This image covers part of the floor of Noctis Labyrinthus at the western end of Valles Marineris.

The cutout shows aeolian (wind-formed) ridges that have a reddish color on their southeast-facing slopes and a bluish color on their northwest-facing slopes. Most likely this color difference is due to deposition or preservation of reddish dust on generally south-facing slopes.

ID: ESP_076582_1730
date: 27 November 2022
altitude: 263 km

https://uahirise.org/hipod/ESP_076582_1730
NASA/JPL-Caltech/UArizona
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