Seasonal Changes on Mars

Seasonal Changes on Far-Northern Mars, in this series of false-color pictures of sand dunes in the north polar region of Mars. The area covered in each of the five panels is about 0.8 mile (1.3 km) wide.   Image © NASA/JPL-Caltech/Univ. of Arizona

The images captured by High Resolution Imaging Science Experiment (HiRISE) camera on NASA’s Mars Reconnaissance Orbiter.



The progression begins at left (Panel A) in early spring, when the ground is covered by a seasonal layer of carbon dioxide ice (dry ice) about 2 feet thick. As spring progresses the ice cracks (Panel B), releasing dark sand from the dune below. When pressurized gas trapped below the ice layer is released, it carries along sand and dust to the top of the ice layer, where it is dropped in fan-shaped deposits downhill and downwind (panels C and D). The final panel shows more and more of the dark dunes as the overlying layer of seasonal ice evaporates back into the atmosphere.

Seasonal Changes on MarsNorthern Mars.   Image © NASA

 

Mars Reconnaissance Orbiter captures the springtime thaw of seasonal carbon dioxide ice on Mars.