Plato 1966 Aug 01 UT 06:14 Observed by Kelsey (Riverside, CA,
USA, 8" reflector x300) The wall from the S to the NNE wouldn't
focus well though at least 4 craterlets on the floor were
clearly seen (Ricker uncertain if real TLP. Cameron thinks it
probably was -- similar to Bartlett's experience on Aris. NASA
catalog weight=2. NASA catalog ID #961. ALPO/BAA weight=1.
On 1938 Jan 16 at UT 00:00 Barker (Chestnut, England, UK, 12.5"
reflector) noticed that Plato crater had a brownish-gold veined
surface, colour irregular - laid on a smooth floor. The Cameron
1978 catalog ID=430 and weight=3. The ALPO/BAA weight=2.
On 1976 Feb 14 at UT23:35-0053 LeCroy (Springfield, VA, USA, 4.5"
reflector, x75, S=6 and T=4.5). A blue haze was seen on the east side
of Aristarchus and red haze on the west side. At 00:00UT details were
more clear and at 00:24UT Aristarchus and Herodotus, were seperated. At
00:34UT colours were gone. At 00:35UT blue was on Aristarchus and the
area was bright, but was black in a red filter. At 00:53UT the features
were clear and the colour gone and the brightness had decreased to 9.
Cameron comments that the colour was not due to temp. inversion because
of being dark in the red filter, implying a medium). The Cameron 1978
catalog TLP ID is 1428 and the weight=1. This is an ALPO report. The
ALPO/BAA weight=1.
On 1996 Dec 24/25 at 18:12-00:02UT P. Moore (Selsey, UK, using a 15"
reflector x250-360, and seeing III) saw a strong orange colour on the
south wall and floor of Aristarchus. He suspected it to be spurious
colour but could not detect colours on any other craters. The colour
remained but at 18:12 UT he suspected a trace on colour on Mons Pico
but was not sure. However he reported it to the TLP coordinator of the
BAA Lunar Section. The orange in Aristarchus gradually faded and had
almost vanished by 00:20UT when seeing was too bad to continue
observing. At 02:30UT he was able to re-observe again and there was
still a very very slight hint of orange in Aristarchus - but he
comments that if he had not been looking for it he might not have
noticed. ALPO/BAA weight=2.
Mare Crisium 1948 Jul 21/22 UT 22:00?-01:00? Observed by Moore
(England, 12" reflector) "Almost featureless except for Peirce &
Picard" NASA catalog weight=3. NASA catalog ID #506. ALPO/BAA
weight=2.
On 1993 Mar 08 at UT 22:30 R. Titford (England, UK, 8.5" reflector,
seeing=III) found a very bright white area on the northern wall, "floor
< Mare Imbrium". The Cameron 2006 catalog ID=456 and weight=3. The
ALPO/BAA weight=2.
Plato 1966 Aug 02 UT 06:26 Observed by Kelsey (Riverside, CA, USA, 8"
reflector x300) "Again E(IAU?) wall would not focus" NASA catalog
weight=2 (low). NASA catalog ID #962.
On 1891 Sep 18 at UT 21:00 Pickering, based at Arequipa, Peru, and
using a 12" reflector, saw in Schroter's Valley and the vicinity
"Varitions in vapor column. Drawings. Time estimated from given
colongitude)." Cameron 1978 catalog ID=271 and weight=1. ALPO/BAA
weight=2.
Aristarchus 1965 Sep 11 UT 08:08-08:15 Observed by Cross,Rasor (Parlos
Verdes, CA, USA, 22" reflector x133, S=F-P) "Red glows,. Photos
obtained but do not show phenom. Haze terminated obs." NASA catalog
weight=5 (very high). NASA catalog ID #894.
Plato 1921 Nov 15? UT 20:00? Observed by Chernov (Russia, 2" refractor
x94) "Temporary increase in brightness of the light band at bottom
noted close to FM. Crater actively noted in Oct. 10." NASA catalog
weight=1 (very low). NASA catalog ID #384.
Aristarchus 1964 Sep 22 UT 02:54-03:03 Observed by Bartlett
(Baltimore, MD, USA, 4" refractor x240, S=5, T=5) "Bright blue-
viol. gl. on NE rim & EWBS; dark viol. nimbus; S. floor 8deg br.
rest of crater 7 deg. Red-brown, changed to coppery, to yellow-
brown (Gilheany, et al. examined crater later, but did not
detect any color in MOON BLINK, so red-brown must have
disappeared." NASA catalog ID #851, NASA catalog weight=4.
ALPO/BAA weight=3.
E. of Pytheas in M. Imbrium 1970 Jun 19/20 UTC 23:54-00:23 Observed by
Sendor-Mark (Szolnok, Hungary, 4" reflector x 200) "Bright spot nr.
Timocharis (on E. Copernican ray?) decreased slowly for next 8min 19
sec. At 00:11:05 flared up. After 2nd decreasing, brightened again at
00:25:54 after which no variablity. Event was star-like < 3km. No
events on 21st." NASA catalog weight=2 (poor). NASA catalog ID=#1262.
Kunowsky 1964 Sep 22 UT 03:25-04:30 Observed by Gilheany, Hall, and
Johnson (Port Tobacco, MD, USA, 16" reflector, Seeing=good) "Red area
detected by Trident's MOON BLINK (MB) device, (Aris. normal)." NASA
catalog weight= 5 (very high). NASA catalog ID #852.
On 1981 Oct 15 at UT06:03-06:51 D. Louderback (South Bend, WA, USA, 3"
refractor, seeing=1-2 and transparency=5) observed that the brightenss
of 4 sun lit bright spots differed in red and blue light. "Appeared as
a cross. the 2 points A & D on his sketch (index) were affceted. They
were 10 pts dimmer in red than blue. Not due to seeing as they did not
fluctuate (as did the seeing)." This report came from the Cameron 2006
catalog and had an ID No. of 156 and a weight=3. The ALPO/BAA weight=2.
Schroter's Valley 1898 Apr 09 UT 04:00 Observed by Pickering
(Cambridge, Mass. USA, 15" refractor) "Variations in vapr col. Break in
main col. Similar to earlier. time est. fr. given col. Date given is
8th LT =9th UT?."NASA catalog weight=2 (low). NASA catalog ID #300.
Aristarchus 1966 Aug 05 UT 05:22-05:38 Observed by Bartlett (Baltimore,
MD, USA, 4" reflector x93, x125, x281, S=4, T=5), "S. part of floor was
granulated & est. at 6 deg bright; faint yellow-brownish tint. Rest of
crater 8 deg bright white."NASA catalog weight=4 (high). NASA catalog
ID 963.
