TLP Repeat Illumination/Libration and Earthshine predictions for: Australia TAS Hobart



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


2025-Dec-01 UT 09:28-09:44 Ill=82% Furnerius observed by Cameron_W on 1961-5-26 *

     Furnerius 1961 May 26 UT 02:20-03:00 Observed by Cameron (Aldephi, MD, 
     USA, 3.5" Questar reflector x160, S=G) "Crater stood out like 
     glittering points (small craters on rim?). Many features examined but 
     effect seen only on this crater and Stevinus (Specular refl. from flat 
     surface?)" NASA catalog weight=1 (very low). NASA catalog ID #738.


2025-Dec-01 UT 09:28-11:20 Ill=82% Gassendi observed by Duckworth on 1969-11-20

     Gassendi 1969 Nov 20 UT 17:06-17:15 Observed by Duckworth 
     (Manchester, England, 8" refractor x250) Faint Pinkish 
     Obscuration on floor. Event in progress at 1706 - left telescope 
     at 1715 to report it, but TLP gone upon return. Gassendi was 
     normal from from 1734-1822h. NASA catalog weight=4. NASA catalog 
     ID #1223. ALPO/BAA weight=3.


2025-Dec-01 UT 09:28-09:58 Ill=82% Plato observed by Watkins_E on 1971-9-30

     Plato 1971 Oct 30 UT 19:35-20:55 E.Watkins (Braintree, UK, 4.5" 
     reflector, x45,x150, x225), thought he saw a faint patch at 
     19:35 and it still was visible at 19:40. At 19:50-19:55 he saw 
     what may have been the remainder. At 20:55 he noticed a shadow 
     in the area. ALPO/BAA weight=1.


2025-Dec-01 UT 09:28-11:25 Ill=82% Plato observed by North_G on 1980-5-25

     Plato 1980 May 25 UT 21:33-22:54 Observed by North (Seaford, 
     UK, seeing III-IV, 460mm Newtonian) Definite strong reddish 
     glow along NNW border, definitely much stronger than spurious 
     colouration and always visible when telescope moved in RA and 
     Dec to eliminate possible chromatic aberation effects in the 
     eyepiece. Effect ended by 21:54 UT. BAA Lunar Section Report. 
     ALPO/BAA weight=2.


2025-Dec-01 UT 10:40-12:36 Ill=83% Hyginus_N observed by Wilkins_HP on 1944-4-4

     Hyginus N 1944 Apr 04 UT 20:00? Observed by Wilkins (Kent, England, 
     15" reflector) "Darker than usual. S. edge of great crater valley was 
     bordered by a narrow dark band for 13km along its length" NASA catalog 
     weight=4 (high). NASA catalog ID #490.


2025-Dec-01 UT 11:48-13:44 Ill=83% Gassendi observed by Becker on 1969-11-20

     Gassendi 1969 Nov 20 UT 19:30-19:45 Observed by Becker (Holland, 4" 
     refractor) "Curious small shadow from NW (ast. ?) wall. (Apollo 12 
     watch)" NASA catalog weight=1 (very low). NASA catalog ID #1224.


2025-Dec-01 UT 12:03-13:51 Ill=83% Aristarchus observed by Becker on 1969-11-20

     Aristarchus 1969 Nov 20 UT 19:45-20:05 Observed by Becker (Holland, 4" 
     refractor) "Sharp whiteness on inner W. (ast. ?) side (Apollo 12 
     watch)" NASA catalog weight=1 (very low). NASA catalog ID #1224.


2025-Dec-01 UT 12:22-13:51 Ill=83% Ross_D observed by Cross on 1965-3-14

     SE of Ross D 1965 Mar 14 UT 07:40 Observed by Cross (Whittier, 
     CA?, USA, 12" reflector). Crater wall partially obscured; 
     bright area. NASA catalog weight=3. NASA catalog ID #872. 
     ALPO/BAA weight=3.


2025-Dec-01 UT 12:33-13:51 Ill=83% Plato observed by Birt_WR on 1870-5-11

     Plato 1870 May 11 UTC 22:00 Observed by Birt (England) "Extraordinary 
     display of lights. Says not effect of sunlight" NASA catalog weight=4 
     (high). NASA catalog ID #167.


2025-Dec-01 UT 12:41-13:44 Ill=83% Aristarchus observed by Armitage_J on 2006-2-9

     Observer noted a bright spot on the interior west wall that seemed
     brighter than what they would have expected. unfortunately the precise
     time of this observation was not recorded so the moon-rise and 
     midnight UT values are used to place a limit on the time of 
     observation. Images by Shaw taken at UT 1754, 18:45 and 23:13
     do not exhibit the effect.


2025-Dec-01 UT 13:04-13:51 Ill=83% Censorinus observed by Cook_MC on 1981-4-15

     Censorinus 1981 Apr 15 UT 22:15-23:10 M. Cook (Frimley, UK), 
     using a 12" reflector,found Censorinus to be glowing exceedingly 
     bright and was brighter than Proclus. It dulled later, but was 
     still brighter than Proclus. Censorinus was also slightly 
     brighter in blue than in red light. Cameron 2006 catalog 
     extension ID=130 and weight=3. ALPO/BAA weight=1.


2025-Dec-01 UT 13:27-13:51 Ill=83% Aristarchus observed by Taboada on 1968-12-31

     Aristarchus-Herodotus 1968 Dec 31 UT 03:30-03:45 Observed by Taboada 
     (Mexico) "Terminator between the two was diminishing in brightness over 
     edge of Herod. at 0345, 2 darker spots seen over same place. (alerted 
     by Middlehurst for tidal predict.?)" NASA catalog weight=1 (very low). 
     NASA catalog ID #1112.


2025-Dec-01 UT 13:27-13:51 Ill=83% Herodotus observed by Taboada on 1968-12-31

     On 1968 Dec 31 at UT 03:30-03:45 Taboada (Mexico) observed the 
     terminator between Aristarchus and Herodotus was diminishing in 
     brightness at 03:45UT over the edge of Herodotus. Two darker spots were 
     seen over same place. Alerted by Middlehurst for tidal predict? The 
     Cameron 1978 catalog ID=1112 and weight=1. The ALPO/BAA weight=1.


2025-Dec-02 UT 09:29-11:37 Ill=90% Kepler observed by Lugo on 1954-11-7 *

     Kepler 1954 Nov 07 UT 23:20 Observed by F.A. Lugo (Caracus, 
     Venezuela, 3.5" scope x125) Bright red star=like point just 
     outside E.wall - visible for an hour. NASA catalog weight=3. 
     NASA catalog ID #580. ALPO/BAA weight=3.


2025-Dec-02 UT 09:29-10:51 Ill=90% Aristarchus observed by Gabriel on 1972-10-19

     Aristarchus 1972 Oct 19 UT 17:55-18:05 Observed by Gabriel (Wettern, 
     Belg. 4" refractor, x166, S=E), Hitchens (Stamine Locks, Eng., 8.5" 
     reflector, S=F), Peters (Kent, Eng., 10" relector), Amery (Reading, 
     Emg. 10?" reflector), Flynn (england, 12" reflector) "At 17:55h noted 
     bluish-purple color area just N. of Aris. & it reached just over N. 
     wall, lasted 2 min. At 1800h color noted again, but not as brilliant & 
     gone at 1801h. Seen again at 1804h & now was on E. (ast. ?) wall,
     lasting M 1min. Sure of its reality but not of lunar origin. All gone 
     at 1805h. Hitchens noted a very bright spot on W. (IAU?) wall between 2 
     prominent bands. Blue darkening in W#38 filter, neg. in W#8,25,58 & 
     integrated light. Other areas gave similar but lesser effects. May be 
     due to damp geletin. (Moore thinks not LTP but many obs. have rep't 
     blue in Aris.) Others obs. later (2100, 2215-2300, 2305h) & noted 
     nothing unusual." NASA catalog weight=2 (low). NASA catalog ID #1346.


2025-Dec-02 UT 09:29-10:14 Ill=90% Aristillus observed by Berger on 1972-12-17 *

     Aristillus 1972 Dec 17 UTC 21:50-22:20 observed by Berger (51.5N, 9E, 
     60mm refractor, T=2, S=3) "Diffuse bright cloud in the NE corner of the 
     crater" - Hilbrecht and Kuveler, Earth, Moon & Planets, 30 (1984), p53-
     61.


