TLP Repeat Illumination/Libration and Earthshine predictions for: Greenland - Nuuk



Ill is percentage illumination of the Moon
*Indicates a repeat illumination and libration event to within +/- 1 deg for both
A non-* indicates just repeat illumination to within +/-0.5 deg


2026-Apr-01 UT 00:00-01:01 Ill=99% Gassendi observed by Kemp_A on 1972-2-27 *

     Gassendi 1972 Feb 27 UT 23:15-00:10 Observed by A.Kemp (Cheshire, 
     UK, 8.5" reflector x286) "Suspicion of blink between Gass. c.p. & 
     Gass A. Clouds prevented confirm. Hedley-Robinson didn't see 
     anything unusual earlier (20:00-20:20)." Note that the duration 
     of the event, or indeed precise UT at which it was seen is not 
     given. NASA catalog weight=1. NASA catalog ID #1324. ALPO/BAA 
     weight=1.


2026-Apr-01 UT 00:40-01:10 Ill=99% Torricelli_B observed by Mobberley_M on 1985-9-27

     On 1985 Sep 27 at UT 20:55 M. Mobberley (Suffolk, UK) found that the 
     brightness of Torricelli B varied and starlike points seen in the 
     crater. There is no Cameron 2006 catalog entry for this TLP report. The 
     ALPO/BAA weight=2.


2026-Apr-01 UT 02:23-03:22 Ill=99% Aristarchus observed by Cook_MC on 2007-4-30

     Interior bands were faint at 22:40 but sharper at 23:20.
     Observer noted some blue spurious colour to the north of
     Aristarchus but this had gone by 23:50.


2026-Apr-01 UT 02:23-03:22 Ill=99% Moltke observed by Cook_MC on 2007-4-30

     Observer noted some variability in the brightness of Moltke 
     and Torricelli B. This observation has an ALPO/BAA weight of 3.


2026-Apr-01 UT 02:23-03:22 Ill=99% Torricelli_B observed by Cook_MC on 2007-4-30

     Observer noted some variability in the brightness of 
     Torricelli B and Moltke. This observation has an
     ALPO/BAA TLP weight of 3.


2026-Apr-01 UT 03:40-06:47 Ill=99% Aristarchus observed by Livesey_R on 1996-10-25 *

     Aristarchus 1996 Oct 25 UTC 19:05-19:55 Observed by Livesey (Scotland, 
     65mm reflector x88) "red colour seen along E/SE rim and along S.edge of 
     SW ray - colouration not visible on other craters. Observations 
     terminated by hazy cloud drifting over Moon. Observer remarked that it 
     looked like chromatic aberation, but telescope was a reflector and no 
     colour was seen elswehere on the Moon. Cook (Frimley, Surrey, UK) 
     19:48-19:55 noted red on E. rim exterior and on SE part of central 
     peak, and blue on N. rim - strongly suspected spurious colour".
     ALPO/BAA weight=1. 


2026-Apr-02 UT 00:12-02:09 Ill=100% Torricelli_B observed by Foley_PW on 1985-9-28 *

     On 1985 Sep 28 UTC 20:54-23:52 P.W. Foley (Suffolk, UK) found (actually 
     before 20:54 UT) brightness variance in Torricelli B. J.D. Cook 
     (Frimley, UK) observed a brief blue coloured patch somewhere in the 
     Torricelli B region, but could not pin it down precisely. At 22:50UT 
     M.C. Cook (Frimley, UK, 30cm reflector, seeing III - occasionally V, 
     transparency moderate to good) Found the crater to have an elongated 
     appearance (in SSW-NNE direction) in white light, similar to the 
     previous night. A bright elongated spot was seen on the NNE floor, 
     close to where the wall should be. Not able to define the rim. There 
     was a very dark surrounding area to the crater, similar to what it was 
     on the previous night (roughly 1/4 brightness of Censorinus). 23:04UT 
     brighter in yellow, then red, then blue. At 23:10 it was seen that blue 
     filter dulled the crater - this was odd because both Censorinus and 
     Proclus were brighter in blue, which is what he would normally expect. 
     At23:15 UT Censorinus was brighter in blue, then yellow then red 
     filters and some orange spurious colour seen to the south of 
     Censorinus. At 23:23UT no spurious colour seen on Proclus or 
     Censorinus. 23:46UT Torricelli B elongated as before, but a very faint 
     ray might have been seen to the south west of the rim. This report is 
     not in the 2006 Cameron catalog. The ALPO/BAA weight=3.