Triesnecker 1966 Jul 10 UTC 02:00-02:15 Observed by Allen (Cambridge,
England) and other observations by Corralitos Observatory (Organ Pass,
NM, USA). Described in NASA catalog as: "Faint illum. of a ridge in
shadow; faded quickly (in BAA judged dubious). Not confirmed by
Corralitos MB." 12?" refractor (x280) used at Cambridge and at
Corralitos 24" reflector. NASA catalog weight=1 (very low). NASA
catalog TLP ID No. #956.
On 1996 Feb 12 at UT 07:30-08:27 J.Sandel (Caycee, SC, USA)
noted a contrast effect inside Tycho at sunset. At 07:30UT there
was a slight, but definite illumination of small areas of the
crater floor west of the central; peak. Also seen by T. Ferrel
(Lawrenceville, GA, USA, SCT C8). This was oval in shape and
gray in colour - Ferrel noted some diffuseness. It brightened
over 30 minutes. At 08:11UT a definite brightness fade noted in
Tycho's central peak. The crater floor had increased
illumination of entire crater floor. ALPO/BAA weight=3.
On 1940 Dec 25 at UT 10:00? Haas (New Mexico, USA, 12" reflector?)
observed the northern horn to be elongated by about 10'. The Cameron
1978 catalog ID=482 and weight=3. The ALPO/BAA weight=2.
On 1940 Dec 25 at UT 10:00? Haas (New Mexico, USA, 12" reflector?)
observed the southern horn to be elongated by about 10'. The Cameron
1978 catalog ID=482 and weight=3. The ALPO/BAA weight=2.
James Short, Dr Harris and Mr Stephens saw initially a streak of
light on the shadowed floor of Plato. They were not expecting to see
any light to reach the floor. Shortly afterwards they saw a second
streak of light parallel to the first and this shortly divided
into two. Gaps in the mountains were found for both streaks,
but they were unable to understand why one of the streaks divided
into two. Cameron's 1978 assigns this TLP an ID of 20 and a weight
of 5. The ALPO/BAA catalog assigns a weight of 1.
During an occultation of lambda Geminorum on the eastern limb
the light from the star took 3 seconds to fade. Cameron 2006 catalog
extension ID=8 and weight=2. ALPO/BAA weight=1.
On 1988 May 18 at UT01:00-02:35 Lubke (Middleton, WI, USA, 8"
reflector, x130) reported that Aristarchus glowed "like an out of focus
star varying with the atmosphere". Darling (Sun Praire, WI, USA, 20x60
binoucular) and Spain (Fairdale, KY, USA, 7x35 and 20x60 binoculars, S=
6/10) found that both Copernicus and kepler were brighter than
Aristarchus in Earthshine. Aristarchus itself looked unusual, though
Spain did not see Aristarchus at all. Darling and Wieir (20x60
binouculars) agreed that it appeared as a star-like point in
binoculars. Cameron 2006 catalog ID=326 and weight=0. ALPO/BAA
weight=1.
On 1988 May 18 at UT01:00-02:35 Lubke (Middleton, WI, USA, 8"
reflector, x130) reported that Aristarchus glowed "like an out of focus
star varying with the atmosphere". Darling (Sun Praire, WI, USA, 20x60
binoucular) and Spain (Fairdale, KY, USA, 7x35 and 20x60 binoculars, S=
6/10) found that both Copernicus and kepler were brighter than
Aristarchus in Earthshine. Aristarchus itself looked unusual, though
Spain did not see Aristarchus at all. Darling and Wieir (20x60
binouculars) agreed that it appeared as a star-like point in
binoculars. Cameron 2006 catalog ID=326 and weight=0. ALPO/BAA
weight=1.
On 1988 May 18 at UT01:00-02:35 Lubke (Middleton, WI, USA, 8"
reflector, x130) reported that Aristarchus glowed "like an out of focus
star varying with the atmosphere". Darling (Sun Praire, WI, USA, 20x60
binoucular) and Spain (Fairdale, KY, USA, 7x35 and 20x60 binoculars, S=
6/10) found that both Copernicus and kepler were brighter than
Aristarchus in Earthshine. Aristarchus itself looked unusual, though
Spain did not see Aristarchus at all. Darling and Wieir (20x60
binouculars) agreed that it appeared as a star-like point in
binoculars. Cameron 2006 catalog ID=326 and weight=0. ALPO/BAA
weight=1.
On 1990 Apr 26 at UT 19:30-20:30 S. Beaumont (Cambridge, UK, seeing=II,
very good) observed Aristarchus to be "very bright" in Earthshine - it
varied in brightness. However she could also see the edges of the mare
and the west limb clearly. Grimaldi was slso seen. Cameron suspects
that these are atmospheric effects. The cameron 2006 catalog ID=400 and
the weight=0. The ALPO/BAA weight=1.
On 1990 Apr 26 at UT 19:30-20:30 S. Beaumont (Cambridge, UK, seeing=II,
very good) noted that Grimaldi was seen well however she could also see
the edges of the mare and the west limb clearly. Cameron suspects
that these are atmospheric effects. The cameron 2006 catalog ID=400 and
the weight=0. The ALPO/BAA weight=1.
In 1821 May 04 at UT 21:30-22:00 Ward (England? Large aperture
telescope, x80), Bailey (England?) and Olbers (Bremen, Germany,
refractor) observed in the Earthlit part of the Moon an apperent small
comet like feature extended from Aristarchus towards Grimaldi. The
light was similar to a glow worm. The observer had never seen anything
like it. The cameron 1978 catalog ID=89 and weight=3. The ALPO/BAA
weight=4.
On 1988 May 19 at UT01:14-02:30 D. Darling (Sun Praire, WI, USA, 7x35
binoculars) was able to see Copernicus OK, Kepler (only just) and
Aristarchus was invisible in Earthshine. He could not see the usual
bright areas in Earthshine either. D. Spain (Fairdale, KY, USA,
3.5"reflector, x30-277) could not see anything in Earthshine. Lubke
(Middleton, WI, USA, 8" reflector, x75 and x130) though was able to see
Aristarchus and it was brighter than its surroundings, however it was a
lot fainter than on the 18th May. Cameron suspects that this was
atmospheric in origin and not a TLP. The Cameron 2006 catalog ID=329
and weight=0. The ALPO/BAA weight=1.
On 1990 Apr 27 at UT20:00-20:30 P. Mugridge (Surrey, UK) observed a
bright light "sometimes 3 lights in form of triangle" in Oceasnus
Procellarum (56W, ~25N), roughly mid way between Schroter's Valley and
Briggs. "Haze surrounds as a mist or fog. poss. < at end of obs."
Cameron comments that this may have been as a result of contrast in the
strong Earthshine. Foley even contemplates if it was a
misidentification of Aristarchus. Cameron comments that it is probably
not due to terrestrial atmosphere. The Cameron 2006 catalog ID=401 and
the weight=1. The ALPO/BAA weight=1.