2025-Dec-02 UT 09:29-09:34 Ill=90% Daniell observed by Crick on 1979-7-6

     Daniell 1979 Jul 06 UT 21:15-22:30 Crick (Belgium, 6" 
     reflector, Seeing=II and transparency=good.) noticed 
     obscuration on a bright spot on the south east wall. This spot 
     was quite prominent through a red Wratten 25 filter. The floor 
     was very dark. Other craters were checked and were normal. A 
     sketch was supplied and the position was the same as in other 
     earlier reports. Cameron 2006 catalog extension ID=60 and 
     weight=3. ALPO/BAA weight=3. 


2025-Dec-02 UT 09:29-10:28 Ill=90% Mons_Piton observed by Foley_PW on 1984-3-14 *

     Mons Piton 1984 Mar 14/15 UT 19:18-01:48 Observed by Foley
     (Kent, England, 12" Reflector seeing I, Transparency Very 
     Good) "Colouration and brightness seen on Piton (CED used)" 
     BAA Lunar Section Report. ALPO/BAA weight=1.


2025-Dec-02 UT 09:29-10:28 Ill=90% Plato observed by Foley_PW on 1984-3-14 *

     Plato 1984 Mar 14/15 UT 19:18-01:48 Observed by Foley (Kent, 
     England, 12" Reflector seeing I, Transparency Very Good) 
     "Obscuration and colour seen on Plato" BAA Lunar Section 
     Report. ALPO/BAA weight=2.


2025-Dec-02 UT 09:29-09:51 Ill=90% Plato observed by Cook_MC on 1987-2-10

     Plato 1987 Feb 10 UT 21:05-22:10. M. Cook (Frimley, UK), "NE 
     ray distinct & also floor E of it, not distinct as on Dec 13 & 
     Jan 11, while March 10, 11 & 12 seen by Price, North, Peters, 
     Foley & M Cook, where rim was clear and sharp." - quote from 
     the 2006 Cameron Catalog extension - TLP ID=297 and weight=5. 
     Cameron gives the observers confirming this TLP as: M. Cook, 
     G. North and Davies. ALPO/BAA weight=2.


2025-Dec-02 UT 09:29-11:17 Ill=90% Herodotus observed by Beaumont_S on 1993-9-28

     On 1993 Sep 28 at UT 04:30-06:10 S.Beaumont (Cambridge, UK)observed 
     that the north east edge of Herodotus appeared as a "highland area 
     spilling over into" the Cobra's Head border or "overlook". The shadow 
     on the elevation was contiguous with a similar shadow over the Cobra's 
     Head "like a darkening of the terrain. Shadow appears softer diffused 
     without sharp bounds of most Lunar shadows. sketch. S. edge of crater 
     started to appear at 0615". The Cameron 1978 catalog ID=468 and the 
     weight=2. The ALPO/BAA weight=1 as the date or UT are wrong.


2025-Dec-02 UT 11:09-13:06 Ill=91% Plato observed by Taylor on 1972-10-19

     Plato 1972 Oct 19 UT 20:10 Observed by Taylor, Phillips, Ford, Kennedy 
     (Dundee, Scot. 10" refractor) "Taylor noted a slight blink on NW wall. 
     Ford said it was neg. Phillips was not sure. Taylor returned to 
     telescope & no blink. Kennedy reported neg." NASA catalog weight=1 
     (very low). NASA catalog ID #1347.


2025-Dec-02 UT 11:34-13:31 Ill=91% Aristarchus observed by Foley_PW on 1981-4-16

     Foley, Kent, UK noted that the floor was slate blue-grey
     with no colour seen elsewhere. 12" reflector used, seeing=II.
     Cameron 2006 extension catalog ID 131 and weight=1. ALPO/BAA
     weight=1.


2025-Dec-02 UT 12:40-14:01 Ill=91% Plato observed by Birt_WR on 1870-5-12

     Plato 1870 May 12 UTC 22:00 Observed by Birt (England) 
     "Extraordinary display of lights. Says not effect of sunlight" 
     However an article by Nigel Logshaw in the Feb 2014 LSC suggests 
     that it was probably just normal fine scale spots and streaks on 
     the floor of the crater. NASA catalog weight=4. ALPO/BAA weight=
     1. NASA catalog ID #167.


2025-Dec-02 UT 12:45-14:01 Ill=91% Plato observed by Cook_AC on 1986-12-13

     Plato 1986 Dec 13 UT 20:30 Observed by A. Cook (Frimley, UK, 
     seeing III) North East quadrant of Plato the crater was blurred 
     and ill-defined. Also no craterlets visible anywhere on the 
     floor of Plato until the central craterlet was just glimpsed 
     later at 23:00-23:45, though seeing now III-IV (cirrus at times 
     in the sky). At this later time the NE rim was less blurred than 
     before. ALPO/BAA weight=1.


2025-Dec-02 UT 12:59-14:01 Ill=91% Vallis_Schroteri observed by Bestwick on 1955-9-28

     Cobra Head 1955 Sep 28 UTC 23:00 Observed by Bestwick (England? 6?" 
     reflector x240) "Diffused brown patch of smoke or vapor, almost 
     obscured -- appeared over plain for a short distance."NASA catalog 
     weight=3. NASA catalog ID #612.


2025-Dec-02 UT 13:12-14:01 Ill=91% Herodotus observed by Taboada on 1969-1-1

     Herodotus 1969 Jan 01 UT 03:15 Observed by Taboada (Mexico) 
     "Brightness in edge of crater dimmed & a heavy darkness was 
     noted thru course of cleft (Schroter's Valley?). (alerted for 
     tidal predict.?)"NASA catalog weight=1. NASA catalog ID #
     1113. ALPO/BAA weight=1.


2025-Dec-02 UT 13:53-15:53 Ill=91% Herodotus observed by Zeller_P on 2016-7-17 *

     On 2016 Jul 17 UT 03:49 P.Zeller (ALPO, Indianapolis, IN, USA) 
     imaged a pseudo-peak with shadow on the floor of Herodotus, 
     however the image scale and quality of this colour image were 
     not great and the observer suspects that it might be an 
     imaging artefact. ALPO/BAA weight=1.


2025-Dec-03 UT 10:43-12:35 Ill=96% Aristarchus observed by Cutts on 1969-11-22

     Aristarchus 1969 Nov 22 UT 18:20-21:13 Observed by D. Cutts 
     (Chester, Eng., 8.5" reflector, x200), Moore (Sussex, Eng., 12" 
     reflector x425), Miles (Coventry, Eng. 5" refractor), Delaye and 
     Jourdran (Marseilles, Fr., 8" reflector) "Pulsating patch on W. 
     wall between 2 radial bands. Faded by 2000h. Returned to normal. 
     (Cutts). Miles saw strong pink in whole interior at 2112h. 
     Strong blink. No blink there at 2210-2212h. Gass., Grim., & 
     Plato were neg. Delaye & Joudan photog. it as very bright. Moore 
     got neg. results at 2135. (confirm. of activity?, Apollo 12 
     watch)." NASA catalog weight=5. NASA catalog ID #1226. ALPO/BAA 
     weight=3.


2025-Dec-03 UT 10:43-11:24 Ill=96% Aristarchus observed by Foley_PW on 1975-9-18

     Aristarchus 1975 Sep 18 UT 21:00? Observed by Foley (Kent, 
     England, 12" reflector) "Deep blue-viol. spot in NW (IAU?) 
     interior corner." NASA catalog weight=3. NASA catalog ID #1414. 
     ALPO/BAA weight=3.


2025-Dec-03 UT 12:47-14:06 Ill=97% Plato observed by Pratt_H on 1870-5-13

     Plato 1870 May 13 UT 22:00? Observed by Pratt (---), Elger (Liverpool, 
     England), (Gledhill (Brighton, England) "Extraordinary display of 
     lights. 27 seen by Pratt, 28 by Elger, only 4 by Gledhill. (independ. 
     confirm. ?" NASA catalog weight=5 (very good) NASA catalog ID #168.
     A bit more of a detailed report is as follows: "Upon the 13th of May, 
     1870, there was an "extraordinary display," according to Birt: 27 
     lights were seen by Pratt, and 28 by Elger, but only 4 by Gledhill, in 
     Brighton. Atmospheric conditions may have made this difference, or the 
     lights may have run up and down a scale from 4 to 28. As to 
     independence of sunlight, Pratt says (Rept. B.A., 1871-88), at to this 
     display, that only the fixed, charted points so shone, and that other 
     parts of the crater were not illuminated, as they would have been to an 
     incidence common throughout.(30) In Pratt's opinion, and, I think, in 
     the opinion of the other observers, these lights were volcanic." 
     ALPO/BAA weight=4.


