Aristarchus 1976 Oct 18 UT 07:42 Observed by Bartlett (Baltimore, MD,
USA, 4.5" reflector and 3" refractor, S=3, T=5) "Inner E. wall 6 deg
with very large EWBS at 8deg. No viol. color anywhere & floor was gray
at 4 deg (very low). C.p. is only 8 deg. At base of c.p. between peak &
advancing shadow a very faint but definite red glow was seen. It was
also seen later in the 3" refr. Was confined to W.base of peak & no
color on E. base tho. carefully searched for. This red glow was unique
in his experience of 28 yrs. His obs. thru. col. 223deg saw nothing
more unusual." Cameron 1978 catalog weight=4 and ID #1455.
In 1837 Mar 19 at UT 18:00 Rankin and Chevalier (France) noted a
singular appearance on the dark side. Luminous spots there & general
glow on upper (S?) limb. Whole shaded part seemed to be a mixture of
light & shades. The Cameron 1978 catalog ID=124 and weight=5. The
ALPO/BAA weight=3.
On 1979 Sep 25 at UT00:40-00:51 D. Darling (Sun Praire, WI, USA, 12.5"
reflector, x62) found the crater to blow and fluctuate between
magnitude approximately 4 and 5. Initially it was bright, then faded,
then brightened again aggroximately x2 and then faded into the
background. The Cameron 2006 catalog ID=70 and weight=0. The ALPO/BAA
weight=1.
Aristarchus 1949 May 01 at UT 20:45 H.P. Wilkins (Kent, UK, 3"
refractor x100) observed Earthshine was very detailed and
Aristarchus was noticeably a bright patch. Upon concentrating on
Aristarchus, he observed that it flared up in brightness
considerably more still for about 2 sec. During this flare up
time, inner terraces and the central peak became visible.
Cameron says that this was confirmed by Barcroft a few hours
later???? The Cameron 1978 catalog ID=518 and Weight=5. The
ALPO/BAA weight=3.
North of Mare Crisium 1958 Oct 16 UT 18:00? Observed by Mayemson
(England?) "Bright spot in dark part" NASA catalog weight=2 (low). NASA
catalog ID #700.
On 1989 Apr 10 at UT01:30-02:00 D. Darling (Sun Praire, WI, USA, 12.5"
reflector, x64, seeing excellent) observed that Earthshine was not as
good as the previous night "~1/4 In 1900 Nov 26 at UT 19:00? an unknown observer (in Europe) observed a
suspicious obscuring phenom on a dark plain (mare). The cameron 1978
catalog ID=307 and the weight=2. The ALPO/BAA weight=1.
1951 Mar 13 UT 01:35:50 L.T.Johnson (USA) observed a faint flash
near W limb in earthshine - just S of Grimaldi.
ALPO/BAA weight=1.
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.
Sirsalis 1990 Mar 01 UT18:30-19:45 M. Holmes (Rochdale, UK,
21.5cm Newtonian, seeing Antoniadi I/II, Transparency very
good) was observing in earthine and saw an intense blue spot
"wink on" near to Sirsalis (sketch shows location on SE rim),
until clouded out at 18:30. When the sky cleared at 19:15UT
the spot was still visible but fainter, with a halo, the size
of Sirsalis A. By 19:35 there was a loss of detail, region
only a faint patch of light covering area twice the size of
Sirsalis crater. Clouded out permanently at 19:45UT. Cameron
2006 catalog event #392, weight=0. ALPO/BAA weight=3.
A lunar aurora on the dark limb was seen by Heywood and others of
Westville, Ohio, USA, using a 2" refractor at x60. Observer saw
misty like light in dark part, not like earthshine - seen
repeatedly by him and others in Nov., Dec, and Mar 29, 30 1884.
Displays on Moon similar similar effects on Earth/Aurora? Cameron
1978 catalog ID=239 and weight=4. ALPO/BAA weight=3.
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.
On 1990 Mar 02 at UT 19:35-19:50 P. Williamson (Shropshire, UK, 14"
reflector, x178, seeing=good and steady) noticed a yellow-orange glow
in Gassendi (from a small illumnated crater?) in Earthshine at 19:35UT
and by 19:40UT it had become very bright white, afterwhich it
completely faded within 10 minutes. The Cameron 2006 catalog ID=393 and
the weight=1. The ALPO/BAA weight=3.
Burg 2020 Dec 20 UT 19:00-20:08 (T.Smith, Codnor, UK, 16"
Newtonian, seeing III-IV) observed visually that this crater
was very red on its western floor and rim. A similar effect
seen in Plinius, elsewhere on the Moon. No red was seen to the
exterior of both craters. The redness on both of these craters
had become diluted by 19:40. Also around this time, it was
noted that Proclus had a slight redness to its western
interior, though by no means as strong as in Burg and Plinius.
A comparison with Censorinus revealed no redness to this
crater. By 20:08 Burg was only showing a hint of red at times.
ALPO/BAA weight=1.
Plinius 2020 Dec 20 UT 19:00-20:13 (T.Smith, Codnor, UK, 16"
Newtonian, seeing III-IV) observed visually that this crater
was very red on its western floor and rim. A similar effect
seen in Burg, elsewhere on the Moon. The central peak of
Plinius was very easy to see and also looked red in colour. No
red was seen to the exterior of both craters. The redness on
both of these craters had become diluted by 19:40. Also around
his time, it was noted that Proclus had a slight redness to
its western interior, though by no means as strong as in Burg
and Plinius. A comparison with Censorinus revealed no redness
to this crater. By 20:08 Plinius still had a slight red hue
but Burg was only showing a hint of red at times. Observations
ceased at 20:14 due to the Moon being hidden by an
obstruction. ALPO/BAA weight=1.
