Layers in a Central Mound in Gale Crater
NASA/JPL/University of Arizona
Layers in a Central Mound in Gale Crater
PSP_001422_1750  Science Theme: Sedimentary/Layering Processes


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This image shows a portion of the central mound in the impact crater Gale that is of interest to scientists because it is composed of light-toned layered deposits.

The layered deposits could have formed in a water environment if a lake once filled the crater. Alternatively, particles suspended in the atmosphere, such as dust or volcanic ash, could have built up the layers over time.

By using HiRISE images to see details in the layers, such as how their thicknesses vary horizontally and vertically, scientists can narrow down the potential origins.

The paucity of impact craters on the layered deposits indicates that either the deposits are very young, or more likely that they are being eroded to remove these craters. Wind erosion has modified the layers after they formed, creating both sharp corners and rounded depressions along the surface. Meter-size boulders are visible at the base of steep cliffs, but the scarcity of boulders elsewhere suggests most of the erosion is occurring by the wind rather than downslope movement of material.

Written by: Cathy Weitz   (11 December 2009)

This is a stereo pair with PSP_001620_1750.

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Acquisition date:15 November 2006 Local Mars time:15:31
Latitude (centered):-4.986° Longitude (East):137.741°
Range to target site:262.4 km (164.0 miles)Original image scale range:26.2 cm/pixel (with 1 x 1 binning) so objects ~79 cm across are resolved
Map projected scale:25 cm/pixel and North is upMap projection:Equirectangular
Emission angle:2.2° Phase angle:58.6°
Solar incidence angle:57°, with the Sun about 33° above the horizon Solar longitude:135.6°, Northern Summer

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