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Hebes Chasma : ウィキペディア英語版
Hebes Chasma

Hebes Chasma is an isolated chasma just north of the Valles Marineris canyon system of Mars. It is centered at 1 degree southern latitude and 76 degrees western longitude, just between the Martian equator and the Valles Marineris system, just east of the Tharsis region.
==Geography==
Hebes Chasma is a completely closed depression in the surface of Mars, with no outflows to the nearby Echus Chasma to the west, Perrotin Crater to the southwest, or Valles Marineris to the south. Its maximum extents are approximately 320 km east to west, 130 km north to south, and 5 to 6 km in depth. At the center of the depression is Hebes Mensa, a large mesa rising some 5 km off the valley floor, nearly as high as the surrounding terrain. This central plateau makes Hebes Chasma a unique valley in Martian geography.
In high resolution pictures of Mars Express ( http://spaceinimages.esa.int/Images/2013/10/Hebes_Chasma )
blue areas at the deepest section of the depression show characteristics of a lake: Sharp borders between the yellow and blue area and light blue near the yellow area, becoming darker away from the border.

抄文引用元・出典: フリー百科事典『 ウィキペディア(Wikipedia)
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