Gassendi 1967 Jan 21 UT 19:36-20:24 Observed initially by
Moore & Moseley (Armagh, N.Ireland, 10" refractor, x360, S=G),
Ringsdore (England, 10" reflector), Sartory (Farnham, England,
15" reflector?), Duckworth (England), Kilburn (Ashton,
England, 6" reflector), Farrant (England, 8" reflector) "Eng.
moon blink at 1936 (no events from 1750-1815h) outside SE
wall, brighter at 1939h, seen vis. at 1940h, faint at 1946h.
Moved NW at 1950h. At 2000h, Moseley saw it farther W., lost
it at 2008h. Seen again at 2026h further toward group of
hills. Moore saw it faint at 2002h, lost it at 2005h, vis. &
blink at 2007h. Checks again at 2010-50h, 2130-50, 2200-20,
2250-2300, 2325-0000h.Duckworth suspected blink in S.Iridium
nr. Bianchini later, but clouds intervened, after clearing
couldn't see it. Neg. obs. in 11 other features, inc.
Alphonsus & Plato. Confirmed Gass blink 2018-2024h" NASA
catalog weight=5. NASA catalog ID #1010. ALPO/BAA weight=4.
Alphonsus 1969 Nov 20 05:27 (UT)? Observed by Argus/Astronet (San
Diego, Sacramento, CA, USA) "Brightening in crater. (San Diego &
Sacramento obs. confirmed, but astronauts did not see anything. Apollo
12 watch)." NASA catalog weight=3 (average). NASA catalog ID #1222.
Gassendi 1971 Oct 29 UT 22:15-22:50 observed by J.Coates and
A.R. Neville (Burnley, UK, 6" reflectir, x192, slight fog,
seeing jumpy but good at times). An in ititial Moonblink
search proved negative. However white light observations by
Coates revealed a golden brown colour between the black
interior shadow and the base of the (bright W (IAU?) wall).
Neville confirmed its appearance as a coppery hue and saw the
colour for 5 minutes before it vanished at 22:55UT. ALPO/BAA
weight=2
On 1990 Sep 30 at D. Darling (Sun Praire, WI, USA, 12.5"
reflector, x150) observed a red spot on the west wall (bright
in red filter and faint in the blue filter. No filter
reactions were found elsewhere. Gassendi had much detail
visible. A sketch was made. BAA observers in the UK were
alerted but they could not observe due to cloud. Cameron
2006 extension catalog ID=411 and weight=5. ALPO/BAA weight=3.
Plato 1966 Dec 23 UT 06:15-07:10 Observed by Kelsey (Riverside, CA,
USA, 6" reflector, S=P, T=G) and Coralitos Observatory (Organ Pass, NM,
USA, 24" reflector +Moonblink) "3 brilliant spots on floor, all showed
blinks, (permanent colored Ground features ?). Not confirmed by
Corralitos MB." NASA catalog weight=2 (low). NASA catalog ID #1005.
In 1820 Oct 17 at UT 20:00 an unkown observer reported in Mare Imbrium,
south of Sinus Iridum (30W, 40N) some brilliant spots. The Cameron 1978
catalog ID=80 and weight=1. The ALPO/BAA weight=1.
Gassendi 1977 May 28/29 UT 20:45-21:15 Observed by D. Sims
(Dawlish, Devon, UK) saw a hazy area on the south east floor
that was normal in red and white light but darker in blue.
This was partly confirmed by J-H Robinson (Devon, England, 10"
reflector) 21:24-23:12 who saw the south east floor of
Gassendi to have a loss of detail - but no colour seen,
although at 21:57-21:58 it was slightly brighter in red than
in blue briefly. P. Doherty (22:45-23:15) did not see anything
ususual. D. Jewitt (22:22-22:55) did not reveal anything
ususual, apart from spurious colour. The Cameron 1978 catalog
ID=3 and ID=1463. The ALPO/BAA weight=3.
Aristarchus, Schroter's Valley, Herodotus 1881 Aug 06 UT 00:00?
Observed by Klein (Cologne, Germany, 6" refractor, 5" reflector)
"Whole region between these features appeared in strong violet
light as if covered by a fog spreading further on 7th. Examined
others around & none showed effect. Intensity not altered if
Aris. placed out of view." NASA catalog weight=4 (high). NASA
catalog ID #224. ALPO/BAA weight=3.
Plato 1982 Jun 02 UT 22:00. Mobberley could not see the
central craterlet on the floor of Plato tonight. Foley notes
that he could only just see the central craterlet on nights of
2-5th Jun and it was of reduced in brightness from normal.
North reported that the floor seemed nearly black, but
brighter in a green filter (x144 magnification used). All
three observers compared the Plato area to other areas for
reference. All the above seems normal, apart from the floor
being brighter in the green filter. Cameron 2006 extension
catalog ID 170 and weight=5. BAA/ALPO weight=1.
On 1985 Mar 02 at 20:00UT? Marshall (Medeline, Colombia, South America)
measured some very low Crater Extinction Device brightness readings of
Censorinus compared to Proclus. The Cameron 2006 catalog extension ID=
261 and the weight=3. ALPO/BAA weight=2.
Brilliant blue color seen at first for seconds, later for min
2h later, in blue filter. Cameron 1978 catalog weight=4 (high).
Cameron 1978 catalog ID 572.
Schroter's Valley 1955 Aug 29 UT 19:45 Observed by Firsoff (Somerset,
England, 6.5" reflector x200, S=P-F) "Valley almost completely
invisible in blue" NASA catalog weight=4 (high). NASA catalog ID #605.
Herodotus 1957 Sep 05 UT 02:55-03:24 Observed by Bartlett
(Baltimore, MD, USA, 5" reflector x180, S=1-5, T=5) Pseudo
peak visible within floor shadow at 03:10h" NASA catalog
weight=4. NASA catalog ID #671. ALPO/BAA weight=3.
Proclus 1970 Oct 12 UT 00:54 Observed by Bartlett (Baltimore, MD, USA,
4" reflector, 51x-181x) "Floor darkened to intensity 1.5 deg (albedo) &
c.p. became invis. Next day c.p. reappared & was 5 deg bright & 6deg
bright on 15th" NASA catalog weight=4 (high). NASA catalog ID #1277.
Schickard 1972 Sep 19 UT 19:45-20:25, 20:00-23:30 Observed by Watkins
(Herts., Eng. 4.5" reflector, x225, S=G) Amery (Reading, Eng.m 12"
reflector?), Fitton (Lancashire, Emg., 8.5" reflector) and Moore
(Selsey, Eng., 12.5" reflector?, 4.5" refractor 45-225x, S=P)
"Luminous, nebulous spot attracted Watkin's att'n. Got brighter.
Checked 'scope--not instru. Obj. had greenish-gray color, size @ 15km.
Amery & Fitton with blink devices noted nothing unusual at later times
(2000-2330h). Aris., Plato, Gass. were neg. at 1930-2025h (date not
given, guessed at fr. available info.). Turbulence, lasting
secs. at a time." NASA catalog weight=2. NASA catalog ID #
1344. ALPO/BAA weight=2.
Aristarchus 1976 Sep 05/06 UT 18:45-01:35 Observed by Prout
(England?, 12" reflector, S=III-II), Foley (England, 12"
reflector), Moore and Spry (Sussex, England, 12" reflector)
"Viol. hue on crater on W. wall, especially NW corner seen by
Prout & 2 Foleys. Moore & Spry did not see color. All obs. noted
that the crater was dull Hobdell, of St Petersburg, FL, USA, using a 2"? refractor?
and Seeing=I-II, saw a bright region on the north west wall
that seemed to change in brightness. In truth, there were
other features elsewhere on the Moon that also fluctuated,
but not as much as Aristarchus was. No colour was noticed.