Theophiuls 2020 Dec 20 UT 19:00 (T.Smith, Codnor, UK, 16"
Newtonian, seeing III-IV) observed visually that the central
peak of this crater appeared excessively/abnormally bright to
his eyes. ALPO/BAA weight=1.
Proclus 2020 Dec 20 UT 19:40 (T.Smith, Codnor, UK, 16"
Newtonian, seeing III-IV) observed visually and noted that
Proclus had a slight redness to its western interior, though
by no means as strong as in Burg and Plinius which exhibited
stronger red colours. A comparison with Censorinus revealed no
redness to this crater. ALPO/BAA weight=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.
On 1979 Mar 04 at UT18:15-21:45 P.W. Foley, (Kent, UK, 12" reflector,
x180, seeing II-I) noticed that Aristarchus was unusually bright
(though colourless) - the northern part being the more brilliant. Other
features seen but less visible, though still quite obvious. A CED
brightness reading of 0.3 was recorded - the highest ever so far. Amery
(Reading, UK, 19?" reflector, 50-100x, obtained photographs. The
Cameron 2006 catalog ID=46 and weight=5. The ALPO/BAA weight=2.
On 1979 Mar 04 at UT18:15-21:45 P.W. Foley, (Kent, UK, 12" reflector,
x180, seeing II-I) noticed that although other features in Earthshine
were quite obvious, Grimaldi was not, though at x200 (should this be
20:00?) Grimaldi "shone with a brilliance to that of a thin cresecent
of 2-3d". Amery (Reading, UK, 19?" reflector, 50-100x, obtained
photographs. The Cameron 2006 catalog ID=46 and weight=5. The ALPO/BAA
weight=3.
On 1993 Dec 19 at UT 16:00-17:00 S. Beaumont (Cambridge, UK, 12"
reflector, x230) observed in Theophilus that the "c.p. > reddish brown
tint to SW (on peak?)" but suspected that it was probably spurious
colour, however no colour was seen later. The ALPO/BAA catalog ID=469
and the weight=3. The ALPO/BAA weight=2.
On 1965 Oct 30 at 23:30-23:50UT Fehring and Garris (Parasmus, NJ, USA,
using a 2.4" refractor x88, seeing very good) saw a fuzzy area --
variations in shape and distinctness, seen in an area east of Atlas
crater. A drawing was made. It was noted that no other area had a
similar effect. Cameron 1978 catalog ID=909 and weight=3. ALPO/BAA
weight=3.
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 1964 Jun 17 at UT 04:15-05:01 Cross et al. (Whittier, CA, USA, 19" ?
reflector, S=7-8) observed near Ross D: "Gas cloud. Motion". The
Cameron 1978 catalog ID=818 and weight=4. The ALPO/BAA weight=4.
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.
Alphonsus 1966 May 27 UT 21:10 Observed by Sartory, Moore,
Mosely (England and Ireland, 8.5" reflector, 10" refractor) "Red
colour on central peak area" NASA catalog ID 937. NASA catalog
weight=5. ALPO/BAA weight=4.
On 1994 Apr 19 at UT 00:00 P. Kursewicz (Epping, NH, USA) observed a
dark patch surrounding Picard crater. The ALPO/BAA weight=1.
On 1982 Jul 28 at UT20:38-20:48UT A.C. Cook (Frimley, Surrey, UK, 12"
reflector, seeing IV-V, some spurious colour prsent) observed that the
central peak of Alphonsus was brighter in red light than in blue, so
much so that at the start of the session the peak could hardly be seen
in blue light. The central peak varied in brightness in red light but
not in white light. The central peak of arzachel was brighter than that
of Alphonsus in white light but had no colour - Arzachel's central peak
did however appear to fade in brightness over time (or was it Alphonsus
getting brighter?). Cameron 2006 catalog ID=177 and weight=3. The
ALPO/BAA weight=2.
Plato 1918 May 20 UT 18:00? Observed by Markov (Russia) "Brightness in
shadow of the light sector & 1 spot" NASA catalog weight=3 (average).
NASA catalog ID #369. ALPO/BAA weight=2.
On 1975 May 18 at UT2115-2145 C. Lord (St Annes-on-sea,
Lancashire, UK, 76mm f/16 refractor, x170, Wratten 25, and 44a
Moon blink filters used, Transparency 4.5/5, no wind, S=F). The
west flank of Maginus, and the interior, appeared to be partly
obscured. No other features in a similar position along the
terminator were obscured. No colour blink was detected with the
filters, though a pronounced red/white light blink was noted; the
device employed a N.D. x4 filter. By 21:45UT the floor was no
longer obscured and only Magninus G was masked in a white haze;
however immediately adjacent to the terminator was an ill defined
misty patch lying where the outer flank of maginus would have
been visible. The rest of the terminator was sharp. The
obscuration was only seen to advantage in blue and int. light,
and the blue/int blink was only very slight. Findlay and
McDonnell observed 21:30-23:00 using a 25cm refractor (Seeing II-
III) but failed to see anything unsual. NASA catalog weight=3.
