TLP Repeat Illumination/Libration and Earthshine predictions for: USA MH Majuro



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-Feb-01 UT 06:41-07:29 Ill=99% Plato observed by Taylor_A on 1971-1-10 *

     Plato 1971 Jan 10 UTC 20:17-20:42 Observed by Taylor (Slough, England, 
     8.5" reflector) "Blink (dark gray to black), 13x3km diam. on E. wall & 
     floor in indentation in wall. Smaller by 2028 h. gone at 2035h. 
     Reappeared at 2028h & gone completely at 2042h)." NASA catalog weight=3 
     (average). NASA catalog ID #1282.


2026-Feb-01 UT 07:39-08:10 Ill=100% Moretus observed by Webb_TW on 1871-12-25

     Moretus? 1871 Dec 25 UTC 22:00? Observed by Webb? (England?, 9" 
     reflector?) "Internal twilight in crater #132- a large circular crater 
     nr. S.pole (crater #132 on Goodacre's map is Plato. Webb's map?)" NASA 
     catalog weight=3 (average). NASA catalog ID #173.


2026-Feb-01 UT 07:39-08:23 Ill=100% Helicon observed by Caruso_J on 1979-8-7

     The area west of Helicon not visible despite the area being 
     fairly bright at Full Moon time. This area was a very bright 
     patch one night. Cameron notes: comensurability of Full Moon & 
     Perigee. Cameron 2006 catalog extension ID=64 and weight=3. 
     Seeing=7 and transparency=4. 2.4" refractor used. ALPO/BAA 
     weight=1.


2026-Feb-01 UT 08:37-09:51 Ill=100% Plato observed by Haas_W on 1937-7-22

     Plato 1937 Jul 22 UT 06:20 Observed by Haas (Alliance, Ohio, 
     USA, 12" reflector?) "Floor distinctly greenish, but was gray on 
     June 23, 1937 at 0430 & col.84 (normal?)" NASA catalog weight=4 
     (high). NASA catalog ID #421. ALPO/BAA weight=3.


2026-Feb-01 UT 09:31-11:28 Ill=100% Plato observed by Chapman on 1982-6-5

     On 1982 Jun 05 at 22:00? UT, Chapman (UK, using a 12" reflector), again 
     using a x2 yellow filter, noticed that the central craterlet 
     detectabilty changed such that sometimes it was visible and sometimes 
     not. Foley (Kent, UK)noticed that the central craterlet could only just 
     be seen between June 2 to June 5 and was much less discernable than 
     during the previous lunation. No CED brightness measurements made. The 
     floor of Plato was noted to be very dark though. Cameron 2006 catalog 
     ID=172 and weight=4. ALPO/BAA weight=2.


2026-Feb-01 UT 11:04-12:54 Ill=100% Aristarchus observed by Weresuik on 1965-5-15

     Aristarchus 1965 May 15 UTC 01:40-02:15 Observed by Weresuik, McClench, 
     Johnson (Pt. Tobacco, MD, USA, 16" reflector x240, S=F, T=G) and Delano 
     (Massachusetts, USA, 12" reflector). "Crater had color(red?) detected 
     by Trident MB & photos were obtained. There were pulsations. Delano saw 
     E. wall of crater unusually bright (confirm. if at same time)." NASA 
     catalog weight=5 (very good). NASA catalog ID #876.


2026-Feb-01 UT 11:11-12:37 Ill=100% Aristarchus observed by Conway_A on 2024-2-23

     Aristarchus. 2024 Feb 23 UT 19:22. A.Conway (Bootle, UK - 20cm 
     Newtonian (dobsonian), 9mm Plossl eyepiece, Samsung A33 mobile 
     phone camera, 36 sec AVI file at 30fps, seeing probably 
     average-good). Noticed a blue tinge on northern rim of the 
     crater. This is probably normal, but we are flagging this up 
     as a weight 1 TLP, in order to obtain some repeat illumination 
     observations and confirm that the strength of the blueness is 
     normal.


2026-Feb-01 UT 12:30-14:34 Ill=100% Eratosthenes observed by Bartlett on 1976-9-8 *

     Eratosthenes 1976 Sep 08 UTC 04:29 Observed by Bartlett (Baltimore, MD, 
     USA, 4.5" reflector 45-225x, S=5-4, T=5) "Psuedo-shadow X3 was present 
     but X disappeared from wall(same intensity?) which was rated 4 deg. 
     Disappearance of X so unexpected that he examined inner S wall very 
     carefully & was certain it was free from psuedo-shad. Had vanished 
     within 24h. Other pseudo-shadows showed no change. X reappeared next 
     nite. (X must have been 4deg; &this is much higher than any other 
     meas.). Variability of wall shadows may habe been what Pickering saw, 
     suggests Bartlett." Cameron 1978 TLP catalog weight=4 and catalog ID
     1452. ALPO/BAA weight=2.


2026-Feb-01 UT 13:34-14:32 Ill=100% Madler observed by Gray_R on 2005-10-17

     Madler 2005 Oct 17 UT 04:14-05:28 Observed by Robin Gray (Winnemucca, 
     NV, USA, 152mm refractor, x228, x343, S=5-8 and T=5-6) "Very bright 
     pinpoint spot seen towards end of observing period on east crater wall, 
     lasting 1 min in duration. Brighter than other spots, possibly 8.5-9 on 
     the Elger scale. The spot was not seen earlier during the long 
     observing session." An ALPO report. The ALPO/BAA weight=3.


2026-Feb-01 UT 13:58-15:43 Ill=100% Madler observed by Haas_W on 1940-9-16

     Madler 1940 Sep 16 UT 02:10 Observed by Haas (New Mexico? USA, 
     12"  reflector?) "Bright spot on S. rim was I=5.8 comp. with 8.9 
     on Aug 17 (see #470)." NASA catalog weight=4. NASA catalog ID #
     473. ALPO/BAA weight=2.


2026-Feb-02 UT 08:34-09:15 Ill=100% Tycho observed by Fock on 1919-11-7

     On 1919 Nov 27 at UT 23:00-01:00 Fock (Germany) observed in the 
     vicinity of Tycho, during an eclipse (mid eclipse at 23:56UT) a long 
     ray in the direction of Longomontanus that remained visible. It was 
     glowing in weak gray-green colour for the whole of the eclipse. The 
     Cameron 1978 catalog ID=373 and weight=2. The ALPO/BAA weight=1.


2026-Feb-02 UT 08:34-09:36 Ill=100% Aristarchus observed by Theiss on 1973-8-13

     Aristarchus 1973 Feb 15 UTC 17:07-19:31 Observed by Theiss (located at 
     51N 5.67E) "area 4-5 diameters of Aristarchus were coloured clearly 
     yellow-red" 120mm reflector used. Ref Hilbrecht & Kuveler (1984) Moon 
     and Planets Vol 30 p53-61. ALPO/BAA weight=1.


2026-Feb-02 UT 09:21-10:57 Ill=100% Kepler observed by Wildey on 1962-7-17

     Kepler 1962 Jul 17 UTC 06:24,08:36 Observed by Wildey, Pohn (Mt Wilson, 
     CA, USA, 60" reflector+photometer) "Crater was at Vmag 2.68 at earlier 
     obs. which was .47 mag brighter than av. mag. at 15d & it faded to near 
     normal at later time to V=3.10(photom. measures), a change of 1/2 mag. 
     or @1.5 times in brightness" NASA catalog weight=5 (very good). NASA 
     catalog ID #761.


