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Image of Mare Tyrrhenum quadrangle (MC-22). Most of the region contains heavily cratered highlands. The central part contains Tyrrhena Patera and the
Image of Mare Tyrrhenum quadrangle (MC-22). Most of the region contains heavily cratered highlands. The central part contains Tyrrhena Patera and the associated ridged plains of Hesperia Planum.
Depression on crater floor, as seen by HiRISE under HiWish program. This scene is enlarged in the next two images.
Depression on crater floor, as seen by HiRISE under HiWish program. This scene is enlarged in the next two images.
Close-up of depression on crater floor, as seen by HiRISE under HiWish program
Close-up of depression on crater floor, as seen by HiRISE under HiWish program
Close-up of west edge of crater depression, as seen by HiRISE under HiWish program
Close-up of west edge of crater depression, as seen by HiRISE under HiWish program
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Viking MDIM of Mare Tyrrhenum quadrangle. Hesperia is the intermediate-toned (dusky) region (left of center) lying between the darker regions Mare Tyr
Viking MDIM of Mare Tyrrhenum quadrangle. Hesperia is the intermediate-toned (dusky) region (left of center) lying between the darker regions Mare Tyrrhenum (left) and Mare Cimmerium (right).
Closeup of the surface of northwestern Hesperia Planum, as seen by HiRISE camera on Mars Reconnaissance Orbiter (MRO).
Closeup of the surface of northwestern Hesperia Planum, as seen by HiRISE camera on Mars Reconnaissance Orbiter (MRO).
Viking orbiter view of wrinkle ridges in Hesperia Planum. North is at upper left. Image is about 107 km (66 mi) across.
Viking orbiter view of wrinkle ridges in Hesperia Planum. North is at upper left. Image is about 107 km (66 mi) across.
THEMIS daytime IR mosaic image of Tyrrhenus Mons. This ancient, eroded volcano was nicknamed the Dandelion when first seen in Mariner 9 images.
THEMIS daytime IR mosaic image of Tyrrhenus Mons. This ancient, eroded volcano was nicknamed the Dandelion when first seen in Mariner 9 images.