 Spectacular Gullies Near Gorgonum Chaos (PSP_003583_1425) Credit: NASA/JPL/University of Arizona
PSP_003583_1425 shows incredible details of a crater with gullies that provides strong evidence for gully formation involving fluid flow.
Of note is the variety of gully morphologies along the crater walls. The north and west walls have gullies, while the south wall has only landslides. "Mass wasting" is the more general term geologists use to describe landslides, slumps, and other movements of the ground in response to gravity. It usually occurs on steep slopes when the force of gravity causes weak or loose material to travel downslope. Mass wasting produces structures that are sometimes similar to gully channels, but which can usually be distinguished by their occurrence
on steep slopes.
The gullies on the north wall have eroded all the way to the crater rim. They appear older than other nearby gullies because they have existed long enough to be modified by permafrost processes as evidenced by the polgyonal fractures found on some of the channel and inter-gully walls. Another noticeable difference among the gullies is channel lengths. The gullies on the north wall and the group just to the left of these have much shorter channels than the gullies on the northwest wall. It is possible that the gullies with shorter channels had less fluid flow through their systems. The gullies appear to originate around a sequence of rocky layers near the crater rim.
Many of the gully channels appear to have boulders littered throughout (see subimage, approximately 640 m across; 2550 x 2000, 14MB). This is suggestive of a fluid flowing in these channels; a fluid would preferentially transport smaller particles and leave behind the larger ones, such as the boulders seen here. There are many overprinted small channels in each gully, as can be seen in the subimage. These are indicative of multiple flow events such that some channels experience flow, then are abandoned.
The subimage also shows several channels merging. Particularly interesting is the channel flowing from the top of the scene. There are several intertwining channels that merge into one just to the right of the center of the subimage. However, the way some channels truncate others suggests that there were at least three episodes of flow through this area.
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OBSERVATION TOOLBOX
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| Acquisition date: | 02 May 2007 |
Local Mars time: | 3:33 PM |
| Latitude (centered): | -37.1 ° |
Longitude (East): | 191.9 ° |
| Range to target site: | 257.0 km (160.6 miles) | Original image scale range: | 25.7 cm/pixel
(with 1 x 1 binning) so objects ~77 cm across are resolved | | Map projected scale: | 25 cm/pixel and north is up | Map projection: | EQUIRECTANGULAR | | Emission angle: | 9.4 ° |
Phase angle: | 58.8 ° | | Solar incidence angle: | 50 °, with the Sun about 40 ° above the horizon |
Solar longitude: | 230.3 °, Northern Autumn |
| For non-map projected products: | | North azimuth: | 97 ° |
Sub-solar azimuth: | 10.5 ° |
| For map projected products: | | North azimuth: | 270° | Sub solar azimuth | 185.879° |
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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.
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