PIA24911: When Did the Light-Toned Layers Form?
 Target Name:  Mars
 Is a satellite of:  Sol (our sun)
 Mission:  Mars Reconnaissance Orbiter (MRO)
 Spacecraft:  Mars Reconnaissance Orbiter (MRO)
 Instrument:  HiRISE
 Product Size:  2880 x 1800 pixels (w x h)
 Produced By:  University of Arizona/HiRISE-LPL
Other products from ESP_070107_1750
 Full-Res TIFF:  PIA24911.tif (15.55 MB)
 Full-Res JPEG:  PIA24911.jpg (927.2 kB)

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Light-toned layered deposits are found throughout central Valles Marineris. Most of the deposits tend to be towards the center of the depressions, away from the walls that define our solar system's largest canyon.

In this image of northwestern Candor Chasma, the light-toned layered deposits are adjacent to the walls. If the deposits are on top of the walls, then we know they were laid down after the chasma had already formed. However, if they are outcropping from within the walls, then they are older deposits that pre-date the chasma's formation.

Determining when the light-toned layered deposits formed is important for understanding the geologic history of Valles Marineris, especially because these deposits are hydrated and most likely formed in the presence of liquid water.

The map is projected here at a scale of 25 centimeters (9.8 inches) per pixel. (The original image scale is 26.6 centimeters [10.5 inches] per pixel [with 1 x 1 binning]; objects on the order of 53.3 centimeters [21.0 inches] across are resolved.) North is up.

The University of Arizona, in Tucson, operates HiRISE, which was built by Ball Aerospace & Technologies Corp., in Boulder, Colorado. NASA's Jet Propulsion Laboratory, a division of Caltech in Pasadena, California, manages the Mars Reconnaissance Orbiter Project for NASA's Science Mission Directorate, Washington.

Image Credit:
NASA/JPL-Caltech/University of Arizona

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