Carbon dioxide glaciers on Mars: Products of recent low obliquity epochs (?)

Mathematics – Logic

Scientific paper

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Scientific paper

Three localized sets of small arcuate ridges associated with slopes in the northern polar area of Mars (˜70°N latitude) are morphologically similar to sets of drop moraines left by episodes of advance and retreat of cold-based glaciers. Comparison with other glacial features on Mars shows that these features differ in important aspects from those associated with water-ice flow. Instead, we interpret these features to be due to perennial accumulation and flow of solid carbon dioxide during recent periods of very low spin-axis obliquity.

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