and arts education called kintv in march of 2020, where he currently performs and teaches music.he was a trumpet player for the third-wave ska band suburban legends from the band's origin in 1998 to may 2005, when he left to start his company, kids imagine with wife, rachel charest.he was known for doing a lot of backing vocals in the band and originated the idea of the band's signature choreography.aaron returned for a final performance with the band on november 29, 2005, at huntington beach high school for a benefit show for the ryan dallas cook memorial fund.since the summer of 2009, aaron has been performing with suburban legends at local shows.as of november 2010, he is listed as an official member of the band.in addition to playing trumpet for suburban legends, he also performed vocals for the band's cover of the gummi bears theme song, the band's cover of rose tint my world and the song powerful game on the album rump shaker.aaron is currently writing children's music under the name kids imagine nation with rachel charest and vince walker. | pronto | camenae | bursas | no related information |
1000 piazzia, provisional designation 1923 nz, is a carbonaceous background asteroid from the outer region of the asteroid belt, approximately 48 kilometers (30 miles) in diameter.it was discovered on 12 august 1923, by german astronomer karl reinmuth at heidelberg observatory in southern germany.the c-type asteroid has a rotation period of 9.5 hours.it was named after italian giuseppe piazzi, who discovered 1 ceres.it orbits the sun in the outer asteroid belt at a distance of 2.4–4.0 au once every 5 years and 8 months (2,063 days; semi-major axis of 3.17 au).its orbit has an eccentricity of 0.26 and an inclination of 21° with respect to the ecliptic.as no precoveries were taken, the body's observation arc begins with its first recorded observation on the night following its official discovery date.he was a director of both the palermo and naples observatories, and known for the compilation of the palermo catalogue, containing the precise position of 7,646 stars.in 1801, piazzi discovered 1 ceres, the first and largest asteroid and the main-belt's only dwarf planet.he is also honored by the lunar crater piazzi.the official naming citation was first mentioned in the names of the minor planets by paul herget in 1955 (h 96).the asteroid is the first of several early 'kilo-numbered' minor planets that were dedicated to renowned scientists or institutions including: 2000 herschel, for william herschel who discovered uranus 3000 leonardo, for the italian polymath of the renaissance, leonardo da vinci 4000 hipparchus, for the ancient greek astronomer hipparchusthese are followed by the asteroids 5000 iau (for the international astronomical union), 6000 united nations (for the united nations), 7000 curie (for the pioneers on radioactivity, marie and pierre curie), and 8000 isaac newton (for isaac newton), while 9000 hal (after hal 9000 from the movie 2001: a space odyssey) and 10000 myriostos (after the greek word for ten-thousandth, and to honor all astronomers) were named based on their direct numeric accordance.1000 piazzia was named as part of trio honoring the events surrounding the discovery of ceres in 1801.a person named carl friedrich gauss who computed the orbit of ceres, and heinrich wilhelm matthias olbers who found it again later that year after it has passed behind the sun.in honor of them, 1001 gaussia for gauss and 1002 olbersia for olbers were named along with 1000 piazzia.in the next few years only three more astronomical bodies were found between mars and jupiter, pallas, juno, and 4 vesta, however it would be 37 years before another asteroid was found, 5 astraea in 1845.by 1868, 100 asteroids had been discovered, however it would not be until 1921 that the 1000th was discovered.the rate accelerated in the 20th century and the ten thousandth would be discovered in 1989.the lightcurve gave a rotation period of 9.47±0.01 hours with a brightness variation of 0.45 magnitude (u=3).a second lightcurve was obtained by astronomer rené roy in march 2007, rendering a period of 9.2±0.2 hours and an amplitude of 0.2 magnitude (u=2).according to the space-based surveys carried out by the infrared astronomical satellite iras, the japanese akari satellite and the neowise mission of nasa's wide-field infrared survey explorer, piazzia measures between 45.72 and 51.55 kilometers in diameter and its surface has an albedo between 0.041 and 0.1119. | 1000 piazzia | epoch | 2015-06-27 <tsp> 1000 piazzia | escapevelocity | 00252 kilometreperseconds <tsp> 1000 piazzia | formername | 1923 nz1951 ob <tsp> 1000 piazzia | orbitalperiod | 4881600 <tsp> 1000 piazzia | periapsis | 3524970000000 | 1000 piazzia, provisional designation 1923 nz, is a carbonaceous background asteroid from the outer region of the asteroid belt, approximately 48 kilometers (30 miles) in diameter. |
antares (), known during early development as taurus ii, is an expendable launch system developed by orbital sciences corporation (now part of northrop grumman) and the pivdenne design bureau to launch the cygnus spacecraft to the international space station as part of nasa's cots and crs programs.able to launch payloads heavier than 8,000 kg (18,000 lb) into low earth orbit, antares is currently the largest rocket operated by northrop grumman.antares launches from the mid-atlantic regional spaceport and made its inaugural flight on april 21, 2013.nasa awarded orbital a commercial orbital transportation services (cots) space act agreement (saa) in 2008 to demonstrate delivery of cargo to the international space station.for these cots missions orbital intends to use antares to launch its cygnus spacecraft.in addition, antares will compete for small-to-medium missions.originally designated the taurus ii, orbital sciences renamed the vehicle antares, after the star of the same name, on december 12, 2011.out of 17 total launches, antares has suffered one failure.during the fifth launch on october 28, 2014, the rocket failed catastrophically, and the vehicle and payload were destroyed.the rocket's first-stage engines were identified as the cause for the failure.a different engine was chosen for subsequent launches, and the rocket had a successful return to flight on october 17, 2016.the antares has flown two major design iterations, the 100 series and 200 series.both series have used a castor 30xl as an upper stage but have differed on the first stage.the 100 series used two kerolox powered aj26 engine in the first stage and launched successfully four times.the 100 series was retired following a launch failure in 2014.the 200 series which first flew in 2016 also featured a kerolox first stage but instead used two rd-181 engine along with other minor upgrades.the 200 series future became uncertain following the russian invasion of ukraine.due to the first stage being produced in ukraine and the engines in russia, future production of the rocket was unable to be continued.as a result northrop grumman entered into an agreement with firefly aerospace to build the first stage of the antares 300 series.northrop also contracted with spacex for 3 falcon 9 launches.a commercial resupply service contract of $1.9 billion for eight flights was awarded in 2008.as of april 2012, development costs were estimated at $472 million.in june 2008, it was announced that the mid-atlantic regional spaceport, formerly part of the wallops flight facility, in virginia, would be the primary launch site for the rocket.launch pad 0a (lp-0a), previously used for the failed conestoga rocket, would be modified to handle antares.wallops allows launches which reach the international space station's orbit as effectively as those from cape canaveral, florida, while being less crowded.the first antares flight launched a cygnus mass simulator.on december 10, 2009, alliant techsystems inc. (atk) test-fired their castor 30 motor for use on the second stage of the antares rocket.in march 2010, orbital sciences and aerojet completed test firings of the aj-26 engines.on february 22, 2013, a hot fire test was successfully performed, the entire first stage being erected on the pad and held down while the engines fired for 29 seconds.as orbital had little experience with large liquid stages and lox propellant, the first stage core was designed and is manufactured in ukraine by kb pivdenne and pivdenmash and includes propellant tanks, pressurization tanks, valves, sensors, feed lines, tubing, wiring and other associated hardware.like the zenit—also manufactured by yuzhmash—the antares vehicle has a diameter of 3.9 m (150 in) with a matching 3.9 m payload fairing. | cardiosclerosis | song | chaetosoma | no related information |
aaron bertram (born april 3, 1981, in lubbock, texas) is a trumpet player for third wave ska band suburban legends, and member of the children's music group kids imagine nation.in the past he has taught music and movement to preschool students in orange county, ca.his music program was called little rockstars.he launched an online streaming service for children's entertainment and arts education called kintv in march of 2020, where he currently performs and teaches music.he was a trumpet player for the third-wave ska band suburban legends from the band's origin in 1998 to may 2005, when he left to start his company, kids imagine with wife, rachel charest.he was known for doing a lot of backing vocals in the band and originated the idea of the band's signature choreography.aaron returned for a final performance with the band on november 29, 2005, at huntington beach high school for a benefit show for the ryan dallas cook memorial fund.since the summer of 2009, aaron has been performing with suburban legends at local shows.as of november 2010, he is listed as an official member of the band.in addition to playing trumpet for suburban legends, he also performed vocals for the band's cover of the gummi bears theme song, the band's cover of rose tint my world and the song powerful game on the album rump shaker.aaron is currently writing children's music under the name kids imagine nation with rachel charest and vince walker. | aaron bertram | associatedband/associatedmusicalartist | suburban legends <tsp> aaron bertram | genre | ska punk <tsp> aaron bertram | activeyearsstartyear | 1998 <tsp> aaron bertram | associatedband/associatedmusicalartist | kids imagine nation <tsp> aaron bertram | background | non vocal instrumentalist | aaron bertram (born april 3, 1981, in lubbock, texas) is a trumpet player for third wave ska band suburban legends, and member of the children's music group kids imagine nation.since the summer of 2009, aaron has been performing with suburban legends at local shows.aaron is currently writing children's music under the name kids imagine nation with rachel charest and vince walker. |
1000 piazzia, provisional designation 1923 nz, is a carbonaceous background asteroid from the outer region of the asteroid belt, approximately 48 kilometers (30 miles) in diameter.it was discovered on 12 august 1923, by german astronomer karl reinmuth at heidelberg observatory in southern germany.the c-type asteroid has a rotation period of 9.5 hours.it was named after italian giuseppe piazzi, who discovered 1 ceres.it orbits the sun in the outer asteroid belt at a distance of 2.4–4.0 au once every 5 years and 8 months (2,063 days; semi-major axis of 3.17 au).its orbit has an eccentricity of 0.26 and an inclination of 21° with respect to the ecliptic.as no precoveries were taken, the body's observation arc begins with its first recorded observation on the night following its official discovery date.he was a director of both the palermo and naples observatories, and known for the compilation of the palermo catalogue, containing the precise position of 7,646 stars.in 1801, piazzi discovered 1 ceres, the first and largest asteroid and the main-belt's only dwarf planet.he is also honored by the lunar crater piazzi.the official naming citation was first mentioned in the names of the minor planets by paul herget in 1955 (h 96).the asteroid is the first of several early 'kilo-numbered' minor planets that were dedicated to renowned scientists or institutions including: 2000 herschel, for william herschel who discovered uranus 3000 leonardo, for the italian polymath of the renaissance, leonardo da vinci 4000 hipparchus, for the ancient greek astronomer hipparchusthese are followed by the asteroids 5000 iau (for the international astronomical union), 6000 united nations (for the united nations), 7000 curie (for the pioneers on radioactivity, marie and pierre curie), and 8000 isaac newton (for isaac newton), while 9000 hal (after hal 9000 from the movie 2001: a space odyssey) and 10000 myriostos (after the greek word for ten-thousandth, and to honor all astronomers) were named based on their direct numeric accordance.1000 piazzia was named as part of trio honoring the events surrounding the discovery of ceres in 1801.a person named carl friedrich gauss who computed the orbit of ceres, and heinrich wilhelm matthias olbers who found it again later that year after it has passed behind the sun.in honor of them, 1001 gaussia for gauss and 1002 olbersia for olbers were named along with 1000 piazzia.in the next few years only three more astronomical bodies were found between mars and jupiter, pallas, juno, and 4 vesta, however it would be 37 years before another asteroid was found, 5 astraea in 1845.by 1868, 100 asteroids had been discovered, however it would not be until 1921 that the 1000th was discovered.the rate accelerated in the 20th century and the ten thousandth would be discovered in 1989.the lightcurve gave a rotation period of 9.47±0.01 hours with a brightness variation of 0.45 magnitude (u=3).a second lightcurve was obtained by astronomer rené roy in march 2007, rendering a period of 9.2±0.2 hours and an amplitude of 0.2 magnitude (u=2).according to the space-based surveys carried out by the infrared astronomical satellite iras, the japanese akari satellite and the neowise mission of nasa's wide-field infrared survey explorer, piazzia measures between 45.72 and 51.55 kilometers in diameter and its surface has an albedo between 0.041 and 0.1119. | 1000 piazzia | epoch | 2015-06-27 <tsp> 1000 piazzia | escapevelocity | 00252 kilometreperseconds <tsp> 1000 piazzia | formername | 1923 nz1951 ob <tsp> 1000 piazzia | orbitalperiod | 4881600 <tsp> 1000 piazzia | periapsis | 3524970000000 | 1000 piazzia, provisional designation 1923 nz, is a carbonaceous background asteroid from the outer region of the asteroid belt, approximately 48 kilometers (30 miles) in diameter. |
antares (), known during early development as taurus ii, is an expendable launch system developed by orbital sciences corporation (now part of northrop grumman) and the pivdenne design bureau to launch the cygnus spacecraft to the international space station as part of nasa's cots and crs programs.able to launch payloads heavier than 8,000 kg (18,000 lb) into low earth orbit, antares is currently the largest rocket operated by northrop grumman.antares launches from the mid-atlantic regional spaceport and made its inaugural flight on april 21, 2013.nasa awarded orbital a commercial orbital transportation services (cots) space act agreement (saa) in 2008 to demonstrate delivery of cargo to the international space station.for these cots missions orbital intends to use antares to launch its cygnus spacecraft.in addition, antares will compete for small-to-medium missions.originally designated the taurus ii, orbital sciences renamed the vehicle antares, after the star of the same name, on december 12, 2011.out of 17 total launches, antares has suffered one failure.during the fifth launch on october 28, 2014, the rocket failed catastrophically, and the vehicle and payload were destroyed.the rocket's first-stage engines were identified as the cause for the failure.a different engine was chosen for subsequent launches, and the rocket had a successful return to flight on october 17, 2016.the antares has flown two major design iterations, the 100 series and 200 series.both series have used a castor 30xl as an upper stage but have differed on the first stage.the 100 series used two kerolox powered aj26 engine in the first stage and launched successfully four times.the 100 series was retired following a launch failure in 2014.the 200 series which first flew in 2016 also featured a kerolox first stage but instead used two rd-181 engine along with other minor upgrades.the 200 series future became uncertain following the russian invasion of ukraine.due to the first stage being produced in ukraine and the engines in russia, future production of the rocket was unable to be continued.as a result northrop grumman entered into an agreement with firefly aerospace to build the first stage of the antares 300 series.northrop also contracted with spacex for 3 falcon 9 launches.a commercial resupply service contract of $1.9 billion for eight flights was awarded in 2008.as of april 2012, development costs were estimated at $472 million.in june 2008, it was announced that the mid-atlantic regional spaceport, formerly part of the wallops flight facility, in virginia, would be the primary launch site for the rocket.launch pad 0a (lp-0a), previously used for the failed conestoga rocket, would be modified to handle antares.wallops allows launches which reach the international space station's orbit as effectively as those from cape canaveral, florida, while being less crowded.the first antares flight launched a cygnus mass simulator.on december 10, 2009, alliant techsystems inc. (atk) test-fired their castor 30 motor for use on the second stage of the antares rocket.in march 2010, orbital sciences and aerojet completed test firings of the aj-26 engines.on february 22, 2013, a hot fire test was successfully performed, the entire first stage being erected on the pad and held down while the engines fired for 29 seconds.as orbital had little experience with large liquid stages and lox propellant, the first stage core was designed and is manufactured in ukraine by kb pivdenne and pivdenmash and includes propellant tanks, pressurization tanks, valves, sensors, feed lines, tubing, wiring and other associated hardware.like the zenit—also manufactured by yuzhmash—the antares vehicle has a diameter of 3.9 m (150 in) with a matching 3.9 m payload fairing. | antares rocket | manufacturer | yuzhnoye design office <tsp> antares rocket | finalflight | 2014-07-13 <tsp> antares rocket | maidenflight | 2014-01-09 <tsp> antares rocket | launchsite | mid-atlantic regional spaceport launch pad 0 <tsp> antares rocket | diameter | 39 metres | antares (), known during early development as taurus ii, is an expendable launch system developed by orbital sciences corporation (now part of northrop grumman) and the pivdenne design bureau to launch the cygnus spacecraft to the international space station as part of nasa's cots and crs programs.able to launch payloads heavier than 8,000 kg (18,000 lb) into low earth orbit, antares is currently the largest rocket operated by northrop grumman.antares launches from the mid-atlantic regional spaceport and made its inaugural flight on april 21, 2013.nasa awarded orbital a commercial orbital transportation services (cots) space act agreement (saa) in 2008 to demonstrate delivery of cargo to the international space station.for these cots missions orbital intends to use antares to launch its cygnus spacecraft.originally designated the taurus ii, orbital sciences renamed the vehicle antares, after the star of the same name, on december 12, 2011.out of 17 total launches, antares has suffered one failure.the antares has flown two major design iterations, the 100 series and 200 series.launch pad 0a (lp-0a), previously used for the failed conestoga rocket, would be modified to handle antares.the first antares flight launched a cygnus mass simulator.on december 10, 2009, alliant techsystems inc. (atk) test-fired their castor 30 motor for use on the second stage of the antares rocket. |
aaron bertram (born april 3, 1981, in lubbock, texas) is a trumpet player for third wave ska band suburban legends, and member of the children's music group kids imagine nation.in the past he has taught music and movement to preschool students in orange county, ca.his music program was called little rockstars.he launched an online streaming service for children's entertainment and arts education called kintv in march of 2020, where he currently performs and teaches music.he was a trumpet player for the third-wave ska band suburban legends from the band's origin in 1998 to may 2005, when he left to start his company, kids imagine with wife, rachel charest.he was known for doing a lot of backing vocals in the band and originated the idea of the band's signature choreography.aaron returned for a final performance with the band on november 29, 2005, at huntington beach high school for a benefit show for the ryan dallas cook memorial fund.since the summer of 2009, aaron has been performing with suburban legends at local shows.as of november 2010, he is listed as an official member of the band.in addition to playing trumpet for suburban legends, he also performed vocals for the band's cover of the gummi bears theme song, the band's cover of rose tint my world and the song powerful game on the album rump shaker.aaron is currently writing children's music under the name kids imagine nation with rachel charest and vince walker. | loculicidal | blowze | photopitometer | no related information |
