Slope Streaks in the Antarctic Dry Valleys: Characteristics, Candidate Formation Mechanisms, and Implications for Slope Streak Formation in the Martian Environment

Details Slope Streaks in the Antarctic Dry Valleys: Characteristics, Candidate Formation Mechanisms, and Implications for Slope Streak Formation in the Martian Environment Slope Streaks in the Antarctic Dry Valleys: Characteristics, Candidate Formation Mechanisms, and Implications for Slope Streak Formation in the Martian Environment

Jul 2007

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2007lpico1353.3114h&link_type=abstract

Seventh International Conference on Mars, held July 9-13, 2007 in Pasadena, California, LPI Contribution No. 1353, p.3114

Physics

Scientific paper

Enigmatic slope streaks on Mars are apparently active today. Remarkably
similar analogs in the Antarctic Dry Valleys hyperarid polar desert
involve near-surface flow of saline meltwater and wicking to the
surface; we examine implications for Mars.

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