Impact Origin for the Martian Crustal Dichotomy: Half-Emptied or Half-Filled?

Details Impact Origin for the Martian Crustal Dichotomy: Half-Emptied or Half-Filled? Impact Origin for the Martian Crustal Dichotomy: Half-Emptied or Half-Filled?

Mar 2010

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2010lpi....41.1988r&link_type=abstract

41st Lunar and Planetary Science Conference, held March 1-5, 2010 in The Woodlands, Texas. LPI Contribution No. 1533, p.1988

Physics

Scientific paper

We suggest an alternative impact origin for the martian crustal
dichotomy in which impact generated melt floods the excavated cavity,
produces thickened crust, and generates an antipodal topographic basin.

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