1000 piazzia, provisional designation 1923 nz, is a carbonaceous background asteroid from the outer region of the asteroid belt, approximately 48 kilometers (30 miles) in diameter.it was discovered on 12 august 1923, by german astronomer karl reinmuth at heidelberg observatory in southern germany.the c-type asteroid has a rotation period of 9.5 hours.it was named after italian giuseppe piazzi, who discovered 1 ceres.it orbits the sun in the outer asteroid belt at a distance of 2.4–4.0 au once every 5 years and 8 months (2,063 days; semi-major axis of 3.17 au).its orbit has an eccentricity of 0.26 and an inclination of 21° with respect to the ecliptic.as no precoveries were taken, the body's observation arc begins with its first recorded observation on the night following its official discovery date.he was a director of both the palermo and naples observatories, and known for the compilation of the palermo catalogue, containing the precise position of 7,646 stars.in 1801, piazzi discovered 1 ceres, the first and largest asteroid and the main-belt's only dwarf planet.he is also honored by the lunar crater piazzi.the official naming citation was first mentioned in the names of the minor planets by paul herget in 1955 (h 96).the asteroid is the first of several early 'kilo-numbered' minor planets that were dedicated to renowned scientists or institutions including: 2000 herschel, for william herschel who discovered uranus 3000 leonardo, for the italian polymath of the renaissance, leonardo da vinci 4000 hipparchus, for the ancient greek astronomer hipparchusthese are followed by the asteroids 5000 iau (for the international astronomical union), 6000 united nations (for the united nations), 7000 curie (for the pioneers on radioactivity, marie and pierre curie), and 8000 isaac newton (for isaac newton), while 9000 hal (after hal 9000 from the movie 2001: a space odyssey) and 10000 myriostos (after the greek word for ten-thousandth, and to honor all astronomers) were named based on their direct numeric accordance.1000 piazzia was named as part of trio honoring the events surrounding the discovery of ceres in 1801.a person named carl friedrich gauss who computed the orbit of ceres, and heinrich wilhelm matthias olbers who found it again later that year after it has passed behind the sun.in honor of them, 1001 gaussia for gauss and 1002 olbersia for olbers were named along with 1000 piazzia.in the next few years only three more astronomical bodies were found between mars and jupiter, pallas, juno, and 4 vesta, however it would be 37 years before another asteroid was found, 5 astraea in 1845.by 1868, 100 asteroids had been discovered, however it would not be until 1921 that the 1000th was discovered.the rate accelerated in the 20th century and the ten thousandth would be discovered in 1989.the lightcurve gave a rotation period of 9.47±0.01 hours with a brightness variation of 0.45 magnitude (u=3).a second lightcurve was obtained by astronomer rené roy in march 2007, rendering a period of 9.2±0.2 hours and an amplitude of 0.2 magnitude (u=2).according to the space-based surveys carried out by the infrared astronomical satellite iras, the japanese akari satellite and the neowise mission of nasa's wide-field infrared survey explorer, piazzia measures between 45.72 and 51.55 kilometers in diameter and its surface has an albedo between 0.041 and 0.1119. | 1000 piazzia | epoch | 2015-06-27 <tsp> 1000 piazzia | escapevelocity | 00252 kilometreperseconds <tsp> 1000 piazzia | formername | 1923 nz1951 ob <tsp> 1000 piazzia | orbitalperiod | 4881600 <tsp> 1000 piazzia | periapsis | 3524970000000 | 1000 piazzia, provisional designation 1923 nz, is a carbonaceous background asteroid from the outer region of the asteroid belt, approximately 48 kilometers (30 miles) in diameter. |
aaron bertram (born april 3, 1981, in lubbock, texas) is a trumpet player for third wave ska band suburban legends, and member of the children's music group kids imagine nation.in the past he has taught music and movement to preschool students in orange county, ca.his music program was called little rockstars.he launched an online streaming service for children's entertainment and arts education called kintv in march of 2020, where he currently performs and teaches music.he was a trumpet player for the third-wave ska band suburban legends from the band's origin in 1998 to may 2005, when he left to start his company, kids imagine with wife, rachel charest.he was known for doing a lot of backing vocals in the band and originated the idea of the band's signature choreography.aaron returned for a final performance with the band on november 29, 2005, at huntington beach high school for a benefit show for the ryan dallas cook memorial fund.since the summer of 2009, aaron has been performing with suburban legends at local shows.as of november 2010, he is listed as an official member of the band.in addition to playing trumpet for suburban legends, he also performed vocals for the band's cover of the gummi bears theme song, the band's cover of rose tint my world and the song powerful game on the album rump shaker.aaron is currently writing children's music under the name kids imagine nation with rachel charest and vince walker. | aaron bertram | associatedband/associatedmusicalartist | suburban legends <tsp> aaron bertram | genre | ska punk <tsp> aaron bertram | activeyearsstartyear | 1998 <tsp> aaron bertram | associatedband/associatedmusicalartist | kids imagine nation <tsp> aaron bertram | background | non vocal instrumentalist | aaron bertram (born april 3, 1981, in lubbock, texas) is a trumpet player for third wave ska band suburban legends, and member of the children's music group kids imagine nation.since the summer of 2009, aaron has been performing with suburban legends at local shows.aaron is currently writing children's music under the name kids imagine nation with rachel charest and vince walker. |
1000 piazzia, provisional designation 1923 nz, is a carbonaceous background asteroid from the outer region of the asteroid belt, approximately 48 kilometers (30 miles) in diameter.it was discovered on 12 august 1923, by german astronomer karl reinmuth at heidelberg observatory in southern germany.the c-type asteroid has a rotation period of 9.5 hours.it was named after italian giuseppe piazzi, who discovered 1 ceres.it orbits the sun in the outer asteroid belt at a distance of 2.4–4.0 au once every 5 years and 8 months (2,063 days; semi-major axis of 3.17 au).its orbit has an eccentricity of 0.26 and an inclination of 21° with respect to the ecliptic.as no precoveries were taken, the body's observation arc begins with its first recorded observation on the night following its official discovery date.he was a director of both the palermo and naples observatories, and known for the compilation of the palermo catalogue, containing the precise position of 7,646 stars.in 1801, piazzi discovered 1 ceres, the first and largest asteroid and the main-belt's only dwarf planet.he is also honored by the lunar crater piazzi.the official naming citation was first mentioned in the names of the minor planets by paul herget in 1955 (h 96).the asteroid is the first of several early 'kilo-numbered' minor planets that were dedicated to renowned scientists or institutions including: 2000 herschel, for william herschel who discovered uranus 3000 leonardo, for the italian polymath of the renaissance, leonardo da vinci 4000 hipparchus, for the ancient greek astronomer hipparchusthese are followed by the asteroids 5000 iau (for the international astronomical union), 6000 united nations (for the united nations), 7000 curie (for the pioneers on radioactivity, marie and pierre curie), and 8000 isaac newton (for isaac newton), while 9000 hal (after hal 9000 from the movie 2001: a space odyssey) and 10000 myriostos (after the greek word for ten-thousandth, and to honor all astronomers) were named based on their direct numeric accordance.1000 piazzia was named as part of trio honoring the events surrounding the discovery of ceres in 1801.a person named carl friedrich gauss who computed the orbit of ceres, and heinrich wilhelm matthias olbers who found it again later that year after it has passed behind the sun.in honor of them, 1001 gaussia for gauss and 1002 olbersia for olbers were named along with 1000 piazzia.in the next few years only three more astronomical bodies were found between mars and jupiter, pallas, juno, and 4 vesta, however it would be 37 years before another asteroid was found, 5 astraea in 1845.by 1868, 100 asteroids had been discovered, however it would not be until 1921 that the 1000th was discovered.the rate accelerated in the 20th century and the ten thousandth would be discovered in 1989.the lightcurve gave a rotation period of 9.47±0.01 hours with a brightness variation of 0.45 magnitude (u=3).a second lightcurve was obtained by astronomer rené roy in march 2007, rendering a period of 9.2±0.2 hours and an amplitude of 0.2 magnitude (u=2).according to the space-based surveys carried out by the infrared astronomical satellite iras, the japanese akari satellite and the neowise mission of nasa's wide-field infrared survey explorer, piazzia measures between 45.72 and 51.55 kilometers in diameter and its surface has an albedo between 0.041 and 0.1119. | 1000 piazzia | epoch | 2015-06-27 <tsp> 1000 piazzia | escapevelocity | 00252 kilometreperseconds <tsp> 1000 piazzia | formername | 1967 ed <tsp> 1000 piazzia | orbitalperiod | 4881600 <tsp> 1000 piazzia | periapsis | 3524970000000 | no related information |
antares (), known during early development as taurus ii, is an expendable launch system developed by orbital sciences corporation (now part of northrop grumman) and the pivdenne design bureau to launch the cygnus spacecraft to the international space station as part of nasa's cots and crs programs.able to launch payloads heavier than 8,000 kg (18,000 lb) into low earth orbit, antares is currently the largest rocket operated by northrop grumman.antares launches from the mid-atlantic regional spaceport and made its inaugural flight on april 21, 2013.nasa awarded orbital a commercial orbital transportation services (cots) space act agreement (saa) in 2008 to demonstrate delivery of cargo to the international space station.for these cots missions orbital intends to use antares to launch its cygnus spacecraft.in addition, antares will compete for small-to-medium missions.originally designated the taurus ii, orbital sciences renamed the vehicle antares, after the star of the same name, on december 12, 2011.out of 17 total launches, antares has suffered one failure.during the fifth launch on october 28, 2014, the rocket failed catastrophically, and the vehicle and payload were destroyed.the rocket's first-stage engines were identified as the cause for the failure.a different engine was chosen for subsequent launches, and the rocket had a successful return to flight on october 17, 2016.the antares has flown two major design iterations, the 100 series and 200 series.both series have used a castor 30xl as an upper stage but have differed on the first stage.the 100 series used two kerolox powered aj26 engine in the first stage and launched successfully four times.the 100 series was retired following a launch failure in 2014.the 200 series which first flew in 2016 also featured a kerolox first stage but instead used two rd-181 engine along with other minor upgrades.the 200 series future became uncertain following the russian invasion of ukraine.due to the first stage being produced in ukraine and the engines in russia, future production of the rocket was unable to be continued.as a result northrop grumman entered into an agreement with firefly aerospace to build the first stage of the antares 300 series.northrop also contracted with spacex for 3 falcon 9 launches.a commercial resupply service contract of $1.9 billion for eight flights was awarded in 2008.as of april 2012, development costs were estimated at $472 million.in june 2008, it was announced that the mid-atlantic regional spaceport, formerly part of the wallops flight facility, in virginia, would be the primary launch site for the rocket.launch pad 0a (lp-0a), previously used for the failed conestoga rocket, would be modified to handle antares.wallops allows launches which reach the international space station's orbit as effectively as those from cape canaveral, florida, while being less crowded.the first antares flight launched a cygnus mass simulator.on december 10, 2009, alliant techsystems inc. (atk) test-fired their castor 30 motor for use on the second stage of the antares rocket.in march 2010, orbital sciences and aerojet completed test firings of the aj-26 engines.on february 22, 2013, a hot fire test was successfully performed, the entire first stage being erected on the pad and held down while the engines fired for 29 seconds.as orbital had little experience with large liquid stages and lox propellant, the first stage core was designed and is manufactured in ukraine by kb pivdenne and pivdenmash and includes propellant tanks, pressurization tanks, valves, sensors, feed lines, tubing, wiring and other associated hardware.like the zenit—also manufactured by yuzhmash—the antares vehicle has a diameter of 3.9 m (150 in) with a matching 3.9 m payload fairing. | acquisite | diazotype | untransitively | no related information |
1000 piazzia, provisional designation 1923 nz, is a carbonaceous background asteroid from the outer region of the asteroid belt, approximately 48 kilometers (30 miles) in diameter.it was discovered on 12 august 1923, by german astronomer karl reinmuth at heidelberg observatory in southern germany.the c-type asteroid has a rotation period of 9.5 hours.it was named after italian giuseppe piazzi, who discovered 1 ceres.it orbits the sun in the outer asteroid belt at a distance of 2.4–4.0 au once every 5 years and 8 months (2,063 days; semi-major axis of 3.17 au).its orbit has an eccentricity of 0.26 and an inclination of 21° with respect to the ecliptic.as no precoveries were taken, the body's observation arc begins with its first recorded observation on the night following its official discovery date.he was a director of both the palermo and naples observatories, and known for the compilation of the palermo catalogue, containing the precise position of 7,646 stars.in 1801, piazzi discovered 1 ceres, the first and largest asteroid and the main-belt's only dwarf planet.he is also honored by the lunar crater piazzi.the official naming citation was first mentioned in the names of the minor planets by paul herget in 1955 (h 96).the asteroid is the first of several early 'kilo-numbered' minor planets that were dedicated to renowned scientists or institutions including: 2000 herschel, for william herschel who discovered uranus 3000 leonardo, for the italian polymath of the renaissance, leonardo da vinci 4000 hipparchus, for the ancient greek astronomer hipparchusthese are followed by the asteroids 5000 iau (for the international astronomical union), 6000 united nations (for the united nations), 7000 curie (for the pioneers on radioactivity, marie and pierre curie), and 8000 isaac newton (for isaac newton), while 9000 hal (after hal 9000 from the movie 2001: a space odyssey) and 10000 myriostos (after the greek word for ten-thousandth, and to honor all astronomers) were named based on their direct numeric accordance.1000 piazzia was named as part of trio honoring the events surrounding the discovery of ceres in 1801.a person named carl friedrich gauss who computed the orbit of ceres, and heinrich wilhelm matthias olbers who found it again later that year after it has passed behind the sun.in honor of them, 1001 gaussia for gauss and 1002 olbersia for olbers were named along with 1000 piazzia.in the next few years only three more astronomical bodies were found between mars and jupiter, pallas, juno, and 4 vesta, however it would be 37 years before another asteroid was found, 5 astraea in 1845.by 1868, 100 asteroids had been discovered, however it would not be until 1921 that the 1000th was discovered.the rate accelerated in the 20th century and the ten thousandth would be discovered in 1989.the lightcurve gave a rotation period of 9.47±0.01 hours with a brightness variation of 0.45 magnitude (u=3).a second lightcurve was obtained by astronomer rené roy in march 2007, rendering a period of 9.2±0.2 hours and an amplitude of 0.2 magnitude (u=2).according to the space-based surveys carried out by the infrared astronomical satellite iras, the japanese akari satellite and the neowise mission of nasa's wide-field infrared survey explorer, piazzia measures between 45.72 and 51.55 kilometers in diameter and its surface has an albedo between 0.041 and 0.1119. | 1000 piazzia | epoch | 2015-06-27 <tsp> 1000 piazzia | escapevelocity | 00252 kilometreperseconds <tsp> 1000 piazzia | formername | 1967 ed <tsp> 1000 piazzia | orbitalperiod | 4881600 <tsp> 1000 piazzia | periapsis | 3524970000000 | no related information |
1000 piazzia, provisional designation 1923 nz, is a carbonaceous background asteroid from the outer region of the asteroid belt, approximately 48 kilometers (30 miles) in diameter.it was discovered on 12 august 1923, by german astronomer karl reinmuth at heidelberg observatory in southern germany.the c-type asteroid has a rotation period of 9.5 hours.it was named after italian giuseppe piazzi, who discovered 1 ceres.it orbits the sun in the outer asteroid belt at a distance of 2.4–4.0 au once every 5 years and 8 months (2,063 days; semi-major axis of 3.17 au).its orbit has an eccentricity of 0.26 and an inclination of 21° with respect to the ecliptic.as no precoveries were taken, the body's observation arc begins with its first recorded observation on the night following its official discovery date.he was a director of both the palermo and naples observatories, and known for the compilation of the palermo catalogue, containing the precise position of 7,646 stars.in 1801, piazzi discovered 1 ceres, the first and largest asteroid and the main-belt's only dwarf planet.he is also honored by the lunar crater piazzi.the official naming citation was first mentioned in the names of the minor planets by paul herget in 1955 (h 96).the asteroid is the first of several early 'kilo-numbered' minor planets that were dedicated to renowned scientists or institutions including: 2000 herschel, for william herschel who discovered uranus 3000 leonardo, for the italian polymath of the renaissance, leonardo da vinci 4000 hipparchus, for the ancient greek astronomer hipparchusthese are followed by the asteroids 5000 iau (for the international astronomical union), 6000 united nations (for the united nations), 7000 curie (for the pioneers on radioactivity, marie and pierre curie), and 8000 isaac newton (for isaac newton), while 9000 hal (after hal 9000 from the movie 2001: a space odyssey) and 10000 myriostos (after the greek word for ten-thousandth, and to honor all astronomers) were named based on their direct numeric accordance.1000 piazzia was named as part of trio honoring the events surrounding the discovery of ceres in 1801.a person named carl friedrich gauss who computed the orbit of ceres, and heinrich wilhelm matthias olbers who found it again later that year after it has passed behind the sun.in honor of them, 1001 gaussia for gauss and 1002 olbersia for olbers were named along with 1000 piazzia.in the next few years only three more astronomical bodies were found between mars and jupiter, pallas, juno, and 4 vesta, however it would be 37 years before another asteroid was found, 5 astraea in 1845.by 1868, 100 asteroids had been discovered, however it would not be until 1921 that the 1000th was discovered.the rate accelerated in the 20th century and the ten thousandth would be discovered in 1989.the lightcurve gave a rotation period of 9.47±0.01 hours with a brightness variation of 0.45 magnitude (u=3).a second lightcurve was obtained by astronomer rené roy in march 2007, rendering a period of 9.2±0.2 hours and an amplitude of 0.2 magnitude (u=2).according to the space-based surveys carried out by the infrared astronomical satellite iras, the japanese akari satellite and the neowise mission of nasa's wide-field infrared survey explorer, piazzia measures between 45.72 and 51.55 kilometers in diameter and its surface has an albedo between 0.041 and 0.1119. | 1000 piazzia | epoch | 2015-06-27 <tsp> 1000 piazzia | escapevelocity | 00252 kilometreperseconds <tsp> 1000 piazzia | formername | 1967 ed <tsp> 1000 piazzia | orbitalperiod | 4881600 <tsp> 1000 piazzia | periapsis | 3524970000000 | no related information |