Cameron suspects fluctuations in our own atmosphere.
Cameron 2006 extension catalog ID 131 and weight=1. ALPO/BAA
weight=1.
On 1990 Oct 1st at 00:44-01:24UT D Darling (Sun Praire, WI, USA)
observed that Gassendi still had a blink effect when viewed through
blue (Wratten 38A) and red (Wratten 25A) filters. No effect was seen on
Aristarchus. Gassendi was brighter in the red filter and this was
confirmed by Weier. Sketches were made and brightness measurements
taken. Both observers used a 12.5" reflector x159. At 01:00UT the NW
wall was 7.5, the SW wall 8.0, the S. wall 7.5, the floor 6.0, the
outer E. wall 8.0, the N. floor 5.5. Gassendi A W. wall was 9.5,l
Aristarchus W. floor was 8.0, NW wall 8.0, shadowed floor 0.0, E. outer
wall 7.0, NBP 5.5, area between Aristarchus and Herodotus 6.0, and the
comet like tail: 8.2 on the E. and 8.5 on the W. The Cameron 2006
catalog extension TLP ID=412 and weight=5. The ALPO/BAA weight=4.
On 2002 Feb 24 UT 05:15-05:35 W. Haas (Las Cruces, NM, USA) observed an
obscuration in Herodotus - the shadown was, almost, but not
completely black. ALPO/BAA weight=2.
On 2002 Feb 24 UT 06:05-06:20 W. Haas (Las Cruces, NM, USA) observed
that the shadow was, almost, but not completely black. This might have
been related to the observing conditions.
ALPO/BAA weight=2.
On 1933 Oct 01 at UT 03:00 Rawstron (USA, 4" refractor, x330) observed
the following in Mons Pico B: "Haze -- much narrower & elongated than
on Sep. 1". The Cameron 1978 catalog ID=407 and weight=3. The ALPO/BAA
weight=2.
On 1955 Oct 28 at UT00:00? Kozyrev (Crimea, Soviet Union, 50"
reflector) detected in Aristarchus Fraunhofer lines in UV spectra that
were much narrower than in the solar spectrum. This indicated
luminescent glow which overlapped contour(?) lines. Greatest after Full
Moon, but fluctuated monthly with no indication of solar activity
effect. The Cameron 1978 catalog ID=621 and the weight=5. The ALPO/BAA
weight=5.
On 1955 Oct 28 at UT 00:06 W. Taylor saw a naked eye flash on the Moon
in the north east area, on the edge of Mare Vaporum. The flash was
intense and radiated to a large area. The duration was 1/4 seconds.
Observed by Haas (Las Cruces, NM, USA) "Temporary greyness seen in
interior shadow." ALPO/BAA weight=3.
Aristarchus, Schroter's Valley, Herodotus 1881 Aug 07 UT 00:00?
Observed by Klein (Cologne, Germany, 6" refractor, 5" reflector) "Whole
region between these features appeared in strong violet light as if
covered by a fog spreading further on 7th. Examined others around &
none showed effect. Intensity not altered if Aris. placed out of
view." NASA catalog weight=4 (high). NASA catalog ID #224.
Aristarchus 1981 Mar 17 UT 22:40-23:25 Observed by Moore
(Selsey, England, 15" reflector, seeing III) "Aristarchus very
bright according to Crater Extinction Device and a coloured
blink detected" BAA Lunar Section TLP report. ALPO/BAA
weight=1.
On 2016 Jun 17 UT 05:00 A.Anunziato (AEA, Argentina Meade ETX
105, seeing 7/10, sketch made) observed a very tiny light spot
where the shadow from topographic relief to the south of
Vallis Schroteri nerges into the crater rim shadow on the
floor of Herodotus. There should be no light spot here.
ALPO/BAA weight=1.
Aristarchus Area 2004 Nov 22 UT 04:58-05:49 Observed by Gray
(Winemucca, NV, USA, 152mm f/9 refractor, seeing 4-5, trasparency 4-5,
x114, x228) "Blinked Herodotus with Wratten filters Blue 38A and Red
25. The illuminated west crater wall stood out brilliantly in blue
light, much more so than in white light. This was true also of
Aristarchus. Red light did not increase contrasts in Herodotus any more
than they were in white light. Shadows in Herodotus appeared as black
as the night west of the terminator and remained that way throughout
the observing period. No TLP seen in Herodotus tonight. A possible TLP
was seen to the west of Herodotus near the terminus of Schroters
Valley. It was noted at the beginning of the observing period that
there were four very bright spots of light, one near the end of
Schroters Valley, the other three grouped together a little farther
north. Although not far from the terminator they were definitely east
of it. It was noted that all of them nearly vanished in the Blue 38A
filter while Aristarchus and the rim of Herodotus gleamed brilliantly.
At 5:19UT it was noted that the most brilliant of the four lights, the
one near the terminus of Schroters Valley, had faded almost to
invisibility in white light. When first seen it had been brighter than
Aristarchus. It remained very dim after this through the remainder of
the observing period, and was unchanged at 7:35-7:49UT when I again
examined the area. The other three bright spots remained brilliant and
unchanged."
Aristarchus 1973 Aug 10 UTC 20:14 observed by Baumeister
(48.63N, 9.25E, 110mm reflector, T=2, S=2) "Orange to red
colours at the crater floor disappeared until 21:04" -
Hilbrecht and Kuveler, Earth, Moon & Planets, 30 (1984),
p53-61. ALPO/BAA weight=2.
Plato 1973 Aug 10 UT 22:45 observed by Robinson (Devon, UK).
Observer noticed that the lighter areas on the floor were more
distinct in red than in the blue filter. ALPO/BAA weight=1.
All observers saw a blue tinge seen inside and outside the
crater. Marshall observed a bright spot in the middle of
the crater floor and thought perhaps that it was a central
peak. No central peak can be found on Lunar Orbiter images.
Cameron 2006 Catalog extension ID=214 and weight=5. ALPO/BAA
weight=4.
Proclus 1976 Sep 06 UT 02:00 Observed by Bartlett (Baltimore, MD, USA,
4.5" reflector 45-300x, S=3, T=5) "Nothing vis. on floor of 2deg
brightness. Usually floor ray & Proc. A are vis. at this col. & c.p. is
5 deg bright. (must have been 2 deg tonite)." NASA catalog weight=4.
NASA catalog ID #1450.
Ross D 1965 Apr 14 UT 06:03-06:22 Observed by Harris (Whittier?, CA?,
USA, 19"? reflector) "Phenomenon description unavailable. Given at an
ALPO meeting" NASA catalog weight=0 (very unreliable). NASA catalog ID
#874.
Babbage 1974 Sep 29 UT 00:00-01:00 Observed by Lord (St Annes-
on-Sea, UK, 10" refractor, Wratten 25 and 44a filters, 125x,
S=II-III). Activity observed in SW floor between A & W. wall.
