Mid-Latitude Pedestal Crater Heights: A Proxy for the Thickness of a Past Climate-related, Ice-rich Substrate

Details Mid-Latitude Pedestal Crater Heights: A Proxy for the Thickness of a Past Climate-related, Ice-rich Substrate Mid-Latitude Pedestal Crater Heights: A Proxy for the Thickness of a Past Climate-related, Ice-rich Substrate

Mar 2009

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2009lpi....40.1313k&link_type=abstract

40th Lunar and Planetary Science Conference, (Lunar and Planetary Science XL), held March 23-27, 2009 in The Woodlands, Texas, i

Physics

Scientific paper

The armored surfaces of mid-latitude pedestal craters (Pd) on Mars
preserve a past climate-related, ice-rich substrate deposited during
periods of higher obliquity. The Pd heights thus provide insight into
the regional thicknesses of the substrate.

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