aaron bertram (born april 3, 1981, in lubbock, texas) is a trumpet player for third wave ska band suburban legends, and member of the children's music group kids imagine nation.in the past he has taught music and movement to preschool students in orange county, ca.his music program was called little rockstars.he launched an online streaming service for children's entertainment and arts education called kintv in march of 2020, where he currently performs and teaches music.he was a trumpet player for the third-wave ska band suburban legends from the band's origin in 1998 to may 2005, when he left to start his company, kids imagine with wife, rachel charest.he was known for doing a lot of backing vocals in the band and originated the idea of the band's signature choreography.aaron returned for a final performance with the band on november 29, 2005, at huntington beach high school for a benefit show for the ryan dallas cook memorial fund.since the summer of 2009, aaron has been performing with suburban legends at local shows.as of november 2010, he is listed as an official member of the band.in addition to playing trumpet for suburban legends, he also performed vocals for the band's cover of the gummi bears theme song, the band's cover of rose tint my world and the song powerful game on the album rump shaker.aaron is currently writing children's music under the name kids imagine nation with rachel charest and vince walker. | ephebeibeia | spavins | literalistic <tsp> ephebeibeia | soundable | abominators | no related information |
antares (), known during early development as taurus ii, is an expendable launch system developed by orbital sciences corporation (now part of northrop grumman) and the pivdenne design bureau to launch the cygnus spacecraft to the international space station as part of nasa's cots and crs programs.able to launch payloads heavier than 8,000 kg (18,000 lb) into low earth orbit, antares is currently the largest rocket operated by northrop grumman.antares launches from the mid-atlantic regional spaceport and made its inaugural flight on april 21, 2013.nasa awarded orbital a commercial orbital transportation services (cots) space act agreement (saa) in 2008 to demonstrate delivery of cargo to the international space station.for these cots missions orbital intends to use antares to launch its cygnus spacecraft.in addition, antares will compete for small-to-medium missions.originally designated the taurus ii, orbital sciences renamed the vehicle antares, after the star of the same name, on december 12, 2011.out of 17 total launches, antares has suffered one failure.during the fifth launch on october 28, 2014, the rocket failed catastrophically, and the vehicle and payload were destroyed.the rocket's first-stage engines were identified as the cause for the failure.a different engine was chosen for subsequent launches, and the rocket had a successful return to flight on october 17, 2016.the antares has flown two major design iterations, the 100 series and 200 series.both series have used a castor 30xl as an upper stage but have differed on the first stage.the 100 series used two kerolox powered aj26 engine in the first stage and launched successfully four times.the 100 series was retired following a launch failure in 2014.the 200 series which first flew in 2016 also featured a kerolox first stage but instead used two rd-181 engine along with other minor upgrades.the 200 series future became uncertain following the russian invasion of ukraine.due to the first stage being produced in ukraine and the engines in russia, future production of the rocket was unable to be continued.as a result northrop grumman entered into an agreement with firefly aerospace to build the first stage of the antares 300 series.northrop also contracted with spacex for 3 falcon 9 launches.a commercial resupply service contract of $1.9 billion for eight flights was awarded in 2008.as of april 2012, development costs were estimated at $472 million.in june 2008, it was announced that the mid-atlantic regional spaceport, formerly part of the wallops flight facility, in virginia, would be the primary launch site for the rocket.launch pad 0a (lp-0a), previously used for the failed conestoga rocket, would be modified to handle antares.wallops allows launches which reach the international space station's orbit as effectively as those from cape canaveral, florida, while being less crowded.the first antares flight launched a cygnus mass simulator.on december 10, 2009, alliant techsystems inc. (atk) test-fired their castor 30 motor for use on the second stage of the antares rocket.in march 2010, orbital sciences and aerojet completed test firings of the aj-26 engines.on february 22, 2013, a hot fire test was successfully performed, the entire first stage being erected on the pad and held down while the engines fired for 29 seconds.as orbital had little experience with large liquid stages and lox propellant, the first stage core was designed and is manufactured in ukraine by kb pivdenne and pivdenmash and includes propellant tanks, pressurization tanks, valves, sensors, feed lines, tubing, wiring and other associated hardware.like the zenit—also manufactured by yuzhmash—the antares vehicle has a diameter of 3.9 m (150 in) with a matching 3.9 m payload fairing. | antares rocket | manufacturer | yuzhnoye design office <tsp> antares rocket | finalflight | 2014-10-28 <tsp> antares rocket | maidenflight | 2013-04-21 <tsp> antares rocket | launchsite | mid-atlantic regional spaceport launch pad 0 <tsp> antares rocket | diameter | 39 metres | antares (), known during early development as taurus ii, is an expendable launch system developed by orbital sciences corporation (now part of northrop grumman) and the pivdenne design bureau to launch the cygnus spacecraft to the international space station as part of nasa's cots and crs programs.able to launch payloads heavier than 8,000 kg (18,000 lb) into low earth orbit, antares is currently the largest rocket operated by northrop grumman.antares launches from the mid-atlantic regional spaceport and made its inaugural flight on april 21, 2013.nasa awarded orbital a commercial orbital transportation services (cots) space act agreement (saa) in 2008 to demonstrate delivery of cargo to the international space station.for these cots missions orbital intends to use antares to launch its cygnus spacecraft.originally designated the taurus ii, orbital sciences renamed the vehicle antares, after the star of the same name, on december 12, 2011.out of 17 total launches, antares has suffered one failure.the antares has flown two major design iterations, the 100 series and 200 series.launch pad 0a (lp-0a), previously used for the failed conestoga rocket, would be modified to handle antares.the first antares flight launched a cygnus mass simulator.on december 10, 2009, alliant techsystems inc. (atk) test-fired their castor 30 motor for use on the second stage of the antares rocket. |
1000 piazzia, provisional designation 1923 nz, is a carbonaceous background asteroid from the outer region of the asteroid belt, approximately 48 kilometers (30 miles) in diameter.it was discovered on 12 august 1923, by german astronomer karl reinmuth at heidelberg observatory in southern germany.the c-type asteroid has a rotation period of 9.5 hours.it was named after italian giuseppe piazzi, who discovered 1 ceres.it orbits the sun in the outer asteroid belt at a distance of 2.4–4.0 au once every 5 years and 8 months (2,063 days; semi-major axis of 3.17 au).its orbit has an eccentricity of 0.26 and an inclination of 21° with respect to the ecliptic.as no precoveries were taken, the body's observation arc begins with its first recorded observation on the night following its official discovery date.he was a director of both the palermo and naples observatories, and known for the compilation of the palermo catalogue, containing the precise position of 7,646 stars.in 1801, piazzi discovered 1 ceres, the first and largest asteroid and the main-belt's only dwarf planet.he is also honored by the lunar crater piazzi.the official naming citation was first mentioned in the names of the minor planets by paul herget in 1955 (h 96).the asteroid is the first of several early 'kilo-numbered' minor planets that were dedicated to renowned scientists or institutions including: 2000 herschel, for william herschel who discovered uranus 3000 leonardo, for the italian polymath of the renaissance, leonardo da vinci 4000 hipparchus, for the ancient greek astronomer hipparchusthese are followed by the asteroids 5000 iau (for the international astronomical union), 6000 united nations (for the united nations), 7000 curie (for the pioneers on radioactivity, marie and pierre curie), and 8000 isaac newton (for isaac newton), while 9000 hal (after hal 9000 from the movie 2001: a space odyssey) and 10000 myriostos (after the greek word for ten-thousandth, and to honor all astronomers) were named based on their direct numeric accordance.1000 piazzia was named as part of trio honoring the events surrounding the discovery of ceres in 1801.a person named carl friedrich gauss who computed the orbit of ceres, and heinrich wilhelm matthias olbers who found it again later that year after it has passed behind the sun.in honor of them, 1001 gaussia for gauss and 1002 olbersia for olbers were named along with 1000 piazzia.in the next few years only three more astronomical bodies were found between mars and jupiter, pallas, juno, and 4 vesta, however it would be 37 years before another asteroid was found, 5 astraea in 1845.by 1868, 100 asteroids had been discovered, however it would not be until 1921 that the 1000th was discovered.the rate accelerated in the 20th century and the ten thousandth would be discovered in 1989.the lightcurve gave a rotation period of 9.47±0.01 hours with a brightness variation of 0.45 magnitude (u=3).a second lightcurve was obtained by astronomer rené roy in march 2007, rendering a period of 9.2±0.2 hours and an amplitude of 0.2 magnitude (u=2).according to the space-based surveys carried out by the infrared astronomical satellite iras, the japanese akari satellite and the neowise mission of nasa's wide-field infrared survey explorer, piazzia measures between 45.72 and 51.55 kilometers in diameter and its surface has an albedo between 0.041 and 0.1119. | 1000 piazzia | mass | 11 kilograms <tsp> 1000 piazzia | orbitalperiod | 4881600 <tsp> 1000 piazzia | periapsis | 3524970000000 <tsp> 1000 piazzia | epoch | 2015-06-27 <tsp> 1000 piazzia | escapevelocity | 00252 kilometreperseconds | no related information |
aaron bertram (born april 3, 1981, in lubbock, texas) is a trumpet player for third wave ska band suburban legends, and member of the children's music group kids imagine nation.in the past he has taught music and movement to preschool students in orange county, ca.his music program was called little rockstars.he launched an online streaming service for children's entertainment and arts education called kintv in march of 2020, where he currently performs and teaches music.he was a trumpet player for the third-wave ska band suburban legends from the band's origin in 1998 to may 2005, when he left to start his company, kids imagine with wife, rachel charest.he was known for doing a lot of backing vocals in the band and originated the idea of the band's signature choreography.aaron returned for a final performance with the band on november 29, 2005, at huntington beach high school for a benefit show for the ryan dallas cook memorial fund.since the summer of 2009, aaron has been performing with suburban legends at local shows.as of november 2010, he is listed as an official member of the band.in addition to playing trumpet for suburban legends, he also performed vocals for the band's cover of the gummi bears theme song, the band's cover of rose tint my world and the song powerful game on the album rump shaker.aaron is currently writing children's music under the name kids imagine nation with rachel charest and vince walker. | aaron bertram | associatedband/associatedmusicalartist | suburban legends <tsp> ska punk | stylisticorigin | ska <tsp> aaron bertram | associatedband/associatedmusicalartist | kids imagine nation <tsp> aaron bertram | genre | ska punk <tsp> ska punk | stylisticorigin | punk rock | aaron bertram (born april 3, 1981, in lubbock, texas) is a trumpet player for third wave ska band suburban legends, and member of the children's music group kids imagine nation.he was a trumpet player for the third-wave ska band suburban legends from the band's origin in 1998 to may 2005, when he left to start his company, kids imagine with wife, rachel charest.since the summer of 2009, aaron has been performing with suburban legends at local shows.aaron is currently writing children's music under the name kids imagine nation with rachel charest and vince walker. |
1000 piazzia, provisional designation 1923 nz, is a carbonaceous background asteroid from the outer region of the asteroid belt, approximately 48 kilometers (30 miles) in diameter.it was discovered on 12 august 1923, by german astronomer karl reinmuth at heidelberg observatory in southern germany.the c-type asteroid has a rotation period of 9.5 hours.it was named after italian giuseppe piazzi, who discovered 1 ceres.it orbits the sun in the outer asteroid belt at a distance of 2.4–4.0 au once every 5 years and 8 months (2,063 days; semi-major axis of 3.17 au).its orbit has an eccentricity of 0.26 and an inclination of 21° with respect to the ecliptic.as no precoveries were taken, the body's observation arc begins with its first recorded observation on the night following its official discovery date.he was a director of both the palermo and naples observatories, and known for the compilation of the palermo catalogue, containing the precise position of 7,646 stars.in 1801, piazzi discovered 1 ceres, the first and largest asteroid and the main-belt's only dwarf planet.he is also honored by the lunar crater piazzi.the official naming citation was first mentioned in the names of the minor planets by paul herget in 1955 (h 96).the asteroid is the first of several early 'kilo-numbered' minor planets that were dedicated to renowned scientists or institutions including: 2000 herschel, for william herschel who discovered uranus 3000 leonardo, for the italian polymath of the renaissance, leonardo da vinci 4000 hipparchus, for the ancient greek astronomer hipparchusthese are followed by the asteroids 5000 iau (for the international astronomical union), 6000 united nations (for the united nations), 7000 curie (for the pioneers on radioactivity, marie and pierre curie), and 8000 isaac newton (for isaac newton), while 9000 hal (after hal 9000 from the movie 2001: a space odyssey) and 10000 myriostos (after the greek word for ten-thousandth, and to honor all astronomers) were named based on their direct numeric accordance.1000 piazzia was named as part of trio honoring the events surrounding the discovery of ceres in 1801.a person named carl friedrich gauss who computed the orbit of ceres, and heinrich wilhelm matthias olbers who found it again later that year after it has passed behind the sun.in honor of them, 1001 gaussia for gauss and 1002 olbersia for olbers were named along with 1000 piazzia.in the next few years only three more astronomical bodies were found between mars and jupiter, pallas, juno, and 4 vesta, however it would be 37 years before another asteroid was found, 5 astraea in 1845.by 1868, 100 asteroids had been discovered, however it would not be until 1921 that the 1000th was discovered.the rate accelerated in the 20th century and the ten thousandth would be discovered in 1989.the lightcurve gave a rotation period of 9.47±0.01 hours with a brightness variation of 0.45 magnitude (u=3).a second lightcurve was obtained by astronomer rené roy in march 2007, rendering a period of 9.2±0.2 hours and an amplitude of 0.2 magnitude (u=2).according to the space-based surveys carried out by the infrared astronomical satellite iras, the japanese akari satellite and the neowise mission of nasa's wide-field infrared survey explorer, piazzia measures between 45.72 and 51.55 kilometers in diameter and its surface has an albedo between 0.041 and 0.1119. | 1000 piazzia | mass | 11 kilograms <tsp> 1000 piazzia | orbitalperiod | 4881600 <tsp> 1000 piazzia | periapsis | 3524970000000 <tsp> 1000 piazzia | epoch | 2015-06-27 <tsp> 1000 piazzia | escapevelocity | 00252 kilometreperseconds | no related information |
antares (), known during early development as taurus ii, is an expendable launch system developed by orbital sciences corporation (now part of northrop grumman) and the pivdenne design bureau to launch the cygnus spacecraft to the international space station as part of nasa's cots and crs programs.able to launch payloads heavier than 8,000 kg (18,000 lb) into low earth orbit, antares is currently the largest rocket operated by northrop grumman.antares launches from the mid-atlantic regional spaceport and made its inaugural flight on april 21, 2013.nasa awarded orbital a commercial orbital transportation services (cots) space act agreement (saa) in 2008 to demonstrate delivery of cargo to the international space station.for these cots missions orbital intends to use antares to launch its cygnus spacecraft.in addition, antares will compete for small-to-medium missions.originally designated the taurus ii, orbital sciences renamed the vehicle antares, after the star of the same name, on december 12, 2011.out of 17 total launches, antares has suffered one failure.during the fifth launch on october 28, 2014, the rocket failed catastrophically, and the vehicle and payload were destroyed.the rocket's first-stage engines were identified as the cause for the failure.a different engine was chosen for subsequent launches, and the rocket had a successful return to flight on october 17, 2016.the antares has flown two major design iterations, the 100 series and 200 series.both series have used a castor 30xl as an upper stage but have differed on the first stage.the 100 series used two kerolox powered aj26 engine in the first stage and launched successfully four times.the 100 series was retired following a launch failure in 2014.the 200 series which first flew in 2016 also featured a kerolox first stage but instead used two rd-181 engine along with other minor upgrades.the 200 series future became uncertain following the russian invasion of ukraine.due to the first stage being produced in ukraine and the engines in russia, future production of the rocket was unable to be continued.as a result northrop grumman entered into an agreement with firefly aerospace to build the first stage of the antares 300 series.northrop also contracted with spacex for 3 falcon 9 launches.a commercial resupply service contract of $1.9 billion for eight flights was awarded in 2008.as of april 2012, development costs were estimated at $472 million.in june 2008, it was announced that the mid-atlantic regional spaceport, formerly part of the wallops flight facility, in virginia, would be the primary launch site for the rocket.launch pad 0a (lp-0a), previously used for the failed conestoga rocket, would be modified to handle antares.wallops allows launches which reach the international space station's orbit as effectively as those from cape canaveral, florida, while being less crowded.the first antares flight launched a cygnus mass simulator.on december 10, 2009, alliant techsystems inc. (atk) test-fired their castor 30 motor for use on the second stage of the antares rocket.in march 2010, orbital sciences and aerojet completed test firings of the aj-26 engines.on february 22, 2013, a hot fire test was successfully performed, the entire first stage being erected on the pad and held down while the engines fired for 29 seconds.as orbital had little experience with large liquid stages and lox propellant, the first stage core was designed and is manufactured in ukraine by kb pivdenne and pivdenmash and includes propellant tanks, pressurization tanks, valves, sensors, feed lines, tubing, wiring and other associated hardware.like the zenit—also manufactured by yuzhmash—the antares vehicle has a diameter of 3.9 m (150 in) with a matching 3.9 m payload fairing. | antares rocket | manufacturer | yuzhnoye design office <tsp> antares rocket | finalflight | 2014-10-28 <tsp> antares rocket | maidenflight | 2013-04-21 <tsp> antares rocket | launchsite | mid-atlantic regional spaceport launch pad 0 <tsp> antares rocket | diameter | 39 metres | antares (), known during early development as taurus ii, is an expendable launch system developed by orbital sciences corporation (now part of northrop grumman) and the pivdenne design bureau to launch the cygnus spacecraft to the international space station as part of nasa's cots and crs programs.able to launch payloads heavier than 8,000 kg (18,000 lb) into low earth orbit, antares is currently the largest rocket operated by northrop grumman.antares launches from the mid-atlantic regional spaceport and made its inaugural flight on april 21, 2013.nasa awarded orbital a commercial orbital transportation services (cots) space act agreement (saa) in 2008 to demonstrate delivery of cargo to the international space station.for these cots missions orbital intends to use antares to launch its cygnus spacecraft.originally designated the taurus ii, orbital sciences renamed the vehicle antares, after the star of the same name, on december 12, 2011.out of 17 total launches, antares has suffered one failure.the antares has flown two major design iterations, the 100 series and 200 series.launch pad 0a (lp-0a), previously used for the failed conestoga rocket, would be modified to handle antares.the first antares flight launched a cygnus mass simulator.on december 10, 2009, alliant techsystems inc. (atk) test-fired their castor 30 motor for use on the second stage of the antares rocket. |
