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NASA Orbiter Catches Mars Sand Dunes in MotionWritten by Dwayne Brown – NASA Headquarters
“Mars either has more gusts of wind than we knew about before, or the winds are capable of transporting more sand,” said Nathan Bridges, planetary scientist at the Johns Hopkins University’s Applied Physics Laboratory in Laurel, MD, and lead author of a paper on the finding published online in the journal Geology. “We used to think of the sand on Mars as relatively immobile, so these new observations are changing our whole perspective.” ![]() A dune in the northern polar region of Mars shows significant changes between two images taken on June 25th, 2008 and May 21st, 2010 by NASA's Mars Reconnaissance Orbiter. (Image credit: NASA/JPL-Caltech/Univ. of Ariz./JHUAPL) MRO was launched in 2005. Initial images from the spacecraft’s High Resolution Imaging Science Experiment (HiRISE) camera documented only a few cases of shifting sand dunes and ripples, collectively called bedforms. Now, after years of monitoring the Martian surface, the spacecraft has documented movements of a few yards (or meters) per year in dozens of locations across the planet.
“Sand moves by hopping from place to place,” said Matthew Golombek, a co-author of the new paper and a member of the Mars Exploration Rover and Mars Reconnaissance Orbiter teams at NASA’s Jet Propulsion Laboratory in Pasadena, CA. “Before the rovers landed on Mars, we had no clear evidence of sand moving.” Not all of the sand on Mars is blowing in the wind. The study also identifies several areas where the bedforms did not move.
According to scientists, the seemingly stationary areas might move on much larger time scales, triggered by climate cycles on Mars that last tens of thousands of years. The tilt of Mars’ axis relative to its orbital plane can vary dramatically. This, combined with the oval shape of Mars’ orbit, can cause extreme changes in the Martian climate, much greater than those experienced on Earth. Mars may once have been warm enough that the carbon dioxide now frozen in the polar ice caps could have been free to form a thicker atmosphere, leading to stronger winds capable of transporting sand.
JPL is managed for NASA by the California Institute of Technology in Pasadena. MRO images and additional information is available online at: www.nasa.gov/mro and http://mars.jpl.nasa.gov/mro/ For more information about NASA Mars missions, visit the Web at: www.nasa.gov/mars . SectionsNewsTopicsDwayne Brown, earth, High Resolution Imaging Science Experiment, HiRISE, Johns Hopkins University Applied Physics Laboratory, Laurel MD, Mars, Mars Reconnaissance Orbiter, NASA, NASA Headquarters, NASA's Jet Propulsion Laboratory, NASA's Mars Exploration Rovers, NASA's Mars Global Surveyor, NASA's Viking Landers, National Aeronautics and Space Administration, Pasadena CA, Priscilla Vega, Red Planet, Sand Dunes |
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