Layered Deposits in Aureum Chaos
NASA/JPL/UArizona
Layered Deposits in Aureum Chaos
PSP_002892_1760  Science Theme: Sedimentary/Layering Processes
This observation shows an outcrop of a large slab of layered deposits in Aureum Chaos.

Chaotic terrains on Mars are disorganized regions of blocks and large mounds which appear to have been produced by the collapse of pre-existing terrain. They are often associated with giant outflow channels, and they may have been the source of the water that carved the channels. This link is an important part of understanding the history of water on Mars. One way to address this is to study the rocks left behind in the chaotic terrains.

The outcrop in this subimage is several kilometers across and light-toned. It has a slab-like appearance, with relatively steep edges and a flat top, although the top has many small knobs and spires. In places, particularly along the left (west) edge of the main slab, it is clear that the light material is composed of many fine layers, which are eroding in a stepped fashion due to the variable resistance of the layers. The flat surface of the outcrop is partially coated with dark dust, obscuring its light tone.

Along the edges, the outcrop is breaking into boulders and eroding away, but it is strong enough that it preserves steep slopes, particularly on the eastern edge.

Away from the large slab, the image consists of hills and mounds characteristic of chaotic terrain. Little detail is visible on the mounds. The low areas have been partially covered by wind-blown sand or dust, forming the pervasive ripples seen in the image. Light material can be seen under the ripples in a few places, indicating that the light layered deposits extend farther than just the slab.



Written by: Colin Dundas  (11 April 2007)

This is a stereo pair with PSP_003525_1760.
 
Acquisition date
09 March 2007

Local Mars time
15:42

Latitude (centered)
-4.009°

Longitude (East)
333.141°

Spacecraft altitude
269.1 km (167.2 miles)

Original image scale range
53.8 cm/pixel (with 2 x 2 binning) so objects ~162 cm across are resolved

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50 cm/pixel and North is up

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Equirectangular

Emission angle
0.0°

Phase angle
55.5°

Solar incidence angle
56°, with the Sun about 34° above the horizon

Solar longitude
197.3°, Northern Autumn

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Sub-solar azimuth:  0.1°
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POSTSCRIPT
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. The HiRISE camera was built by Ball Aerospace and Technology Corporation and is operated by the University of Arizona.