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Alpine Glaciers

Sept. 3, 2003
NASA's Mars Odyssey spacecraft captured this image in August 2003, showing part of the western flank of Arsia Mons, the southernmost of the three great Tharsis Montes on Mars. The surface shows parallel ridges.
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Released 27 August 2003

This image shows part of the western flank of Arsia Mons, the southernmost of the three great Tharsis Montes. The surface shows parallel ridges more reminiscent of a Zen garden than any typical geological feature. These ridges are not typical of lava flow fronts, so a different explanation has been proposed by Mars scientists. These ridges may instead be ancient signs of previously existing glaciers that formed high on the volcano's flank. As glaciers retreat with the seasons and shifting climate, they leave behind a mound of debris along their receding edge. Successive retreats can produce a series of parallel ridges similar to those seen here.

Image information: VIS instrument. Latitude -6.9, Longitude 230.5 East (129.5 West). 19 meter/pixel resolution.

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