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text: 17 Powerful Quotes To Help You Get Through Hard Times Anthony Find funny inspirational love life. Thanks for checking out these great motivational picture quotes about hard times. 36 Positive Quotes To Get You Through Hard Times Yes Pinterest Positive and inspirational quotes about life to encourage optimism. ...Read more


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text: We are swapping the long haul flight for long walks along the beach this holiday season. Avoiding that needing a holiday after a holiday feeling by exploring local sunshine coast spot - Noosa. Located on the sunshine coast, Noosa is equal parts glamour and natural beauty. Packing will be a breeze only needing the summer essentials. We are loving these white Gucci sunglasses, Helen Kiminski straw visor and the Urban Prima Mermaid swirls one-piece. Don't forget to slip, slop slap. Happy holidays!


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How weather forecasts could trigger disaster aid
If you are unable to listen to this podcast, please update your browser or click here to download [1.6 MB]
The humanitarian impact of climate change is the next big challenge for both local communities and international aid organisations.
Natural disasters hit developing countries hardest, but while the international community can be generous when a disaster makes the headlines, smaller extreme events often slip under the radar.
In this interview, recorded at Earth to Paris, an event in the French capital during the UN's COP 21 summit, Maarten van Aalst discusses a possible solution to the problem.
Van Aalst, an expert in disaster reduction who runs the Red Cross/Red Crescent Climate Centre and was a lead author for the latest set of assessment reports produced by UN advisory body the Intergovernmental Panel on Climate Change, explains how forecast-based finance projects could protect communities by automatically releasing the money they need when disaster risk is elevated, without waiting for the extreme event to happen.
He also sheds light on a new branch of science called 'attribution of extreme events' that studies the links between disasters and climate change.


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so, the blogging from a-z challenge ended on monday…yet every day this week has seen me post an entry.
you know what happened? i got used to visiting with you every day…and now
i am addicted again i am just really enjoying blogging!
i love this time of year!
this week's happy serendipities continued into wednesday's aunti day in toronto: i decided to wear the gingham hair clip that mom and got at stitch n kitsch. and look what outfit little e had picked out for the day!
we swapped our barrettes, and little e rocked the completely gingham look:
yesterday, it was finally warm and humid enough to wear the outfit that i have been dying to sport for a few weeks now:
can't wait to wear my orange sweater – must knit faster!
mom and dad went to visit the blanket at joseph schneider haus yesterday!
tomorrow is both the mississauga marathon and the toronto marathon. for you out-of-towners, this means two marathons within spitting distance – ok, 30 kilometers – of each other. i'm going to keep my mouth shut on the
questionable logic fiery politics of this situation, and just wish all participants a good race!
happy weekend! no blog post tomorrow – promise.