2025-Dec-03 UT 12:49-14:06 Ill=97% Aristarchus observed by Mobberley_M on 1981-4-17

     Mobberley of Suffolk, UK, and using a 14" reflector and
     seeing=I-II saw yellowish/brown streaks within Aristarchus. A
     sketch indicates that these extended from a region on the east
     floor to the north west corner, and then finally onto the
     bands on the west wall. Cameron 2006 extension catalog ID=132
     and weight=4. ALPO/BAA weight=1.


2025-Dec-07 UT 15:58-17:49 Ill=89% Madler observed by Wildey on 1962-4-22

     Madler 1962 Apr 22 UTC 08:24 Observed by Wildey, Pohn (1st measurement) 
     (Mt Wilson, CA, USA, 60" reflector with photometer) "Photometric 
     measures show change in brightness from Vmag=3.79 to V=4.40. The 
     average brightness for age 17d is V=3.99. Crater faded from .2 mag 
     brighter than av. to .4 mag. fainter (@1.5 times fainter) than av., a 
     range of .6 magnitude, or @ 1.5 times diff. in brightness". NASA 
     catalog weight=5 (very high). NASA catalog ID #757.


2025-Dec-07 UT 15:58-17:26 Ill=89% Cleomedes observed by North_G on 1993-9-3

     Cleomedes Alpha 1993 Sep 03 UT2200-22:20 G. North (UK, 18.25" 
     reflector, x86 & x144) observed it to be a strikingly brilliant 
     'splodge' seen in the mostly shadow filled interior of 
     Cleomedes, and around this splodge was a faint halo extending 
     symetrically in an eastwards direction. The splodge was the 
     mountain Cleomedes Alpha. Strangely no shadow from the mountain 
     was seen to be cast onto the halo on the east. Observer alerted 
     other observers by phone, and upon returning to the scope found 
     that the splodge had faded in brightness and continued to fade 
     over the next hour as one would expect from a mountain at 
     sunset. Some heavy spurious colour was present. J. Cook & M. 
     Cook (Frimley, UK) observed at 22:20-22:25 and found the bright 
     splodge, but no halo. M. Cook re-observed later and confirmed 
     normal fading of splodge. Roscoe observed from 00:30UT next day, 
     but by that time Cleomedes Alpha had set and was no longer 
     visible in the shadow filled floor. S. Beaumont had observed 
     earlier at 20:00 but had recorded all as normal in Cleomedes. 
     The Cameron 2006 catalog ID=466 and weight=5. 
     The ALPO/BAA weight=2.


2025-Dec-08 UT 15:52-16:32 Ill=81% Eratosthenes observed by Haas_W on 1936-10-4

     1936 Oct 04 UT07:42 W.Haas drew bands, many smaller spots on 
     floor. Pickering's atlas 9D col 141 shows bands but no bright 
     spots. Haas' location Aliance, OH, USA. Reference: Haas, W. 
     J.Royal Astr. Soc. Canada. Cameron 1978 catalog ID=416 and 
     weight=3. ALPO/BAA weight=2.


2025-Dec-08 UT 18:04-18:30 Ill=81% Aristarchus observed by Bartlett on 1955-10-5

     In 1955 Oct 05 at UT 03:40-03:48 Bartlett (Baltimore, MD, USA, 5" 
     reflector, x180, S=6, T=5) observed in aristarchus an itenseley bright 
     blue-violet glare on EWBS, E, and NE wall. The Cameron 1978 catalog IF=
     620 and weight=4. The ALPO/BAA weight=2.


2025-Dec-09 UT 16:25-18:20 Ill=72% Jansen observed by Grego_P on 2013-8-26

     Jansen 2013 Aug 26 UT 00:30-01:30 P. Grego (Cornwall, UK, 20cm 
     SCT, x200, seeing II, transparency good) observed a dark patch 
     just east of Jansen D. He had not seen this before. There maybe 
     a depression here hinted at in LOLA ndata. ALPO/BAA weight=1.


2025-Dec-09 UT 18:16-18:30 Ill=72% Posidonius_J observed by Holt_D on 2008-10-19

     On 2008 Oct 19 during 05:40-06:30UT D. Holt of Chipping, UK observed an 
     anomalous patch of illumination just to the west of the centre of the 
     Posidonius J crater. It is possible that this is just some high ground 
     on the floor protruding through the shadow filled crater at sunset. 
     Therefore this has been assigned a weight of 1 for now, just in case it 
     is a TLP - until proven otherwise.


2025-Dec-10 UT 16:07-16:44 Ill=62% Aristarchus observed by Garbett_P on 1976-8-15

     Aristarchus 1976 Aug 15 UT 23:00-23:45 Observed by Garbott (2) 
     (Bedfordshire, England, 10" reflector x500, seeing Antoniadi I) 
     and by Moore (Sussex, England, 15" reflector, x360, seeing 
     Antoniadi IV) "Noted blue color on N. wall extending toward 
     Herod. Also saw orange color in S. region. Confirmed by father. 
     (similar to many of Bartlett's rept's.), More noted nothing 
     unusual at 2320h." NASA catalog weight=4. NASA catalog ID #1444. 
     ALPO/BAA weight=2.


2025-Dec-10 UT 16:07-17:05 Ill=62% Cabeus observed by LCROSS on 2009-10-9

     On 2009 Oct 09 UT11:00-11:04 NASA's LCROSS upper centaur stage, 
     followed 4 min later by the observation spacecraft, is due to impact 
     into a the crater Cabeus in the hope of kicking up some dust and 
     possible frozen volatiles. Note that this description is intended for 
     observers on the date of impact and it is doubtful that any new
     science could be achieved by re-observing the same area months
     after the impact. If you are observing on the date of impact, then 
     please observe around 11:00-11:04UT and ignore the predicted times in 
     the headings. However this report is included as techniqcally
     if something is seen it is a TLP, albeit man-made! For those observing 
     on the date in question here are a few observing tips to maximize 
     the science of your observations: (1) If you are imaging, then please 
     try to obtain images before the impact because you can then subtract 
     these from images taken during the impact and hence show up faint 
     changes that you might normally miss. (2) If you have a spare scope and 
     camera,use this to observe through filters such as UBVR or I, or if you
     have narrow band interference filters, try observing in
     say Hydrogen Alpha, Methane, OH, or indeed any volatile that you 
     might expect to see in a comet (the main source of water at the poles).
     (3) Please try checking the area long after the impact, just in
     case other effects might trigger a TLP. (4) Please go to some trouble 
     to ensure accurate timings- these will be essential in order to 
     understand the sequence of events - assuming any are seen. Timings can 
     be obtained using a short wave radio or via a GPS. Note that you should 
     always use UT or UTC. (5) Please send any observations that you make 
     into the upload section of the LCROSS campaign observers web site. If 
     you belong to an astronomical society e.g. BAA or ALPO, then do please 
     send copies of your observations to the Lunar Sections of your society 
     or club. (6) Finally this desription will be updated a day or two after 
     the planned impact.


2025-Dec-10 UT 16:19-17:44 Ill=62% Cabeus observed by Grego_P on 2009-9-9

     On 2009 Sep 09 UT23:31:43 P.Grego (St Dennis, Cornwall, UK, seeing II-
     III) suspected a flash south of Cabeus, just beyond the terminator.
     It was not bright, and lasted a fraction of a second. Thinks it might
     have been illusory as he saw some fainter flashes (cosmic rays?) 
     during that nights observing session. ALPO/BAA weight=1.


2025-Dec-10 UT 18:13-18:30 Ill=61% Hansen observed by Androsan on 1973-10-17

     On 1973 Oct 17 at Ut 11:30 Androsan (Edmonton, Canada, 6" reflector, 
     x230) observed a glow 1-2 sec reappearance of Saturn's rings at a place 
     of ring's appearance on the dark limb. The observers attributed it to 
     Saturn and its rings. Cameron speculates that it might be due to gas or 
     dust at the lunar surface. Eye was attacted to the glow which 
     delineated the limb at a position angle of 210 deg at emersion, at 
     Earthshine at Edmonton. The Cameron 1978 catalog ID= and weight=2. The 
     ALPO/BAA weight=1.


2025-Dec-11 UT 16:19-17:05 Ill=52% Aristarchus observed by Cowan on 1974-9-8

     Aristarchus 1974 Sep 08 UT 04:45-06:30 Observed by Cowan and Johnson 
     (Dublin, TX, 8" reflector, x59, x152, S=7) "Saw a bright luminous, 
     blue, misty cloud on th NE rim. Obscur. for 1st hr. then gave way to 
     pink & features became vis. Cloud was tear-drop shape. No movement to 
     glow. Pink cloud glowed too. Very tenuous by 0130h. (Nakamura says 
     there were no seismic events within several hrs. of this time). Another 
     person saw it without being advised as the where it was." NASA catalog 
     weight=5. NASA catalog ID #1393. ALPO/BAA weight=4.


