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Part of Hesperia Planum region, taken by Mars color camera (MCC)

Part of Hesperia Planum regionImage shows part of Hesperia Planum region, taken by Mars color camera (MCC) on 31-01-2015 at a spatial resolution of 58m from an altitude of 1132km. Wrinkle ridges and craters of smaller diameters are clearly seen in this image. Wrinkle ridges on planetary surface are formed due to compressional stress regime. Ridge means linear/ curvilinear elongated raised structure.