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On 2012 May 26 UT21:21 J. Moeller (Syracuse, NY, USA, using a Konica Minolta DIMAGE Z5 digital camera, f/7.1, 1/250 sec exposure, ISO-50, 69mm focal length, digital zoom x3) captured a hand held image of the Moon in daylight. On the SW limb of the dark side of the Moon a bright spot can be seen. This has a brightness comparable to that of Mare Serenitatis. There is also a fainter dark blurred marking further inside the dark side. ALPO/BAA weight=1.
Near Desseilgny in Mare Serenitatis (29E, 25N) 1971 Feb 01 UT 19:40- 20:15 Observed by Persson (Hvidore, Denmark, 2.5" refractor, x100, S=G) "Obscur. (blurred & dark) starting between Plinius & Menelaus moving towards Posidonius. Normal after 2 min. A little crater (white spot) periodically disappeared for several secs regularly every few min. There was haze above onlt this spot. A tiny crater SE of it was invis. till 2015h then became clear & steady. Color was reddish-brown. Drawing. (Apollo 14 watch)." NASA catalog weight=2 (low). NASA catalog ID 1293.
On 1964 Jun 17 at UT 04:15-05:01 Cross et al. (Whittier, CA, USA, 19" ? reflector, S=7-8) observed near Ross D: "Gas cloud. Motion". The Cameron 1978 catalog ID=818 and weight=4. The ALPO/BAA weight=4.
Agrippa 1966 Nov 19/20 UTC 23:58-00:14 Observed by Bartlett (Baltimore, MD, USA, 5" reflector x283, S=4, T=5) "Faint bluish tinge seen at base of NW wall beneath landslip" NASA catalog weight=4 (high). NASA catalog ID #995.
Cassini E 2002 Dec 11 UT 16:30-18:46 Observed by Knott (Liverpool, England, 216mm Newtonian, x216, red and blue filters used) seeing III, transparency good) "Observations carried out of the area extending from the Alpine Valley to the Crater Cassini. At 17:12 a pin point bright flash was seen NW of the rim of the crater E in white light. A 2nd pin point flash was also seen at 18:18, this time thru a blue filter. The 2nd flash was also seen on the NW rim of the crater E. The observer does not think this was a TLP as the seeing was III, but the flash was so bright as to be startling. Other peaks within the Alps were bright but were much less so in red and ble filters, where the rim of the crater E. NW edge was very bright in all filters, including white light. Incoming cloud prevented further observation." BAA Lunar Section report.
On 1982 Dec 22 at UT 19:20-20:10 J-H Robinson (Teighmouth, Devon, UK, 10" reflector, x150, seeing=IV-V) could not distinguish between Messier and Messier A. The tail of these features was very bright - two telescopes were used. Moore (Selsey, UK, 12" reflector, seeing=III) could see Messier A but found Messier itself obscured - just see the west wall and thought that the comet like tail was unusual as it did not appear divided. The Cameron 2006 catalog ID=192 and weight=5. The ALPO/BAA weight=3.
Alphonsus and limb 1967 Apr 17 UTC 21:30 Observed by Wise (England, 6.5" reflector, x90) "3 dark patches (Alphonsus) prominent. Suspected red patch (blink ?). (indep. confirm. of Cross 1h later?)." NASA catalog weight=3 (average). NASA catalog ID #1024.
Plato 1967 Apr 17 UTC 21:30 Observed by Wise (England, 6.5" reflector, x90) "Suspected a blink, (red?)" NASA catalog weight=2 (low). NASA catalog ID #1025.
On 1967 Apr 17 UT 21:30 Observed by Wise (England, 6.5" reflector, x90) saw a brilliant object nr. E(ast. ?) limb (West Lim IAU?) for 15m. Check on star maps neg. (indep. confirm. of Cross 1h later?)." NASA catalog weight=3 (average). NASA catalog ID #1024.
On 1975 May 18 at UT2115-2145 C. Lord (St Annes-on-sea, Lancashire, UK, 76mm f/16 refractor, x170, Wratten 25, and 44a Moon blink filters used, Transparency 4.5/5, no wind, S=F). The west flank of Maginus, and the interior, appeared to be partly obscured. No other features in a similar position along the terminator were obscured. No colour blink was detected with the filters, though a pronounced red/white light blink was noted; the device employed a N.D. x4 filter. By 21:45UT the floor was no longer obscured and only Magninus G was masked in a white haze; however immediately adjacent to the terminator was an ill defined misty patch lying where the outer flank of maginus would have been visible. The rest of the terminator was sharp. The obscuration was only seen to advantage in blue and int. light, and the blue/int blink was only very slight. Findlay and McDonnell observed 21:30-23:00 using a 25cm refractor (Seeing II- III) but failed to see anything unsual. NASA catalog weight=3. NASA catalog ID #1407. ALPO/BAA weight=2.
Vallis Alpes 1983 Jun 18 UT 22:01-22:23 P.Madej (Huddersfield, UK, 77mm refractor, x83,x250, seeing II-III, transparency fair). After studying the whole length of this valley, the observer saw a change in "albedo" and a small change in colour of the valley floor near to the Plato end. This colour was not seen in a yellow Wratten 15 filter but was noted in a purple Wratten 35 filter, and was strong in a red filter. Also the crater Trouvelot was not seen at x250 with a x2 Barlow.Wratten 25. ALPO/BAA weight=1.
Daniell 1983 Jun 18 UT 22:06-22:25) P.Madej (Huddersfield, UK, 77mm refractor, x83,x166, seeing II-III, transparency fair). Noted on the inside W eall a faint red rose like glow (with a diameter? about it). The red glow varied in brightness with a period of about 2 minutes. It looked somewhat brighter at x166. The glow was still visible when the observation ended at 22:15 ALPO/BAA weight=1.
On 1988 Feb 25 at UT20:00? P.W. Foley (Kent, UK, 12" reflector) found that Aristarchus was very bright (especially in the UV end of the spectrum) despite other features not being seen in Earthshine. The cameron 2006 catalog ID=318 and the weight=1. The ALPO/BAA weight=1.
Plato 1886 Sep 06 UT 19:00? Observed by Valderama (Italy?) "Streak of light on dark floor of crater in shadow. (sunlight between peaks on walls?)" NASA catalog weight=0 (most unlikely to be a TLP). NASA catalog ID #251. ALPO/BAA catalog weight=1.
Plato 1967 Apr 18 UT 03:10-04:00 Observed by Kelsey (Riverside, CA, USA, 8" reflector x300, S=8, T-4-5). "Streak on floor showed slight enhancement in red filter comp. to blue. Later, a 2nd streak formed. Probably the sun shining thru a valley in the rim. Red enhancement permanent? (Wise suspected a blink here 6h earlier)." NASA catalog weight=3. NASA catalog ID #1027. ALPO/BAA weight=1.
In 1824 Jul 04 at UT23:00? Emmett (England, UK) observed a star-like light on the rim (in the dark). The Cameron 1978 catalog ID=100 and the weight=3. The ALPO/BAA weight=2.
On 1992 Jun 09 at UT 18:52 G. Kolovos, Thessaloniki, 40.63111N, 22.9597W, height 28m, Greece) photographed two blue spots on the terminator region of the Moon in one of a series of Ektachrome film pictures. The rest of the Moon was a white-yellow colour. The ALPO/BAA weight=1.
Linne 1868 Jul 28 UT 20:00? Observed by Tacchini (Palermo, Italy) "Shadow not so marked-had a light penumbra, indicated a feeble cavity. Other craters had a black shad. On 29th appeared completely white. Crater normal on 26th. (letter to Madler Sep. 16, 1868)." NASA catalog weight=4 (high). NASA catalog ID #159.
Copernicus 1939 Mar 29 UT 19:00-19:15 Observed by Wilkins (Kent, England, 6" reflector) "C.P. diffuse light spot, faint glow s as tho in a luminous mist (3h before SR) Some indication of E.terraces, then vanished." NASA catalog weight=4. NASA catalog ID #447. ALPO/BAA weight=3.
On 1989 Feb 15 at UT 03:15-03:30 M. Dixon (Palenque Ruins, Mexico, 7x35 binouculars) observed a point of light that was very bright in or near Mare Humorum. It was visible for 5 minutes then vanished. The Cameron 2006 catalog ID=353 and weight=1. The ALPO/BAA weight=1.
On 1971 Jul 31 at UT 21:40 (18:40 local time?) Miranda (Plaui, Brazil, 4" Refractor, 80x, 160x, Moon 70deg in altitude) observed an intermittent and curious brilliance on top of a peak (with irregular reflection) north of Mons Hadley (5E, 27N). The Cameron 1978 catalog ID=1302 and weight=2. The ALPO/BAA weight=2.
On 1952 Feb 05 at UT 05:10 J.Carle (USA, 8" reflector, x180) observed the following in Plato: "A shadow in a depression, or a cloud, or an optical illus.? Oval dark area nr. center, disappeared in 15m clear & prominenet at first then vanished. 4 of 14 spots nr. center continuously seen while remaining ones seen only momentarily. (seeing?) Drawing includes sketch on March 7. His sketch shows 18 spots, 13 same as here". The Cameron 1978 catalog ID=549 and the weight=2. The ALPO/BAA weight=2.
On 1969 Mar 27 at UT 18:42-18:47 Ringsdore (England, 15" reflector, x350), Moseley (Armagh, Northern Ireland) and P. Moore (Selsey, UK) observed nothing unusual in Alphonsus at 18:40UT, but at 18:45UT Ringsdore saw a blurring. At 18:43UT Mosely saw a reddush-orange patch and this was confirmed by Moore. NNW of the central peak, Mosely got a blink, but Moore did not because of too much stray light. The colour was like Jupiter's red spot, but less pronounced. The Cameron 1978 catalog ID=1118 and weight=5. The ALPO/BAA weight=4.
Alphonsus 1966 Nov 22 UT 03:17-03:40 Observed by kelsey (Riverside, CA, USA, 8" relector x300) "Seen first with (Eng.) moon blink, red filter but not in the green. Not seen at 03:42h" NASA catalog weight=4 (high). NASA catalog ID #998.
Copernicus 1932 Mar 16 UTC 18:45-19:30 Observed by Barker (Cheshunt, England, 12.5" reflector, x310) "Term. from Cop. to lat.20S was misty & hard to define. Rest was usual sharp definition. Mistiness cleared at 1930. Cleaned his eyepiece & prism but it persisted." NASA catalog weight=3 (average). NASA catalog ID #402.
On 1989 Feb 16 at UT02:46-03:01 D. Darling (Sun Praire, WI, USA, 3" refractor, x140, seeing=6/10) found that the brightness of the rim of Proclus was 9.0 (normal?). The Cameron 2006 catalog ID=354 and the weight=0. The ALPO/BAA weight=1.
127mm f/12 GoTo scope, x62-x154, seeing: best and transparency= 6) observed that an unoficially named mountain (Lambert Gamma or Mons Undest), near Lambert, had a "very strong glow", especially the part that was facing the line of the terminator and this was brighter than the side facing away. The No other object nearby was casting as much light, even Mons La Hire. The effect was seen for 40 minutes and the glow was present throughout. The ALPO/BAA weight=2.
Gassendi 1967 Oct 13 UTC 19:17-20:00 Observers: Henshaw (Mansfield, UK, 8.5" reflector x112) and Corralitos Observator (Organ Pass, NM, USA, 24" reflector) "Phenomenon (brightening ?) nr. NW (ast. ?) lasting for 3s. Cont'd for 45m but nothing else unusual, (nr. Gass or in it?). Corralitos MB did not confirm." NASA catalog weight=3 (average). NASA catalog ID #1050.
On 1882 May 27 ay UT 20:00 an unknown observer (10" reflector) saw a bright luminous ray near west (astronomical?) wall on floor of Plato. Cameron suggests sunlight between peaks?. The Cameron 1978 catalog ID= 233 and weight=0. The ALPO/BAA weight=1.
Archimedes 1971 Aug 01 UT 22:00(?) (19:00 originally given probably local time) Miranda (Plaui, Brazil, 4" refractor, x80) observed two grooves going from east to west, broadening towards the west, across Archimedes. A drawing was supplied. Apparently this was the first time that this was ever seen. Cameron suggests rays? and also says that in fact a similar phenomenon reported before in neasrly the same position (Apollo 15 watch?). The Cameron 1978 catalog ID=1303 and weight=2. The ALPO/BAA weight=1.
On 1980 Jul 22 at UT20:08-21:50 G.North (Sussex, UK, 8" reflector, x144 and x207, seeing III-V and transparency fair) suspected an obscuration on the north and north west wall. The effect came and went. May have been due to seeing and image contrast? Cameron 2006 catalog ID=101 and weight=1. ALPO/BAA weight=1.
On 1987 Oct 03 at UT 01:0?0-02:00 R. Manske (Brooklyn, WI, USA, 8" reflector, x226) observed sunlight glinting of the walls in spectacular display of colours. White (even gold) was seen at the centre, and blue on the top most part of the rim. The white (or gold) band was thin in comparison to other bands. The observer suspects that this effect was terrestrial atmosphere related. Cameron 2006 catalog ID=307 and weight= 0. ALPO/BAA weight=1.
Ross D 1966 Nov 23 UT 04:50-05:02 Observed by Cross (Whittier, CA, USA, 19" reflector, x250 & 2390, S=4-5 (sometimes 6), T=4, excellent contrast) Activity level 5, eastern third of Ross D's circumference possibly partly obscured. ALPO/BAA weight=1.
Plato 1998 Mar 08 UT 19:30-20:10 S. Beaumont (Windermere, UK, 30cm reflector, Meade 23A and 38A filters, seeing III, transparency fairly good, some haze) observed a whitish misty effect seen bordering the shadows of the SE rim. It appeared intermittently and was not seen in the violet or red filters. Observers wonders if it could have been an effect associated with the Earth's atmosphere, which was unsteady with some haze. However, other craters appeared normal. The ALPO/BAA weight=1.
On 1964 Jan 24 at 20:00? Scarfe (UK) obtained spactra showing luminescence? The Cameron 1978 catalog ID=796 and weight=5. The ALPO/BAA weight=3.
On 1955 Jan 05 at 01:00-01:30 UT D.A. Logue (Larchment, PA, USA, 15cm reflector at x340, seeing Good) saw a strange blue light above the surface of the Moon where the night and the day meet. He observed this light for more than 30 min and it did not appear to move. It appeared like a star in that the rays of light came from it. The observer adds that he first thought thst the objects was a star, but later decided that it had to be on the Moon itself. A drawing shows the blue spot near the rugged south west (IAU?) limb of the Moon. The editor of the Strolling Astronomer (Vol 8, No. 11-12, Nov-Dec 1954, p146) was unable to identify the craters drawn. The editor speculates that the observer saw a high mountain peak with its summit in sunlight and detached from the illuminated regions - however this would not explain the blue colour. Note this is an ALPO observation and does not apear in the Cameron catalogs. ALPO/BAA weight=2.
On 1964 Jun 21 at UT 03:43-05:44 Harris, Cross and Helland (Whittier, CA, USA, 19" reflector) observed south of Ross D: "Moving dark area". The Cameron 1978 catalog ID=819 and weight=4. The ALPO/BAA weight=4.
On 1989 Feb 17 at UT00:55 D. Darling (Sun Praire, WI, USA, 12.5" reflector, x248) found that the brightness of the rim of Proclus was 9.0, the north west wall to be 9.5, the west wall to be 5.2, and the east wall 8.2 (normal?). The Cameron 2006 catalog ID=355 and the weight=1. The ALPO/BAA weight=2.
Near Hyginus 1959 Sep 13 UT Observed by Bradford (S.Shields, England, 15"? reflector), Feist, Lovas (Hungary), Moore, Wilkins (Kent, England, 7" refractor, x500) "Obliterated by a hovering cloud (Feist disagrees). Budapest obs. saw a cloud at 21:02:30, lasting 5 m. Moore & Wilkins saw burst of light & dust cloud at 21:02:35 (confirm.) Drawing by Lovas." NASA catalog weight=5 and catalog ID #722. The ALPO/BAA weight=1.
Littrow, 1959 Sep 13 UT Observed by Bradford (S.Shields, England, 15"? reflector), Feist, Lovas (Hungary), Moore, Wilkins (Kent, England, 7" refractor, x500) "Obliterated by a hovering cloud (Feist disagrees). Budapest obs. saw a cloud at 21:02:30, lasting 5 m. Moore & Wilkins saw burst of light & dust cloud at 21:02:35 (confirm.) Drawing by Lovas." NASA catalog weight=1 and catalog ID #722. The ALPO/BAA weight=1.
Plato 1906 Mar 06 UT 22:00? Observed by Fauth (Germany? 6" refractor) "Color (brightness?) greatly enhanced as it was to be on the next nite" NASA catalog weight=3 (average). NASA catalog ID #324.
On 1991 Jan 26 at UT 23:38-23:50 D. Darling (Sun Praire, WI, USA, 12.5" reflector, x159 and 3" refractor x90, seeing 5/10, transparency 3/6) found that Aristarchus was brighter through a red filter than through a blue filter on its western wall. He checked Aristarchus in two telecopes and obtained the same result. The Cameron 2006 catalog ID=419 and the weight=4. The ALPO/BAA weight=3.
Moon 1967 Apr 21 UTC 02:30-09:30 Observed by Dunlap et al (Corralitos Observatory, Organ PAss, NM, USA, 24" reflector + moonblink) "UV excess relative to red & visual images. Greatest (30%) at subsolar pt. nr. limb, grading down to 0% at term. Seen Apr 22 also with a gradient of 10% at term. to 25-30% at subsolar pt. (137 deg long). Filters well balanced. Neg. (normal) on Apr. 20 & 23rd. Bandpass 3700-4900A on image enhancement & filter equip. (coincided with Lyrid meteor shower. They had seen this phenom. many times since. NASA catalog weight=5 (very high). NASA catalog ID #1039.
On 1980 Jul 23 at UT22:00 G.W. Amery (Reading, UK, 8" reflector, x144 and x207, seeing=III-V and transparency=fair) found that the interior shadow was a light grey. BAA TLP coordinator (Foley) suggests that this was light reflecting from the illuminated walls? Cameron 2006 catalog TLP ID=102 and weight=1. ALPO/BAA weight=2.
On 1977 Apr 29 at UT21:40-23:20 an unknown UK observer reported a TLP in Gassendi crater. The following are reports by observers attempting to confirm activity: J.W. Napper (Didcot, UK, 30cm reflector, x287, Wratten 25 and 44a, conditions clear 5+) received a telephone alert call at 22:00 but the sky was cloudy until 22:30. An initial look revealed nothing unusual, then at 22:54 he observed a colour blink just inside the north wall, appearing bright in red and normal in blue or white light. No loss of detail seen and the effect lasted only 2 minutes. A sketch was made. However the observer stresses that the very bad seeing casts some doubt on this observation. L. Fitton observed using a 8.5" reflector, with Moon blink device at x200, seeing was I- II. All areas negative, including Gassindi from 21:40-21:55 and again 22;00-22:25 and finally 22:50-23:30 negative. Mike Brown (Huntington, York, UK, 30cm reflector, x220 and x350, seeing 3-4/5, and transparency 5/5) - observed from 22:00-23:25UT no colour seen, nor obsecuration, all filters negative, despite seeing a lot of fine setail inside this crater.
