|   | 
Credit: Rich    
Richins    
    
    
Explanation:
An analemma    
is that figure-8 curve you get when you mark    
the position of the Sun at the same    
time each day for one year.    
    
But the trick to imaging    
an analemma of the Moon is to understand    
that on average the    
Moon    
returns to the same position in the sky    
about 51 minutes later each day.    
    
So, if you    
photograph    
the Moon 51 minutes later on successive days, over    
one lunation or    
lunar month it will trace out an    
analemma-like curve as the actual position of the Moon    
wanders compared to the average --    
due to the Moon's tilted and elliptical orbit.    
    
For this excellent demonstration of the lunar analemma, astronomer    
Rich Richins chose the lunar month containing this year's    
northern hemisphere    
summer    
solstice.    
    
The southernmost    
Full Moon rises at the lower right    
above the Organ Mountains in southern New Mexico, USA,    
with the New Moon phase at the upper left.    
    
The multiple exposure image required some digital    
manipulation, particularly to include thin crescent phases in    
daytime    
skies.    
    
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NASA Web Site Statements, Warnings, and Disclaimers
NASA Official: Jay Norris. Specific rights apply.
A service of: LHEA at NASA / GSFC
& Michigan Tech. U.
Based on Astronomy Picture
Of the Day
Publications with keywords: analemma - Moon - lunation - phase - full moon - new moon
Publications with words: analemma - Moon - lunation - phase - full moon - new moon
See also:
