Simulating the Landscape Evolution of the Martian Residual CO2 Ice Cap

Details Simulating the Landscape Evolution of the Martian Residual CO2 Ice Cap Simulating the Landscape Evolution of the Martian Residual CO2 Ice Cap

Mar 2011

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2011lpi....42.2728b&link_type=abstract

42nd Lunar and Planetary Science Conference, held March 7–11, 2011 at The Woodlands, Texas. LPI Contribution No. 1608, p.2728

Physics

Scientific paper

I model the observed landscape evolution of the martian ice ca, where
expanding pits were interpreted as evidence of climate change. Model
results show no such change is necessary and predict an ice cap
continuously being destroyed and recreated.

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