On 1987 Oct 04 at UT 02:20 D. Darling (sun Praire, WI, USA, 12.5" reflector, x170, S=8, VG, T=5) obtained the brightest measurement he had ever recorded on the northern rim of Proclus. Brightness 9 and adjacent plain was of brightness 6.5. The Cameron 2006 catalog ID=308 and the weight=3. The ALPO/BAA weight=3.
Gassendi 1976 Oct 04 UT 20:55-20:58 Observed by Robinson (Devon, England) - observer noted that the east outside wall was bright in red and normal in blue. Note that the Moon was 30 deg above the horizon at the time of the observation. The crater returned to normal at 20:58. Also seen by Moore (Selsey, UK) and Foley (Kent, UK). At 21:25-21:50 D. Sims (Dawlish, UK, 25cm reflector, x300, seeing IV and some cloud at times) noticed a possible obscuration over the southern part of Gassendi. He had been observing earlier at 18:40-19:30 but had not detected a TLP in Gassendi then. 22:11UT Robinson notices that the spot outside the east wall is again bright in red., though by 22:25 it had faded and was gone by 22:28UT. The Cameron 1978 catalog further quotes: "Vivid red spots & general red color seen around rim by 2 obs. At 2209h blood red small area was seen. 1 h later the most westerly (IAU?) of the peaks had become hazy white all other areas were sharp. (Indep. confirm.)." Cameron 1978 catalog weight=5 and catalog ID #1454. The ALPO/BAA weight=3.
Gassendi 1966 May 01 UT 19:30-00:21 Observed by Sartory (UK, 8.5" reflector, x500, S=G), Moore, Moseley (Northern Ireland, 12.5" reflector x350, S=E) and by Corralitos Observatory (Organ Pass, NM, USA, 24" reflector + moon blink) "Eng. moonblink & obscuration, also vis. confirm (Moore & Moseley alerted by Sartory. Corralitos MB did not confirm. - but they may not have been observing at the ame time?)." NASA catalog weight=5. NASA catalog ID #932. ALPO/BAA weight=4.
On 1980 Jul 24 at UT02:00 F. Graham (East Pittsburgh, PA, USA, 6" reflector) took some photos (albeit out of focus) that showed a bright spot on the west rim. Cameron comments that this spot was sharp compared to the rest of the photograph, so was probably a photographic artifact. The effect was not seen in the finder scope. The Cameron 2006 catalog ID=103 and weight=2. The ALPO/BAA weight=1.
Aristarchus 1966 May 01 UT 21:55-22:45 Observed by Paterson, Brown, Sartory, Ringsdore (England, 12" reflector x252 for the former and 8.5"? reflector for the latter) "Eng. moon blink system detected red spots with vis. by all but Ringsdore. Brown saw intense white spot NW of crater wall" NASA catalog weight=5. NASA catalog ID 933. ALPO/BAA weight=4.
On 1993 Jun 02 at Ut 04:30-05:45 S. Beaumont (Cambridge, UK) saw that the shadow of the Cobra's Head in Schroter's Valley was lighter and more diffuse seen at user defined locations of C or B rim (these were black versus medium gray for Cobra's Head). The TLP had vanished by 05:45UT. The Cameron 2006 catalog ID=462 and weight=3. The ALPO/BAA weight=1 because the date or time is wrong.
On 2004 May 01 at UT 22:20 R. Lena (GLR, Italy) received an image from one of his observers showing possible blue colour in Aristarchus crater and part of the ray towards Herodotus. The ALPO/BAA weight=1.
In 1949 Nov 03 UT 01:06 J.Bartlett (3.5" refractor, x100) noted that the floor of Herodotus was very dark, the east wall was very bright, and the floor contained a central bright peak. The BAA/ALPO weight=3.
Aristillus 1972 Dec 17 UTC 21:50-22:20 observed by Berger (51.5N, 9E, 60mm refractor, T=2, S=3) "Diffuse bright cloud in the NE corner of the crater" - Hilbrecht and Kuveler, Earth, Moon & Planets, 30 (1984), p53- 61.
Aristarchus, Schroter's Valley 1963 Dec 28 UTC 01:15-02:00 Observed by Olivarez, Edinburgh?, TX?, USA, 17" reflector) "In poorer moments of seeing, red on Aris. rim & Sch. Valley. Spurious seeing effects?". NASA catalog weight=1 (very low). NASA catalog ID #788.
Aristarchus 1919 Jun 10 UT 19:00-19:30 Observed by Lapshin (Russia) a "Greenish-yellow light shone from inside the crater for 1/2 hr. after which it returned to normal. Violet tint on W. bank & surrounding area & the dark color of the saddle & dark spot were distinct. Term. slightly E. of Herodotus. (Ast. E)=IAU W." NASA catalog weight=3. NASA catalog ID #372. ALPO/BAA weight=3.
On 1982 Dec 27 at UT 23:00 M. Price (Camberley, Surrey, UK, Seeing=III and transparency=good) observed that Piazzi-Smyth was brighter than Mon Piton at 23:00. Photographic atlas was checked to verify that this was abnormal. The Cameron 2006 catalog ID=193 and weight=4. The ALPO/BAA weight=2.
Plato 1906 Mar 07 UT 22:00? Observed by Fauth (Germany? 6" refractor) "Color (brightness?) greatly enhanced as on the previous nite" NASA catalog weight=3 (average). NASA catalog ID #324.
Moon 1967 Apr 22 UT 02:30 Observed by Dunlap et al. (Corralitos Observatory, Organ Pass, NM, USA, 24" reflector) "UV excess as in # 1029. Gradient was 10# at term. to 25-30$ at subsolar pt. (153 deg long)." NASA catalog weight=5 (very high). NASA catalog ID #1031.
On 1980 Jul 24 at UT22:10-22:55 P. Moore (Selsey, UK, 15" reflector, x360 and x400) found an area just south east of the central peak (and upto the wall) to be quite dark in blue light, but normal brightness in red light or in white light. All other features were normal colour- wise. At 22:55UT Tycho was normal again. Cameron 2006 catalog ID=103 and weight=4. ALPO/BAA weight=3.
On 2004 May 02 at UT03:24 M. and L. van Son (Bremerton, WA, May 1st 7:24PM PST) saw a naked eye flash on the Moon. The observers were glancing up at the Moon in daylight when they saw a bright white flash (observer and his wife together) in the upper/mid Mare Serenitatis region, west of the crater Posidonius. "Larger than how Venus appears". "It was a quick flash like white, intense lightning. I'm not sure how to report degrees of arc but if the face we see is 900, and we start from the east then the flash occurred about 225 arc seconds to the west. This was observed by the naked eye, with clear skies between us and the moon." The observers checked for signs of aircraft vapour trails but could not see any. There is a possibility that it could have been sun glint from an Iridium satellite, but this needs to be checked out and usually these last longer than the observed effect. It would be useful to obtain whole Moon images under the same illunination and libration so that we can judge this observation properly. The ALPO/BAA weight=4.
Herodotus 1965 Jun 11 UTC 21:35-21:40 Observed by Porta, Garau (Mallorca, Baleares, 4" refractor x250) "Red glow in crater at 2140, then clouds stopped obs. After clouds, floor was abnormal rose color" NASA catalog weight=5. NASA catalog ID #879. ALPO/BAA weight=4.
Cobra Head 1966 May 02 UT 20:05 Observed by Sartory (England, 8.5" reflector x400) "Eng. moon blink detected red spots, seen visually also". NASA catalog weight=4 (good). NASA catalog ID #934.
Gassendi 1966 May 02 UT 20:18-20:19 Observed by Sartory (England, 8.5" reflector x400) "Eng. moon blink detected red spots, seen visually also." NASA catalog weight=4 (high). NASA catalog ID #935.
On 1978 Mar 21 at UT 20:57 an Unknown observer observed a TLP in Aristarchus crater. The details for this report are still being looked up in the archives. In view of the uncertain details this TLP has been given an ALPO/BAA weight of 1.
Aristarchus 1982 Jul 03/04 UTC 20:55-01:08 Observed by Foley (Kent, UK, Seeing Antoniadi III) "Brightness variance" - CED 3.6-4.1-4.9. When the crater was dark it had a slate-blue-grey interior. Moore found the crater to be exceptionally bright and this was confirmed by J.D. Cook (CED 3.8-4.1). The Cameron 2006 catalog ID=174 and weight=5. The ALPO/BAA weight=3.
On 1982 Jul 03/04 at UT 20:45-01:08 J.D. Cook (Frimley, Surrey, UK) found the Mare Frogoris area, north of Plato was pink at 20:45UT. Saxton found flashes in Mare Frigoris and near thye Alps. The Cameron 2006 catalog ID=174 and the weight=5. The ALPO/BAA weight=2.
Interior craterlets could not be seen and some of the walls and exterior features were fuzzy. ALPO/BAA weight=1.
S. of Aristarchus 1951 Sep 13 UTC 14:00? Observed by Osawa (Japan, 6" reflector) "Bownish-red color, blue on NW rim of A." NASA catalog weight=3 (average). NASA catalog ID #546.
On 1965 Jun 12 at UT > 00:00 an unknown observer (Porta?) reported that the area of Herodotus and the Cobra Head expanded and the colour went to rose. The next night the floor was normal. In filters, phenomenon accentuated in orange. The cameron 1978 catalog ID=880 and weight=3. The ALPO/BAA weight=2.
On 1964 Jun 23 at UT 04:45-05:05 Bartlett (Baltimore, MD, USA, 5" reflector, x180, S=4-1 and T=3) observed a blue-violet glare on the north east rim and a strong violet tinge in the nimbus. The effect was absent 1 hour earlier. The Cameron 1978 catalog ID=821 and weight=4. The ALPO/BAA weight=2.
Aristarchus-herodotus 1967 Apr 22 UT 20:20 Observed by Schobel (Hirschfelde, Germany, 5"? refractor) "Interference filter. (indep. confirm. of Darnella?)" NASA catalog weight=5. NASA catalog ID #1032. ALPO/BAA weight=2.
Aristarchus 1967 Apr 22 UT 21:00? Observed by Classen (Pulsnitz Obs., E. Germany) & by Corralitos Observatory (Organ Pass, New Mexicoo, 24" reflector+Moonblink). "Crater was so bright it could be seen with the naked eye (indep. confirm. of Darnella & Schobel of activity here?). Corralitos M.B. did not confirm." NASA catalog weight=3. NASA catalog ID #1034. ALPO/BAA weight=3.
Aristarchus, Schroter's Valley, Herodotus 1967 Apr 22 UT 21:45 Observed by Darnella (Copenhagen, Danemark, 3.5" refractor) & Coralitos Observatory (Organ Pass, New Mexico, USA (24" reflector + Moonblink). "Red pts. suspected in same areas as in #1030, but seeing was bad. (confirm by Schobel?). Corralitos MB did not confirm" NASA catalog weight=5. NASA catalog ID #1033. ALPO/BAA weight=2.
Aristarchus normal in red and blue filters however the Cobra Head part of Schroter's Valley was brighter in blue. Indeed it was very dull in red - Louderback says that this was not surprising as the whole areas around Aristarchus is brighter in blue. Louderback is an experienced observer of the Aristarchus area of more than 10 years. Cameron 2006 extended catalogID=63 and weight=1. ALPO/BAA weight=1.
LeCroy Jr. and Sr. (Springfield, VA, 4.5" reflector, x75, x300, S=3, T= 4) observed the following in the Aristarchus and Herodotus region: "Both were fused together as an oval & had a bluish cast on the E.rim. In W#25 filter it was white. At 0100h albedo decreased from 10+ to 9.5 & more detail could be seen. Separation of the 2 craters began to be seen at 0007h, details much brighter, incl. c.p. in Aris. @ 0110h main brightness & blue tint shifted to N. rim. At 0116h the SW rim was brightest & no color. At 0122h ray was brightest & no color. At 0122h ray had decreased in length & more details seen in oval. At 0123h ray was broken & smaller, becoming very small at 0125h & at 0126. The knob was gone & the edges not bright any more. Albedo=9. Sketches. (Seeing variations meas. were 1/2s in length so LTP variations not due to local atm. cond. Alt. = 65 deg". The Cameron 1978 catalog ID=1416 and weight=3. The ALPO/BAA weight=3.
Gassendi 1976 Oct 04 UT 21:30 P. Moore (Selsey, UK, x400, seeing poor) observed redness in the c.p. area. The ALPO/BAA weight=1.
On 2009 Jan 09 at UT 20:00 P. Brierley (UK) took a CCD image of the Aristarchus area - P.Grego upon examining this comments that he thinks that Schiaparelli crater looked "muted in brightness -- it is normally quite bright to look at". Though Grego comments that it might have something to do with the image processing aplied to the image. The ALPO/BAA weight=1.
Eratothenes 1954 Jul 14 UT 04:18-05:00 Observed by Bartlett (Baltimore, MD, USA, 5" reflector, x150, S=4, T=3) "Violet glare on E. wall bright spot (EWBS)" NASA catalog weight=4 (high). NASA catalog ID #565. ALPO /BAA catalog weight=3.
On 1964 Jan 27 at 21:00? Scarfe (UK) obtained spactra showing luminescence? The Cameron 1978 catalog ID=797 and weight=5. The ALPO/BAA weight=3.
Alphonsus 1966 May 03 UTC 21:30 Observed by Smith (England, 10" reflector) and Corralitos Observatory (Organ Pass, NM, USA, 24" reflector, Moonblink) "Reddish patches. Not confirmed by Corralitos MB (but in their report they give the feature as Gassendi)." NASA catalog weight=2. NASA catalog ID #936. ALPO/BAA weight=1.
On 1987 Mar 13 at UT 20:52 M. Mobberley (Suffolk, UK, S=VG) obtained some video that shows variation in Aristarchus crater e.g. � visual oddity in the SE corner" (Foley was interpreting the video). H.Hatfield took some film of the TLP (Unstudied yet). The Cameron 2006 catalog ID= 301 and the weight=5.
On 1987 Mar 13 at UT 20:52 M. Mobberley (Sussex, UK) found that Mons Pico varied in its north east section. This was recorded on video tape. The Cameron 2006 catalog ID=301 and weight=5. The ALPO/BAA weight=2.
Madler 2005 Oct 17 UT 04:14-05:28 Observed by Robin Gray (Winnemucca, NV, USA, 152mm refractor, x228, x343, S=5-8 and T=5-6) "Very bright pinpoint spot seen towards end of observing period on east crater wall, lasting 1 min in duration. Brighter than other spots, possibly 8.5-9 on the Elger scale. The spot was not seen earlier during the long observing session." An ALPO report. The ALPO/BAA weight=3.
Madler 1940 Sep 16 UT 02:10 Observed by Haas (New Mexico? USA, 12" reflector?) "Bright spot on S. rim was I=5.8 comp. with 8.9 on Aug 17 (see #470)." NASA catalog weight=4. NASA catalog ID # 473. ALPO/BAA weight=2.
On 1980 Aug 25 at UT06:55-07:10 Bartlett (Baltimore, MD, USA, 4.5" reflector, x40-150, seeing=4 and transparency=4) found the west wall bands of Aristarchus to be faint initially and at 07:00 a pale red colour appeared suddenly (and lasted for 2 minutes) on the inner south east wall, and then into south west BS to the west BS. "BS" meaning in Bartlett's notation a bright spot. There was no violet glare this time. Cameron 2006 catalog ID=106 and weight=4. ALPO/BAA weight=3.
Aristarchus 1969 Apr 01 UT 18:35 Observed by Kozyrev (Crimea, Ukraine, 40" reflector). "Spectrograms of an unusual red spot on W. slope at ?=.405, eta=.680. Spot = 1-2 km in diam. Molecules identified were N2 & C2. Later thru clouds crater was bluer in Corralitos (New Mexico) MB (confirm. of activity at Ariz. ?)." NASA catalog weight=5. NASA catalog ID #1119. ALPO/BAA weight=5.
Plato 1967 Apr 24 UT 02:50 K.Simmons (Jacksonville, FL, USA, 10" reflector) observed a large bright (intensity 6.5) oval area on near the central floor. According to Ricker and Kelsey (ALPO selected area coordinators) this is unusual. ALPO/BAA weight=1.
On 1969 Sep 25 at 19:00?UT Azeau (Paris, France, 12" reflector, x100, Seeing = good, altitude=20 deg) observed during an eclipse brilliant points for 30 minutes in Ross. Cameron says that the date given originally (16th Sep) was wrong because the age was 5 days and not full Moon. There was however a peumbral eclipse on Sep 25th at 20:10 (max). The Cameron 1978 catalog ID=1201 and weight=1. The ALPO/BAA weight=1.
On 1950 Sep 26 at UT 02:52, 03:10 Reid (Montreal, Canada, 6" reflector x48) and Venor (Montreal, Canada, 12" reflector) observed a brightening, fading, and brightening in Aristarchus crater during totality. There was a phosphorescent glow (date not given but times match this eclipse). cameron suggests that this is a confirmation report. The cameron 1978 catalog ID=538 and weight=5. The ALPO/BAA weight=3.
On 1964 Jan 28 at 21:00? Scarfe (UK) obtained spactra showing luminescence? The Cameron 1978 catalog ID=798 and weight=5. The ALPO/BAA weight=3.
On 1975 May 25 at UT 05:00-06:00 an unknown US observer took a photograph of a lunar eclipse that shows Aristarchus gleaming white. The Cameron 1978 catalog ID=1406 and weight=5. The ALPO/BAA weight=2.
On 1975 May 25 at UT 05:00-06:00 an unknown US observer took a photograph of a lunar eclipse that shows a bright spot on the east (IAU?) rim of mare Serenitatis (Romer?). The Cameron 1978 catalog ID= 1406 and weight=5. The ALPO/BAA weight=2.
eclipse an unconfirmed impact flash on the Moon. The ALPO/BAA weight=3.
On 1938 May 14 at UT 05:00-09:25 deWitt (Nashville, Tennessee, 12" reflector) observed during an eclipse the fading of the dark spot in Riccioli to be pronounced. Cameron says that the mid eclipse was at 03:39, photos?. Cameron 1978 catalog ID=436 and weight=3. ALPO/BAA weight=2.
On 1903 Apr 11 at UT 23:44 Zlatinsky (Russia) observed the following for Tycho? or Aristarchus?: "Dur. a lunar eclipse a bright extension of lunar (rays?) in shadow for 30m until mid-ecl." was seen. W.W. Magness (England, UK, 3" refractor) also saw two bright streaks of light, either side of the uneclipsed crsecent of the Moon. The Cameron 1978 catalog ID=217 and weight=2. The ALPO/BAA weight=2.
On 1906 Aug 04 at UT 12:30-13:30 Ward (England?) observed during a lunar eclipse Aristarchus to shine conspicuously. Cameron says that UT time is on the new system (as opposed to local time) with the mid eclipse at 13:00UT. The cameron 1978 catalog ID=325 and the weight=1. The ALPO/BAA weight=1.
Aristarchus 1971 Aug 06 UTC 03:45 Observed by Nelson Travnik (Matias Barbosa, Minas, Brazil, 6" refractor) "Color photo showing crater very bright comp. with all other features. Says glare at Aris. (seen vis. ? Apollo 15 watch? Date typed 06-08-71. European format? if date = June 8, aux. data are same except solar 3-.14+ & fates & times of Perigee, apogee, & FM differ)." NASA catalog weight=5. NASA catalog ID #1304. ALPO/BAA weight=2.
On 1910 Apr 01 at UT 22:00-23:00 LeRoy (France?) during an eclipse, observed Tycho to be visible as a very bright spot standing out in the slate grey shadow. Apparently only Tycho was seen during the elipse. The mid eclipse point was at 22:14UT. The Cameron 1978 catalog ID=236 and the weight=1. The ALPO/BAA weight=2.
