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PIA12881: Gullies and... Gullies? in Terra Sirenum
 Target Name:  Mars
 Is a satellite of:  Sol (our sun)
 Mission:  Mars Reconnaissance Orbiter (MRO)
 Spacecraft:  Mars Reconnaissance Orbiter (MRO)
 Instrument:  HiRISE
 Product Size:  2560 x 1920 pixels (w x h)
 Produced By:  University of Arizona/HiRISE-LPL
 Other  
Information: 
Other products from image PSP_001697_1390
 Full-Res TIFF:  PIA12881.tif (14.76 MB)
 Full-Res JPEG:  PIA12881.jpg (717.4 kB)

Click on the image above to download a moderately sized image in JPEG format (possibly reduced in size from original)

Original Caption Released with Image:

Click here for larger version of figure 1 for PIA12881
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This observation shows part of an unnamed crater, itself located inside the much larger Newton Crater, in Terra Sirenum. This unnamed crater is approximately 7 kilometers in diameter (over 4 miles) and some 700 meters (760 yards) deep.

Numerous gully systems are visible on the east- and south-facing walls of the crater; their characteristics are astonishingly diverse.

The subimage (Figure 1) covers an area of nearly 610 x 740 meters (670 x 800 yards). Downhill is toward the bottom of the image, north is up; illumination is from the northwest. This subimage 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.

The University of Arizona, Tucson, operates the HiRISE camera, which was built by Ball Aerospace & Technologies Corp., Boulder, Colo. NASA's Jet Propulsion Laboratory, a division of the California Institute of Technology, Pasadena, manages the Mars Reconnaissance Orbiter for the NASA Science Mission Directorate, Washington. Lockheed Martin Space Systems, Denver, is the spacecraft development and integration contractor for the project and built the spacecraft.

Image Credit:
NASA/JPL-Caltech/University of Arizona

Image Addition Date:
2010-03-03