Analysis of Possible Interfacial Water Driven Seepages on Mars

Details Analysis of Possible Interfacial Water Driven Seepages on Mars Analysis of Possible Interfacial Water Driven Seepages on Mars

Mar 2008

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2008lpi....39.1555k&link_type=abstract

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

Physics

2

Scientific paper

Based on observations and theoretical considerations, seepage-like
structures on polar dunes emanate from Dark Dune Spots are probably
caused by interfacial water at subzero temperatures.

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