Mars: Periglacial Morphology and Implications for Future Landing Sites
At the Mars Phoenix landing site and in much of the Martian northern plains, there is ice-cemented ground beneath a layer of dry permafrost. Unlike most permafrost on Earth, though, this ice is not liquid at any time of year. However, in past epochs at higher obliquity the surface conditions during...
Main Authors: | , , , , , , |
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Format: | Other/Unknown Material |
Language: | unknown |
Published: |
2015
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Subjects: | |
Online Access: | http://hdl.handle.net/2060/20150023012 |