Southern Cusps 1912 Jun 17 UT 20:00 Observed by Stolyarenko (Russia)
"Sharply outlined edges of new moon easily extended in 25 deg band over
unlit part. S. horn larger than N. one" NASA catalog weight=1 (very
low). NASA catalog ID #340.
On 1989 Apr 09 at 00:00? R.Horton (N.Scituate, RI, USA, 6" reflector)
found Aristarchus (and Kepler) to be much less bright than Copernicus.
Photographs show this. The Cameron 2006 catalog ID=359a and the weight=
3. The ALPO/BAA weight=2.
On 1989 Apr 09 at UT 00:00? R. Horton (N. ScN. Scituate, RI, USA, 6"
reflector) took an Earthshine photograph that revealed Copernicus to be
brighter than Aristarchus and Kepler. Cameron comments that usually
Aristarchus is the brighter and thought it a bit odd because Copernicus
should have been less visible, being nearer the terminator3 The Cameron
2006 catalog ID=359a and the weight=5. The ALPO/BAA weight=2.
On 1989 Apr 09 at UT 00:00-04:45 D. Darling (Sun Praire, WI, USA, 11"
reflector, 3" refractor, S=9/10 and T=6) observed the central peak of
Tycho in Earthshine and that the crater "glowed". However Earthshine
was exceptionally bright tonight. The Cameron 1978 catalog ID=359b and
weight=3. The ALPO/BAA weight=1.
On 1990 Apr 28 at UT 00:00-00:30 F. Graham (Marshall TWP, OH, USA, 6"
reflector) during a failed attempt to observe the occultation of X6493
that was thwarted by clouds, noticed that Gassendi was "Gass,>>,>Aris
or anything else". The crater had a "milky lustre". It is possible that
another occultation observing group may have a video of the Earthshine
at this time. Darling (Sun prairem WI, USA, 20x50 binoculars) could not
see Earthsine, though the sky was bright at the time. The Cameron 2006
catalog ID=402 and the weight=0. The ALPO/BAA weight=1.
On 1883 Mar 12 at UT 20:00 Hopkins (located somewhere in the eastern
USA) saw a line of light-well seen (similar to Cameron's TLP catalog ID
235, except for the apparent phase. The Cameron 1978 catalog ID=235 and
the weight=1. The ALPO/BAA weight=1.
On 1969 Jul 18 at UT06:15-08:00 Heath (Christchurch, New Zealand) noted
that Aristarchus was brighter than normal (Apollo 11 watch). The
Cameron 1978 catalog ID=1157 and weight=1. The ALPO/BAA weight=1.
On 1980 Oct 12 at UT23:30 D.Darling (Sun Praire, WI, USA, 12.5"
reflector, x75, seeing 10/10) observed the crater to be glowing faintly
- photos showed it to be blue. Cameron 2006 TLP catalog ID=113 and
weight=3. ALPO/BAA weight=1.
In 1821 May 06 at UT 21:45 Ward (England? Large aperture
telescope, x80), Bailey (England?) and Olbers (Bremen, Germany,
refractor) observed in the Earthlit part of the Moon an apperent small
comet like feature extended from Aristarchus towards Grimaldi. The
light was similar to a glow worm. The observer had never seen anything
like it. The cameron 1978 catalog ID=89 and weight=5. The ALPO/BAA
weight=3.
In 1937 Feb 15 at UT 16:00? Arkhipov (Russia) observed in Cassini:
"Blue-greenish scintillating spots at bottom of crater were vis. on
ashen light background. (confirm of Andrenko?)". The Cameron 1978
catalog ID=419 and weight=5. The ALPO/BAA weight=3.
On 1939 Feb 23 at UT 23:00 Andrenko (Sao Paulo?, Brazil)
observed Aristarchus as a bright spot -- bluish (Cameron says
confirmation of Malakhov), The cameron 1978 catalog ID=445 and
weight=5. The ALPO/BAA weight=3.
Cusps 1953 Apr 18 UT 21:00? Observed by Wilkins (Kent, England, 15"?
reflector) "Faint extension of the cusps. (high peaks in sunlight)."
NASA catalog weight=2 (low). NASA catalog ID 558.
Cusps 1953 Apr 18 UT 21:00? Observed by Wilkins (Kent, England, 15"?
reflector) "Faint extension of the cusps. (high peaks in sunlight)."
NASA catalog weight=2 (low). NASA catalog ID #558.
On 1969 Jul 19 at UT 06:30 Whelan (Wellington, New Zealand) observed a
pulsating glow in Aristarchus crater, extending towards the north. The
Cameron 1978 catalog ID=1162 and weight=2. The ALPO/BAA weight=2.
On 1983 Sep 11 at UT 23:52 K.P. Marshall (Columbia, 12"
reflector, x268, seeing II), whilst sketching the crater
Janssen noticed a tenuous red patch on the southern junction
of the valley which joins Fabricius to A. Nothing resembling
this found on nearby areas. The ALPO/BAA weight=1.
On 2010Apr18 at UT 20:45-21:00 P. Grego (St Dennis, UK, 17"
reflector - first practice run) observed that Aristarchus in
Earthishine was the brightest that he had seen it before. The
effect had faded to normal in the next 15 minutes though. "The
bright spot was initially thought to be part of the wall of
Aristarchus, but on closer examination the spot was probably the
crater’s central peak. At around this time I estimated the
brightness of the peak to be around magnitude 8, but this is a
poor estimate as no suitable comparison stars in the immediate
vicinity of the field of view were to be seen. Aristarchus’
outline was visible, as was a clearly defined sweep of
brightness to its west (presumably the high albedo markings
southeast of Herodotus) and another illuminated area to the
north of Aristarchus (presumably the Vaisala area), and a small
illuminated patch on the eastern flanks of Aristarchus. No other
areas of the Moon in earthshine appeared to be as bright as
these markings, and there were certainly no other clearly-
defined spots as brilliant as the one that lay in Aristarchus. A
watch was kept until 22:00 UT, when the Moon went out of view
behind a tree. During this period it appeared that the spot was
becoming less bright and less clearly-defined, although the
other albedo markings in its vicinity remained visible; this may
have been a consequence of the Moon’s diminishing altitude.
ALPO/BAA weight=1.
On 1967 Jul 20 at UT 07:00 Whelan, (Wellington, New Zealnd) saw a
pulsating glow from Aristarchus crater, and this continued, although
less pronounced. This was during the apolo 11 watch. The Cameron 1978
catalog ID=1172 and the weight=2. The ALPO/BAA weight=2.