2026-Apr-02 UT 05:10-07:19 Ill=100% Vallis_Schroteri observed by Pickering_WH on 1897-6-14 *

     On 1897 Jun 14 at UT 23:00 Pickering (Cambridge, Mass. USA) observed in 
     "Schroter's valley and the vicinity variations in vapor colum. Break in 
     col. toward F and eruption of crater D. 3.4 d after sunrise". The 
     Cameron 1978 catalog ID=389 and the weight=3. The ALPO/BAA weight=2.


2026-Apr-03 UT 01:09-01:39 Ill=99% Plato observed by Barker_R on 1938-1-17 *

     On 1938 Jan 17 Barker (Chestnut, England, UK, 12.5" reflector) 
     noticed that Plato crater had a brownish-gold veined surface, 
     colour irregular - laid on a smooth floor. It had extended 
     further E than on the previous night. The ALPO/BAA weight=2.


2026-Apr-03 UT 06:45-06:56 Ill=98% Aristarchus observed by Foley_PW on 1975-2-26 *

     Aristarcus 1975 Feb 26/27 UTC 21:00-00:30 Observed by: Foley (Kent, UK, 
     12" reflector), Kennedy (Dundee, UK, 8" reflector), Gannon (Middlesex, 
     UK, 6" reflector), Amery (Reading, UK, 10" reflector), Fitton 
     (Lancashire, UK, 8" reflector), Turner (Sussex, UK, 8" reflector) 
     "Foley) Neg. at 2100h. At 2123h NE wall was blue, decr. at 2220h. New 
     spot at 2221h due N. At 2227h blue fr. ENE to N. & faint blue on rim. 
     Interior clear detail, but obscur. at ENE-N, (Kennedy) at 2222h got 
     neg., also at 2229h-2300h. (Gannon) at 2245-2253h got neg. (Amery) at 
     2315h saw crater bright, bands clear, c.p. bright & very bright pt. to 
     NE of c.p. N. wall bluisg gray mist extending into N. part of crater. 
     Got slight blink in red till 2335h. (Fitton) at 2330h saw blue in N. 
     interior but no blink, no obscur. in long exam. Blue varied with 
     position in FOV. Polariz. with many rotations showed normal. Blue only 
     in Aris., none elsewhere till 2359h. (Turner at 2330h got neg. till 
     2359h. (Amery) at 2359h saw most detail clear. Blink distinct in red. 
     At 0030h(27th) saw blue mist now gray, seeing deteriorating. Herod. was 
     normal, (Fitton explains obs. as due to high press. system W. of
     obs with temp. inversions). NASA catalog weight=5 (very high). NASA 
     catalog ID #1399.


2026-Apr-19 UT 23:05-23:58 Ill=9% Aristarchus observed by Ward on 1821-5-4

     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.


2026-Apr-19 UT 23:05-23:26 Ill=9% Aristarchus observed by Darling_D on 1988-5-19

     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. 


2026-Apr-19 UT 23:05-23:39 Ill=9% Oceanus_Procellarum observed by Mugridge_P on 1990-4-27

     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.


2026-Apr-19 UT 23:11-00:04 Ill=9% Aristarchus observed by Horton_R on 1989-4-9

     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.


2026-Apr-19 UT 23:11-00:04 Ill=9% Copernicus observed by Horton_R on 1989-4-9

     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.


2026-Apr-19 UT 23:12-00:04 Ill=9% Tycho observed by Darling_D on 1989-4-9

     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.


2026-Apr-19 UT 23:23-00:04 Ill=9% S_Pole observed by Stolyarenko on 1912-6-17

     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.


2026-Apr-20 UT 23:08-00:25 Ill=17% W_Limb observed by Hopkins_BJ on 1883-3-12

     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.


2026-Apr-20 UT 23:08-23:39 Ill=17% Mare_Crisium observed by Braga_R on 1998-1-31

     Mare Crisium 1998 Jan 31 UT 17:15-17:35 R. Braga (Corsica 
     (MI), Italy, 102mm f8.8 refractor, x180, with no diagonal, 
     seeing II, Transparency poor). A very bright point located at 
     23N 54.5E this was normal! - what was unusual was that it 
     vanished when viewed through a blue Wratten 38A filter (this 
     filter absorbs red, UV, and some green light). The ALPO/BAA 
     weight=2.