1924 Aug 14 UT 20:00 Herodotus observed by Chernov (Russia, 2" refractor?). Weak luminescence seen in mid lunar eclipe. The Cameron 1978 catalog ID=390 and weight=3. The ALPO/BAA weight=2.
eclipse an unconfirmed impact flash on the Moon. The ALPO/BAA weight=3.
Aristarchus 1968 Mar 14 UT 01:32-02:06 Observed by Olivarez, Maley, Etheridge (Edinburgh, TX, USA, 17" reflector, x125 + Moon Blink) and Corralitos Observatory (Organ Pass, NM, USA, 24" reflector, Moon Blink) "S=5 (F-G) for the TX observations. "Trident Moon Blink on S. wall creet & c.p. & white spots in crater. No color seen vis. Blink not seen earlier or later. Other craters blinked some but not as strongly. Only Aris. areas blinked when Moon blink was moved around. Observers consider blinks real. Alt. of moon was 50 deg. Drawings. Corralitos say they did not confirm, but they rep't Copernicus, not Aris." NASA catalog weight=5 (very high). NASA catalog ID #1062.
Moving glows seen around the middle of the disk during a lunar eclipse. It is possible that the TLP referred to might have been from the 1783 Mar 18 eclipse instead?
On 1881 Dec 05 at UT 17:09 Johnson observed a dark lunar eclipse. Aristarchus was seen as a white spot in the coppery disk and continued so. Cameron comments that this is the normal apeparance in an eclipse? The Cameron 1978 catalog ID=226 and the weight=0. The ALPO/BAA weight=1.
On 1978 Sep 16 at UT 18:28-18:57 G.Searle (Concord, Sydney, NSW, Australia, 8" reflector, x100, x160, S=III) observed a bright star-like point on the western (IAU) edge of Mare Tranquilitatis (x100) that appeared unlike any other crater and a check of the location revealed no suitably bright crater in that region (from a map?). Changed to a higher power (x160) and it was still there, but not as conspicuous. Observer thinks that this may have been due to the Moon's low altitiude (16 deg) and the seeing. At 18:35 he compared it to the brilliant crater Proclus and found the star-like point to be 75% of the brightness of Proclus. Ken Wallace (Australia) had been taking photos and observed the object at 17:37.5UT. The object gradually faded over the next 15 minutes and by 18:52UT could only be seen in averted vision at x100. By 18:57UT it was gone. The Cameron 2006 catalog ID=38 and weight=5. The ALPO/BAA weight=3.
In 1954 Jan 19 at UT 03:00 Porta (Mallorca, Baleares, Spain, 3" refractor, x50) observed the following during a total lunar eclipse: "3 brilliant yellowish-white spots between Picard & Peirce. Phosphor. light distinguished easily against gray-green background of mare. Irreg., intermittent. Did not perceive them all dur. totality. Next day had impression that all of area was less clear & lightly veiled.". The Cameron 1978 catalog ID=561 and weight=3. The ALPO/BAA weight=2.
On 1942 Aug 26 at UT 04:00 Haas (New Mexico?, USA, 12" reflector?, very clear sky and good seeing) observed (during an lunar eclipse) found an unmistakable lightening of a dark albedo area in Atlas. This area returned to normal darkness during the 4 houres after Atlas re-entered sunlight. Cameron says that the mid eclipse was at 04:00. The Cameron 198 catalog ID=489 and weight=4. The ALPO/BAA weight=2.
On 1954 Jan 18 at UT 23:30-03:30 Dubois (Floira, France) observed in Oceanus_Procellarum and East Mare Fecunditatis, during a lunar eclpise (mid eclipse at 03:00) a spectrographic excess luminescence: 1) waxing totality max. sready near 445nm at 50' from centre of umbra; 2) waning tolatity, 470-505nm, max near 490nm, 25% at 50' from centre of umbra. Other observers noted a thin sliver of white on the edge of the Moon, despite it being in totality. The Cameron 1978 catalog ID=560 and weight=5. The ALPO/BAA weight=5.
On 1978 Sep 16 at UT19:30 R. McKin (Colchester, Essex, UK, 216mm reflector and binoculars) observed that Aristarchus, in the lighter region, during the lunar eclipse, was duller than usual but no less conspicuous than expected. The Cameron 2006 catalog ID=38 and weight=5. The ALPO/BAA weight=1.
On 1964 May 26 UT 04:10-04:35 Bartlett (Baltimore, MD, USA, S=5, T=5). observed that Aristarchus had a strong blue-violet glow on the east wall and EWBS, with a strong violet tinge on the nimbus. Crater was hazy, could not focus it in red, green or blue light. The Cameron 1978 catalog ID= and weight=4. The ALPO/BAA weight=2.
On 1982 Jan 09 at UT18:46-21:42 P. Moore, (Selsey, UK) and others found that Aristarchus and Plato changed in brightness and colour during a lunar eclipse. Aristarchus was especially bright during the lunar eclipse. Cameron 2006 catalog ID=162 and weight=5. ALPO/BAA weight=3.
On 1982 Jan 09 at UT 18:46-21:42 P. Moore (Selsey, UK) and other observers noted Censorinus was exceptionally bright. Cameron 2006 catalog ID=162 and weight=5. ALPO/BAA weight=2.
On 1982 Jan 09 at UT18:46-21:42 Henderson, Sykes and Radley saw an obscuration near Le Verrier - a completely circular halo with dark mare showing through it for a duration of 15 minutes. This was during a total eclipse of the Moon. Cameron 2006 catalog ID=162 and weight=5. ALPO/BAA weight=3.
On 1982 Jan 09 at UT21:37 P. Moore (Selsey, UK) observed that Plato underwent brightness and colour changes, during a total lunar eclipse. At 20:07UT Madej observed a "slight anomaly in Plato". Cameron 2006 catalog ID=162 and weight=5. ALPO/BAA weight=3.
On 1982 Jan 09 at UT 18:46-21:42 M.Mobberley (UK) observed that Schmidt was very bright compared to its surroundings during a total lunar eclipse. Cameron 2006 catalog ID=162 and weight=5. ALPO/BAA weight=2.
On 1982 Jan 09 at UT18:46-21:42 Bouron (UK?) observed that the west limb, during a total lunar eclipse, had dark orange on it. Cameron 2006 catalog ID=162 and weight=5. ALPO/BAA weight=1.
On 1984 Dec 07 at UT 19:30-23:30 M. Mobberley (St Edmunds, UK, seeing=IV-V, transparency=good, spurious colour seen) found 2 bright pathces on the east rim on alternate sides of a bright region. The band from the central 16km wide region was dark on the east side. Foley (Kent, UK, 12"reflector, seeing=II-III) found Aristarchus to be not as bright as normal, apart from the band that Mobberley found (1 hour later). The dark regions were a murky green colour (bright through green, blue and yellow filters and dark through red and orange filters). Cook (Frimley, UK, transparency=excellent, CCD camera used) found a bright "bulge"on the eastern side. Apparently data suggests that the band was brighter in red than in near IR light. Cook's calibrated brightness measurements suggest that there was no change in brightness over the crater with time. Two other bright points were seen: one at the Cobra's Head and another half way between the east rim of Aristarchus and passes Herodotus. Wratten 29 (deep red), Wratten 87 (near IR) and combined Wratten 29 and Wratten 87 were used. In the red Wratten 29 filter the brightness falls at22:20 at Shroters valley and then rises in the bright ray. They return to normal at 22:30UT. There was however a lot of measurement noise from the brightness readings of points B and D. The Cameron 2006 catalog ID=256 and the weight=5. The ALPO/BAA weight=3.
On 1963 Dec 30 at UT11:00 many observers reported seeing a red glow on the North East (IAU?) limb of the Moon. This was also captured on a photograph. Cameron suggests eclipse geometry as an explanation. Thye Cameron 1978 catalog ID=792 and weight=1. The ALPO/BAA weight=1.
On 1953 Jan 29/30 UT 23:00?, 01:00? Dubois (Floirae, France) observed excess luminescence, in Mare Fecunditatis, between 420nm and 470nm (maximum at 435nm) and between 480nm and 520nm (maximum near 505nm). 20-60% during eclipse at 50' from the centre of the umbra, during a lunar eclipse. The cameron 1978 catalog ID=557 and weight=5. The ALPO/BAA weight=4.
On 2000 Jan 21 UT04:40 G. Emersen (Golden, CO, USA, 30cm focal length lens with Wratten 25 ref filter) took 43 CCD images of the eclipse of the Moon and on one of them at 04:40UT (exposure 0.3 sec) a relatively bright spot appeared in the southern part of Mare Fecunditatis. The spot looks sharper than the rest of the Moon and so might be a cosmic ray? CCD images taken from Washington D.C. by A.C. Cook at this time, do not show this spot, however exposures were at intervals of 0.25 sec and so might have missed this spot if it happened during image readout. The ALPO/BAA weight=1.
On 1953 Jan 29-30 UT 23:05-01:40 G. Brown (UK?) observed a white patch of light of low brightness was seen to move around the north polar area. Coloured bands were also seen on the Moon.
On 1877 Feb 27 at UT19:19 Prof. Dorna (Turin, Italy) observed a flickering light on the lunar surface during a lunar eclipse. The Cameron 1978 catalog ID=186 and the weight=2. The ALPO/BAA weight=2.
Kepler 1962 Jul 17 UTC 06:24,08:36 Observed by Wildey, Pohn (Mt Wilson, CA, USA, 60" reflector+photometer) "Crater was at Vmag 2.68 at earlier obs. which was .47 mag brighter than av. mag. at 15d & it faded to near normal at later time to V=3.10(photom. measures), a change of 1/2 mag. or @1.5 times in brightness" NASA catalog weight=5 (very good). NASA catalog ID #761.
On 1963 Jul 06 UT 20:35-23:00 during a partial eclipse of the Moon, some feathery fingers of light were seen in the shadow.
On 1963 Jul 06 at UT 21:00 (estimated) Chernov (Russia) observed that the dark spot in Riccioli size increased suddenly during a lunar eclipse as it entered the shadow, before merging with the shadow. The mid eclipse was at 22:03UT. The cameron 1978 catalog ID=774 and weight=1. The ALPO/BAA weight=1.
On 1956 Nov 18 J.P. Bagby organized a lunar eclipse observing session in the USA. He recorded 35 bright objects against the Moon, 5 of these were seen by 3 other observers. J. Mavrogianis and 4 other observers observed 25 transient luminous objects - mostly stationary yellow flashes. However another group at Cheyenne noted a 4 sec duration light. This report is described in H. Hars "The Total Lunar Eclipse of November 18, 1956", Strolling Astronomer, 11:64, 1957.
On 1884 Oct 04 at UT 22:00 Bye (Brussels, Belgium) observed during an eclipse that the peaks were visible as brilliant points with slight red aureoles during a lunar eclipse. Cameron says that this was a confirmation of #2443. The Cameron 1978 catalog ID= and the weight=5. The ALPO/BAA weight=2.
Parsehlan of England? saw Tycho as a 2nd magnitude star during a total lunar eclipse. The Cameron 1978 catalog ID=244 and weight=5. The ALPO/BAA weight=3.
On 1893 Apr 01 at UT 22:00 deMoraes of the Azores, Portugal, saw a shaft of light projecting from the Moon. Cameron 1978 catalog ID=280 and weight=0. ALPO/BAA weight=1.
In 1921 Oct 16 at UT 22:00-00:00 Genin and others (Russia) observed during a partial eclipse that different parts of Aristarchus crater had brightness of phosphorecence. Cameron says that this is independent confirmation. The Cameron 1978 catalog ID=383 and weight=5. The ALPO/BAA weight=3.
On 1971 Aug 06 at UT 20:30 Chernov (Crimea?, Ukraine, Soviet Union) observed a dark spot in Riccioli that was very dark for 3 minutes, before coming out of shadow - however the dimensions were normal. This was during the lunar eclipse. The Cameron 1978 catalog ID=1305 and weight=3. The ALPO/BAA weight=1.
On 1971 Aug 06 at UT 21:00 Chernov (Crimea?, Ukraine, Soviet Union) observed that two large spots in Atlas were not visible in the penumbra after totality (brighter than normal?). The Cameron 1978 catalog ID= 1306 and weight=2. The ALPO/BAA weight=1.
On 1975 Nov 18/19 at UT 23:15-0005 LeCroy Jr and Sr (Springfield, VA, 4.5" reflector, S=7) observed that Delambra was one of four glowing spots on the Moon during a lunar eclipse (including Aristarchus). At 23:50UT 3 of these patches emerged from the dark and appeared as bright spots compared to other craters "�lbedo=10+". The Albedos of Manilius and Delambre were 8.5 at 00:05UT. Details became apparent in all 3 features. The Cameron 1978 catalog ID=1419 abd weight=0. The ALPO/BAA weight=1.
On 1975 Nov 18/19 at UT 23:15-0005 LeCroy Jr and Sr (Springfield, VA, 4.5" reflector, S=7) observed that Manilius was one of four glowing spots on the Moon during a lunar eclipse (including Aristarchus). At 23:50UT 3 of these patches emerged from the dark and appeared as bright spots compared to other craters "�lbedo=10+". The Albedos of Manilius and Delambre were 8.5 at 00:05UT. Details became apparent in all 3 features. The Cameron 1978 catalog ID=1419 abd weight=0. The ALPO/BAA weight=1.
On 1975 Nov 18/19 at UT 23:15-0005 LeCroy Jr and Sr (Springfield, VA, 4.5" reflector, S=7) observed that Menelaus was one of four glowing spots on the Moon during a lunar eclipse (including Aristarchus). At 23:50UT 3 of these patches emerged from the dark and appeared as bright spots compared to other craters "�lbedo=10+". At 23:55UT a ray appeared out of the north east rim of menelaus (Normal?). It appeared just before the artea emerged and increased in brightness. At 23:58UT it decreased and continued to do so. The north east edge of Menelaus appeared very dark at the point that the ray was extending from SW edge (a ridge there) and apperared to obscure features along its path (Albedo=9). The Albedos of Manilius and Delambre were 8.5 at 00:05UT. At 00:05UT the rays were still apparent but seemed to have returned to normal. Details became apparent in all 3 features. The Cameron 1978 catalog ID=1419 abd weight=0. The ALPO/BAA weight=1.
On 1888 Jan 28 ~UT 23:20 Dyer observed that in this fairly bright lunar eclipse was a dark isosceles triangle, with the base to the north. Other observers noted this effect.
Moving glows seen around the middle of the disk during a lunar eclipse.
On 1963 Jul 06 at UT 23:00 (estimated) Chernov (Russia) observed in Atlas 2 large spots that were not visible in penumbra after totality. The cameron 1978 catalog ID=775 and weight=2. The ALPO/BAA weight=1.
On 1891 May 23 at 18:36-19:15 UT, Jackson of Sheffield, England, using a 6" refractor, saw "1/2 hour before the end of a totl eclipse, a region of the crater and just north of it, become conspicuous and increased in brightness from then on" Cameron thinks this is just the edge of the shadow and possibly normal. Cameron 1978 catalog ID=268 and weight=0. ALPO/BAA weight=1.
On 1978 Mar 24 UT16:10-17:45 Anderson (England?, 8" reflector, x55 and x155). Censorinus seemed brighter than normal. Cameron 2005 catalog report ID=26 and weight=1. ALPO/BAA weight=1.
On 1978 Mar 24 UT16:10-17:45 Anderson (England?, 8" reflector, x55 and x155). noticed a faint twinkling star like point in Dionyius - remained constant but when changed to x155 at 16:25 the effect was at the limits of visibilty. - suspected that this was due to the atmospheric conditions. However this effect was not seen in Aristarchus. By 16:45 the twinkling area got brighter, but went back to normal at 17:45. Cameron 2005 catalog report ID=26 and weight=1. ALPO/BAA weight=1.
In 1954 Jul 16 at UT 01:12 Chernov (Russia, 2" refractor, x33) observed the following for Aristarchus: "Activity noted in it * in extension of Moon's shadow on sky for 12 min during .17phase of ecl.(source gave date as June 16, but ecl was July 16)". The Cameron 1978 catalog ID=566 and weight=1. The ALPO/BAA weight=1.
Bright light seen during eclipse. Date given as 8th but the Full Moon was on 6th according to Goldatine's "New & Full Moon's"). ALPO/BAA catalog weight=1. Cameron catalog weight=3. Cameron Catalog ID: 4. Julian date 1096 Aug 06. Gregorian date 1096 Aug 12.
On 1905 Aug 15 at UT 03:30 Rey (Marseilles, France) observed Tycho during a lunar eclipse to be visible, indeed it was described as brilliant during the eclipse (mid eclipse 03:31UT). The Cameron 1978 catalog ID=322 and weight=1. The ALPO/BAA weight=1.
Plato 1967 Nov 17 UTC 18:36-18:50 Observed by Moore, Moseley (Armagh, Northern Ireland, 10" refractor x260) "Faint blink under SW wall. Nothing seen vis. Gone by 1839h. Reappeared at 1841, then gone by 1850h. Checks till 0200h were neg. Obs. dubious of reality of phen." NASA catalog weight=2. NASA catalog ID #1054. ALPO/BAA weight=1.
Kepler 1967 Oct 19 UTC 05:00 Observed by Classen (Pulnitz Obs. East Germany, 8" reflector) and Corralitos Observatory (Organ Pass, NM, USA, 24" reflector + moonblink) "It was 1 mag brighter than aristarchus when normally Aris. is 0.3mag. brighter than Kep. Corralitos MB did not confirm." NASA catalog weight=4 (good). NASA catalogue ID #1052.
On 1906 Feb 08 after a lunar eclipse, Frost and Stebbins determined that Linne had enlarged by 1" in size.
East of Picard 1864 Oct 16/17 UT 23:00-01:00? Observed by Ingall (Camberwell ?, UK) "Remarkable bright spot" NASA catalog weight=3. NASA catalog ID #135. ALPO/BAA weight=3.
Macrobius 1938 Nov 08 UTC 18:00? Observed by McLeod (England? 5" ? reflector) "Changes in dark areas. (near Proclus where Green saw phenomenom. see #443)" NASA catalog weight=2 (low). NASA catalog ID # 444.
Gassendi 1940 Sep 18 UTC 03:15 Observed by Haas (New Mexico? 12" ? reflector) "Largest bright spot in SE part of floor had I=6.1, but I=6.7 & 8.6 on other nites. (same ph. see #469, 472 & 475)" NASA catalog weight=4. NASA catalog ID #474. ALPO/BAA weight=2.
On 1992 Jul 16 at UT 03:32-09:31 D. Louderback (South Bend, WA, USA, 3" refractor, x134) detected yellow on the southern rim of Aristarchus, and the colour looked "darker" through a yellow filter and the region was "duller" than normal. The region was 1 intesnsity step brighter on the 2nd measurement, "on all points in it". The comet tail-like ray had 3 sections and was "mottled" in appearance. Finally the Cobra Head region had possible variations in brightness. The cameron 2006 catalog ID=451 and the weight=3. The ALPO/BAA weight=2.
On 1967 Apr 26 at UT 03:00 Kozyrev (Crimea?, Soviet Union) observed Gas luminescence in Aristarchus crater. The Cameron 1978 catalog ID=1069 and weight=3. The ALPO/BAA weight=3.
In 1954 Jul 17 at UT06:50-07:15 Bartlett (Baltimore, MD, USA, S= 5, T=5-1) observed near Aristarchus: "Pale violet tint on surface NE of crater, no color elsewhere". The Cameron 1978 catalog ID=568 and weight=4. The ALPO/BAA weight=1.