On 1974 Feb Weith-Knudson (Copenhagen, Denmark, 12" refrlector, x72)
observed a magnitude 7.7 flash (comparison between SAO093043=mag 7,8
and SAO093052 mag=7.5 that happened to lie in the field of view at the
time) in Earthshine. The observer speculates whether this was a lunar
meteorite impact or a reflection from an artificial satellite (or
indeed as Cameron suggests from an Earth meteor?). The cameron 1978
catalog ID=1388 and weight=0. The ALPO/BAA weight=1.
Proclus NW ray 2003 Sep 02 UTC 02:20-03:35 Observed by Haas (Las
Cruces, NM, USA) "Everyone knows the bright ray running northwest from
Proclus. In this view from 2:20 to 2:36, UT on September 2 I remarked a
thin, pink southwest border to the ray. One thinks of chromatic
aberration, and the position supports this interpretation; but other
bright lunar features showed no such effect. The pink border lay 1 to
2.5 diameters away from Proclus (S=2, T=3.5). At 2:55, UT (S=1-2, S=
3.5) the border was gone; neither its appearance nor disappearance was
observed. At 03:25 UT there is no sign of the pink border (S=2, T=3),
moreover the Moon was lower, so atmospheric dispersion must be greater
by now? 12.5" Newtonian x321 at 02:20-02:36, x202 at other times.?"
Note that experiments to simulate spurious colour using Adobe Photoshop
were able to recreate colour in the correct place on the NW ray -
however there should have been colour reported on the SW ray too and
there was no mention of this, therefore the observational report is
intriguing. The ALPO/BAA weight=2.
M. Price of Camberley, UK noticed that an area in relation
to the central area of the floor could not be resolved. Averted
vision was used, but this did not help to resolve detail. The crater
was close to the terminator and was in general sharply in focus
apart from the suspect area. No spurious colour seen. Sketch
supplied.P. Foley wonders if the effect was due to the resolution
limit of Price's scope? Cameron 2006 extension catalog ID=78
and weight=2. ALPO/BAA weight=2. 6" reflector x64 and x120.
Seeing=III-IV and Transparency=good.
On 1969 Jul 20 at UT 0845 McIntosh (Auckland, New Zealand, 14"
reflector) saw Aristarchus crater to be brighter in red light. This was
during the Apollo 11 watch. The Cameron 1978 catalog ID=1173 and
weight=3. The ALPO/BAA weight=3.
On 1975 Mar 18 at UT17:30 M.Kidger (Winterbourne Down, Bristol, UK,
60mm refractor, x36, very good conditions with a very sharp image and
the sky was almost perfectly clear apart from a very few small clouds).
In Mare Crisium it was observed that only a ray of Proclus could be
seen to cross the floor - normally there are at least four craters
visible inside mare Crisium on good nights and at least one being
visible under bad conditions. So despite it being very clear and the
image quality being good, the observer found it odd that no craters
were visible on the floor of mare Crisium. This is a BAA Lunar Section
report. The ALPO/BAA weight=2.
Observations made by Challis of Cambridge, and N. Pogson of Hartwell,
both of the UK. Before the occultation, Saturn's rings were
distorted. A dark border was seen around the Moon. Just before
re-appearance a sea green colour was noticed. Cameron 2006
catalog extension ID=5 and weight=2-5. ALPO/BAA weight=1.
Theophilus 1972 May 19 UT 23:48 Theophilus observed by Ruchatz (51N
10E, 60mm refractor, T=4, S=2) "Diminution of brightness of the S wall
for a short time" - Hilbrecht and Kuveler, Earth, Moon & Planets, 30
(1984), p53-61.
On 1985 Jun 14 UT 21:16-21:40 Observed by A.C. Cook Frimley, UK,
30cm reflector, seeing IV, transparency moderate, very litle
spectral dispersion noticed - Wratter 25 and 44a filters used)
UT 21:16-21:19 Censorinus slightly brighter in red and more
detail seen. Observed other features before and after this.
Checked again UT21:31-21:40 - same appearance. Torricelli and
Torricelli B in comparison looked normal with other craters of
similar size. ALPO/BAA weight=1.
Proclus NW ray 2003 Sep 03 UTC 02:46-03:07 Observed by Haas (Las
Cruces, NM, USA) "The curious reddish edge to the conspicuous bright
ray running N2 from Proclus is seen again (x321, x366 (S=1-3, T=3.5-
2.5). It lies on the SW side of the ray, with no corresponding blue
border on its NE edge. The effect persists as the Moon drifts across
the whole eyepiece field. However at 03:46 (x202) the coloured edge is
not recognized now, but perhaps only because of worse conditions (S=3,
T=2) 12.5" Newtonian reflector used." The ALPO/BAA weight=3.
On 2010 Apr 20 some time between UT 22:00 and 23:00 I.
Bryukhanov (Minsk, Zeiss Refractor at the Minsk planetarium)
observed an orange-brown tint a little to the west of Zollner
and Kant craters. Apparently images were obtained. ALPO/BAA
weight=1.
Sabine 1967 Sep 11 UT 00:32,00:45 Observers: Jean at al. (27 obs., 21
telescopes, Montreal, Canada, 3-6" refractors, reflectors) "A black,
rectangular-shaped cloud vis. in M.Tranquill, moving W-E (IAU ?) &
dissipated nr. term., surrounded by viol. colour. Bright yellow flash
at 00:45, (obs. in response to request to obs. impact of Surveyor V at
0046) NASA catalog weight=3. NASA catalog ID #1043. ALPO/BAA weight=2.
On 1988 Jul 21 at UT 01:00? an Unknown observer (name and geographical
position not given in the cameron catalog) detected a darkening on the
floor of Proclus crater - this was also seen by other observers - some
of whom were making observations independently. The Cameron 2006
catalog ID=330 and the weight=1.
Posidonius 1969 May 23 UT 11:35-12:45 Observed by Osawa (Hyogo-ken,
Japan, 8" reflector x286) "W.(ast. ?) rim of crater was yellow in
integ. light, brownish to deep yellow in filter, with no blink.
Hue seen thruout obs. (true ground color? or seeing ? or true LTP?)
thin clouds. (Apollo 10 watch)". NASA catalog weight=3 average. NASA
catalog ID #1141.
On 1969 Jul 20 at UT09:30 Whelan (Wellington, New Zealand, 10"
and 6" reflectors. Other observers involved were: Mackrell
(New Zealand, 6" reflector) and Spellman (4" reflector)
observed Maskelyne crater undergoing a whitish glowing
brightening. Shadowy filling of whole crater. Apollo 11 watch.
The Cameron 1978 catalog ID=1179 and the weight=3. The
ALPO/BAA weight=2.
On 1970 Apr 13 at UT09:00-09:03 Whelan (Walters, New Zealand, using a
10" reflector) observed Menelaus to have a deep red cloud that seemed
to surge upward from outside the southern edge of the crater wall and
disperse around the outside edge, spreading out on reaching Mare
Serentiatis. All clear again though by 09:03UT, (Apollo 13 watch).