2026-Apr-20 UT 23:13-01:06 Ill=17% Aristarchus observed by Darling_D on 1980-10-12

     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.


2026-Apr-21 UT 00:37-01:26 Ill=17% Aristarchus observed by Argelander on 1825-4-22

     In 1825 Apr 22 at UT0030 Argelander (England) and Gobel (Koburg, 
     Germany) saw the following in the vicinity of Aristarchus: "Points of 
     light in center. In low magn. appeared as a small star, somewhat 
     scintillating. At higher magn. became larger & diffused. (date 1824 ? 
     Ref. refers to a ref. dated 1824 -- If so age would have been 23rd" 
     Cameron 1978 catalog ID=107 and weight=5. ALPO/BAA weight=3.


2026-Apr-21 UT 00:40-01:26 Ill=17% Aristarchus observed by Darling_D on 1989-4-10

     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


2026-Apr-21 UT 00:17-03:57 Ill=18% Earthshine: Lyrids: ZHR=15 (vel=47km/s) & Pi Puppids: ZHR=var (vel=18km/s)

2026-Apr-21 UT 23:11-00:15 Ill=26% Aristarchus observed by Ward on 1821-5-6

     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.


2026-Apr-21 UT 23:11-23:39 Ill=26% Cassini observed by Arkhipov on 1937-2-15

     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.


2026-Apr-21 UT 23:11-23:54 Ill=26% Aristarchus observed by Andrenko on 1939-2-23

     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.


2026-Apr-21 UT 23:11-00:44 Ill=26% N_Pole observed by Wilkins_HP on 1953-4-18

     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.


2026-Apr-21 UT 23:11-00:44 Ill=26% S_Pole observed by Wilkins_HP on 1953-4-18

     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.


2026-Apr-21 UT 23:11-23:18 Ill=26% Aristarchus observed by Whelan on 1969-7-19

     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.


2026-Apr-21 UT 23:11-00:11 Ill=26% Messier observed by Evans_D on 1981-9-3

     Messier 1981 Sep 03 UT 19:15-19:55 Observed by Evans (England, 254mm 
     Newtonian, seeing II-III, transparency fair). "Messier was under going 
     obscuration" BAA Lunar Section Circular report. ALPO/BAA weight=1.


2026-Apr-22 UT 00:21-04:00 Ill=28% Earthshine: Lyrids: ZHR=15 (vel=47km/s) & Pi Puppids: ZHR=var (vel=18km/s)

2026-Apr-22 UT 23:14-23:51 Ill=37% Aristarchus observed by Whelan on 1969-7-20

     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.


2026-Apr-22 UT 23:14-00:15 Ill=37% Earthshine observed by Weith_Knudson on 1974-2-27

     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.


2026-Apr-22 UT 23:14-00:49 Ill=37% Daniell observed by Price_M on 1979-12-24

     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.


2026-Apr-22 UT 23:14-23:28 Ill=37% Proclus observed by Haas_W on 2003-9-2

     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.


2026-Apr-22 UT 23:39-01:36 Ill=37% Aristarchus observed by McIntosh on 1969-7-20

     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.


2026-Apr-23 UT 00:26-02:18 Ill=38% Mare_Crisium observed by Kidger_M on 1975-3-18

     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.


2026-Apr-23 UT 00:54-02:36 Ill=38% Limb observed by Challis on 1859-5-8

     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.


2026-Apr-23 UT 02:06-03:11 Ill=38% W_Limb observed by Webb_TW on 1855-6-20

     In 1855 Jun 20 at UT 21:00 T.W. Webb (England) observed a trace of 
     twilight (Cameron says also seen by Gruithuisen, Henry and others at 
     times). Webb gives a low weight to his own observation, saying "for 
     want of better optical means". The Cameron 1978 catalog ID=130 and 
     weight=1. The ALPO/BAA weight=1. 


2026-Apr-23 UT 00:24-03:49 Ill=39% Earthshine: Lyrids: ZHR=15 (vel=47km/s) & Pi Puppids: ZHR=var (vel=18km/s)

2026-Apr-23 UT 23:18-00:35 Ill=49% Sabine observed by Jean on 1967-9-11

     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.


