Lunar Observing Schedule for: Greenland - Nuuk



Produced by the Department of Physics at Aberystwyth University, UK
Ill is percentage illumination of the Moon


2025-Nov-02 UT 00:32-01:29 Ill=83% Aristarchus

     ALPO Request: On 2013 Apr 22 Paul Zellor noticed that the two 
     closely spaced NW dark bands in Aristarchus had some (non-blue) 
     color to them. Can we confirm his observation of natural colour 
     here? Ideally you should be using a telescope of 10" aperture, or 
     larger. Please send any high resolution color images, detailed 
     sketches, or visual descriptions to: a t c @ a b e r . a c. u k .


2025-Nov-04 UT 05:59-07:11 Ill=97% Riccioli

     ALPO Request: Either visually observe or obtain a colour image 
     of this crater shortly after it has emerged from the sunrise 
     terminator. Minimum sized aperture scope needed: 5". Any 
     observations  or images should be emailed to: 
     a t c @ a b e r . a c . u k


2025-Nov-07 UT 01:12-01:47 Ill=96% Mons_Vinogradov

     ALPO Request: Please supply images, or sketches, of this area, 
     especially covering the area to the east. Any size scope can be 
     used for this study. All observations should be emailed to: 
     a t c @ a b e r . a c. u k 


2025-Nov-08 UT 04:52-06:14 Ill=90% Torricelli_B

     BAA Request: Sketches or images needed of Toricelli B - of 
     sufficient resolution to reveal shadow. All observations, 
     including sketches or images shouild be emailed to: 
     a t c @ a b e r . a c. u k .


2025-Nov-08 UT 23:04-08:31 Ill=83% Cyrillus

     BAA Request: Cyrillus. There is a small white craterlet just 
     north of the three central peaks. We are interested to receive 
     high resolution images of this in order to find out at what 
     selenographic colongitude, in the lunar evening, that it loses 
     it's white spot appearence. Please use scopes largher than 6 
     inches in diameter. 
     Please email these to: a t c @ a b e r . a c . u k


2025-Nov-10 UT 03:05-04:05 Ill=72% Jansen

     BAA Request: On 2013 Aug 26 Peter Grego observed a dark patch 
     just east of Jansen D. He had not seen this before, therefore it 
     is important to repeat this observation under simuilar 
     illumination conditions. It maybe a buried crater? Ideally 
     suited to scopes of aperture 8" or larger. Please send 
     any high resolution images, detailed scetches, or 
     visual descriptions to: a t c @ a b e r . a c. u k .


2025-Nov-12 UT 04:23-10:50 Ill=48% Earthshine: Northern Taurids, ZHR=5 vel=29km/s

     These can only be observed using low-light level cameras running at 25 frames per sec,
     or faster, and capable of recording 9th or 10th magnitude stars in real time.
     Dates/UTs of observing runs, or detections of impacts, should be emailed to:
     ALPO - email: c u d n i k @ s b c g l o b a l . n e t
     BAA - email: a t c @ a b e r . a c . u k
     UAI - email: a m . 5 4 8 5 2 @ g m a i l . c o m


2025-Nov-13 UT 09:25-11:01 Ill=38% Tycho

     Tycho: "V-shaped pearl neckless" effect - this is a Clair-Obscur effect. 
     Clair-Obscur have no scientific importance and are just tricks of the 
     light that make us think we see something like a letter of the alphabet 
     or a shape or face. Clair-Obscur effects are scientifically pointless 
     to observe. However, if you want to be thrilled, or obtain an image to 
     impress someone then give them a go. This effect was first spotted by 
     David Darling in 1992 Aug 21 and was considered to be a possible TLP 
     until the effect was seen repeated at similar illumination. If you do 
     observe, or image this, by all means send your observation into ALPO 
     or the BAA, but we probably won't publish, but will nevertheless 
     retain in our archives, just in case features 
     elsewhere in the image are of interest to future researchers.


2025-Nov-13 UT 05:59-10:53 Ill=37% Earthshine: sporadic meteors

     These can only be observed using low-light level cameras running at 25 frames per sec,
     or faster, and capable of recording 9th or 10th magnitude stars in real time.
     Dates/UTs of observing runs, or detections of impacts, should be emailed to:
     ALPO - email: c u d n i k @ s b c g l o b a l . n e t
     BAA - email: a t c @ a b e r . a c . u k
     UAI - email: a m . 5 4 8 5 2 @ g m a i l . c o m


2025-Nov-14 UT 06:17-10:55 Ill=28% Earthshine: Leonids: ZHR=15 vel=71km/s

     These can only be observed using low-light level cameras running at 25 frames per sec,
     or faster, and capable of recording 9th or 10th magnitude stars in real time.
     Dates/UTs of observing runs, or detections of impacts, should be emailed to:
     ALPO - email: c u d n i k @ s b c g l o b a l . n e t
     BAA - email: a t c @ a b e r . a c . u k
     UAI - email: a m . 5 4 8 5 2 @ g m a i l . c o m


2025-Nov-15 UT 07:16-10:58 Ill=20% Earthshine: Leonids: ZHR=15 vel=71km/s

     These can only be observed using low-light level cameras running at 25 frames per sec,
     or faster, and capable of recording 9th or 10th magnitude stars in real time.
     Dates/UTs of observing runs, or detections of impacts, should be emailed to:
     ALPO - email: c u d n i k @ s b c g l o b a l . n e t
     BAA - email: a t c @ a b e r . a c . u k
     UAI - email: a m . 5 4 8 5 2 @ g m a i l . c o m


