Simulation of Early Martian Atmosphere Controlled by Impacts

Details Simulation of Early Martian Atmosphere Controlled by Impacts Simulation of Early Martian Atmosphere Controlled by Impacts

Mar 2011

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2011lpi....42.1137s&link_type=abstract

42nd Lunar and Planetary Science Conference, held March 7–11, 2011 at The Woodlands, Texas. LPI Contribution No. 1608, p.1137

Physics

Scientific paper

The model of atmosphere evolution during late accretion of asteroids and
comets (Zahnle, JGR, 1993) with impactor and target vaporization is
applied to an early Mars, using impact erosion and retention
coefficients calculated by Shuvalov (M&PS;, 2009).

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