Low-Temperature Aqueous Fluids on Mars

Details Low-Temperature Aqueous Fluids on Mars Low-Temperature Aqueous Fluids on Mars

Mar 2008

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2008lpi....39.1176c&link_type=abstract

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

Physics

1

Scientific paper

Ferric sulphate solutions remain liquid at average martian surface
temperatures, down to 201 K, and present very low evaporation rates,
which make them the best candidates to explain the formation of martian
flow features and gullies.

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