LaLande 1973 Jul 17 UT 03:30-03:45 Observed by Galgoey (Washington, NJ, USA, 2" refractor x46, x117), S=VG, T=5) "Star-like pt., variations, 1- 2s, seen only at 40x, not at higher powers. LTP albedo =10, normal=8, nearby plain =6 (geom, instrum. & atm. & refl. material at site effects?)" NASA catalog weight=1 (very low). NASA catalog ID #1371.
(Baltimore, MD, USA, 5" reflector x180) "Strong violet glare on E. rim, changing to brown. At 0220 dark viol. in nimbus, at 0235 viol. changed to brown. At 0255 viol. suddenly reappeared, but faded to invis. at 0300. Again at 0308 reapp. Only time he ever saw such color changes." NASA catalog weight=4. NASA catalog ID 583. ALPO/BAA weight=3.
On 1990 Jan 14 at UT 01:14-01:55 M.C. Cook (Frimley, UK, seeing=poor) observed that Aristarchus did not appear normal for this illumination. the northern half of Aristarchus was "2x>" than the southern half of the crater. There were two white patches of apron material near to the crater Herodotus that were 50% of the brightness of the southern half of Aristarchus. Furthermore the southern half of Aristarchus had a circle - "dull patch on inner S wall with a bright point shining through it. (Bartlett's EWBS?)". The Cameron 2006 catalog ID=389 and the weight=4. The ALPO/BAA weight=2.
On 1980 Mar 04 at UT10:30-10:34 D. Darling (Sun Prairie, WI, USA, 12.5" reflector, x344) detected a pin-point light in the shadowed area of Mare Crisium that varied in brightness then faded. Cameron 2006 catalog ID=84 and weight=0. ALPO/BAA weight=1.
Gassendi 1940 Sep 19 UTC 06:00 Observed by Haas (New Mexico, 12?" reflector) "Largest bright spot in SE part of floor, had I= 6.7, but 6 for last nite & 5.6 on others (see #'s 469, 472, & 474)." NASA catalog weight=4. NASA catalog ID #475. ALPO/BAA weight=2.
Furnerius A 1983 Jan 02 UT 00:10 H. Hill (UK) observed that this crater was piercingly bright, which he thought was a bit unusual. ALPO/BAA weight=1.
Cleomedes 1991 Dec 23 UTC 22:50 Observed by Mizon (Colehill, Dorset, UK, 8" f/6 reflector x216) "Oval or pear-shaped ashy glow visible for 2 min, then vanished quite suddenly" - Ref. personal communication received by BAA Lunar Section.
Plato 1938 May 17 UTC 08:00 Observed by Haas? (New Mexico?, USA, 12" reflector?) "Floor-least bit greenish (other colors on other dates, e.g. Je 23, 7/22/37, & 7/15/38)." NASA catalog weight=3 (average). ALPO/BAA weight=2. NASA catalog ID #437.
Peirce A (Swift=IAU name?) 1937 Dec 23 UTC 22:00 Observed by Wilkins (England, UK, 12.5" reflector) "Obscuration on floor if crater. Crater invis. (similar to #394, 396)." NASA catalog weight=4 (high). NASA catalog ID #412.
On 2005 Oct 21 at UT 13:07-14:27 R. Gray (Winnemucca, NV, USA, 15cm F/9 refractor, x228, seeing 4-5, transparency 5-6) observed a possible TLP in Macrobius. His report is as follows: "Blinked Macrobius with Wratten Filters Blue 38A and Red 29. Macrobius became almost invisible through the Blue 38A and essentially the same as in white light through the Red 29. The interior of the crater was completely in shadow. The only part of the east wall that was visible was an apparent high point still in the sun and seen as a bright point of light. This faded into darkness before 13:56UT. No sign of any illumination of the east wall crater interior or the interior of the west wall was seen during the observation period. The outer west wall was a rough looking, complicated mix of deep shadow and illuminated sunlit terrain." The observer concluded that there was not a TLP - although he did get a filter reaction, this may have been due to the different densities of the filters? ALPO/BAA weight=2.
Macrobius 1898 Dec 31 UTC 20:00 Observed by Goodacre (Crouch End, England, 12" reflector) "Interior nearly filled with shadow at sunset. Inner E.wall very bright-a distinct penumbral fringe to black shad. cast on it from W.wall. Seen best using high powers. (Firsoff & MBMW give date as just 1895 but must be wrong-phase - see app.ref.)" NASA catalog weight=4 and catalog ID #304. ALPO/BAA weight=2.
On 1989 Aug 20 at UT13:55 M. Lucas (Melbourne, Australia, naked eye) witnessed a "pin-point flash" in the middle of the lower right quadrant of the Full Moon. Foley suspects that this was in the Proclus region? The Cameron 2006 catalog ID=374 and the weight=2. The ALPO/BAA weight=2.
On 1989 Jan 26 at UT 03:45 De Groof (Belgium) noted a white few second long flash from Copernicus crater. The Cameron 2006 catalog ID=347 and weight=3. The ALPO/BAA weight=3.
Messier A 1951 Oct 20 UT 00:00? Observed by Moore (England) "Brilliant white circular patch in it. has seen it & Messier blurred several times." NASA catalog weight=4 (good). NASA catalog ID #545 Note that the date and time given are probably wrong as the Sun is ~7deg below the local horizon at this time. ALPO/BAA weight=1 to reflect this error.
Aristarchus 1957 Oct 13 UT 07:00?$ W.Haas, according to the 1978 NASA Catalog is supposed to have seen a bright spot of light -- "explosion" in this crater. Confirmation of activity in Aristarchus - Three independent observations within 4 hours. Cameron 1978 catalog weight=5 and TLP ID No.=676. Private comunication with Haas shows that he recorded nothing unusual on the 12th or 13th. Therefore an ALPO/BAA weight of 1 has been given until this matter is cleared up.
On 1991 Jul 31 at UT 07:50 D. Louderback (South Bend, WA, USA, 3" refractor) observed that the south floor of Aristarchus was wellow - "almost gold, spilled over S wall on ray toward Herodotus". Cameron comments that Bartlett often reported a yellow floor but not a spill of the colour over to the external ray. Cameron also comments that Louderback's refractor would refract more in blue light than in yellow, therefore she did not think that it was due to chromatic aberation. The Cameron 2006 catalog ID=431 and the weight=3. The ALPO/BAA weight=2.
On 1991 Jul 31 at UT 07:50 D. Louderback (South Bend, WA, USA, 3" refractor) found that all of Mons Piton was "unusually dark". Points D, C (E and S resp), usually brightest points, but this time were not bright. "Whole mt was as dark as W wall usually is at this time. In violet filter Piton disappeared completely, but was a little brighter in red filter and points D & G showed. Color not seen by eye. No albedo measured. Suggests red event." Cameron rules out chromatic aberation from Louderback's refractor. The Cameron 2006 catalog ID=431 and the weight=3. The ALPO/BAA weight=1.
Plato 1975 Jun 28/29 UT 23:00-01:20. Foley (Wilmington, UK, 12" reflector, seeing, III, good clarity transparency). At 23:00, 00:30, and 01:15 blue was seen on the inner wall:floor southern boundary, and red on the corresponding northern floor:wall boundary. However by 01:20, blue was now on the S-NW floor:wall boundary, and red on the NE-SE floor:wall boundary. Atmospheric spectral dispersion existed in many regions, but did not change like the colours in Plato. Similar appearance craters such as Grimaldi, Schickard, and Riccioli, were checked for a similar change in colour, but no change was noticed in these. ALPO/BAA weight=1.
Stochard of Dublin, Ireland, saw naked eye at 10:30UT on 1862 Nov 12 Aristarchus as extraordinarily bright as a bright spot on the Moon. This was seen in daylight with the waning crescent. Cameron 2006 extension catalog ID=6 and weight=3. ALPO/BAA weight=2.
Callipus 1952 Sep 09 UT 21:00-21:20 Observed by Moore (England) "Hazy broad line of light seen fr. NW wall to SE wall over shad. floor. Gone next nite at 0120. He gave low wt. to obs. (sunlight between peaks?)." NASA catalog weight=1. NASA catalog ID #553. ALPO/BAA weight=1.
On 1991 Dec 28 at UT 02:10 P. Moore (Selsey, UK) could see no detail on the floor of Plato crater. This report needs to be read in context with the comments by Cameron for A.C. Cook's observation of the floor of Plato on 1992 Jan 18 - Cameron 2006 catalog ID=438.
1837 Mar10 UT 13:46 (19:07 local time) T.G. Taylor (Madras, India) whilst observing a 9th magnitude star being occulted, noticed a 6th magnitude nebulous spot where Aristarchus should be. Had never seen anything quite as bright as this on previous occasions. ALPO/BAA weight=2.
On 1983 May 15 at UT20:30-21:05 P.W. Foley (Kent, UK, 12" reflector) was unable to see Aristarchus in Earthshine, though other craters were clearly visible. However by 21:30 the Cooks could clearly see Aristarchus. The Cameron 2006 catalog ID=215 and the weight=0. The ALPO/BAA weight=2.
W.limb 1983 May 15 UT 20:30-21:00 R.Moseley (Coventry,UK, 6" reflector, x60) observed a faint but extensive brightening of the W.limb, perhaps a little stronger at PA=80-90 deg. No other features seen in Earthshine. Observation confirmed br R.Martiott (Northampton, UK, 8.5" reflector). ALPO/BAA weight=1.
On 1987 May 03 at UT 19:00-19:30 H. Miles (Cornwall, UK, 5" refractor, x30) found the Earthshine to be both pink and bright with prominent features clearly visible. A "brilliant" star-like point was seen in Aristarchus crater. There was another, albeit less bright spot near Darney-Agatharides. Spots pesisted despite various tests. Foley also confirmed that the Moon looked pink to him as well. The Cameron 2006 catalog ID=298 and weight=1. The ALPO/BAA weight=1.
On 1987 May 03 at UT 19:00-19:30 H. Miles (Cornwall, UK, 5" refractor, x30) found the Earthshine to be both pink and bright with prominent features clearly visible. A bright spot was seen near Darney- Agatharides. An even more "brilliant" star-like point was seen in Aristarchus crater. Spots pesisted despite various tests. Foley also confirmed that the Moon looked pink to him as well. The Cameron 2006 catalog ID=298 and weight=1. The ALPO/BAA weight=1.
On 1983 May 15 at UT21:30-22:30 M.C. Cook and J.D. Cook (Frimley, UK) could clearly see Aristarchus in Earthshine, whereas earlier that night P.W. Foley (Kent, UK) could not see the crater although other features were cisible. The Cameron 2006 catalog ID=215 and the weight=2. The ALPO/BAA weight=1.
On 1991 Dec 09 at UT 22:50 D. Darling (Sun Praire, WI, USA, 3" refractor, x36) witnessed a flash in Grimaldi crater. Cameron comments that others had seen a flash there earlier, and there was a meteor swarm. Fritschel (madison, WI, USA, naked eye observing) detected 3 flashes in Grimaldi and also at the western limb of the Moon. D. Weier (Sun Praire, WI, USA, 3" refractor, x36) was also observing. The Cameron 2006 catalog ID=436 and the weight=5. The ALPO/BAA weight=2.
On 1880 Nov 06 at UT 20:00 an unknown observer observed a TLP at an unknown location on the Moon. The Cameron catalog has an entry for this date and time but does not specify the location, the observer or what was seen. The Cameron 1978 catalog ID=218 and the weight=0. The ALPO/BAA weight=1.
On 1966 Apr 24 at 21:30UT R.Livsey (Scotland, 6" reflector at x275) observed that Aristarchus was "fluorescent" in Earthshine. It is uncertain whether the description of "fluorescent" should be involve this observation being categorized as a TLP, however just for safety it will be assigned an ALPO/BAA weight=1. This was a BAA Lunar Section report.
On 1983 May 16 at UT20:35-22:10 P.W. Foley (Kent, UK) noted that Aristarchus was dull in Earthshine (UT21:36-21:40). The floor was a luminous rose/violet colour. The Cameron 2006 catalog ID=219 and the weight=0. The ALPO/BAA weight=1.
On 1987 Mar 04 at UT 19:03-19:47 H. Miles (Cornwall, UK, 5" refractor, x30, S=clear) found at 19:03 that Aristarchus was exceptionally bright (even without blocking out the sunlit side of the Moon), being the most easily seen crater on the Moon, and this was despite the sky not yet being dark. The crater had faded by 19:20UT and at 19:47UT Earthshine was no longer visible. CED brightness measurements were made and were less than usual and the inside of the crater may have had a blue/gray colour (unclear from the Cameron 2006 catalog description). The Cameron 2006 catalog ID=299 and the weight=2. The ALPO/BAA weight=2.
On 1981 Jun 07 at UT02:30-03:00 B. Hobdell (St Petersberg, FL, USA, 10" and 4" reflectors, seeing=I) at 02:30UT saw a flash from Aristarchus and another one from Schroter's valley. By 02:45UT Aristarchus was starting to be difficult to see and had occasionally a bluish cast. By 03:00UT the crater could only barely be seen. This was odd because visibility on the Earthlit side was really rather good. The Cameron 2006 catalog ID=143 and weight=0. The ALPO/BAA weight=1.
On 1981 Jun 07 at UT02:30-03:00 B. Hobdell (St Peterberg, FL, USA, 10 and 4" reflectors, seeing=1) saw Copernicus to be very bright in blue. Clarty of Earthsine was exceptional tonight. The Cameron 2006 catalog ID=143 and weight=0. The ALPO/BAA weight=1.
W.limb 1983 May 16 UT 22:00-23:00 R.Moseley (Coventry,UK, 6" reflector, x60) observed a faint but extensive brightening of the W.limb, perhaps a little stronger at PA=80-90 deg. No other features seen in Earthshine although Aristarchus suspected. ALPO/BAA weight=1.
1837Mar11 UT 15:27 (20:48 local time) T.G. Taylor (Madras, India) whilst observing a star being occulted, noticed a 6th magnitude nebulous spot where Aristarchus should be. Had never seen anything quite as bright as this on previous occasions (except the day before). ALPO/BAA weight=2.
North shore of Mare Crisium 1915 Dec 11 UT 06:00? Observed by Thomas (Glenorchy, Tasmania) "star-like pt. on N. shore of mare. (Eimmart?) Particularly bright spot. Tho't it was sunlight from rim of sm. crater." NASA catalog weight=0 NASA catalog ID #358. ALPO/BAA weight=1.
On 1981 Jun 08 at UT01:48-02:45 B. Hobdell (St Petersberg, FL, USA, 10 and 4" reflectors) could hardly see Aristarchus crater, however at 01:48UT it brightened in blue for about 3 minutes. Then at 02:20UT there was a bright flash, and by 02:25UT the crater was very bright, but by 02:45UT it was no longer visible. Cameron 2006 catalog ID=144 and weight=0. The ALPO/BAA weight=1.
On 1983 May 17 at UT20:13-20:40 P. Madej (Huddersfield, UK, x38 and x63) found that Aristarchus was normal in appearance, but at 20:19 a blood red disk was seen as bright as a 6th magnitude star. The colour did not vary but the brightness changed from 4 to 8 over a 1.5-3min period, on the south west wall. Foley (Kent, UK, 12" reflector)observed Aristarchus at 22:10 and noted that it had the same rose-violet colour as had been seen by him a day earlier. The Cameron 2006 catalog ID=220 and the weight=0. The ALPO/BAA weight=3.
On 1983 May 17 Foley (Kent, UK, 12" reflector)observed Aristarchus at 22:10 and noted that it had the same rose-violet colour as had been seen by him a day earlier. The Cameron 2006 catalog ID=220 and the weight=0. The ALPO/BAA weight=2.
Daniell 1979 Apr 02 UT 21:45-22:14 Obseved by Madej (Huddersfield, UK, 158mm reflector, f/4.2, x36-110, seeing II-III) "Obscuration seen" BAA Lunar Section Report. Cameron says that this was a bright white cloud that covered three quarters of the crater. A yellow filter was used at 21:48, but the cloud was still white, albeit thinner (at x110). By 22:14UT the TLP was barely visible and again no colour seen. Buczynski (Lancaster, UK, seeing = poor) saw spurious colour. Later (22:31- 22:46UT?) Mellor obtained some photos, but these revealed no colour. The Cameron 1978 catalog ID=48 and the weight=3. The ALPO/BAA weight=2.
On 1983 Jan 19 at UT 18:00-19:00 G. Amery (Reading, UK) discovered that Aristarchus could not be seen in Earthshine, this was odd because less prominent features could be seen. Other observers (Moore and Foley) confirmed the very low brightness of the crater. The Cameron 2006 catalog ID=197 and the weight=2. The ALPO/BAA weight=2.
On 1983 Jan 19 at UT 18:00-19:00 G.W. Amery (Reading, UK) found that Messier was difficult to define. The Cameron 2006 catalog ID=197 and the weight=2. The ALPO/BAA weight=1.
Linne 1867 Aug 06 UT 21:00? Observed by Buckingham (England?) "Crater in darkness, he saw a "rising oval spot". Other obs. saw it as a triang. Bold black spot pointing to earth, slowly diffused white & drift of white on slope of pyramid. (indep. confirmation?)" NASA catalog weight=5 and catalog ID #155. ALPO/BAA weight=2.
Near Ross D (23E, 12N) 1964 May 18 UT 03:54-04:53 Observed by Harris, Cross et al. (Whittler, CA, USA, 19" relector x720, 8" reflector x322, S=G) "White gas obscuration. Moved 20mph, decreased in extent. Phenom. repeated. Drawing." NASA catalog weight=5. NASA catalog ID 811. ALPO/BAA weight=4.
White spot near Censorinus 1966 Dec 18 UT 23:40-23:46 Observed by Enie (Pittsburgh, Pennsylvania, USA, 8" reflector x100, S=G) "Attention drawn to pink color in this usually white patch. Brightened to a light reddish tinge for 2 mins, then faded back to pink, then to white, Sketch." NASA catalog weight=4 (high). NASA catalog ID #1002.
On 2000 Feb 11 at UT19:00 G. North (Norfolk, UK) telephoned TLP coordinator, Patrick Moore, to report a possible colour anomaly in Aristarchus. Moore had poor conditions in Selsey (UK) and saw nothing unusual. However by this time North was reporting that, the colour was fading. Two other BAA members were alerted, but were clouded out. The ALPO/BAA weight=3.
On 2001 Apr 29 at UT 20:50 R. Braga (Italy) reported that without any filter, the brightness of the east wall of Torricelli B was halfway Torricelli C (faintest) and Moltke (brightest). By insering a Wratten 25 red filter though, the crater was slightly more evident. However using a blue Wratten 39A filter, the crater vanished completely, whilst Toricelli C remained. The ALPO/BAA weight=3.
Webb (England, using a fluid achromat) saw brilliant minute spots and streaks in Mare Crisium dotting its surface. This was seen near first quarter. Cameron states that Schroter, Betr?, Madler, Slack and Ingall had all seen it this way at times. Cameron 1978 catalog iD=111 and weight=3. ALPO/BAA weight=2.


