Layered Deposits in Becquerel Crater
NASA/JPL/University of Arizona
Layered Deposits in Becquerel Crater
PSP_004078_2015  Science Theme: Tectonic Processes
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This image shows light-toned layered deposits along the floor of Becquerel Crater, an impact crater in Arabia Terra. The deposits consist of stacked, repeating layers which consistently appear to be only a few meters thick. The surface of the deposits also appears to be cracked into blocks a meter or so in length.

Layered deposits, such as these, form from sediments once deposited within the crater. Possible origins for the sediments include windblown debris, volcanic ash falling from the sky, or sediments that accumulated in a lake on the crater floor. The regular thickness of the layers suggests that they were most likely deposited in a water environment or by wind in a cyclic process.

Some of the layering has a dark appearance that produces an alternating bright-dark “zebra” banding. This may be the result of a thin surface layer of coarser and darker basalt sand collected on the more level surfaces, rather than indicating compositional differences in the eroded layered beds. Faults can also be seen displacing portions of the layered bed. An example of this can be seen just left of center in the bottom half of the subimage. The faulting indicates that the deposits have experienced disruption since their emplacement.

Written by: Maria Banks   (25 June 2007)

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Acquisition date
10 June 2007

Local Mars time:
15:05

Latitude (centered)
21.305°

Longitude (East)
352.002°

Range to target site
287.6 km (179.8 miles)

Original image scale range
28.8 cm/pixel (with 1 x 1 binning) so objects ~86 cm across are resolved

Map projected scale
25 cm/pixel and North is up

Map projection
Equirectangular

Emission angle:
8.8°

Phase angle:
57.3°

Solar incidence angle
64°, with the Sun about 26° above the horizon

Solar longitude
254.7°, Northern Autumn

North azimuth:
97°

Sub-solar azimuth:
322.3°
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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.