On the floors of some channels are features called lineated floor deposits. They are ridged and grooved materials that seem to deflect around obstacles. They are believed to be ice-rich. Some glaciers on the Earth show such features. Lineated floor deposits may be related to lobate debris aprons, which have been proven to contain large amounts of ice. Reull Vallis, as pictured below, displays these deposits.

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  Drainage features in Reull Vallis, as seen by THEMIS. Click on image to see relationship of Reull Vallis to other features.
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  Reull Vallis with lineated floor deposits, as seen by THEMIS. Click on image to see relationship to other features.
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  Layers in Reull Vallis, as seen by THEMIS.
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  Fretted terrain near Reull Vallis, as seen by HiRISE.
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  Close-up of fretted terrain near Reull Vallis, as seen by HiRISE. This area would be a challenge to walk across.
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  Layers in Monument Valley, Utah. These are accepted as being formed, at least in part, by water deposition. Since Mars contains similar layers, water remains as a major cause of layering on Mars.

• Dao Vallis
• Harmakhis Vallis

Wikimedia Commons has media related to Reull Vallis.

• Google Mars map centred on Reull Vallis.
• Geologic Map of Reull Vallis Region of Mars, by Astrogeology Science Center, U.S. Geological Survey

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