2026-Apr-23 UT 23:18-23:21 Ill=49% Theophilus observed by Ruchatz on 1972-5-19

     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.


2026-Apr-23 UT 23:18-23:50 Ill=49% Censorinus observed by Cook_AC on 1985-6-24

     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.


2026-Apr-23 UT 23:18-23:56 Ill=49% Proclus observed by Haas_W on 2003-9-3

     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.


2026-Apr-23 UT 23:18-00:10 Ill=49% Descartes observed by Bryukhanov_I on 2010-4-20

     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.


2026-Apr-23 UT 23:28-01:20 Ill=49% Proclus observed by Unknown_Observer on 1988-7-21

     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.


2026-Apr-24 UT 00:27-02:24 Ill=49% Maskelyne observed by Whelan on 1969-7-21

     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.


2026-Apr-24 UT 00:33-02:28 Ill=49% Posidonius observed by Osawa on 1969-5-23

     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.


2026-Apr-24 UT 00:46-02:27 Ill=49% Menelaus observed by Whelan on 1970-4-13

     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.


2026-Apr-24 UT 00:28-03:37 Ill=50% Earthshine: sporadic meteors

2026-Apr-24 UT 23:21-00:13 Ill=60% Alphonsus observed by Warner_B on 1960-1-6

     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.


2026-Apr-24 UT 23:21-23:30 Ill=60% Alphonsus observed by Harris on 1966-6-26

     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.


2026-Apr-24 UT 23:21-23:47 Ill=60% Archimedes observed by Try on 2001-9-25

     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.


2026-Apr-24 UT 23:30-01:16 Ill=60% Jansen observed by deBerard on 1966-8-24

     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.


2026-Apr-25 UT 00:03-01:53 Ill=60% Proclus observed by Foley_PW on 1988-7-22

     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.


2026-Apr-25 UT 00:29-04:24 Ill=60% Mons_Pico observed by Adee_J on 2008-4-13 *

     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.


2026-Apr-25 UT 00:34-04:29 Ill=60% Montes_Apenninus observed by Armitage_J on 2008-4-13 *

     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.


2026-Apr-25 UT 00:53-02:50 Ill=60% Ptolemaeus observed by Firsoff on 1954-5-10

     Flash seen in Ptolemaeus (A?) - possibly a meteor. Cameron 1978
     catalog weight=1. Cameron 1978 catalog ID=863.


2026-Apr-25 UT 00:53-02:50 Ill=60% Herschel observed by del_Valle_D on 2005-8-13

     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.


2026-Apr-25 UT 00:56-02:41 Ill=60% Arzachel observed by Barcroft on 1941-1-6

     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. 


2026-Apr-25 UT 02:11-03:46 Ill=61% Proclus observed by Dean on 1970-7-11

     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.


2026-Apr-25 UT 02:11-03:46 Ill=61% Secchi observed by Dean on 1970-7-11

     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.


2026-Apr-25 UT 02:25-03:46 Ill=61% Eimmart observed by Louderback_D on 1983-9-15

     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.


2026-Apr-25 UT 03:45-03:46 Ill=61% Purbach observed by Osawa on 1970-4-14

     Purbach 1970 Apr 14 UT 12:00-14:00 Observed by Osawa (Awajt-Shima, 
     Japan, 8" reflector, x288) "Photos in blue and orange taken. Ill-
     defined obscur. in blue photo in S. part of crater compared with 
     orange. (neg. is so faint it is doubtful. Apollo 13 watch. Similar to 
     Alter's findings in Alphonsus)." NASA catalog weight=2 (low). NASA 
     catalog ID #1250.


2026-Apr-25 UT 23:24-00:58 Ill=70% Alphonsus observed by Wilkins_HP on 1958-12-19

     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.


2026-Apr-26 UT 00:54-02:51 Ill=71% Eratosthenes observed by Cattermole_P on 1954-5-11

     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.


2026-Apr-26 UT 01:01-02:58 Ill=71% Alpetragius observed by Barnard on 1889-9-4

     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.


2026-Apr-26 UT 01:43-03:29 Ill=71% Proclus observed by Darling_D on 1988-7-23

     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. 


