Thermal Contraction Crack Polygons on Mars: Classification, Distribution, and Context for Phoenix from North and South Polar HiRISE Observations

Details Thermal Contraction Crack Polygons on Mars: Classification, Distribution, and Context for Phoenix from North and South Polar HiRISE Observations Thermal Contraction Crack Polygons on Mars: Classification, Distribution, and Context for Phoenix from North and South Polar HiRISE Observations

Mar 2009

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2009lpi....40.1616l&link_type=abstract

40th Lunar and Planetary Science Conference, (Lunar and Planetary Science XL), held March 23-27, 2009 in The Woodlands, Texas, i

Physics

Scientific paper

Thermal contraction crack polygon morphology is used to understand the
deposition and modification of young, ice-rich mantling units across
martian mid-high latitudes and at the Phoenix landing site. Signatures
of excess ice and sublimation dominate.

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