Interactions Between Hypervelocity Impact Ejecta and Planetary Atmospheres: From the Early Earth to Mars

Details Interactions Between Hypervelocity Impact Ejecta and Planetary Atmospheres: From the Early Earth to Mars Interactions Between Hypervelocity Impact Ejecta and Planetary Atmospheres: From the Early Earth to Mars

Mar 2011

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2011lpi....42.2766g&link_type=abstract

42nd Lunar and Planetary Science Conference, held March 7–11, 2011 at The Woodlands, Texas. LPI Contribution No. 1608, p.2766

Computer Science

Scientific paper

Using a two-phase fluid flow code, we compare the reentry of high speed
impact ejecta into the atmospheres of the modern Earth, the Archean
Earth, Venus, and Mars.

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