On 1970 Aug 05 at UT 23:00-23:30 Celis (Paso Hondo, Chile, 3"
refractor, x60, x100, x135, seeing=good?) saw the same characteristics
in Aristarchus as had been seen the previous night, but of lower grade
intensity. Somewhat difficult to see because of the small crescent..
The Cameron 1978 catalog ID=1270 and weight=1. The ALPO/BAA weight=1.
On 1825 Jan 23 at UT 02:00 Engineering officers on board HMS Coronation
(Gulf of Siam, naked eye or spy glass?) observed a star like point in
Aristarchus crater. The Cameron 1978 catalog ID=105 and the weight=5.
The ALPO/BAA weight=2.
On 1970 Aug 05 at UT 23:00-23:30 Celis (Paso Hondo, Chile, 3"
refractor, x60, x100, x135, seeing=good?) saw the same characteristics
in Aristarchus (bright patches with electric blue colour) as had been
seen on Aug 04, but the intensity was less. The Cameron 1978 catalog
ID=1271 and weight=1. The ALPO/BAA weight=1.
On 1950 Apr 22 at UT 03:15-0440 Barcroft (Madera, CA, USA, 10"
reflector x74 & x98) observed that Aristarchus glowed in
Earthshine. However Earthshine visibility was exceptionally
good. The Cameron 1978 catalog ID=526 and weight=3. The ALPO/BAA
weight=1.
On 1970 apr 11 atUT 05:29 Lucas (San Diego, CA, USA, 10" refelctor,
seeing=fair) and others (Oregon, USA) obtained a photometric record of
light level changes in Grimaldi crater. Visible reports by others
during the same time. The photometer paper chart pen moved off scale on
a 10mV scale adjusted to 1000mV. The peaks correlate with the visible
observers from California and Oregon. Bright flashes, 3-5 events
(confirmation during the Apollo 13 watch). The Cameron 1978 catalog ID=
1237 and weight=5. The ALPO/BAA weight=4.
On 1903 Mar 03 at UT 18:30 Rey (Marseilles, France) observed a star-
like point of light in the Aristarchus region, on the dark part of the
Moon (indep. confirm?). The Cameron 1978 catalog ID=315 and the weight=
5. The ALPO/BAA weight=2.
On 1988 Mar 23 at UT 01:15-01:30 M. Wisniewski (Chicago, IL, USA, S=F)
observed that Aristarchus was the brightest (mag 5), and only feature
visible in Earthshine. It had the appearance of a steady blue-white
star like point. Darling (Sun Praire, WI, USA) though observed other
features as well: Proclus, Theophilus, Cyrillus and Censorinus - all of
which were normal. The cameron 2006 catalog ID=319 and the weight=0.
The ALPO/BAA weight-1.
Theophilus 1971 Mar 02 UT 20:30-22:50 Observed by Ringsdore
(Stoneleigh, England, 15" reflector, x360, seeing=good)
"Suspected TLP on c.p. 2 other obs. did not confirm. Orange-
pink glow. Faded for 10 min then reappeared." NASA catalog
weight=2. NASA catalog ID 1286. ALPO/BAA weight=1.
In 2005Apr14 at UT18:32.5 +/-2.5 min A.Brosio (Rosarno (Reggio
Calabria, Italy, Latitude: 38d 29' N, Longitude: 15d 58'E, 152mm
reflector, x75) observed a small square form in Earthshine near
Archimedes. This is a UAI observation.
Bright spot seen. The Cameron 1978 catalog
gives this TLP an ID No. of 36 and a weight
of 1. The ALPO/BAA catalog weight is also 1.
1948 Oct 08 UT 21:00? Barker's Quadrangle (SE Mare Crisium)
Observer: Moore (UK, 12?" reflector) "Nebulous white patch in
place of quadrangle. (In Capuanus ? See Wilkins & Moore, The
Moon, p124. Area in darkness" NASA catalog ID #511. NASA catalog
weight=4. ALPO/BAA weight=3.
On 1962 Sep 05 at UT 00:48-00:55 Chalk (USA?) observed in the
vicinity of Walther a faint point of light, near the
terminator. Cameron suspects an illuminated peak in the dark.
The Cameron 1978 catalog ID=767 and weight=1. The ALPO/BAA
weight=1.
A German observer by the pseudonym of "R" on 1883 Nov 05 UT 18:00 saw
Aristarchus as a vry bright 7-8th magnitude star in the dark part of
the Moon. The Cameron 1978 catalog assigns this event an ID of 240 and
a weight of 3. The ALPO/BAA weight is 1.
Macrobius 1939 Oct 19 UT 02:00? Observed by Barcroft (Madera, CA, USA,
6" reflector) "Reddish-brown hue (unusual) usually absent" NASA
catalog weight=2 (low). NASA catalog ID #463.
Mare Nectaris 1880 Jan 18 UT 20:00? Observed by Gaudibert (France?,
seeing poor) "Whole of sea was foggy. Fog extended into Fracastorius.
Gruithuissen said seeing was unsatisfactory" NASA catalog weight=0
(very unreliable). NASA catalog ID #216. ALPO/BAA catalog weight=1.
On 1964 Jul 16 at 03:55-04:10UT Cragg (Mt Wilson, CA, USA, 6"
reflector, x180, seeing 7, transparency 6) observed a pseudo hill
(700m high) some 3 km in diameter and casting a shadow, south
east of Ross D. The Cameron 1978 catalog TLP ID=830 and the
weight=4. The ALPO/BAA weight=3.
Madler 1971 Mar 03 UT 21:30-21:45 J Andrews (Christchurch, UK,
8.5" reflector, x240, seeing I) observed a red fan shaped area to
the south of Madler - it covered part pf the mountainous area to
the south. The colour started fading at 21:45UT and had gone
within 5 minutes. ALPO/BAA weight=1.
