Grain Shape Analysis of Sand- and Silt-Size Sediments at the Phoenix Mars Lander Site from Images Acquired by the Phoenix Optical Microscope

Details Grain Shape Analysis of Sand- and Silt-Size Sediments at the Phoenix Mars Lander Site from Images Acquired by the Phoenix Optical Microscope Grain Shape Analysis of Sand- and Silt-Size Sediments at the Phoenix Mars Lander Site from Images Acquired by the Phoenix Optical Microscope

Mar 2011

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2011lpi....42.1516v&link_type=abstract

42nd Lunar and Planetary Science Conference, held March 7–11, 2011 at The Woodlands, Texas. LPI Contribution No. 1608, p.1516

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Scientific paper

Differences in grain roundness between Phoenix samples suggest
differences in grain accumulation, abrasion, fracturing, or aggregation
in the trough adjacent to the periglacial polygon relative to the other
periglacial geomorphic settings examined.

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