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Layers in Galle Crater (PSP_002655_1280)

Layers in Galle Crater
Layers in Galle Crater (PSP_002655_1280)
Credit: NASA/JPL/University of Arizona

This image shows part of a large mass of layered rock in Galle Crater, in the southern cratered highlands of Mars.

At low resolution, layers appear as bands and swirls which are nearly horizontal. This causes them to interact dramatically with topography, producing the appearance of folds and loops wrapping around small hills much like lines on a contour map. Zooming in at higher resolution, some long cracks (hundreds of meters long) are cutting across the layers, generally trending northeast-southwest.

At full resolution, details of the layers are often obscured by ripples of wind-blown dust or textured patterns of erosion now eroding the rock. In the best exposures, such as that in the cutout section (2196x1442, 3 MB) the layers are fractured into blocks. Some of the layers are relatively resistant, and appear as ridges or fins in the cutout, often with little material supporting them from below. Although this seems to indicate relatively strong, coherent material, few boulders are visible. The ridge-forming layers may be weak, but separated by material with virtually no cohesion.

Polygonal fracture patterns in the dark regolith between distinct layers could be due to ground ice, or regional tectonic stresses.
Written by: Colin Dundas

OBSERVATION TOOLBOX
Acquisition date:19 February 2007 Local Mars time: 3:54 PM
Latitude (centered):-51.8 ° Longitude (East):330.0 °
Range to target site:256.3 km (160.2 miles)Original image scale range:25.6 cm/pixel
(with 1 x 1 binning) so objects ~77 cm across are resolved
Map projected scale:25 cm/pixel and north is upMap projection:EQUIRECTANGULAR
Emission angle:2.9 ° Phase angle:71.5 °
Solar incidence angle:69 °, with the Sun about 21 ° above the horizon Solar longitude:186.6 °, Northern Autumn
For non-map projected products:
North azimuth:96 ° Sub-solar azimuth:28.7 °
F O R   M A P   P R O J E C T E D   P R O D U C T S
North azimuth:270°Sub solar azimuth203.0°
A N A G L Y P H   P R O D U C T S
Right observation:PSP_003156_1280Convergence angle18.3°

 

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Sedimentary/Layering Processes

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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: Image: NASA/JPL/University of Arizona


P O S T S C R I P T

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.