These hills are surrounded by small gullies, where there is likely activity related to recurring slope lineae, perhaps even slumps, which are masses of loosely consolidated material or rock layers that move a short distance down a slope. These features are similar to well-monitored hills in Juventae Chasma. Eos is located in the southern part of the Valles Marineris canyon system.

ID: ESP_072598_1630
date: 21 January 2022
altitude: 264 km

https://uahirise.org/hipod/ESP_072598_1630
NASA/JPL-Caltech/UArizona
#Mars #science #NASA