The objective of this observation is to examine a group of cones that are in a shallow valley. Some have suggested that these features are mud volcanoes. These are in locations where watery sediments seep onto the surface. Because of Mars’ low temperatures and pressures, the mud quickly freezes.

ID: ESP_075584_2180
date: 10 September 2022
altitude: 298 km

https://uahirise.org/hipod/ESP_075584_2180
NASA/JPL-Caltech/UArizona
#Mars #science #NASA