HiRISE: High Resolution Imaging Science ExperimentThe University of Arizona
Home  New Images  Catalog  Anaglyphs  Stereo Pairs  Science in Motion  FAQ  HiBLOG  Themes  Software  Contact  Search


Bouncing Boulder Blocks a Slope Streak (ESP_014394_2045)

Bouncing Boulder Blocks a Slope Streak
Bouncing Boulder Blocks a Slope Streak (ESP_014394_2045)
Credit: NASA/JPL/University of Arizona

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, 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

OBSERVATION TOOLBOX
Acquisition date:22 August 2009 Local Mars time: 2:13 PM
Latitude (centered):24.4 ° Longitude (East):217.6 °
Range to target site:287.7 km (179.8 miles)Original image scale range:57.6 cm/pixel
(with 2 x 2 binning) so objects ~173 cm across are resolved
Map projected scale:50 cm/pixel and north is upMap projection:EQUIRECTANGULAR
Emission angle:8.8 ° Phase angle:44.0 °
Solar incidence angle:50 °, with the Sun about 40 ° above the horizon Solar longitude:325.4 °, Northern Winter
For non-map projected products:
North azimuth:96 ° Sub-solar azimuth:318.9 °
F O R   M A P   P R O J E C T E D   P R O D U C T S
North azimuth:270°Sub solar azimuth134.8°

 

....................

SCIENCE THEME
Mass Wasting Processes

IMAGE PRODUCT INFORMATION
Grayscale label description
Color product label
EDR products


SUBIMAGES IN THIS OBSERVATION
[stunning subimage]
(9MB)



RESOURCES
About color products (PDF)
IAS Viewer help
HiRISE Online Image Viewer

WALLPAPER
800x600
1024x768
1152x864
1280x960
1440x1080
1600x1200
1920x1440
2048x1536
2560x1600


REFERENCE SHEET
PDF Reference Sheet


HiFLYER
HiFlyer 11 x 17 inches
PDF, 11x17, 3MB



Share on Facebook


TRANSLATE

U S A G E   P O L I C Y

All of the images produced by HiRISE and accessible on this site are within the public domain: there are no restrictions on their usage by anyone in the public, including news or science organizations. We do ask for a credit line where possible: Image: NASA/JPL/University of Arizona


P O S T S C R I P T

For information about NASA and agency programs on the Web, visit: http://www.nasa.gov. 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. Lockheed Martin Space Systems is the prime contractor for the project and built the spacecraft. The HiRISE camera was built by Ball Aerospace and Technology Corporation and is operated by the University of Arizona. The image data were processed using the U.S. Geological Survey’s ISIS3 software.