Narrow Gullies over High Sand Dunes on Mars: Evidence for Flows Triggered by Liquid Water Near Surface

Details Narrow Gullies over High Sand Dunes on Mars: Evidence for Flows Triggered by Liquid Water Near Surface Narrow Gullies over High Sand Dunes on Mars: Evidence for Flows Triggered by Liquid Water Near Surface

Mar 2002

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2002lpi....33.1215m&link_type=abstract

33rd Annual Lunar and Planetary Science Conference, March 11-15, 2002, Houston, Texas, abstract no.1215

Physics

1

Scientific paper

Recent gullies have been detected on MOC images of the flanks of large
dunes at mid latitudes of Mars. Their formation is likely due to flows
involving liquid water coming from the melting of near-surface ice
during a recent period of high obliquity.

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