aaron bertram (born april 3, 1981, in lubbock, texas) is a trumpet player for third wave ska band suburban legends, and member of the children's music group kids imagine nation.in the past he has taught music and movement to preschool students in orange county, ca.his music program was called little rockstars.he launched an online streaming service for children's entertainment and arts education called kintv in march of 2020, where he currently performs and teaches music.he was a trumpet player for the third-wave ska band suburban legends from the band's origin in 1998 to may 2005, when he left to start his company, kids imagine with wife, rachel charest.he was known for doing a lot of backing vocals in the band and originated the idea of the band's signature choreography.aaron returned for a final performance with the band on november 29, 2005, at huntington beach high school for a benefit show for the ryan dallas cook memorial fund.since the summer of 2009, aaron has been performing with suburban legends at local shows.as of november 2010, he is listed as an official member of the band.in addition to playing trumpet for suburban legends, he also performed vocals for the band's cover of the gummi bears theme song, the band's cover of rose tint my world and the song powerful game on the album rump shaker.aaron is currently writing children's music under the name kids imagine nation with rachel charest and vince walker. | aaron bertram | associatedband/associatedmusicalartist | suburban legends <tsp> ska punk | stylisticorigin | ska <tsp> aaron bertram | associatedband/associatedmusicalartist | kids imagine nation <tsp> aaron bertram | genre | ska punk <tsp> ska punk | stylisticorigin | punk rock | aaron bertram (born april 3, 1981, in lubbock, texas) is a trumpet player for third wave ska band suburban legends, and member of the children's music group kids imagine nation.he was a trumpet player for the third-wave ska band suburban legends from the band's origin in 1998 to may 2005, when he left to start his company, kids imagine with wife, rachel charest.since the summer of 2009, aaron has been performing with suburban legends at local shows.aaron is currently writing children's music under the name kids imagine nation with rachel charest and vince walker. |
1000 piazzia, provisional designation 1923 nz, is a carbonaceous background asteroid from the outer region of the asteroid belt, approximately 48 kilometers (30 miles) in diameter.it was discovered on 12 august 1923, by german astronomer karl reinmuth at heidelberg observatory in southern germany.the c-type asteroid has a rotation period of 9.5 hours.it was named after italian giuseppe piazzi, who discovered 1 ceres.it orbits the sun in the outer asteroid belt at a distance of 2.4–4.0 au once every 5 years and 8 months (2,063 days; semi-major axis of 3.17 au).its orbit has an eccentricity of 0.26 and an inclination of 21° with respect to the ecliptic.as no precoveries were taken, the body's observation arc begins with its first recorded observation on the night following its official discovery date.he was a director of both the palermo and naples observatories, and known for the compilation of the palermo catalogue, containing the precise position of 7,646 stars.in 1801, piazzi discovered 1 ceres, the first and largest asteroid and the main-belt's only dwarf planet.he is also honored by the lunar crater piazzi.the official naming citation was first mentioned in the names of the minor planets by paul herget in 1955 (h 96).the asteroid is the first of several early 'kilo-numbered' minor planets that were dedicated to renowned scientists or institutions including: 2000 herschel, for william herschel who discovered uranus 3000 leonardo, for the italian polymath of the renaissance, leonardo da vinci 4000 hipparchus, for the ancient greek astronomer hipparchusthese are followed by the asteroids 5000 iau (for the international astronomical union), 6000 united nations (for the united nations), 7000 curie (for the pioneers on radioactivity, marie and pierre curie), and 8000 isaac newton (for isaac newton), while 9000 hal (after hal 9000 from the movie 2001: a space odyssey) and 10000 myriostos (after the greek word for ten-thousandth, and to honor all astronomers) were named based on their direct numeric accordance.1000 piazzia was named as part of trio honoring the events surrounding the discovery of ceres in 1801.a person named carl friedrich gauss who computed the orbit of ceres, and heinrich wilhelm matthias olbers who found it again later that year after it has passed behind the sun.in honor of them, 1001 gaussia for gauss and 1002 olbersia for olbers were named along with 1000 piazzia.in the next few years only three more astronomical bodies were found between mars and jupiter, pallas, juno, and 4 vesta, however it would be 37 years before another asteroid was found, 5 astraea in 1845.by 1868, 100 asteroids had been discovered, however it would not be until 1921 that the 1000th was discovered.the rate accelerated in the 20th century and the ten thousandth would be discovered in 1989.the lightcurve gave a rotation period of 9.47±0.01 hours with a brightness variation of 0.45 magnitude (u=3).a second lightcurve was obtained by astronomer rené roy in march 2007, rendering a period of 9.2±0.2 hours and an amplitude of 0.2 magnitude (u=2).according to the space-based surveys carried out by the infrared astronomical satellite iras, the japanese akari satellite and the neowise mission of nasa's wide-field infrared survey explorer, piazzia measures between 45.72 and 51.55 kilometers in diameter and its surface has an albedo between 0.041 and 0.1119. | 1000 piazzia | mass | 11 kilograms <tsp> 1000 piazzia | orbitalperiod | 4881600 <tsp> 1000 piazzia | periapsis | 3524970000000 <tsp> 1000 piazzia | epoch | 2015-06-27 <tsp> 1000 piazzia | escapevelocity | 00252 kilometreperseconds | no related information |
aaron deer (born november 1, 1980) is an american songwriter and multi-instrumentalist originally from indianapolis, indiana, united states, now residing in oakland, california.he is best known for his work in the bloomington music scene in the early 2000s, playing with bands such as the impossible shapes, john wilkes booze, and the horns of happiness.in the winter of 2009, deer relocated to california and continues work with the horns of happiness, royal geography society, farmer dave scher and wee giant, among others, while co-running the magnetic south cassette label.in 1999, deer and barth moved to bloomington to attend indiana university and they restarted the band there.the group released their first record, 'the great migration', in 2000 and followed with 2 subsequent releases with indianapolis-based label recordhead/mr.whiggs.in 2003, the impossible shapes signed with bloomington label secretly canadian released 'we like it wild' and toured nationally and internationally.around the same time, john wilkes booze was reformed in its classic 'five pillars of soul' line-up.after touring the western us in 2004, john wilkes booze was signed to olympia, wa-based kill rock stars.his solo debut by the horns of happiness a sea as a shore was released by secretly canadian in 2004.in 2005, deer teamed up with drummer and visual artist shelley harrison to form the first performance version of the horns of happiness touring extensively through the us, sharing the stage with acts such as man man, silver jews, old time relijun, danielson famile, joanna newsome, and the dirty projectors, among others, while garnering acclaim in publications such as magnet, dusted and skyscraper magazines. | odontaspis | pitometer | chorioids <tsp> odontaspis | airship | terphenyl | no related information |
gaussia (minor planet designation: 1001 gaussia), provisional designation 1923 oa, is a dark background asteroid from the outer regions of the asteroid belt, approximately 73 kilometers in diameter.it was discovered on 8 august 1923, by soviet astronomer sergey belyavsky at the simeiz observatory on the crimean peninsula.the asteroid was named after german mathematician carl friedrich gauss.gauss computed the orbit of ceres, and 1001 gaussia was named along with 1000 piazzia, and 1002 olbersia in part for their work on ceres, with names for giuseppe piazzi, who found ceres, and heinrich wilhelm matthias olbers, who recovered it later that year.it orbits the sun in the outer main-belt at a distance of 2.8–3.6 au once every 5 years and 9 months (2,100 days).its orbit has an eccentricity of 0.13 and an inclination of 9° with respect to the ecliptic.the asteroid was first identified as a907 xc at taunton observatory (803) in december 1907.the body's observation arc begins at unso in january 1908, more than 15 years prior to its official discovery observation at simeiz.its type is closest to the primitive p-type asteroids, followed by the common carbonaceous c-type asteroids.lightcurve analysis gave a well-defined rotation period of 20.99 hours with a brightness amplitude of 0.11 magnitude (u=3).lower-rated lightcurves with a divergent period of 4.08 and 9.17 hours were previously obtained in 2005 and 2009, respectively (u=1/2-).he is also honored by the lunar crater gauss.1001 gaussia was named as part of trio honoring the events surrounding the discovery of ceres in 1801.carl friedrich gauss who computed the orbit of ceres was for 1001 gaussia, 1000 piazzia for giuseppe piazzi and 1002 olbersia for heinrich wilhelm matthias olbers.olbers recovered ceres after it has passed behind the sun and returned.in the next few years only three more astronomical bodies were found between mars and jupiter, pallas, juno, and 4 vesta, however it would be 37 years before another asteroid was found, 5 astraea in 1845. | preindicate | twitted | calamitous <tsp> preindicate | malpoise | tidily | no related information |
aaron deer (born november 1, 1980) is an american songwriter and multi-instrumentalist originally from indianapolis, indiana, united states, now residing in oakland, california.he is best known for his work in the bloomington music scene in the early 2000s, playing with bands such as the impossible shapes, john wilkes booze, and the horns of happiness.in the winter of 2009, deer relocated to california and continues work with the horns of happiness, royal geography society, farmer dave scher and wee giant, among others, while co-running the magnetic south cassette label.in 1999, deer and barth moved to bloomington to attend indiana university and they restarted the band there.the group released their first record, 'the great migration', in 2000 and followed with 2 subsequent releases with indianapolis-based label recordhead/mr.whiggs.in 2003, the impossible shapes signed with bloomington label secretly canadian released 'we like it wild' and toured nationally and internationally.around the same time, john wilkes booze was reformed in its classic 'five pillars of soul' line-up.after touring the western us in 2004, john wilkes booze was signed to olympia, wa-based kill rock stars.his solo debut by the horns of happiness a sea as a shore was released by secretly canadian in 2004.in 2005, deer teamed up with drummer and visual artist shelley harrison to form the first performance version of the horns of happiness touring extensively through the us, sharing the stage with acts such as man man, silver jews, old time relijun, danielson famile, joanna newsome, and the dirty projectors, among others, while garnering acclaim in publications such as magnet, dusted and skyscraper magazines. | aaron deer | associatedband/associatedmusicalartist | wee giant <tsp> aaron deer | background | solo singer <tsp> aaron deer | genre | psychedelia <tsp> aaron deer | origin | indiana <tsp> aaron deer | origin | united states | aaron deer (born november 1, 1980) is an american songwriter and multi-instrumentalist originally from indianapolis, indiana, united states, now residing in oakland, california.in the winter of 2009, deer relocated to california and continues work with the horns of happiness, royal geography society, farmer dave scher and wee giant, among others, while co-running the magnetic south cassette label.in 1999, deer and barth moved to bloomington to attend indiana university and they restarted the band there. |
gaussia (minor planet designation: 1001 gaussia), provisional designation 1923 oa, is a dark background asteroid from the outer regions of the asteroid belt, approximately 73 kilometers in diameter.it was discovered on 8 august 1923, by soviet astronomer sergey belyavsky at the simeiz observatory on the crimean peninsula.the asteroid was named after german mathematician carl friedrich gauss.gauss computed the orbit of ceres, and 1001 gaussia was named along with 1000 piazzia, and 1002 olbersia in part for their work on ceres, with names for giuseppe piazzi, who found ceres, and heinrich wilhelm matthias olbers, who recovered it later that year.it orbits the sun in the outer main-belt at a distance of 2.8–3.6 au once every 5 years and 9 months (2,100 days).its orbit has an eccentricity of 0.13 and an inclination of 9° with respect to the ecliptic.the asteroid was first identified as a907 xc at taunton observatory (803) in december 1907.the body's observation arc begins at unso in january 1908, more than 15 years prior to its official discovery observation at simeiz.its type is closest to the primitive p-type asteroids, followed by the common carbonaceous c-type asteroids.lightcurve analysis gave a well-defined rotation period of 20.99 hours with a brightness amplitude of 0.11 magnitude (u=3).lower-rated lightcurves with a divergent period of 4.08 and 9.17 hours were previously obtained in 2005 and 2009, respectively (u=1/2-).he is also honored by the lunar crater gauss.1001 gaussia was named as part of trio honoring the events surrounding the discovery of ceres in 1801.carl friedrich gauss who computed the orbit of ceres was for 1001 gaussia, 1000 piazzia for giuseppe piazzi and 1002 olbersia for heinrich wilhelm matthias olbers.olbers recovered ceres after it has passed behind the sun and returned.in the next few years only three more astronomical bodies were found between mars and jupiter, pallas, juno, and 4 vesta, however it would be 37 years before another asteroid was found, 5 astraea in 1845. | 1001 gaussia | discoverer | sergey belyavsky <tsp> 1001 gaussia | epoch | 2015-06-27 <tsp> 1001 gaussia | formername | 1923 oaa907 xc <tsp> 1001 gaussia | orbitalperiod | 575 days <tsp> 1001 gaussia | periapsis | 41911339455312 kilometres | gaussia (minor planet designation: 1001 gaussia), provisional designation 1923 oa, is a dark background asteroid from the outer regions of the asteroid belt, approximately 73 kilometers in diameter. |
aaron deer (born november 1, 1980) is an american songwriter and multi-instrumentalist originally from indianapolis, indiana, united states, now residing in oakland, california.he is best known for his work in the bloomington music scene in the early 2000s, playing with bands such as the impossible shapes, john wilkes booze, and the horns of happiness.in the winter of 2009, deer relocated to california and continues work with the horns of happiness, royal geography society, farmer dave scher and wee giant, among others, while co-running the magnetic south cassette label.in 1999, deer and barth moved to bloomington to attend indiana university and they restarted the band there.the group released their first record, 'the great migration', in 2000 and followed with 2 subsequent releases with indianapolis-based label recordhead/mr.whiggs.in 2003, the impossible shapes signed with bloomington label secretly canadian released 'we like it wild' and toured nationally and internationally.around the same time, john wilkes booze was reformed in its classic 'five pillars of soul' line-up.after touring the western us in 2004, john wilkes booze was signed to olympia, wa-based kill rock stars.his solo debut by the horns of happiness a sea as a shore was released by secretly canadian in 2004.in 2005, deer teamed up with drummer and visual artist shelley harrison to form the first performance version of the horns of happiness touring extensively through the us, sharing the stage with acts such as man man, silver jews, old time relijun, danielson famile, joanna newsome, and the dirty projectors, among others, while garnering acclaim in publications such as magnet, dusted and skyscraper magazines. | chortled | abrenounce | zabti <tsp> chortled | gaieties | subregularity | no related information |
gaussia (minor planet designation: 1001 gaussia), provisional designation 1923 oa, is a dark background asteroid from the outer regions of the asteroid belt, approximately 73 kilometers in diameter.it was discovered on 8 august 1923, by soviet astronomer sergey belyavsky at the simeiz observatory on the crimean peninsula.the asteroid was named after german mathematician carl friedrich gauss.gauss computed the orbit of ceres, and 1001 gaussia was named along with 1000 piazzia, and 1002 olbersia in part for their work on ceres, with names for giuseppe piazzi, who found ceres, and heinrich wilhelm matthias olbers, who recovered it later that year.it orbits the sun in the outer main-belt at a distance of 2.8–3.6 au once every 5 years and 9 months (2,100 days).its orbit has an eccentricity of 0.13 and an inclination of 9° with respect to the ecliptic.the asteroid was first identified as a907 xc at taunton observatory (803) in december 1907.the body's observation arc begins at unso in january 1908, more than 15 years prior to its official discovery observation at simeiz.its type is closest to the primitive p-type asteroids, followed by the common carbonaceous c-type asteroids.lightcurve analysis gave a well-defined rotation period of 20.99 hours with a brightness amplitude of 0.11 magnitude (u=3).lower-rated lightcurves with a divergent period of 4.08 and 9.17 hours were previously obtained in 2005 and 2009, respectively (u=1/2-).he is also honored by the lunar crater gauss.1001 gaussia was named as part of trio honoring the events surrounding the discovery of ceres in 1801.carl friedrich gauss who computed the orbit of ceres was for 1001 gaussia, 1000 piazzia for giuseppe piazzi and 1002 olbersia for heinrich wilhelm matthias olbers.olbers recovered ceres after it has passed behind the sun and returned.in the next few years only three more astronomical bodies were found between mars and jupiter, pallas, juno, and 4 vesta, however it would be 37 years before another asteroid was found, 5 astraea in 1845. | 1001 gaussia | discoverer | sergey belyavsky <tsp> 1001 gaussia | epoch | 2015-06-27 <tsp> 1001 gaussia | formername | a911 md <tsp> 1001 gaussia | orbitalperiod | 575 days <tsp> 1001 gaussia | periapsis | 41911339455312 kilometres | no related information |
aaron deer (born november 1, 1980) is an american songwriter and multi-instrumentalist originally from indianapolis, indiana, united states, now residing in oakland, california.he is best known for his work in the bloomington music scene in the early 2000s, playing with bands such as the impossible shapes, john wilkes booze, and the horns of happiness.in the winter of 2009, deer relocated to california and continues work with the horns of happiness, royal geography society, farmer dave scher and wee giant, among others, while co-running the magnetic south cassette label.in 1999, deer and barth moved to bloomington to attend indiana university and they restarted the band there.the group released their first record, 'the great migration', in 2000 and followed with 2 subsequent releases with indianapolis-based label recordhead/mr.whiggs.in 2003, the impossible shapes signed with bloomington label secretly canadian released 'we like it wild' and toured nationally and internationally.around the same time, john wilkes booze was reformed in its classic 'five pillars of soul' line-up.after touring the western us in 2004, john wilkes booze was signed to olympia, wa-based kill rock stars.his solo debut by the horns of happiness a sea as a shore was released by secretly canadian in 2004.in 2005, deer teamed up with drummer and visual artist shelley harrison to form the first performance version of the horns of happiness touring extensively through the us, sharing the stage with acts such as man man, silver jews, old time relijun, danielson famile, joanna newsome, and the dirty projectors, among others, while garnering acclaim in publications such as magnet, dusted and skyscraper magazines. | aaron deer | genre | indie rock <tsp> aaron deer | associatedband/associatedmusicalartist | wee giant <tsp> aaron deer | background | solo singer <tsp> aaron deer | origin | indianapolis <tsp> aaron deer | origin | indiana | aaron deer (born november 1, 1980) is an american songwriter and multi-instrumentalist originally from indianapolis, indiana, united states, now residing in oakland, california.in the winter of 2009, deer relocated to california and continues work with the horns of happiness, royal geography society, farmer dave scher and wee giant, among others, while co-running the magnetic south cassette label.in 1999, deer and barth moved to bloomington to attend indiana university and they restarted the band there. |
