Interior Layered Deposits in the Eastern Valles Marineris and Chaotic Terrains on Mars

Details Interior Layered Deposits in the Eastern Valles Marineris and Chaotic Terrains on Mars Interior Layered Deposits in the Eastern Valles Marineris and Chaotic Terrains on Mars

Mar 2007

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2007lpi....38.1568s&link_type=abstract

38th Lunar and Planetary Science Conference, (Lunar and Planetary Science XXXVIII), held March 12-16, 2007 in League City, Texas

Physics

Scientific paper

Most interior layered deposits occur as isolated light-toned mounds but
they vary in appearance. We show differences in morphology, elevation,
relative thickness, and surface structure. We also present measurements
in layer geometry.

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