Near-Surface Ice Likely Cause of Thermal Anomaly in Martian North Polar Erg

Details Near-Surface Ice Likely Cause of Thermal Anomaly in Martian North Polar Erg Near-Surface Ice Likely Cause of Thermal Anomaly in Martian North Polar Erg

Mar 2010

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2010lpi....41.2495p&link_type=abstract

41st Lunar and Planetary Science Conference, held March 1-5, 2010 in The Woodlands, Texas. LPI Contribution No. 1533, p.2495

Physics

Scientific paper

The anomalously low apparent thermal inertia of the north polar erg on
Mars is attributed to a thermal effect of a layered surface with ~20 cm
of normal sand over an ice-cemented substrate, obviating the need to
invoke exotic agglomerations of dust.

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