2025-Dec-11 UT 17:05-18:31 Ill=52% Alphonsus observed by Brook_C on 2009-9-11

     On 2009 Sep 11 UT00:15-00:20 and 01:00-01:05 C.Brook (Plymouth, UK, 5" 
     O.G., x100, seeing tremourlous but definition improving over time) 
     noticed that the central peak(s) in Alphonsus were brightening 
     gradually. No effect was seen earlier at UT23:30-23:35. One presumes
     that the effect also occured between these two observing times?
     The observer suspects that this was not a TLP, but is uncertain.
     ALPO/BAA weight=1.


2025-Dec-11 UT 16:19-17:52 Ill=51% Earthsine: Monocerotids & Sigma Hydrids: Combined ZHR=10 vel=41 & 58km/s

2025-Dec-12 UT 16:33-17:28 Ill=42% Tycho observed by Carvalho_F on 2006-1-22

     Tycho 2006 Jan 22 UT 06:34-06:36 Observed by Fabio Carvalho 
     (Assis, Sao Paulo Brazil, 25cm f/6 Newtonian) "Green colouration 
     seen on a rim of Tycho, effect remained visible for only 2 
     minutes. Attempts to image it shortly afterwards failed as it 
     had finished by then" An REA-Brasil observational report. 
     ALPO/BAA weight=3.


2025-Dec-12 UT 16:33-17:54 Ill=42% Tycho observed by Cook_MC on 2009-9-11

     On 2009 Sep 11/12 UT23:28-00:00 M.C. Cook (Mundesley, UK, 90mm Questar,
     x80 and x190, seeing II and transparency moderate-poor) observed
     pink on the north west rim of Tycho and green-blue on the inner
     SW rim. No sign of colour elsewhere on the Moon except for the
     S-E rim of Plato that was red. The Moon was about 20 deg in altitude
     at the time. The effect had gone by the end of the observing period. 
     A simulation of spurious colour in different directions 
     was generated by the BAA Lunar Section and found to possibly account 
     for these colours, although there should have been some strong colours 
     seen elsewhere in Tycho and none were. The BAA/ALPO weight=2.


2025-Dec-12 UT 16:19-17:52 Ill=41% Earthshine: Geminids: ZHR>100 vel=34km/s & Coma Berencides: ZHR=3 vel=64km/s

2025-Dec-13 UT 16:14-17:52 Ill=32% Earthshine: Geminids: ZHR>100 vel=34km/s & Coma Berencides: ZHR=3 vel=64km/s

2025-Dec-14 UT 16:15-17:52 Ill=23% Earthshine: Geminids: ZHR>100 vel=34km/s & Coma Berencides: ZHR=3 vel=64km/s

2025-Dec-14 UT 18:30-18:31 Ill=23% Mare_Nubium observed by Hirst on 1878-10-21

     Mare Numbium 1878 Oct 21 UT 01:02-03:00? Observed by Hirst (England) 
     "Half of the Moon's term. obliterated for 3h. (that part over dark mare 
     & blended in?)" NASA catalog weight=0 (very unreliable). NASA catalog 
     weight=205.


2025-Dec-15 UT 16:20-17:53 Ill=16% Earthshine: Geminids: ZHR>100 vel=34km/s & Coma Berencides: ZHR=3 vel=64km/s

2025-Dec-16 UT 16:31-17:53 Ill=10% Earthshine: Geminids: ZHR>100 vel=34km/s & Coma Berencides: ZHR=3 vel=64km/s

2025-Dec-23 UT 09:45-10:12 Ill=10% Taruntius observed by Osawa on 1968-12-23

     On 1968 Dec 23 at UT 08:40-08:45 Osawa (Kyoto-Ken, Japan, 8" 
     reflector, x167 and x212, S=3-4, saw Taruntius crater (and a 
     wrinkle ridge) to be bright through a red filter. Cameron 
     mentions that this was during the Apollo 8 watch. The Cameron 
     1978 catalog ID=1108 and weight=3? The ALPO/BAA weight=2.


2025-Dec-23 UT 09:45-10:12 Ill=10% Aristarchus observed by Mackey on 1971-10-22

     Aristarchus 1971 Oct 22 UT 19:43-19:56 A.Mackay (Hatton, UK, 15cm 
     reflector, x50) observed a pale pink on the W(IAU?) half of 
     Aristarchus and a pale shade of blue on the E(IAU?) half. The 
     effect faded from 19:56UT onwards and had gone 2 minutes later. 
     No information on whether other craters exhibited this effect, 
     given. Burgess, who observed later did not see any colour. 
     ALPO/BAA weight=1.


2025-Dec-23 UT 09:45-10:12 Ill=10% Littrow observed by Madej_P on 1980-4-18

     On 1980 Apr 18 at UT 19:00-22:30 P. Madej (Huddersfield, UK) saw two 
     very bright flashes on the eastern edge of Littrow, spaced 40 seconds 
     apart. Ricketts observed blue flashes approximately 20-30 sec apart and 
     Foley saw faint blue. Cameron 2006 catalog ID=86 and weight=5. ALPO/BAA 
     weight=3.


2025-Dec-23 UT 09:47-10:12 Ill=10% Aristarchus observed by Foley_PW on 1980-4-18

     On 1980 Apr 16 at UT 20:00-22:20 P.W. Foley (Kent,UK, 12" reflector, 
     seeing II-III) found that Aristarchus could barely be seen. Therefore 
     it was not possible to take CED brightness measurements. Strangely 
     Cassini, Kepler, Plato and Mons Pico could be seen. However at 
     20:16 UT St Elmo fire-like flashes were seen coming from the interior 
     south east corner of Aristarchus at 20:16 UT and then the brightnesss 
     spread to fill the rest of he crater. Duration was about 5-20 sec 
     (Cameron comments: atmospheric effects?). The crater reached peak 
     brightness at 20:17UT (CED reading of 8). Foley comments that the 
     crater rim and area 16-24km around this (including Herodoyus) had a 
     translucent radiance. However at 20:25UT the brightness reduced 
     (including Herodotus) down to CED 3, however the blue radiance 
     remained. At 21:07UT Foley saw a star-like flash in the south east of 
     the floor (CED 3-4). Grimaldi was found to be of constant brightness by 
     comparison using the CED Brightness=2). At 20:20UT Amery (Reading, UK) 
     found Aristarchus to be a well visible circular fluorescent patch. At 
     20:40 Amery found the region between Aristarchus and Herodoutus was 
     glowing - appeared almost as a flare from Aristarchus and by 20:55UT 
     there was also a flare to the west of Aristarchus. At 20:27 Madej 
     (Huddersfield) detected only a slight glow from Aristarchus and the 
     region affected was small - indeed the glow had gone by 20:46. At 20:40 
     Ricketts detected a "continuous blue emission" - this had a cycle of 5-
     10 sec (Cameron comments: atmosphere?). Saxton (Leeds, UK) detected at 
     20:42 "translucent effects and variations" at 20:42 noticed a star-like 
     point. At 19:00-21:40 M. Price (Camberley, UK) decided that Aristarchus 
     was fainter in brightness than normal. Peters observed a faint nebulous 
     spot at at 20:25-21:00 that changed in brightness in an irregular way. 
     Cameron 2006 catalog ID=86 and weight=5. ALPO/BAA weight=3. 


2025-Dec-23 UT 10:04-10:12 Ill=10% Promontorium_Agarum observed by Middleton_RW on 1967-1-14

     Cape Agarum 1967 Jan 14 UT 17:17-17:35 Observed by Middleton, 
     Colchester, England, 4" refractor, x240, S=G) "Cape was hazy or 
     obscured whereas Piccard, Pierce, & Cape Olivium were quite clear. Has 
     seen this area obscured many times" NASA catalog weight=3 (average). 
     NASA catalog ID #1008.


2025-Dec-23 UT 10:06-10:12 Ill=10% Gassendi observed by Kilburn on 1969-1-22

     On 1969 Jan 22 at UT 00:10-00:30 Kilburn (England, UK, 6" reflector 
     x192, English Moon Blink device) observed a colour blink on the outer 
     east wall of Gassendi. Cameron says: "in dark!". The Cameron 1978 
     catalog ID=1117 and weight=3. The ALPO/BAA weight=2.  


2025-Dec-24 UT 09:46-10:04 Ill=17% Aristarchus observed by Taylor_TG on 1837-3-11

     1837Mar11 UT 15:27 (20:48 local time) T.G. Taylor (Madras,
     India) whilst observing a star being occulted, noticed a 
     6th magnitude nebulous spot where Aristarchus should be. Had 
     never seen anything quite as bright as this on previous 
     occasions (except the day before). ALPO/BAA weight=2. 