Details not obscured in either filter, but slightly more
darker than surroundings in the blue filter. NASA catalog
weight=2. NASA catalog ID #1395. ALPO/BAA weight=2.
On 1990 Oct 02 at 02:25-02:45UT D. Darling (Sun Praire, WI, USA using a
12.5" reflector at x159, with red and blue filters), saw a blink
effect on the west wall of Plato i.e. brighter through a blue filter
than through the red. No Colour blinks seen on Gassendi or Aristarchus.
Cameron 2006 Catalog TLP=413 and weight=4.
On 1977 May 30 at 21:04-02:13UT J.H.-Robinson noted a loss of
detail inside Gassendi, however he did not regard this as a
TLP. The effect was also seen by P.W. Foley. Cameron 2006
extension catalog TLP ID=16 and weight=0 ALPO/BAA weight=1.
Schroter's Valley 1897 Oct 08 UT 22:00 Observed by Pickering
(Cambridge, Maas., USA, 15"? refractor) "Variations in vapor col.
Tillsow, C was largest compared with D&E& most conspicuous 1.3 d after
sunrise. Drawing. (time est. fr. given colon.)" NASA catalog weight=3
(average). NASA catalog ID #291.
On 1988 Jan 02 at 05:57-06:13 UT D. Louderback (South Bend, WA, USA,
using a 8" reflector, seeing 4 out of 10) observed that points B and D
on Cape Agarum faded suddenly from 7.0 to 6.4 (B) and 6.0 (D). However
these returned to their normal levels at 06:13 UT. Cameron 2006
extension catalog ID=316 and weight=4. ALPO/BAA weight=3.
On 1984 Feb 14 P. Moore (Selsey, UK) thought that there was something
odd about Mons Pico in that it looked very bright and gave a good
impression of a crater. Cameron 2006 catalog extension ID=241 and
weight=5. ALPO/BAA weight=2.
On 1984 Feb 14 P. Moore (Selsey, UK) observed that Plato was darker
than the nearby mare and no detail could be seen on the floor or the
eastern wall - the later was obscured. At 23:40UT some dimming was
still present on the north east wall and still no detail on the floor
of Plato. Cook noticed that the eastern floor close to the wall was
misty and also noted no detail on the floor. Amery though noted that
all parts of the floor were sharp although some darkening was visible
in the north west and a hint of obscurtion. The east wall though was
quite sharp. Mosely could see the central craterlet but from 8-6
o'clock tricky to define (Foley says that this effect has been seen at
this colongitude before). Streak ray across the floor of Plato seen
(North) - filter measurements made. Cameron 2006 catalog extension ID=
241 and weight=5. ALPO/BAA weight=2.
On 1988 Jan 02 at 06:41-07:08 UT D. Louderback (South Bend, WA, USA,
using a 8" reflector, seeing 4 out of 10) observed that at 06:56 UT
Aristarchus floor (point F) brightened rapidly from an intensity of 5.2
to 6, however at 07:08 UT the spot returned to normal. He also noticed
that the bands on the walls varied every few minutes. A mist like
appearance was seen on the floor of Aristarchus. Through a red filter
he could see through the haze, but floor detail could not be seen
through a blue filter. Cameron 2006 extension catalog ID=316 and
weight=4. ALPO/BAA weight=3.
Vallis Schroteri 1991 Aug 23 UT 02:19-02:49. Flashing spot at
end of SV fluctuated. Herzog, Darling & Weier confirmed spot
but not fluctuation. Spot brighter in red than blue, but Cobra
Head was bright in blue. No other region was abnormal.
On 1980 Apr 28, Louderback (South Bend, WA, USA using a 8" reflector
and a 2.5" refractor) observed a very bright reg region on top of the
south west rim of Aristarchus crater. This was on the same side as the
ray system between Aristarchus and Herodotus. Louderback noticed some
chromatic aberation - blue where he had seen the red patch before.
Louderback suspects chromatic aberation was the cause although did not
see red in that region ever again. "Patch was between his observation
points A and C. Point C was 5 points brighter in the red filter than in
the blue." A sketch was made. Cameron suspects that the TLP was real.
Cameron 2006 TLP catalog extension ID=92 and weight=3. ALPO/BAA
weight=2.
On 1821 Jan 16 at UT 21:00 S. Cooke (Stonehouse, UK) An
effusion of smoke effect, which lasted about a minute, seen.
It appeared like the fluttering of a bird and passed over the
Moon before it evaporated, and must have been foreshortened,
as it seemed in effect to have passed over the whole disc,
starting from west of Menelaus, and near Plinius. ALPO/BAA
weight=1.
Peter Foley (Kent, UK, 8" reflector, seeing=II) noticed that
the floor beneath the north wall, and the area over the north
wall were indistinct (almost out of focus). Despite looking
elsewhere in the crater and surrounds, no other blurring
(obscuration of detail) could be seen, indeed everywhere else
was sharp and detailed. Foley tried several eyepieces but this
made no difference. He used a crater extinction device but
found no variations in brightness. There was a slight
darkening when he used a red filter in the Moon Blink device.
The obscuration effect weakened between UT20:56 and 21:10,
was difficult to see at 21:13 and had finished by 00:15.
Patrick Moore (12" reflector, Dublin, Ireland) saw nothing
unusual when he started observing at UT 22:00. Cameron says
"Photos marked at location of phenomenon". Cameron 2006
extension catalog ID=37 and weight=5. ALPO/BAA weight=3.
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.
Mare Humboldtianum 1951 Jan 21 20:47-22:00 UT observed by Baum
(Chester, England). The appearance of some mountains on the
limb appeared to change over time, with some mistiness. ALPO/BAA
weight=2.
Schickard 1940 May 20 UT 20:00 Observed by Moore (England, 12?"
eflector) "Fog on floor -- milky appearance, less pronounced
than on 8/2/39 (see #456)." NASA catalog ID #465. NASA catalog
weight=4. ALPO/BAA weight=2.
Plato 1971 Jan 10 UTC 20:17-20:42 Observed by Taylor (Slough, England,
8.5" reflector) "Blink (dark gray to black), 13x3km diam. on E. wall &
floor in indentation in wall. Smaller by 2028 h. gone at 2035h.
Reappeared at 2028h & gone completely at 2042h)." NASA catalog weight=3
(average). NASA catalog ID #1282.
Madler 1940 Aug 17 UT 06:45 (Cameron gives 07:30 but Haas says
this is wrong) Observed by Haas (New Mexico?, USA, 12"
reflector?) Bright spot on S. rim had I=5.8 on this date but
8.9 on Aug. 17, when observing conditions were similar (see #
473). NASA catalog weight=4. NASA catalog ID #470.
ALPO/BAA weight=3.
Aristarchus 1989 Oct 13 UTC 21:00 Observed by Cook (Frimley, Surrey,
UK, 20cm reflector (visual and video)) "Aristarchus had what appeared
to be a outline of a ghost crater on it's eastern side - quite large
and bright". Cameron 2006 extended catalog TLP ID No=378 and weight=5.
ALPO/BAA weight=4.
Plato 1937 Jul 22 UT 06:20 Observed by Haas (Alliance, Ohio,
USA, 12" reflector?) "Floor distinctly greenish, but was gray on
June 23, 1937 at 0430 & col.84 (normal?)" NASA catalog weight=4
(high). NASA catalog ID #421. ALPO/BAA weight=3.
