The Subsurface Geology of Mars: Remote Sensing of Impact Craters Using THEMIS, TES, MOC and MOLA

Details The Subsurface Geology of Mars: Remote Sensing of Impact Craters Using THEMIS, TES, MOC and MOLA The Subsurface Geology of Mars: Remote Sensing of Impact Craters Using THEMIS, TES, MOC and MOLA

Mar 2006

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2006lpi....37.1739t&link_type=abstract

37th Annual Lunar and Planetary Science Conference, March 13-17, 2006, League City, Texas, abstract no.1739

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Impact craters provide natural exposures of subsurface composition,
stratigraphy and, in some cases, geologic features that are not
otherwise exposed at the surface. Here we present results from a
THEMIS-based remote sensing study of martian impact craters that expose
subsurface materials.

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