A possible new impact site (formed at most between February 2004 and December 2011) is the likely cause of these slope streaks. Dark blast zones not seen in other images with lower resolution than HiRISE can often trigger a request for us to take a closer look.

ID: ESP_055232_2110
date: 9 May 2018
altitude: 290 km

https://uahirise.org/hipod/ESP_055232_2110
NASA/JPL-Caltech/UArizona
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