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Friday, July 20th, 2007
Google Gears for Offline Data Entry
Jack Herrington has written his second article in his series on Gears. The article goes into detail on creating a form based data entry application that works offline. This means that entries are batched up, so when the user goes online they can be sync'd up. The forms are sent using Prototype and Ajax.Updater. Jack Read the rest…
Posted by Dion Almaer at 12:01 am
8 Comments


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Type: Posts; User: Justin87
samething happened to me
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Who do u think is go to win vegas


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Applying design of the master bedroom floor plans will take us on how to maximize the availability of space and other supporting components in order to create a cozy bedroom look. Before applying the design that we want, then enter a number of things into careful planning is essential that we have to do from a design that will ensure that we apply to keep it simple, make sure the amount of funds allocated to us, and ensure the goals we want to achieve with implement the design.
Having established the above things, then the next step we need to do is conduct a search of ideas for bedroom floor plans through a variety of sources ranging from magazines to the Internet. Get copies of the design plans that we want to use an online plans program offered by some sites for free.
When we have established the design that we will apply to the master bedroom, then the next thing we can do is to get the furniture and fixtures. Determine whether we will get a set of furniture for the master bedroom to produce a harmonized tones in decor overall, or whether we will get the furniture separately. If we want to take advantage of the availability of space to the maximum then choose to get a set of furniture will be the perfect solution. Do not forget to measure the room so we did not get in trouble when they want to enter a number into the master bedroom furniture. As for the equipment, then we have to pay attention to some supporters who were able to add items bedrooms look like the type of lighting. We have to make sure to get the right kind of lighting for a bedroom in accordance with the atmosphere we wanted. Taking into account the type of flooring that will be applied in the master bedroom floor plans is the next thing to get our attention. Make sure we choose the type of flooring that can work well with the overall style and were able to give effect to help improve the look of the room.