2026-Feb-02 UT 09:36-10:43 Ill=100% Plato observed by Livesey_R on 1973-8-13

     Plato 1973 Aug 13 UT 22:25-22:35 observed by Pedler (Devon, UK). 
     Observer noticed a slight blink on a lighter patch on the floor 
     just beneath the south(?) rim using Moon blink filters. 
     ALPO/BAA weight=1.


2026-Feb-02 UT 11:33-13:09 Ill=100% Kepler observed by Wildey on 1962-7-17

     Kepler 1962 Jul 17 UTC 06:24,08:36 Observed by Wildey, Pohn (Mt Wilson, 
     CA, USA, 60" reflector+photometer) "Crater was at Vmag 2.68 at earlier 
     obs. which was .47 mag brighter than av. mag. at 15d & it faded to near 
     normal at later time to V=3.10(photom. measures), a change of 1/2 mag. 
     or @1.5 times in brightness" NASA catalog weight=5 (very good). NASA 
     catalog ID #761.


2026-Feb-02 UT 11:54-12:50 Ill=100% Tycho observed by Chrevremont on 1898-1-8

     On 1898 Jan 08 at UT 00:00-01:00 Chrevremont (France?) notcied that 
     during a lunar eclipse, the mid-eclipse shadow was so dark that details 
     of the surface disappeared, all except for the Tycho SSW ray . Cameron 
     comments that it is unsual for that ray to remain when usually the ones 
     towards Kepler and Aristarchus are the ones to stand out? The Cameron 
     1978 catalog ID=297 and the weight=0. The ALPO/BAA weight=1.


2026-Feb-02 UT 12:29-14:22 Ill=99% Aristarchus observed by Coates_J on 1978-8-18

     On 1978 Aug 18 at UT 22:00 Coates (England?, UK, 3" refractor, 
     seeing=II) found that the inner bands of Aristarchus were hard to see, 
     this was odd because the seeing conditions were good and he usually 
     sees them? However he did not believe that there was any obscuration 
     going on. The Cameron 2006 catalog ID=37 and weight=0. The ALPO/BAA 
     weight=1.


2026-Feb-02 UT 13:27-15:10 Ill=99% Moon observed by deMoraes on 1893-4-1

     On 1893 Apr 01 at UT 22:00 deMoraes of the Azores, Portugal, saw a 
     shaft of light projecting from the Moon. Cameron 1978 catalog ID=280 
     and weight=0. ALPO/BAA weight=1.


2026-Feb-02 UT 16:15-18:58 Ill=99% Aristarchus observed by Porter on 1978-8-19 *

     On 1978 Aug 19 at UT02:45-04:00 Porter (Naragansetts, RI, USA, using a 
     6" reflector, Seing = 6/10) noticed blue on the north east corner of 
     Aristarchus and an orange glow on the south east wall. They detected no 
     movement or change in brightness. The observer used both eyes, to make 
     sure it was not an eye defect, and three filters: red Wratten 25, blue 
     Wratten 82 and Violet Wratten 47. Porter found that the colours faded 
     for a duration of 5 minutes and then returned. Their right eye gave a 
     good view and using their left eye they suspected that it was 0.5 steps 
     brighter than the remainder of the crater. The suspected colour 
     remained visible, even under moments of good seeing conditions. The 
     colour eventually faded over time and was eventually gone. Porter 
     reportd seein gcolour here on the following night. Apparently other 
     bright spots showed no colour. Fitton suggests that the filters used 
     confirm that the south east wass was definitely red in colour. The 
     Cameron 2006 catalog ID=37 and the weight=0. ALPO/BAA weight=1.


2026-Feb-02 UT 16:30-17:26 Ill=99% Manilius observed by Firsoff on 1955-8-3

     Manillus 1955 Aug 03 UTC 21:00 Observed by Firsoff (Sommerset, England, 
     6.5" reflector, x200) "Maniluus very bright in all colors, especially 
     blue, extraordinarily so" NASA catalog weight=4 (good). NASA catalog ID 
     #602.


2026-Feb-02 UT 16:30-17:26 Ill=99% Timocharis observed by Firsoff on 1955-8-3

     Timocharis 1955 Aug 03 UTC 21:00 Observed by Firsoff (Sommerset, 
     England, 6.5" reflector, x200) "Crater was bright in blue, seemed large 
     & diffused." NASA catalog weight=4 (good). NASA catalog ID #602.


2026-Feb-02 UT 17:13-17:59 Ill=99% Aristarchus observed by Chernov on 1954-7-16

     In 1954 Jul 16 at UT 01:12 Chernov (Russia, 2" refractor, x33) observed 
     the following for Aristarchus: "Activity noted in it * in extension of 
     Moon's shadow on sky for 12 min during .17phase of ecl.(source gave 
     date as June 16, but ecl was July 16)". The Cameron 1978 catalog ID=566 
     and weight=1. The ALPO/BAA weight=1. 


2026-Feb-03 UT 09:24-10:59 Ill=97% Littrow observed by Unknown_English_Observer on 1915-1-31

     Littrow 1915 Jan 31 UTC 22:00? Observer: unknown (England?) "6 to 7 
     spots arranged like a gamma first seen on this nite. (Kuiper atlas. 
     Rect. 14-c shows spots in form of a 7 or a cap. gamma backwards, but 
     not l.c. gamma)". NASA catalog weight=0 (almost certainly not a TLP). 
     NASA catalog ID #349. ALPO/BAA weight=1.


2026-Feb-03 UT 09:24-09:54 Ill=97% Copernicus observed by Rawlings_G on 1978-4-23

     On 1978 Apr 23 at UT20:35 (Rawlings, UK, finderscope, x50) 
     observed a bright flash (~0.3 sec duration) near to Copernicus (20W, 
     9N) with rays to the south east whilst he looked through a finder 
     scope. Moore, who studied the drawing, suggests that the area of the 
     flash was near Copernicus. However Cameron says this cannot be the case 
     if the flash was in darkness as mentioned in the BAA Lunar Section 
     circular. She comments that it might have been a meteor? The Cameron 
     2005 catalog ID=28 and weight=1. The ALPO/BAA weight=1.


2026-Feb-03 UT 09:27-10:50 Ill=97% Proclus observed by Bartlett on 1955-11-1

     Proclus 1955 Nov 01 UTC 02:50-03:05 Observed by Bartlett (Baltimore, 
     MD, USA, 3.5" reflector x100, S=6, T=5) "Proc. D normally 5 deg bright 
     was vis. tonite only in blue light, whereas usually is vis. in 
     integrated light. However at col. 110.5 deg it was a dark spot (see #
     816) C.p. tonite was normal 5 deg bright but in Oct. lun. was dark". 
     NASA catalog weight=4 (good). NASA catalog ID #625. Note Proclus D does 
     not refer to the crater Proclus D as defined by the IAU, but probably 
     to a spot inside the crater that Bartlett designated D!


2026-Feb-03 UT 09:35-10:37 Ill=97% Aristarchus observed by Thomas on 1970-2-22

     Aristarchus 1970 Feb 22 UTC 07:00? Observed by Thomas, Stump, Corral. 
     Obs. (Organ Pass, NM, 24" reflector+Moonblink) "Bluing around crater -- 
     vis. in monitor, but not photographable due to clouds." NASA catalog 
     weight=4 (good). NASA catalog ID #1235.


2026-Feb-03 UT 12:59-14:35 Ill=97% Mare_Crisium observed by Wildey on 1962-7-18

     Mare Crisium 1962 Jul 18 UTC 09:54 Observed by Wildey & Pohn (Mt 
     Wilson, CA, USA, 60" reflector + Photometer) "Photometric meas. showed 
     change in brightness of the area of over a mag. during the nite. 
     Recorded at Vmag=3.56 first, & a few min(?) later at 4.62. It was .95 
     mag. brighter (@2.5x) than av. for that age & then returned to 
     normal." NASA catalog weight=5 (very high). NASA catalog ID #762.


