This observation site includes both fluvial features and possible volcanic features.A high resolution image can contribute towards a better understanding of the fluvial and volcanic histories of this region. Marte Vallis is a valley that has been identified as an outflow channel, possible created by a catastrophic release of water from aquifers beneath the Martian surface.

ID: ESP_065203_1910
date: 24 June 2020
altitude: 278 km

https://uahirise.org/hipod/ESP_065203_1910
NASA/JPL-Caltech/UArizona
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