Do Mega Impacts Leave Craters? Characterizing Mega Impacts and Their Relation to the Mars Hemispheric Dichotomy

Details Do Mega Impacts Leave Craters? Characterizing Mega Impacts and Their Relation to the Mars Hemispheric Dichotomy Do Mega Impacts Leave Craters? Characterizing Mega Impacts and Their Relation to the Mars Hemispheric Dichotomy

Jul 2007

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2007lpico1353.3354m&link_type=abstract

Seventh International Conference on Mars, held July 9-13, 2007 in Pasadena, California, LPI Contribution No. 1353, p.3354

Physics

Scientific paper

We simulate planetary-scale impacts, and relate their attributes to the
Mars hemispheric dichotomy. We find that slow, head-on impacts melt much
of the surface, but faster and oblique impacts are less disruptive and
preserve attributes of the event.

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