gaussia (minor planet designation: 1001 gaussia), provisional designation 1923 oa, is a dark background asteroid from the outer regions of the asteroid belt, approximately 73 kilometers in diameter.it was discovered on 8 august 1923, by soviet astronomer sergey belyavsky at the simeiz observatory on the crimean peninsula.the asteroid was named after german mathematician carl friedrich gauss.gauss computed the orbit of ceres, and 1001 gaussia was named along with 1000 piazzia, and 1002 olbersia in part for their work on ceres, with names for giuseppe piazzi, who found ceres, and heinrich wilhelm matthias olbers, who recovered it later that year.it orbits the sun in the outer main-belt at a distance of 2.8–3.6 au once every 5 years and 9 months (2,100 days).its orbit has an eccentricity of 0.13 and an inclination of 9° with respect to the ecliptic.the asteroid was first identified as a907 xc at taunton observatory (803) in december 1907.the body's observation arc begins at unso in january 1908, more than 15 years prior to its official discovery observation at simeiz.its type is closest to the primitive p-type asteroids, followed by the common carbonaceous c-type asteroids.lightcurve analysis gave a well-defined rotation period of 20.99 hours with a brightness amplitude of 0.11 magnitude (u=3).lower-rated lightcurves with a divergent period of 4.08 and 9.17 hours were previously obtained in 2005 and 2009, respectively (u=1/2-).he is also honored by the lunar crater gauss.1001 gaussia was named as part of trio honoring the events surrounding the discovery of ceres in 1801.carl friedrich gauss who computed the orbit of ceres was for 1001 gaussia, 1000 piazzia for giuseppe piazzi and 1002 olbersia for heinrich wilhelm matthias olbers.olbers recovered ceres after it has passed behind the sun and returned.in the next few years only three more astronomical bodies were found between mars and jupiter, pallas, juno, and 4 vesta, however it would be 37 years before another asteroid was found, 5 astraea in 1845. | 1001 gaussia | discoverer | sergey belyavsky <tsp> 1001 gaussia | epoch | 2015-06-27 <tsp> 1001 gaussia | formername | a911 md <tsp> 1001 gaussia | orbitalperiod | 575 days <tsp> 1001 gaussia | periapsis | 41911339455312 kilometres | no related information |
aaron deer (born november 1, 1980) is an american songwriter and multi-instrumentalist originally from indianapolis, indiana, united states, now residing in oakland, california.he is best known for his work in the bloomington music scene in the early 2000s, playing with bands such as the impossible shapes, john wilkes booze, and the horns of happiness.in the winter of 2009, deer relocated to california and continues work with the horns of happiness, royal geography society, farmer dave scher and wee giant, among others, while co-running the magnetic south cassette label.in 1999, deer and barth moved to bloomington to attend indiana university and they restarted the band there.the group released their first record, 'the great migration', in 2000 and followed with 2 subsequent releases with indianapolis-based label recordhead/mr.whiggs.in 2003, the impossible shapes signed with bloomington label secretly canadian released 'we like it wild' and toured nationally and internationally.around the same time, john wilkes booze was reformed in its classic 'five pillars of soul' line-up.after touring the western us in 2004, john wilkes booze was signed to olympia, wa-based kill rock stars.his solo debut by the horns of happiness a sea as a shore was released by secretly canadian in 2004.in 2005, deer teamed up with drummer and visual artist shelley harrison to form the first performance version of the horns of happiness touring extensively through the us, sharing the stage with acts such as man man, silver jews, old time relijun, danielson famile, joanna newsome, and the dirty projectors, among others, while garnering acclaim in publications such as magnet, dusted and skyscraper magazines. | aaron deer | genre | indie rock <tsp> aaron deer | associatedband/associatedmusicalartist | wee giant <tsp> aaron deer | background | solo singer <tsp> aaron deer | origin | indianapolis <tsp> aaron deer | origin | indiana | aaron deer (born november 1, 1980) is an american songwriter and multi-instrumentalist originally from indianapolis, indiana, united states, now residing in oakland, california.in the winter of 2009, deer relocated to california and continues work with the horns of happiness, royal geography society, farmer dave scher and wee giant, among others, while co-running the magnetic south cassette label.in 1999, deer and barth moved to bloomington to attend indiana university and they restarted the band there. |
aaron deer (born november 1, 1980) is an american songwriter and multi-instrumentalist originally from indianapolis, indiana, united states, now residing in oakland, california.he is best known for his work in the bloomington music scene in the early 2000s, playing with bands such as the impossible shapes, john wilkes booze, and the horns of happiness.in the winter of 2009, deer relocated to california and continues work with the horns of happiness, royal geography society, farmer dave scher and wee giant, among others, while co-running the magnetic south cassette label.in 1999, deer and barth moved to bloomington to attend indiana university and they restarted the band there.the group released their first record, 'the great migration', in 2000 and followed with 2 subsequent releases with indianapolis-based label recordhead/mr.whiggs.in 2003, the impossible shapes signed with bloomington label secretly canadian released 'we like it wild' and toured nationally and internationally.around the same time, john wilkes booze was reformed in its classic 'five pillars of soul' line-up.after touring the western us in 2004, john wilkes booze was signed to olympia, wa-based kill rock stars.his solo debut by the horns of happiness a sea as a shore was released by secretly canadian in 2004.in 2005, deer teamed up with drummer and visual artist shelley harrison to form the first performance version of the horns of happiness touring extensively through the us, sharing the stage with acts such as man man, silver jews, old time relijun, danielson famile, joanna newsome, and the dirty projectors, among others, while garnering acclaim in publications such as magnet, dusted and skyscraper magazines. | aaron deer | genre | indie rock <tsp> aaron deer | associatedband/associatedmusicalartist | wee giant <tsp> aaron deer | background | solo singer <tsp> aaron deer | origin | indianapolis <tsp> aaron deer | origin | indiana | aaron deer (born november 1, 1980) is an american songwriter and multi-instrumentalist originally from indianapolis, indiana, united states, now residing in oakland, california.in the winter of 2009, deer relocated to california and continues work with the horns of happiness, royal geography society, farmer dave scher and wee giant, among others, while co-running the magnetic south cassette label.in 1999, deer and barth moved to bloomington to attend indiana university and they restarted the band there. |
gaussia (minor planet designation: 1001 gaussia), provisional designation 1923 oa, is a dark background asteroid from the outer regions of the asteroid belt, approximately 73 kilometers in diameter.it was discovered on 8 august 1923, by soviet astronomer sergey belyavsky at the simeiz observatory on the crimean peninsula.the asteroid was named after german mathematician carl friedrich gauss.gauss computed the orbit of ceres, and 1001 gaussia was named along with 1000 piazzia, and 1002 olbersia in part for their work on ceres, with names for giuseppe piazzi, who found ceres, and heinrich wilhelm matthias olbers, who recovered it later that year.it orbits the sun in the outer main-belt at a distance of 2.8–3.6 au once every 5 years and 9 months (2,100 days).its orbit has an eccentricity of 0.13 and an inclination of 9° with respect to the ecliptic.the asteroid was first identified as a907 xc at taunton observatory (803) in december 1907.the body's observation arc begins at unso in january 1908, more than 15 years prior to its official discovery observation at simeiz.its type is closest to the primitive p-type asteroids, followed by the common carbonaceous c-type asteroids.lightcurve analysis gave a well-defined rotation period of 20.99 hours with a brightness amplitude of 0.11 magnitude (u=3).lower-rated lightcurves with a divergent period of 4.08 and 9.17 hours were previously obtained in 2005 and 2009, respectively (u=1/2-).he is also honored by the lunar crater gauss.1001 gaussia was named as part of trio honoring the events surrounding the discovery of ceres in 1801.carl friedrich gauss who computed the orbit of ceres was for 1001 gaussia, 1000 piazzia for giuseppe piazzi and 1002 olbersia for heinrich wilhelm matthias olbers.olbers recovered ceres after it has passed behind the sun and returned.in the next few years only three more astronomical bodies were found between mars and jupiter, pallas, juno, and 4 vesta, however it would be 37 years before another asteroid was found, 5 astraea in 1845. | gildsman | lustre | boltspreet <tsp> gildsman | uncivilish | upflicker | no related information |
gaussia (minor planet designation: 1001 gaussia), provisional designation 1923 oa, is a dark background asteroid from the outer regions of the asteroid belt, approximately 73 kilometers in diameter.it was discovered on 8 august 1923, by soviet astronomer sergey belyavsky at the simeiz observatory on the crimean peninsula.the asteroid was named after german mathematician carl friedrich gauss.gauss computed the orbit of ceres, and 1001 gaussia was named along with 1000 piazzia, and 1002 olbersia in part for their work on ceres, with names for giuseppe piazzi, who found ceres, and heinrich wilhelm matthias olbers, who recovered it later that year.it orbits the sun in the outer main-belt at a distance of 2.8–3.6 au once every 5 years and 9 months (2,100 days).its orbit has an eccentricity of 0.13 and an inclination of 9° with respect to the ecliptic.the asteroid was first identified as a907 xc at taunton observatory (803) in december 1907.the body's observation arc begins at unso in january 1908, more than 15 years prior to its official discovery observation at simeiz.its type is closest to the primitive p-type asteroids, followed by the common carbonaceous c-type asteroids.lightcurve analysis gave a well-defined rotation period of 20.99 hours with a brightness amplitude of 0.11 magnitude (u=3).lower-rated lightcurves with a divergent period of 4.08 and 9.17 hours were previously obtained in 2005 and 2009, respectively (u=1/2-).he is also honored by the lunar crater gauss.1001 gaussia was named as part of trio honoring the events surrounding the discovery of ceres in 1801.carl friedrich gauss who computed the orbit of ceres was for 1001 gaussia, 1000 piazzia for giuseppe piazzi and 1002 olbersia for heinrich wilhelm matthias olbers.olbers recovered ceres after it has passed behind the sun and returned.in the next few years only three more astronomical bodies were found between mars and jupiter, pallas, juno, and 4 vesta, however it would be 37 years before another asteroid was found, 5 astraea in 1845. | 1001 gaussia | discoverer | sergey belyavsky <tsp> 1001 gaussia | epoch | 2015-06-27 <tsp> 1001 gaussia | orbitalperiod | 575 days <tsp> 1001 gaussia | periapsis | 41911339455312 kilometres <tsp> 1001 gaussia | absolutemagnitude | 97 | no related information |
aaron deer (born november 1, 1980) is an american songwriter and multi-instrumentalist originally from indianapolis, indiana, united states, now residing in oakland, california.he is best known for his work in the bloomington music scene in the early 2000s, playing with bands such as the impossible shapes, john wilkes booze, and the horns of happiness.in the winter of 2009, deer relocated to california and continues work with the horns of happiness, royal geography society, farmer dave scher and wee giant, among others, while co-running the magnetic south cassette label.in 1999, deer and barth moved to bloomington to attend indiana university and they restarted the band there.the group released their first record, 'the great migration', in 2000 and followed with 2 subsequent releases with indianapolis-based label recordhead/mr.whiggs.in 2003, the impossible shapes signed with bloomington label secretly canadian released 'we like it wild' and toured nationally and internationally.around the same time, john wilkes booze was reformed in its classic 'five pillars of soul' line-up.after touring the western us in 2004, john wilkes booze was signed to olympia, wa-based kill rock stars.his solo debut by the horns of happiness a sea as a shore was released by secretly canadian in 2004.in 2005, deer teamed up with drummer and visual artist shelley harrison to form the first performance version of the horns of happiness touring extensively through the us, sharing the stage with acts such as man man, silver jews, old time relijun, danielson famile, joanna newsome, and the dirty projectors, among others, while garnering acclaim in publications such as magnet, dusted and skyscraper magazines. | arenig | pasis | sixing <tsp> arenig | ampelography | displumed | no related information |
gaussia (minor planet designation: 1001 gaussia), provisional designation 1923 oa, is a dark background asteroid from the outer regions of the asteroid belt, approximately 73 kilometers in diameter.it was discovered on 8 august 1923, by soviet astronomer sergey belyavsky at the simeiz observatory on the crimean peninsula.the asteroid was named after german mathematician carl friedrich gauss.gauss computed the orbit of ceres, and 1001 gaussia was named along with 1000 piazzia, and 1002 olbersia in part for their work on ceres, with names for giuseppe piazzi, who found ceres, and heinrich wilhelm matthias olbers, who recovered it later that year.it orbits the sun in the outer main-belt at a distance of 2.8–3.6 au once every 5 years and 9 months (2,100 days).its orbit has an eccentricity of 0.13 and an inclination of 9° with respect to the ecliptic.the asteroid was first identified as a907 xc at taunton observatory (803) in december 1907.the body's observation arc begins at unso in january 1908, more than 15 years prior to its official discovery observation at simeiz.its type is closest to the primitive p-type asteroids, followed by the common carbonaceous c-type asteroids.lightcurve analysis gave a well-defined rotation period of 20.99 hours with a brightness amplitude of 0.11 magnitude (u=3).lower-rated lightcurves with a divergent period of 4.08 and 9.17 hours were previously obtained in 2005 and 2009, respectively (u=1/2-).he is also honored by the lunar crater gauss.1001 gaussia was named as part of trio honoring the events surrounding the discovery of ceres in 1801.carl friedrich gauss who computed the orbit of ceres was for 1001 gaussia, 1000 piazzia for giuseppe piazzi and 1002 olbersia for heinrich wilhelm matthias olbers.olbers recovered ceres after it has passed behind the sun and returned.in the next few years only three more astronomical bodies were found between mars and jupiter, pallas, juno, and 4 vesta, however it would be 37 years before another asteroid was found, 5 astraea in 1845. | coagulin | noninterleaved | ectases <tsp> coagulin | homeostases | plerosis | no related information |
aaron deer (born november 1, 1980) is an american songwriter and multi-instrumentalist originally from indianapolis, indiana, united states, now residing in oakland, california.he is best known for his work in the bloomington music scene in the early 2000s, playing with bands such as the impossible shapes, john wilkes booze, and the horns of happiness.in the winter of 2009, deer relocated to california and continues work with the horns of happiness, royal geography society, farmer dave scher and wee giant, among others, while co-running the magnetic south cassette label.in 1999, deer and barth moved to bloomington to attend indiana university and they restarted the band there.the group released their first record, 'the great migration', in 2000 and followed with 2 subsequent releases with indianapolis-based label recordhead/mr.whiggs.in 2003, the impossible shapes signed with bloomington label secretly canadian released 'we like it wild' and toured nationally and internationally.around the same time, john wilkes booze was reformed in its classic 'five pillars of soul' line-up.after touring the western us in 2004, john wilkes booze was signed to olympia, wa-based kill rock stars.his solo debut by the horns of happiness a sea as a shore was released by secretly canadian in 2004.in 2005, deer teamed up with drummer and visual artist shelley harrison to form the first performance version of the horns of happiness touring extensively through the us, sharing the stage with acts such as man man, silver jews, old time relijun, danielson famile, joanna newsome, and the dirty projectors, among others, while garnering acclaim in publications such as magnet, dusted and skyscraper magazines. | flaxen | supremeness | shrug <tsp> flaxen | passival | doghole | no related information |
helena (minor planet designation: 101 helena) is a large, rocky main-belt asteroid.it was discovered by canadian-american astronomer j. c. watson on august 15, 1868, and was named after helen of troy in greek mythology.this object is orbiting the sun with a period of 4.16 years and an eccentricity of 0.14.its orbital plane is inclined by 10.2° to the plane of the ecliptic.radar observations were made of this object on oct 7 and 19, 2001 from the arecibo observatory.analysis of the data gave an estimated ellipsoidal diameter of 71×63×63 ± 16% km.the mean diameter estimated from iras infrared measurements is 66 km, in agreement with the radar findings.it is classified as an s-type asteroid in the tholen system, suggesting a predominantly silicate composition.101 helena is spinning on its axis with a period of 23 hours. | 101 helena | discoverer | james craig watson <tsp> james craig watson | almamater | university of michigan <tsp> 101 helena | absolutemagnitude | 833 <tsp> james craig watson | nationality | canada <tsp> james craig watson | deathplace | madison wisconsin | no related information |
helena (minor planet designation: 101 helena) is a large, rocky main-belt asteroid.it was discovered by canadian-american astronomer j. c. watson on august 15, 1868, and was named after helen of troy in greek mythology.this object is orbiting the sun with a period of 4.16 years and an eccentricity of 0.14.its orbital plane is inclined by 10.2° to the plane of the ecliptic.radar observations were made of this object on oct 7 and 19, 2001 from the arecibo observatory.analysis of the data gave an estimated ellipsoidal diameter of 71×63×63 ± 16% km.the mean diameter estimated from iras infrared measurements is 66 km, in agreement with the radar findings.it is classified as an s-type asteroid in the tholen system, suggesting a predominantly silicate composition.101 helena is spinning on its axis with a period of 23 hours. | 101 helena | discoverer | james craig watson <tsp> james craig watson | almamater | university of michigan <tsp> 101 helena | absolutemagnitude | 833 <tsp> james craig watson | nationality | canada <tsp> james craig watson | deathplace | madison wisconsin | no related information |
aaron deer (born november 1, 1980) is an american songwriter and multi-instrumentalist originally from indianapolis, indiana, united states, now residing in oakland, california.he is best known for his work in the bloomington music scene in the early 2000s, playing with bands such as the impossible shapes, john wilkes booze, and the horns of happiness.in the winter of 2009, deer relocated to california and continues work with the horns of happiness, royal geography society, farmer dave scher and wee giant, among others, while co-running the magnetic south cassette label.in 1999, deer and barth moved to bloomington to attend indiana university and they restarted the band there.the group released their first record, 'the great migration', in 2000 and followed with 2 subsequent releases with indianapolis-based label recordhead/mr.whiggs.in 2003, the impossible shapes signed with bloomington label secretly canadian released 'we like it wild' and toured nationally and internationally.around the same time, john wilkes booze was reformed in its classic 'five pillars of soul' line-up.after touring the western us in 2004, john wilkes booze was signed to olympia, wa-based kill rock stars.his solo debut by the horns of happiness a sea as a shore was released by secretly canadian in 2004.in 2005, deer teamed up with drummer and visual artist shelley harrison to form the first performance version of the horns of happiness touring extensively through the us, sharing the stage with acts such as man man, silver jews, old time relijun, danielson famile, joanna newsome, and the dirty projectors, among others, while garnering acclaim in publications such as magnet, dusted and skyscraper magazines. | amain | dazzling | autonephrotoxin <tsp> amain | decapitalize | checkerboard | no related information |
helena (minor planet designation: 101 helena) is a large, rocky main-belt asteroid.it was discovered by canadian-american astronomer j. c. watson on august 15, 1868, and was named after helen of troy in greek mythology.this object is orbiting the sun with a period of 4.16 years and an eccentricity of 0.14.its orbital plane is inclined by 10.2° to the plane of the ecliptic.radar observations were made of this object on oct 7 and 19, 2001 from the arecibo observatory.analysis of the data gave an estimated ellipsoidal diameter of 71×63×63 ± 16% km.the mean diameter estimated from iras infrared measurements is 66 km, in agreement with the radar findings.it is classified as an s-type asteroid in the tholen system, suggesting a predominantly silicate composition.101 helena is spinning on its axis with a period of 23 hours. | 101 helena | discoverer | james craig watson <tsp> james craig watson | almamater | university of michigan <tsp> 101 helena | absolutemagnitude | 833 <tsp> james craig watson | nationality | canada <tsp> james craig watson | deathplace | madison wisconsin | no related information |
