Lunar Observing Schedule for: Russia - Veliky_Novgorod



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


2026-Apr-02 UT 00:29-00:42 Ill=100% Copernicus

     ALPO Request: Can you see a darkening on the northen floor of 
     this crater? All visual reports, sketches or color images should 
     be emailed to: 
     t o n y . c o o k @ a l p o - a s t r o n o m y . o r g


2026-Apr-20 UT 18:35-20:02 Ill=15% Yerkes

     Yerkes: a "Woodpecker" shaped shadow - 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. This particular Clair-Obscur effect was first
     reported by KC Pau.


2026-Apr-20 UT 18:06-19:21 Ill=15% 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


2026-Apr-21 UT 18:08-21:51 Ill=26% Earthshine: Lyrids: ZHR=15 (vel=47km/s) & Pi Puppids: ZHR=var (vel=18km/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


2026-Apr-22 UT 18:11-21:58 Ill=36% Earthshine: Lyrids: ZHR=15 (vel=47km/s) & Pi Puppids: ZHR=var (vel=18km/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


2026-Apr-23 UT 18:25-19:21 Ill=46% Apollo_11

     Apollo 11: This is what Mare Tranquillitatis would have looked 
     like on the night that Apollo 11's Neil Armstrong made the first 
     footprint on the lunar surface. Aim for the area north of Moltke 
     crater. 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: 


2026-Apr-23 UT 18:25-18:45 Ill=46% Torricelli

     ALPO Request: On 2011 Dec 31 Raffaello Braga found the north rim 
     or Torricelli to be very bright at the start of the observing 
     session but dimmed considerably later. He was not sure on the 
     normal appearance of this crater, hence why it is really 
     imortant to establish this by re-observing under similar 
     illumination. Minimum telescope aperture required: 3", and try 
     to use a refractor if possible. Please send any high resolution 
     images, detailed scetches, or  visual descriptions to: 
     a t c @ a b e r . a c. u k .


2026-Apr-23 UT 18:14-21:54 Ill=48% Earthshine: Lyrids: ZHR=15 (vel=47km/s) & Pi Puppids: ZHR=var (vel=18km/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


2026-Apr-24 UT 17:22-18:16 Ill=57% Albategnius

     Face of Albategnius: you can see the profile of a face in a shadow 
     from the eastern edge of this crater - 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.


2026-Apr-24 UT 17:22-22:12 Ill=57% Montes_Caucasus

     Monte Caucasus: "shadow face" silhouette Clair-Obscur effect. 
     Clair-Obscur effects have no scientific importance 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 useless to observe. However, if 
     you want to be thrilled, or obtain an image to impress someone 
     then give them a go. This effect on the southern end of Montes 
     Caucuses looks like the side silhouette of a cartoon human face. 
     We are still slightly undertain about the precise colongitude 
     range, so if you do not see the face, try again later. 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.
     Note that we have some uncertainty in the colongitude range 
     - so if you don't see it, please tells us the date and UT so 
     we can make some improvements in the predictions.


2026-Apr-25 UT 18:09-19:51 Ill=68% 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.


2026-Apr-28 UT 22:55-23:09 Ill=93% Alphonsus

     BAA Request: Monitor the central peak for brightness changes. Do 
     they change with atmospheric seeing conditions? Any brightness 
     measurements or image sequences made should be emailed to: 
     a t c @ a b e r . a c . u k