Constraints on the Proposed Formation Models for Martian Central Pit Craters

Details Constraints on the Proposed Formation Models for Martian Central Pit Craters Constraints on the Proposed Formation Models for Martian Central Pit Craters

Mar 2011

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2011lpi....42.1149b&link_type=abstract

42nd Lunar and Planetary Science Conference, held March 7–11, 2011 at The Woodlands, Texas. LPI Contribution No. 1608, p.1149

Physics

Scientific paper

We are conducting a study of the distribution and characteristics of
martian central pit craters. Based on an analysis of 1312 central pit
craters, we find that the melt-drainage model is most consistent with
our data.

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