Near Theophilus - south of Madler - 1971 Mar 03 UT 21:30-21:35, 21:47
Observed by Hedley-Robinson (England, 3.75" refractor, x164, S=G,
steady haze) "Reddening in a fan form on bright area of that
formation, but red did not extend fully over it. Blink patrol started
at 2005h but no red till 2130h. Definte blink at 2147h" NASA catalog
weight=3 (average). NASA catalog ID #1287.
On 1984 Jun 05 at UT20:00 Marshall (Covington, UK) saw an unusual
darkening on the floor of Proclus and irregular shape. The Cameron 2006
catalog ID=243 and the weight=2. The ALPO/BAA weight=1.
Torricelli 2011 Dec 31 UT 16:39-17:00 R.Braga (Milan, Italy,
80mm refractor) found the north rim or Torricelli to be very
bright at the start of the observing session but dimmed
considerably at around 17:00UT. Observer not sure on the
normal appearance of this crater. ALPO/BAA weight=2 followinf
repeat illumination images in the 2021 Apr ALPO TLO..
Noble (England?, seeing=fair) observed a badly defined white patch east
of Picard. Cameron 1978 catalog ID=201 and weight=3. ALPO/BAA weight=2.
Godin, Agrippa, Mare Crisium, and Webb's spot.... 1882 Apr 24
UT 21:30-22:00 Observed by Ridd (England?) "Shadow anomalies-
strange appearance. (he often noticed appear. that could only
be haze. Shadows blurred and oscillated. Shadows in Aristotles
were steady. E. of Agrippa shadows were misty as the foggy
which lifted & then became obscur. again. Intervals being 1o
min. (not terr. atmos.). Shadows never became clear whole time
of obs. Also saw a white spot NW of 5 on Nelson's map (Webb's
spot). " NASA catalog weight=2. NASA catalog ID #231. ALPO/BAA
weight=2.
Godin, Agrippa, Mare Crisium, and Webb's spot.... 1882 Apr 24
UT 21:30-22:00 Observed by Ridd (England?) "Shadow anomalies-
strange appearance. (he often noticed appear. that could only
be haze. Shadows blurred and oscillated. Shadows in Aristotles
were steady. E. of Agrippa shadows were misty as the foggy
which lifted & then became obscur. again. Intervals being 1o
min. (not terr. atmos.). Shadows never became clear whole time
of obs. Also saw a white spot NW of 5 on Nelson's map (Webb's
spot). " NASA catalog weight=1. NASA catalog ID #231.ALPO/BAA
weight=1.
Godin, Agrippa, Mare Crisium, and Webb's spot.... 1882 Apr 24
UT 21:30-22:00 Observed by Ridd (England?) "Shadow anomalies-
strange appearance. (he often noticed appear. that could only
be haze. Shadows blurred and oscillated. Shadows in Aristotles
were steady. E. of Agrippa shadows were misty as the foggy
which lifted & then became obscur. again. Intervals being 1o
min. (not terr. atmos.). Shadows never became clear whole time
of obs. Also saw a white spot NW of 5 on Nelson's map (Webb's
spot). " NASA catalog weight=1. NASA catalog ID #231. ALPO/BAA
weight=1.
On 1982 Jul 27 at UT 20:04 P. Madej (Newsome, Huddersfield, UK, 16cm
reflector, x33, seeing I to II, transparency fair, Hoya linear type
polarizer filter) observed that when the filter was used on Mare
Crisium, that the north part became a bright gray when turned to 45deg,
but when turned the other way it returned to normal. The ALPO/BAA
weight=3.
On 1994 Apr 18 at UT14:40 C.D. Hua (China) found that the wall of
Picard had changed to dark. The ALPO/BAA weight=1.
Ptolemeus 2020 Jul 27 UT 23:00 N. Travnik (Brazil) observed
visually for 2nd time ever (first seen back in 1970), an
effect on the floor of this crater at local lunar sunrise:
"kind of glimmering mist lifted and wafted inside the shady
hollow of the crater". Almost certainly this is a combination
of atmopsheric seeing on the narrow shadow spires, but we
would like observers to look at this visually or obtain time
sequence images to try to replicate this effect. This report
is assigned an ALPO/BAA weight of 1 for now.
On 1993 May 28 at UT 21:02-21:30 M.C. Cook (Frimley, UK, 3.3" Questar
telescope, x80-x130, atmosphere hazey - poor transparency) noticed that
the east side rims were slightly fuzzy and suspects that this might
have been due to the illumination angle. A.C. Cook (Frimley, UK)
obtained some CCD images that revealed that the effect was to some
extent still there one hour later. The Cameron 2006 catalog ID=461 and
the weight=5. The ALPO/BAA weight=2.
Mare Vaporum 1969 Apr 24 UT 19:34 Observed by Bentley (England,
8" reflector, x320, S=E) "NW part of mare obscured for 4 min.,
gradually thinning." NASA catalog weight=3. NASA catalog ID No.
1123. ALPO/BAA weight=2.
Large plume-like diffuse cloud over central peak, very
large compared to central peak (@ approx 30km diameter)
with intensity much different from other parts. Brightness
between walls and shadowed floor. Would take 3 minutes to
collapse, so continuously fed. 13-14 days later, at SS,
central peak was normal. Kuiper took photos after Kozyrev's
observations, but saw nothing abnormal. Drawing. Haas saw
nothing in 12inch reflector at the time. Cameron 1978
catalog TLP ID=705 and weight=4. ALPO/BAA weight=2.
