Difference between revisions of "January 13, 2010"
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=Almost Dry= | =Almost Dry= | ||
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| − | <em>image by [mailto:paolo@lazzarotti-optics.com Paolo R. Lazzarotti], Massa, Italy</em><br /> | + | <em>image by [mailto:paolo@lazzarotti-optics.com" rel="nofollow 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 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&pos=59 mosaic] shows a steep-sided mound or perhaps a dome at about the same place.<br /> | + | 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&pos=59" rel="nofollow 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 Chuck Wood]</em><br /> | + | <em>[mailto:tychocrater@yahoo.com" rel="nofollow 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 Full Size image]<br /> | + | [http://www.lazzarotti-hires.com/2010/01/librazione-estrema.html?lan=english" rel="nofollow 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 LPOD!]<br /> | + | <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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===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 18:17, 4 January 2015
Almost Dry
image by " rel="nofollow 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 " 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 " rel="nofollow mosaic shows a steep-sided mound or perhaps a dome at about the same place.
" rel="nofollow Chuck Wood
Related Links
" rel="nofollow Full Size image
Rükl plate 7
COMMENTS?
Click on this icon File:PostIcon.jpg at the upper right to post a comment.