Plato 1916 Oct 10 UT 21:00? Observed by M, Maggeni (Florence
Obs., Italy) "Reddish shadow spread over part of crater. Looked like
vapor (like nitrous vapor) and obscured underlying craters. The Cameron
1978 catalog weight=3 and ID = 365. The ALPO/BAA weight=3.
Aristarchus. 2024 Feb 23 UT 19:22. A.Conway (Bootle, UK - 20cm
Newtonian (dobsonian), 9mm Plossl eyepiece, Samsung A33 mobile
phone camera, 36 sec AVI file at 30fps, seeing probably
average-good). Noticed a blue tinge on northern rim of the
crater. This is probably normal, but we are flagging this up
as a weight 1 TLP, in order to obtain some repeat illumination
observations and confirm that the strength of the blueness is
normal.
Plato 1878 Nov 09 UTC 21:00 UTC Observed by Klein (Cologne, Germany,
6" refractor?) "Faint, but unmistakable white cloud not seen before."
NASA catalog weight=4. NASA catalog ID #207.
On 1989 Oct 14 UT 19:00?, 22:00? P.W. Foley (Kent, U.K., using a 12"
reflector) noted that although the brightness of Aristarchus crater
seemed steady, that there was just too much detil to see inside the
crater than one would expect. Appeared as two craters - Cameron
commented that this was often seen by Bartlett. Several observers
apparently confirmed this TLP? Cameron 1978 catalog extension ID=379
and weight=5. ALPO/BAA weight=2.
Aristarchus 1973 Feb 15 UTC 17:07-19:31 Observed by Theiss (located at
51N 5.67E) "area 4-5 diameters of Aristarchus were coloured clearly
yellow-red" 120mm reflector used. Ref Hilbrecht & Kuveler (1984) Moon
and Planets Vol 30 p53-61. ALPO/BAA weight=1.
Plato 1973 Aug 13 UT 22:25-22:35 observed by Pedler (Devon, UK).
Observer noticed a slight blink on a lighter patch on the floor
just beneath the south(?) rim using Moon blink filters.
ALPO/BAA weight=1.
David Darling observed bright glittering on Aristarchus. This
was followed by a flare up in brightness at 00:38:05 UT in the
comet-like ray area of the crater equivalent in intensity to the
central peak. Then he saw another one on the north east rim of
Aristarchus of the same brightness. A third flare was seen at
00:49UT in south of Herodotus, on the comet-like ray. Another
two flares were observed at 00:56UT on the north west rim of
Aristarchus. Darling suspects that these effects were due
to seeing effects and Cameron agrees. However Weier suspects
that they were TLP? Brightness measurements by Weier were for
the south west rim of Herodotus 8.0, for a spot at the Cobra's
Head 9.0 and 7.5 for C.H. Cameron apparently did not see the flashes
but did suspect that the interior of Aristarchus was a bit unusual.
Don Spain did not see anything unsual at all. Cameron 2006 extended
catalog ID=380 and the observation weight=3. The ALPO/BAA weight=2.
Aristarchus 1962 May 20 UTC 08:00? Observed by Wildey, Pohn (Mt Wilson,
CA ?, 60" reflector? Photometer) "Reddish color in Aris. 0.88
magnitudes brighter than normal (photometry)." NASA catalog weight=5
(very good). NASA catalog ID #758. ALPO/BAA weight=3.
Bullialdus 1962 May 20 UTC 08:00? Observed by Wildey, Pohn (Mt Wilson,
CA ?, 60" reflector? Photometer) "1.05 magnitudes brighter than normal
(photometry)." NASA catalog weight=5 (very good). NASA catalog ID #758.
ALPO/BAA weight=2.
Kepler 1962 May 20 UTC 08:00? Observed by Wildey, Pohn (Mt Wilson, CA
?, 60" reflector? Photometer) "1.03 magnitudes brighter than normal
(photometry)." NASA catalog weight=5 (very good). NASA catalog ID #758.
Enhancement of spectrum in UV and CaI recorded on photoelectric
spectrometer scans by Grainger and Ring in Italy. Effect seen on
Aristarchus. Cameron 1978 catalog ID=740 and weight=5. ALPO/BAA
weight=5.
Proclus 1955 Nov 01 UTC 02:50-03:05 Observed by Bartlett (Baltimore,
MD, USA, 3.5" reflector x100, S=6, T=5) "Proc. D normally 5 deg bright
was vis. tonite only in blue light, whereas usually is vis. in
integrated light. However at col. 110.5 deg it was a dark spot (see #
816) C.p. tonite was normal 5 deg bright but in Oct. lun. was dark".
NASA catalog weight=4 (good). NASA catalog ID #625. Note Proclus D does
not refer to the crater Proclus D as defined by the IAU, but probably
to a spot inside the crater that Bartlett designated D!
On 1970 Nov 14 UT20:10 J.Coates (Burnley Astromical Society,
8.5" reflector, x102 and x204) saw a dirty green colour on the
NW region of the crater, in patches, with a green area nearby.
ALPO/BAA weight=1.
1969Jan04 UT19:30-20:00 W.Deane (Hendon, UK, 2" refractor)
observed a bright yellow spot just E of Aristarchus, stretching
from the S. end of Montes Harbinger to the S. wall of Prinz. The
ALPO/BAA weight=1. ALPO/BAA weight=1.
In 1955 Sep 07 at UT 03:45-05:20 Bartlett (Baltimore, MD, USA, S=5, T=
3) observed the following in Aristarchus crater: "Strong blue-viol. gl.
in E, NE rim & E. base of c.p. Dark viol. nimbus, granular aspect of
floor". Cameron suggests that this is confirmation of Firsoff's TLP of
the same day? The Cameron 1978 catalog ID=609 and weight=5. The
ALPO/BAA weight=2.
Copernicus 1955 Sep 07 UT 03:20 Observed by Firsoff (Somerset, England,
6.5" reflector x200, S=VG) "Brightening up of crater in the blue
filter" NASA catalog weight=4 (high). NASA catalog ID #607.
Eratosthenes 1976 Sep 14 UTC 04:24 Observed by Bartlett (Baltimore, MD,
USA, 4.5" reflector, 45-300x, S=6, T=3 hazy) "Pseudo shadow F
disappeared & wall here is same intensity as whole inner crater wall, =
4deg. No change in X, X3 or X2 (4 deg much brighter than normal)." NASA
catalog weight=4 (good). Cameron c1978 atalog ID=1453 and weight=4. The
ALPO/BAA weight=2.
Observations made with a variable polarizer (akin to a crater
extinction device) to measure brighness with red and blue filters.
Some variability in brightness noted. With the Kodak Wratten
25 and 38A filters there was little or no increase in contrast with the
red filter, but with the blue filter there was a great increase in
contrast of the brighter areas of the crater - the crater floor and
patches of lighter material, especially at the north end. The remaining
areas were supressed with the Blue 38A. ALPO/BAA weight=3.
Copernicus 1939 Jul 09 UT 05:00 Observed by Haas? (NM?, USA, 12"
reflector?) "Dark area at foot of N. inner wall was I=1.8. Comp. with
I=4.8 on 9/6/39 (see #460)" NASA catalog weight=4 (high). NASA catalog
ID #451.