2025-Dec-24 UT 09:48-12:06 Ill=17% Moon observed by Marokwic on 1881-9-27 *

     On 1881 Sep 27 at UT 19:00 Marokwic (South Africa) observed a comet-
     like object pulling across the Mon. The Cameron 1978 catalog ID=225 and 
     the weight=2. The ALPO/BAA weight=1.


2025-Dec-24 UT 09:51-10:41 Ill=17% Atlas observed by Osawa on 1968-12-24

     Atlas 1968 Dec 24 at UT 09:15-10:45 Osawa (Kyoto-Ken, Japan, 8" 
     reflector, 9mm Ortho, Seeing=5, later worse) saw a slight 
     brownish hue on the northern shadowy bed in the crater. It was 
     difficult to see the difference between the glow and chromatic 
     aberation of the eyepiece. The tint never showed up in filters. 
     The ALPO/BAA weight=1.


2025-Dec-24 UT 10:12-10:41 Ill=17% Aristarchus observed by Madej_P on 1980-4-19

     On 1980 Apr 19 at UT 20:37-20:49) P. Madej (Huddersfield, UK, 
     77mm refractor, x83 and x111) at 20:37 UT saw a slight glow at 
     x83, quite small in size. At 20:46UT no glow was seen at x83. 
     At 20:49 a slight glow seen again, but unclear and 
     illdefined - appeared larger in area at x111. Observatons 
     ceased at 21:56 dues to clid. ALPO/BAA weight=1. 


2025-Dec-24 UT 10:15-10:41 Ill=17% Taruntius observed by Buczynski_DG on 1980-4-19

     On 1980 Apr 19 at UT20:30-22:59. The following is quoted from the 
     Cameron 2006 catalog.... "(Buczynski) alerted by colleague (Greenwood) 
     who used filters W15 (IR), W25 (red), W44A (blue), & W58 (UV) and had 
     located a possible blink in it. (Bucz) used W15, W44A & W25. C.P was 
     very bright in W25 (red), dull but vis. In W44A (blue) & floor was 
     noticibly darker in W44A than in W25. Bright cp vis. In W15 & floor was 
     of a light shade. Other craters checked for color, none found. In 44A 
     floor lost some definition (gas?). Sketches from Bucz. & Greenwood. 
     (Pedler) at 2140, floor area around cp was seen in white & red as 
     normal but blink was vis in white, darker in blue. Checks of other 
     features were negative. (Amery) small dark center & small dark area - 
     not shadow - under S wall. N wall obscured by dark area extending N 
     onto surrounding mare. (normal?) which was difficult to focus (gas?). 
     At 2155 N wall now sharper & dark area less intense. Craterlet Cameron 
     in N wall clearly seen which was invisible 1/2 h earlier. (Saxton) 
     whole crater flashed and blinked at 2155. Could see detail in brighter 
     W 1/2 of crater - not seen earlier. At 2205 seeing poor, at 2215 it was 
     normal. (Blair) at 2155 used red & blue filters & in blue it was darker
     than in red. W. wall not well defined. (J. Cook) saw spurious color on 
     N & S rims. Saw a pink tinge on SE rim. (A. Cook) saw spur. Color on 
     most craters as seeing deteriorated. Got a blink on SE region > red 
     than blue". The Cameron 2006 catalog ID=87 and the weight=5. The 
     ALPO/BAA weight=3.


2025-Dec-24 UT 10:26-10:43 Ill=17% Earthshine: sporadic meteors

2025-Dec-25 UT 09:46-10:17 Ill=25% Moon observed by Hirst on 1879-10-20

     In 1879 Oct 20 UT 23:00 (Local time Oct 21 9AM) Hirst (Blue Mountains, 
     NSW, Australia) saw a large part of the Moon covered with a dark shadow 
     that was as dark as the Earth's shadow would have been if there had 
     been an eclipse. Cameron says that this is a confirmed observation. 
     Note that the Moon was just before first quarter. The Cameron 1978 
     catalog ID=215 and the weight=4. The ALPO/BAA weight=3.


2025-Dec-25 UT 09:46-11:04 Ill=25% Aristarchus observed by Lagunas on 1969-11-15

     On 1969 Nov 15 at UT 02:20-03:20 Lagunas (Santiago, Chile, 10" 
     reflector) observed some brightenings in Aristarchus during the Apollo 
     12 watch. The Cameron 1978 catalog ID=1209 and weight=0. The ALPO/BAA 
     weight=1.


2025-Dec-25 UT 09:46-11:01 Ill=25% Aristarchus observed by Foley_PW on 1980-4-20

     On 1980 Apr 20 at UT 19:25-23:43 P.W. Foley (Kent, UK, 10" reflector, 
     seeing II-III) found that Aristarchus was very bright in Earthshine 
     (also found on the photographs that he took), giving off a blue 
     "incadescence", the CED brightness reading was 5. Occasionally Foley 
     could see a star-like point in the south east corner. For comparison in 
     brightness he used highland terrain near to Grimaldi (CED=2). By 
     comparison, Buczynski and Lord, could not see Aristarchus. Earlier, 
     Geenwood saw the crater easily as a star-like point with a diffuse 
     exterior glow. Cameron says thyat this was confirmed by Buczynski and 
     Lord (?). At 20:35UT Amery decided that Aristarchus looked brighter 
     than normal. Pedler though described the crater as "small dim nebulous 
     blue or blue-green" that was invisible by 20:27UT. At 20:28-22:01 Blair 
     could not detect Aristarchus, nor could J-H Robinson at 20:40UT though 
     he did see it at 20:55UT as both diffuse and blue. Ricketts detected a 
     blow glow with irregularly spaced flashes of roughly 5-10 sec apart. 
     Cook's at Frimley, UK, saw no features in Earthshine. Cameron 2006 
     catalog ID=88 and weight=4. ALPO/BAA weight=2.


2025-Dec-25 UT 09:46-11:06 Ill=25% Copernicus observed by Cook_JD on 1980-4-20

     On 1980 Apr 20 at UT20:05-21:02 J.D. Cook (Frimley, UK, 12" reflector, 
     x60, seeing III-IV) at the start of this session found some bright 
     spots in the area of Copernicus, and at 21:02 detected some flashes in 
     this region. Cameron 2006 catalog ID=88 and weight=1. ALPO/BAA 
     weight=1.


2025-Dec-25 UT 09:46-11:06 Ill=25% Piccolomini observed by Cook_MC on 1980-4-20

     On 1980 Apr 20 at UT 19:45-22:45 M.C.Cook (Frimley, UK) - colour 
     (probably spurious) seen on Piccolomini. Cameron 2006 catalog ID=88 and 
     weight=4. ALPO/BAA weight=1.


2025-Dec-25 UT 10:06-11:06 Ill=26% Grimaldi observed by Price_M on 1980-4-20

     On 1980 Apr 20 at UT20:27 M.Price (Camberley, UK) saw a flash in the 
     Grimaldi-Aristarchus area. Cameron 2006 catalog TLP ID=88 and weight=4. 
     ALPO/BAA weight=2.


2025-Dec-25 UT 10:51-11:06 Ill=26% Fracastorius observed by Robinson_JH on 1980-4-20

     On 1980 Apr 20 at UT21:12-22:45 J-H Robinson (Teignmouth, UK, 10.5" 
     reflector, x180) found, using a Moon Blink device, evidence of colour 
     on the flor patches of Fracastorius crater, brighter in blue than in 
     red. Also the floor to center varied in brightness in blue and in red. 
     Peters observed in white light and found the south east-south wall had 
     a slight orange cast and when a Moon blink was used it was less bright 
     in blue than in red light. M. Cook found spurious colour on the south 
     rim and also on Mons Pico. There was a colour blink reaction on the 
     southeast floor of Fracastorius - this was both faint and blurred and 
     not seen in white light. A.C Cook detected the permanent blink in the 
     south east floor of the crater at 21:47 and a fainter one in the north 
     west (marginally brighter in red than in blue). J.D. Cook found no 
     colour with the Moon blink device. 21:22-22:10 P.W. Foley got a strong 
     colour reaction with the Moon Blink device - brighter in red than in 
     blue and detected a pink colour visually on the south east wall 22:10-
     22:45 (this did not give a blink effect though). Cameron 2006 catalog 
     ID=88 and weight=4. ALPO/BAA weight=2.


