Morphometry of Quasi-Circular Depressions in the Southern Hemisphere of Mars: Implications for QCD Formation and Resurfacing History

Details Morphometry of Quasi-Circular Depressions in the Southern Hemisphere of Mars: Implications for QCD Formation and Resurfacing History Morphometry of Quasi-Circular Depressions in the Southern Hemisphere of Mars: Implications for QCD Formation and Resurfacing History

Mar 2007

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2007lpi....38.1460r&link_type=abstract

38th Lunar and Planetary Science Conference, (Lunar and Planetary Science XXXVIII), held March 12-16, 2007 in League City, Texas

Physics

1

Scientific paper

The post-impact fill thickness on the floors of large quasi-circular
depressions (QCDs) on Mars is virtually independent of the distance from
the Hellas and Argyre impact basins. This implies that ejecta from these
basins is not the dominant source of QCD

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