UT 08:30 or UT 20:30? SW inner wall of Aristarchus was intesnsity
I=0.5, but was I=2.5 on July 2 at Col. 195. Observing conditions were
identical. Band is darkening near col. 180. (Observation made in
daylight?). Cameron 1978 NASA catalog ID=425 and weight=4
(very experienced observer). ALPO/BAA weight=1.
Riccioli 1937 Sep 29 UT 09:10 Observed by Haas (Alliance, OH
USA, 12?" reflector) "Vivid deep purple (Deep purple color on
the previous day), but on July 2, 1937 at col. 195deg it was
gray tinged with brownish purple. Obs. conditions similar on
all." NASA catalog weight=4. NASA catalog ID #426. ALPO/BAA
weight=3.
Aristarchus 1973 Aug 22 UT 00:22-00:23 Observed by Germann (Observer at
47.3N, 8.9E, 200mm reflector, S=2, T=2) "Well Observed bright point
disappeared within a minute". - Hilbrecht and Kuveler, Earth, Moon &
Planets, 30 (1984), p53-61
Tycho 1991 Sep 02 UT 07:34-08:40 Observed by Darling (Sun Praire, WI,
USA, 12.5" f/5 Newtonian, 159-248x with red and green filters) "Central
peak appeared initially star-like with occasional glimpses of a
nebulous patch. At 07:54 an arch of light seen inside the crater.
Various starlike or blurriness states seen to the central peak. The
luminescence seen was brighter in the red filter than in the blue." An
ALPO report - for further details see:
http://www.ltpresearch.org/ltpreports/ltp19910902.htm
Riccioli 1937 Sep 29 UT 09:10 Observed by Haas (Alliance, OH USA, 12?"
reflector) "Vivid deep purple (Deep purple color on the previous day),
but on July 2, 1937 at col. 195deg it was gray tinged with brownish
purple. Pbs. conditions similar on all." NASA catalog
weight=4 (high). NASA catalog ID #426. ALPO/BAA weight=3.
Aristarchus 1787 Oct 07 UT 03:00? Observed by Schroter (Lileinthal,
Germany). Cameron 1978 catalog weight=1 (very low). Cameron 1978
catalog ID=36. ALPO/BAA catalog weight=1.
On 1788 Aug 27 at UT00:00 Schroter (Lillienthal, Germany) reported a
TLP. The Cameron 1978 catalog does not give the geographical location
of the TLP. The Cameron catalog ID=49 and the weight=1. the ALPO/BAA
weight=1.
On 1983 Feb 08 at 06:30UT Toricelli B was observed by P.W. Foley (Kent,
UK, 12" reflector) to be visible in Earthshine as a luminous patch.
This was rather odd because it is only a small crater and not normally
bright. The Cameron 2006 catalog extension ID=201 and the weight=2. The
ALPO/BAA weight=2.
In 1824 Oct 18 at UT 05:00 Gruihuisen (Munich, Germany) observe
near Aristarchus a mingling of all kinds of colours in small
spots North west of the crater. Cameron suggest the wrong date
and suggests seeing her TLP ID No, 121). The Cameron 1978
catalog ID=101 and the weight=4. The ALPO/BAA weight=3.
On 1968 Dec 22 at UT 23:00 Ivan Mourilhe Silva (Rio de Janeiro,
Brazil, 8.5" refractor) observed a light inside Aristarchus
crater. This was during the Apollo 8 watch. The Cameron 1978
catalog ID=1107 and weight=2. The ALPO/BAA weight=1.
1980 May 17 at 21:00UT P.W. Foley (Kent, UK, using a 12" reflector)
observed that Aristarchus was dull on the Earthlit side of the Moon.
This was odd because other features were clerly seen. Cameron 2006
catalog extension ID=94 and weight=1. ALPO/BAA weight=2.
On 1983 Apr 16 at UT 02:00-03:00 W. Haas (Las Cruces, NM, USA) observed
a bright phosphorescent, gray-green (like a "tritium lighted LCD
watch", albeit much brighter) spot in the vicinity of Aristotles (16E,
45N) or Eudoxus (17E, 50N) craters. This was seen in Earthshine. The
Cameron 2006 catalog ID=211 and the weight=2. The ALPO/BAA weight=3.
On 1957 Jul 31 UT 02:24 C. Johnson (4" reflector, x91, seeing 10/10)
observed a slight ring of light reaching around the north limb of the
Moon. The ring was only just brighter than Earthshine and about 1600km
long. The Moon's age was 3.9 days. The reference for this comes from;
Johnson, Craig, L. "Lunar Limb Brightening", Strolling Astronomer,
11:118, 1957.
On 1980 May 18 at UT 20:10-22:35 J.D. Greenwood (Morecombe, UK, 10"
reflector and 3" refractor, seeing II-III, conditions very good) noted
that the inside of Aristarchus had a star-like point contained within a
diffuse blue-green hue coloured glow. There were also intermittent
flashes visible during short irregular periods using a Wratten 44a
(blue-green filter)but were difficult to see trhough a Wratten 25 (red)
filter. The Moon was at a low altitude and the observation ceased at
22:25UT. P.W. Foley (Hent, UK, seeing II) observed flashes in
Aristarchus and occasional star-like points - he also observed the area
to be in a bluish translucent glow extending for about 40 miles all
around the crater. In order to check on the visibility of Earthshine, a
region of highland, near Grimaldi was checked and found to be 0.2
bright with no variations. However Aristarchus itself varied from a CED
freading of 0.6 to unmeasurable. Foley observed from 20:10-22:30UT. P.
Madej (Huddersfield, UK, 77m refractor, seeing I-III) observed at
22:17UT and saw the crater as a "ghostlike gossamer light". Cook, Moore
and North returned negative reports. Cameron 2006 catalog extension ID=
95 and weight=2. ALPO/BAA weight=2.
On 1980 May 18 at UT 22:27 P. Madej (Huddersfield, UK, 12" reflector,
seeing very good) observed Taruntius crater (in Earthshine) to change
brightness from black to light grey in about 30 seconds. Cameron 2006
catalog extension ID=95 and weight=2. ALPO/BAA weight=1.
1950 Nov 14 UT23:38 L.T. Johnson (La Plata, MD, USA, 10"
reflector, x179) observed a mag 10 flash in Earthshine. ALPO/BAA
weight=1.
CCD images were captured in white light that seemed to show that
the relative brightness between Aristarchus or Pytheas differed
considerably to what they were to be one night later on 2008 Nov 26.
Either Aristarchus was brighter on the 25th or Pytheas was darker.
Which feature, and which night, the abnormality occurred on is
uncertain. One possible explanation might be a brightness
gradient from glare from the sunlit side affecting the image contrast
quality of the CCD images for relative photometric measurements.
This TLP is being assigned a weight of 3 for now.
CCD images were captured in white light that seemed to show that
the relative brightness between Aristarchus or Pytheas differed
considerably to what they were to be one night later on 2008 Nov 26.
Either Aristarchus was brighter on the 25th or Pytheas was darker.
Which feature, and which night, the abnormality occurred on is
uncertain. One possible explanation might be a brightness
gradient from glare from the sunlit side affecting the image contrast
quality of the CCD images for relative photometric measurements.
This TLP is being assigned a weight of 3 for now.
