PIA09401: Lobate Debris Apron in Tempe Terra/Mareotis Fossae
Target Name: Mars
Is a satellite of: Sol (our sun)
Mission: Mars Reconnaissance Orbiter (MRO)
Spacecraft: Mars Reconnaissance Orbiter (MRO)
Instrument: HiRISE
Product Size: 2048 x 2611 pixels (width x height)
Produced By: University of Arizona/HiRise-LPL
Full-Res TIFF: PIA09401.tif (5.353 MB)
Full-Res JPEG: PIA09401.jpg (670.8 kB)

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Original Caption Released with Image:

This image shows a portion of a large lobate debris apron along the bottom of a hill in the Tempe Terra/Mareotis Fossae region of Mars. Debris aprons were first discovered in regions of "fretted terrain" from analyses of images sent back by the Viking Orbiter spacecrafts in the 1970s. Features in areas of fretted terrain appear "softened" as if some geologic process(es) had smoothed and rounded features that normally would be sharply defined, such the crest of a narrow, steep ridge. Scientists inferred that the processes causing this degradation must have involved the incorporation and creep of ice in the surface materials. If so, these mixtures of ice and debris could have flowed away from topographically high areas leaving features much less sharply-defined. The flow behavior described here is similar to slow-moving glacial or permafrost features on Earth. The debris apron in the upper left of the image also has several subtle "ridge" features on its surface from low sun illumination. The ridges are roughly parallel to the base of the hill and their shapes mimic one another along their lengths. Similar ridges are seen on other debris aprons in this region where the aprons are located directly below large piles of debris accumulating along the bottom of hillslopes. These observations have led to the hypothesis that ridges on debris aprons are accumulated piles of debris from a period of abnormally high erosion. If this was indeed the case, each ridge may indicate a change in the climate or local environment that would have implications for our overall understanding of the Martian climate.

Image PSP_001390_2290 was taken by the High Resolution Imaging Science Experiment (HiRISE) camera onboard the Mars Reconnaissance Orbiter spacecraft on November 12, 2006. The complete image is centered at 48.9 degrees latitude, 283.9 degrees East longitude. The range to the target site was 300.6 km (187.9 miles). At this distance the image scale ranges from 30.1 cm/pixel (with 1 x 1 binning) to 60.1 cm/pixel (with 2 x 2 binning). The image shown here has been map-projected to 25 cm/pixel and north is up. The image was taken at a local Mars time of 3:20 PM and the scene is illuminated from the west with a solar incidence angle of 51 degrees, thus the sun was about 39 degrees above the horizon. At a solar longitude of 134.4 degrees, the season on Mars is Northern Summer.

NASA's Jet Propulsion Laboratory, a division of the California Institute of Technology in Pasadena, manages the Mars Reconnaissance Orbiter for NASA's Science Mission Directorate, Washington. Lockheed Martin Space Systems, Denver, is the prime contractor for the project and built the spacecraft. The High Resolution Imaging Science Experiment is operated by the University of Arizona, Tucson, and the instrument was built by Ball Aerospace and Technology Corp., Boulder, Colo.

Image Credit:
NASA/JPL/Univ. of Arizona

Image Addition Date:
2006-12-13