File:Light-Toned Deposits in Noctis Labyrinthus.jpg
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Summary
[edit]DescriptionLight-Toned Deposits in Noctis Labyrinthus.jpg |
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) |
Date | |
Source | http://www.uahirise.org/ESP_014353_1685 |
Author | NASA |
Other versions | Noctis Labyrinthus formation on Mars.jpg |
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[edit]Public domainPublic domainfalsefalse |
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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current | 22:56, 27 April 2014 | 2,560 × 1,920 (4.28 MB) | Sneeuwschaap (talk | contribs) | User created page with UploadWizard |
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Orientation | Normal |
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Horizontal resolution | 72 dpi |
Vertical resolution | 72 dpi |
Software used | Adobe Photoshop CS4 Macintosh |
File change date and time | 13:47, 6 October 2009 |
Color space | sRGB |
Image width | 2,560 px |
Image height | 1,920 px |
Date and time of digitizing | 08:51, 15 September 2009 |
Date metadata was last modified | 06:47, 6 October 2009 |
Unique ID of original document | uuid:183BB7C606F9DD11BA66D1AD63D425C6 |