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Dust Devil Etch-A-Sketch
NASA/JPL/University of Arizona

Dust Devil Etch-A-Sketch
ESP_013751_1115  Science Theme: Landscape Evolution
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This “etch-a-sketch” appearance indicates the presence of dust devil activity in the Thyles Rupes region of Mars.

The dark streaks are a result of a surface-atmosphere interaction that creates thermally-driven vortices. These Martian vortices are giant dust devils that “vacuum” the bright surface dust revealing the darker subsurface rock.

This image was taken in the late southern summer and shows that the dust devil direction of movement changes with the winds as the season progresses from spring to fall. Dust devils are sensitive to changes in low-speed ambient winds and will follow the dominant daytime wind direction.

The direction of the vortex is visible by the scallop pattern that is left behind as a dust devil will erase the front part of the circular track as it follows the wind.

Written by: Circe Verba   (19 August 2009)



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Acquisition date:02 July 2009 Local Mars time: 2:50 PM
Latitude (centered):-68.5 degrees Longitude (East):145.0 degrees
Range to target site:251.0 km (156.9 miles)Original image scale range:50.2 cm/pixel (with 2 x 2 binning) so objects ~151 cm across are resolved
Map projected scale:50 cm/pixelMap projection:POLAR STEREOGRAPHIC
Emission angle:6.8 degrees Phase angle:57.9 degrees
Solar incidence angle:53 degrees, with the Sun about 37 degrees above the horizon Solar longitude:296.3 degrees, Northern Winter
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North azimuth:97 degrees Sub-solar azimuth:45.4 degrees
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North azimuth:55.02 degreesSub solar azimuth:3.319 degrees

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