aaron deer (born november 1, 1980) is an american songwriter and multi-instrumentalist originally from indianapolis, indiana, united states, now residing in oakland, california.he is best known for his work in the bloomington music scene in the early 2000s, playing with bands such as the impossible shapes, john wilkes booze, and the horns of happiness.in the winter of 2009, deer relocated to california and continues work with the horns of happiness, royal geography society, farmer dave scher and wee giant, among others, while co-running the magnetic south cassette label.in 1999, deer and barth moved to bloomington to attend indiana university and they restarted the band there.the group released their first record, 'the great migration', in 2000 and followed with 2 subsequent releases with indianapolis-based label recordhead/mr.whiggs.in 2003, the impossible shapes signed with bloomington label secretly canadian released 'we like it wild' and toured nationally and internationally.around the same time, john wilkes booze was reformed in its classic 'five pillars of soul' line-up.after touring the western us in 2004, john wilkes booze was signed to olympia, wa-based kill rock stars.his solo debut by the horns of happiness a sea as a shore was released by secretly canadian in 2004.in 2005, deer teamed up with drummer and visual artist shelley harrison to form the first performance version of the horns of happiness touring extensively through the us, sharing the stage with acts such as man man, silver jews, old time relijun, danielson famile, joanna newsome, and the dirty projectors, among others, while garnering acclaim in publications such as magnet, dusted and skyscraper magazines. | sclaffer | resight | grammaticalness <tsp> sclaffer | gingalls | macarism | no related information |
aaron deer (born november 1, 1980) is an american songwriter and multi-instrumentalist originally from indianapolis, indiana, united states, now residing in oakland, california.he is best known for his work in the bloomington music scene in the early 2000s, playing with bands such as the impossible shapes, john wilkes booze, and the horns of happiness.in the winter of 2009, deer relocated to california and continues work with the horns of happiness, royal geography society, farmer dave scher and wee giant, among others, while co-running the magnetic south cassette label.in 1999, deer and barth moved to bloomington to attend indiana university and they restarted the band there.the group released their first record, 'the great migration', in 2000 and followed with 2 subsequent releases with indianapolis-based label recordhead/mr.whiggs.in 2003, the impossible shapes signed with bloomington label secretly canadian released 'we like it wild' and toured nationally and internationally.around the same time, john wilkes booze was reformed in its classic 'five pillars of soul' line-up.after touring the western us in 2004, john wilkes booze was signed to olympia, wa-based kill rock stars.his solo debut by the horns of happiness a sea as a shore was released by secretly canadian in 2004.in 2005, deer teamed up with drummer and visual artist shelley harrison to form the first performance version of the horns of happiness touring extensively through the us, sharing the stage with acts such as man man, silver jews, old time relijun, danielson famile, joanna newsome, and the dirty projectors, among others, while garnering acclaim in publications such as magnet, dusted and skyscraper magazines. | aaron deer | genre | indie rock <tsp> aaron deer | origin | united states <tsp> aaron deer | background | solo singer <tsp> aaron deer | origin | indiana <tsp> aaron deer | associatedband/associatedmusicalartist | the horns of happiness | aaron deer (born november 1, 1980) is an american songwriter and multi-instrumentalist originally from indianapolis, indiana, united states, now residing in oakland, california.in the winter of 2009, deer relocated to california and continues work with the horns of happiness, royal geography society, farmer dave scher and wee giant, among others, while co-running the magnetic south cassette label.in 1999, deer and barth moved to bloomington to attend indiana university and they restarted the band there.in 2005, deer teamed up with drummer and visual artist shelley harrison to form the first performance version of the horns of happiness touring extensively through the us, sharing the stage with acts such as man man, silver jews, old time relijun, danielson famile, joanna newsome, and the dirty projectors, among others, while garnering acclaim in publications such as magnet, dusted and skyscraper magazines. |
helena (minor planet designation: 101 helena) is a large, rocky main-belt asteroid.it was discovered by canadian-american astronomer j. c. watson on august 15, 1868, and was named after helen of troy in greek mythology.this object is orbiting the sun with a period of 4.16 years and an eccentricity of 0.14.its orbital plane is inclined by 10.2° to the plane of the ecliptic.radar observations were made of this object on oct 7 and 19, 2001 from the arecibo observatory.analysis of the data gave an estimated ellipsoidal diameter of 71×63×63 ± 16% km.the mean diameter estimated from iras infrared measurements is 66 km, in agreement with the radar findings.it is classified as an s-type asteroid in the tholen system, suggesting a predominantly silicate composition.101 helena is spinning on its axis with a period of 23 hours. | trans | goethite | antwise <tsp> trans | scapulars | kokos | no related information |
aaron deer (born november 1, 1980) is an american songwriter and multi-instrumentalist originally from indianapolis, indiana, united states, now residing in oakland, california.he is best known for his work in the bloomington music scene in the early 2000s, playing with bands such as the impossible shapes, john wilkes booze, and the horns of happiness.in the winter of 2009, deer relocated to california and continues work with the horns of happiness, royal geography society, farmer dave scher and wee giant, among others, while co-running the magnetic south cassette label.in 1999, deer and barth moved to bloomington to attend indiana university and they restarted the band there.the group released their first record, 'the great migration', in 2000 and followed with 2 subsequent releases with indianapolis-based label recordhead/mr.whiggs.in 2003, the impossible shapes signed with bloomington label secretly canadian released 'we like it wild' and toured nationally and internationally.around the same time, john wilkes booze was reformed in its classic 'five pillars of soul' line-up.after touring the western us in 2004, john wilkes booze was signed to olympia, wa-based kill rock stars.his solo debut by the horns of happiness a sea as a shore was released by secretly canadian in 2004.in 2005, deer teamed up with drummer and visual artist shelley harrison to form the first performance version of the horns of happiness touring extensively through the us, sharing the stage with acts such as man man, silver jews, old time relijun, danielson famile, joanna newsome, and the dirty projectors, among others, while garnering acclaim in publications such as magnet, dusted and skyscraper magazines. | aaron deer | genre | indie rock <tsp> aaron deer | origin | united states <tsp> aaron deer | background | solo singer <tsp> aaron deer | origin | indiana <tsp> aaron deer | associatedband/associatedmusicalartist | the horns of happiness | aaron deer (born november 1, 1980) is an american songwriter and multi-instrumentalist originally from indianapolis, indiana, united states, now residing in oakland, california.in the winter of 2009, deer relocated to california and continues work with the horns of happiness, royal geography society, farmer dave scher and wee giant, among others, while co-running the magnetic south cassette label.in 1999, deer and barth moved to bloomington to attend indiana university and they restarted the band there.in 2005, deer teamed up with drummer and visual artist shelley harrison to form the first performance version of the horns of happiness touring extensively through the us, sharing the stage with acts such as man man, silver jews, old time relijun, danielson famile, joanna newsome, and the dirty projectors, among others, while garnering acclaim in publications such as magnet, dusted and skyscraper magazines. |
helena (minor planet designation: 101 helena) is a large, rocky main-belt asteroid.it was discovered by canadian-american astronomer j. c. watson on august 15, 1868, and was named after helen of troy in greek mythology.this object is orbiting the sun with a period of 4.16 years and an eccentricity of 0.14.its orbital plane is inclined by 10.2° to the plane of the ecliptic.radar observations were made of this object on oct 7 and 19, 2001 from the arecibo observatory.analysis of the data gave an estimated ellipsoidal diameter of 71×63×63 ± 16% km.the mean diameter estimated from iras infrared measurements is 66 km, in agreement with the radar findings.it is classified as an s-type asteroid in the tholen system, suggesting a predominantly silicate composition.101 helena is spinning on its axis with a period of 23 hours. | 101 helena | discoverer | james craig watson <tsp> james craig watson | almamater | university of michigan <tsp> 101 helena | epoch | 2006-12-31 <tsp> james craig watson | nationality | canada <tsp> james craig watson | deathplace | madison wisconsin | no related information |
helena (minor planet designation: 101 helena) is a large, rocky main-belt asteroid.it was discovered by canadian-american astronomer j. c. watson on august 15, 1868, and was named after helen of troy in greek mythology.this object is orbiting the sun with a period of 4.16 years and an eccentricity of 0.14.its orbital plane is inclined by 10.2° to the plane of the ecliptic.radar observations were made of this object on oct 7 and 19, 2001 from the arecibo observatory.analysis of the data gave an estimated ellipsoidal diameter of 71×63×63 ± 16% km.the mean diameter estimated from iras infrared measurements is 66 km, in agreement with the radar findings.it is classified as an s-type asteroid in the tholen system, suggesting a predominantly silicate composition.101 helena is spinning on its axis with a period of 23 hours. | 101 helena | discoverer | james craig watson <tsp> james craig watson | almamater | university of michigan <tsp> 101 helena | epoch | 2006-12-31 <tsp> james craig watson | nationality | canada <tsp> james craig watson | deathplace | madison wisconsin | no related information |
arianespace sa is a french company founded in 1980 as the world's first commercial launch service provider.it undertakes the operation and marketing of the ariane programme.the company offers a number of different launch vehicles: the heavy-lift ariane 5 for dual launches to geostationary transfer orbit, the soyuz-2 as a medium-lift alternative, and the solid-fueled vega for lighter payloads.as of may 2021, arianespace had launched more than 850 satellites in 287 launches over 41 years.the first commercial flight managed by the new entity was spacenet f1 launched on 23 may 1984.arianespace uses the guiana space centre in french guiana as its main launch site.through shareholding in starsem, it can also offer commercial soyuz launches from the baikonur spaceport in kazakhstan.it has its headquarters in évry-courcouronnes, essonne, france.prior to the esa's formation, france had been lobbying for the development of a new european expendable launch system to serve as a replacement for the europa rocket.accordingly, one of the first programmes launched by the esa was the ariane heavy launcher.the express purpose of this launcher was to facilitate the delivery of commercial satellites into geosynchronous orbit.france was the largest stakeholder in the ariane development programme.french aerospace manufacturer aérospatiale served as the prime contractor and held responsibility for performing the integration of all sections of the vehicle, while french engine manufacturer société européenne de propulsion (sep) provided the first, second and third stage engines (the third stage engines were produced in partnership with german aerospace manufacturer mbb).other major companies involved included the french firms air liquide and matra, swedish manufacturer volvo, and german aircraft producer dornier flugzeugwerke.development of the third stage was a major focus point for the project - prior to ariane, only the united states had ever flown a launcher that utilised hydrogen-powered upper stages.immediately following the successful first test launch of an ariane 1 on 24 december 1979, the french space agency centre national d'études spatiales (cnes) and the esa created a new company, arianespace, for the purpose of promoting, marketing, and managing ariane operations.according to arianespace, at the time of its establishment, it was the world's first launch services company.following a further three test launches, the first commercial launch took place on 10 september 1982, which ended in failure as a result of a turbopump having failed in the third stage.the six remaining flights of the ariane 1 were successful, with the final flight occurring during february 1986.as a result of these repeated successes, orders for the ariane launcher quickly mounted up; by early 1984, a total of 27 satellites had been booked to use ariane, which was estimated to be half of the world's market at that time.as a result of the commercial success, after the tenth ariane mission was flown, the esa formally transferred responsibility for ariane over to arianespace.by early 1986, the ariane 1, along with its ariane 2 and ariane 3 derivates, were the dominant launcher on the world market.the ariane 2 and ariane 3 were short-lived platforms while the more extensive ariane 4 was being developed; it was a considerably larger and more flexible launcher that the earlier members of its family, having been intended from the onset to compete with the upper end of launchers worldwide.in comparison, while the ariane 1 had a typical weight of 207 tonnes and could launch payloads of up to 1.7 tonnes into orbit; the larger ariane 4 had a typical weight of 470 tonnes and could orbit payloads of up to 4.2 tonnes.despite this, the ariane 4 was actually 15 per cent smaller than the ariane 3.on 15 june 1988, the first successful launch of the ariane 4 was conducted. | arianespace | locationcity | courcouronnes <tsp> guiana space centre | headquarter | kourou french guiana <tsp> ela-3 | site | guiana space centre <tsp> ariane 5 | launchsite | ela-3 <tsp> ela-3 | operator | arianespace | arianespace sa is a french company founded in 1980 as the world's first commercial launch service provider.arianespace uses the guiana space centre in french guiana as its main launch site.french aerospace manufacturer aérospatiale served as the prime contractor and held responsibility for performing the integration of all sections of the vehicle, while french engine manufacturer société européenne de propulsion (sep) provided the first, second and third stage engines (the third stage engines were produced in partnership with german aerospace manufacturer mbb).development of the third stage was a major focus point for the project - prior to ariane, only the united states had ever flown a launcher that utilised hydrogen-powered upper stages.immediately following the successful first test launch of an ariane 1 on 24 december 1979, the french space agency centre national d'études spatiales (cnes) and the esa created a new company, arianespace, for the purpose of promoting, marketing, and managing ariane operations. |
aaron deer (born november 1, 1980) is an american songwriter and multi-instrumentalist originally from indianapolis, indiana, united states, now residing in oakland, california.he is best known for his work in the bloomington music scene in the early 2000s, playing with bands such as the impossible shapes, john wilkes booze, and the horns of happiness.in the winter of 2009, deer relocated to california and continues work with the horns of happiness, royal geography society, farmer dave scher and wee giant, among others, while co-running the magnetic south cassette label.in 1999, deer and barth moved to bloomington to attend indiana university and they restarted the band there.the group released their first record, 'the great migration', in 2000 and followed with 2 subsequent releases with indianapolis-based label recordhead/mr.whiggs.in 2003, the impossible shapes signed with bloomington label secretly canadian released 'we like it wild' and toured nationally and internationally.around the same time, john wilkes booze was reformed in its classic 'five pillars of soul' line-up.after touring the western us in 2004, john wilkes booze was signed to olympia, wa-based kill rock stars.his solo debut by the horns of happiness a sea as a shore was released by secretly canadian in 2004.in 2005, deer teamed up with drummer and visual artist shelley harrison to form the first performance version of the horns of happiness touring extensively through the us, sharing the stage with acts such as man man, silver jews, old time relijun, danielson famile, joanna newsome, and the dirty projectors, among others, while garnering acclaim in publications such as magnet, dusted and skyscraper magazines. | fortressed | mystagog | callityped <tsp> fortressed | nonspeculativeness | sealless | no related information |
helena (minor planet designation: 101 helena) is a large, rocky main-belt asteroid.it was discovered by canadian-american astronomer j. c. watson on august 15, 1868, and was named after helen of troy in greek mythology.this object is orbiting the sun with a period of 4.16 years and an eccentricity of 0.14.its orbital plane is inclined by 10.2° to the plane of the ecliptic.radar observations were made of this object on oct 7 and 19, 2001 from the arecibo observatory.analysis of the data gave an estimated ellipsoidal diameter of 71×63×63 ± 16% km.the mean diameter estimated from iras infrared measurements is 66 km, in agreement with the radar findings.it is classified as an s-type asteroid in the tholen system, suggesting a predominantly silicate composition.101 helena is spinning on its axis with a period of 23 hours. | 101 helena | discoverer | james craig watson <tsp> james craig watson | almamater | university of michigan <tsp> 101 helena | orbitalperiod | 15166700000000003 days <tsp> james craig watson | nationality | canada <tsp> james craig watson | deathplace | madison wisconsin | no related information |