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Betsy Cain was born in 1949 in Tuscaloosa, and grew up in Fairfield, Alabama. She received both her Bachelor's and Master's of Fine Arts from The University of Alabama, but did formative undergraduate work at Auburn University and Institute Allende, San Miguel de Allende, Mexico.
For the past thirty years she has maintained a studio in Savannah, Georgia, where she lives with her husband, David Kaminsky.


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|Basic info
|Item number
The Webkinz Chipmunk was released in September 2008 and it was retired on May 28th 2009. It does not have a Lil'Kinz version and wasn't Pet of the Month before. Its special item is the Acorn Barbecue, and its special food is Sweet Peanut Pie. There is a virtual Ganz eStore Figurine called the Toy Aviator Chipmunk.
There's nothing quite as sweet as a cheerful Chipmunk! These adorable little rodents are active, energetic and excited to participate in almost any game or challenge! Chipmunks also really love to learn, so visit the Kinzville Academy and Quizzy's!
See AlsoEdit
|Rodents of Webkinz World
Beaver | Chipmunk | Cotton Candy Bunny | Grey Squirrel | Groundhog | Guinea Pig | Lil'Kinz White Mouse | Porcupine | Rabbit | Sherbert Bunny | Skunk | Spring Celebration Bunny | Red velvet raccoon | Sassy skunk | Petal print skunk