Drawing supplied. Cameron 978 catalog ID=1246 and weight=3. ALPO/BAA
weight=3.
Alphonsus 1960 Jan 06 UT 18:00 Observed by Warner and Hole (London,
England, 18" refractor and 24" reflector, Moon blink used) "Red spot.
Hole saw this on several other occasions(indep. confirm)." NASA catalog
weight=5 (very good). NASA catalog ID 727.
Near archimedes 2001 Sep 25 UT 08:30 Observed by Try (Whangarei, New
Zealand, 4" f/10 reflector) "observed two possible L.T.Ps. on the edge
of the terminator near the crater Archimedes. They appeared to be two
bright points of light about the size of Mount Piton. They seem to
form a triangle with Mount Piton. He observed them for two hours and
they were still visible when he ended his observing session. He was
observing with a 4" f10 reflector. Then Moon age was 7.9 days old and
the colongitude was 4.83. submitted a drawing showing the area where
the lights were observed." ALPO report. ALPO/BAA weight=1.
Jansen 1966 Aug 24 UT 04:15-04:25 Observed by deBerard (Flossmoor, IL,
USA, 6" reflector, x360, S=V, moonblink used) "Bright green glow --
using red & blue filters & green polariz. filter." NASA catalog weight=
3 (average). NASA catalog ID #965.
On 1988 Jul 22 at UT 02:15-04:00 P.W. Foley (Kent, UK, 11"
reflector) made a sketch of a dark area of the (East) floor of
Proclus that revealed a large anomalous dark region - there
should be no shade here when the sun is at an altitude of above
50 deg!. BAA lunar section archives reveal similar dark shadings
- however on this night it was a different shaped dark area. The
appearance was confirmed by several observers. Foley reported
that the region affected stretched from Proclus to Theophilus.
The TLP was seen in the USA too by D, Darling as early as
01:31UT and by others on his TLP network - brightness
measurements of the "c.p." were 3.5 and the remainder of the
floor was 5.5. However the observers did not all agree on the
same position for this dark area. The Cameron 2006 catalog ID=
331 and the weight=2. The ALPO/BAA weight=2.
On 1941 Jan 06 at UT04:00 Barcroft (Madera, CA, USA, 6"
reflector) saw an anomalous shadow in Arzachel crater. Cameron
1978 catalog ID=482 and weight=3. ALPO/BAA weight=3.
Flash seen in Ptolemaeus (A?) - possibly a meteor. Cameron 1978
catalog weight=1. Cameron 1978 catalog ID=863.
Herschel 2005 Aug 13 UT 00:07-00:29 Observed by Daniel del Valle
Hernandez (Aguadilla, PR, 8"SCT, x225, S=7, T=4) "Interesting
configuration of shadows with umbra and penumbra. Effect seemed to
reduce over time." An ALPO report. The ALPO/BAA report=2.
2009 Apr 13 UT 18:55-20:00 J. Adee (UK) and later A. Jarwaski (UK) saw
Mons Pico to be incredibly bright. Adee reported naked eye visibility,
though this does not show up in later CCD images. Jarwaski saw another
nearby Mt very bright as well. This has been assigned an ALPO/BAA
weight of 1, though I suspect it is just normal for Pico to get quite
bright at sunrise.
Patches of brightness seen in the area between craters Aratus and Joy.
Seemed to the observer to be perhaps slightly brighter than one would
expect - the observer thought that their observation only barely
constitured a TLP but decided to send the report in anyway. This
has been assigned an ALPO/BAA weight of 1.
On 1983 Sep 15 at UT 05:20-05:24 Louderback (South Bend, WA, USA,
8" reflector and 3" refractor, seeing poor) found that the west wall of
Eimmart was unusually bright (8.3) and apparently it was almost as
bright as the "WEBS(of Aris?) at its brightest". The crater was
apparently normal again on Sep 20 and 26. The Cameron 2006 catalog ID=
228 and the weight=3. The ALPO/BAA weight=2.
Proclus 1970 Jul 11 UT 20:35-20:45 Observed by Dean, Jamieson,
Sparks (Ruislip, ------, England, 6" relector x156) "Dean saw
something in Proclus, alerted Jamieson who saw nothing unusual
at 2043h, but tho't Secchi was quite bright. At 2035 Sparks saw
Proc. fluctuate. Red & blue filters showed some reduction in
brightness. E. edge showed darkening, but not as dark as in
shadows. 10 min later, returned to normal. (Sparks confirmed
Dean)." NASA catalog weight=5. NASA catalog ID #1267. ALPO/BAA
weight=3.
1970 Jul 11 UT 20:35-20:45 During a TLP alert for Proclus, Jamieson
saw nothing unusual, but found instead that Secchi was quite bright.
NASA catalog weight=5 (very good). NASA catalog ID #1267. ALPO/BAA
weight=1.
On 1990 May 03 at UT 02:03 D. Darling (Sun Praire, WI, USA, seeing
steady) observed a point of light inside Alphonsus just to the north
of the central peak, along the "center ridge". It was seen again, half
way between the central peak and the noth west rim - along the ridge.
All other features were normal. The Cameron 2006 catalog ID=403 and the
weight=3. The ALPO/BAA weight=3.
On 1989 Jun 12 at UT 21:18-22:25 G. North (Herstmonceaux, UK,
Coude, seeing=V) noted at 21:18UT that Torricelli B was
"barely visible"- possibly this was seeing related. M. Cook
(Frimley, UK, 8" reflector, seeing=IV) found Toricelli B to be
ëxtremely dull - impossible to judge shadows on floor in
contrast to Cens." Holmes (Rockdale, England, UK, 8"
reflector, seeing=II-III) at UT21:30 also found Toricelli B
difficult to find at magnifications less than 200x. Cameron
comments that "Dulling is common on it at high Sun but
illumination doesn't seem to be the cause or related". The
Cameron 2006 catalog ID=365 and weight=5.
The ALPO/BAA weight=2.
Alphonsus 1958 Dec 19 UT 20:00? Observed by Wilkins (Kent, UK)
described in the NASA catalog as: "Reddish patch on central
peak" 15" reflector used. NASA catalog weight=4. NASA catalof
TLP ID No. 711. ALPO/BAA weight=3.
Eratosthenes 1954 May 11 UTC 20:00 Observer: Catermole (UK, 3"
refractor) "Central peak invis. tho surroundings were sharp".
NASA catalog ID #563, NASA weight=4 (high). ALPO/BAA weight=2.
