"Wet" Mechanism for Slope Streak Formation on Mars

Details "Wet" Mechanism for Slope Streak Formation on Mars "Wet" Mechanism for Slope Streak Formation on Mars

Mar 2008

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2008lpi....39.1411k&link_type=abstract

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

Physics

4

Scientific paper

We propose that slope streaks are formed by seasonally occurring
concentrated CaCl2 brines in the soil. This mechanism
explains some observations better than the traditional "dry" mechanism.
We also report some new supporting observations.

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