File:016vallesmarineris reduced0.25.jpg
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[edit]Description016vallesmarineris reduced0.25.jpg |
English: A ragged geological scar crosses the belly of Mars. Long enough to reach from New York City to Los Angeles, this great rift in the martian crust is named Valles Marineris, or Mariner Valley. It was discovered in 1972 by the Mariner 9 spacecraft. Formed out of several parallel, connecting troughs, Valles Marineris dwarfs Earth's Grand Canyon in every respect, being wider, longer, deeper, and older. It easily earns the title of Grandest Canyon of All.
This mosaic image of Valles Marineris - colored to resemble the martian surface - comes from the Thermal Emission Imaging System (THEMIS), a visible-light and infrared-sensing camera on NASA's Mars Odyssey orbiter. Mars Odyssey was built by Lockheed Martin and the mission is operated by the Jet Propulsion Laboratory. Built from more than 500 daytime infrared photos, the mosaic shows the whole valley in more detail than any previous composite photo. Despite the valley's huge extent - including its western extension through Noctis Labyrinthus, it reaches some 3,000 kilometers (2,000 miles) long - the smallest details visible in the image are about the size of a football field: 100 meters (328 feet). This is a reduced size (approximately one fourth the linear pixel density) and cropped (at the bottom) version of the original 23,711 x 11,856 pixel THEMIS mosaic, and has also been adjusted in hue and saturation. |
Date | |
Source | http://themis.asu.edu/vallesspecial |
Author | NASA / JPL-Caltech / Arizona State University |
Other versions |
016vallesmarineris reduced0.5.jpg - larger, uncropped version (12,000 × 6,000 pixels, 35.67 MB) |
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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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Date/Time | Thumbnail | Dimensions | User | Comment | |
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current | 06:10, 16 September 2012 | 6,000 × 2,600 (8.88 MB) | WolfmanSF (talk | contribs) | adjust hue, saturation | |
23:16, 15 September 2012 | 6,000 × 2,600 (8.17 MB) | WolfmanSF (talk | contribs) | cropped at bottom | ||
22:30, 15 September 2012 | 6,000 × 3,000 (9.45 MB) | WolfmanSF (talk | contribs) | User created page with UploadWizard |
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This file contains additional information such as Exif metadata which may have been added by the digital camera, scanner, or software program used to create or digitize it. If the file has been modified from its original state, some details such as the timestamp may not fully reflect those of the original file. The timestamp is only as accurate as the clock in the camera, and it may be completely wrong.
Orientation | Normal |
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Horizontal resolution | 72 dpi |
Vertical resolution | 72 dpi |
Software used | Adobe Photoshop Elements 9.0 Windows |
File change date and time | 23:07, 15 September 2012 |
Color space | sRGB |
Image width | 6,000 px |
Image height | 2,600 px |
Date and time of digitizing | 23:32, 14 September 2012 |
Date metadata was last modified | 16:07, 15 September 2012 |
Unique ID of original document | xmp.did:200F98CAC4FFE111A395D7792B1EE82D |
Structured data
Items portrayed in this file
depicts
November 2005
image/jpeg
0bcd31b119d24f63fa399a67182fe660700d4cda
9,314,226 byte
2,600 pixel
6,000 pixel
- Valles Marineris
- Photos of Coprates quadrangle by THEMIS
- Ganges Catena
- Ceti Chasma
- Baetis Chasma
- Hydrae Chasma
- Hydrae Chaos
- Hydrae Cavus
- Ophir Catenae
- Juventae Cavi
- Juventae Chasma
- Dittaino Valles
- Sepik Vallis
- Juventae Dorsa
- Tithoniae Fossae
- Tithoniae Catenae
- Sinai Fossae
- Sinai Dorsa
- Nia Fossae
- Melas Dorsa
- Coprates Catena
- Ophir Cavus
- Ganges Cavus
- Allegheny Vallis
- Ophir Planum