NASA catalog ID #1407. ALPO/BAA weight=2.
Vallis Alpes 1983 Jun 18 UT 22:01-22:23 P.Madej (Huddersfield, UK,
77mm refractor, x83,x250, seeing II-III, transparency fair).
After studying the whole length of this valley, the observer saw
a change in "albedo" and a small change in colour of the valley
floor near to the Plato end. This colour was not seen in a
yellow Wratten 15 filter but was noted in a purple Wratten 35
filter, and was strong in a red filter. Also the crater
Trouvelot was not seen at x250 with a x2 Barlow.Wratten 25.
ALPO/BAA weight=1.
Daniell 1983 Jun 18 UT 22:06-22:25) P.Madej (Huddersfield, UK,
77mm refractor, x83,x166, seeing II-III, transparency fair).
Noted on the inside W eall a faint red rose like glow (with a
diameter? about it). The red glow varied in brightness with a
period of about 2 minutes. It looked somewhat brighter at x166.
The glow was still visible when the observation ended at 22:15
ALPO/BAA weight=1.
On 2001 Jun 29 at UT22:16-22:22 C. Brook (Plymouth, UK, 60mm refractor,
x120, no spurious colour seen, seeing I) observed that the central
peaks of Alphonsus looked bright at 22:16UT but had dimmed by 22:22UT.
The three dark patches on the floor of Alphonsus were clearly seen. The
ALPO/BAA weight=1.
On 2001 Jun 29 at UT 22:16-22:20 C. Brook (Plymouth, UK, seeing
conditions very good, x120) reported that the central peak of Alphonsus
was brighter than the central peak of Arzachel (or was it the other way
around?). Cook observed 4 hours later from Washington DC, USA and found
that on CCD images that the central peak of Alphonsus was only slightly
less than that of Arzachel. The ALPO/BAA weight=2.
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.
Alphonsus 1966 May 28 UT 23:00-01:00 Observed by Smith (England, 10"
reflector) Birney (VA?, USA, 8" refactor + Moonblink) Corralitos Obs.
(NM, USA, 24" reflector + Moonblink) "Red patches (Smith), Trident Moon
Blink device suspected(?? log)earlier at 22:40. Birney observed at
2300-0100?, and gave indep. confirm? Corralitos did not confirm MB
(however they report Gassendi-- misident. ?)" NASA catalog weight=5. NASA catalog ID #938. ALPO/BAA weight=4.
On 1994 Apr 20 at UT 01:31 D. Darling (Sun Praire, WI, USA) found that
Picard crater was surrounded by a dark nebulous patch - it was
impossible to resolve detail inside this dark zone. The ALPO/BAA
weight=1.
On 1992 Jun 09 at UT 18:52 G. Kolovos, Thessaloniki, 40.63111N,
22.9597W, height 28m, Greece) photographed two blue spots on the
terminator region of the Moon in one of a series of Ektachrome film
pictures. The rest of the Moon was a white-yellow colour. The ALPO/BAA
weight=1.
Copernicus 1939 Mar 29 UT 19:00-19:15 Observed by Wilkins (Kent,
England, 6" reflector) "C.P. diffuse light spot, faint glow s as
tho in a luminous mist (3h before SR) Some indication of
E.terraces, then vanished." NASA catalog weight=4. NASA catalog
ID #447. ALPO/BAA weight=3.
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.
On 1968 Oct 01 at UT 21:00? Bartlett (Baltimore, MD, USA) and Beck
(Ohio, USA, x437) observed lack of detail on the floor of Plato,
however the wall of the crater was easily resolved. Cameron says that
this was an independent confirmation. The Cameron 1978 catalog ID=1092
and weight=5. The ALPO/BAA weight=3.
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.
Alphonsus 1966 May 29 UT 21:45-22:45 Observed by Wise (England, 4.5"
reflector, x125). and Corralitos Observatory (NM, USA). "Glint lasting
1.5s. (onset of Smith's anomaly? Specular reflection should last
longer). Not confirmed by Corralitos MB, (however they report Gassendi?
misident., or did they obs. another feature?). At UT 22:45 Smith and
Brown (England, UK, 10" reflector) observed reddish patches in
Alphonsus. Negative results from Brown though at 21:21Ut and 22:25UT).
The Cameron 1978 catalog ID=939 and 940 and weight=4. The ALPO/BAA
weight=3.
On 1984 Jun 09 at UT 04:55-05:14 P. Jean (Outremont, Canada) detected
in the dark side of the Moon, a few km east of Kies crater, a bright
point that should not be poking out of the shadow (according to Foley).
The Cameron 2006 catalog ID=244 and the weight=3. The ALPO/BAA
weight=2.
On 1974 Jan 03 at UT 18:30 a Norwegian amateur astronomer,
Hoydalsvik (Hakonsgate, in West Norway, 60mm refractor)
photographed the Moon using High Speed Ektacrome (400ASA) film
with good focus. The TLP was located on the southern slope of
Sasserides H and was pink in colour with some bluish in it.
The coloured area was circular with a diameter of 0.5 minutes
of arc. Only one exposure was taken. The photograph was
checked by the Institute of Theoretical Astrophysics,
University of Oslo. Although they thought it was probably
genuine (could have been an impact flash?) suggestions by the
BAA lunar section favoured static electrical discharge on the
film. It is uncertain whether the film was ever examined by a
Photographic developing lab such as Kodak, who would be able
to tell if it was real or an artefact. ALPO/BAA weight=1.
