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_2230
date: 27 November 2019
altitude: 301 km

https://uahirise.org/hipod/ESP_062507_2230
NASA/JPL-Caltech/UArizona
#Mars #science #NASA