Alphonsus 1966 Jun 26 UT 04:30-04:40 Observed visually by
D.Harris and E.Arriola (Whittier, CA, USA, 19" reflector x146,
and spectrum, S=4, T=1-0) "Absorp. spectrum (visual) of c.p.
band at 475+/-5nm (1st est.); 2nd est. at 485+/-5nm. Band
degraded towards the viol. Band nr.Hydrogen Beta. as if
abnormally broadened. So sign of anything unusual visually in
central peak in white light. Absorption appeared only on C.P.,
not over walls. Calibration corrections put band at 491+/-4nm"
NASA catalog weight=5. NASA catalog ID #948. ALPO/BAA weight=5.
On 1985 Oct 11 at UT 04:56-05:12 D. Louderback (South Bend, WA, USA,
4" refractor, x95, seeing=1-2-1 and transparency=4) detected a change
in brightness of Mons Piton point D (his designation) during 04:56-
04:59. The whole of the east slope was affected - initially bright and
then faded and there was a blue colour (detected with filters). The
variabilty was 8-11sec (Cameron suspects atmosphere as the altitude was
low). The brightness stabilized at 05:12UT, but variability resumed
until observing finished. As a comparison Aristillus was not seen to
change. The Cameron 2006 catalog ID=287 and the weight=1. The ALPO/BAA
weight=1.
A dome-like feature, sketched by Herring and confirmed in a photograph
by Larson. This had not been seen before by Herring in hundreds of
hours of observing. No other reports of this. The photograph was taken
at 02:50h. Cameron 1978 catalog ID=878 and weight=5. ALPO/BAA weight=3.
On 1988 Mar 26 at UT20:00 M.C. Cook (Frimley, UK, Frimley, UK, 12"
reflector, seeing=III) reported Cenosrinus to be "foggy/fuzzy" and this
this effect was not seen in other adjacent regions. The cameron 2006
catalog ID=320 and weight=4. The ALPO/BAA weight=2.
On 1981 Aug 09 at UT05:08-05:21 D. Louderback (South Bend, WA, USA, 3"
refractor) found that the bright patch in the southern part of Eimmart,
could only be seen well in red light (this is between A, C and D in his
feature notation) i.e. 5 brightness values higher than in white or blue
light. Indeed in white light this bright area was closer to the east
wall bright spot. The Cameron 2006 catalog ID=149 and weight=4. The
ALPO/BAA weight=2.
Cusps 1941 Mar 07 UT 04:00? Observed by Barcroft (Madera, CA, USA, 6"
reflector) "Prolongation suspected. (date reported =6th, but if loc.
time =7th UT). In this case we have assumed the 7th" NASA catalog
weight=1 (very low) NASA catalog ID #485.
Cusps 1941 Mar 07 UT 04:00? Observed by Barcroft (Madera, CA,
USA, 6" reflector) "Prolongation suspected. (date reported =6th,
ut if loc. time =7th UT). In this case we have assumed the 7th"
NASA catalog weight=1 (very low) NASA catalog ID #485. ALPO/BAA
weight=1.
Apr 25 UT 20:20 Observed by Bentley (England, 8" rteflector
x320, S=VG) "Flashing star-like pts, in area beyond the
terminator, (atmosphere?)" NASA catalog weight=1. NASA catalog
ID #1124. ALPO/BAA weight=1.
On 1994 Apr 19 at UT 22:00 R. Knopp (Berlin, Germany) noticed a
darkening of the interior of the crater Atlas. The ALPO/BAA weight=1.
Plato 1937 Dec 12 UT 16:45-21:00 Observed by Barker (Chestnut,
England, 12.5" reflector x420) and Fox (Newark, England, 6.5"
reflector, 24?x) "Strong streak of orange-brown on E.wall. Floor
nearly clear of shad. composed of many veins & thin streaks
interwoven. At 21h irreg. extension seen spreading eastward down
wall. Confirmed by Barker's younger son. NASA catalog weight=5
(very high). ALPO/BAA weight=4. NASA catalog ID #428.
Peirce A 1927 Dec 03 UT 22:00 Observed by Wilkins (England, 15"
reflector) "Invisible (date in MBM) is wrong, would be only 6h before
NM. Sunrise on crater is at 3d & ? h. No interposition of dates works
e.g. 13th or 1926 or Dec 26 1923. Only Dec 3 1927 is feasible as it
would be just after 1st Q. & more similar to the May obs.)" NASA
catalog weight=4? NASA catalog ID #396. ALPO/BAA weight=2.
On 1988 Mar 27/28 UT23:30-00:30 M.C. Cook (Frimley, UK, 12" reflector)
found Censorinus to have a "foggy/fuzzy" appearance that was not seen
in adacent areas. The Cameron 2006 catalog ID=321 and weight=4.
ALPO/BAA weight=2.
On 1988 Mar 27/28 at UT 23:30-00:30? M.C. Cook (Frimley, UK, 12"
reflector) noted that the crater Proclus was bright visibly, but the
CED brightness measurement gave the same brightness as Censorinus
crater. The Cameron 2006 catalog ID=321 and the weight=4. The ALPO/BAA
weight=2.
SE of Ross D 1966 Oct 24 UT 03:17 Observed by Cross (Whittier,
CA, USA, 19" reflector, x300, S=3-5, T=3-4) Ross D activity at
level 5. ALPO/NAA weight=1 as it is not mentioned in the Cameron
catalog.
In 1962 Sep 09 at UT 01:42-02:00 Bartlett (Baltimore, MD, USA,
5" reflector, x180, S=5-4, T=3) observed in Agrippa the shadow
of the central peak to be grayish, not much darker than the
floor, estimated at 3deg bright, whereas on 1962 Jul 12, at col
28deg, in the 5" telescope the dhadow was anormal black and
sharply defined against the floor which was 3 deg bright. The
Cameron 1978 catalog ID=768 and the weight=4. The ALPO/BAA
weight=2.
