Inverted Topography near Juventae Chasma
NASA/JPL/University of Arizona

Inverted Topography near Juventae Chasma
ESP_020602_1755  Science Theme: Fluvial Processes
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This image displays several nice examples of inverted channels near Juventae Chasma, part of the Valles Marineris system.

Inverted topography - when a feature that ordinarily would be lower in elevation than the surrounding terrain is instead higher in elevation - forms when low-lying features are filled with erosion-resistant materials (like lava, large rocks or cemented sediments). The softer surrounding material is more easily eroded, which results in the filled-in feature becoming a high spot instead of a dip.

In this image, the inverted relief preserves sinuous branching features, possibly ancient streambeds. And while it isn't exactly inverted topography, several of the craters in the image also seem to have been subject to a similar process - the erosion-resistant ejecta blankets stand higher than the surrounding terrain, forming an abrupt transition at the edge of the ejecta.

Written by: Nicole Baugh   (12 January 2011)

This is a stereo pair with PSP_005346_1755.

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Acquisition date:18 December 2010 Local Mars time: 3:44 PM
Latitude (centered):-4.290° Longitude (East):296.453°
Range to target site:274.3 km (171.4 miles)Original image scale range:27.4 cm/pixel (with 1 x 1 binning) so objects ~82 cm across are resolved
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