Difference between revisions of "February 28, 2010"

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<em>image by [mailto:raffaele.barzacchi@fastwebnet.it" rel="nofollow Raffaele Barzacchi], Italy</em><br />
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<em>image by [mailto:raffaele.barzacchi@fastwebnet.it Raffaele Barzacchi], Italy</em><br />
 
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We mostly observe areas of the Moon that are illuminated. but sometimes the lack of light creates patterns that are evocative and informative. Here the first rays of sunrise reflect brightly from the upper walls of Plato, and faintly from the exterior eastern rim. This emphasizes that the inner wall is steep and relatively smooth, accounting for the brightness, whereas the outer rim has a low slope covered with boulders and rubble.<br />
 
We mostly observe areas of the Moon that are illuminated. but sometimes the lack of light creates patterns that are evocative and informative. Here the first rays of sunrise reflect brightly from the upper walls of Plato, and faintly from the exterior eastern rim. This emphasizes that the inner wall is steep and relatively smooth, accounting for the brightness, whereas the outer rim has a low slope covered with boulders and rubble.<br />
 
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<em>[mailto:tychocrater@yahoo.com" rel="nofollow Chuck Wood]<br />
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<em>[mailto:tychocrater@yahoo.com Chuck Wood]<br />
 
I leave for the 41st Lunar and Planetary Science Conference today and will try to post some results from the meeting.</em><br />
 
I leave for the 41st Lunar and Planetary Science Conference today and will try to post some results from the meeting.</em><br />
 
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<div>You can support LPOD when you buy any book from Amazon thru [http://www.lpod.org/?page_id=591" rel="nofollow LPOD!]<br />
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<div>You can support LPOD when you buy any book from Amazon thru [http://www.lpod.org/?page_id=591 LPOD!]<br />
 
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Revision as of 17:16, 11 January 2015

Hole Full of Shadow

LPOD-Feb28-10.jpg
image by Raffaele Barzacchi, Italy

We mostly observe areas of the Moon that are illuminated. but sometimes the lack of light creates patterns that are evocative and informative. Here the first rays of sunrise reflect brightly from the upper walls of Plato, and faintly from the exterior eastern rim. This emphasizes that the inner wall is steep and relatively smooth, accounting for the brightness, whereas the outer rim has a low slope covered with boulders and rubble.

Chuck Wood
I leave for the 41st Lunar and Planetary Science Conference today and will try to post some results from the meeting.


Technical Details
Jan 23, 18:38 UT. C14 XLT, f/20 + R+IR filter.

Related Links
Rükl plate 3


You can support LPOD when you buy any book from Amazon thru LPOD!

COMMENTS?

Register, and click on the Discussion tab at the top of the page.