On 1986 May 18 at UT 20:45-22:25 M. Mobberley (Suffolk, UK, seeing II-
IV) found that the central craterlet of Plato was an ëasily seen "white
splodge" although it was quite difficult to see when imaged with video.
Foley and Cameron comment on IR sensitivity of the CCD camera used. The
Cameron 2006 catalog ID=285 and the weight=1. The ALPO/BAA weight=1.
On 1989 Jul 14 at UT 03:28 D. Darling (Sun Praire, WI, USA) found a
darkening in the crater Proclus, but the shadow seen by Cook and Moore,
from a few hours earlier was not seen. The Cameron 2006 catalog ID=371
and the weight=2. The ALPO/BAA weight=1.
Sinus Iridum 2004 May 29 UT 20:44 Observed by Clementelli (Rome, Italy,
102mm diameter Vixen refractor 80-160x, sky conditions: clear, no wind)
"A blue/violet streak, lasting ~10 minutes was seen on the floor of
Sinus Iridum between crater Bianchini and Promontorium Heraclides. The
suspect TLP mybe an effect of instrumental achromatic aberration, but
there is the small possibility that the effect was real." A UAI
observational report. The ALPO/BAA weight=1.
Archimedes 1979 Oct 01 UT 20:57-21:00 Observed by Cook (Frimley, UK,
13mm Monocentric + Barlow eyepiece, Seeing IV, transparency: thin
cloud) "Red seen on east, blue seen on west - almost certainly spurious
colour".
Bullialdus 1979 Oct 01 UT 21:04-21:07 Observed by Cook (Frimley, UK,
13mm Monocentric + Barlow eyepiece, Seeing IV, transparency: thin
cloud) "Red seen on east, blue seen on west - almost certainly spurious
colour". ALPO/BAA weight=1.
Plato 1967 May 20 UT 01:13 K.Simmons (Jacksonville, FL, USA, 10"
reflector) observed a large bright (intensity 6.5) oval area on
near the central floor. According to Ricker and Kelsey (ALPO
selected area coordinators) this is unusual. ALPO/BAA weight=1.
On 1980 Aug 21 at UT20:00 J.H. Robinson (Teighmouth, Devon, UK)
detected colour, using a Moon Blink device, and "mistiness" on the
southern floor of Tycho crater. The seeing was poor! Cameron 2006
catalog ID=104 and weight=1. ALPO/BAA weight=1.
On 1991 Feb 25 at UT 01:26-01:49 D. Darling (Sun Praire, WI, USA,
12.5" reflector, x248, seeing=10/1, transparency=good) found
Gassendi's western rim to be bright in red and diffuse in blue
light. A sketch was provided. The Cameron 2006 catalog ID=420 and
the weight=4. The ALPO/BAA weight=2.
SE of Ross D 1966 Oct 25 UT 03:46 Observed by Cross (Whittier,
CA, USA, 19" reflector, x300, S=2-4 (sometimes 5), T=3-4) "Large
bright area obscuring 1/2 of Ross D crater wall. Not present Oct
24" NASA catalog weight=3 (average). NASA catalog ID 986.
Actually some activity was observed the fay before according to
the original notes. ALPO/NAA weight=2.
Archimedes 1973 Jun 11 UTC 21:05-21:15 observed by Pasternak (53deg
20'N, 7deg 30'E, 75mm reflector) "Faint red area at the E of Archmedes,
diminution from 21.10-21.15UT" - Hilbrecht and Kuveler, Earth, Moon &
Planets, 30 (1984), p53-61
On 1963 Nov 27 at UT 03:00 Olivarez (New Jersey?, USA, 17" reflector)
and Fisher (Colfax, CA, 8" reflector, x300) observed a red glow in
Anaximander in the dark part of the Moon. The Cameron 1978 catalog ID=
784 and weight=5. The ALPO/BAA weight=3.
On 1963 Nov 27 at UT 03:00 Olivarez (New Jersey?, USA, 17"
reflector) observed a red glow in Aristarchus in the dark
part of the Moon. The Cameron 1978 catalog ID=
784 and weight=5. The ALPO/BAA weight=3.
Om 1987 Sep 04 at UT 03:00 J. Caruso (Middletown, CT, USA, 3"
refractor, x155, S=6/10 and T=8/10) found that Bianchini G was not
visible, however Heraclides E, Helicon G, and indeed many other smaller
craters could be seen. There were two small mountains in the general
area of Bianchini G. and a mare ridge - all these were clearly seen.
Caruso states that Bianchini G should normally be much more clearly
seen than the other features mentioned and is the same size as
Heraclides E. The Cameron 2006 catalog ID=305 and the weight=3. The
ALPO/BAA weight=1.
Aristarchus 1880 Jan 23 UT 20:00? Observed by Trouvelot
(Meudon, France) "Luminous light like a luminous cable or
shining wall". NASA catalog weight=3. NASA catalog ID #217.
ALPO/BAA weight=2.
Gassindi 1966 Oct 25 UTC 22:30-23:10 Observed by Moore and
Moseley (Armagh, Northern Ireland, 10" refractor) and Sartory
(England, 8.5" ? reflector) "2 faint blinks (Eng.) on NW (IAU
?) wall. (Indep. confirm.?). NASA catalog weight=5. NASA
catalog ID #987. ALPO/BAA weight=4.
