In the infrared, these channels contrast clearly with the surrounding terrain, but are likely relatively shallow. High-resolution stereo observations could shed some additional light on the character and age of these channels, allowing them to be placed in context with nearby features like the Cerberus Fossae.

ID: ESP_075175_1935
date: 9 August 2022
altitude: 278 km

https://uahirise.org/hipod/ESP_075175_1935
NASA/JPL-Caltech/UArizona
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