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PIA21187: Gusev Crater Windstreaks
This image captured by NASA's 2001 Mars Odyssey spacecraft shows some of the numerous dark linear streaks on the floor of Gusev Crater. These streaks are formed by wind action.
 Target Name:  Mars
 Is a satellite of:  Sol (our sun)
 Mission:  2001 Mars Odyssey 
 Spacecraft:  2001 Mars Odyssey
 Instrument:  THEMIS 
 Product Size:  685 x 1428 pixels (w x h) 
 Produced By:  Arizona State University 
 Full-Res TIFF:  PIA21187.tif (681.8 kB)
 Full-Res JPEG:  PIA21187.jpg (79.53 kB)  

Click on the image above to download a moderately sized image in JPEG format (possibly reduced in size from original)

Original Caption Released with Image:

Context image for PIA21187
Context image

Today's VIS image shows some of the numerous dark linear streaks on the floor of Gusev Crater. These streaks are formed by wind action. The dark streaks are where dust devils have removed the surface dust, revealing the darker rock beneath. Gusev Crater is the home of the MER Spirit lander.

Orbit Number: 65898 Latitude: -14.5 Longitude: 175.545 Instrument: VIS Captured: 2016-10-21 21:54

Please see the THEMIS Data Citation Note for details on crediting THEMIS images.

NASA's Jet Propulsion Laboratory manages the 2001 Mars Odyssey mission for NASA's Science Mission Directorate, Washington, D.C. The Thermal Emission Imaging System (THEMIS) was developed by Arizona State University, Tempe, in collaboration with Raytheon Santa Barbara Remote Sensing. The THEMIS investigation is led by Dr. Philip Christensen at Arizona State University. Lockheed Martin Astronautics, Denver, is the prime contractor for the Odyssey project, and developed and built the orbiter. Mission operations are conducted jointly from Lockheed Martin and from JPL, a division of the California Institute of Technology in Pasadena.

Image Credit:
NASA/JPL-Caltech/ASU

Image Addition Date:
2016-12-12