Lobate flows are common in the Martian mid-latitude region (30-45 degrees). Some are pristine-looking and highly reminiscent of terrestrial glaciers, whereas others appear more degraded. The flow deposit shown here is a good example of a degraded flow deposit.

The uphill “head” toward the left has carved out an amphitheater-shape into the escarpment, and the “toe,” to the right, is lobate in shape. The surface is highly degraded and eroded, and the deposit shows evidence of deflation (loss of volume, probably from the sublimation of ice), as lateral moraines (ridges running along the length of the feature) are visible.

ID: ESP_028352_2245
date: 13 August 2012
altitude: 302 km

https://uahirise.org/hipod/ESP_028352_2245
NASA/JPL-Caltech/University of Arizona
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