On 1981 Apr 09 at UT 19:44 M. Price (Camberley, Surrey, UK, 6"
reflector, 58x and 117x) saw a 4 sec brightening in Aristarchus in the
clear Earthshine. Other features visible were: Grimaldi and some mare.
Foley found the crater to be "luminous & translucent". Cameron 2006
catalog ID=129 and weight=0. ALPO/BAA weight=1.
On 1931 Feb 22 at UT 20:30 Joulia (Castelnaudary, Aude, France?)
observed in the Aristarchus region: "Reddish-yellow glimmer of light,
very variable with nearly complete extinction. (similar to Herschel's
1787 & Tempel's 6/10/1866 obs.)". The Cameron 1978 atalog ID=399 and
weight=3.
On 1821 Nov ? at UT 19:00 an unknown observer (in England) reported
"Bright spots on the moon. (if early phase, date would be 26th-29th) 4
other instances mentioned. Fixed streaks of light in dark part -- first
one stated as moving. The cameron 1978 catalog ID=94 and weight=2. The
ALPO/BAA weight=1.
CCD images were captured in white light that seemed to show that
the relative brightness between Aristarchus or Pytheas differed
considerably to what they were to be one night earlier on 2008 Nov 25.
Either Pytheas was brighter tonight or Aristarchus was darker.
Which feature, and which night, the abnormality occurred on is
uncertain. One possible explanation might be a brightness
gradient from glare from the sunlit side affecting the image contrast
quality of the CCD images for relative photometric measurements.
This TLP is being assigned a weight of 3 for now.
CCD images were captured in white light that seemed to show that
the relative brightness between Aristarchus or Pytheas differed
considerably to what they were one night earlier on 2008 Nov 25.
Either Pytheas was brighter tonight or Aristarchus was darker.
Which feature, and which night, the abnormality occurred on is
uncertain. One possible explanation might be a brightness
gradient from glare from the sunlit side affecting the image contrast
quality of the CCD images for relative photometric measurements.
This TLP is being assigned a weight of 3 for now.
On 1988 Nov 15 at 10:07-10:40 UT P. Jean (Outremont, Quebec,
Canada, 4" refractor?) saw in the SE part of Mare Serenitatis
a luminescent area just over on the night side of the
terminator - it was cone shapes and coppery in colour. Cameron
comments that maybe it was a very low sun angle effect and she
has seen something similar, but on the bright side of the
terminator. Jean then goes onto comment that at 10:25UT a very
dark line was seen south of the cone i.e. east of the
terminator. A sketch was provided and P.Foley commented that
the cone did not correspond to any terrain. Cameron 2006
Catalog Extension ID=339 and weight=3. ALPO/BAA weight=2.
2004 Dec 18 UT 02:00 F. Serio (Houston, TX, USA) may have
imaged aperiod of brightening in this crater in images -
though Darling comments that it could be a Registax issue.
ALPO/BAA weight=1.
Ross D 1967 Dec 8 UT 02:30-02:40 Observer: Harris (Tucson?,
AZ?), colourless bright area SW of Ross D with repeated
condensations that appeared then dissipated in thirty seconds to
a minute. ALPO/BAA weight=1.
Proclus 2003 February 8,2003 UTC 02:09-03:07 Observed by Gray
(Winnemucca, NV, USA, 152mm F9 refractor Seeing 6-7, Transparency 6
305x) "Blinked Proclus with Wratten Red 25 and Blue 38A filters.
Features seen through the red filter were basically seen with the same
degree of clarity as in white light, in the case of sunlit walls, maybe
a little bit better in the red. With the Blue 38A filter only the
brightest part of the crater walls (north end) was visible-the rest of
Proclus was dark shadow. At 3:07UT I compared the brightest parts of
Proclus with Censorinus and Dionysius. The brightest parts of Proclus
and Dionysius were comparable. Censorinus was much less bright than
either of the above craters-the halo and crater were much faded over
its usual brilliant appearance. Both Censorinus and Censorinus A
were visible as distinct craters at 114x. The black shadow covering the
east 40% of Proclus last night had broken up into three patches
separated from each other by lighter bands. These were confined to
the east crater wall. Only the central patch was black, the other two
were considerably lighter. Running along the southwest edge of the
crater floor of the crater floor appeared to be a hill to the north
of which was a less elevated plateau. As the observing period
progressed part of the brilliantly illuminated north crater wall
developed a darker area which gradually became more prominent. As
the sun is getting higher I would expect shadows and dark areas to
diminish-what was happening here is unknown. However, this is not an
unusual event for this part of Proclus". The ALPO/BAA weight=2.
Theophilus 1966 Jan 28 UTC 01:24-03:45 Observed by Cross &
Ariola (Whittier, CA, USA, 19" reflector, x300, S=6-4, T=4, "3
red patches appearing and dissappearing at different times.
Obscurred at sunrise on it. Later, red patch appeared on the
floor." NASA catalog weight=5. NASA catalog ID #920. ALPO/BAA
weight=3.
On 1969 Nov 16 at UT 16:43-19:22 Dall'Ara (Switzerland, 4"? reflector),
Stucchi (Switzerland, 12" reflector) observed in Aristarchus
intermittent pulsations - Cameron speculates atmopsheric and also
mentions the Apollo 12 watch. The Cameron 1978 catalog ID=1211 and
weight=3. The ALPO/BAA weight=2.
Maskelyne 1969 Nov 16 UTC 16:28-17:10 Observed by Persson (Hvidore,
Denmark, 3" refractor) "Brightening & obscur. (Apollo 12 watch)." NASA
catalog weight=2 (low). NASA catalog ID #1210.
On 1979 Jul 01 at 22:00?UT D.J. Raden (Fort Meade, FL, USA, using a
10" reflector) detected a flare near to Halley (5E, 9S) visually with
the eye and it lasted about 3-4 min - a sketch was made. However it was
also found on one photographic slide taken with an exposure of 35
seconds. The observer comments that visually the flare was not as
bright as it appeared in the photograph. In an area near Halley. The
Cameron 2006 catalog extension ID=57 and weight=5. The ALPO/BAA
weight=4.
Alphonsus 1965 Apr 08 UTC 20:00? Observed by Hoffman (Germany?) "Saw
variable shining bright lights". NASA catalog weight=1 (very low). NASA
catalog ID #873.
Aristarchus 1965 Apr 08 UTC 20:00? Observed by Hoffman (Germany?) "Saw
variable shining bright lights". NASA catalog weight=1 (very low). NASA
catalog ID #873.
Censorinus 1965 Apr 08 UTC 20:00? Observed by Hopmann (Czecholovakia?)
"Green flash or brightening (date correct ? written 8-4-65. First taken
as American convention, thus as Aug. 4, but now think it was in
European convention of day first then month)." NASA catalog weight=2
(low). NASA catalog ID #873a.
Hyginius N 1965 Apr 08 UTC 20:00? Observed by Hoffman (Germany?) "Saw
variable shining bright lights". NASA catalog weight=1 (very low). NASA
catalog ID #873.
Linne 1965 Apr 08 UTC 20:00? Observed by Hoffman (Germany?) "Saw
variable shining bright lights". NASA catalog weight=1 (very low). NASA
catalog ID #873.
Proclus 1965 Apr 08 UTC 20:00? Observed by Hoffman (Germany?) "Saw
variable shining bright lights". NASA catalog weight=1 (very low). NASA
catalog ID #873.