2025-Nov-16 UT 08:21-11:01 Ill=12% Earthshine: Leonids: ZHR=15 vel=71km/s

     These can only be observed using low-light level cameras running at 25 frames per sec,
     or faster, and capable of recording 9th or 10th magnitude stars in real time.
     Dates/UTs of observing runs, or detections of impacts, should be emailed to:
     ALPO - email: c u d n i k @ s b c g l o b a l . n e t
     BAA - email: a t c @ a b e r . a c . u k
     UAI - email: a m . 5 4 8 5 2 @ g m a i l . c o m


2025-Nov-17 UT 09:33-11:03 Ill=7% Earthshine: Leonids: ZHR=15 vel=71km/s

     These can only be observed using low-light level cameras running at 25 frames per sec,
     or faster, and capable of recording 9th or 10th magnitude stars in real time.
     Dates/UTs of observing runs, or detections of impacts, should be emailed to:
     ALPO - email: c u d n i k @ s b c g l o b a l . n e t
     BAA - email: a t c @ a b e r . a c . u k
     UAI - email: a m . 5 4 8 5 2 @ g m a i l . c o m


2025-Nov-18 UT 10:57-11:06 Ill=3% Earthshine: Leonids: ZHR=15 vel=71km/s

     These can only be observed using low-light level cameras running at 25 frames per sec,
     or faster, and capable of recording 9th or 10th magnitude stars in real time.
     Dates/UTs of observing runs, or detections of impacts, should be emailed to:
     ALPO - email: c u d n i k @ s b c g l o b a l . n e t
     BAA - email: a t c @ a b e r . a c . u k
     UAI - email: a m . 5 4 8 5 2 @ g m a i l . c o m


2025-Nov-28 UT 20:30-22:27 Ill=56% Clavius

     Eyes of Clavius: you can see this crater with two eyes, Clavius C and 
     Clavius D - this is a Clair-Obscur effect. Clair-Obscur have no 
     scientific importance and are just tricks of the light that make 
     us think we see something like a letter of the alphabet 
     or a shape or face. Clair-Obscur effects are scientifically pointless 
     to observe. However, if you want to be thrilled, or obtain an image to 
     impress someone then give them a go. If you do observe, or image this, 
     by all means send your observation into ALPO or the BAA, but we 
     probably won't publish, but will nevertheless retain in our archives, 
     just in case features elsewhere in the image are of interest to 
     future researchers.


2025-Nov-28 UT 20:36-22:31 Ill=56% Eratosthenes

     ALPO Request: This request comes about because of two 
     observations. Firstly on 2009 Nov 25 Paul Abel and others 
     detected some colour on the inner west illumntated slopes of 
     this crater. No similar colour existed elsewhere. On 2012 Aug 
     25 Charles Galdies imaged this crater and detected a similar 
     colour, approximately in the same location, though he also 
     imaged colour elsewhere. It is important to replicate this 
     observation to see if it was natural surface colour, 
     atmospheric spectral dispersion, or some effect in the camera 
     that Charles was using, namely a Philips SPC 900NC camera. 
     The minimum sized telescope to be used would ideally a 8" 
     reflector. Please send any high resolution images, detailed 
     sketches, or visual descriptions to: 
     a t c @ a b e r . a c. u k .


2025-Nov-29 UT 22:19-23:18 Ill=67% Apollo_14

     Apollo 14: This is what the lunar surface would have looked like 
     when Apollo 14 touched down on the Moon. Aim for the area 
     north of Fra Mauro. The illumination and the shadows are
     exactly the same. There is no scientific value in imaging 
     this, but from the nostalgic point of view it might be interesting 
     to observe. Feel free to send your observation in to the BAA or 
     ALPO and we will put it in our archives, but as we have 
     a lot of these images already, we may not publish it, unless it is 
     exceptionally high in resolution. Minimum diameter scope to use 
     would be 20cm, but larger apertures are preferred: 


2025-Nov-29 UT 23:40-00:38 Ill=68% Apollo_12

     Apollo 12: This is what the lunar surface would have looked like 
     when Apollo 12 touched down on the Moon. Aim for the area 
     SW of Lansberg. The illumination and the shadows are
     exactly the same. There is no scientific value in imaging 
     this, but from the nostalgic point of view it might be interesting 
     to observe. Feel free to send your observation in to the BAA or 
     ALPO and we will put it in our archives, but as we have 
     a lot of these images already, we may not publish it, unless it is 
     exceptionally high in resolution. Minimum diameter scope to use 
     would be 20cm, but larger apertures are preferred: 


2025-Nov-30 UT 02:07-02:30 Ill=69% Montes_Jura

     "Jewelled Handle": in Montes Jura - this is a Clair-Obscur effect. Its
     an illuminated arc. Clair-Obscur have no scientific importance and are 
     just tricks of the light that make us think we see something like a 
     letter of the alphabet or a shape or face. Clair-Obscur effects are 
     scientifically pointless to observe. However, if you want to be 
     thrilled, or obtain an image to impress someone then give them a go. 
     If you do observe, or image this, by all means send your observation 
     into ALPO or the BAA, but we probably won't publish, but will 
     nevertheless retain in our archives, just in case features elsewhere 
     in the image are of interest to future researchers.