Fluvial erosion on Mars

Numéro d’image : 11882460
Fluvial erosion on Mars
Fluvial erosion on Mars. Colour enhanced satellite image of the Candor Chasma region of the Valles Marineris canyon. It is thought that this canyon initially formed as the result of tectonic fracturing of the upper crust of Mars. The fractures,or joints,are visible as approximately vertical thin blue lines bordered by yellow areas (upper left to lower left). The yellow areas are halos,interpreted as areas of rock that have been chemically altered by fluid flowing through the joints. This image was obtained by the High Resolution Imaging Science Experiment (HiRise) camera on board the Mars Reconnaissance Orbiter,September 30th,2006
Licence : Droits gérés
Crédit: Science Photo Library / NASA / JPL / University of Arizona
Taille de l’image : 2381 px × 3743 px
Model Release : Non requis
Property Release : Non requis
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