Alpetragius 1889 Sep 4 UTC 02:30-03:00 Observed by E.E. Barnard (Lick
Observatory, CA, USA, 36" refractor x150, x700) "Shadow of CP diffused
& pale. Entire inside of crater seemed filled with haze or smoke. Shad.
of E.wall was black & sharp. CP & floor seen thru haze. No other
craters showed this appear. (date&time rep't=Sep3, 1830L.T)." N.B. Sun
above the horizon at 02:30 - sun sets at Lick at 02:37! NASA catalog
weight=4 (good). NASA catalog ID #264. ALPO/BAA weight=3.
On 1972 Apr 22 at UT 17:30-18:15 Iwanoff (60mm refractor, 1000mm focal
length,transparency 3 out of 5 and seeing 3 out of 5, located at 53deg
5' N and 8deg 45'E) At Censorinus a diffuse bright area, greater than
the crater itself, yellow to white in colour. Published in Hilbrecht
and Kuveler, Moon and Planets, 30 (1984) p53-61. ALPO/BAA weight=1.
Tycho observed by G. North (UK) seen to have greyness
inside parts of its shadow. Confirmed by J.D. and M.C. Cook
Possibly light scattered of illuminated wall into shadow
or highland starting to break through the shadow.
ALPO/BAA weight=2.
On 1988 Jul 23 at UT03:07 D. Darling (Sun Praire, WI, USA, 12"
reflector, x150, seeing = 6/10) discovered that the dark area on the
floor of Proclus, seen earlier by UK observers was still present, but
less so (?) and the shape changed. When viewed through a green filter
it was less distinct. "Change with two other filters. Polarizer gave a
circular shape with a knot on SE side & W58 in White." The measured
brightness of Proclus was 9 on three sides and 8.5 on its west rim. The
floor was 5.5, but the dark spot was 4. Alphonsus, Bullialdus,
Copernicus, Eratosthenes, Plato and Ptolemeaus were all normal. The
Cameron 2006 catalog ID=332 and the weight=1. The ALPO/BAA weight=1.
Plato 1952 Apr 04 UT 02:45 Observer: T.A.Cragg (Mt Wilson, CA,
USA, 31cm reflector, x420, seeing fairly good, transparency
fair) - Obscur. of floor (seen a few hours after Wilkins & Moore
obs. confirm.?) " - indeed Haas in Stolling Astronomer 2002 Vol
45, p29 states that Cragg was amazed to see Plato's floor with
absolutely nothing on it! He was able to draw details elsewhere
in other features. NASA catalog weight=5. NASA TLP ID No. #551.
ALPO/BAA weight=2.
On 1972 Apr 22 at UT 18:58-00:28 Hopp (75mm refractor, 1200mm focal
length,transparency 4 out of 5 and seeing 4 out of 5, located at 52deg
30' N and 13deg 15'E) Censorinus brighter than normal relative to
Proclus. Published in Hilbrecht and Kuveler, Moon and Planets, 30
(1984) p53-61. ALPO/BAA weight=1.
Agrippa 1966 Aug 26 UTC 01:52-02:24 Observer: Bartlett
(Baltimore, MD, USA, 5" reflector x437) "Shadow of C.p. was
grayish, wall shad. was normal black, C.p.itself barely disting.
from floor" S=5, T=3. NASA catalog weight=4 (high). NASA catalog
ID #966. ALPO/BAA weight=1.
Shadow of central peak barely distinguishable.
Residual wall shadow normal black. Landslip very
conspicuous, 10 deg bright. Cameron 1978 catalog
TLP ID=1040 and weight=4. Cameron 2006 Catalog
Extension ID=12 and weight=4. ALPO/BAA weight=2.
On 1974 Mar 3 at UT 19:06-20:20 J-H Robinson (Teighmouth, Devon,
UK, 10" refractor, x200, seeing=poor) got a Moon Blink reaction
on the South east wall of Plato, adjacent to the rim shadow and
alerted the BAA TLP network. Ford reported a negtive result at
19:35UT, although Robinson was still getting a blink reaction at
19:40UT, albeit fainter, red at times. Findlay at 19:43-19:52
and 20:00-20:05 saw nothing unusual. Robinson at 19:56UT no
longer saw a blink, but it returned at 20:05UT. Light in bothred
and blue filters. Not steady, but coming and going and gone at
20:09UT. Moore at 19:59-21:00, kennedy at 20:12-20:30, Taylor at
20:48-21:03 and Fitton at 20:05UT all got negative results. The
latter time coincides with Robinson's second blink reaction.
Cameron 1978 catalog ID=1390 and weight=1. ALPO/BAA weight=1.
On 1988 Jul 24 D. Darling (Sun Praire, WI, USA, 12" reflector,
x150, S=7/10, T=3) observed the following in Proclus: "At 0213
the previously observed gray area was 1/3 of July 22 and V
shaped and fanned out across the floor. Could see hint of knot
seen before. Craters named in 7/23/88 (#319) were all normal
this time too". Is it possible that this report refers to the
crater "Gray" rather than "Proclus" as the column field suggests
in the Cameron catalog? The Cameron 1978 catalog ID=333 and
weight=5. The ALPO/BAA catalog weight=2.
On 1981 Sep 08 at UT 21:28-21:34 P. Madej (Huddersfield, UK, seeing
III-IV and trasnaparency good) observed a light orange transparent
cloud extending from the north east inner corner across over the floor
of Plato. Camero comments that this report was confirmed by 3 othr
observers. The shape of this clud varied. The Cameron 2006 catalog ID=
153 and weight=4. The ALPO/BAA weight=3.
Gassendi 1979 Dec 29 UTC 20:09-22:04 - Observer: Cook (Frimley, Surrey,
UK) "Colour seen - almost certainly spurious colour and not a TLP".
ALPO/BAA weight=1.
Alphonsus - 1966 Aug 27 UTC 06:05-06:25 observed by Haris, Eastman,
Bornhusrt, Cameron, astronet observers (Tucson, AZ, USA - 21" reflector
x200) and by Corralitos observatory (Organ Pass, NM, USA, 24"
reflector) "W. dark-haloed area varying & the small dark-haloed (40%)
area also varying. Seen by others present incl. the author (WBC) who
attributes the variations to "seeing". Not confirmed by Corralitos MB."
NASA catalog weight=1 (low). NASA catalog ID=968.
Ross D area - 1966 Aug 27 UT 06:06-06:25 observed by Harris, Eastman,
Bornhusrt, Cameron, astronet observers (Tucson, AZ, USA - 21" reflector
x200) and by Corralitos observatory (Organ Pass, NM, USA, 24"
reflector) "Obscuration on E. wall, bright area E. of crater at its
brightest. (I (WSC) was present at obs. but did not note anything not
attributable to bad seeing, but am not familiar with the area in normal
aspect. Others present did not see anything unusual, but Bornhurst &
Eastman confirmed). Corralitos Obs. found due to changing light
conditions. NASA catalog weight=1. NASA catalog ID=967.
