Mid-Latitude Amazonian Glaciation on Mars: Controls on Accumulation and Glacial Flow Patterns

Details Mid-Latitude Amazonian Glaciation on Mars: Controls on Accumulation and Glacial Flow Patterns Mid-Latitude Amazonian Glaciation on Mars: Controls on Accumulation and Glacial Flow Patterns

Mar 2012

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2012lpi....43.1296f&link_type=abstract

43rd Lunar and Planetary Science Conference, held March 19–23, 2012 at The Woodlands, Texas. LPI Contribution No. 1659, id.1296

Physics

Scientific paper

A model of flow into a crater from episodic layering events driven by
obliquity demonstrates that even at Amazonian temperatures, concentric
crater fill can be formed in as little as 50 m.y., whereas flow from a
single persistent layer takes 450 m.y.

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