Difference between revisions of "November 28, 2010"
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<em>LRO WAC image M116419373ME processed by [mailto:revans_01420@yahoo.com Richard Evans]</em><br /> | <em>LRO WAC image M116419373ME processed by [mailto:revans_01420@yahoo.com Richard Evans]</em><br /> | ||
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| − | Marth is an odd crater, even for a [mailto:tychocrater@yahoo.com Chuck Wood]</em><br /> | + | Marth is an odd crater, even for a [https://the-moon.us/wiki/Concentric_Crater concentric crater]. Its inner rim seems taller than average and it fills Marth's entire floor, |
| + | counting the small ridge in the 7 o'clock position. Rick's processing of an LRO Wide Angle Camera image reveals something that is visible in early images, but that I hadn't noticed before. An apron of mare lava surrounds Marth, being most | ||
| + | extensive to the east, and not at all visible to the west. The apron is a slight rise - as indicated by the narrow inflection | ||
| + | caused by a thin partial shadow cast by the edge of the elevated mare. A small round patch of elevated mare material is | ||
| + | often a volcanic dome, but it is not clear if that is the case here; however, the fact that it surrounds Marth suggests the | ||
| + | two are related. Often times a dome-like swelling surrounds pre-existing hills, and that may be the explanation. It appears | ||
| + | that the Marth apron interrupts the rille near it, [[August_4,_2009|Ramsden II]], which would mean that the apron is younger material. But | ||
| + | Ramsden II is also interrupted just to the southwest of Marth, where no observable younger material is apparent. So, Marth | ||
| + | sits on an apron of marginally elevated mare - but I don't think this implies that the concentric crater Marth is volcanic. | ||
| + | <br /> | ||
| + | <br /> | ||
| + | <em>[mailto:tychocrater@yahoo.com Chuck Wood]</em><br /> | ||
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<strong>Related Links</strong><br /> | <strong>Related Links</strong><br /> | ||
| − | Rükl plate [ | + | Rükl plate [https://the-moon.us/wiki/R%C3%BCkl_63 63]<br /> |
<br /> | <br /> | ||
<hr /> | <hr /> | ||
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| − | -- | + | </td> |
| − | === | + | <p><b>Yesterday's LPOD:</b> [[November 27, 2010|Audouin Dollfus]] </p> |
| − | + | <p><b>Tomorrow's LPOD:</b> [[November 29, 2010|A New Collection]] </p> | |
| + | <!-- End of content --> | ||
| + | {{wiki/ArticleFooter}} | ||
Latest revision as of 18:54, 13 October 2018
An Apron
LRO WAC image M116419373ME processed by Richard Evans
Marth is an odd crater, even for a concentric crater. Its inner rim seems taller than average and it fills Marth's entire floor,
counting the small ridge in the 7 o'clock position. Rick's processing of an LRO Wide Angle Camera image reveals something that is visible in early images, but that I hadn't noticed before. An apron of mare lava surrounds Marth, being most
extensive to the east, and not at all visible to the west. The apron is a slight rise - as indicated by the narrow inflection
caused by a thin partial shadow cast by the edge of the elevated mare. A small round patch of elevated mare material is
often a volcanic dome, but it is not clear if that is the case here; however, the fact that it surrounds Marth suggests the
two are related. Often times a dome-like swelling surrounds pre-existing hills, and that may be the explanation. It appears
that the Marth apron interrupts the rille near it, Ramsden II, which would mean that the apron is younger material. But
Ramsden II is also interrupted just to the southwest of Marth, where no observable younger material is apparent. So, Marth
sits on an apron of marginally elevated mare - but I don't think this implies that the concentric crater Marth is volcanic.
Chuck Wood
Related Links
Rükl plate 63
Yesterday's LPOD: Audouin Dollfus
Tomorrow's LPOD: A New Collection
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