2026-Feb-03 UT 14:58-16:55 Ill=96% Aristarchus observed by Louderback_D on 1992-7-16

     On 1992 Jul 16 at UT 03:32-09:31 D. Louderback (South Bend, WA, USA, 
     3" refractor, x134) detected yellow on the southern rim of Aristarchus, 
     and the colour looked "darker" through a yellow filter and the region 
     was "duller" than normal. The region was 1 intesnsity step brighter on 
     the 2nd measurement, "on all points in it". The comet tail-like ray had 
     3 sections and was "mottled" in appearance. Finally the Cobra Head 
     region had possible variations in brightness. The cameron 2006 catalog 
     ID=451 and the weight=3. The ALPO/BAA weight=2.  


2026-Feb-03 UT 15:13-16:58 Ill=96% Gassendi observed by Haas_W on 1940-9-18

     Gassendi 1940 Sep 18 UTC 03:15 Observed by Haas (New Mexico? 12" 
     ? reflector) "Largest bright spot in SE part of floor had I=6.1, 
     but I=6.7 & 8.6 on other nites. (same ph. see #469, 472 & 475)" 
     NASA catalog weight=4. NASA catalog ID #474. ALPO/BAA weight=2. 


2026-Feb-03 UT 15:21-17:05 Ill=96% Picard observed by Ingall on 1864-10-16

     East of Picard 1864 Oct 16/17 UT 23:00-01:00? Observed by 
     Ingall (Camberwell ?, UK) "Remarkable bright spot" NASA 
     catalog weight=3. NASA catalog ID #135. ALPO/BAA weight=3.


2026-Feb-04 UT 10:12-11:18 Ill=92% Plato observed by Gledhill on 1870-2-17

     Plato 1870 Feb 18 UTC 00:00? Observed by Gledhill (Halifax, England, 
     9" refractor) "Illum. of another group of craters different from group 
     in Aug. & Sep. obs. (date is F18 if phase is similar to Ap 1870)
     NASA catalog weight=2 (low). NASA catalog ID #164.


2026-Feb-04 UT 10:12-10:38 Ill=92% Aristarchus observed by Corralitos on 1970-2-23

     Aristarchus 1970 Feb 23 UTC 07:00? Observed by Thomas & Stump 
     (Corralitos Observatory, Organ PAss, NM, USA, 24" refletor+Moon Blink) 
     "Bluring around crater -- vis. in monitor, but not photographed due to 
     clouds." NASA catalog weight=4 (good). NASA catalog ID #1235.


2026-Feb-04 UT 10:12-10:46 Ill=92% Mons_Piton observed by Louderback_D on 1990-8-8

     On 1990 Aug 08 at OT 07:47-09:00 UT D. Louderback (South Bend, WA, USA, 
     3" refractor, x173) "(SS) Piton's all pts were << but nearby plain was 
     normal. Ridges at 5.3 at B, C, D but 3 alb at B, C, D (norm = 7) but 
     bearby plain was normal. At A 3, was hazy but ill defined. Parts of mt 
     brightened but others didn't. Times between brightening were 6-8s. 
     Similar to seeing fluctuations. In red mt stayed dull & steady. In blue 
     it blinked." - this is a direct quote from the Cameron 2006 catalog 
     because it is very difficult to summarize. Louderback comments that the 
     TLP was still going on at 09:00UT. The Cameron 2006 catalog ID=406 and 
     the weight=4. The ALPO/BAA weight=3.


2026-Feb-04 UT 10:12-10:46 Ill=92% Promontorium_Agarum observed by Darling_D on 1990-8-8

     On 1990 Aug 08 at UT 07:47-09:00 D. Darling (Sun Praire, WI, USA, 3" 
     refractor, x173) reported the following TLP in Promontorium Agarum 
     (Cape Agarum): "W flank of CA >>, even> Proc. interior." The cameron 
     2006 catalog ID=406 and the weight=4. The ALPO/BAA weight=3.


2026-Feb-04 UT 10:41-12:17 Ill=92% Mare_Crisium observed by Wildey on 1962-7-19

     Mare Crisium 1962 Jul 19 UTC 07:30 Observed by Wildey & Pohn (Mt 
     Wilson, CA, USA, 60" reflector + Photometer) "Photometric meas. showed 
     change in brightness from Vmag=3.46 to V=3.07, where av. mag. for that 
     age=3.26, or a brightening of .58 mag." NASA catalog weight=5 (very 
     high). NASA catalog ID #763.


2026-Feb-04 UT 11:32-13:27 Ill=92% Plato observed by Haas_W on 1938-6-15

     Plato 1938 Jun 15 UTC 08:00 Observed by Haas? (New Mexico?, 12?" 
     reflector) "NW. end of floor had intensity I=2.0, but on 7/15/38, I=
     3.7, conditions similar." NASA catalog weight=4 (high). NASA catalog ID 
     #439.


2026-Feb-04 UT 12:43-14:34 Ill=92% Unknown observed by Cragg on 1965-5-18

     On 1965 May 18 at UT 03:00-03:30 Cragg (Mt Wilson?, CA, USA, 6" 
     refractor?) observed a TLP (no feature nor description given in 
     the Cameron 1978 catalog) on the Moon. The Cameron 1978 catalog ID=877 
     and weight=4. The ALPO/BAA weight=1.


2026-Feb-04 UT 13:00-14:36 Ill=92% Mare_Crisium observed by Wildey on 1962-7-19

     Mare Crisium 1962 Jul 19 UTC 09:48 Observed by Wildey & Pohn (Mt 
     Wilson, CA, USA, 60" reflector + Photometer) "Photometric meas. showed 
     change in brightness from Vmag=3.46 to V=3.07, where av. mag. for that 
     age=3.26, or a brightening of .58 mag." NASA catalog weight=5 (very 
     high). NASA catalog ID #763.


2026-Feb-04 UT 13:01-16:57 Ill=92% Aristarchus observed by Pedler_J on 1990-1-13 *

     On 1990 Jan 13 at UT 22:15-23:05 J. Pedler (Bristol, UK, seeing=III and 
     transparency=excellent, no spurious colour) detected a blue region on 
     the north of Aristarchus, varying in sharpness/diffuseness. The crater 
     rim in this region could not be descerned. Eleswhere the crater rim was 
     normal as too were other features. When a Moon blink device was used, 
     no colour blink was detected, however through the blue filter the 
     suspected area was bright and the crater rim indistinct. Whereas 
     through the red filter the area looked perfectly normal. At 22:30UT the 
     effect had vanished and everywhere was normal. The Cameron 2006 catalog 
     ID=388 and the weight=5. The ALPO/BAA weight=3.


2026-Feb-04 UT 16:00-18:58 Ill=91% Aristarchus observed by Cook_MC on 1990-1-14 *

     On 1990 Jan 14 at UT 01:14-01:55 M.C. Cook (Frimley, UK, seeing=poor) 
     observed that Aristarchus did not appear normal for this illumination. 
     the northern half of Aristarchus was "2x>" than the southern half of 
     the crater. There were two white patches of apron material near to the 
     crater Herodotus that were 50% of the brightness of the southern half 
     of Aristarchus. Furthermore the southern half of Aristarchus had a 
     circle - "dull patch on inner S wall with a bright point shining 
     through it. (Bartlett's EWBS?)". The Cameron 2006 catalog ID=389 and 
     the weight=4. The ALPO/BAA weight=2.


