This image can help us determine whether there are one or multiple ejecta lobes in this region. Hale Crater is often imaged by HiRISE for the presence of recurring slope lineae, or flows that may or may not be briny liquid.

ID: ESP_055057_1415
date: 25 April 2018
altitude: 254 km

https://uahirise.org/hipod/ESP_055057_1415
NASA/JPL-Caltech/University of Arizona
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