HiPOD: Friday, 19 May 2023
Inverted Channels on Fan in Saheki Crater

Inverted Channels on Fan in Saheki Crater

Inverted Channels in Saheki Crater
The large alluvial fans in the southern Martian highlands have the potential to provide key insights into the history of water on the planet’s surface. The ridges on these fans are inferred to be the preserved remains of the fluvial channels responsible for fan formation. Saheki is 82 kilometers in diameter and was named after Tsuneo Saheki, a Japanese amateur astronomer (1916-1996).

ID: ESP_042368_1580
date: 10 August 2015
altitude: 259 km

https://uahirise.org/hipod/ESP_042368_1580
NASA/JPL-Caltech/University of Arizona
#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.