2026-Apr-26 UT 01:46-02:30 Ill=71% Plato observed by Marshall_KP on 1982-11-24

     Plato 1982 Nov 24 UT 22:00-23:30. K.P. MArshall (Columbia, 12" 
     reflector, x100, x200, x480, seeing III, reasonably steady, but 
     some turbulence. No craters could be seen on Plato's floor, 
     despite observing conditions being acceptable. The floor was 
     evenly toned, and the walls were sharply defined. By 23:10 there 
     was a suspicion that the central craterlet was there, but he 
     could not quite make it out, even with averted vision. ALPO/BAA 
     weight=1.


2026-Apr-26 UT 01:46-03:36 Ill=71% Tycho observed by North_G on 1995-3-10

     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.


2026-Apr-26 UT 02:07-03:46 Ill=71% Plato observed by Cragg on 1952-4-4

     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.


2026-Apr-26 UT 02:57-03:46 Ill=71% Censorinus observed by Iwanoff on 1972-4-22

     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.


2026-Apr-26 UT 03:42-03:46 Ill=72% Kepler observed by Morales on 1884-2-5

     Morales of France?, observed "an illumination" in Kepler on 1884 Feb 05 
     at UT20:00?. The Cameron 1978 catalog ID is 241 and the weight=1. The 
     ALPO/BAA weight=1.


2026-Apr-26 UT 23:27-00:14 Ill=79% Agrippa observed by Bartlett on 1967-7-17

     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.


2026-Apr-26 UT 23:55-01:46 Ill=79% Plato observed by Robinson_JH on 1974-3-3

     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.


2026-Apr-27 UT 00:42-02:24 Ill=80% Proclus observed by Darling_D on 1988-7-24

     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.


2026-Apr-27 UT 00:45-02:29 Ill=80% Plato observed by Madej_P on 1981-9-8

     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. 


2026-Apr-27 UT 01:56-03:12 Ill=80% Dawes observed by Porter on 1973-2-12

     Dawes 1973 Feb 12-23 UT 22:30-01:20 Observed by Porter (Narragansett?, 
     RI, USA, 6" reflector x96, S=9, T=0-4, alt=55-75deg?) "Brightening of 
     some of permanent pts. monitored while others stayed steady & normal 
     brightness. (Other nites' obs. suggest that he saw end of dimming event 
     & return to normal). Distinct fluctuations." NASA catalog weight=4 
     (good). NASA catalog ID #1361.


2026-Apr-27 UT 23:30-00:09 Ill=87% Anaximander observed by Olivares on 1963-11-27

     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.


2026-Apr-27 UT 23:30-00:09 Ill=87% Aristarchus observed by Olivares on 1963-11-27

     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.


2026-Apr-27 UT 23:36-01:31 Ill=87% Gassendi observed by Cook_AC on 1979-12-29

     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.


2026-Apr-28 UT 01:14-03:02 Ill=87% Jansen observed by Lourencon on 1991-5-24

     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. 


2026-Apr-28 UT 01:20-03:04 Ill=87% Alphonsus observed by Harris on 1966-8-27

     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.


2026-Apr-28 UT 01:20-03:04 Ill=87% Ross_D observed by Harris on 1966-8-27

     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.


2026-Apr-28 UT 02:01-03:04 Ill=88% Proclus observed by Davis_H on 1988-7-25

     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.


2026-Apr-28 UT 02:36-03:04 Ill=88% Calippus observed by Frank on 1973-2-13

     Callipus and vicinity 1973 Feb 13 UT 23:16-23:50 Observed by Frank 
     (E.Pepperell, Massachusetts, USA, 6" reflector x100, Seeing=good, 
     altitude=45 deg). "Large dark patch, albedo=3 present E. of Calippus. 
     Drawing. (Shows it into Callippus also). Never seen before or since. 
     Albedo normal (4.5) at 2350h. (obs. monitors Callippus in ALPO-LTP 
     program)." NASA catalog weight=3 (average). NASA catalog ID #1362.


2026-Apr-29 UT 23:36-00:45 Ill=97% Aristarchus observed by Seeliger on 1967-9-16 *

     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. 


2026-Apr-29 UT 23:36-03:00 Ill=97% Aristarchus observed by no on 1967-9-17 *

     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.