Tycho 1998 Feb 06 UT 22:48-22:54 R. Braga (Corsica (MI),
Italy, 102mm f8.8 refractor, x180, with diagonal, Wratten 23A,
80A and an OR5 filter, seeing II, Transparency good). Observer
noticed that the floor darkened towards the NW (IAU),
particularly with the blue Wratten 80A filter. The ALPO/BAA
weight=1.
127mm f/12 GoTo scope, x62-x154, seeing: best and transparency=
6) observed that an unoficially named mountain (Lambert Gamma or
Mons Undest), near Lambert, had a "very strong glow", especially
the part that was facing the line of the terminator and this was
brighter than the side facing away. The No other object nearby
was casting as much light, even Mons La Hire. The effect was
seen for 40 minutes and the glow was present throughout. The
ALPO/BAA weight=2.
Gassendi 1967 Oct 13 UTC 19:17-20:00 Observers: Henshaw (Mansfield, UK,
8.5" reflector x112) and Corralitos Observator (Organ Pass, NM, USA,
24" reflector) "Phenomenon (brightening ?) nr. NW (ast. ?) lasting for
3s. Cont'd for 45m but nothing else unusual, (nr. Gass or in it?).
Corralitos MB did not confirm." NASA catalog weight=3 (average). NASA
catalog ID #1050.
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
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.
Gassendi 1966 May 30 UT 20:32-20:59 Observed by Sartory (England, 8.5"
reflector + filters) "Orange patch & obscuration -- detected by Eng.
moon blink system. Color seen visually."NASA catalog weight=4 (good).
NASA catalog ID #941.
On 1955 Jan 05 at 01:00-01:30 UT D.A. Logue (Larchment, PA,
USA, 15cm reflector at x340, seeing Good) saw a strange blue
light above the surface of the Moon where the night and the
day meet. He observed this light for more than 30 min and it
did not appear to move. It appeared like a star in that the
rays of light came from it. The observer adds that he first
thought thst the objects was a star, but later decided that it
had to be on the Moon itself. A drawing shows the blue spot
near the rugged south west (IAU?) limb of the Moon. The editor
of the Strolling Astronomer (Vol 8, No. 11-12, Nov-Dec 1954,
p146) was unable to identify the craters drawn. The editor
speculates that the observer saw a high mountain peak with its
summit in sunlight and detached from the illuminated regions -
however this would not explain the blue colour. Note this is
an ALPO observation and does not apear in the Cameron
catalogs. ALPO/BAA weight=2.
On 1964 Jun 21 at UT 03:43-05:44 Harris, Cross and Helland (Whittier,
CA, USA, 19" reflector) observed south of Ross D: "Moving dark area".
The Cameron 1978 catalog ID=819 and weight=4. The ALPO/BAA weight=4.
On 1982 Aug 01 at 00:00-01:00 K. Marshall (Medellin, Columbia, 12"
reflector, seeing I-II) noted shading on the east floor of Plato that
was apparently lighter than the rest of the floor and this was seen at
both low and high magnifications. Foley notes that this was unusual.
There were three craterlets visible on the floor - the central one was
the brightest. Cameron 1978 catalog ID=178 and weight=3. ALPO/BAA
weight=1.
A.S.Williams of West Brighton, UK, using a 5.25" Calver, x150 and
definition fairly good. Observer noticed that the Mare seemed covered
with a close network of innumerable streaks, and spotted with countless
numbers of light specks, so that it would hardly be possible to
delineate them all in one night. The spots and streaks together must
have numbered ~1000. The observer had never seen anything like the
number of spots and streaks. Peirce A, was not at all easy to see and
neighboring spots almost as bright made it difficult to distinguish
which one was Peirce A. ALPO/BAA weight=3.
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.
On 1825 Jan 01 UT17:00? an unknown Russian observer noticed a
cloud in Mersenius.
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.
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.
Herodotus 1950 Mar 30 UT 19:00? Observed by Wilkins (Kent,
UK, 15" reflector) "Transient c.p. (similar phen. to
Bartlett's in later yrs.? see #532). NASA catalog weight=4
(good). NASA catalog ID #523. ALPO/BAA weight=3.
On 1997 Oct 13 at UT11:09-11:21 D. Rodway (Oamaru, South Island, New
Zealand, 8.5" reflector, x270) saw a deep salmon-pink colouration in
the south east corner interior of the crater Aristarchus. This colour
was confirmed by the observers wife. By 11:21 UT the colour had faded
completely. Rodway had been a lunar observer since 1958, using a wide
range of instruments from 3 inch refractors to 12 inch reflectors and
had observed a TLP in Gassendi back in 1966 (from L'ondon, UK), and so
was an experienced observer. The ALPO/BAA weight=4.
Herodotus 2022 Nov 06 UT 00:05-00:38 A. Anunziato (Parna,
Argentina - 105mm Meade EX 105, x154). Glimpsed an elongated
light patch on the floor, slightly east of the centre of the
floor. Observer was a bit uncertain if this was a genuine
observation, or a biased observation – based upon the written
account in the repeat illumination predictions. Detailed
sketch made. Anyway, seeing detail on the floor of Herodotus
was at the limit of his telescope. We shall therefore assign
an ALPO/BAA weight of 1.
