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Images of rocks in the canyon walls almost always show layers. Some layers appear tougher than others. In the image below of Ganges Chasma Layers, as seen by HiRISE, one can see that the upper, light-toned deposits are eroding much faster than the lower darker layers. Some cliffs on Mars show a few darker layers standing out and often breaking ...
Candor Chasma in mosaic of THEMIS infrared images, with parts of Ophir, Melas and Juventae chasmata at top, lower left and extreme upper right, respectively. Massive landslide deposits, the Melas Labes, are visible near the junction of Candor and Melas chasmata at bottom, just left of center.
Echus Chasma is approximately 100 km long and 10 km wide, with valleys ranging in depth from around 1 km to 4 km. [1] It is the source region of the Kasei Valles outflow channel, which extends northward from it. It is situated just west of Hebes Chasma, to which it does not connect.
Tithonium Chasma is a large canyon in the Coprates quadrangle of Mars at 4.6° south latitude and 84.7° west longitude. It is about 810 km long and was named after a classical albedo feature . [ 1 ]
Ius Chasma is a large canyon in the Coprates quadrangle of Mars at 7° south latitude and 85.8° west longitude. It is about 938 km long and was named after a classical albedo feature name. It is about 938 km long and was named after a classical albedo feature name.
Ophir Chasma in mosaic of THEMIS infrared images, with part of Candor Chasma at bottom. Ophir Chasma / ˈ oʊ f ər ˈ k æ z m ə / is a canyon in the Coprates quadrangle of Mars at 4° south latitude and 72.5° west longitude. It is about 317 km long and was named after Ophir, a land mentioned in the Bible.
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