Inverted Riverbed in Gale Crater
NASA/JPL/University of Arizona
Inverted Riverbed in Gale Crater
PSP_009149_1750  Science Theme: Fluvial Processes
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Gale Crater is a large, approximately 152 kilometer-diameter impact crater that lies near the Martian equator. Contained within the crater is a massive central mound of layered material. With an average vertical thickness of almost 4 km (2.4 miles), the Gale Crater layered deposits are twice as thick as the layers exposed along the Grand Canyon on Earth.

Shown here is a portion of the mound with an inverted fluvial or river channel. Topographic inversion occurs when sediments are cemented together, forming a harder layer that is resistant to later erosion. This later erosion has preferentially removed material outside the channel, leaving the former riverbed exposed as a ridge—a topographic high. This inverted channel was originally detected by scientists using Mars Orbiter Camera (MOC) images onboard the Mars Global Surveyor spacecraft.

Color variations visible in this image are mostly due to variable amounts of loose dark sediment that has accumulated unevenly across the scene.

Written by: Brad Thomson   (5 September 2008)

This is a stereo pair with PSP_009294_1750.

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Acquisition date
09 July 2008

Local Mars time:
15:28

Latitude (centered)
-4.799°

Longitude (East)
137.412°

Range to target site
276.4 km (172.8 miles)

Original image scale range
27.7 cm/pixel (with 1 x 1 binning) so objects ~83 cm across are resolved

Map projected scale
25 cm/pixel and North is up

Map projection
Equirectangular

Emission angle:
14.0°

Phase angle:
48.7°

Solar incidence angle
59°, with the Sun about 31° above the horizon

Solar longitude
96.3°, Northern Summer

North azimuth:
95°

Sub-solar azimuth:
38.2°
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ANAGLYPHS
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DIGITAL TERRAIN MODEL (DTM)
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ADDITIONAL INFORMATION
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HiView

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IRB: infrared-red-blue
RGB: red-green-blue
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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.