On 1982 Aug 01 at UT20:50 M. Mobberley (Suffolk, UK, 14" reflector,
seeing III-IV) found that LaPlace A was significantly more prominent
than usual - comparisons were made with photographs in books. The
Cameron 2006 catalog ID=178 and weight=3. The ALPO/BAA weight=1.
Proclus 1990 Mar 09 UT 00:12-00:13 Observed by Marie Cook (Frimley, UK,
3.5" Questar telescope) observed a "long plume of light" the brightness
was the same as the wall region. It went from the southern rim about
half of the way across to the centre in the "northerly". The plume
feature was not seen at higher magnifications. Change in brightness
also noted. The Cameron 2006 catalog ID=394 and the weight=1. The
ALPO/BAA weight=1.
On 1993 Jun 02 at Ut 04:30-05:45 S. Beaumont (Cambridge, UK) saw that
the shadow of the Cobra's Head in Schroter's Valley was lighter and
more diffuse seen at user defined locations of C or B rim (these were
black versus medium gray for Cobra's Head). The TLP had vanished by
05:45UT. The Cameron 2006 catalog ID=462 and weight=3. The ALPO/BAA
weight=1 because the date or time is wrong.
On 1984 Nov 05 at UT18:00 Marshall (England) noted that there was no
normal brightening on the floor just next to the southern most
craterlet. The Cameron 2006 catalog ID=251 and the weight=2. The
ALPO/BAA weight=1.
On 1994 Apr 23 at UT02:41 D. Fryback (Madison, WI, USA) observed a
starlike flash in Alphonsus crater. The ALPO/BAA weight=2.
On 1994 Apr 23 at UT 03:30 the US Navy Clementine Spacecraft, in orbit
around the Moon, obtained images of the Cobra Head region of
Aristarchus crater that suggested a ~15x colour ratio increase (0.4
microns / 1.0 microns) in comparison with images obtained on 1994 Mar
03. This was presented as a poster paper 18.04 at AAS 31st DPS meeting.
However it was later suggested that this was due to incorrect
radimetric calibration procedures being followed. The ALPO/BAA
weight=1.
On 1985 May 31 at UT 20:23-22:00 G. North (Sussex, UK, turbulent
seeing) found Torricelli B at 20:23 to be mauve in colour and to be
very bright. However the colul had gone by 20:29UT. "Varied in albedo
2s then image blurred at 5-10s (atm) at 2034 became pink). At 21:35UT
M. Mobberley (Suffolk, UK) found a white patch in the crater centre and
a mag 8 flash was seen (confirmed independently by a 2nd observer ~
113km away)- there was no shadow. At UT 20:30 P.W. Foley (Kent, UK,
12"reflector, seeing excellent) found no colour, but the brightness was
changiong and he confirmed the bright patch on the crater's floor,
variable 22:15-22:25UT, "then expanded over rim". The Cameron 2006
catalog ID=277 and weight=5. the ALPO/BAA weight=4.
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 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.
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.
Oenopides-Selecucus 1951 Aug 15 UT 13:11 T,Osawa (Japan)
observed a brownish tinge to the terminator region in the
vicinity of these two craters. ALPO/BAA weight=1,
Aristarchus 1967 Sep 17 UTC 02:05-02:21 Observers: Delano (Fall River,
MA, USA) and Corralitos Observatory (Organ Pass, NM, USA). The former
used a 12.5" reflector at 400x and the latter a 24" reflector. The NASA
catalog states the following: "A rimtop cratelet on SW rim appeared
almost as bright as c.p. thru a Wratten 25 filter (red) but no brighter
than a lower central wall & rim thru a Wratten 48 (blue) filter. Inner
W. slope of craterlet displayed a bright red color which became less &
less noticeable until 0212h It was no longer brighter than other parts.
At 0217 it flared again brighter red for 1m. (indep. confirm. of
Seeliger for activity in Aris. ?) Corralitos MB did not confirm. NASA
catalog weight=4. NASA catalog TLP ID No. #1045.
ALPO/BAA weight=2.
Aristarchus 1982 Nov 28 UTC 23:35-23:55 Observed by Foley (Kent, UK,
Antionadi III, Transparency Moderate) - Colouration Seen - Ref: BAA
Lunar Section Circular. ALPO/BAA weight=2.
Aristarchus 1975 May 23 P.W. Foley (Wilmington, UK, 12"
reflector, x200, x360, x624, atmospheric clarity good, seeing
III from 20:15-22:30, but the clouded out at 22:30, and from
23:15-01:15 seeing was IV-V with poor transparency) observed
(22:20-20:45 UT) variation in the SE corner of the
Aristarchus, namely the usual dark bands were alternating
light to dark, not in keeping with otyher crater features.
