The Deepest Basin on Mars is Formed by Aeolian Erosion

Details The Deepest Basin on Mars is Formed by Aeolian Erosion The Deepest Basin on Mars is Formed by Aeolian Erosion

Mar 2012

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2012lpi....43.1105h&link_type=abstract

43rd Lunar and Planetary Science Conference, held March 19–23, 2012 at The Woodlands, Texas. LPI Contribution No. 1659, id.1105

Physics

Scientific paper

The trough forming NW floor of Hellas Planita has been deepened by at
least 1 km by wind erosion as evidenced by geomorphic evidence and
mesoscale atmospheric modeling.

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