HiPOD: Wednesday, 26 April 2023
Flow-Like Feature within Chryse Planitia

Flow-Like Feature within Chryse Planitia

A Flow-Like Feature within Chryse Planitia
This image covers a flow-like feature that is hypothesized to be the result of subsurface sediment mobilization. With it, we can investigate details about the associated mud movement over the Martian surface. The flow is showing an interesting shape that might be evidence of the former presence of an icy-muddy crust.

ID: ESP_072993_2000
date: 20 February 2022
altitude: 284 km

https://uahirise.org/hipod/ESP_072993_2000
NASA/JPL-Caltech/UArizona
#Mars #science #NASA

Black & white is less than 5 km across; enhanced color is less than 1 km. For full observation details, visit the ID link.