Lunar Observing Schedule for: Iceland - Reykjavik



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


2024-Jul-28 UT 02:17-02:42 Ill=50% Earthshine: Jul Zeta Draconids + S.Delta Aquarids + Alpha Capricornids

     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-Jul-29 UT 02:24-02:49 Ill=39% Earthshine: Jul Zeta Draconids + S.Delta Aquarids + Alpha Capricornids

     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-Jul-29 UT 02:53-04:37 Ill=39% Plato

     BAA Request: Its around this Co-Longitude that some observers 
     have reported seeing an Ashen Light effect on the shadowed floor 
     of Plato, caused by scattered light off of an illuminated peak 
     on the rim. Please have a go either visually, or with long 
     exposure time lapse imagery to see if you can pick up the 
     development of this weak illumination effect on the floor. 
     Please send any sketches or images to: 
     a t c @ a b e r . a c. u k .


2024-Jul-30 UT 02:43-02:56 Ill=28% Earthshine: Jul Zeta Draconids + S.Delta Aquarids + Alpha Capricornids

     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