Difference between revisions of "January 13, 2010"

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<em>image by [mailto:paolo@lazzarotti-optics.com" rel="nofollow Paolo R. Lazzarotti], Massa, Italy</em><br />
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<em>image by [mailto:paolo@lazzarotti-optics.com Paolo R. Lazzarotti], Massa, Italy</em><br />
 
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Humboldtianum is another relatively dry basin. Like Nectaris and Orientale much of its lava is concentrated in a smallish pond on the middle of the floor. Mare Humboldtianum is so thin that at least one sizeable crater on its floor almost completely submerged. Additional lava did seep out in the moat between the main two rings - it is visible in low spots, especially on the side of the moat visible here. As is true of most maria away from the [http://www.lpod.org/?m=20070219" rel="nofollow Procellarum KREEP Terrain] there are few or no volcanic features such as sinuous rilles. A small darker area of the southern edge of the mare may be pyroclastics, and a Lunar Orbiter [http://www.lpod.org/coppermine/displayimage.php?album=28&amp;pos=59" rel="nofollow mosaic] shows a steep-sided mound or perhaps a dome at about the same place.<br />
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Humboldtianum is another relatively dry basin. Like Nectaris and Orientale much of its lava is concentrated in a smallish pond on the middle of the floor. Mare Humboldtianum is so thin that at least one sizeable crater on its floor almost completely submerged. Additional lava did seep out in the moat between the main two rings - it is visible in low spots, especially on the side of the moat visible here. As is true of most maria away from the [http://www.lpod.org/?m=20070219 Procellarum KREEP Terrain] there are few or no volcanic features such as sinuous rilles. A small darker area of the southern edge of the mare may be pyroclastics, and a Lunar Orbiter [http://www.lpod.org/coppermine/displayimage.php?album=28&amp;pos=59 mosaic] shows a steep-sided mound or perhaps a dome at about the same place.<br />
 
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<em>[mailto:tychocrater@yahoo.com" rel="nofollow Chuck Wood]</em><br />
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<em>[mailto:tychocrater@yahoo.com Chuck Wood]</em><br />
 
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<strong>Related Links</strong><br />
 
<strong>Related Links</strong><br />
[http://www.lazzarotti-hires.com/2010/01/librazione-estrema.html?lan=english" rel="nofollow Full Size image]<br />
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[http://www.lazzarotti-hires.com/2010/01/librazione-estrema.html?lan=english Full Size image]<br />
 
Rükl plate [http://the-moon.wikispaces.com/R%C3%BCkl+7 7]<br />
 
Rükl plate [http://the-moon.wikispaces.com/R%C3%BCkl+7 7]<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 17:14, 11 January 2015

Almost Dry

LPOD-Jan13-10.jpg
image by Paolo R. Lazzarotti, Massa, Italy

Humboldtianum is another relatively dry basin. Like Nectaris and Orientale much of its lava is concentrated in a smallish pond on the middle of the floor. Mare Humboldtianum is so thin that at least one sizeable crater on its floor almost completely submerged. Additional lava did seep out in the moat between the main two rings - it is visible in low spots, especially on the side of the moat visible here. As is true of most maria away from the Procellarum KREEP Terrain there are few or no volcanic features such as sinuous rilles. A small darker area of the southern edge of the mare may be pyroclastics, and a Lunar Orbiter mosaic shows a steep-sided mound or perhaps a dome at about the same place.

Chuck Wood

Related Links
Full Size image
Rükl plate 7


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

COMMENTS?

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