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Auto Publishers Price Starting at
*Based on model year EPA mileage ratings. Use for comparison purposes only. Your atual mileage will vary, depending on how you drive and maintain your vehicle, driving conditions, battery pack age/condition (hybrid only) and other factors.VIEW OUR INVENTORY
Acceleration, braking, and handling; serious sports-car attitude; intimate cabin feel; transmission downshift rev-matching; performance value for the money
An all-new 370Z Roadster joins the 370Z Coupe for 2010. With a power-operated soft-top design and intimate cockpit-style interior, the Convertible gets all the performance revisions and upgrades that the 370Z Coupe got last year, when it was completely redesigned. The 370Z Coupe carries into 2010 with no changes, but a new NISMO 370Z performance model--specially tuned for track performance--joins the lineup, with limited availability.


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Goodness me, has the year really gone by or what? To give you guys a quick update, there has been a few changes happening with me lately and I've been taking it easy for awhile. I'm feeling super rundown and my energy levels have been extremely low because I feel like even though my body can recuperate somewhat in response to more sleep, my mind is still racing as soon as I wake and I can't seem to switch off. Don't worry, it's all under control, it just means I need to step back a little bit, so you may find that I'm only active on some platforms for the latter part of the year.
I know a lot of you wait with bated breath for the prompt cycles, and thank you to everyone who has participated in them and have enjoyed them. Here are the July and August Daily and Self-care prompt cycles:
As promised in the previous prompt cycle post, I was going to suggest a few ways you can reflect on your year using the prompts. This part really isn't compulsory, and you can easily do this every quarter of the year, too, or any sort of frequency within the year, just make sure you have at least 3 months worth of responses to work with. This is really just a nice way to dig a bit deeper into your mindful practices:
- Choose from either the Daily prompt cycle list of the Self-care prompts (depending on whether you wrote down after thoughts in the latter prompt cycles)
- Pick a prompt that you've really enjoyed writing about (or doing), or even one that you didn't particularly enjoy
- Go through each month and have a look at your responses for that prompt
- Can you find an underlying thought or theme or message that this prompt might be giving you
- Use this information to make changes in certain parts of your life, or even just pay gratitude for these moments
- Repeat the process across however many prompts you'd like to analyse
- Write down what you've learned from these experiences
- Keep these thoughts somewhere safe so you can return to them during each of your reviews
And it's really that simple. I find that oftentimes when we write a journal or diary, we traditionally don't really look back on the entries quite as often. Sometimes I won't look at entries in my journal until years have passed, and even then I'm having to sift through a whole lot of information to figure out what it is I'm trying to learn of myself. Having the prompts in the prompt cycles gives me a focus. I will usually do a 3-month review and pick 5 prompts that have really appealled to me. This whole process can take as long as you'd like it to, but I usually set aside an hour and a half to really dig deep, and sometimes, the messages I get tell me things that I may have missed, like maybe my anxiety has been creeping back and needs some attention to help me get back on track. Whatever you decide, remember this is for you to learn something of yourself, so be kind.
NOTE: If you're new to the Prompt Cycle concept, go here for an explanation, but please note that I haven't included calendars this year, as people have found them a bit confusing, sooooo I've created printables with each prompt typed out. If you'd prefer the calendar layout, send me an email and I can send that through to you.
Til next time…


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Huawei is being held to an impossible standard
Even so, the company must work harder to build trust.
China's ZTE estimates at least $3.1 bln loss from U.S. sanctions -Bloomberg
The report also said ZTE is hopeful that the United States and China will be able to soon reach a deal that would remove the ban
Google CEO Sundar Pichai poised to cash in $380 million award this week
In 2016, CEOs of S&P 500 companies realized an average of $16.2 million from shares that vested or exercising stock options, according to data compiled by Bloomberg.
Rs 1-lakh iPhone X sold out in minutes
The phones were available online with bank cashback offers, in addition to exchange offers, adding up to a discount of Rs 30,000-35,000. Amazon was also giving 70% buyback guarantee on iPhone X for those using a Reliance Jio connection. Flipkart also had a similar offer of buyback up to Rs 52,000.
View: Two sides to Apple's story in battle to save China sales
Chinese consumers buy iPhones because they're a secure product developed by a company that prides itself on its respect for privacy and putting customers first.
View: India's big brother may be getting a bit too big
In the absence of any legal protections, citizens are left trusting Aadhaar's administrators, a body called the Unique ID Authority of India.
Mukesh Ambani has to double Jio numbers for RIL investors to get a decent harvest
If Ambani can double the number of subscribers, and get at least $4 from each of them, investors who endured seven lean years will get a decent harvest.
Charting the good, the bad and the ugly for the year in technology
The combined market value of tech's Five Fab - Apple, Alphabet, Microsoft, Amazon.com and Facebook - was $2.4 trillion as of December 27.
Apple reboots car project; lays off employees
Apple is rethinking what it plans to do about self-driving cars, just as other big tech companies appear ready to plow ahead with competing efforts.
Yahoo: What went wrong and what will happen next
After 16 years of stagnating business and poor investments, Yahoo's end was inevitable
Dalal street cuts bullish calls on telecom stocks
68% of analysts tracking Bharti Airtel, the country's largest telecom operator, have a 'buy' call on the stock; that's two out of every three analysts.
Telecoms giant MTN pays USD 250 mn in Nigeria fine dispute
The company also said it had agreed to withdraw its legal challenge over the huge fine in a case that was adjourned in Lagos High Court to enable the two parties to try to negotiate a settlement.
IT and ITeS firms emerge biggest office occupiers in 2015
Tata Consultancy Services, India's biggest software exporter, overtook consultancy firm Deloitte in 2015 as the largest office space occupier.
Awards for the most fascinating stories of 2015
Here are the awards for the most fascinating stories of 2015, with the added bonus that the qualifying events have implications that will reverberate into 2016 and beyond.
India's top 5 IT firms like TCS, Infosys, Wipro, HCL & Tech Mahindra may see single-digit revenue growth in FY16
Slowest pace since the global financial meltdown following the 2008 Lehman Brothers crisis on lower tech spend, currency impact and Chennai floods.
Best IIT-Madras geeks get midnight call from Google, Microsoft
A midnight talent hunt by some of the largest technology corporations including Google & Microsoft yielded high-profile jobs for 6 undergraduates at IIT-Madras.
Satya Nadella has an 8-hour meeting with his leadership team every month
The Microsoft CEO has been known to tell employees to skip pointless meetings that waste their time.
Facebook's mobile ad revenue soars to $2.9 billion
Many digital media companies have seen their ad revenues decline as their audiences have shifted to smaller screens. Not Facebook.
Chinese tastes decide iPhone colours: Tim Cook
Apple CEO Tim Cook has said in an interview that the gold iPhone was introduced to please the Chinese customers.
At $135 mn, SoftBank's Nikesh Arora third highest paid Chief
Fisher, 67, president and founder of SoftBank Holdings Inc., helped lead Son's campaign in the US, including the Sprint acquisition.


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Making of Meringue Cookies
Meringue cookies, light and airy and you can make them colorful too very easily. Try these very easy to make cookies at home and let us know how you like them.
4 egg whites
1 cup sugar
1. Put 4 egg whites and 1 cup sugar in a bowl and put it over a boiler or a pot of
simmering water (water should not touch the bowl on top)
2.Start beating them together. After 3 minutues, take the bowl away from heat and start beating again.
3. Continue beating for about 7 minutes until the mix is glossy and the stiff peak forms. You will know it is ready
when the mix does not fall out even after turning the bowl upside down.
4. Add a teaspoon of lemon juice (this is optional).
5. If you want the colored swirl, brush some gel color inside the pastry bag. Fill it with meringue and pipe
on a try lined with perchmant paper with any nozzle tip you want. We used star tip.
6. Bake in a preheated oven (200 degree celcius) for about 75 to 90 minutes.


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THE Geek Fest 2018
Thursday, November 8, 2018
9 am - 1 pm
@CPCC Levine Campus
Building Blocks @ LV 2150
11:20 a.m. — 11:59 a.m.
Blockchain will change the world - visibly and invisibly. But what the heck is it? Come hear fascinating predictions and hard realities about the most important innovation in transactions of the last millenia. Maybe you could learn enough to be entertaining at parties?


text: Fruganism is a division of Vegetarianism. This word is derived from the word "Frugan" which, itself, is elicited from the combination of Frugivore and Vegan. Although the moral criteria of the fruganism is very similar to veganism, there is a main basic difference between these two, since fruganism respects animal life as well as plant life.


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Last month the Australian General Manager for Stampin' Up!, Dave Abbott, passed away from a rare blood disease. This is made particularly sad by the fact that Dave leaves behind a wife & 3 young children (you can see thier picture in the scrap page below)
Because Stampin' Up! is such a caring company & want to not only honour Daves memory, but also help his family, they have pre-released a special All In The Family stamp set. During November Stampin' Up! are donating 100% of the sales worldwide to a fund set up for Daves family. Click here for more details.
This 28 piece set will retail for $73.95, but during Nov I will be passing my demonstrator discount on to you, so it will only cost $59.16 plus postage. Please support this worthwhile cause, you will not only receive a fantastic stamp set, but be helping a grieving young family. If you would like to help, but don't wish to purchase the stamp set , you can contribute directly to the fund - email me for details firstname.lastname@example.com.
Whether for business or pleasure, contact me today to learn how becoming a Stampin' Up! Demonstrator can benefit you!
Thursday, 1 November 2007
Dave Abbott Family Fund
Posted by Alana Galagher at 2:09 pm
Labels: Specials and Promotions, Stampin' Up
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