The valleys in this crater flow to the crater’s central pit. The valleys are relatively small for Mars (about 100 meters). In order to determine the paleo-discharges of potential paleo-rivers into the pit, high resolution imagery and digital terrain models are needed. With this data a better understanding of the water requirements for this crater can be determined.

ID: ESP_074754_1825
date: 8 July 2022
altitude: 272 km

https://uahirise.org/hipod/ESP_074754_1825
NASA/JPL-Caltech/UArizona
#Mars #science #NASA