2026-Feb-04 UT 16:51-18:00 Ill=91% Mare_Crisium observed by Eysenhard on 1774-7-25

     Four bright spots seen in Mare Crisium. There was also peculiar 
     behaviour of the terminator. Source: Midlehurst 1968 catalog TLP ID=16. 
     Ref Web 1962 p62-76. The ALPO/BAA weight=1.


2026-Feb-04 UT 17:22-18:58 Ill=91% Peirce observed by Darling_D on 1980-3-4

     On 1980 Mar 04 at UT10:30-10:34 D. Darling (Sun Prairie, WI, USA, 
     12.5" reflector, x344) detected a pin-point light in the shadowed area 
     of Mare Crisium that varied in brightness then faded. Cameron 2006 
     catalog ID=84 and weight=0. ALPO/BAA weight=1.


2026-Feb-04 UT 17:28-18:58 Ill=91% Gassendi observed by Haas_W on 1940-9-19

     Gassendi 1940 Sep 19 UTC 06:00 Observed by Haas (New Mexico, 
     12?" reflector) "Largest bright spot in SE part of floor, had I=
     6.7, but 6 for last nite & 5.6 on others (see #'s 469, 472, & 
     474)." NASA catalog weight=4. NASA catalog ID #475. ALPO/BAA 
     weight=2.


2026-Feb-05 UT 12:49-14:12 Ill=85% Aristarchus observed by Brook_C on 2002-5-30

     On 2002 May 30 at UT02:30-02:44 C. Brook (Plymouth, UK) suspected that 
     Aristarchus crater looked dimmer than normal. The ALPO/BAA weight=1.


2026-Feb-06 UT 12:33-14:29 Ill=77% Romer observed by Darling_D on 1979-8-12

     On 1979 Aug 12 at UT07:00-10:35 D. Darling and wife (Sun Prarie, WI, 
     USA, 12.5" reflector, x342, photos, S=9/10) observed a cigar shaped 
     protruberance in Romer crater that cast a 32km long shadow, nestled in 
     a valley rille next to Romer. This was a confirmed observation. The 
     effect persisted intil sunset. The top of the object and two points on 
     the crater rim were reflecting the Sun's rays. "Top of obj. & 2 pts on 
     crater rim reflected suns rays. It was as high as the crater rim 
     whereas the rill wall was not. Took photos. he has studied this area 
     and never saw such a phenom before. Photos did not show it". The 
     Cameron 1978 catalog ID=65 and weight=5. The ALPO/BAA weight=2.


2026-Feb-06 UT 16:15-18:13 Ill=76% Aristarchus observed by Dachille on 1957-10-13

     Observed by Dachille & daughter (Univ. Park, Pennsylvania, 10.5"
     reflector, x75) "Flash -- then a brownish - red color patch. Alt. @
     20deg. (MBMW has Oct. 12, but is 13th UT)". NASA catalog weight=5 
     (very good). NASA catalog ID #674.


2026-Feb-07 UT 15:31-16:18 Ill=67% Aristarchus observed by Doherty_EG on 1964-1-5

     In 1964 Jan 05 at UT 22:00? Doherty (Stoke-on-Trent, UK, 3" refractor, 
     8" or 10" reflector) observed aristarchus to be purplish-blue in 
     colour. The Cameron 1978 catalog ID=794 and weight=3. The ALPO/BAA 
     weight=2.


2026-Feb-08 UT 13:45-15:34 Ill=58% Gassendi observed by Whippey_MR on 1966-12-4

     Gassendi 1966 Dec 04 UTC 01:05-01:23 Observed by Whippey (Northolt? 
     England, 6" reflector, x212) "Abrupt flash of red, setling in 
     immediately to a pt. of red haze nr. NW (ast.?) wall. Continuous till 
     0123 (date given was 4-12-66 = European convention?)." NASA catalog 
     weight=3 (average). NASA catalog ID #1000.


2026-Feb-08 UT 14:10-15:29 Ill=58% Gassendi observed by Whippey_MR on 1966-4-12

     On 1966 Apr 12 at UT 01:05-01:23 Whippey (Northolt, England, UK, 6" 
     reflector x212) and Corralitos Observatory (Organ Pass, NM, USA, 24" 
     Moon Blink) observed in Gassendi: "Abrupt flash of red, settling 
     immediately to a point of red haze near NW (IAU?) wall. Continuous till 
     0123h. (Not confirmed at Corralitos Obs. MB--at same time?". The 
     Cameron 1978 catalog ID=927 and weight=3. The ALPO/BAA weight=2. 


2026-Feb-08 UT 15:18-16:29 Ill=58% Unknown observed by Markov on 1964-1-6

     On 1964 Jan 06 at 02:00? Markov and Khoshlova (Russia) observed 
     anomalous IR radiation on the Moon. The Cameron 1978 catalog ID= and 
     weight=5. The ALPO/BAA weight=3.


2026-Feb-08 UT 17:51-18:57 Ill=57% Kepler observed by deBerard on 1966-12-4

     Kepler 1966 DEc 04 UTC 05:10 Observed by de Beraud (Flossmoore, 
     Ilinois, USA, 6" reflector, x360, S=G) "Saw a bright area thru. blue 
     filter but could not see it in red filter. Decided it was a bluish 
     phenomenon." NASA catalog weight=3 (average). NASA catalog ID #1001.


2026-Feb-08 UT 18:30-18:57 Ill=57% Aristarchus observed by Madej_P on 1983-1-5

     On 1983 Jan 05 at UT22:00 P. Madej (Huddersfield, UK) noticed some 
     colour on Aristarchus. The Cameron 2006 catalog ID=195 and the weight=
     2. The ALPO/BAA weight=1.


2026-Feb-09 UT 14:13-18:34 Ill=48% Earthshine: Alpha Centaurids: ZHR=6 (vel=58km/s)

2026-Feb-10 UT 15:06-16:03 Ill=39% Aristarchus observed by Pasternak on 1973-12-18

     On 1973 Dec 18 at UT06:35-06:38 Pasternak (53deg 20' N and 7deg 30' E, 
     using 75mm reflector, focal length 700mm, transparency 1 out of 5 and 
     seeing 2 out of 5) observed a faint brightening in the south wall of 
     Aristarchus. Published in Hilbrecht and Kuveler, Moon and Planets, 30 
     (1984) p53-61. ALPO/BAA weight=1.


2026-Feb-10 UT 15:51-17:45 Ill=39% Aristarchus observed by Moseley_R on 1983-12-28

     On 1983 Dec 28 at UT03:30-05:00 Moseley (Covington, England, UK, 
     seeing=V-IV and transparency=good) detected some detail within the 
     shadow under good moments of seeing. The external brightness was 
     extended to the east wall at a clock position of 9 O'clock, but did not 
     go outside the rim. It was less bright at the 11 O'clock position. The 
     Cameron 2006 catalog ID=236 and the weight=3. The ALPO/BAA weight=2.


2026-Feb-10 UT 15:06-18:34 Ill=38% Earthshine: sporadic meteors

2026-Feb-11 UT 16:00-18:34 Ill=29% Earthshine: sporadic meteors

2026-Feb-12 UT 17:40-17:49 Ill=21% Posidonius observed by Dzapiashvili on 1956-7-3

     On 1956 Jul 30 at UT 19:13 Dzapiashvili (Pulkova, Russia) observed the 
     following in Posidonius: "Short term sharp changes in polarization in 
     crater (in ashen light)". The Cameron 1978 catalog ID=643 and weight=5. 
     The ALPO/BAA weight=5.