ALPO/BAA weight=1.
On 1991 May 24 at UT 20:00? Romualdo Lourencon (Sao Paulo,
Brazil, 60mm refractor, seeing=III) detected a circular cloud in
Jansen B and H? (Gazateer report says F and K). "The crater of
the event 100km diam. compared to Copernicus, dark with crescent
obscured region below it. Was S of Jansen. A circular depression
there was before LTP in darkness. Wonders if circ. depr. was
shadow of cloud? The Cameron 2006 catalog ID=428a and the
weight=3. The ALPO/BAA weight=1.
On 1988 Jul 25 at UT03:15 H. Davis (Madison, WI, USA) stated that
Proclus was normal apart from a "slightly darker area in SW (Ast) SE
(IUE) corner." The Cameron 2006 catalog ID=334 and the weight=0. The
ALPO/BAA weight=1.
On 1975 Mar 23 at UT 20:40 P.W. Foley (Kent, UK) found a brownish
colour on the north west wall. This is a BAA Lunar Section report. The
ALPO/BAA weight=2.
Bullialdus 1979 Oct 31 UT 20:20-20:30 G.W. Amery (Reading, UK)
observed a plateau area to be dark and distinct in blue light
(Wratten 44a), but only just visibly in red (Wratten 25) and
yellow light. Observer wonders if this is natural surface
colour? ALPO/BAA weight=1.
On 1992 Mar 16 at UT 00:39-01:14 D. Weier (Sun Praire, WI, USA, 11"
reflector) at 00:39UT noted some soft, diffused, faint ïllumination
within the shadow projected over the Cobra Head area, though it had a
sharp appearance to the edge of the shadow. D. Darling (Sun Praire, WI,
USA, 11" reflector) was taking photographs from UT 00:51 and making
drawings and visual descriptions. The first 3 photographs in the
sequence have the crater as normal. Four other photographs reveal an
abnormality. Seeing conditions were excellent and a great deal of
surface detail was seen inside Aristarchus crater - however the
apeparance of the Cobra's Head was "washed out" and again shadows near
to this were illuminated. The NASA catalog ID=442 and the weight=5. The
ALPO/BAA weight=3.
On 1993 Apr 03 at 23:39UT C. Adams (FL, USA, 24" reflector, x168)
noticed a "translucent orange" colour in Gassendi crater within a 35deg
sector (apex at the centre) - row of 3 central peaks extending west -
the western central peak appeared as a dome with a summit craterlet.
The Cameron 2006 catalog ID=450 and the weight=3. The ALPO/BAA
weight=3.
On 1993 Apr 03 at 23:39UT D. Weier (Sun Praire, WI, USA, 7x50
binoculars) observed 2 flashes within the Proclus crater. The Cameron
2006 catalog ID=450 and the weight=3. The ALPO/BAA weight=2.
On 2001 Aug 30 at UT20:35-21:15 C. Brook (Plymouth, UK) found a dimming
in the central peak of Alphonsus, however it had returned to normal by
Aug 31 UT 00:29-00:50UT when A.C. Cook (Alexandria, VA, USA, 8"
reflector) examined the area, though there were some slight brightness
variations that were attributed to seeing conditions. The ALPO/BAA
weight=2.
Hislop of England? saw Aristarchus as nebulous at the centre, despite
the fact that elsewhere features were well defined. The Cameron 1978
catalog ID=246 and the weight=3. The ALPO/BAA weight=2.
Cavendish 1956 Jan 24 UTC 20:34-20:45 Observed by Houghton and Warner
(England) "Variable flashes seen from W. inner(?) wall of crater, then
a little inside the terminator. Flashes began with a bright glare at
20:34, were very bright for ~3 min, then faded. Flash rate
approximately every 1.5 sec. Other point like peaks did not flash. Also
indications were seen of reflections of flashes from E. (inner?) wall
and the crater's floor was faintly lit by a glare. Ref: Strolling
Astronomer p27, Vol 45, 2003. 17cm reflector x230. Seeing good-
excellent. NASA catalog assigns this observation a weight of 4 (good).
NASA TLP ID No. #631.
On 1985 Jun 29 at UT 22:56 M.C. Cook (Frimley, UK, seeing poor)
observed that Torricelli B looked as bright as a mountain to its south
west - no colour was seen. Cameron comments that this was similar to
Marshall's 1985 Jul 1 observation. The cameron 2006 catalog ID=278 and
the weight=3.
E. of Picard 1948 Aug 16/17 UTC 22:30-02:26 Observed by Moore & Baum
(Chester, UK) described in NASA catalog as: "2 areas E. of Picard
appeared featureless. Cloud-like patches, 12(?)inch reflector. NASA
catalog weight=4 (high). NASA catalog ID No. #509.
Alphonsus 1966 Aug 28 UTC 06:00-08:00 Observers from Astronet (Tucson,
AZ, USA). NASA catalog states: "Brightenings in 2 dark patches & near
fainter (40%) dark patch (40% of way from the c.p. to W. wall). 21"
x200 reflector used. NASA catalog weight=2 (poor). NASA catalog TLP ID
No. 969.
Promontory LaPlace 1977 Jan 31 UT 20:49-23:00 Observed by Foley
(England, 11.75" reflector, x360), Prout (England, 4" refractor or
reflector?), Findlay (Dundee, Scotland, 10" reflector, x180, S=VG),
Ford (Dundee, Scotland), Mooney (Dundee, Scotland) "With filters in
eyepiece, tho't he saw a possible darkening in the blue but no
variation in red. Altho. a deep shadow is normal to the W. of the cape
at this period, (then cape must have a slope > 30deg!). he wondered if
shad. was more extensive than usual? Prout noted a dark inky coma-
shaped spot. Dundee obs. concluded it was a shadow. Took photos.
Analysis of them was underway at time of rep't." NASA catalog weight=5
(very high). NASA catalog ID #1462.
Herodotus 2002 Sep 18 UT 22:00 Observed by Raffaello Lena (GLR,
Italy). Event described was of two pseudo-peak/hill-like
features, one on the southern floor of the crater, and another
just slightly to the NW of the centre. on the southern
floor of the crater. Lena suspects a combination of seeing
effects and albedo markings on the floor. However this effect of
two spots on the floor has not been repeated again.For further
information, theory, and a sketch please see Fig
5 in this web link:
http://utenti.lycos.it/gibbidomine/analisi123.htm ALPO/BAA
weight=2.
On 1975 Mar 24 at UT19:08-19:45 P.W. Foley (Kent, UK) observed blueness
in the North East (Classical?) corner of Aristarchus. Moon blink seen -
pale in red. Most other observers clouded out. The ALPO/BAA weight=3.
