File:Close to Ma'adim Vallis, in 3D ESA200053.jpg

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English: Mars Express image of a region close to Ma’adim Vallis, one of the largest canyons on Mars. After Valles Marineris, Ma’adim Vallis is one of the largest canyons on Mars. The imaged region lies south-east of Ma’adim Vallis; the pictures are centred at about 29°S and 182°E and have a ground resolution of 15 m/pixel.

Ma’adim Vallis is located between the volcanic region of Tharsis, which harbours four volcanoes, including the largest in the Solar System, and the Hellas Planitia impact basin. The canyon, 20 km wide and 2 km deep, originates in the southern highlands close to the ‘dichotomy boundary’ and ends in Gusev crater. The dichotomy boundary is a narrow region separating the cratered highlands, located mostly in the southern hemisphere of Mars, from the northern hemisphere's lowland plains.

The 3D image was calculated from the nadir and one stereo channel. Stereoscopic glasses are required for viewing.
Date
Source http://www.esa.int/spaceinimages/Images/2009/07/Close_to_Ma_adim_Vallis_in_3D
Author European Space Agency
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ESA/DLR/FU Berlin (G. Neukum),CC BY-SA 3.0 IGO
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Title
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Close to Ma'adim Vallis, in 3D
Mission
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Mars Express
Activity
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Space Science

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Attribution: ESA/DLR/FU Berlin (G. Neukum)
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Date/TimeThumbnailDimensionsUserComment
current15:55, 24 May 2017Thumbnail for version as of 15:55, 24 May 20174,000 × 2,007 (1.28 MB) (talk | contribs)European Space Agency, Id 200053, http://www.esa.int/spaceinimages/Images/2009/07/Close_to_Ma_adim_Vallis_in_3D, User:Fæ/Project_list/ESA

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