2026-Feb-12 UT 16:52-18:34 Ill=21% Earthshine: sporadic meteors

2026-Feb-13 UT 17:43-18:33 Ill=14% Earthshine: sporadic meteors

2026-Feb-13 UT 18:33-18:56 Ill=14% Alphonsus observed by Cross on 1966-4-17

     Alphonsus 1966 Apr 17 UT 05:06 Observed by Cross (England) "Blink on SW 
     floor of Alphonsus (moon rise @ 04:20, rotating filterblink rechnique 
     without image tube that Tridant and Corralitos had)." NASA catalog 
     weight=3 (average). NASA catalog ID #928


2026-Feb-14 UT 18:31-18:33 Ill=7% Earthshine: sporadic meteors

2026-Feb-19 UT 06:44-00:00 Ill=3% Aristarchus observed by Sadler_H on 1874-4-18

     On 1874 Apr 18 at before 21:30UT? H. Sadler saw Aristarchus looking 
     like a magnitude 9.5 star. However it faded at 21:30UT by 0.5 
     magnitudes. Some faint light streaks could be seen coming from it in 
     north east and westerly directions. Three fainter spots were seen, 
     probably at: Menelaus, Manilius and Sosigenes (this was the faintest).
     Ref: English MEchanic, Vol 19, p146, 1874.


2026-Feb-19 UT 06:44-00:00 Ill=3% Manilius observed by Sadler_H on 1874-4-18

     On 1874 Apr 18 at before 21:30UT? H. Sadler saw Aristarchus looking 
     like a magnitude 9.5 star. Some faint light streaks could be seen 
     coming from it in north east and westerly directions. Three fainter 
     spots were seen, probably at: Menelaus, Manilius and Sosigenes (this 
     was the faintest). Ref: English MEchanic, Vol 19, p146, 1874.


2026-Feb-19 UT 06:44-00:00 Ill=3% Menelaus observed by Sadler_H on 1874-4-18

     On 1874 Apr 18 at before 21:30UT? H. Sadler saw Aristarchus looking 
     like a magnitude 9.5 star. Some faint light streaks could be seen 
     coming from it in north east and westerly directions. Three fainter 
     spots were seen, probably at: Menelaus, Manilius and Sosigenes (this 
     was the faintest). Ref: English MEchanic, Vol 19, p146, 1874.


2026-Feb-19 UT 06:44-00:00 Ill=3% Sosigenes observed by Sadler_H on 1874-4-18

     On 1874 Apr 18 at before 21:30UT? H. Sadler saw Aristarchus looking 
     like a magnitude 9.5 star. Some faint light streaks could be seen 
     coming from it in north east and westerly directions. Three fainter 
     spots were seen, probably at: Menelaus, Manilius and Sosigenes (this 
     was the faintest). Ref: English MEchanic, Vol 19, p146, 1874.


2026-Feb-20 UT 06:51-07:34 Ill=9% Promontorium_Olivium observed by Rodriguez_H on 1988-2-20

     On 1988 Feb 20 at UT22:25-22:34 H. Rodriguez Moreira (Fortaleza, 
     Brazil, 4" refractor) observed a rapid rise in brightness at 
     22:25UT in Promintorium Olivium. About 4 minutes after this the 
     brighness fluctuated 3 times and the TLP faded in 9 minutes 
     after it started, returning everything to normal. "Bluish light 
     point on darkside of it" - apparently a Greek observer (Aguirre) 
     observed a flash but no date was given. The Cameron 2006 catalog 
     ID=317 and the weight=3. The ALPO/BAA weight=3.


2026-Feb-20 UT 07:09-07:36 Ill=9% Earthshine: sporadic meteors

2026-Feb-21 UT 07:51-08:23 Ill=16% Aristarchus observed by Schroter on 1786-12-24

     Schroter observed Aristarchus to be extraordinarily bright on the dark
     side of the Moon. Cameron 1978 catalog ID=30 and weight=4. ALPO/BAA 
     catalog weight=2.


2026-Feb-21 UT 07:09-08:25 Ill=16% Earthshine: sporadic meteors

2026-Feb-22 UT 06:45-07:15 Ill=25% Aristarchus observed by Foley_PW on 1977-4-23

     1977 Apr 23 UT19:30-22:45 Foley (10.75" Newtonian and 4.5" 
     refractor, seeing II, transpaency excellent) saw som every large 
     variations in the brightness of Aristarchus whereas other 
     features in Earthshine remained stable. Aristarchus was seen to 
     be blue/violet. ALPO/BAA weight=2.


2026-Feb-22 UT 07:09-09:17 Ill=26% Earthshine: sporadic meteors

2026-Feb-23 UT 07:53-09:08 Ill=36% Censorinus observed by Nicolini on 1959-9-8

     Censorinus 1959 Sep 08 UT 22:45-23:50 Observed by Jean Nicolini 
     (Brazil) "Much brighter than Proclus" NASA catalog weight=2. 
     NASA catalog ID #721. ALPO/BAA weight=2.


2026-Feb-23 UT 07:53-09:44 Ill=36% Messier observed by Robinson_JH on 1981-2-10

     Messier 1981 Feb 10 UT 19:20-20:10 TLP discoevered by Hedley 
     Robinson (Devon, England) "Messier was brighter than Aristarchus 
     in both red and blue filters and also appeared indistinct, later 
     becoming invisible - lost in a bright streak. In comparison 
     Aristarchus was clear. Another observer, Amery confirmed that 
     Aristarchus was sharp in appearance but Messier certainly was 
     not. Cook likewiese found Messier not to be as sharp as Messier 
     A dueto a big shadow in Messier A. Pedler found that the sun 
     facing wall of Messier was OK but that the shadow was changing 
     from black to grey periodically at intervals of 2-3 minutes to a 
     few seconds. By contrast he found that Messier A remained quite 
     well defined. He tried red and blue filters but found no blink 
     effect. At 20:23UT Pedler found that the shadow had stabilized 
     to a shade of "mid grey" although remaining ill-defined. North 
     also found that Messier A was distinct but Messier itself was 
     ill-defined. Moore found the same thing but thinks that this is 
     normal for Messier under this illumination to appear indistinct. 
     More also saw the grey interior shadow. Price saw similar 
     appearance to Moore and suspected that this was normal for this 
     stage in illumination. Ratcliffe suspected everything normal - 
     just commenting that Messier was smaller and no detail in 
     comparison to Messier A. Madej and Taylor provided a sketch that 
     showed again a grey interior and merging with the east 
     wall/mare. Foley found Messier's pale grey interior to be un-
     focusable but in comparison Messier A was sharp. He says that he 
     would expect a grey interior and the east wall to merge with the 
     mare. However the complete loss of deatil and variability were 
     not normal. Cameron comments that the Kuiper atlas confirms the 
     fuzzy indistinct appearance of Messier and that a Lunar Orbiter 
     picture shows a grey shadow. The Cameron extended catalog 
     weight=5. The ALPO/BAA weight=2.


2026-Feb-23 UT 08:04-08:46 Ill=36% Aristarchus observed by d_Adhuda on 1891-11-7

     On 1891 Nov 07 at UT=19:00 d'Adjuda of Lisbon, Portugal (seeing fair) 
     whilst observing Aristarchus noticed that the crater appeared as  very 
     distinct luminous point in the dark. Cameron 1978 catalog ID=275 and 
     weight=3. ALPO/BAA weight=1.