On 1967 May 20 at UT 21:05-21:20 Kelsey (Riverside, CA, 8" reflector,
x300) using an English Moonblink device found colour on the south west
part of the floor. Note that for the times given by Cameron, the Moon
was below the horizon from California - so possibly these are local
times and these times need to be correctly converted into UT? The
Cameron 1978 catalog ID=1037 and weight=3. The ALPO/BAA weight=1.
On 1983 Jul 21 at UT 21:02-23:18 P.W. Foley (Kent, UK, 12" reflector,
seeing=III) found the region around the cleft on the souther rim to be
out of focus - however atmospheric conditions were turbulent until
23:18UT. An unsual dark triangular region (long base against rim) was
seen to extend from the inner rim at 12 o'clock onto the floor for 13-
16km. The crater had lots of detail elsewhere. M. Cook (Frimley, UK)
found the south east to soth west to be obscured again, but not as
badly as she had seen on the 20th July. J. Cook (Frimley, UK) found the
dark region had 2 white bands on the side and the south west wall was
blurred like it was on the 20th July - this time tough colour was not
present. There were also two light patches on the floor. Mosely
(Coventry, UK) observed the south wall at x120 and found the wall out
of focus at the 11 o'clock location. Through a yellow filter he saw a
"white mistiness: on the top of the southern rim and only the south
east cleft could be seen (no colour). By 22:40-23:00 the effect had
cleared up. No dark triangular patch was seen. When Marshall (Surrey,
UK) observed (22:30-03:00) nothing unsual was seen, though a sketch
provided shows a light patch on the floor located at 11 o'clock. All
observations, made by all observers had some atmospheric turbulence,
however trsnparency was good. The Cameron 2006 catalog ID=225 and the
weight=5. The ALPO/BAA weight=3.
Aristarchus 1971 Mar 08 23:00-23:10 Observed by Lyttle (Northern
Ireland, 6" reflector, x98) "Suspicion of white spot W of N-S radial
band, slightly brighter than wall. Diam. @5-6km. Area affected by temp.
?Term. passed over it just 5h before. Gradual decline in brightness
over the 10m period." NASA catalog weight=1 (very low). NASA catalog ID
1288.
On 1992 May 13 at UT 22:30 R. Turner (Wolverhampton, UK, 3.6"
reftactor, x50) noticed that there was a white spot on the WSW rim that
he had not seen earlier. The Cameron 2006 catalog ID=445 and weight=5.
ALPO/BAA weight=1.
Plato 1873 Nov 01 UTC 20:00? Observed by Pratt (England?) "Unusual
Appearance". NASA catalog weight=1 (very low). NASA catalog ID #182.
ALPO/BAA weight=1.
On 1976 Nov 03 at UT20:00-21:40 P.W. Foley (Kent, UK) reported a TLP in
Gassendi - some obsevers detected colour, others did not. P. Moore did
not notice anything unsual earlier at 18:50-19:00, though his seeing
was IV-V. Nor did he see anything unsual from 21:53-00:20, but seeing
was still IV-V. D. Jewitt, observing 20:34-21:25 and 22:55-23:20 also
reported nothing unusual. Amery (Reading, UK, 25cm reflector, x300) did
however notice a small reddish spot to west of central ridge, but by
20:30UT the colour was less obvious, but the spot was back again at
20:45, but not easily seen at 21:00 and gone completely by 21:45UT.
N.Bryant (Ilfracombe, UK, 25.4cm reflector, x260), observed 3 red
patches on the floor between 20:54 and 21:31UT. A BAA Lunar Section
report. ALPO/BAA weight=3.
On 1963 Nov 28 at UT 00:30-01:45 Barr, Greenacre, Hall and
Dungan (Flagstaff, AZ, USA, 24" refractor, and 69" reflector)
observed pink on the outer SW rim and a red spot towards the S of
this. A red spot was seen on the eastern side of Vallis Schroteri
but only by Barr and Dungan. Other features checked for
atmospheric spectral dispersion and chromatic aberation - but the
colours in Aristarchus were not due to these. Smaller 12" scope
checked but no effects seen - presumably due to resolution and
image contrast issues? Pink on the SW rim may have been seen in a
69" scope by Boyce and Ford. ALPO/BAA weight=4.
On 1980 Aug 22 at UT20:15-21:29 J-H Robinson () detected violet on the
west wall of Aristarchus. Cameron 2006 catalog ID=105 and weight=5.
ALPO/BAA weight=2.
On 1980 Aug 22 at 02:15-21:29UT J-H Robinson (Teighmouth, Devon, UK,
12" reflector, x200, seeing=II) noticed in the area south east of
Manilius that it was brighter in red light than in blue light at
20:15UT whereas 1 minute later it was the same brightness in each
filter. The effect reappeared at 20:21UT and was particularly strong at
20:32UT. Foley (Kent, UK) verified this at 21:01UT - the blink area was
of high reflectivity in white light and was bright in red at 21:15UT,
thougjh the south east area stopped giving a colour reaction at
21:25UT. Madej (Huddersfield) found Manilius B to be norm al at 23:52UT
however at 23:55UT it was surrounded by a transient white ring that
varied in visibility in an irregular way. Foley found Manilius B had a
vivid blue interior and in blue light the ring was black. and not at
all seen in red or white light. The CED brightness measurement varied
from 1.9 to 2.4. All other regions observed were normal in brightness.
Violet was seen on the west wall of Aristarchus though. M.Price
(Camberley, UK) found a possible blink in Manilius B but was observing
under poor seeing conditions. Cameron 2006 catalog ID=105 and weight=5.
ALPO/BAA weight=4.
Herodotus 1966 Jun 30 UTC 03:10-03:35 Observed by Bartlett (Baltimore,
MD, USA) described in the NASA catalog as: "Bright pseudo-peak again
vis. within floor shadow. Peak est. 5 bright. Had seen it at successive
lunations in '66" 4" x280 refractor used. NASA catalog weight=4 (high).
