Difference between revisions of "January 14, 2004"

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<p class="story" align="center"><b>First and Last</b></p>
 
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<p class"story"> <b>Tomorrow's LPOD:</b> Gassendi Compared</p>
 
<p class"story"> <b>Tomorrow's LPOD:</b> Gassendi Compared</p>
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===COMMENTS?===  
 
===COMMENTS?===  
 
Click on this icon [[image:PostIcon.jpg]] at the upper right to post a comment.
 
Click on this icon [[image:PostIcon.jpg]] at the upper right to post a comment.

Revision as of 18:07, 4 January 2015

First and Last

LPOD-2004-01-14.jpeg
Image Credit:

NSSDC and USGS

First and Last

In 1959 the Soviet probe Luna 3 swept behind the Moon and took the first photograph (left) of the lunar farside (in fact, the first picture EVER of any extraterrestrial planetary body from space). And the most recent image of the lunar farside is this (right) mosaic of Clementine frames acquired in 1994. Other than some Apollo and Lunar Orbiter photos, the farside, almost as alien as a tenth planet, remains little imaged and little studied. The extensive areas of brightness across the Luna picture demonstrate that the farside has far less maria (dark) than the lunar nearside. The patches of darkness at the lower left of the the Luna image are the mostly frontside maria Crisium, Marginis, Smythii and Fecunditatis - none of which show up on the Clementine mosaic. The isolated dark patch in the upper right of the Luna view is Mare Moscoviense - also seen left of center on the right image. The small black spot with a white dot in the center is Tsiolkovskiy. And finally, the largest, mottled dark area bottom center-right on the Clementine image is the South Pole-Aitken Basin.

Related Links:
Luna 3
Clementine

Tomorrow's LPOD: Gassendi Compared


Author & Editor:
Charles A. Wood

Technical Consultant:
Anthony Ayiomamitis

A service of:
ObservingTheSky.Org

Visit these other PODs:
Astronomy | Mars | Earth

 


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Click on this icon File:PostIcon.jpg at the upper right to post a comment.