The objective of this observation is to examine the margin of a crater’s ejecta. The ejecta on this side looks different than on the opposite side. Ares Vallis is an outflow channel, likely carved by fluids in the distant past.

ID: ESP_054490_2100
date: 12 March 2018
altitude: 291 km

https://uahirise.org/hipod/ESP_054490_2100
NASA/JPL-Caltech/UArizona
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