Layered Rocks in Orson Welles Crater
NASA/JPL/University of Arizona
Layered Rocks in Orson Welles Crater
PSP_008391_1790  Science Theme: Sedimentary/Layering Processes
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This image shows part of the floor of Orson Welles Crater, an old impact crater now connected with the Shalbatana Valles outflow channel. Part of the floor of the crater is comprised of large hummocks comparable to those found in other “chaotic terrain” on Mars; such areas are often the sources of giant flood channels.

Examined closely, the light-toned areas consist of finely-layered materials, partially buried by dark mantling material and sand dunes. Such light-toned rocks are found at a number of sites on Mars and are thought to be sedimentary. Notable color variations occur in the rocks may be a result of different compositions.

In addition to the varying light and dark bands, some of the rocks appear pale blue in the false color image while others have a yellowish tone. Another sign of variation in the rocks is the way some layers seem to form benches, while others have steep edges. This indicates that layers have different strengths, and that whatever process formed these rocks varied during deposition of the layers.

The origin of such light, layered rocks on Mars is still uncertain and probably variable. Some may be wind-deposited sandstone, like that at the MER Opportunity landing site while other outcrops could be volcanic ash like that at the MER Spirit landing site. Others may be lakebed deposits. Unraveling the history of these rocks helps provide a window into events in the Martian past.



Written by: Colin Dundas  (16 July 2008)

This is a stereo pair with ESP_028566_1790.
 
Acquisition date
11 May 2008

Local Mars time
15:11

Latitude (centered)
-0.975°

Longitude (East)
313.955°

Spacecraft altitude
272.0 km (169.1 miles)

Original image scale range
27.4 cm/pixel (with 1 x 1 binning) so objects ~82 cm across are resolved

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25 cm/pixel and North is up

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Emission angle
6.4°

Phase angle
57.7°

Solar incidence angle
53°, with the Sun about 37° above the horizon

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70.3°, Northern Spring

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Sub-solar azimuth:  36.7°
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POSTSCRIPT
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. The HiRISE camera was built by Ball Aerospace and Technology Corporation and is operated by the University of Arizona.