Ice Flow in Debris Aprons and Central Peaks, and the Application of Crater Counts

Details Ice Flow in Debris Aprons and Central Peaks, and the Application of Crater Counts Ice Flow in Debris Aprons and Central Peaks, and the Application of Crater Counts

Mar 2009

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2009lpi....40.1204h&link_type=abstract

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

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We apply studies of decameter-scale craters to studies of probable
ice-flow-related features on Mars, to interpret both chronometry and
geological processes among the features. We find losses of
decameter-scale craters relative to nearby plains, probably due to
sublimation.

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