Difference between revisions of "February 9, 2010"
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=Too Small To Fail?= | =Too Small To Fail?= | ||
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| − | <em>image by [mailto:g.tarsoudis@freemail.gr George Tarsoudis], Greece</em><br /> | + | <em>image by [mailto:g.tarsoudis@freemail.gr" rel="nofollow George Tarsoudis], Greece</em><br /> |
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The nearly total lack of remnant rim structure indicates that the impact basin filled by Mare Nubium is old. The basin's reality was reaffirmed by Kaguya [http://lpod.wikispaces.com/November+6%2C+2009 topographic mapping] that shows the broad center of the mare is indeed depressed compared to its edges. Nubium seems to have more submerged craters than other lava flooded basins, and unlike most basins they are everywhere, not just around the shallow edges. Kies and Lubinezky are in the basin's periphery but Wolf, Gould and many unnamed ghost rings are more in the middle. This means that the earlier surface that these ghostly craters formed on was shallow enough so that later lavas surrounded or overtopped the craters, but did not completely bury them. In Serentitatis, Imbrium and Crisium, there is evidence that the basin centers subsided as lava was added to the basin. This deepened the basin centers so that craters originally formed there became completely submerged by 2-4 km of later lavas. Nubium is a smaller basin and mare, and apparently did not undergo subsidence. That is consistent with the paucity of circumferential faults, differing from Serenitatis and nearby Humorum. <br /> | The nearly total lack of remnant rim structure indicates that the impact basin filled by Mare Nubium is old. The basin's reality was reaffirmed by Kaguya [http://lpod.wikispaces.com/November+6%2C+2009 topographic mapping] that shows the broad center of the mare is indeed depressed compared to its edges. Nubium seems to have more submerged craters than other lava flooded basins, and unlike most basins they are everywhere, not just around the shallow edges. Kies and Lubinezky are in the basin's periphery but Wolf, Gould and many unnamed ghost rings are more in the middle. This means that the earlier surface that these ghostly craters formed on was shallow enough so that later lavas surrounded or overtopped the craters, but did not completely bury them. In Serentitatis, Imbrium and Crisium, there is evidence that the basin centers subsided as lava was added to the basin. This deepened the basin centers so that craters originally formed there became completely submerged by 2-4 km of later lavas. Nubium is a smaller basin and mare, and apparently did not undergo subsidence. That is consistent with the paucity of circumferential faults, differing from Serenitatis and nearby Humorum. <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>Technical Details</strong><br /> | <strong>Technical Details</strong><br /> | ||
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<strong>Related Links</strong><br /> | <strong>Related Links</strong><br /> | ||
Rükl plate [http://the-moon.wikispaces.com/R%C3%BCkl+53 53]<br /> | Rükl plate [http://the-moon.wikispaces.com/R%C3%BCkl+53 53]<br /> | ||
| − | George's astro [http://www.lunar-captures.com/ website]<br /> | + | George's astro [http://www.lunar-captures.com/" rel="nofollow website]<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 19:19, 4 January 2015
Too Small To Fail?
image by " rel="nofollow George Tarsoudis, Greece
The nearly total lack of remnant rim structure indicates that the impact basin filled by Mare Nubium is old. The basin's reality was reaffirmed by Kaguya topographic mapping that shows the broad center of the mare is indeed depressed compared to its edges. Nubium seems to have more submerged craters than other lava flooded basins, and unlike most basins they are everywhere, not just around the shallow edges. Kies and Lubinezky are in the basin's periphery but Wolf, Gould and many unnamed ghost rings are more in the middle. This means that the earlier surface that these ghostly craters formed on was shallow enough so that later lavas surrounded or overtopped the craters, but did not completely bury them. In Serentitatis, Imbrium and Crisium, there is evidence that the basin centers subsided as lava was added to the basin. This deepened the basin centers so that craters originally formed there became completely submerged by 2-4 km of later lavas. Nubium is a smaller basin and mare, and apparently did not undergo subsidence. That is consistent with the paucity of circumferential faults, differing from Serenitatis and nearby Humorum.
" rel="nofollow Chuck Wood
Technical Details
See upper right.
Related Links
Rükl plate 53
George's astro " rel="nofollow website
COMMENTS?
Click on this icon File:PostIcon.jpg at the upper right to post a comment.
