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9 July 2004 The processes that have eroded and exposed sedimentary rock outcrops in many of the Valles Marineris troughs are unclear. However, this Mars Global Surveyor (MGS) Mars Orbiter Camera (MOC) image shows an example from western Tithonium Chasma that is unambiguous. The ridges are

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      EUN,LOM,LRE4,hdl:10494/256843,work-cmr-id:256843,http://photojournal.jpl.nasa.gov:http://photojournal.jpl.nasa.gov/catalog/PIA06369,ilox,learning resource exchange,LRE metadata application profile,LRE

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