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Heavily Eroded Crater on Mars.
This perspective image of an eroded crater on Mars was taken by the European Space Agency's Mars Express spacecraft in May 2004. It's at Solis Planum, in the Thaumasia region of Mars. The larger eroded impact crater is about 53 km (32 miles) across, and the crater rim is nearly a kilometre high. The blue-white areas at the upper left have light clouds, changing the colour.
This image, taken by the High Resolution Stereo Camera (HRSC) on board ESA’s Mars Express spacecraft, shows part of a heavily eroded impact crater at Solis Planum, in the Thaumasia region of Mars.
The image was taken during orbit 431 in May 2004 with a ground resolution of approximately 48 metres per pixel. The displayed region is located south of Solis Planum at longitude 271º East and latitude of about 33º South.
The larger eroded impact crater in the lower left of the image has a diameter of about 53 kilometres and its eastern crater rim is about 800 metres high.
The blue/white tint in the eastern (top left) part of the scene indicates a near-surface haze or clouds.
To the south (right), tectonic 'graben’ structures can be seen running in three different directions (north-west, north-east and east-north-east), which show three different phases of development.
A graben is a down-dropped block of the crust resulting from extension, or pulling, of the crust. They are often seen together with features called 'horsts’, which are upthrown blocks lying between two steep-angled fault blocks. Some of the graben shown here are about five kilometres wide.
The northern end of the higher region, or upper left in this image, contains an almost circular plateau, which is 15 kilometres across.
It may be an old impact crater, filled by sediments, which developed a harder consistency than the surrounding material over the course of time.
Later, the more easily eroded material was removed and the harder inner filling remained. This phenomenon is called 'inverted relief’.
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