2026-Feb-23 UT 08:15-11:16 Ill=36% Langrenus observed by Dollfus_A on 1992-12-30 *

     On 1992 Dec 30 at UT 17:36 A. Dollfus (Meudon, France, 1m aperture 
     telescope used) detected evidence for a dust cloud using CCD 
     polarimetry. The ALPO/BAA weight=5.


2026-Feb-23 UT 10:04-10:09 Ill=37% Julius_Caesar observed by Colesanti_C on 1993-6-25

     On 25 Jun 1993 at UT 23:30-23:52 Carlos Colesanti (Mairinque, 
     Brazil) obtained two CCD images of Julius Caesar crater and 
     noticed a brilliant fuzzy area on the rim of the crater. This 
     appeared in both images and resembled a fuzzy white blob. Note 
     that this is a REA-Brazil observation. ALPO/BAA weight=1. 
     Cameron (2006) ID=463.


2026-Feb-23 UT 07:09-10:11 Ill=37% Earthshine: sporadic meteors

2026-Feb-24 UT 06:45-07:59 Ill=47% Messier observed by Robinson_JH on 1982-12-22

     On 1982 Dec 22 at UT 19:20-20:10 J-H Robinson (Teighmouth, Devon, UK, 
     10" reflector, x150, seeing=IV-V) could not distinguish between Messier 
     and Messier A. The tail of these features was very bright - two 
     telescopes were used. Moore (Selsey, UK, 12" reflector, seeing=III) 
     could see Messier A but found Messier itself obscured - just see the 
     west wall and thought that the comet like tail was unusual as it did 
     not appear divided. The Cameron 2006 catalog ID=192 and weight=5. The 
     ALPO/BAA weight=3.


2026-Feb-24 UT 07:09-11:09 Ill=49% Earthshine: sporadic meteors

2026-Feb-25 UT 06:57-08:36 Ill=59% Plato observed by Valderama on 1886-9-6

     Plato 1886 Sep 06 UT 19:00? Observed by Valderama (Italy?) "Streak of 
     light on dark floor of crater in shadow. (sunlight between peaks on 
     walls?)" NASA catalog weight=0 (most unlikely to be a TLP). NASA 
     catalog ID #251. ALPO/BAA catalog weight=1.


2026-Feb-25 UT 08:05-09:51 Ill=59% Plato observed by Kelsey on 1967-4-18

     Plato 1967 Apr 18 UT 03:10-04:00 Observed by Kelsey 
     (Riverside, CA, USA, 8" reflector x300, S=8, T-4-5). "Streak 
     on floor showed slight enhancement in red filter comp. to 
     blue. Later, a 2nd streak formed. Probably the sun shining 
     thru a valley in the rim. Red enhancement permanent? (Wise 
     suspected a blink here 6h earlier)." NASA catalog weight=3. 
     NASA catalog ID #1027. ALPO/BAA weight=1.


2026-Feb-25 UT 08:09-10:06 Ill=59% Aristarchus observed by Emmett on 1824-7-4

     In 1824 Jul 04 at UT23:00? Emmett (England, UK) observed a star-like 
     light on the rim (in the dark). The Cameron 1978 catalog ID=100 and the 
     weight=3. The ALPO/BAA weight=2.


2026-Feb-25 UT 09:25-10:12 Ill=60% Plato observed by Markov on 1916-7-8

     Plato 1916 Jul 8 UT 19:00? Observed by Markov (Russia) "Light on the 
     shadow of the bands at the bottom (similar to #362)" NASA catalog 
     weight=3 (average). NASA catalog ID #364. ALPO/BAA weight=2.


2026-Feb-25 UT 09:39-11:36 Ill=60% Alphonsus observed by Cook_AC on 1990-2-3

     Alphonsus 1990 Feb 03 UT 18:00-18:23 Observed by A.C. Cook 
     (Frimley, UK, CCD video camera, seeing III-IV). At 18:06 W and 
     SE dark floor patches, equally dark, but at 18:10 and 18:23 the 
     W dark patch was the darker of the two?. Between 18:06 and 18:23 
     and a bright patch to the north of the central peak brightned 
     slightly wrt the its surroundings. However seeing conditions 
     worsened as the observing session progressed, and in view of 
     this the ALPO/BAA weight=1.


2026-Feb-25 UT 10:10-12:03 Ill=60% Plato observed by Fauth on 1907-1-22

     Plato 1907 Jan 22 UT 20:00 Observed by Fauth (Germany?) "Glow of light 
     in part of crater" NASA catalog weight=3 (average). NASA catalog 
     ID 327.


2026-Feb-25 UT 11:10-12:08 Ill=60% Tycho observed by Shaw_B on 2003-5-9

     Tycho 2003 May 09 UT 21:04 Observer Brendan Shaw (UK) "CCD 
     image of  central peak - Sun's altitude suggested that this 
     should not have been directly illuminated this early - may 
     have been from secondary reflectance off illuminated W wall?" 
     ALPO/BAA weight=1.


2026-Feb-25 UT 11:34-12:08 Ill=60% Alphonsus observed by Brook_C on 1990-2-3

     Alphonsus 1990 Feb 03 UTC 20:05-21:22 Observed by Brook (Plymouth, UK, 
     10" reflector)  "Brightness variance noted". The Cameron 2006 catalog 
     does not have an entry for this observation. The ALPO/BAA weight=2.


2026-Feb-26 UT 06:45-08:14 Ill=70% Copernicus observed by Barker_R on 1932-3-16

     Copernicus 1932 Mar 16 UTC 18:45-19:30 Observed by Barker (Cheshunt, 
     England, 12.5" reflector, x310) "Term. from Cop. to lat.20S was misty & 
     hard to define. Rest was usual sharp definition. Mistiness cleared at 
     1930. Cleaned his eyepiece & prism but it persisted." NASA catalog 
     weight=3 (average). NASA catalog ID #402.


2026-Feb-26 UT 06:45-07:14 Ill=70% Plato observed by Carle on 1952-2-5

     On 1952 Feb 05 at UT 05:10 J.Carle (USA, 8" reflector, x180) 
     observed the following in Plato: "A shadow in a depression, or 
     a cloud, or an optical illus.? Oval dark area nr. center, 
     disappeared in 15m clear & prominenet at first then vanished. 
     4 of 14 spots nr. center continuously seen while remaining 
     ones seen only momentarily. (seeing?) Drawing includes sketch 
     on March 7. His sketch shows 18 spots, 13 same as here". The 
     Cameron 1978 catalog ID=549 and the weight=2. The ALPO/BAA 
     weight=2.


2026-Feb-26 UT 06:45-07:48 Ill=70% Alphonsus observed by Kelsey on 1966-11-22

     Alphonsus 1966 Nov 22 UT 03:17-03:40 Observed by kelsey (Riverside, CA, 
     USA, 8" relector x300) "Seen first with (Eng.) moon blink, red  filter 
     but not in the green. Not seen at 03:42h" NASA catalog weight=4 (high). 
     NASA catalog ID #998.


2026-Feb-26 UT 06:45-07:44 Ill=70% Alphonsus observed by Ringsdore_P on 1969-3-27

     On 1969 Mar 27 at UT 18:42-18:47 Ringsdore (England, 15" 
     reflector, x350), Moseley (Armagh, Northern Ireland) and P. 
     Moore (Selsey, UK) observed nothing unusual in Alphonsus at 
     18:40UT, but at 18:45UT Ringsdore saw a blurring. At 18:43UT 
     Mosely saw a reddush-orange patch and this was confirmed by 
     Moore. NNW of the central peak, Mosely got a blink, but Moore 
     did not because of too much stray light. The colour was like
     Jupiter's red spot, but less pronounced. The Cameron 1978 
     catalog ID=1118 and weight=5. The ALPO/BAA weight=4.


