Image Credit: NASA/JPL/ASU
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Context image credit: NASA/JPL/MOLA
View on map Detailed information on this image is available at the
THEMIS Data Releases website.
Please see the THEMIS Data Citation Note for details on crediting THEMIS images.
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 remniscent 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.
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