Recurring slope lineae are Martian seasonal features characterized by a low brightness (albedo) during local spring/summer that fade during winter/late summer. Their daily characterization through a coordinated observation with HiRISE and the CaSSIS instrument on the ExoMars Trace Gas Orbiter provides additional insights into their nature and formation mechanisms.

ID: ESP_065369_1475
date: 7 July 2020
altitude: 255 km

https://uahirise.org/hipod/ESP_065369_1475
NASA/JPL-Caltech/University of Arizona
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