Bouncing Boulder Blocks a Slope Streak
NASA/JPL-Caltech/UArizona
Bouncing Boulder Blocks a Slope Streak
ESP_014394_2045  Science Theme: Mass Wasting Processes
A boulder track is visible in the center of this subimage.

The track formed on the sloping wall of an impact crater when a rock bounced or rolled downhill leaving behind marks on the surface. In the full image, you can see its whole path, starting from a cliff to the east, from which it presumably originated. The boulder itself is visible as a brighter rock in the middle of the dark slope streak, where it finally came to a halt.

Slope streaks begin at a point, and it only takes a small disturbance at that point to initiate the streak, such as a dust devil or an impact crater. We have seen these streaks appear before, so this is an ongoing process on Mars. The streaks tend to start out dark and fade as they get older; we have even seen some that are lighter in color than their surroundings. Scientists think these are caused by dry avalanches of dust or sand falling downhill, revealing darker material underneath. The streaks are very shallow and don't appear to disturb pre-existing features on the surface, like ripples, or in this case, the boulder tracks. This case is particularly interesting because the slope streak appears to have flowed around the boulder, leaving a patch of brighter material undisturbed in the lee of the rock. From this relationship, you can tell that the boulder must have fallen before the slope streak formed.

For scale, the boulder is about 6 meters (approximately 20 feet) across, and the dark streak is about 125 meters (approximately 400 feet) wide at its widest point.

Thanks to the sharp-eyed HiRISE fan Daniel who brought this image to our attention!

Written by: Ingrid Daubar Spitale  (14 October 2009)
 
Acquisition date
22 August 2009

Local Mars time
14:13

Latitude (centered)
24.355°

Longitude (East)
217.602°

Spacecraft altitude
284.4 km (176.7 miles)

Original image scale range
57.6 cm/pixel (with 2 x 2 binning) so objects ~173 cm across are resolved

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50 cm/pixel and North is up

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Equirectangular

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8.8°

Phase angle
44.0°

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50°, with the Sun about 40° above the horizon

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325.4°, Northern Winter

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Sub-solar azimuth:  319.5°
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POSTSCRIPT
NASA’s Jet Propulsion Laboratory, a division of the California Institute of Technology in Pasadena, Calif., manages the Mars Reconnaissance Orbiter for NASA’s Science Mission Directorate, Washington. The HiRISE camera was built by Ball Aerospace and Technology Corporation and is operated by the University of Arizona.