File:Light-Toned Deposits in Noctis Labyrinthus.jpg

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English: CRISM observations of this region of the Noctis Labyrinthus formation have shown indications of iron-bearing sulfates and phyllosilicate (clay) minerals. (CRISM is another instrument on the Mars Reconnaissance Orbiter.)

HiRISE observations have revealed exposed layers which are possibly the sources of the signatures seen by CRISM. The layering, is visible in the lower part of the image. To the upper left one can see a dune field which covers other beds.

Written by: Nicolas Thomas (7 October 2009)
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Source http://www.uahirise.org/ESP_014353_1685
Author NASA
Other versions Noctis Labyrinthus formation on Mars.jpg

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Public domain This file is in the public domain in the United States because it was solely created by NASA. NASA copyright policy states that "NASA material is not protected by copyright unless noted". (See Template:PD-USGov, NASA copyright policy page or JPL Image Use Policy.)
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current22:56, 27 April 2014Thumbnail for version as of 22:56, 27 April 20142,560 × 1,920 (4.28 MB)Sneeuwschaap (talk | contribs)User created page with UploadWizard

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