This effect was not linked to atmospheric turbulence. Also
projected image of bands beyond the crater W. wall were
repeatedly noted. The observer broke away from observing at
20:45UT to make a telephonealert call. At 20:55UT they noted
that the area between Vallis Schroteri and Herodotus seemed
very light/bright, also the E. exterior of the crater wall of
Herodotus. From 21:01-21:11 A slight blueness was seen to
extend from the NE corner of Aristarchus, along the exterior
rim, acrossand beyond Herodotus to the SW. A tgorough search
was made of many bright areas, both near the terminator and to
the E., but no blueness could be detected elsewhere. A slight
orange hue was noted along the E. limb of theMoon (Spurious
colour). From 21:18;22:30 Aristarchus seemed normal again, and
likewise the head of Vallis Schoteri too. The observer was
clouded out from 22:30-23:15and from 23:15-01:30 the seeing
was so appaling that no colour or projection of the bands
could be seen. A Moon Blink was used during the session, but
no colour was detected in this? Another observer, R.W. Rose
(Devon, UK) observed 21:20-21:30 but had IV seeing, and saw
nothing unusual, but commented that if TLP wactivity had been
taking place, then they would probably not have seen it. The
ALPO/BAA weight=1.
Aristarchus 2015 Mar 03 UT 23:58 Brendan Shaw (UK) saw a flash
on the NW rim of Aristarchus on his computer screen - the camera
was working in the near IR. Seeing was not very good at the
time. Unfortunately this flash occurred in between imaging
sessions. No other flashes seen, despite looking. The observer
considerd the possibility that it might have been a cosmic ray
detection, but cannot say for sure. The ALPO/BAA TLP weight=1.
Colour seen between Aristarchus and Herodotus by P. Moore
and G. North. ALPO/BAA weight=3.
On 1964 Jun 23 at UT 04:45-05:05 Bartlett (Baltimore, MD, USA, 5"
reflector, x180, S=4-1 and T=3) observed a blue-violet glare on the
north east rim and a strong violet tinge in the nimbus. The effect was
absent 1 hour earlier. The Cameron 1978 catalog ID=821 and weight=4.
The ALPO/BAA weight=2.
On 1994 Apr 24 at UT 03:50 R. Manske (Waunakee, WI, USA) found that the
Cobra Head appeared to have an obscuration on the top eastern half. The
ALPO/BAA weight=2.
On 1992 Jan 18 at UT 22:34-23:48 A.C. Cook (Frimley, UK, 8" reflector,
seeing=III) was able to see 4 craterlets and two rays on the floor of
Plato. This was suprising because Moore, using a larger telescope and
magnification, was unable to see any detail here on 1991 Dec 12th at
02:10 - according to Cameron. The Cameron 2006 catalog ID=438 and the
weight=2. The ALPO/BAA weight=1.
On 1988 Apr 01 atUT01:15-03:20 H.Hill (Lancaster, UK, 10" reflector,
x286) observed that east of Lichtenberg were ëxtensive rosy areas"
around the northern edge of the lava sheet. Hill believes that it may
have been the same effect as seen by Madler (Germany), Barcroft (USA)
and Baum's (UK) 1951 observation. The colour was "ünmistakable" and
nothing to do with the atmospheric spurious colour. Other features were
checked. the cameron 2006 catalog ID=322 and the weight=3. THe ALPO/BAA
weight=2.
On 1892 May 10th at 19:00UT? Pickering, based at Arequipa. Peru, using
a 12" reflector, saw varitions in vapor col. Drawings were made. Time
calculated from the given colongitude. Cameron 1978 catalog ID= and
weight=3. ALPO/BAA weight=2.
Riccioli 1974 Jan 07 UT 16:30-17:00 Observed by McKay (South Downs,
England, 3" refractor, x135, S=IV boiling) "Bright spot and dark patch
changing in size (atmos. aberr. ?)" NASA catalog weight=1 (very low).
NASA catalog ID #1385.
Aristarchus 1982 Nov 29 UT 21:47 Observed by P. Madej
(Huddersfield, UK) flashes seen to NW. ALPO/BAA weight=1.
1969 Aug 26 UT 22:15-23:30 Observer: Whippey (Middlesex, UK,
6" reflector x177) "Small dark spot in oval whitish patch
typoical under high sun for it." NASA catalog weight=2. NASA
catalog ID #1200. ALPO/BAA weight=1.
Plato 1969 Aug 26 UTC 22:15-23:30 Observed by Whippey "Plato's
defuse white patch in center flanked by two radial diffused
bands diverging to S. wall. Later E. band disappeared under
better seeing. NASA catalog weight=2. ALPO/BAA weight=1."
During an eclipse of the Moon the crater appeared normal until it
emerged from the shadow. In the north east the dark floor was
not its normal hue and two light areas appeared to join. The
emerging patches became less and less bright, finally disappearing
at 0345 UT when the crater returned to normal. Cameron 2006 catalog
extension ID=10 and weight=2. ALPO/BAA weight=2.
1963Dec29/30 UT 22:00-03:00. Doherty (Small Thorne, UK) 8.5"
reflector, x110, x200 & x274, S=8-8.5, T=8, Moon 57 deg in alt)
and 3 others, using the same instrument, saw a bright purple-
blue patch in Aristarchus. Other areas checked for colour and
none sen elsewhere. Attempts were made to contact observers
elsewhere but with no success. Sketch made and shows the patch
covering the floor area of Aristarchus and extending out beyond
the east rim. Patch was elliptical in shape and the semi-major
diameter was approximately 2/3rds of the diameter of
Aristarchus, or about 27 km. The event lasted 5 hours and
gradually faded. NASA catalog weight=5 (very high quality)".
ALPO/BAA weight=4.
1982 Mar 08 Daniell UT 22:49-22:57 P.Madej (Hudersfield, UK) -
A colour and brightness anomaly was seen a TLP alert was put
out. Cameron 2006 catalog extension weight=165 and weight=3.
