Martian Microcrater Production at Low and High Elevation in Response to Obliquity-driven Atmospheric Pressure Variations

Details Martian Microcrater Production at Low and High Elevation in Response to Obliquity-driven Atmospheric Pressure Variations Martian Microcrater Production at Low and High Elevation in Response to Obliquity-driven Atmospheric Pressure Variations

Mar 2008

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2008lpi....39.2385s&link_type=abstract

39th Lunar and Planetary Science Conference, (Lunar and Planetary Science XXXIX), held March 10-14, 2008 in League City, Texas.

Physics

Scientific paper

We characterize the potential effects of obliquity-driven climate
variations on impact crater production rates through Monte Carlo
simulations at mean martian surface elevations, and at elevations
characteristic of high altitude Tharsis calderas.

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