Lunar Observing Schedule for: Russia - Novokuznetsk



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


2024-Mar-11 UT 12:37-15:06 Ill=2% Moon

     BAA Request: Please try to image the Moon as a very thin 
     crescent, tryimg to detect Earthshine. A good telephoto lens 
     will do on a DSLR, or a camera on a small scope. We are 
     attempting to monitor the brightness of the edge of the 
     earthshine limb in order to follow up a project suggested by 
     Dr Martin Hoffmann at the 2017 EPSC Conference in Riga, 
     Latvia. This is quite a challenging project due to the sky 
     brightness and the low altitude of the Moon. Please do not 
     attempt if the Sun is still above the horizon. Do not bother 
     observing if the sky conditions are hazy. Any images 
     should be emailed to: 
     a t c @ a b e r . a c . u k


2024-Mar-13 UT 12:21-13:29 Ill=14% Picard

     BAA Request: On 2013 Feb 17 UAI observer: Giuseppe Macalli 
     observed visually an orange cloud form just to the west of 
     Picard crater, and then dissappear. The effect lasted about 1 
     minute. Obviously we are not likely to see whatever this was 
     (?) again under similar illumination, but just for the record 
     it would be useful to have a high resolution monochrome or 
     colour image of this area, at the requested observing 
     time.N.B. an image in the 2018 Jun LSC suggests that the date 
     given of 2013 Feb 17 may have been Feb 18? Please send any 
     high resolution images to: a t c @ a b e r . a c. u k .


2024-Mar-13 UT 12:41-13:47 Ill=14% Picard

     ALPO Request: Compare the crater in red and blue light - if 
     possible use Wratten 25 and Wratten 38A filters. Please 
     use a telescope of aperture 6 or larger (refractor if 
     possible) and at appromimately x250. Any visual descriptions, 
     sketches, or colour 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


2024-Mar-13 UT 13:15-14:47 Ill=14% 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 morning, that it 
     starts to show 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


2024-Mar-13 UT 12:48-14:13 Ill=14% 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


2024-Mar-14 UT 12:50-15:37 Ill=24% 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


2024-Mar-15 UT 12:51-16:55 Ill=34% 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


2024-Mar-16 UT 12:53-18:05 Ill=45% 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


2024-Mar-17 UT 12:55-16:33 Ill=55% 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


2024-Mar-17 UT 18:47-19:41 Ill=56% Eudoxus

     BAA Request: Eudoxus - please try to image the interior of 
     this crater. We are trying to detect bright spots and a linear 
     features within the shadow of the east wall at sunrise. Nigel 
     Longshaw (BAA) suspects that this might explain Trouvelot's 
     obsevation in 1877 of a luminous rope-like feature.
     Please send any images to: a t c @ a b e r . a c. u k .


2024-Mar-17 UT 18:58-19:41 Ill=56% Eudoxus

     BAA Request: Eudoxus - please try to image or skecth the 
     crater. This is to try to explain a line of light effect seen 
     inside this crater by French astronomer Trouvelot back in 
     Victorian times. The BAAs Nigel Longshaw says that this may be 
     seen between colongitudes of 0.3 to 1.2 degrees. Please send 
     any images or sketches to: a t c @ a b e r . a c. u k .


2024-Mar-18 UT 14:53-15:27 Ill=64% Plato

     BAA Request: It has been noticed that a bright carterlet can 
     appear very suddenly on the floor of Plato in between needle 
     like shadows, during local lunar sunrise. This happens in the 
     space of just a minute or so, and can look really quite dramatic.
     This effect was first spotted by Brian Halls on 2014 Oct 31 
     Please send any high resolution images, detailed scetches, or 
     visual descriptions to: a t c @ a b e r . a c. u k .


2024-Mar-18 UT 18:49-19:24 Ill=66% Tycho

     BAA Request: How early can you see the central peak of this 
     crater illuminated by scattered light off the crater's west 
     illuminated rim? High resolution and/or long exposures needed 
     to capture detail inside the floor shadow. All images should 
     be sent to me on the email adrress below, whether or not you 
     were successful in capturing the central peak: 
     a t c @ a b e r . a c. u k 


2024-Mar-19 UT 13:32-14:31 Ill=73% Copernicus

     BAA Request: On 2012 Sep 24 E. Horner noticed a very strong red 
     colour around part of the sunlit inner rim of Copernicus, 
     sometimes a 1/4 and sometimes 1/2 around the interior. Quite 
     likely this was some form of atmospheric spectral dispersion - 
     though the observer checked for similar effects on other craters 
     but saw none. But to be sure we would like to obtain some colour 
     images or visual observations of this crater. The minimum sized 
     telescope to be used would ideally a 6" reflector. Low elevation 
     angles for the Moon are ideal as we want to try to replicate 
     this effect if it is indeed due to atmospheric spectral 
     dispersion. Please send any high resolution images, detailed 
     sketches, or visual descriptions 
     to: a t c @ a b e r . a c. u k .


2024-Mar-19 UT 13:47-14:46 Ill=73% Apollo_17

     BAA Request: Take high resolution images of the area south of 
     Littrow to capture a view of what the lunar surface would 
     have looked like from Earth at the moment Apollo 17 lifted off 
     of the Moon. Minimum diameter scope 20cm, larger 
     apertures preferred: 
     a t c @ a b e r . a c . u k


2024-Mar-21 UT 16:56-17:53 Ill=89% 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 .


2024-Mar-26 UT 17:27-18:02 Ill=98% 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 


2024-Mar-27 UT 19:42-20:41 Ill=94% Cleomedes

     BAA Request: In 1991 Dec 23 Bob Mizon (BAA) sketched the 
     crater Cleomedes and Mare Cisrium. In the floor of the shadow 
     filled Cleomedes was an dusky oval area - presumably the last 
     rays of the Sun reaching the floor. We would like yuo to 
     either sketch, or image, over time, how the shape of this oval 
     area changes, and eventually vanishes. How late in terms of 
     colongitude can it still be seen? Is there any hint of colour 
     present? Telescopes of aperture 6 inche or larger should be 
     used. Please send any observation 
     you make to: 
     a t c @ a b e r . a c . u k


2024-Mar-27 UT 21:05-22:05 Ill=94% 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 .


2024-Mar-28 UT 20:00-21:16 Ill=89% 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