Origin of Closely-Spaced Groups of Pits in Martian Craters

Details Origin of Closely-Spaced Groups of Pits in Martian Craters Origin of Closely-Spaced Groups of Pits in Martian Craters

Mar 2012

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2012lpi....43.1017b&link_type=abstract

43rd Lunar and Planetary Science Conference, held March 19–23, 2012 at The Woodlands, Texas. LPI Contribution No. 1659, id.1017

Physics

Scientific paper

A model of explosive degassing of thin deposits of suevite-like
fall-back is proposed for the origin of closely-spaced pits formed in
thin impactite deposits superposed on well-preserved martian impact
craters.

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