Small Crater on Arcuate Ridge West of Olympia Mensae
NASA/JPL/University of Arizona

Small Crater on Arcuate Ridge West of Olympia Mensae
PSP_009717_2545  Science Theme: Impact Processes
Italiano  Greek


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This image features arcuate ridges in the high northern plains. It has been suggested that arcuate ridges were formed by ancient glaciers on Mars.

The plains surrounding the arcuate ridges have two textures. The plains on the left half of the image have linear streaks trending from the top to the bottom. These might have been caused by wind moving material. The plains on the right side have more of a pitted texture that was probably caused by the removal of ground ice.

There are two craters in the center of the image. One formed on top of a ridge, while the other (faint circular feature) appears to be getting exposed by erosion.

Written by: Kelly Kolb   (17 December 2008)



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Acquisition date:22 August 2008 Local Mars time: 2:53 PM
Latitude (centered):74.3 degrees Longitude (East):93.7 degrees
Range to target site:314.9 km (196.8 miles)Original image scale range:31.5 cm/pixel (with 1 x 1 binning) so objects ~95 cm across are resolved
Map projected scale:25 cm/pixelMap projection:POLAR STEREOGRAPHIC
Emission angle:1.9 degrees Phase angle:55.2 degrees
Solar incidence angle:57 degrees, with the Sun about 33 degrees above the horizon Solar longitude:116.3 degrees, Northern Summer
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North azimuth:101 degrees Sub-solar azimuth:328.7 degrees
For map-projected products
North azimuth:176.3 degreesSub solar azimuth:45.87 degrees

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