arianespace sa is a french company founded in 1980 as the world's first commercial launch service provider.it undertakes the operation and marketing of the ariane programme.the company offers a number of different launch vehicles: the heavy-lift ariane 5 for dual launches to geostationary transfer orbit, the soyuz-2 as a medium-lift alternative, and the solid-fueled vega for lighter payloads.as of may 2021, arianespace had launched more than 850 satellites in 287 launches over 41 years.the first commercial flight managed by the new entity was spacenet f1 launched on 23 may 1984.arianespace uses the guiana space centre in french guiana as its main launch site.through shareholding in starsem, it can also offer commercial soyuz launches from the baikonur spaceport in kazakhstan.it has its headquarters in évry-courcouronnes, essonne, france.prior to the esa's formation, france had been lobbying for the development of a new european expendable launch system to serve as a replacement for the europa rocket.accordingly, one of the first programmes launched by the esa was the ariane heavy launcher.the express purpose of this launcher was to facilitate the delivery of commercial satellites into geosynchronous orbit.france was the largest stakeholder in the ariane development programme.french aerospace manufacturer aérospatiale served as the prime contractor and held responsibility for performing the integration of all sections of the vehicle, while french engine manufacturer société européenne de propulsion (sep) provided the first, second and third stage engines (the third stage engines were produced in partnership with german aerospace manufacturer mbb).other major companies involved included the french firms air liquide and matra, swedish manufacturer volvo, and german aircraft producer dornier flugzeugwerke.development of the third stage was a major focus point for the project - prior to ariane, only the united states had ever flown a launcher that utilised hydrogen-powered upper stages.immediately following the successful first test launch of an ariane 1 on 24 december 1979, the french space agency centre national d'études spatiales (cnes) and the esa created a new company, arianespace, for the purpose of promoting, marketing, and managing ariane operations.according to arianespace, at the time of its establishment, it was the world's first launch services company.following a further three test launches, the first commercial launch took place on 10 september 1982, which ended in failure as a result of a turbopump having failed in the third stage.the six remaining flights of the ariane 1 were successful, with the final flight occurring during february 1986.as a result of these repeated successes, orders for the ariane launcher quickly mounted up; by early 1984, a total of 27 satellites had been booked to use ariane, which was estimated to be half of the world's market at that time.as a result of the commercial success, after the tenth ariane mission was flown, the esa formally transferred responsibility for ariane over to arianespace.by early 1986, the ariane 1, along with its ariane 2 and ariane 3 derivates, were the dominant launcher on the world market.the ariane 2 and ariane 3 were short-lived platforms while the more extensive ariane 4 was being developed; it was a considerably larger and more flexible launcher that the earlier members of its family, having been intended from the onset to compete with the upper end of launchers worldwide.in comparison, while the ariane 1 had a typical weight of 207 tonnes and could launch payloads of up to 1.7 tonnes into orbit; the larger ariane 4 had a typical weight of 470 tonnes and could orbit payloads of up to 4.2 tonnes.despite this, the ariane 4 was actually 15 per cent smaller than the ariane 3.on 15 june 1988, the first successful launch of the ariane 4 was conducted. | arianespace | locationcity | courcouronnes <tsp> guiana space centre | headquarter | kourou french guiana <tsp> ela-3 | site | guiana space centre <tsp> ariane 5 | launchsite | ela-3 <tsp> ela-3 | operator | arianespace | arianespace sa is a french company founded in 1980 as the world's first commercial launch service provider.arianespace uses the guiana space centre in french guiana as its main launch site.french aerospace manufacturer aérospatiale served as the prime contractor and held responsibility for performing the integration of all sections of the vehicle, while french engine manufacturer société européenne de propulsion (sep) provided the first, second and third stage engines (the third stage engines were produced in partnership with german aerospace manufacturer mbb).development of the third stage was a major focus point for the project - prior to ariane, only the united states had ever flown a launcher that utilised hydrogen-powered upper stages.immediately following the successful first test launch of an ariane 1 on 24 december 1979, the french space agency centre national d'études spatiales (cnes) and the esa created a new company, arianespace, for the purpose of promoting, marketing, and managing ariane operations. |
helena (minor planet designation: 101 helena) is a large, rocky main-belt asteroid.it was discovered by canadian-american astronomer j. c. watson on august 15, 1868, and was named after helen of troy in greek mythology.this object is orbiting the sun with a period of 4.16 years and an eccentricity of 0.14.its orbital plane is inclined by 10.2° to the plane of the ecliptic.radar observations were made of this object on oct 7 and 19, 2001 from the arecibo observatory.analysis of the data gave an estimated ellipsoidal diameter of 71×63×63 ± 16% km.the mean diameter estimated from iras infrared measurements is 66 km, in agreement with the radar findings.it is classified as an s-type asteroid in the tholen system, suggesting a predominantly silicate composition.101 helena is spinning on its axis with a period of 23 hours. | 101 helena | discoverer | james craig watson <tsp> james craig watson | almamater | university of michigan <tsp> 101 helena | orbitalperiod | 15166700000000003 days <tsp> james craig watson | nationality | canada <tsp> james craig watson | deathplace | madison wisconsin | no related information |
aaron deer (born november 1, 1980) is an american songwriter and multi-instrumentalist originally from indianapolis, indiana, united states, now residing in oakland, california.he is best known for his work in the bloomington music scene in the early 2000s, playing with bands such as the impossible shapes, john wilkes booze, and the horns of happiness.in the winter of 2009, deer relocated to california and continues work with the horns of happiness, royal geography society, farmer dave scher and wee giant, among others, while co-running the magnetic south cassette label.in 1999, deer and barth moved to bloomington to attend indiana university and they restarted the band there.the group released their first record, 'the great migration', in 2000 and followed with 2 subsequent releases with indianapolis-based label recordhead/mr.whiggs.in 2003, the impossible shapes signed with bloomington label secretly canadian released 'we like it wild' and toured nationally and internationally.around the same time, john wilkes booze was reformed in its classic 'five pillars of soul' line-up.after touring the western us in 2004, john wilkes booze was signed to olympia, wa-based kill rock stars.his solo debut by the horns of happiness a sea as a shore was released by secretly canadian in 2004.in 2005, deer teamed up with drummer and visual artist shelley harrison to form the first performance version of the horns of happiness touring extensively through the us, sharing the stage with acts such as man man, silver jews, old time relijun, danielson famile, joanna newsome, and the dirty projectors, among others, while garnering acclaim in publications such as magnet, dusted and skyscraper magazines. | pecht | botryoid | empowerment <tsp> pecht | gipon | cecitis | no related information |
arianespace sa is a french company founded in 1980 as the world's first commercial launch service provider.it undertakes the operation and marketing of the ariane programme.the company offers a number of different launch vehicles: the heavy-lift ariane 5 for dual launches to geostationary transfer orbit, the soyuz-2 as a medium-lift alternative, and the solid-fueled vega for lighter payloads.as of may 2021, arianespace had launched more than 850 satellites in 287 launches over 41 years.the first commercial flight managed by the new entity was spacenet f1 launched on 23 may 1984.arianespace uses the guiana space centre in french guiana as its main launch site.through shareholding in starsem, it can also offer commercial soyuz launches from the baikonur spaceport in kazakhstan.it has its headquarters in évry-courcouronnes, essonne, france.prior to the esa's formation, france had been lobbying for the development of a new european expendable launch system to serve as a replacement for the europa rocket.accordingly, one of the first programmes launched by the esa was the ariane heavy launcher.the express purpose of this launcher was to facilitate the delivery of commercial satellites into geosynchronous orbit.france was the largest stakeholder in the ariane development programme.french aerospace manufacturer aérospatiale served as the prime contractor and held responsibility for performing the integration of all sections of the vehicle, while french engine manufacturer société européenne de propulsion (sep) provided the first, second and third stage engines (the third stage engines were produced in partnership with german aerospace manufacturer mbb).other major companies involved included the french firms air liquide and matra, swedish manufacturer volvo, and german aircraft producer dornier flugzeugwerke.development of the third stage was a major focus point for the project - prior to ariane, only the united states had ever flown a launcher that utilised hydrogen-powered upper stages.immediately following the successful first test launch of an ariane 1 on 24 december 1979, the french space agency centre national d'études spatiales (cnes) and the esa created a new company, arianespace, for the purpose of promoting, marketing, and managing ariane operations.according to arianespace, at the time of its establishment, it was the world's first launch services company.following a further three test launches, the first commercial launch took place on 10 september 1982, which ended in failure as a result of a turbopump having failed in the third stage.the six remaining flights of the ariane 1 were successful, with the final flight occurring during february 1986.as a result of these repeated successes, orders for the ariane launcher quickly mounted up; by early 1984, a total of 27 satellites had been booked to use ariane, which was estimated to be half of the world's market at that time.as a result of the commercial success, after the tenth ariane mission was flown, the esa formally transferred responsibility for ariane over to arianespace.by early 1986, the ariane 1, along with its ariane 2 and ariane 3 derivates, were the dominant launcher on the world market.the ariane 2 and ariane 3 were short-lived platforms while the more extensive ariane 4 was being developed; it was a considerably larger and more flexible launcher that the earlier members of its family, having been intended from the onset to compete with the upper end of launchers worldwide.in comparison, while the ariane 1 had a typical weight of 207 tonnes and could launch payloads of up to 1.7 tonnes into orbit; the larger ariane 4 had a typical weight of 470 tonnes and could orbit payloads of up to 4.2 tonnes.despite this, the ariane 4 was actually 15 per cent smaller than the ariane 3.on 15 june 1988, the first successful launch of the ariane 4 was conducted. | puritanical | shareowner | pseudophellandrene <tsp> puritanical | material | sphagnums | no related information |
helena (minor planet designation: 101 helena) is a large, rocky main-belt asteroid.it was discovered by canadian-american astronomer j. c. watson on august 15, 1868, and was named after helen of troy in greek mythology.this object is orbiting the sun with a period of 4.16 years and an eccentricity of 0.14.its orbital plane is inclined by 10.2° to the plane of the ecliptic.radar observations were made of this object on oct 7 and 19, 2001 from the arecibo observatory.analysis of the data gave an estimated ellipsoidal diameter of 71×63×63 ± 16% km.the mean diameter estimated from iras infrared measurements is 66 km, in agreement with the radar findings.it is classified as an s-type asteroid in the tholen system, suggesting a predominantly silicate composition.101 helena is spinning on its axis with a period of 23 hours. | 101 helena | discoverer | james craig watson <tsp> james craig watson | almamater | university of michigan <tsp> 101 helena | orbitalperiod | 15166700000000003 days <tsp> james craig watson | nationality | canada <tsp> james craig watson | deathplace | madison wisconsin | no related information |
aaron deer (born november 1, 1980) is an american songwriter and multi-instrumentalist originally from indianapolis, indiana, united states, now residing in oakland, california.he is best known for his work in the bloomington music scene in the early 2000s, playing with bands such as the impossible shapes, john wilkes booze, and the horns of happiness.in the winter of 2009, deer relocated to california and continues work with the horns of happiness, royal geography society, farmer dave scher and wee giant, among others, while co-running the magnetic south cassette label.in 1999, deer and barth moved to bloomington to attend indiana university and they restarted the band there.the group released their first record, 'the great migration', in 2000 and followed with 2 subsequent releases with indianapolis-based label recordhead/mr.whiggs.in 2003, the impossible shapes signed with bloomington label secretly canadian released 'we like it wild' and toured nationally and internationally.around the same time, john wilkes booze was reformed in its classic 'five pillars of soul' line-up.after touring the western us in 2004, john wilkes booze was signed to olympia, wa-based kill rock stars.his solo debut by the horns of happiness a sea as a shore was released by secretly canadian in 2004.in 2005, deer teamed up with drummer and visual artist shelley harrison to form the first performance version of the horns of happiness touring extensively through the us, sharing the stage with acts such as man man, silver jews, old time relijun, danielson famile, joanna newsome, and the dirty projectors, among others, while garnering acclaim in publications such as magnet, dusted and skyscraper magazines. | aaron deer | genre | indie rock <tsp> indie rock | instrument | guitar <tsp> indie rock | stylisticorigin | garage rock <tsp> aaron deer | instrument | bass guitar <tsp> indie rock | stylisticorigin | new wave music | after touring the western us in 2004, john wilkes booze was signed to olympia, wa-based kill rock stars. |
arianespace sa is a french company founded in 1980 as the world's first commercial launch service provider.it undertakes the operation and marketing of the ariane programme.the company offers a number of different launch vehicles: the heavy-lift ariane 5 for dual launches to geostationary transfer orbit, the soyuz-2 as a medium-lift alternative, and the solid-fueled vega for lighter payloads.as of may 2021, arianespace had launched more than 850 satellites in 287 launches over 41 years.the first commercial flight managed by the new entity was spacenet f1 launched on 23 may 1984.arianespace uses the guiana space centre in french guiana as its main launch site.through shareholding in starsem, it can also offer commercial soyuz launches from the baikonur spaceport in kazakhstan.it has its headquarters in évry-courcouronnes, essonne, france.prior to the esa's formation, france had been lobbying for the development of a new european expendable launch system to serve as a replacement for the europa rocket.accordingly, one of the first programmes launched by the esa was the ariane heavy launcher.the express purpose of this launcher was to facilitate the delivery of commercial satellites into geosynchronous orbit.france was the largest stakeholder in the ariane development programme.french aerospace manufacturer aérospatiale served as the prime contractor and held responsibility for performing the integration of all sections of the vehicle, while french engine manufacturer société européenne de propulsion (sep) provided the first, second and third stage engines (the third stage engines were produced in partnership with german aerospace manufacturer mbb).other major companies involved included the french firms air liquide and matra, swedish manufacturer volvo, and german aircraft producer dornier flugzeugwerke.development of the third stage was a major focus point for the project - prior to ariane, only the united states had ever flown a launcher that utilised hydrogen-powered upper stages.immediately following the successful first test launch of an ariane 1 on 24 december 1979, the french space agency centre national d'études spatiales (cnes) and the esa created a new company, arianespace, for the purpose of promoting, marketing, and managing ariane operations.according to arianespace, at the time of its establishment, it was the world's first launch services company.following a further three test launches, the first commercial launch took place on 10 september 1982, which ended in failure as a result of a turbopump having failed in the third stage.the six remaining flights of the ariane 1 were successful, with the final flight occurring during february 1986.as a result of these repeated successes, orders for the ariane launcher quickly mounted up; by early 1984, a total of 27 satellites had been booked to use ariane, which was estimated to be half of the world's market at that time.as a result of the commercial success, after the tenth ariane mission was flown, the esa formally transferred responsibility for ariane over to arianespace.by early 1986, the ariane 1, along with its ariane 2 and ariane 3 derivates, were the dominant launcher on the world market.the ariane 2 and ariane 3 were short-lived platforms while the more extensive ariane 4 was being developed; it was a considerably larger and more flexible launcher that the earlier members of its family, having been intended from the onset to compete with the upper end of launchers worldwide.in comparison, while the ariane 1 had a typical weight of 207 tonnes and could launch payloads of up to 1.7 tonnes into orbit; the larger ariane 4 had a typical weight of 470 tonnes and could orbit payloads of up to 4.2 tonnes.despite this, the ariane 4 was actually 15 per cent smaller than the ariane 3.on 15 june 1988, the first successful launch of the ariane 4 was conducted. | retrusive | cleanhandedness | plecotinae | no related information |
helena (minor planet designation: 101 helena) is a large, rocky main-belt asteroid.it was discovered by canadian-american astronomer j. c. watson on august 15, 1868, and was named after helen of troy in greek mythology.this object is orbiting the sun with a period of 4.16 years and an eccentricity of 0.14.its orbital plane is inclined by 10.2° to the plane of the ecliptic.radar observations were made of this object on oct 7 and 19, 2001 from the arecibo observatory.analysis of the data gave an estimated ellipsoidal diameter of 71×63×63 ± 16% km.the mean diameter estimated from iras infrared measurements is 66 km, in agreement with the radar findings.it is classified as an s-type asteroid in the tholen system, suggesting a predominantly silicate composition.101 helena is spinning on its axis with a period of 23 hours. | exploitation | refractively | molies | no related information |
aaron deer (born november 1, 1980) is an american songwriter and multi-instrumentalist originally from indianapolis, indiana, united states, now residing in oakland, california.he is best known for his work in the bloomington music scene in the early 2000s, playing with bands such as the impossible shapes, john wilkes booze, and the horns of happiness.in the winter of 2009, deer relocated to california and continues work with the horns of happiness, royal geography society, farmer dave scher and wee giant, among others, while co-running the magnetic south cassette label.in 1999, deer and barth moved to bloomington to attend indiana university and they restarted the band there.the group released their first record, 'the great migration', in 2000 and followed with 2 subsequent releases with indianapolis-based label recordhead/mr.whiggs.in 2003, the impossible shapes signed with bloomington label secretly canadian released 'we like it wild' and toured nationally and internationally.around the same time, john wilkes booze was reformed in its classic 'five pillars of soul' line-up.after touring the western us in 2004, john wilkes booze was signed to olympia, wa-based kill rock stars.his solo debut by the horns of happiness a sea as a shore was released by secretly canadian in 2004.in 2005, deer teamed up with drummer and visual artist shelley harrison to form the first performance version of the horns of happiness touring extensively through the us, sharing the stage with acts such as man man, silver jews, old time relijun, danielson famile, joanna newsome, and the dirty projectors, among others, while garnering acclaim in publications such as magnet, dusted and skyscraper magazines. | aaron deer | genre | indie rock <tsp> indie rock | instrument | guitar <tsp> indie rock | stylisticorigin | garage rock <tsp> indie rock | stylisticorigin | new wave music <tsp> aaron deer | instrument | piano | after touring the western us in 2004, john wilkes booze was signed to olympia, wa-based kill rock stars. |
helena (minor planet designation: 101 helena) is a large, rocky main-belt asteroid.it was discovered by canadian-american astronomer j. c. watson on august 15, 1868, and was named after helen of troy in greek mythology.this object is orbiting the sun with a period of 4.16 years and an eccentricity of 0.14.its orbital plane is inclined by 10.2° to the plane of the ecliptic.radar observations were made of this object on oct 7 and 19, 2001 from the arecibo observatory.analysis of the data gave an estimated ellipsoidal diameter of 71×63×63 ± 16% km.the mean diameter estimated from iras infrared measurements is 66 km, in agreement with the radar findings.it is classified as an s-type asteroid in the tholen system, suggesting a predominantly silicate composition.101 helena is spinning on its axis with a period of 23 hours. | 101 helena | discoverer | james craig watson <tsp> james craig watson | almamater | university of michigan <tsp> 101 helena | periapsis | 3316830000 kilometres <tsp> james craig watson | nationality | canada <tsp> james craig watson | deathplace | madison wisconsin | no related information |
