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Gullies and... Gullies? in Terra Sirenum (PSP_001697_1390)

Gullies and... Gullies? in Terra Sirenum
Gullies and... Gullies? in Terra Sirenum (PSP_001697_1390)
Credit: NASA/JPL/University of Arizona

Image PSP_001697_1390 shows part of an unnamed crater, itself located inside the much larger Newton Crater, in Terra Sirenum. This unnamed crater is approximately 7 km in diameter (over 4 miles) and some 700 m (760 yards) deep. Numerous gully systems are visible on the east- and south-facing walls of the crater; their characteristics are astonishingly diverse, though.

The image's subset shown here (1223 x 1425 pixels, 2 MB) covers an area of nearly 610 x 740 m (670 x 800 yards). Downhill is toward the bottom of the image, north is up; illumination is from the northwest. This subset depicts several gullies or troughs carved in the southwest-facing wall of the crater.

These troughs are extremely rectilinear, lack tributaries, and do not seem to have terminal fan deposits: they terminate rather abruptly, some of them in a spatula-like shape. Their characteristics contrast sharply with those of gully systems elsewhere in this same crater, which are sinuous, have numerous tributaries, and show distinct fan deposits.

HiRISE is unveiling the large diversity exhibited by Martian gully systems, thanks to its high-resolution, stereo, and color capabilities. The diverse types of gullies observed may have been produced by different mechanisms. Current leading hypotheses explaining the origin of gullies include erosion from seepage or eruption of water from a subsurface aquifer, melting of ground ice, or surface snow; and dry landslides.
Written by: Sara Martinez-Alonso

OBSERVATION TOOLBOX
Acquisition date:06 December 2006 Local Mars time: 3:40 PM
Latitude (centered):-40.8 ° Longitude (East):200.2 °
Range to target site:256.4 km (160.3 miles)Original image scale range:51.3 cm/pixel
(with 2 x 2 binning) so objects ~154 cm across are resolved
Map projected scale:50 cm/pixel and north is upMap projection:EQUIRECTANGULAR
Emission angle:9.0 ° Phase angle:81.6 °
Solar incidence angle:74 °, with the Sun about 16 ° above the horizon Solar longitude:146.3 °, Northern Summer
For non-map projected products:
North azimuth:96 ° Sub-solar azimuth:39.8 °
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 azimuth213.9°

 

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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.