2026-Feb-26 UT 06:45-00:00 Ill=70% Mons_Hadley observed by Miranda on 1971-7-31

     On 1971 Jul 31 at UT 21:40 (18:40 local time?) Miranda (Plaui, Brazil, 4" Refractor, 80x, 160x, Moon 70deg in altitude) 
     observed an intermittent and curious brilliance on top of a peak 
     (with irregular reflection) north of Mons Hadley (5E, 27N). The 
     Cameron 1978 catalog ID=1302 and weight=2. The ALPO/BAA 
     weight=2.


2026-Feb-26 UT 10:54-12:39 Ill=71% Archimedes observed by Theiss on 1973-1-13

     Archimedes 1973 Jan 13 UTC 19:06-19:40 Observed by Theiss (51N, 9.67E, 
     75mm refractor) "Yellow to green colours at wall of Archimedes, became 
     stronger until 19:09UT, constant brightness until 19:10UT and 
     dissappeared at 19:16UT" Ref: Hilbrecht & Kuveler (1984) Moon & Planets 
     30, pp53-61.


2026-Feb-26 UT 11:18-13:03 Ill=71% Proclus observed by Krojer on 1973-1-13

     Proclus 1973 Jan 13 UTC 19:30-19:35 Observed by Krojer (48.25N, 11.5E, 
     60mm refractor) "North East wall of Proclus extraordinarilly bright, 
     observation interrupted by fog." Ref: Hilbrecht & Kuveler (1984) Moon & 
     Planets 30, pp53-61.


2026-Feb-26 UT 11:26-12:05 Ill=71% Mons_La_Hire observed by Klein_HJ on 1887-2-2

     La Hire 1887 Feb 02 UTC 20:00? Observed by Klein (Cologne, Germany, 6" 
     refractor) "Intense yellow streak that cast shadows around neighboring 
     features". NASA catalog weight=4 (good). NASA catalog ID #255.
     


2026-Feb-26 UT 11:50-13:11 Ill=71% Censorinus observed by Leitzinger on 1973-1-13

     Censorinus 1973 Jan 13 UTC 20:02-20:14 Observed by Leitzinger (48.25N, 
     11.5E, 60mm refractor) "Censorinus Extraordinarily bright, pure white" 
     Ref: Hilbrecht & Kuveler (1984) Moon & Planets 30, pp53-61.


2026-Feb-26 UT 11:55-14:22 Ill=71% Mons_Pico observed by Mobberley_M on 1987-3-9 *

     On 1987 Mar 09 at UT20:00 M. Mobberley (Sussex, UK) obtained some video 
     of Mons Pico - apparently these show the mountain with a puzzling 
     appearance (not sure whether it was the observer who claimed this or 
     some one who analyzed the tape). The Cameron 2006 catalog ID=300 and 
     the weight=5. ALPO/BAA=1. 


2026-Feb-26 UT 12:52-13:11 Ill=72% Alphonsus observed by Smith_S on 1966-4-29

     Alphonsus 1966 Apr 20 UT 22:28 Observed by Smith (Nottingham, 
     England, 10" reflector) Reddish patch possibly detected on SE 
     flank of central peaks, but more dubious than that from 28th 
     Apr. ALPO/BAA weight=1.


2026-Feb-27 UT 06:45-07:10 Ill=80% Plato observed by Unknown_Observer on 1882-5-27

     On 1882 May 27 ay UT 20:00 an unknown observer (10" reflector) saw a 
     bright luminous ray near west (astronomical?) wall on floor of Plato. 
     Cameron suggests sunlight between peaks?. The Cameron 1978 catalog ID=
     233 and weight=0. The ALPO/BAA weight=1.


2026-Feb-27 UT 07:39-09:30 Ill=80% Sinus_Iridum observed by Manske_R on 1987-10-3

     On 1987 Oct 03 at UT 01:0?0-02:00 R. Manske (Brooklyn, WI, USA, 8" 
     reflector, x226) observed sunlight glinting of the walls in spectacular 
     display of colours. White (even gold) was seen at the centre, and blue 
     on the top most part of the rim. The white (or gold) band was thin in 
     comparison to other bands. The observer suspects that this effect was 
     terrestrial atmosphere related. Cameron 2006 catalog ID=307 and weight=
     0. ALPO/BAA weight=1. 


2026-Feb-27 UT 07:54-09:14 Ill=80% Ross_D observed by Cross on 1966-11-23

     Ross D 1966 Nov 23 UT 04:50-05:02 Observed by Cross (Whittier, 
     CA, USA, 19" reflector, x250 & 2390, S=4-5 (sometimes 6), T=4, 
     excellent contrast) Activity level 5, eastern third of Ross D's 
     circumference possibly partly obscured. ALPO/BAA weight=1.


2026-Feb-27 UT 11:58-12:59 Ill=81% Gassendi observed by Sartory on 1966-4-30

     Gassendi 1966 Apr 30 UT 21:30-23:28 Observed by Sartory, 
     Ringsdore (England, 8.5" reflector, S=E), Moore, Moseley 
     (Armagh, Northern Ireland, 10" refractor, S=VG), Coralitos 
     Observatory (Organ Pass, NM, USA, 24" reflector, Moon Blink) 
     "English moon blink system detected red spots with vis. 
     confirm. Ringsdore says no color but saw obscuration. (LRL 
     60-in photos showed nothing unusual by my casual inspection). 
     Indep. confirm. (even E. wall was in dark). Corralitos did 
     not confirm by MB." N.B. event had finished by the time 
     Corralitos came on-line. NASA catalog weight=5. NASA catalog 
     ID #931. ALPO/BAA weight=4.


2026-Feb-28 UT 06:45-08:16 Ill=88% Hyginus observed by Bradford on 1959-9-13 *

     Near Hyginus 1959 Sep 13 UT Observed by Bradford (S.Shields, 
     England, 15"? reflector), Feist, Lovas (Hungary), Moore, Wilkins 
     (Kent, England, 7" refractor, x500) "Obliterated by a hovering 
     cloud (Feist disagrees). Budapest obs. saw a cloud at 21:02:30, 
     lasting 5 m. Moore & Wilkins saw burst of light & dust cloud at 
     21:02:35 (confirm.) Drawing by Lovas." NASA catalog weight=5 and 
     catalog ID #722. The ALPO/BAA weight=1.


2026-Feb-28 UT 06:45-08:16 Ill=88% Littrow observed by Bradford on 1959-9-13 *

     Littrow, 1959 Sep 13 UT Observed by Bradford (S.Shields, 
     England, 15"? reflector), Feist, Lovas (Hungary), Moore, Wilkins (Kent, 
     England, 7" refractor, x500) "Obliterated by a hovering cloud (Feist 
     disagrees). Budapest obs. saw a cloud at 21:02:30, lasting 5 m. Moore & 
     Wilkins saw burst of light & dust cloud at 21:02:35 (confirm.) Drawing 
     by Lovas." NASA catalog weight=1 and catalog ID #722. The ALPO/BAA 
     weight=1.


2026-Feb-28 UT 07:00-08:46 Ill=88% Aristarchus observed by Darling_D on 1991-1-26

     On 1991 Jan 26 at UT 23:38-23:50 D. Darling (Sun Praire, WI, 
     USA, 12.5" reflector, x159 and 3" refractor x90, seeing 5/10, 
     transparency 3/6) found that Aristarchus was brighter through 
     a red filter than through a blue filter on its western wall. 
     He checked Aristarchus in two telecopes and obtained the same 
     result. The Cameron 2006 catalog ID=419 and the weight=4. The 
     ALPO/BAA weight=3. 


