Persistent Surface Changes in Solis Lacus, Mars

Details Persistent Surface Changes in Solis Lacus, Mars Persistent Surface Changes in Solis Lacus, Mars

Mar 2012

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2012lpi....43.2598g&link_type=abstract

43rd Lunar and Planetary Science Conference, held March 19–23, 2012 at The Woodlands, Texas. LPI Contribution No. 1659, id.2598

Physics

Scientific paper

Orbital monitoring has shown that the Solis Lacus region experiences
continual, drastic albedo changes due to eolian activity. Images from
HiRISE help explain the activity, and show evidence for lateral surface
transport of dust deposits.

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