Fresh Crater with Gullies
NASA/JPL/University of Arizona
Fresh Crater with Gullies
PSP_004060_1440  Science Theme: Impact Processes
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This observation shows a fresh, approximately 7.5 kilometer diameter crater that resides in a larger crater in the Southern hemisphere.

The crater shown here has very few craters superposed on it, which attests to its youth. It also has very steep slopes and a sharp rim; more evidence of its young age. Young, fresh craters are of interest on Mars because they help place constraints on the rate at which new impact craters and other young features have formed in recent times.

This fresh crater is particularly interesting because it contains gullies. Gullies are slope features that are proposed to require some amount of liquid water to form. The gullies must have formed after the crater did, which means that if liquid water was involved in the formation of these gullies, then it existed on the surface of Mars more recently. The existence of recent liquid water is especially important in terms of the search for life on Mars and its future exploration.

Several of the gullies show features such as terraces, discontinuous channels, and abandoned channels. All of this implies that more than one flow event occurred. It is unknown whether or not such multiple flows would have been closely spaced in time.

Terraces are thought to indicate past flow levels. Discontinuous channels may represent some subsurface flow in addition to surface flow, or they may be channels that were once continuous that have since been filled in with wind-blown sediment and dust. The latter is the most likely in the subimage. For example, see the discontinuous channel near the center; it appears to have sediment infilling it. Abandoned channels are paths that fluid flowed through in the past before another flow took a different direction.

Written by: Kelly Kolb   (27 October 2010)

This is a stereo pair with PSP_005550_1440.

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Acquisition date
08 June 2007

Local Mars time:
15:13

Latitude (centered)
-35.722°

Longitude (East)
129.426°

Range to target site
254.8 km (159.2 miles)

Original image scale range
25.5 cm/pixel (with 1 x 1 binning) so objects ~76 cm across are resolved

Map projected scale
25 cm/pixel and North is up

Map projection
Equirectangular

Emission angle:
5.2°

Phase angle:
48.2°

Solar incidence angle
43°, with the Sun about 47° above the horizon

Solar longitude
253.8°, Northern Autumn

North azimuth:
96°

Sub-solar azimuth:
7.4°
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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:
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.