2026-Feb-28 UT 07:36-09:22 Ill=89% Moon observed by Corralitos on 1967-4-21

     Moon 1967 Apr 21 UTC 02:30-09:30 Observed by Dunlap et al (Corralitos 
     Observatory, Organ PAss, NM, USA, 24" reflector + moonblink) "UV excess 
     relative to red & visual images. Greatest (30%) at subsolar pt. nr. 
     limb, grading down to 0% at term. Seen Apr 22 also with a gradient of 
     10% at term. to 25-30% at subsolar pt. (137 deg long). Filters well 
     balanced. Neg. (normal) on Apr. 20 & 23rd. Bandpass 3700-4900A on image 
     enhancement & filter equip. (coincided with Lyrid meteor shower. They 
     had seen this phenom. many times since. NASA catalog weight=5 (very 
     high). NASA catalog ID #1039.


2026-Feb-28 UT 08:20-09:23 Ill=89% Gassendi observed by Unknown_English_Observer on 1977-4-29

     On 1977 Apr 29 at UT21:40-23:20 an unknown UK observer reported a TLP 
     in Gassendi crater. The following are reports by observers attempting 
     to confirm activity: J.W. Napper (Didcot, UK, 30cm reflector, x287, 
     Wratten 25 and 44a, conditions clear 5+) received a telephone alert 
     call at 22:00 but the sky was cloudy until 22:30. An initial look 
     revealed nothing unusual, then at 22:54 he observed a colour blink just 
     inside the north wall, appearing bright in red and normal in blue or 
     white light. No loss of detail seen and the effect lasted only 2 
     minutes. A sketch was made. However the observer stresses that the very 
     bad seeing casts some doubt on this observation. L. Fitton observed 
     using a 8.5" reflector, with Moon blink device at x200, seeing was I-
     II. All areas negative, including Gassindi from 21:40-21:55 and again 
     22;00-22:25 and finally 22:50-23:30 negative. Mike Brown (Huntington, 
     York, UK, 30cm reflector, x220 and x350, seeing 3-4/5, and transparency 
     5/5) - observed from 22:00-23:25UT no colour seen, nor obsecuration, 
     all filters negative, despite seeing a lot of fine setail inside this 
     crater.


2026-Feb-28 UT 09:04-10:49 Ill=89% Proclus observed by Darling_D on 1987-10-4

     On 1987 Oct 04 at UT 02:20 D. Darling (Sun Praire, WI, USA, 
     12.5" reflector, x170, S=8, VG, T=5) obtained the brightest 
     measurement he had ever recorded on the northern rim of 
     Proclus. Brightness 9 and adjacent plain was of brightness 
     6.5. The Cameron 2006 catalog ID=308 and the weight=3. The 
     ALPO/BAA weight=2. 


2026-Feb-28 UT 09:25-10:28 Ill=89% Aristarchus observed by Zeller_P on 2013-4-22

     On 2013 Apr 22 UT 01:39-02:37 P. Zeller (Indianapollis, USA, 
     10" f/4 reflector, x200, seeing 6, Transparency 3 - scattered 
     cirrus) observed visually (depicted in sketch) the two closely 
     spaced NW wall dark bands) to have a rusty-red hue. The colour 
     of these bands did not change over the period of the observing 
     session. Images were taken, but resolution and image S/N is 
     not sufficient to resolve separate bands here, or to detect 
     colour. The ALPO/BAA weight=1.


2026-Feb-28 UT 10:03-11:02 Ill=89% Gassendi observed by Sartory on 1966-5-1

     Gassendi 1966 May 01 UT 19:30-00:21 Observed by Sartory (UK, 
     8.5" reflector, x500, S=G), Moore, Moseley (Northern Ireland, 
     12.5" reflector x350, S=E) and by Corralitos Observatory 
     (Organ Pass, NM, USA, 24" reflector + moon blink) "Eng. 
     moonblink & obscuration, also vis. confirm (Moore & Moseley 
     alerted by Sartory. Corralitos MB did not confirm. - but they 
     may not have been observing at the ame time?)." NASA catalog 
     weight=5. NASA catalog ID #932. ALPO/BAA weight=4.


2026-Feb-28 UT 10:41-11:23 Ill=89% Plato observed by North_G on 1981-8-11

     On 1981 Aug 11 at UT21:05-21:36 G. North (England, seeing=poor) 
     detected, in green light, a darkening on the floor of Plato. This 
     effect was not seen elsewhere. J-H Robinson (Teighmouth, Devon, UK) 
     detected on the SSE rim (inner and beyond) a triangle that appeared 
     hazy in a wide range of filters at 21:05UT. However at 21:36UT it was 
     only hazy in green and blue light. No similar effect was seen 
     elsewhere. The Cameron 2006 catalog ID=150 and weight=5. The ALPO/BAA 
     weight=3.


2026-Feb-28 UT 12:17-13:29 Ill=89% Herodotus observed by Martini_A on 2017-2-8

     On 2017 Feb 08 UT 01:45 A.Martini Jr (10" Schmidt-Cassegrain 
     with ASI 120 MC camera +IR filter, Gain 40, Gamma 36, 
     exposure 0.003 sec) saw on a computer monitor screen a flash 
     to far to the west of Herodotus and Aristarchus at the 
     location 54.53W, 23.5N. It had a duration of 0.5 sec and on a 
     brightness scale of 0 = night side of the Moon to 10 = 
     Aristarchus, ranked 7. Unfortunately they were not recording 
     at the time. As there was no confirmation observation and it 
     could be a cosmic ray air shower detection, the ALPO/BAA 
     weight=1


2026-Feb-28 UT 12:28-13:28 Ill=89% Aristarchus observed by Paterson on 1966-5-1

     Aristarchus 1966 May 01 UT 21:55-22:45 Observed by Paterson, 
     Brown, Sartory, Ringsdore (England, 12" reflector x252 for the 
     former and 8.5"? reflector for the latter) "Eng. moon blink 
     system detected red spots with vis. by all but Ringsdore. Brown 
     saw intense white spot NW of crater wall" NASA catalog weight=5. 
     NASA catalog ID 933. ALPO/BAA weight=4.


2026-Feb-28 UT 13:38-14:29 Ill=90% Mons_Pico observed by Rawstron on 1934-2-25

     In 1934 Feb 25 at UT 18:30 Rawstron (USA?, 4" refractor, x250, S=6/12) 
     observed in Pico B: "A large patch of haze appeared & drifted off 
     across the mare in same direction as haze from Pico (white patch). It 
     was obs. on 20 other occasions. Drawing". The Cameron 1978 catalog ID=
     410 and weight=3. The ALPO/BAA weight=2.


2026-Feb-28 UT 14:11-15:11 Ill=90% Gassendi observed by Albert_J on 2023-5-2

     Gassendi. 2023 May 02 UT 01:35-02:23. J. Albert (Lake Worth, 
     FL, USA - ALPO. 8” SCT via a 9mm ortho eyepiece. Transparency 
     magnitude 3 and seeing was 7/10) checked the crater without 
     filters as well as comparing with W25 red and W44A blue 
     filters using 226x. He saw no color on the SW part of the 
     crater floor or on the NW wall.  Using the filters, however, 
     he did note that the high peak on the S wall was brighter in 
     blue than red.  He tried this filter blink a number of times 
     because he had never seen this before in Gassendi, but the 
     result was the same each time. A colour image was taken 
     earlier at 01:21UT but shows not colour on S wall as it was 
     saturated. ALPO/BAA weight=2.