File:Features around Ceraunius Tholus and Uranius Tholus ESA223670.tiff

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English: Ceraunius Tholus and Uranius Tholus are two volcanoes in the Tharsis region of Mars. The flanks of Ceraunius Tholus display deeply incised valleys of which the longest and deepest is about 3.5 km wide and 300 m deep [box 1]. This valley terminates with a fan of deposited material in the northern end of the elongated Rahe crater. The crater itself [box 2] is 35 km by 18 km and was created by the oblique impact of a meteorite. Other impacts have scarred this region, too. One in particular has ejected material over the flanks of the smaller volcano [box 3]. This image has been derived from data acquired during three separate orbits of Mars Express, which took place between 25 November 2004 and 22 June 2006.
Date
Source http://www.esa.int/spaceinimages/Images/2011/03/Features_around_Ceraunius_Tholus_and_Uranius_Tholus
Author European Space Agency
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(Reusing this file)		 ESA/DLR/FU Berlin (G. Neukum),CC BY-SA 3.0 IGO
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Features around Ceraunius Tholus and Uranius Tholus
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Mars Express
Activity
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Space Science

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This file is licensed under the Creative Commons Attribution-ShareAlike 3.0 IGO license.
Attribution: ESA/DLR/FU Berlin (G. Neukum)
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Date/TimeThumbnailDimensionsUserComment
current13:21, 24 May 2017Thumbnail for version as of 13:21, 24 May 20176,839 × 4,089 (21.48 MB)Fæ (talk | contribs)European Space Agency, Id 223670, http://www.esa.int/spaceinimages/Images/2011/03/Features_around_Ceraunius_Tholus_and_Uranius_Tholus, User:Fæ/Project_list/ESA

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