On 1987 Nov 28 at UT 04:16-04:45 D. Louderback (South Bend, WI, USA,
3"reflector, x150, S=E) observed that the Promontorium Agarum plateau
was rather dull and grayish - usually it was "tannish" "even > sunlit
areas, & twin craters at his point A which are always > spots on
plateau. At 0420 whole plateau sank into complete darkness, hard to
distinguish from mare plain. albedo dropped to 5 from 6.8 reading.
Nearby plain was normal 5 so phenomena had not spread to it. At 0424
Cape started to reappear to albedo 6 until 0445, when it returned to
normal, but not sharply defined - like through haze. Detail better in
red than in blue filter, sketches. The Cameron 2006 catalog ID=315 and
the weight=4. The ALPO/BAA weight=3.
Hyginus Nova 1877 Nov 13 UT 20:00? Observed by Crain, Klein, Eng.
officer (France?, Cologne (Germany), Enland?, 6" refractor?, S=E)
"Standing out with such prominence, seen at a glance. No trace of it on
14th, in excell seeing. (indep. confirm.?)"NASA catalog weight=5 (very
high). NASA catalog ID #198. ALPO/BAA weight=3.
Fauchier of Marseilles, France, seeing=good - fair and the Moon at a
high altitude, saw two lights on the Moon brighter than any others
during similar circumstances. They had colour. These had not been seen
before and he ruled out cromatic aberation. Cameron 1978 catalog ID=249
and weight=3. ALPO/BAA weight=2.
Menelaus 1969 Nov 17 UT 16:00-19:00 Observed by Rubens de
Azevedo,A. Monghilhot, E. Leal e Jose Fernandes (Joao Pessoa,
Paraiba, Brazil, 8" and 10" reflectors) "Entire crater of
Men. illum. by pale greenish light. (Azevedo)" NASA catalog
weight=5 NASA catalog ID #1211a. ALPO/BAA weight=4.
Proclus 1972 Oct 15 UT 20:48 Observed by Hopp (13.25E, 52.5N,
75mm refractor) "Bright flash at the NW wall but poor seeing."
T=3, S=5. Ref: Hilbrecht & Kuveler Moon & Planets (1984) Vol
30, pp53-61. ALPO/BAA weight=1.
2004 Dec 20 UT 02:51-03:26 R. Gray (Winumma, USA) noted that
the crater had exceptional brightness to nimbus surrounding it. ALPO/BAA
weight=1.
On 1995 Jul 06 at UT 03:22-03:57 R. Spellman (Los Angeles, USA
found that the floor of Proclus appeared to darken slightly
through a blue filter. The ALPO/BAA weight=2. Source of this
observation came from Spellman's web site.
In 1878 Oct 04 at UT 20:00 an Unknown observer noted that Hyginus Nova
could not be seen, whereas the night before the crater had the most
conspicuous of all appearances. The Cameron 1978 catalog ID=201 and
weight=3. The ALPO/BAA weight=2.
Hyginus Nova 1867 Nov 14 UT 20:00? Observed by Crain, Klein, Eng.
officer (France?, Cologne (Germany), Enland?, 6" refractor?, S=E) "On
13th it was standing out with such prominence, seen at a glance. No
trace of it on 14th, in excell seeing. (indep. confirm.?)"NASA catalog
weight=5 (very high). NASA catalog ID #198.
Tycho 1940 Jul 14 UT 02:00? Observed by Haas (NM? USA, 12"?
reflector) "Luminous marks in shadow, ragged edged & irreg.
shape. E. wall had a milky luminosity" NASA catalog weight=4.
NASA catalog ID #468. ALPO/BAA weight=2.
On 1964 Feb 22 at UT 05:00 Harris (Whittier, CA, 19" reflector, x100)
observed the appearance of a ring to the south east of Ross D. Cameron
says that 7 persons have seen this over a 2.5 year period. The Cameron
1978 catalog ID=801 and weight=1. The ALPO/BAA weight=1.
Gassendi 1967 Feb 18 UT 20:30-20:40 Observed by Moore, Moseley
(Armagh, Northern Ireland, 10" refractor, x300) "Red color in
crater (in dark)". NASA catalog weight=4. NASA catalog ID #1015.
ALPO/BAA weight=4.
On 1980 May 23 at UT21:14-21:55 J.H. Robinson (Teighmouth, Devon, UK,
12" reflector, seeing II-III) could see Aristarchus in blue and clear
filters, but not in red light. Robinson saw some variability in this
effect with time. Cameron 2006 catalog ID=96 and weight=3. ALPO/BAA
weight=2.
On 1980 May 23 at UT 21:14-21:18 Marco Petek (Porto Alegre,
Brazil) saw a shadow extending south east from Campanus
opposite to the Sun - however Foley thinks this is normal.
Cameron 2006 catalog ID=96 and weight=0 or 1.
ALPO/BAA weight=1.
On 1980 May 23 at UT21:14-22:18 G. Blair (Bridge of Weir,
Scotland, UK, 216mm reflector, seeing II-IV) found a red tinge
along the western wall of Coperncius, perhaps 32km in length.
This was invisible in a blue-green Wratten 44a filter, but was
unmistakble in a red Wratten 25 filter. Could have been
spurious colour - but no other regiosn were affected. The
ALPO/BAA weight=2.
On 1980 May 25 at UT 22:18 G. Blair (Bridge of Weir, Scotland, 216mm
reflector, seeing II-IV) suspected a short sharp flash, white in colour
north of Tycho's north wall. Nothing more seen. ALPO/BAA weight=1.
On 1980 May 23 at UT22:30 (P.W. Foley (Kent, UK, 10" reflector, seeing
II) described Aristarchus as a "blue luminous patch", but it was too
faint to obtain a CED brightness measurement. Cameron 2006 catalog ID=
96 and weight=3. ALPO/BAA weight=2.
2012 Sep 24 UT 22:00-23:00 Copernicus. E. Horner (Salisbury,
UK, 15cm reflector) observed a prominent red arc where the
sunlit part of the interior wall met the shadow. Sometimes the
arc was 1/4 the way around the interior, and sometimes half of
the way around. Telescope moved, but the red arc stayed where
it was. Eyepieces change, but the effect remained. Other parts
of the Moon checked, but no red seen. There were however
splashes of green e.g. Longomontanus on the terminator,
elsewhere further inland from the termionator, and little
splashes of green on Mare Frigoras - but lasting a brief time.
The red colour was as strong as a red LED and the green similar
to that of the northern lights. The observer's husband was asked
to independetly check Copernicus and remarked that he could see
a little bit of green at the top and some red near the bottom,
along the line of the internal shadow. Although there were
checks for red elsewhere on the Moon and none were seen, the
Moon was starting to get low and it is typical of spurious
colour in a few respects. Therefore the ALPO/BAA weight=1 for
safety.
Atlas 1966 Dec 21 UT 17:10 Observed by Andre (Belgium, 3" refractor)
"Bright spot on SE part of floor, not seen in photo on 12/18/66" NASA
catalog weight=2 (low). NASA catalog ID #1003.
Mons la Hire 1972 Nov 15 UT 09:45-10:18 M.Geisel (Brisbane,
Australia, 12.5" f/8 reflector, x90) discovered the TLP, P.
