Fig. 7From: Surface environment of Phobos and Phobos simulant UTPSSimulated surface of Phobos using UTPS-TB with the observed crater size-frequency distributions and incidence angles of 70 degrees (a) and 10 degrees (b). Close-up views of Phobos’ surface (c, d; parts of MGS Mars Orbiter camera image 55,103)Back to article page