2025-Dec-25 UT 10:27-11:08 Ill=26% Earthshine: sporadic meteors

2025-Dec-26 UT 09:46-11:26 Ill=35% Censorinus observed by Holmes_D on 1988-11-15

     On 1988 Nov 15 UT 19:15 Holmes (Rockdale, UK, 215mm Newtonian) noticed 
     the Censorinus apron (just east of the crater and including the rim) 
     was fuzzy but the crater was clear - a sketch was provided. A BAA Lunar 
     Section observation.Cameron 2006 Catalog Extension ID=339 and weight=3.
     ALPO/BAA weight=3.


2025-Dec-26 UT 09:46-10:25 Ill=35% Apianus_D observed by Power_F on 2011-10-3

     Apianus D On 2011 Oct 03 UT 21:00-21:20 F. Power (Meath, 
     Ireland, 11" SCT) observed changing colours (blue, white, and 
     red) on the inner western rim of this crater. He changed 
     eyepieces and moved the scope around to look at dufferent parts 
     of the Moon, but nowhere else exhibited anything similar. As 
     another test he asked his wife to have a look without telling 
     her what he was seeing. She confirmed the same effect. 5 digital 
     camera images had been taken. Most of these were out of focus 
     and the first one was saturated, however one of them showed a 
     approximately 35 km long, by 11 km wide (at the north) lopsided 
     carrot shaped orange colour to the western rim of Apianus D. No 
     similar strong colour could be seen anywhere else on the image, 
     nor on the other 4 images. This TLP is being given an ALPO/BAA 
     weight of 1 as the Moon was low, but an image taken looks 
     interesting.


2025-Dec-26 UT 10:19-11:26 Ill=35% Torricelli_B observed by Braga_R on 2001-4-29

     On 2001 Apr 29 at UT 20:50 R. Braga (Italy) reported that without any 
     filter, the brightness of the east wall of Torricelli B was halfway 
     Torricelli C (faintest) and Moltke (brightest). By insering a Wratten 
     25 red filter though, the crater was slightly more evident. However 
     using a blue Wratten 39A filter, the crater vanished completely, whilst 
     Toricelli C remained. The ALPO/BAA weight=3. 


2025-Dec-26 UT 10:27-11:28 Ill=36% Earthshine: sporadic meteors

2025-Dec-27 UT 09:47-10:41 Ill=46% Ross_D observed by Harris on 1964-3-21

     Near Ross D (24E, 11N) 1964 Mar 21 UT 05:00-06:20 Observed by 
     Harris, Crow, Cross (Whittier, CA, USA) - negative confirmation 
     from Las Cruces. NASA catalog weight=0 (unreliable). NASA catalog 
     ID #805. ALPO/BAA weight=1.


2025-Dec-27 UT 09:47-10:14 Ill=46% Mons_Piton observed by Horne_P on 1983-3-21

     On 1983 Mar 21 at UT 21:05-22:00 P. Horne and J. Horne (Hertz, England, 
     UK, 11" reflector, x180 and x330) found that Mons Piton (totally 
     illuminated and brightest feature on the Moon - but no variability) was 
     brighter than Aristarchus (would have been if it had been in sunlight)
     and the mountain was contained within a circular illuminated patch. 
     "Brilliant white and no shadow. Size ~16km." There was no details 
     visible but the adjacent features had distinct shadows. Hutton was also 
     observing. Foley examined the photographs and believes that they are 
     inconclusive. D. Mansbridge was photographing the Moon at 19:30UT and 
     detects Piton but it is not bright. However in a photograph taken by D. 
     Mansbrdige and 20:30UT the mountain is much brighter than any other 
     sunward facing slopses on the northern part of the Moon's terminator. 
     R. Mosley had been observing earlier at 18:10-19:40 and although 
     finding the mountain to be shining briliantly beyond the terminator, he 
     also comments that this is normal. Cameron though has seen the 
     photographs taken and thinks it might be a real TLP. The Cameron 2006 
     catalog ID=208 and weight=5. The ALPO/BAA weight=2.


2025-Dec-27 UT 09:47-12:19 Ill=46% Torricelli_B observed by Mobberley_M on 1984-4-8 *

     On 1984 Apr 08 UT 19:50 Mobberley (14" reflector, x194, seeing 
     III-IV, Transparency Fair-Poor, Cockfield, UK) found that 
     Torricelli B's shadow was 1/2 the way across the floor, which 
     was normal, but that there was a very dar grey/brown shroud 
     around the carter, out to several radii. 
     The ALPO/BAA weight=1.


2025-Dec-27 UT 09:47-10:35 Ill=46% Censorinus observed by Cook_MC on 1988-11-16

     On 1988 Nov 16 at UT 18:20 M.C. Cook (Frimley, UK) observed that a ray 
     north east of censorinus appeared to be very diffuse and this did not 
     change during the observation. This was odd because proclus ray 
     material remained clear. The apron material of Censorinus was diffuse 
     E-W and the northern part was dull, but not fuzzy. The Cameron 2006 
     catalog ID=340 and the weight=3. The ALPO/BAA weight=2.


2025-Dec-27 UT 09:47-10:35 Ill=46% Torricelli_B observed by Cook_MC on 1988-11-16

     On 1988 Nov 16 at UT 18:20 M.C. Cook (Frimley, UK) observed that 
     Torricelli B changed in brightness (at times), but thinks that this was 
     due to atmospheric transparency. The Cameron 2006 catalog ID=340 and 
     the weight=3. The ALPO/BAA weight=1.


2025-Dec-27 UT 10:19-11:43 Ill=46% SE_Limb observed by Rohslberger_R on 1980-4-22

     On 1980 Apr 22 at UT20:30 R.Rohslberger (Hittfield, (near Hamburg) West 
     Germany, 8" reflector, x170 25mm occular used, 300mm focal length?) 
     took some photographs using projection. One of these recorded an 
     apparent "ejecta curtain". Cameron considered lens flare, but the other 
     photographs did not show this. If real then the plume was at a height 
     of ~40km and the ray was ~130km. Cameron concludes that this was an 
     impact photograph. The Cameron 2006 catalog ID=90 and the weight=5. The 
     ALPO/BAA weight=3.


2025-Dec-27 UT 10:35-11:43 Ill=46% Alphonsus observed by Lenham_AP on 1952-11-24

     Alphonsus 1952 Nov 24 UT 18:00 A.P. Lenham (Swindon, UK, 3-
     inch efractor x120) noted that the usual dark spots were not 
     visible, but floor ridges and craterlets were surperbly seen. 
     This may not be a TLP but has been given a TLP category as it 
     is a curious appearance and needs to be verified on a repeat 
     repeat illumination apeparance. ALPO/BAA weight=1.


2025-Dec-27 UT 11:20-11:43 Ill=46% W_Limb observed by Miles_H on 1987-1-7

     On 1987 Jan 07 at UT19:10-20:30 H.Miles of Cornwall, UK saw two bright 
     patches were seen in Earthshine at clock positions of 4 (this patch was 
     defined by the dark limb and the brightness faded inwards to the disk, 
     over a short distance. "Centred at 60 deg along the limb from the north 
     - a sketch showed approximately 10-15 deg along it") and 5:30 (this 
     second patch was smaller and not so bright as the first patch - it was 
     west of the north pole. P. Foley (Kent, UK) also detcted the patches 
     and said that one was not far from the sunrise terminator. 
     The Cameron 2006 Extension catalog gives this TLP an ID of 291 and a 
     weight of 2. The ALPO/BAA weight=2.


2025-Dec-27 UT 10:27-11:45 Ill=46% Earthshine: sporadic meteors

2025-Dec-28 UT 09:47-09:59 Ill=57% Plato observed by Schroter on 1789-7-30

     Plato 1789 Jul 30 UTC 21:00? Observed by Schroter (Lilienthal, Germany) 
     NASA Catalog Event #61, NASA Weight=2 (slightly low) Event described 
     as: "Soon after sunrise saw a kind of fermentation on the floor which 
     clearly resembled a kind of twilight, (due to some kind of aberration 
     unknown to the observer?)" For further details see reference: 
     Middlehurst, B.M., Burley, J.M., Moore, P.A. and Welther, B.L., 1968, 
     NASA TR R-277.


2025-Dec-28 UT 09:47-11:02 Ill=57% Eratosthenes observed by Lenham_AP on 1952-11-25

     Eratosthenes 1952 Nov 25 UT 16:30 A.P. Lenham (Swindon, UK, 3-
     inch refractor x150, Definition Good) noted that there was 
     faint/slightly bright detail inside the interior shadow - 
     observer comments "presumably peaks of central mountains & W. 
     Wall ridge, but very faint" - however this is worth checking 
     out. ALPO/BAA weight=1.