arianespace sa is a french company founded in 1980 as the world's first commercial launch service provider.it undertakes the operation and marketing of the ariane programme.the company offers a number of different launch vehicles: the heavy-lift ariane 5 for dual launches to geostationary transfer orbit, the soyuz-2 as a medium-lift alternative, and the solid-fueled vega for lighter payloads.as of may 2021, arianespace had launched more than 850 satellites in 287 launches over 41 years.the first commercial flight managed by the new entity was spacenet f1 launched on 23 may 1984.arianespace uses the guiana space centre in french guiana as its main launch site.through shareholding in starsem, it can also offer commercial soyuz launches from the baikonur spaceport in kazakhstan.it has its headquarters in évry-courcouronnes, essonne, france.prior to the esa's formation, france had been lobbying for the development of a new european expendable launch system to serve as a replacement for the europa rocket.accordingly, one of the first programmes launched by the esa was the ariane heavy launcher.the express purpose of this launcher was to facilitate the delivery of commercial satellites into geosynchronous orbit.france was the largest stakeholder in the ariane development programme.french aerospace manufacturer aérospatiale served as the prime contractor and held responsibility for performing the integration of all sections of the vehicle, while french engine manufacturer société européenne de propulsion (sep) provided the first, second and third stage engines (the third stage engines were produced in partnership with german aerospace manufacturer mbb).other major companies involved included the french firms air liquide and matra, swedish manufacturer volvo, and german aircraft producer dornier flugzeugwerke.development of the third stage was a major focus point for the project - prior to ariane, only the united states had ever flown a launcher that utilised hydrogen-powered upper stages.immediately following the successful first test launch of an ariane 1 on 24 december 1979, the french space agency centre national d'études spatiales (cnes) and the esa created a new company, arianespace, for the purpose of promoting, marketing, and managing ariane operations.according to arianespace, at the time of its establishment, it was the world's first launch services company.following a further three test launches, the first commercial launch took place on 10 september 1982, which ended in failure as a result of a turbopump having failed in the third stage.the six remaining flights of the ariane 1 were successful, with the final flight occurring during february 1986.as a result of these repeated successes, orders for the ariane launcher quickly mounted up; by early 1984, a total of 27 satellites had been booked to use ariane, which was estimated to be half of the world's market at that time.as a result of the commercial success, after the tenth ariane mission was flown, the esa formally transferred responsibility for ariane over to arianespace.by early 1986, the ariane 1, along with its ariane 2 and ariane 3 derivates, were the dominant launcher on the world market.the ariane 2 and ariane 3 were short-lived platforms while the more extensive ariane 4 was being developed; it was a considerably larger and more flexible launcher that the earlier members of its family, having been intended from the onset to compete with the upper end of launchers worldwide.in comparison, while the ariane 1 had a typical weight of 207 tonnes and could launch payloads of up to 1.7 tonnes into orbit; the larger ariane 4 had a typical weight of 470 tonnes and could orbit payloads of up to 4.2 tonnes.despite this, the ariane 4 was actually 15 per cent smaller than the ariane 3.on 15 june 1988, the first successful launch of the ariane 4 was conducted. | arianespace | locationcity | courcouronnes <tsp> guiana space centre | location | french guiana <tsp> ela-3 | site | guiana space centre <tsp> ariane 5 | launchsite | ela-3 <tsp> ela-3 | operator | arianespace | arianespace sa is a french company founded in 1980 as the world's first commercial launch service provider.arianespace uses the guiana space centre in french guiana as its main launch site.french aerospace manufacturer aérospatiale served as the prime contractor and held responsibility for performing the integration of all sections of the vehicle, while french engine manufacturer société européenne de propulsion (sep) provided the first, second and third stage engines (the third stage engines were produced in partnership with german aerospace manufacturer mbb).development of the third stage was a major focus point for the project - prior to ariane, only the united states had ever flown a launcher that utilised hydrogen-powered upper stages.immediately following the successful first test launch of an ariane 1 on 24 december 1979, the french space agency centre national d'études spatiales (cnes) and the esa created a new company, arianespace, for the purpose of promoting, marketing, and managing ariane operations. |
aaron deer (born november 1, 1980) is an american songwriter and multi-instrumentalist originally from indianapolis, indiana, united states, now residing in oakland, california.he is best known for his work in the bloomington music scene in the early 2000s, playing with bands such as the impossible shapes, john wilkes booze, and the horns of happiness.in the winter of 2009, deer relocated to california and continues work with the horns of happiness, royal geography society, farmer dave scher and wee giant, among others, while co-running the magnetic south cassette label.in 1999, deer and barth moved to bloomington to attend indiana university and they restarted the band there.the group released their first record, 'the great migration', in 2000 and followed with 2 subsequent releases with indianapolis-based label recordhead/mr.whiggs.in 2003, the impossible shapes signed with bloomington label secretly canadian released 'we like it wild' and toured nationally and internationally.around the same time, john wilkes booze was reformed in its classic 'five pillars of soul' line-up.after touring the western us in 2004, john wilkes booze was signed to olympia, wa-based kill rock stars.his solo debut by the horns of happiness a sea as a shore was released by secretly canadian in 2004.in 2005, deer teamed up with drummer and visual artist shelley harrison to form the first performance version of the horns of happiness touring extensively through the us, sharing the stage with acts such as man man, silver jews, old time relijun, danielson famile, joanna newsome, and the dirty projectors, among others, while garnering acclaim in publications such as magnet, dusted and skyscraper magazines. | aaron deer | genre | indie rock <tsp> indie rock | instrument | guitar <tsp> indie rock | stylisticorigin | garage rock <tsp> indie rock | stylisticorigin | new wave music <tsp> aaron deer | instrument | piano | after touring the western us in 2004, john wilkes booze was signed to olympia, wa-based kill rock stars. |
helena (minor planet designation: 101 helena) is a large, rocky main-belt asteroid.it was discovered by canadian-american astronomer j. c. watson on august 15, 1868, and was named after helen of troy in greek mythology.this object is orbiting the sun with a period of 4.16 years and an eccentricity of 0.14.its orbital plane is inclined by 10.2° to the plane of the ecliptic.radar observations were made of this object on oct 7 and 19, 2001 from the arecibo observatory.analysis of the data gave an estimated ellipsoidal diameter of 71×63×63 ± 16% km.the mean diameter estimated from iras infrared measurements is 66 km, in agreement with the radar findings.it is classified as an s-type asteroid in the tholen system, suggesting a predominantly silicate composition.101 helena is spinning on its axis with a period of 23 hours. | 101 helena | discoverer | james craig watson <tsp> james craig watson | almamater | university of michigan <tsp> 101 helena | periapsis | 3316830000 kilometres <tsp> james craig watson | nationality | canada <tsp> james craig watson | deathplace | madison wisconsin | no related information |
aaron deer (born november 1, 1980) is an american songwriter and multi-instrumentalist originally from indianapolis, indiana, united states, now residing in oakland, california.he is best known for his work in the bloomington music scene in the early 2000s, playing with bands such as the impossible shapes, john wilkes booze, and the horns of happiness.in the winter of 2009, deer relocated to california and continues work with the horns of happiness, royal geography society, farmer dave scher and wee giant, among others, while co-running the magnetic south cassette label.in 1999, deer and barth moved to bloomington to attend indiana university and they restarted the band there.the group released their first record, 'the great migration', in 2000 and followed with 2 subsequent releases with indianapolis-based label recordhead/mr.whiggs.in 2003, the impossible shapes signed with bloomington label secretly canadian released 'we like it wild' and toured nationally and internationally.around the same time, john wilkes booze was reformed in its classic 'five pillars of soul' line-up.after touring the western us in 2004, john wilkes booze was signed to olympia, wa-based kill rock stars.his solo debut by the horns of happiness a sea as a shore was released by secretly canadian in 2004.in 2005, deer teamed up with drummer and visual artist shelley harrison to form the first performance version of the horns of happiness touring extensively through the us, sharing the stage with acts such as man man, silver jews, old time relijun, danielson famile, joanna newsome, and the dirty projectors, among others, while garnering acclaim in publications such as magnet, dusted and skyscraper magazines. | aaron deer | genre | indie rock <tsp> indie rock | instrument | guitar <tsp> indie rock | stylisticorigin | garage rock <tsp> indie rock | stylisticorigin | new wave music <tsp> aaron deer | instrument | piano | after touring the western us in 2004, john wilkes booze was signed to olympia, wa-based kill rock stars. |
arianespace sa is a french company founded in 1980 as the world's first commercial launch service provider.it undertakes the operation and marketing of the ariane programme.the company offers a number of different launch vehicles: the heavy-lift ariane 5 for dual launches to geostationary transfer orbit, the soyuz-2 as a medium-lift alternative, and the solid-fueled vega for lighter payloads.as of may 2021, arianespace had launched more than 850 satellites in 287 launches over 41 years.the first commercial flight managed by the new entity was spacenet f1 launched on 23 may 1984.arianespace uses the guiana space centre in french guiana as its main launch site.through shareholding in starsem, it can also offer commercial soyuz launches from the baikonur spaceport in kazakhstan.it has its headquarters in évry-courcouronnes, essonne, france.prior to the esa's formation, france had been lobbying for the development of a new european expendable launch system to serve as a replacement for the europa rocket.accordingly, one of the first programmes launched by the esa was the ariane heavy launcher.the express purpose of this launcher was to facilitate the delivery of commercial satellites into geosynchronous orbit.france was the largest stakeholder in the ariane development programme.french aerospace manufacturer aérospatiale served as the prime contractor and held responsibility for performing the integration of all sections of the vehicle, while french engine manufacturer société européenne de propulsion (sep) provided the first, second and third stage engines (the third stage engines were produced in partnership with german aerospace manufacturer mbb).other major companies involved included the french firms air liquide and matra, swedish manufacturer volvo, and german aircraft producer dornier flugzeugwerke.development of the third stage was a major focus point for the project - prior to ariane, only the united states had ever flown a launcher that utilised hydrogen-powered upper stages.immediately following the successful first test launch of an ariane 1 on 24 december 1979, the french space agency centre national d'études spatiales (cnes) and the esa created a new company, arianespace, for the purpose of promoting, marketing, and managing ariane operations.according to arianespace, at the time of its establishment, it was the world's first launch services company.following a further three test launches, the first commercial launch took place on 10 september 1982, which ended in failure as a result of a turbopump having failed in the third stage.the six remaining flights of the ariane 1 were successful, with the final flight occurring during february 1986.as a result of these repeated successes, orders for the ariane launcher quickly mounted up; by early 1984, a total of 27 satellites had been booked to use ariane, which was estimated to be half of the world's market at that time.as a result of the commercial success, after the tenth ariane mission was flown, the esa formally transferred responsibility for ariane over to arianespace.by early 1986, the ariane 1, along with its ariane 2 and ariane 3 derivates, were the dominant launcher on the world market.the ariane 2 and ariane 3 were short-lived platforms while the more extensive ariane 4 was being developed; it was a considerably larger and more flexible launcher that the earlier members of its family, having been intended from the onset to compete with the upper end of launchers worldwide.in comparison, while the ariane 1 had a typical weight of 207 tonnes and could launch payloads of up to 1.7 tonnes into orbit; the larger ariane 4 had a typical weight of 470 tonnes and could orbit payloads of up to 4.2 tonnes.despite this, the ariane 4 was actually 15 per cent smaller than the ariane 3.on 15 june 1988, the first successful launch of the ariane 4 was conducted. | plowman | narciscissi | faeculence | no related information |
aaron deer (born november 1, 1980) is an american songwriter and multi-instrumentalist originally from indianapolis, indiana, united states, now residing in oakland, california.he is best known for his work in the bloomington music scene in the early 2000s, playing with bands such as the impossible shapes, john wilkes booze, and the horns of happiness.in the winter of 2009, deer relocated to california and continues work with the horns of happiness, royal geography society, farmer dave scher and wee giant, among others, while co-running the magnetic south cassette label.in 1999, deer and barth moved to bloomington to attend indiana university and they restarted the band there.the group released their first record, 'the great migration', in 2000 and followed with 2 subsequent releases with indianapolis-based label recordhead/mr.whiggs.in 2003, the impossible shapes signed with bloomington label secretly canadian released 'we like it wild' and toured nationally and internationally.around the same time, john wilkes booze was reformed in its classic 'five pillars of soul' line-up.after touring the western us in 2004, john wilkes booze was signed to olympia, wa-based kill rock stars.his solo debut by the horns of happiness a sea as a shore was released by secretly canadian in 2004.in 2005, deer teamed up with drummer and visual artist shelley harrison to form the first performance version of the horns of happiness touring extensively through the us, sharing the stage with acts such as man man, silver jews, old time relijun, danielson famile, joanna newsome, and the dirty projectors, among others, while garnering acclaim in publications such as magnet, dusted and skyscraper magazines. | aaron deer | genre | indie rock <tsp> indie rock | stylisticorigin | garage rock <tsp> aaron deer | instrument | bass guitar <tsp> indie rock | stylisticorigin | new wave music <tsp> aaron deer | background | solo singer | after touring the western us in 2004, john wilkes booze was signed to olympia, wa-based kill rock stars. |
arianespace sa is a french company founded in 1980 as the world's first commercial launch service provider.it undertakes the operation and marketing of the ariane programme.the company offers a number of different launch vehicles: the heavy-lift ariane 5 for dual launches to geostationary transfer orbit, the soyuz-2 as a medium-lift alternative, and the solid-fueled vega for lighter payloads.as of may 2021, arianespace had launched more than 850 satellites in 287 launches over 41 years.the first commercial flight managed by the new entity was spacenet f1 launched on 23 may 1984.arianespace uses the guiana space centre in french guiana as its main launch site.through shareholding in starsem, it can also offer commercial soyuz launches from the baikonur spaceport in kazakhstan.it has its headquarters in évry-courcouronnes, essonne, france.prior to the esa's formation, france had been lobbying for the development of a new european expendable launch system to serve as a replacement for the europa rocket.accordingly, one of the first programmes launched by the esa was the ariane heavy launcher.the express purpose of this launcher was to facilitate the delivery of commercial satellites into geosynchronous orbit.france was the largest stakeholder in the ariane development programme.french aerospace manufacturer aérospatiale served as the prime contractor and held responsibility for performing the integration of all sections of the vehicle, while french engine manufacturer société européenne de propulsion (sep) provided the first, second and third stage engines (the third stage engines were produced in partnership with german aerospace manufacturer mbb).other major companies involved included the french firms air liquide and matra, swedish manufacturer volvo, and german aircraft producer dornier flugzeugwerke.development of the third stage was a major focus point for the project - prior to ariane, only the united states had ever flown a launcher that utilised hydrogen-powered upper stages.immediately following the successful first test launch of an ariane 1 on 24 december 1979, the french space agency centre national d'études spatiales (cnes) and the esa created a new company, arianespace, for the purpose of promoting, marketing, and managing ariane operations.according to arianespace, at the time of its establishment, it was the world's first launch services company.following a further three test launches, the first commercial launch took place on 10 september 1982, which ended in failure as a result of a turbopump having failed in the third stage.the six remaining flights of the ariane 1 were successful, with the final flight occurring during february 1986.as a result of these repeated successes, orders for the ariane launcher quickly mounted up; by early 1984, a total of 27 satellites had been booked to use ariane, which was estimated to be half of the world's market at that time.as a result of the commercial success, after the tenth ariane mission was flown, the esa formally transferred responsibility for ariane over to arianespace.by early 1986, the ariane 1, along with its ariane 2 and ariane 3 derivates, were the dominant launcher on the world market.the ariane 2 and ariane 3 were short-lived platforms while the more extensive ariane 4 was being developed; it was a considerably larger and more flexible launcher that the earlier members of its family, having been intended from the onset to compete with the upper end of launchers worldwide.in comparison, while the ariane 1 had a typical weight of 207 tonnes and could launch payloads of up to 1.7 tonnes into orbit; the larger ariane 4 had a typical weight of 470 tonnes and could orbit payloads of up to 4.2 tonnes.despite this, the ariane 4 was actually 15 per cent smaller than the ariane 3.on 15 june 1988, the first successful launch of the ariane 4 was conducted. | arianespace | locationcountry | france <tsp> arianespace | locationcity | courcouronnes <tsp> ela-3 | site | guiana space centre <tsp> ariane 5 | launchsite | ela-3 <tsp> ela-3 | operator | arianespace | no related information |
aaron deer (born november 1, 1980) is an american songwriter and multi-instrumentalist originally from indianapolis, indiana, united states, now residing in oakland, california.he is best known for his work in the bloomington music scene in the early 2000s, playing with bands such as the impossible shapes, john wilkes booze, and the horns of happiness.in the winter of 2009, deer relocated to california and continues work with the horns of happiness, royal geography society, farmer dave scher and wee giant, among others, while co-running the magnetic south cassette label.in 1999, deer and barth moved to bloomington to attend indiana university and they restarted the band there.the group released their first record, 'the great migration', in 2000 and followed with 2 subsequent releases with indianapolis-based label recordhead/mr.whiggs.in 2003, the impossible shapes signed with bloomington label secretly canadian released 'we like it wild' and toured nationally and internationally.around the same time, john wilkes booze was reformed in its classic 'five pillars of soul' line-up.after touring the western us in 2004, john wilkes booze was signed to olympia, wa-based kill rock stars.his solo debut by the horns of happiness a sea as a shore was released by secretly canadian in 2004.in 2005, deer teamed up with drummer and visual artist shelley harrison to form the first performance version of the horns of happiness touring extensively through the us, sharing the stage with acts such as man man, silver jews, old time relijun, danielson famile, joanna newsome, and the dirty projectors, among others, while garnering acclaim in publications such as magnet, dusted and skyscraper magazines. | aaron deer | genre | indie rock <tsp> indie rock | stylisticorigin | garage rock <tsp> aaron deer | instrument | bass guitar <tsp> indie rock | stylisticorigin | new wave music <tsp> aaron deer | background | solo singer | after touring the western us in 2004, john wilkes booze was signed to olympia, wa-based kill rock stars. |
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