This image acquired on July 11, 2021 by NASAs Mars Reconnaissance Orbiter, shows light-toned layered deposits adjacent to the walls of northwestern Candor Chasma.

September 29, 2021

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Slope streaks are common in the tropics of Mars. Once thought to be caused by flowing water, most scientists now believe that they are avalanches of dust. They are typically darker than their surroundings and often fan outwards downslope. This suggests that the dust sediment is sticky, so that the avalanche broadens as it flows downhill.

Slope streaks are known to fade over time, but the slope streaks at this monitoring site in Arabia Terra go beyond that. Here, old slope streaks appear to be brighter than the surrounding terrain. A comparison between HiRISE images taken in 2008 and in 2019 shows very few changes in the dark and bright streaks.

We can see three new dark streaks in our more recent image. These were the only changes spotted among the hundreds of streaks observed in the monitoring site, suggesting that new streak formation and fading take place on time scales of at least decades.

The map is projected here at a scale of 50 centimeters (19.7 inches) per pixel. (The original image scale is 55.6 centimeters [21.9 inches] per pixel [with 2 x 2 binning]; objects on the order of 167 centimeters [65.7 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.

Credit

NASA/JPL-Caltech/University of Arizona

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