Long-Term Aeolian Modification of the North Polar Cap and Formation of the North Polar Chasmata, Mars

Details Long-Term Aeolian Modification of the North Polar Cap and Formation of the North Polar Chasmata, Mars Long-Term Aeolian Modification of the North Polar Cap and Formation of the North Polar Chasmata, Mars

Jul 2007

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2007lpico1353.3178w&link_type=abstract

Seventh International Conference on Mars, held July 9-13, 2007 in Pasadena, California, LPI Contribution No. 1353, p.3178

Physics

Scientific paper

In this report we re-examine the debate over the origin of the north
polar chasmata on Mars. We conclude that a model for chasmata formation
that emphasizes long-term aeolian erosion and retreat of the polar
layered material best explains the observations and available imagery.

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