Our objective is to look for recurring slope lineae in the Martian mid-summer, features that we have not seen in previous images. Are the RSL caused by dry ice or granular flows? This image shows the northern part of Arandas, a 25-kilometer impact crater.
ID:
ESP_062507_2230date: 27 November 2019
altitude: 301 km
https://uahirise.org/hipod/ESP_062507_2230
NASA/JPL-Caltech/UArizona
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