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PRESS RELEASE
01.04.2016

Rover Rounds Martian Dune to Get to the Other Side

This Dec. 18, 2015, view of the downwind face of "Namib Dune" on Mars covers 360 degrees, including a portion of Mount Sharp on the horizon. The component images were taken by the Mast Camera on NASA's Curiosity Mars rover. The site is part of the dark-sand "Bagnold Dunes" field of active dunes.
Credit: NASA/JPL-Caltech

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NASA's Curiosity Mars rover, partway through the first up-close study ever conducted of extraterrestrial sand dunes, is providing dramatic views of a dune's steep face, where cascading sand has sculpted very different textures than the wavy ripples visible on the dune's windward slope.
Slip face on Downwind Side of 'Namib' Sand Dune on Mars
Slip face on Downwind Side of 'Namib' Sand Dune on Mars
This view from NASA's Curiosity Mars Rover shows the downwind side of a dune about 13 feet high within the Bagnold Dunes field on Mars. The rover's Navigation Camera took the component images on Dec. 17, 2015. As on Earth, the downwind side of an active sand dune has a steep slope called a slip face. Credit: NASA/JPL-Caltech

Panoramic scenes dominated by the steep face of a dune called "Namib Dune" are online at these sites:

http://mars.nasa.gov/multimedia/images/?ImageID=7627
http://mars.nasa.gov/multimedia/images/?ImageID=7623

Researchers are using Curiosity to examine examples of the Bagnold Dunes, a band of dark sand dunes lining the northwestern flank of Mt. Sharp, the layered mountain the rover is climbing. A characteristic that sets true dunes apart from other wind-shaped bodies of sand, such as drifts and ripples previously visited by Mars rovers, is a steep, downwind slope known as the slip face. Here, sand blowing across the windward side of the dune suddenly becomes sheltered from the wind by the dune itself. The sand falls out of the air and builds up on the slope until it becomes steepened and flows in mini-avalanches down the face.

The mission's dune-investigation campaign is designed to increase understanding about how wind moves and sorts grains of sand, in an environment with less gravity and much less atmosphere than well-studied dune fields on Earth. The Bagnold Dunes are active. Sequential images taken from orbit over the course of multiple years show that some of these dunes are migrating by as much as a yard, or meter, per Earth year.

Curiosity has not caught a sand slide in action, but the rover's images of the Namib Dune slip face show where such slides have occurred recently. These dunes likely are most active in Mars' southern summer, rather than in the current late-fall season.

A few days of rover operations were affected in December due to an arm-motion fault, diagnosed as a minor software issue. Normal use of the arm resumed Dec. 23.

Curiosity has been working on Mars since early August 2012. It reached the base of Mount Sharp in 2014 after fruitfully investigating outcrops closer to its landing site and then trekking to the mountain. The main mission objective now is to examine successively higher layers of Mount Sharp.

For more information about Curiosity, visit:

http://mars.nasa.gov/msl


All Related Images
  • This view from NASA's Curiosity Mars Rover shows the downwind side of a dune about 13 feet high within the Bagnold Dunes field on Mars. The rover's Navigation Camera took the component images on Dec. 17, 2015. As on Earth, the downwind side of an active sand dune has a steep slope called a slip face.
    Slip Face on Downwind Side of 'Namib' Sand Dune on Mars
  • This view from NASA's Curiosity Mars Rover shows the downwind side of a dune about 13 feet high within the Bagnold Dunes field on Mars. The rover's Navigation Camera took the component images on Dec. 17, 2015. As on Earth, the downwind side of an active sand dune has a steep slope called a slip face.
    Slip face on Downwind Side of 'Namib' Sand Dune on Mars (Labeled)
  • This stereo view from NASA's Curiosity Mars Rover shows the downwind side of a dune about 13 feet high within the Bagnold Dunes on Mars. The image appears three-dimensional when viewed through red-blue glasses with the red lens on the left. Curiosity's Navcam took the component images on Dec. 17, 2015.
    Downwind Side of 'Namib' Sand Dune on Mars, Stereo
  • This Dec. 17, 2015, view combines multiple images from the telephoto-lens camera of the Mast Camera (Mastcam) on NASA's Curiosity Mars rover to reveal fine details of the downwind face of "Namib Dune." Sand on this face of the dark dune has cascaded down a slope of about 26 to 28 degrees.
    Mastcam Telephoto of a Martian Dune's Downwind Face
  • This Dec. 18, 2015, view of the downwind face of "Namib Dune" on Mars covers 360 degrees, including a portion of Mount Sharp on the horizon. The component images were taken by the Mast Camera on NASA's Curiosity Mars rover. The site is part of the dark-sand "Bagnold Dunes" field of active dunes.
    Full-Circle Panorama Beside 'Namib Dune' on Mars

2016-001

Guy Webster
Jet Propulsion Laboratory, Pasadena, Calif.
818-354-6278
guy.webster@jpl.nasa.gov

Dwayne Brown / Laurie Cantillo
NASA Headquarters, Washington
202-358-1726 / 202-358-1077
dwayne.c.brown@nasa.gov / laura.l.cantillo@nasa.gov

Credit: NASA/JPL-Caltech

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