ALPO/BAA weight=2.
Aristarchus 1966 Jun 03 UT 01:00-01:45 Observed by Gordon (2), Delano
(Ackerman, PR?, 5" reflector / Massachussets, 3" (x92) & 10" reflector
T=4) "Deep blue color on N. wall. S.part of crater was brownish, (not
on alert). Delano saw E.wall bright spot unusually bright, confirm, ?"
NASA catalog weight=5. NASA catalog ID #947. ALPO/BAA weight=3.
On 1959 Mar 24 at UT 1851 Chernov (Russia) observed the follwing in
Oceanus Procellarum during a lunar eclipse: "During penumbra of ecl.
separate light pts. were sharply g?listing?. Possibly connected with
transparancy of the penumbra. (time given was 0851 UT but must have
been loc. time p.m. penum. phase started at 1756UT & umbral at
1916UT)". The cameron 1978 catalog ID=717 and weight=2. The ALPO/BAA
weight=1.
In 1950 Apr 02 at UT 20:00 Chernov (Russia) observed two dark spots in
Atlas during a penumbral phase of a lunar eclipse to quickly darken and
become sharp in detail. The cameron 1978 catalog ID=524 and weight=1.
The ALPO/BAA weight=1.
Gauss 1967 Sep 19 UT 02:33 Observer: Chilton (Hamilton, ON,
Canada, 12.5" Gregorian, 200x and a 4" refractor). In a polaroid
filter the west wall was missing. Effect seen in large scope and
also in 4-in finder. His conclusion was that W. wall reflected
polarized light. Cameron 1978 catalog weight=3 (good)
and TLP ID #1047. ALPO/BAA weight=4.
On 1982 Aug 04 at UT19:25 Arkhipov (Ukraine). found that for 3 minutes
Aristarchus brightened. Cameron 2006 catalog ID=180 and weight=0.
ALPO/BAA weight=1.
On 1982 Aug 04 at UT19:25 Arkhipov (Ukraine). found that for 5 minutes
Copernicus flashes. Cameron 2006 catalog ID=180 and weight=0. ALPO/BAA
weight=1.
On 1905 at Feb 19 at UT 18:00-19:03 Moye (Montpelier, France) observed
Aristarchus shining as a star in the dark, during a lunar eclipse. The
Cameron 1978 catalog ID=320 and he weight=3. The ALPO/BAA weight=3. The
ALPO/BAA weight=2.
On 1968 Apr 13 at UT05:00-05:45 Cameron and Laczo (Greenbelt, MD, USA,
6" refractor, x50, 36" reflector x400, 12" reflector x80, seeing=
excellent) observed for the folliwing craters: Aristarchus, Pytheas,
Euler?, Censorinus, Plinius?, Proclus, Menelaus, Manilius: "Star-like
pts. in the craters. Only Aris. identified certainly, rest fairly
certain except Euler & Plinius. Seen in 6-in refr. at 50x but not in
36-in refl. at 400x where they were bright, but not star-lie pts. Seen
later in 12-in refl. at 80x. In another bldg. Seen 1st @ 1/2h before
totality ended, but not earlier dur. tot. tho't by author (WSC) to be
geom. & instrumental = power effect". Chilton, K.E. reports in RASCJ
that another observer did not report any of what the Greenbelt observers
saw at all?The Cameron 1978 catalog ID=1065 and weight=4. The
ALPO/BAA weight=1.
On 1892 May 11 at 22:53UT an Unknown observer, during a partial eclipse
noticed an extension of the Earth;s shadow beyond the north cusp.
Cameron 1978 catalog ID=278 and weight=0. ALPO/BAA weight=1.
On 1892 May 11 at 22:53UT an Unknown observer, during a partial eclipse
noticed an extension of the Earth's shadow beyond the south cusp.
Cameron 1978 catalog ID=278 and weight=0. ALPO/BAA weight=1.
On 1975 Nov 18 at UT 19:38-23:34 Moore (Johannesburg, South Africa, 2"
refractor, S=II), Peters (Kent, UK, 8.5" reflector, x120, S=IV), Good
(Guilford, UK, binoculars), Foley (Dartford, Kent, UK, 12" reflector
and photographs), and McKay (Kingston, England, UK, 6" reflector, x48)
observed the following in Aristarchus during a lunar eclipse: "It
appeared much fainter than ever before seen in ecl. by Moore. Fainter
than Proc., Cop., & Tycho. Others rated brightness in order-- Hell,
Stevinus, Furnerius, proc.; & Proc., Tycho, Hell, Aris. Photos
confirmed dimness of it. For some observers it became invis. at S=II
(good). Good ranked at least 4 other craters brighter than Aris. & that
at 2035h it dimmed. Earthshine cond. extraordinarily good. Peters, at
S=IV (fair?) rated Aris. brightest". At 23:50UT LeCroy Jr and Sr
(Springfield, VA, 4.5" reflector, S=7) observed four glowing spots on
the Moon during a lunar eclipse (including Aristarchus). At 23:50UT
Aristarchus was an oval shape with no details seen. It had a ray
extending from the south west rim (normal). The north rim was slightly
blue and the south west rim very very slightly red. At 23:55UT it was
clearing and details showed. At 00:02UT it was clear. Sketches were
provided. Cameron comments that the colours fit Fitton's predictions on
spectral dispersion in our atmosphere from atmospheric inversions. The
brightness measued was 10+ and normal should be 9, and the plain is
4.5. The Moon's altitude at the LeCroy site was 45 deg. The Cameron
1978 catalog ID=1418-1420 and weight=5 (1-0 for LeCroy report). The
ALPO/BAA weight=3.