Aristarchus 2014 Dec 04 UT 03:14-03:15 M.P. Homan (Grand Rapids,
MI, USA, Nikon P520 x48) 11 digital images taken. These show
possible blue colour in the Aristarchus area e.g. on the ray
between Herodotus an Aristarchus. ALPO/BAA weight=1.
Aristarchus 1972 Apr 25 UTC 19:15-19:20 Observer Ventzke (located at
48.67N, 12.00E) - diffuse brightening on inner N. wall, reddish. 60mm
refractor used. Ref. p53-61 of Hilrecht & Kuveler Moon & Planets vol
30, 1984.
Aristarchus, Herodotus - 1967 Sep 16 UTC 23:50-23:55 observed by
Seeliger (Dresden, Germany, 30" reflector, 90, 140x) "Dark streaks on
E.(ast. ?) outside walls of both craters. No shadow from Herod. wall.
Drawings (wall < 18 deg slope if no shadow normally)." NASA catalog
weight=3 (average). NASA catalog ID=#1044.
On 2010 Apr 27 at UT 00:10-00:30 and 01:45-02:00 P. Grego (St
Dennis, UK, 20 and 30cm reflectors) noticed a craterlet just
to the east of Briggs and an E-W trending lineament or wrinkle
ridge that did not show on NASA LAC charts. Further checks did
not reveal it on Lunar Orbiter mosaics, but the craterlets
(and not the E-W trending ridge) were visible in LROC
topography data. The ridge is possibly a very low relief
feature that shows only under very shallow illumination
conditions. The ALPO/BAA weight=1 until we get confirmation at
repeat illumination.
Plato 1976 Jan 14 UT 20:50 Observed by J.H-Robinson (Teignmouth,
UK, 26cm Newtonian, Wratten 25 and 44a filters, x200, seeing
fair to poor). The Plato floor patches were clearer in red than
in blue light. ALPO/BAA weight=1.
Schickard 1944 Aug 31 UTC 21:00? Observed by Wilkins (Kent, England)
described in the NASA catalog as: "Saw a mist in it which was gone next
nite. interor was dotted with white spots, contrasting sharply with
dark areas. All very clear on Aug 15 at sunset". 8.5" reflector. NASA
catalog weight=4 {high). NASA catalog TLP ID No. #492. ALPO/BAA
weight=3.
On 1975 Mar 25 at UT18:50-20:50 P.W. Foley (Kent, UK) observed
blue/grey in Aristarchus. The ALPO/BAA weight=1.
On 1983 Sep 20 at UT 05:08-06:13 Louderback (South Bend, WA, USA,
3" refractor, x150, seeing poor and chromatic aberation on the limb)
detected "purple"in the vicinity of Aristarchus crater and this was
stongest on the north and north west external rims, however there was
no "violet glare"from inside the crater. However the region of the
central peak was very bright - though he could not detect the central
peak. The brightness of the TLP was 4.5 and it should normally be 3
(nimbus area). Near the "big plain"it was 7. The chromatic aberation
seen on the crater. There was also violet on the northen wall of
Herodotus crater and the Cobra Head. Ït appeared dark blue in the blue
filter", the surrounds remained gray". Apparently on the 26th the"ring
was still dark with faint violet - nearly normal". Cameron comments
that the TLP was due to spurious colour. The Cameron 2006 catalog ID=
229 and the weight=3. The ALPO/BAA weight=2.
On 1975 Mar 25 at UT19:59-20:02 P.W. Foley (Wilmington, Dartford, Kent,
UK, 30cm Newtownian) observed blueness along the inner southern wall of
Plato. This is a BAA report. The ALPO/BAA weight=1.
On 1985 Jul 01 at 02:00-03:00 UT K. Marshall (Medellin, Columbia)
observed thatTorricelli B was very bright - verified using a C.E.D. No
colour was seen though. the Cameron 2006 catalog ID=279 and the weight=
4. The ALPO/BAA weight=3.
On 1980 Jan 01 at UT 00:10-00:21 A.C.Cook (Frimley, UK, 12" reflector,
Wratten 29 and 44A filters, Seeing II-III and transparency poor-
moderate) suspected that the floor was slightly brighter in blue light
than in red. No such effect was seen earlier at 23:54-23:57. Cameron
2006 catalog ID=81 and weight=3. ALPO/BAA weight=1.
Plato 1938 Feb 14 UT 00:25 Observed by Fox (Newark, England,
6.5" reflector, x240) "Prominent gold-brown spot on E. wall
with yellow glow without definite boundary, spreading over
floor." NASA catalog weight=3. NASA catalog ID #431. ALPO/BAA
weight=3.
Aristarchus 1950 Jun 29 UT 05:20-05:41 Observed by Bartlett
(Baltimore, MD, USA, 3.5" reflector x100, S=6, T=5) "Strong
bluish glare on E..SE wall." NASA catalog weight=4. NASA
catalog ID #529.
(65E, 56N) near Endymion & Mare Humboldt 1968 Jun 10 UT 02:35 Observed
by Provenmire, Robinson et al. (Hamburg, PA, USA, 6" reflector x105,
Seeing=good, alt=20deg) "While waiting for reappearance of Antares from
a grazing occultation at 13+/-4deg P.A. saw a prolonged blue flash
lasting from minimum of 1/2 to a max. of 2.0 s. Several others along
obs. path of several miles also saw it so not a local phenom. (located
38 deg from cusp, azimuth=157 deg?)" NASA catalog weight=5 (very good).
NASA catalog ID #1078.
On 1977 Dec 24 at UT 19:30-23:20 P.Foley (Kent, UK, 12" reflector).
CED Brightness changes were noted in the central peak and the west
wall. The following features remained relatively steady in comparison:
Proclus, Mon Pico north peak, Mons Piton and Censorinus. Cameron 2006
catalog ID=19 and weight=4. ALPO/BAA weight=3.
On 1963 Nov 01/12 at UT 22:30-03:00 P. Moore (UK, 12" reflector)
observed something unusual in Aristarchus/Copernicus/Kepler -
the Cameron catalog is not very clear which. The Cameron 1978
catalog ID=779 and weight=5. ALPO/BAA weight=1.
On 1963 Nov 01 at UT 00:20-00:35 Kopal and Rackham (Pic du
Midi, France, 24" reflector) observed in Kepler an
enhancement in red light at 672.5nm and 545.0nm. Luminescence
~86% +/-3% of background. According to the Cameron catalog,
Moore(12" reflector, UK) noted something unsual between 22:30
and 03:00 but this might apply to Kepler, Coperncius, and/or
Aristarchus and that was seen 23:30-03:00? - the catalog is not
very clear. The Cameron 1978 catalog ID=779 and weight=5. The
ALPO/BAA weight=4.