Mars Express puts craters on a pedestal

Feb 04, 2011
Extending 159 km by 87 km, this image shows a region with an area of about 13865 sq km, a third of the size of Denmark. Named after a feature on Giovanni Schiaparelli’s 19th-century Mars map, Arabia Terra is part of the highlands of Mars, stretching east to west across 4500 km. With a ground resolution of about 18 m per pixel, the data were acquired near 27°N/56°E during orbit 7457 of Mars Express 7457 on 26 October 2009. Credits: ESA/DLR/FU Berlin (G. Neukum)

(PhysOrg.com) -- ESA's Mars Express has returned new views of pedestal craters in the Red Planet's eastern Arabia Terra.

Craters are perhaps the quintessential planetary geological feature. So much so that early planetary geologists expended a lot of effort to understand them. You could say they put craters on a pedestal. This latest image of shows how the does it in reality.

Craters are the result of impacts by asteroids, comets and meteorites. In a pedestal crater, the surrounding terrain is covered by pulverised rock thrown out of the crater. This material creates a platform or pedestal around the crater often with steep cliffs, and is usually rich in volatile materials such as water and ice.

Arabia Terra is part of the highlands of Mars, stretching east to west across 4500 km in the northern hemisphere, and named for a feature drawn on Giovanni Schiaparelli’s 19th-century map of Mars.

The whole area is characterised by steep-sided hills, valleys and ancient impact craters that have been extensively resurfaced by old lava flows and modified by profound erosion over millions of years. The eastern areas rise up to 4 km above the low-lying north-western parts. To the north, Arabia Terra drops and blends into the northern lowlands.

This is the eastern part of Arabia Terra, part of the highlands of Mars. Large, irregular deposits have proved more resistant to erosion than their surroundings. Credits: ESA/DLR/FU Berlin (G. Neukum)

Pedestal craters are visible in this new view of a 159 km by 87 km region of eastern Arabia Terra, taken by the High Resolution Stereo Camera on ESA’s orbiter.

The large crater to the top centre has a pedestal that looks like a skirt, rising almost up to the crater rim. Mounds and table mountains on the floors of the larger craters show layered deposits that could be the result of volcanic processes, or that may have been deposited by wind or water.

In the north (right), layered deposits appear as smooth plains covering the highlands. These were thought to have formed during the Late Noachian and Early Hesperian eras, about 4 billion years ago.

Later, the deposits experienced heavy erosion by wind and partially by water, leading to the variety of landscapes seen in this region today.

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