Aristarchus 1974 Jan 08/09 UT i18:15-00:00 Observed by
Billington (England), Robinson (Devon, England), Amery (REading,
England), Moore (Selsey, England) "Orange & viol. hue in crater
seen by Billington. Robinson, Amery & Moore reported neg. blink
results at this time. (Prob. chrom. aberr., Moore concurs)."
NASA catalog weight=0. NASA catalog ID #1386. ALPO/BAA weight=1.
On 1989 Aug 17 at UT 01:02-04:20 G. Kolvos (Thesaloniki, Greece,
4"reflector) measured (using photometry) that although there was a
gradual fade over the Moon as the eclipse progressed, there was a 2"%
rise in brightness of Aristarchus.Graphs were submitted and photos.
A.C. Cook supplied CCD images and CCD photometry. A photograph by
Conway (Sun Prarie, WI, USA) at the start of the eclipse reveal a
bright colourless spot (aparently confirmed). The Cameron 2006 catalog
ID=373 and weight=5. The ALPO/BAA weight=2.
In 1921 Oct 16 at UT 22:00-00:00 Genin and others (Russia) observed
during a partial eclipse that different parts of Aristarchus crater had
brightness of phosphorecence. Cameron says that this is independent
confirmation. The Cameron 1978 catalog ID=383 and weight=5. The
ALPO/BAA weight=3.
On 1893 Sep 25 at UT 21:00? Gaboreau (Paris, France), saw a shaft
of light projecting from the Moon. Cameron 1978 catalog ID=281
and weight=0. ALPO/BAA weight=1.
40.5W, 45.7N 1965 Nov 09 UTC 04:59 Observed by McCord (Mt Wilson, CA,
USA, 60" reflector + spectrograph) "Line depth anomaly, low compared
with 23 other areas". NASA catalog weight=5 (very high). NASA catalog
ID #912.
On 1988 Apr 03 at UT02:25-02:30 Culver (Harker Heights, X, USA, Meade
2045 reflector, x40, seeing=turbulent) detected flashes coming from
just north of the centre of Mare Tranquilitatis. Some of these flashes
were of a duration of seconds whilst others were several minutes.
Altogether ~20 flashes were seen, and not in the same place. "5 small
star-like points could be located - and there were lots of craterlets".
The spots were "lined up E-W at N of 10 deg latitude." Colour was not
visible on these nor variations. Apparently the observer had seen this
type of TLP before but had not reported them. The Cameron 2006 catalog
ID=323 and weight=2. the ALPO/BAA weight=2.
Mare Crisium 1965 Oct 11 UTC 07:32 Observed by McCord (Mt Wilson,
CA, 100" reflector + spectrogram) "Line depth ratios a/b (H),,
c/d (K) abnormally high compared with 23 other areas (including
Aristarchus?)." NASA catalog weight=5 (very high). NASA catalog
ID 902.
Mare Crisium 1965 Oct 11 UTC 10:10 Observed by McCord (Mt Wilson, CA,
100" reflector + spectrogram) "Line depth ratios a/b (H),, c/d (K)
abnormally high compared with 23 other areas (including
Aristarchus?)." NASA catalog weight=5 (very high). NASA catalog ID 902.
Aristarchus 1983 Oct 22 UT 22:00 G.W. Amery, (Reading, UK, Seeing
III-IV) found Aristrachus so bright that the CED was unable to
give a reading. The crater's interior was also diffuse in
appearance. The Cameron 2008 catalog ID=232 and weight=4. The
ALPO/BAA weight=3.
On 1958 Nov 01 at UT 00:00 a TLP was seen on the Moon (location and
observer not given). The Reference for this is Palm, 1967. The Cameron
1978 catalog ID=702 and weight=0. The ALPO/BAA weight=1.
On 1964 Jun 30 at UT 05:50-06:10 Bartlett (Baltimore, MD, USA) observed
the following in Aristarchus: "Nimbus only -- dark viol. hue. S. part
of Aris. floor was granualated & a brown tinge -- changed to yellow & a
brown tinge at 0500. First time he ever saw such a change in color.
(this obs.listed in 210 & MBMW as June 20, but is a misprint)". The
Cameron 1978 catalog ID=828 and weight=4. The ALPO/BAA weight=3.
Aristarchus 1976 Nov 13 UT 05:25 Observed by Bartlett (Baltimore, MD,
USA, 3" refractor, 54-200x, S=6, T=4) "Floor 8deg except S.=6deg which
is also granulated & la pale yellow. Different aspect fr. other obs. at
same col. Viol. in outer nimbus. Bright blue-viol. glare where viol.
radiance was on 11th. SWBS still large & 9 deg bright." NASA catalog
weight=4 (high). NASA catalog ID #1457.
On 1982 Aug 11 at UT03:30-04:15 Mobberley (Suffolk, UK) obtained a
photograph and made a sketch that revealed a needle-like shadow from
the west wall to near by the central craterlet - the latter was quite
clearly visible. What were not visible were the other four craterlets.
The Cameron 2006 catalog ID=183 and weight=4. The ALPO/BAA weight=2.