Martian H2O Ice Outliers may Result from Wintertime Near-Surface CO2 Snows

Details Martian H2O Ice Outliers may Result from Wintertime Near-Surface CO2 Snows Martian H2O Ice Outliers may Result from Wintertime Near-Surface CO2 Snows

Mar 2008

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2008lpi....39.1422b&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

The presence of summer "ice patches" suggests winter near-surface
CO2 snow formation from orographic lifting. This CO2 snow
becomes a cold trap for H2O. We test this hypothesis using
data from MGS, ODY, MEX, and MRO.

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