2025-Dec-28 UT 09:53-11:38 Ill=57% Eratosthenes observed by Abel_P on 2009-11-25

     On 2009 Nov 25 UT18:42-21:03 P.Abel, T.Little and C.North (Selsey, UK, 
     15" reflector, seeing II-III, transparency very good), all saw visually 
     a brownish tinge on the north west rim of Eratosthenes crater. P.Abel 
     made a sketch and T.Little took some high resolution CCD images, some 
     of which were through coloured filters. Checks were made for spurious 
     colour, but none was seen elsewhere on the Moon. The eyepiece was 
     changed but this made no difference. M.C.Cook (Mundesley) was observing 
     with a smaller scope at the same time, but saw no colour, however 
     observing conditions were worse. W.Leatherbarrow (Sheffield, UK) was 
     observing with a instrumenet mid way in size, and saw a brownish tinge 
     in the NW rim area, but saw a similar colour elsewhere and put this 
     down to spurious colour. Normally multiple observers seeing the same 
     thing would result in a weight of 4, however as this was only observers 
     at Selsey and some of the evidence contradicts, I am allocating an 
     ALPO/BAA weight=3.


2025-Dec-28 UT 10:18-11:56 Ill=57% Pallas observed by Stuart_L on 1953-11-15

     Pallas-Schroter 1953 Nov 13 UTC 02:00 Observed by L.Stuart (USA) 
     "Saw and photographed a bright spot on term. between these two 
     craters. Used Kodak 103aF3." NASA catalog weight=5 and catalog 
     ID #559. ALPO/BAA weight=5.


2025-Dec-28 UT 10:25-11:56 Ill=57% Eratosthenes observed by Galdies_C on 2012-8-25

     On 2012 Aug 25 UT1944-1952 Eratosthenes crater was imaged by C. 
     Galdies (Malta,Nexstar 8SE, Philips SPC 900NC camera). 4 
     Registaxed images were produced covering 19:45, 19:48, 19:49, 
     and 19:51. All but the first image, once first order spurious 
     colour had been removed, showed orange on the shaded terraces on 
     the western illuminated rim (similar to what Paul Abel and 
     others saw in 2009, albeit just confined to the NW rim), and the 
     interior floor shadow was slightly smaller in red light. However 
     orange colour was also seen on the eastern side of mountains to 
     the south of the crater, which infers that the spurios colour 
     removal did not fully acomplish its main goal. The effects were 
     not caused by the registax software as the orange colour is 
     visible on individual images. Although probably the colour is 
     not lunar in orgin, its explanation is not fully explaianed, 
     therfore an ALPO/BAA weight of 1 is used for now.


2025-Dec-28 UT 11:12-11:56 Ill=57% Aristarchus observed by Loocks on 1969-11-18

     On 1969 Nov 18 at UT 04:22 Loocks (Valparaiso, Chile, 12" reflector) 
     observed a flash of light of magnitude 12. Cameron speculates a meteor 
     and mentions the apollo 12 watch. The Cameron 1978 catalog ID=1214 and 
     weight=1. The ALPO/BAA weight=1.


2025-Dec-28 UT 11:27-11:56 Ill=57% N_Pole observed by Harris on 1912-1-28

     North (?) (left) Cusp 1912 Jan 28 UT 00:00 (27th 20:00 L.T.) Observed 
     by Harris (Philadelphia? Pennsylvania?, naked eye?): Intensely black 
     curved object 400x240km, shaped like a "crow". Cameron 1978 weight=1 
     (very low) and ID=334. ALPO/BAA weight=1.


2025-Dec-28 UT 11:47-11:56 Ill=58% Eratosthenes observed by Longshaw_N on 2017-5-4

     Eratosthenes: On 2017 May 04 UT 21:50-22:10 N. Longshaw (BAA, 
     UK, 78mm APO refractor, x125 & x175, seeing II-III, 
     transparency Good). A brownish (orange) tint was seen on the 
     inner NW wall light terraces - this was immediately obvious 
     when first looking at the crater, but as time progressed the 
     effect became less bright. Other craters were checked for 
     similar coloured tints, but none were seen elsewhere on the 
     Moon. UAI observers in Italy (F. Taggogna & A. Tonon) had been 
     imaging the region in colour 17:57-21:47, but their images do 
     not show any colour on the inner NW rim terraces, the their 
     last image is 3 min before Longshaw saw the colour. The 
     ALPO/BAA weight=2.


2025-Dec-29 UT 09:47-11:28 Ill=68% Eratosthenes observed by Haas_W on 1936-10-25

     On 1936 Oct 25 at 01:35 UT W. Haas (Alliance, OH, USA, 12" 
     reflector) saw small bright spots on the floor of Eratosthenes, 
     (Pickering's atlas 9A, col. 30deg, shows no spots - according to 
     Cameron). Cameron 1978 catalog TLP=417 and weight=4. ALPO/BAA 
     weight=1.


2025-Dec-29 UT 09:47-10:27 Ill=68% Aristillus observed by Haas_W on 1939-7-26

     Aristillus 1939 Jul 26 UT 02:30 Observed by Haas? (NM?, USA, 12?" 
     reflector) "Dark area to W. part of floor was I=3.7. (see #450, 459 & 
     461). Used diff. telescopes but can not explain difference)" NASA 
     catalog weight=4 (good). NASA catalog ID #454.


2025-Dec-29 UT 09:47-11:41 Ill=68% Copernicus observed by Lovell on 1966-3-1

     Copernicus 1966 Mar 01-02 UT 22:06-09:45 Observed by Lovell (Auburn, 
     OH, 4" refractor, x120m S=E, T=3.5) "As sun rose higher, west (ast.?) 
     outer wall was bathed in a soft viol. color -- not in evidence on flat 
     ground below the wall" NASA catalog weight=3, NASA catalog ID #922.


2025-Dec-29 UT 10:21-12:08 Ill=68% Alphonsus observed by Argus on 1969-11-19

     Alphonsus 1969 Nov 19 UT 03:30 Observed by Argus/Astronet (CA?, USA) 
     Brightening in W. rim & S. central floor, seen by 2 obs. (Apollo 12 
     watch)" NASA catalog weight 3 (average). NASA catalog ID #1219.


2025-Dec-29 UT 11:03-12:08 Ill=68% Plato observed by Brook_C on 2005-12-10

     Plato 2005 Dec 10 UT 20:46 Observed by Brook (Plymouth, UK, 4" 
     refractor. Conditions excellent with the Moon at a high altitude) "2 
     second duration white flash seen on the floor of the crater" - BAA 
     Lunar Section Report.


2025-Dec-30 UT 09:47-09:59 Ill=78% Daniell observed by Price_M on 1979-6-5

     Daniell 1979 Jun 05 UT 20:15-21:10 Observed by Price (Camberley, 
     England, 152mm reflector x64 and x128, seeing III, transparency good) 
     "Obscuration seen" BAA Lunar Section report.


2025-Dec-30 UT 09:47-09:59 Ill=78% Posidonius observed by Price_M on 1979-6-5

     Daniell 1979 Jun 05 UT 20:15-23:00 Observed by Price (Camberley, 
     England, 152mm reflector x64 and x128, seeing III, transparency good) 
     observed that Posidonius lacked sharpness.


2025-Dec-30 UT 09:47-10:23 Ill=78% Plato observed by Smith_T on 2024-11-11

     Plato. 2024 Nov 11 UT 20:33-20:52. T.Smith (Codnor, UK - 16 
     inch Newtonian, seeing IV) the inner northern rim was an 
     orange-white colour and this faded, and had vanished by 20:52. 
     Observation ceased at 20:56. the effect was not present 
     earlier at 17:49-18:04, nor during a visual check at 
     23:14-23:24. No other features on the Moon exhibited this 
     effect at the time. Colour imagery by C.Longthorn at 20:14 and 
     A.Cook at 20:54 failed to detect any colour in this region, 
     but these lay outside Smith's observing window. ALPO/BAA 
     weight=1.


2025-Dec-30 UT 09:54-11:45 Ill=78% Bullialdus observed by Cook_MC on 1979-6-5

     Bullialdus 1979 Jun 05 UT 22:00-23:00 Observed by Cook M.C. 
     and J.D. (Frimley, UK, 12-inch reflector, Seeing III-IV, good 
     transparency). MC Cook observed internittently over this time 
     period (due to cloud) and found the crater sharper in a blue 
     filter than in a red filter. No obscuration seen apart from a 
     darkish patch on the SW rim and spreading over onto an area 
     surrounding the rim, which she took to be shadow, though the 
     main shadow was along the east rim of the crater. JD. Cook 
     observed an orange colouration seen on eastern and the cleft 
     on the SW rim. Dark area seen on southern floor of crater, 
     south of central peak. ALPO/BAA weight=1.


