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This image shows a trough that has been carved in Mars' north polar layered deposits by erosion. The conical mound part-way down the slope is indicate a buried crater underneath the ice-rich deposits. Credit: NASA/JPL/University of Arizona


This subimage shows an example of a rare, small crater in the surface of Mars north polar cap, or Planum Boreum. Scientists can count these shallow craters to attain an estimate of the age of the upper few meters of the Planum Boreum surface. Credit: NASA/JPL/University of Arizona

Impact Crater Exhumed from Mars Ice
By Andrea Thompson
Senior Writer
posted: 16 October 2008
12:09 pm ET

New images taken by NASA's Mars Reconnaissance Orbiter have revealed rare evidence of an impact crater in Mars' north polar region.

Around the red planet's north pole is a feature called the north polar layered deposits, which are a series of ice-rich layers deposited over time and up to several kilometers thick.

The new images from MRO's High Resolution Imaging Science Experiment (HiRISE) camera revealed an odd, solitary hill rising part-way down an eroding slope of the layered terrain. The exposed section of the deposits is about 1,640 feet (500 meters) thick, and the conical mound is about 130 feet (40 meters) high.

"The mound may be the remnant of a buried impact crater, which is now being exhumed," said HiRISE team member Shane Byrne, of the University of Arizona.

If it sounds backwards for a crater to be revealed by a mound, there's a fairly simple explanation:

The crater formed as the north polar ice layers were being deposited. The crater itself would have been filled in by ice after it formed.

Most of these craters are buried under the Martian surface and inaccessible to scientists and their instruments. But this crater and its associated ice mound were exhumed as erosion formed a trough above and around it.

"For reasons that are poorly understood right now, the ice beneath the site of the crater is more resistant to this erosion, so that as the trough is formed, ice beneath the old impact site remained, forming this isolated hill," Byrne said.

At high resolution, the HiRISE image shows that the mound is made up of polygonal blocks as big as 33 feet (10 meters) across. The blocks are covered by the reddish dust that is ubiquitous on Mars, but otherwise resemble ice-rich blocks seen in other images of the north polar layered deposits.

Another new HiRISE image showed a small impact crater on the surface of Planum Boreum, or the north polar cap. This smaller crater is only about 125 yards (115 meters) in diameter.

The dearth of craters around Mars' north polar region has led scientists to suggest that either the north polar cap is only about 100,000 years old, and therefore would have accumulated fewer impacts, or that the craters disappear as the ice relaxes, just as imperfections in an old window disappear as the glass relaxes.

 

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