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22 May 2005 This Mars Global Surveyor (MGS) Mars Orbiter Camera (MOC) image shows yardangs formed by wind erosion of materials exposed on the floor of western Tithonium Chasma. The winds responsible for these landforms blew from the north/northeast (top/upper right). Tithonium Chasma is part of the Valles Marineris system.
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