Anderson (9.5" reflector) independently confirmed that the TLP
had an effect in his Moon Blink device - but the effect
(suspected that the blink was caused by the extreme nrightness
of the mountain?) was weak and thought it not worth further
investigation. Photographs taken by Anderson. Geisel believes
the effect to be real and states that the area remained sharp
and clear throughout. ALPO/BAA weight=2.
Proclus 1969 Nov 18 UT 20:00? Observed by Classen (Pulnitz,
Czechoslovakia, 8" refractor) "Brightened, exceeded normal.
Brightness is monitored relative to Censorinus. (started July,
1969) Obs. thinks all bright craters are variable. (Apollo 12
watch)." NASA catalog weight=2. NASA catalog ID #1216.
ASLPO/BAA weight=1.
In 1872 Mar 19 at UT 23:17 an unknown observer observed in Sinus
Iridum: "Covered with a light gray shadow thru which he saw dimly the
surface below - indicating obscuring matter over it. (Cameron says:
only w. 1/3 of bay would be in shadow as boundaries are 25-37W)". The
Cameron 1978 catalog ID=178 and the weight=3.
Agrippa and vicinity 1878 Dec 04 UT 20:00? Observed by Capron (France?)
"Odd, misty look as if vapor were in or about them" NASA catalog
weight=3 (average). NASA catalog ID #209.
Alphonsus 1966 Apr 01 UT(?) 03:00-03:20 Observed by Jenning,
Harris (Coral Estates, CA, USA, 12" reflector) "Red patch from
c.p. to W. wall (no confirm. from Corralitos obs. moon blink
device & obs. at that time)" NASA catalog weight=3. NASA
catalog ID #924. ALPO/BAA weight=2.
Alphonsus 1967 Feb 19 UT 20:30-21:11 Observed by Moore,
Moseley (Armagh, Northern Ireland, 10" refractor, x360) "Blink
area between 1900 & 1940 with neg. results. Suddenly at 2030
there was a bright red glow, brightest Moseley had ever seen,
at Feb 17 suspectec place. Moore returned at 2037h in time to
see fading effect. Brief return at 2105-2111; neg. from
2120-2250h then clouds. Nothing on Feb 20. confirmation)."
NASA catalog weight=5. NASA catalog ID #1016.
ALPO/BAA weight=4.
Colour seen, mostly blueness on south rim and exterior of south
rim at Bullialdus crater. Blueness seen too on Plato on inner SSW
rim, but no colour reported on any other craters. Seeing III,
12" reflector used x200 and x360.
Colour seen, mostly blueness on inner SSW rim. Blueness also seen
on south rim and exterior of south rim at Bullialdus crater. No colour
reported on any other craters. Seeing III, 12" reflector used x200 and
x360.
Arsyukhin and others (Moscow, USSR), with naked eye and binouculars
saw three dark spots suddenly appear on Mare Crisium and disappear
approximately 30 minutes later. Cameron 2006 catalog extension ID=145
and catalog weight=4. ALPO/BAA weight=2.
Arsyukhin and others (Moscow, USSR), with naked eye and binouculars
saw TLP activity in Plato that Cameron thinks confirms what UK
observers saw later. Cameron 2006 catalog extension ID=145
and catalog weight=4. ALPO/BAA weight=1.
Observed by G.H. Johnstone of Albuquerque, NM, USA on 1954 Nov 05 UT
20:00 (according to Cameron), but 02:00-04:00 according to the
original observation and at colongitudes 34.7 to 35.7 deg. 4"
reflector, x150 used. The obsewrver reported that the western part
(about 1/3rd of the interior) was pitch black with shadow. However
there was a zone about as wide, or perhaps only a fourth of the total
width that was distinctly a lighter bluish shade, almost like twilight.
The shadows of the peaks on the western edge of the rim were clearly
seen crossing this bluish shadowed area. Then this area ended sharply,
and the farside was bathed in light from the rising sun. The shadows of
the peak were sharply defined across the twilight zone, and the edge of
the pitch black shadow was easily defined but not as sharp as the
darker shadows crossing the the blue twilight zone. The observer
checked other craters but did not see this condition in any of them -
they all had the abrupt division between black and white that we would
normally expect to see. Cameron 1978 catalog ID=579 and weight=2.
Reference 1962 edition of ALPO's Journal: The Stolling Astronomer.
ALPO/BAA weight=3.
Censorinus 1969 Nov 19 UT 1922 Observed by Brandli (Wald,
Switzerland, 6" reflector, x90) "Brightening -- photo, (the
author, WBC, cannot verify from photo. It is brighter, but so
are Proc. & Dionys. -- it being between. i.e. Proc. > Censor. >
Dionys. Apollo 12 watch)." NASA catalog weight=5 (very high).
NASA catalog ID #1220. ALPO/BAA weight=1.
Plato 1870 May 10 UTC 22:00 Observed by Birt (England) "Extraordinary
display of lights. Says not effect of sunlight" NASA catalog weight=4
(high). NASA catalog ID #167.
P. Moore at 21:10 found the southern wall (and ontothe southern floor)
of the crater to be indistinct. Elsewhere in the crater everything was
sharp. The effect was still seen at 21:42UT, but less strong. A check
was made for colour with aq Moonblink device, but none was seen. There
was still a trace of this effect at 21:44UT, although detail was now
becoming visible. By 21:48UT vertical streaks were seen crossing
the floor from the obscuration area and these were more visible in the
red filter and not in the blue. Cameron comments that undefined patches
on the floor of Plato are not normal. By 21:55UT some craterlets on the
floor started to become visible and the TLP for Moore ended by UT22:23.
P.Foley was alerted by Moore and saw a "amssive dense obsecuration
on the south wall, south floor and south outer glacis to the Mare".
Foley noted that by 21:50UT the effect was fading and finished by
22:03UT. Foley reported an orange translucent haze covering half of the
floor, but floor craterlets could be seen on and off - however his
atmospheric seeing conditions were IV. At 22:00 UT Foley reported the
floor close to the north wall to be "milky or misty". No detail was
visible at 21:15UT and variability in the floor continued until
23:10UT. Hedly-Robinson was aleted at 21:35UT and found no difference
between red and blue views of the area, however he did find that the
south rim was indistinct although this effect had lessened by 22:00 UT
and was normal by 22:17UT. M. Mobberly saw a white spot on the floor at
21:20 UT, whereas he normally would have expected to see craterlets.
Mobberly was alerted at 21:40 UT and took some colour photos. He also
made sketches that showed variability in the floor and dark lines and
patches in the north west corner. However the altitude of the Moon was
low. Cameron mentions that two of the photos show loss of detail at the
south wall and beyond.and also a change in the floor markings.The north
wall at 21:50UT was strangely reddish (didn't think this was spurious
colour). The rest of the wall was sharp at 22:20UT through a yellow
filter. Large bright patch in the centre and rest of the floor was
apparently of the same shading as Mare Imbrium. The above notes are
based upon the Cameron 2006 catalog extension TLP ID 145 and weight=4.
ALPO/BAA weight=2.
Piton 1969 Nov 19 UT 21:15-22:00 Observed by Baum (England,
4.5" refractor) "Traces of cloudiness on E. slope at 2115h.
Increased at 2150h in extent & brightness. Spread onto plain.
Summit & shadow in W. part sharp & clear. (Apollo 12 watch)."
NASA catalog weight=2. NASA catalog ID #1221.
ALPO/BAA weight=2.