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Impact crater candidate
Posted on Friday, January 23, 2015
Uploaded by
Waspie_Dwarf
Image credit: ESA/Rosetta/MPS for OSIRIS Team MPS/UPD/LAM/IAA/SSO/INTA/UPM/DASP/IDA
Uploader comment: The surface of Comet 67P/Churyumove–Gerasimenko is almost devoid of recognisable impact craters, but this candidate may be an example formed by debris that was first ejected from the surface but subsequently fell back down. It measures about 35 m across and has been partially covered by dust.
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