A digital terrain model generated from a stereo pair of images provides this synthesised, oblique view of a portion of the wall terraces of Mojave Crater in the Xanthe Terra region of Mars
A digital terrain model generated from a stereo pair of images provides this synthesised, oblique view of a portion of the wall terraces of Mojave Crater in the Xanthe Terra region of Mars. (c) NASA/JPL-Caltech/University of Arizona
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Enhanced 3D model of Mars crater edge shows ups and downs

Science Centric | 22 February 2010 17:58 GMT — Votes (1)
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A dramatic 3D Mars view based on terrain modelling from NASA's Mars Reconnaissance Orbiter data shows 'highs and lows' of Mojave Crater. The vertical dimension is exaggerated three-fold compared with horizontal dimensions in the synthesised images of a portion of the crater's wall. The resulting images look like the view from a low-altitude aircraft. They reflect one use of digital modelling derived from two observations by the orbiter's High Resolution Imaging Science Experiment camera.

This enhanced view shows material that has pounded and is backed up behind massive blocks of bedrock in the crater's terrace walls. Hundreds of Martian impact craters have similar pounding with pitted surfaces. Scientists believe these 'pitted ponds' are created when material melted by the crater-causing impacts is captured behind the wall terraces.

Mojave Crater, one of the freshest large craters on Mars, is about 60 kilometres (37 miles) in diameter. In a sense, it is like the Rosetta Stone of Martian craters, because it is so fresh. Other craters of this size generally have already been affected by erosion, sediment and other geologic process. Fresh craters like Mohave reveal information about the impact process, including ejecta, melting and deposits.

Source: Jet Propulsion Laboratory, NASA


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