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Properties of Seasonal Ice at Sisyphi Cavi and Implications for Current Modification of Martian Gullies
Martian gullies are geologically recent landforms that may form either through liquid-water activity and/or through processes involving CO2 ice. We investigated the mechanisms responsible for the formation or modification of these features by focusing on the active site of Sisyphi Cavi (68°S, 1°E),
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