The French expression that "the more things change, the more they stay the same" is perhaps best applicable for the moon. The observation of
the moon on a daily basis will readily identify its constantly changing behaviour as it evolves from a very thin crescent at the start of a
new lunation to a noticeable crescent, first quarter and eventually a full moon as part of its waxing repertoire. This scenario will then
continue but in reverse order, for the waning moon will now proceed in an orderly manner from full to a very thin crescent in a similar gradual
but organized manner. Of course, this changing behaviour will repeat itself incessantly in precisely the same sequence and rate ad infinitum
approximately every 29 days.
Note: The image of the full moon below was taken at the minimum perigee for 2008 as well as for the period
1993-2016.
Body: Moon Mass: 0.0123 x Earth Mean Eq Diameter: 0.2719 x Earth Distance: 356,566 km Sidereal Rev: 27d 07h 43m 11s Age: 14d 23h 44m Phase: 99.8% Diameter: 34.10' Magnitude: -12.6 Light Time: 0h 0m 1.2s Rukl: N/A |
|
Date: Dec 12, 2008 23:33:18 UT+2 Location: Athens, Greece Equipment: AP 160 f/7.5 StarFire EDF AP 1200GTO GEM Canon EOS 350D Exposure(s): 1 x 1/250 sec ISO 100 RAW image format 3456x2304 image size Manual Mode Software: Digital Photo Pro V2.1.1.4 Photoshop CS2 Processing: RAW to TIFF (16-bit) Conv Desaturation Cropping Brightness/Contrast Levels Unsharp Masking Resampling JPG Compression |