2025-Dec-30 UT 11:31-12:15 Ill=79% Eimmart observed by Louderback_D on 1981-4-15

     On 1981 Apr 15 at UT06:27-06:40 D. Louderback (South Bend, WA, USA 
     using a 3" refractor x134 and S=4.5-5 and T=5-0) saw a bright spot on 
     the western wall of Eimmart (sketch supplied) have an unusual 
     brightening and shade. Variations occurred over 2-3 minute intervals. 
     Louderback commented that the spot looked like a flare with its apex 
     located at the crater wall and there was some blurring effect on the 
     spot - it decreased in size during the phenomenon. Seeing worsened 
     later. Apparently on the 18th and 19th of April everything was back to 
     normal. Cameron comments that there is no bright spot on the Moon at 
     this location. Lunar Orbiter IV plates 192-3.2 shows evening 
     conditions. Cameron 2006 Catalog Extension TLP ID=130 and weight=3. 
     ALPO/BAA weright=3.


2025-Dec-31 UT 10:04-10:58 Ill=87% Mersenius_C observed by Ward_G on 2005-11-13

     G. Ward (a lunar observer for 15 years) observed an area just south 
     west of Mersenius C to be blurred and in a greenish cloud. The green 
     colour was more like that of dead grass than one gets from a neon bulb.
     The effect was seen from 04:50-04:57UT, but could have been going on 
     before it was first noted at 04:50-UT. Seeing was 6-7/10 4" Refractor 
     (2 element). refractor had been used hundreds of hours before (over a 
     10 year period) with no similar colour was seen. The observer checked 
     other areas but did not see any similar effects. They also rotated and 
     changed eyepieces, but this made no difference to the TLP. The TLP site 
     seen was picked up on an image taken earlier at 04:47UT by W. Bailley,
     from Sewell, NJ, USA. Unfortunately the area concerned, a mountain on 
     the image, was saturated and so we cannot tell if a colour was present 
     there and the seeing was poor.


2025-Dec-31 UT 10:04-10:38 Ill=87% Torricelli_B observed by Serio_R on 2005-1-22

     Torricelli B 2005 Jan 22 UT 01:00 Observed by Serio (Houston, TX, USA, 
     6" Cassegrain, x150 and x180, Seeing 3, high deck of Cirrus clouds) 
     "Torricelli B hard to make out in the videos taken, but images taken 
     through cloud. A check on the image received by the coordinator shows 
     that Torricelli B is in fact visible, but perhaps not very bright. A 
     later observational sequence of images by Raul Salvo (Montevideo, 
     Uraguay UT 03:15-03:23) showed similarly that Torricelli B was dark, 
     and there was some brightness variability although the 
     background setting on these was low" An ALPO report.


2025-Dec-31 UT 10:04-11:32 Ill=87% Bullialdus observed by Gray_R on 2006-12-2

     At 03:30UT observer noticed a hint of yellow colour
     on the floor of the crater and by 03:57UT the south
     east and central parts of the floor and the circular
     feature on the south west floor had turned a deep
     yellow colour. The rest of the crater remained colourless.
     Other craters also remained colourless. By 04:05UT the colour
     was fading and by 04:15UT it was gone. Maurice Collins
     in New Zealand took some low resolution colour images about
     4 hours later but these failed to show any yellow colour.
     Zac Pujic obtained colour images at a different time of
     natural surface colour on the Moon and finds that Bullialdus
     does actually have a natural yellow cast to most of the floor.
     However this does not explain the variability in colour strength
     seen by Robin Gray. ALPO/BAA weight=3.


2025-Dec-31 UT 10:26-12:12 Ill=87% Timocharis observed by Firsoff on 1954-10-8

     Observed by Firsoff (Somerset, England, 6.5" reflector? x240) "Red 
     glow." NASA catalog weight=4 (high). NASA catalog ID #573.


2025-Dec-31 UT 10:27-12:12 Ill=87% Aristarchus observed by Grego_P on 1987-1-11

     On 1987 Jan 11 at UT 18:15-23:00 P. Grego (Birmingham, UK, 6" 
     reflector, seeing=III) sketched Aristarchus crater and saw two 
     luminous circular patches on the exterior west wall - these 
     were less bright than the inner wall but brighter than the 
     outer wall. The Cameron 1978 catalog ID=292 and weight=5. 
     ALPO/BAA weight=2.


2025-Dec-31 UT 10:27-12:12 Ill=87% Plato observed by Moore_P on 1987-1-11

     On 1987 Jan 11 at UT P. Moore (Sussex, UK) found the the floor of Plato 
     was much more drk than the adjacent Mare Imbrium. Furthemore there was 
     a blurring of detail over the northeast wall and onto the nearby floor. 
     detail elsewhere in the crater was OK. By 23:00UT there was less lack 
     of detail effects. M. Cook (Frimley, UK) at 21:55UT noted the obscured 
     area but decided that it was narrower than the same effect one month 
     ago and suspected that she may have been observing towards the end of 
     this TLP. The effect gradually dimmed between 21:55 and 22:45UT. Other 
     craters were normal. G. North was affected by poor seeing conditions. 
     Davies detected a slight obscurtion on the north east corner - it was a 
     misty gray feature at x200. The Cameron 2006 catalog extension ID was 
     292 and the weight was 5. Tha ALPO/BAA weight was 4.


2025-Dec-31 UT 10:38-12:12 Ill=87% Gassendi observed by Unknown_Observer on 1889-5-11

     On 1889 May 11 at 22:00? UT an unknown observer saw an ink black spot 
     on the rampart of Gassendi. It had not been seen before ar at the next 
     lunation or indeed ever again. Cameron 1978 catalog ID=261 and 
     weight=3. ALPO/BAA weight=2.


2025-Dec-31 UT 10:39-12:12 Ill=87% Vallis_Schroteri observed by Thornton_FH on 1949-2-10

     Cobra Head 1949 Feb 10 UT 00:00? Observed by Thorton (Northwich, 
     England, 18" reflector) "I was examining the Cobra Head of the Schroter 
     Valley, when I noticed what seemed to be a diffuseed patch of thin 
     smoke or vapour, apparently originating from the valley on the E. Side 
     where the landslip is, and spread over the edge on to the plain for a 
     short distance. Every detail of the edge of the valley was perfectly 
     clear and distinct except where this patch occurred, but there the 
     definition was poor and very blurred" NASA catalog 
     weight=4 and catalog ID #515. ALPO/BAA weight=1.


2025-Dec-31 UT 10:46-12:12 Ill=87% Bullialdus observed by Findlay_MW on 1974-9-27

     Bullialdus 1974 Sep 27 UT  22:45-23:40 Observed by Findlay, Ford 
     (Dundee, Scotland, 10" refractor, 150x, 180x, filters) "Saw yellowish-
     orange color in crater. After clouds passed at 2300h color still there 
     & gave a slight blink which no other craters did. Not seen in red 
     filter, dark in blue. Ford saw it along ridge fr. c.p. to SW wall. 
     Alert did not bring confirm. as clouds intervened for all others." NASA 
     catalog weight=4. NASA catalog ID #1394. ALPO/BAA weight=3.


2025-Dec-31 UT 11:03-12:12 Ill=88% Torricelli_B observed by Salvo_R on 2005-1-22

     Torricelli B 2005 Jan 22 UT 03:15-03:23 Observed by Raul Salvo 
     (Montevideo, Uraguay UT 03:15-03:23) showed that Torricelli B 
     was dark, and there was some brightness variability although the 
     background setting on these images was low and seeing could 
     account for the brightness variation? An ALPO report.


2025-Dec-31 UT 11:26-12:12 Ill=88% Gassendi observed by Darling_D on 1990-10-1

     On 1990 Oct 1st at 00:44-01:24UT D Darling (Sun Praire, WI, USA) 
     observed that Gassendi still had a blink effect when viewed through 
     blue (Wratten 38A) and red (Wratten 25A) filters. No effect was seen on 
     Aristarchus. Gassendi was brighter in the red filter and this was 
     confirmed by Weier. Sketches were made and brightness measurements 
     taken. Both observers used a 12.5" reflector x159. At 01:00UT the NW 
     wall was 7.5, the SW wall 8.0, the S. wall 7.5, the floor 6.0, the 
     outer E. wall 8.0, the N. floor 5.5. Gassendi A W. wall was 9.5,l 
     Aristarchus W. floor was 8.0, NW wall 8.0, shadowed floor 0.0, E. outer 
     wall 7.0, NBP 5.5, area between Aristarchus and Herodotus 6.0, and the 
     comet like tail: 8.2 on the E. and 8.5 on the W. The Cameron 2006 
     catalog extension TLP ID=412 and weight=5. The ALPO/BAA weight=4.