NASA catalog TLP ID No. #950. ALPO/BAA weight=3.
Aristarchus 1973 Feb 14 UTC 18:31-18:34 observed by Fuger (49N, 8.42E,
75mm refractor, T=1, S=2) "Violet colours on S. of the crater" -
Hilbrecht and Kuveler, Earth, Moon & Planets, 30 (1984), p53-61
On 1891 Oct 14 at UT 18:00 Pickering, based at Arequipa, Peru, and
using a 12" reflector, saw is Schroter's Valley and the vicinity
"Varitions in vapor column and visibility of craterlets A, C and F
(Plate B) in early period at Peru. Directional vaporjet towards F
varied but was always continuous. Later, in Musa. There was a break in
it. D was quiescent in early period. (due to change in telescope &
atmosphere ? Time estimated from given colongitude)." Cameron 1978
catalog ID=273 and weight=3. ALPO/BAA weight=2.
On 2017 Sep 02/03 UT 23:55-00:30 A.Anunziato (Parana,
Argentina, 105 mm Maksutov-Cassegrain, x154, seeing 6/10, some
interuption from clouds) observed a light spot SE of the
centre of the floor of the crater, which came and went in
visibility. There is a light spot here, but what was unusual
was that the visibility decreased over time.
ALPO/BAA weight=1.
Aristarchus 1982 Nov 27 UT 20:13-01:00 J-H Robinson (Teighmouth, Devon,
UK) found that the bands of Aristarchus were clearer in red than in
blue light. North found that the sunlit part of the crater was very
bright. M. Cook described the crater as a "kaleidoscope of colour.
Foley observed UT 23:05-01:00 (Kent, UK, Antionadi III, Transparency
Moderate) - Colouration Seen - Ref: BAA Lunar Section Circular. The
Cameron 2006 catalog ID=190 and weight=5. The ALPO/BAA weight=3.
On 1825 Jan 01 UT17:00? an unknown Russian observer noticed a
cloud in Mersenius.
nr Fra Mauro 1970 Aug 14 UT 05:00? Observed by Bell (Californina).
"Bright blue-white flare (meteor?)(call for obs. at Fra Mauro at
perigee because of moonquakes there -- therefore biased to tidal
hypothesis. That was the original location given for the A1 moonquake
site, but it is located elsewhere now. Ancill. data given for 1970)."
NASA catalog weight=1. NASA catalog ID #1273. ALPO/BAA weight=1.
Herodotus 1971 Jul 05 UT 03:48 Observed by Bartlett (Baltimore,
MD, USA) described in the NASA catalog as: Pseudo-c.p. I=
4(albdeo) appeared to cast a distinct shadow. 1st time seen.
(Apollo 15 photo shows an apparent slight elev. nr. center --
very very low hills? 5" refelctor x79,283x, NASA catalog weight=1
(low). ALPO/BAA weight=2.
On 1963 Nov 28 at UT 22:30-00:00 Fisher (Colefax, CA, USA, 8"
Newtonian reflector)observed a yellow on crater rims adjacent to
Anaximander. Yellow colour also seen on Aristarchus that night.
The ALPO/BAA weight=1.
Aristarchus and Cobra Head 1966 Oct 27 UTC 02:30-03:00 Observed by
Delano (New Bedford, Massachusetts, USA, 12.5" reflector, x360) and
Corralitos Observatory (Organ Pass, NM, USA, 24" reflector, Moonblink).
"C.p. of Aris. noticeably less bright thro blue filter but very bright
thru red & no filter. Shadow of c.p. faint & grayish whereas wall shad.
were normal black. (confirm. of Gordon, even tho 2h later?). Sketch.
C.p. rated 10deg in red & no filter, & 8deg in blue. Other features
rated same in all 3. Cobra Head had 2 red patches. Sketches. Not
confirmed by Corralitos MB." NASA catalog weight=5. NASA catalog ID
989.
On 1980 Sep 22 at UT05:00? D. Louderback (South Bend, WA, USA, 8"
reflector, x140 and 2.5" refractor) observed in Promitorium Agarum that
one of his pre-designated points, called "A", through to "C and "D" was
at least 5 brightness points brighter in red than in blue light. The
reverse was true on Sep 25th. Tonight the red seemed to be on a narrow
strip on the western edge. The Cameron 2006 catalog ID=109 and the
weight=3. The ALPO/BAA weight=3.
On 1987 Sep 05 at 20:55UT A.C. Cook (Frimley, UK, 90mm questar
telescope, x130, seeing III-IV, Moon 16 deg in altitude) observed a
dusky dark gray area just north of Herodotus and just south of the
Cobra Head. The interior shadow on the east of Herodotus by comparison
wad black and distinct. No change was seen when viewed through a
rotated polaroid filter. Apparently D. Darling (Sun Praire, WI, USA)
was observing at the same time but had better observing conditions and
could see detail in this region, suggesting that it was not a TLP.
There is no Cameron entry for this report. The ALPO/BAA weight=1.
Gassendi 1987 Sep 05 UT 20:25 Observed by Moore (Selsey, Sussex, UK, Antoniadi
III seeing, 12.5" reflector) "Intensely bright craterlet south of central
peak, surrounded by a luminous nimbus. Foley (Kent, UK, 12" reflector)onfirmed
the crater was highly luminous at 21:20, and surrounded by a blue halo that
had a darker blue band within it. This craterlet faded over time, and by 21:20
Moore considered that it was no longer prominent, by 21:22 Foley confirmed the
reduced brilliance, and by 21:30 Moore considered it to be perfectly normal.
