Erosion Of Scalloped Terrain On Mars
In this observation, it looks like we can view a couple of erosional windows in the scalloped (ice-rich) unit. This area is a good place for imaging samples of the contact to understand the deposition and erosion.
We can also sample boulders and polygons at full resolution. Expansion and contraction of underground ice is responsible for the polygon formation.
ID: ESP_072026_2225
date: 7 December 2021
altitude: 298 km
https://uahirise.org/hipod/ESP_072026_2225NASA/JPL-Caltech/UArizona