Intra-Crater Deposits in Nilosyrtis
NASA/JPL/UArizona
Intra-Crater Deposits in Nilosyrtis
PSP_006250_2200  Science Theme: Aeolian Processes
Both ancient and modern deposits within craters in the northern lowlands area of Nilosyrtis are visible in this observation. This crater and its neighbors are partially filled with sediments that display unusual morphologies, having patterned interiors and radial filaments.

The crater centers are occupied by heavily eroded mounds of material that probably once buried the craters in this region. Horizontal layering is visible in similar mounds elsewhere in this image, and close inspection shows that these mounds are covered by rocks, presumably ejecta from distant impacts.

The accumulation of ejecta on their surfaces indicates that the mounds are not recent deposits of dust or sand, but rather are ancient sediments perhaps deposited in a primordial sea. The radial filaments are much more recent deposits, as shown by the lack of ejecta on their surfaces, and are likely made up of dust and sand that is trapped between the older mounds and the crater walls.



Written by: Paul Geissler  (16 January 2008)
 
Acquisition date
26 November 2007

Local Mars time
14:10

Latitude (centered)
39.594°

Longitude (East)
89.515°

Spacecraft altitude
296.7 km (184.4 miles)

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from 29.7 cm/pixel (with 1 x 1 binning) to 59.4 cm/pixel (with 2 x 2 binning)

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25 cm/pixel and North is up

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Equirectangular

Emission angle
0.3°

Phase angle
52.2°

Solar incidence angle
52°, with the Sun about 38° above the horizon

Solar longitude
353.3°, Northern Winter

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North azimuth:  97°
Sub-solar azimuth:  318.6°
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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.