Moore considers the nimbus effect to be normal. The Cameron 2006 catalog ID=
306 and weight=5. The ALPO/BAA catalog weight=3.
Aristarchus 1973 Feb 15 UTC 17:07-19:31 Observed by Theiss (51N, 9.67E,
75mm refractor) "Area 4-5 diameters of Aristarchus were coloured
clearly yellow to red" Ref: Hilbrecht & Kuveler (1984) Moon & Planets
30, pp53-61.
Aristarchus, Cobras Head 1966 Oct 27 UTC 02:30-03:00 Observed by Delano
(new Bedford, Massachusetts, USA, 12.5" reflector x360) and Corralitos
Observatory (Organ Pass, NM, USA, 24" reflector & Moonblink) "C.p. of
Aris. noticeably less bright thro blue filter but very bright thru red
& no filter. Shadow of C.p. faint & grayish whereas wall shad. were
normal black, (confirm. of Gordon, even tho 2h later?). Sketch of C.p.
rated at 10deg in red & no filter, & 8deg in blue. Other features rated
same in all 3. Cobra Head had 2 red patches. Sketches. Not confirm. by
Corralitos MB". NASA catalog weight=5 (very high). NASA catalog ID 989.
On 1963 Nov 29 at UT 01:30-03:00 Fisher (Colefax, CA, USA, 20cm
reflector, thin streamers of cloud across sky, but no wind)
Aristarchus had a faint pale yellow tint along the rim and the
crater was very bright. No detail seen in in Vallis Schroteri.
Yellow spot also seen on the northern limb (Carpenter and
Pythagoras?). Both effects had been seen the previous night and
were confirmed by friends. Colour still present when observing
stopped at 03:00 UT. The ALPO/BAA weight=1.
On 1963 Nov 29 at UT 01:30-03:00 Fisher (Colefax, CA, USA, 20cm
reflector, thin streamers of cloud across sky, but no wind.)
Carpenter had a yellow tint along the W rim. Ywllow tint seen
on Pythagoras and also Aristarchus. Effect had been seen the
previous night and were confirmed by friends. Colour still
present when observing stopped at 03L00 UT. The ALPO/BAA
weight=1.
On 1963 Nov 29 at UT 01:30-03:00 Fisher (Colefax, CA, USA, 20cm
reflector, thin streamers of cloud across sky, but no wind.)
Pythagoras had a yellow tint along the W rim. Ywllow tint seen
on Carpenter and also Aristarchus. Effect had been seen the
previous night and were confirmed by friends. Colour still
present when observing stopped at 03L00 UT. The ALPO/BAA
weight=1.
On 1977 Apr 01 at UT 20:40-21:10 D.Sims (Devon Valley, Dawlish, Devon,
UK, 25.4cm reflector, Wratten 25 and 44a filters, x300, seeing II)
found Schroter's valley clearer in red than in blue. No colour filter
reactions seen on other features. This is a BAA Lunar Section
observation. ALPO/BAA weight=2.
Near Furnerius 1920 Nov 23 UTC 20:00? Observed by an unknown observer
(England?) "Shaft of light projecting from Moon, or spot so bright it
appeared to (strong ray?)" NASA catalog weight=1 (very low). NASA
catalog ID #378
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 1915 Jul 24 at UT 22:00? Barabashovihi (Russia) observed a TLP on
the west limb: "When phi Strettsa (?) approached the edge but still
separated, the star began to stretch in a belt 3X its own length & then
instantly disappeared. Probably no significant atm. or vapors. (similar
to other reports of fading occult. Gives limb as E. but that is in ast.
convention)". The 1978 Cameon catalog ID= 357 and weight=2. The
ALPO/BAA weight=1.
were fainter. The third (about 0.066 deg from the northern limb)
showed an erruption of fire or luminous matter. The brightness
of this third volcano was much brighter than Mechain's comet.
Webb thinks that these other two volcanos were Menelaus and
Manilius. The Cameron 1978 catalog ID=32 and weight=4. The
ALPO/BAA catalog weight=3.
were fainter. The third (about 0.066 deg from the northern limb)
showed an erruption of fire or luminous matter. The brightness
of this third volcano was much brighter than Mechain's comet.
Webb thinks that these other two volcanos were Menelaus and
Manilius. The Cameron 1978 catalog ID=32 and weight=4. The
ALPO/BAA catalog weight=1.
were fainter. The third (about 0.066 deg from the northern limb)
showed an erruption of fire or luminous matter. The brightness
of this third volcano was much brighter than Mechain's comet.
Webb thinks that these other two volcanos were Menelaus and
Manilius. The Cameron 1978 catalog ID=32 and weight=4. The
ALPO/BAA catalog weight=3.
A guest star trespassed against the moon. Cameron
suspects that this was a meteor? ALPO/BAA catalog weight=1.
Cameron 2006 catalog weight=0. Julian date 1356 May 03.
Gregorian date 1356 May 11.
William Herschel and Mrs Lind saw a red, 4th magnitude brightness, less
than 3 arc sec in diameter. Herschel believed that he was seeing a
lunar volcano in erruption.
the previous night". Its diameter is less than 3"
(5-6 km) as judged by comparing with the angular diameter
of Jupiter and also Jupiter's third satellite (the
diameter of the active part of the volcano was at least
twice the angular diameter of Jupiter's Moon). The shape
was an irregular round figure with very sharply defined edges.
