MRO’s HiRISE Views Frosty Martian Dunes

A color image of the Martian surface from above looks like the bumpy, scaly skin of a reptile, with the high spots in shades of light turquoise and tan, and the crevices appearing a dark copper color. Among all this are a dozen oblong bumps, angled from the upper left toward lower right, also mainly copper-colored; some of them look like coffee beans, others resemble partially deflated, wrinkled balloons. They’re lighted from a source beyond the lower-left edge of the frame; on their shadowed sides, some have patches of white or light turquoise.
NASA/JPL-Caltech/University of Arizona
December 20, 2024
CreditNASA/JPL-Caltech/University of Arizona
Historical DateSeptember 8, 2022
PIA NumberPIA26517
Language
  • english

These Martian dunes in Mars' northern hemisphere were captured from above by NASA's Mars Reconnaissance Orbiter using its High-Resolution Imaging Science Experiment (HiRISE) camera on Sept. 8, 2022. Scientists use such images to track the amount of frost that settles on the landforms and then disappears as the weather warms in spring.

Martian dunes migrate just like dunes on Earth, with wind blowing away sand on one side of the dune and building up on another. Recent research has shown that winter frost stops the movement of sand grains, locking the dunes in place until the spring thaw.

The University of Arizona, in Tucson, operates HiRISE, which was built by BAE Systems in Boulder, Colorado. NASA's Jet Propulsion Laboratory, a division of Caltech in Pasadena, California, manages the Mars Reconnaissance Orbiter Project for NASA's Science Mission Directorate, Washington.