PIA09709: Very Fine Layers in Juventae Chasma
 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 4657 pixels (w x h)
 Produced By:  University of Arizona/HiRISE-LPL
 Full-Res TIFF:  PIA09709.tif (9.547 MB)
 Full-Res JPEG:  PIA09709.jpg (824.5 kB)

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This HiRISE image (PSP_002590_1765) shows a portion of the light-toned layered deposits in Juventae Chasma.

Juventae Chasma is a large trough just north of the main part of Valles Marineris, and may have been the source region for giant floods long ago. There are currently several large hills of layered rock on the chasma floor, likely remnants of a deposit which was once more extensive. Among the possible origins of the layered deposits are lake sediments, volcanic material of various origins (possibly erupted under ice), or deposits of aeolian sand and dust.

The subimage shows some extremely thin beds within one of the mounds (center). These are probably sheets of material lying nearly flat, and are some of the finest-scale layers observed on Mars. It is possible that in places layer boundaries are accentuated by variable amounts of dark wind-blown dust, which buries the layers in some parts of the image; nevertheless, some of the layering must be extremely thin.

The layers are actually even more thin than they appear, since the slope of the mound makes them appear wider. The occurrence of many thin layers indicates many events or variations in deposition while this material was forming.

Observation Toolbox
Acquisition date: 2 February 2007
Local Mars time: 3:43PM
Degrees latitude (centered): -3.3
Degrees longitude (East): 298.3
Range to target site: 266.8 km (166.7 miles)
Original image scale range: 26.7 cm/pixel (with 1 x 1 binning) so objects ~80 cm across are resolved
Map-projected scale: 25 cm/pixel and north is up
Emission angle: 2.4
Phase angle: 53.6
Solar incidence angle: 56, with the Sun about 34 above the horizon
Solar longitude: 183.7, 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

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