It resembled a small piece of burning charcoal, when it is covered
by a thin coat of white ash. The other two volcanos were
much further towards the centre of the Moon and
resembled large faint nebulae that are gradually
much brighter in the middle; but with no well defined luminous
spot within them. These three spots are plainly to be
distinguished from the rest of the marks upon the Moon;
for the reflection of the Sun's rays from Earth is, in its present
situation, sufficiently bright with a ten-foot reflector, to
show the Moon's spots, even the darkest of them. Such
similar phenomena were not perceived in the previous month,
despite using the same telescope. The volcano was not as bright
as his 4th May 1783 sighting (resembling a 4th magnitude star as
seen with the naked eye), though the latter was smaller in diameter.
Cameron's 1978 ALPO catalog has a TLP ID No. of 33 and a weight of
4. The ALPO/BAA catalog weight is 3.
the previous night". Its diameter is less than 3"
(5-6 km) as judged by comparing with the angular diameter
of Jupiter and also Jupiter's third satellite (the
diameter of the active part of the volcano was at least
twice the angular diameter of Jupiter's Moon). The shape
was an irregular round figure with very sharply defined edges.
It resembled a small piece of burning charcoal, when it is covered
by a thin coat of white ash. The other two volcanos were
much further towards the centre of the Moon and
resembled large faint nebulae that are gradually
much brighter in the middle; but with no well defined luminous
spot within them. These three spots are plainly to be
distinguished from the rest of the marks upon the Moon;
for the reflection of the Sun's rays from Earth is, in its present
situation, sufficiently bright with a ten-foot reflector, to
show the Moon's spots, even the darkest of them. Such
similar phenomena were not perceived in the previous month,
despite using the same telescope. The volcano was not as bright
as his 4th May 1783 sighting (resembling a 4th magnitude star as
seen with the naked eye), though the latter was smaller in diameter.
Cameron's 1978 ALPO catalog has a TLP ID No. of 33 and a weight of
4. The ALPO/BAA catalog weight is 2.
There were two other volcanos were much further towards the centre of
the Moon and resembled large faint nebulae that are gradually
much brighter in the middle; but with no well defined luminous
spot within them. These three spots are plainly to be
distinguished from the rest of the marks upon the Moon;
for the reflection of the Sun's rays from Earth is, in its present
situation, sufficiently bright with a ten-foot reflector, to
show the Moon's spots, even the darkest of them. Such
similar phenomena were not perceived in the previous month,
despite using the same telescope. The volcano was not as bright
as his 4th May 1783 sighting (resembling a 4th magnitude star as
seen with the naked eye), though the latter was smaller in diameter.
Cameron's 1978 ALPO catalog has a TLP ID No. of 33 and a weight of
4. The ALPO/BAA catalog weight is 2.
In 1824 May 01 at UT 21:00 Gobel (Koburg, Germany) observed near
Aristarchus, a blinking light of magnitude 9-10, in Earthshine. The
ALPO/BAA ID=99 and the weight=4. The ALPO/BAA weight=3.
Leibnitz Mountains 1955 May 24 UT 21:30-22:00 Observed by Firsoff
(Somerset, England 6.5" reflector, x240, seeing = very good). "Changing
lights over a period of time, lunar aurora? Beyond cusps were 2 bright
pts. 1 was sparkling and dancing and weaker intensity. Then a faint
beam detached itself & shot up vertically, becoming more intense but
faded at the base. Total length @ 160 km. Endured for > 2 s. Due to
telescope spider or lunar aurora?" NASA catalog weight=4 (good). NASA
catalog ID #593.
On 1981 Jan 09 at UT 00:30-00:45 D. Darling (Sun Praire, WI, USA,
12.5" reflector, seeing=8/10, transparency clear, but Moon low at 7 deg
above the horizon) found that despite Aristarchus being seen to be
bright in Earthshine, it was not as bright as Menelaus and Manilius.
Cameron 2006 catalog ID=121 and weight=1. ALPO/BAA weight=1.
On 1981 Jan 09 at UT 00:30-00:45 D. Darling (Sun Praire, WI, USA,
12.5" reflector, seeing=8/10 and the sky was clear - the Moon was at
7deg altitude though) saw that Manilius outshone Aristarchus - or was
it that Aristarchus was especially faint tonight? Manilius could be
seen even when the illuminated part of the Moon was in the eyepiece.
The Cameron 2006 catalog ID=121 and weight=1. The ALPO/BAA weight=1.
On 1981 Jan 09 at UT 00:30-00:45 D. Darling (Sun Praire, WI, USA,
12.5" reflector, seeing=8/10 and the sky was clear - the Moon was at
7 deg altitude though) saw that Menelaus outshone Aristarchus - or was
it that Aristarchus was especially faint tonight? Menelaus could be
seen even when the illuminated part of the Moon was in the eyepiece.
The Cameron 2006 catalog ID=121 and weight=1. The ALPO/BAA weight=1.
Picard 2002 Sep 10 UT 02:30-03:21 Observed by Gray (Winnemucca, NV,
USA, 152mm refractor x248,S=2-3, T=5) "observed in White light and
through Wratten Red 25 and Blue #38A filters. The crater through the
Red 25 filter looked very similar to the view in White light. Using the
Blue 38A filter Picard almost dissapeared - it looked like a dim,
faintly observable black spot with the sunlit, east facing west crater
wall barely visible. Observer had not observed Picard very often, so
was not too familiar with it but it seemed odd that it almost vanished
through the blue filter." ALPO observational report. The ALPO/BAA
weight=3.
In 1965 Jul 02 at UT 04:20-05:50 Albert and Welch (Azuss, CA, USA, 8"
reflector, x375) and Emanuel (West Covina, CA, USA, 4.5" reflector)
observed 4th magnitude star-like flashes to blotches in Aristarchus, in
ashen light. Cameron says that this is independent confirmation and
also that the date in MBMW is 7/1/65 which is local time + 2nd UT. The
Cameron 1978 catalog ID=881 and weight=3. The ALPO/BAA weight=3.