Uplift in Oudemans Crater
NASA/JPL/University of Arizona
Uplift in Oudemans Crater
ESP_011966_1700  Science Theme: Geologic Contacts/Stratigraphy
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Oudemans Crater is about 120 kilometers in diameter and it is located in western Valles Marineris just to the south of Noctis Labyrinthus.

Light-toned layering is visible in the central peak which represents material brought up from substantial depth (greater than 6 km) and provide evidence for older deposits buried beneath the lava flows of the Hesperian-aged plains.

In this HiRISE image, which is located to the east of the central peak but along the floor of the crater, numerous hills are visible. The subimage reveals layered rocks in the hills that are tilted so that they stand almost vertically. The rocks were originally laid down horizontally so the force and uplift during formation of the crater peaks caused sections of the rocks to be broken apart and rotated.

Written by: Cathy   (9 March 2009)

This is a stereo pair with ESP_012467_1700.

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Acquisition date
13 February 2009

Local Mars time:
15:47

Latitude (centered)
-9.733°

Longitude (East)
268.624°

Range to target site
258.7 km (161.7 miles)

Original image scale range
25.9 cm/pixel (with 1 x 1 binning) so objects ~78 cm across are resolved

Map projected scale
25 cm/pixel and North is up

Map projection
Equirectangular

Emission angle:
2.5°

Phase angle:
58.4°

Solar incidence angle
56°, with the Sun about 34° above the horizon

Solar longitude
209.4°, Northern Autumn

North azimuth:
97°

Sub-solar azimuth:
357.1°
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ANAGLYPHS
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Full resolution JP2 download
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ADDITIONAL INFORMATION
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Color label
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Merged RGB label
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HiView

NB
IRB: infrared-red-blue
RGB: red-green-blue
About color products (PDF)

Black & white is 5 km across; enhanced color about 1 km
For scale, use JPEG/JP2 black & white map-projected images



USAGE POLICY
All of the images produced by HiRISE and accessible on this site are within the public domain: there are no restrictions on their usage by anyone in the public, including news or science organizations. We do ask for a credit line where possible:
NASA/JPL/University of Arizona



Postscript
For information about NASA and agency programs on the Web, visit: http://www.nasa.gov. NASA's Jet Propulsion Laboratory, a division of the California Institute of Technology in Pasadena, Calif., manages the Mars Reconnaissance Orbiter for NASA's Science Mission Directorate, Washington. Lockheed Martin Space Systems is the prime contractor for the project and built the spacecraft. The HiRISE camera was built by Ball Aerospace and Technology Corporation and is operated by the University of Arizona. The image data were processed using the U.S. Geological Survey’s ISIS3 software.