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03 FEB. 2010
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The Mars Express High Resolution Stereo Camera has imaged craters both young and old in this view of the Southern Highlands of Mars.
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Sirenum Fossae
Part of the Sirenum Fossae region in the Southern Highlands, the area in this image is centred at about 28°S / 185°E. The image captures an area to the north of the Magelhaens Crater. It extends some 230 km by 127 km and covers about 29 450 sq km, roughly the size of Belgium. The image resolution is approximately 29 metres per pixel.
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Perspective view of Sirenum Fossae
Sirenum Fossae extends for more than 2500 km to the southwest of the Tharsis volcanic region, which contains Olympus Mons, the highest volcano in our Solar System. Sirenum Fossae is a system of grabens, formed by stresses placed on the crust during the uprising of the Tharsis region. A graben is visible as two sets of parallel lines running from top to bottom to the left of centre.
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Sirenum Fossae’s central plateau
The Southern Highlands are older than the Northern Lowlands, based on the larger number of impact craters seen to cover the region. Craters of 50 km in diameter are common in this area and have usually suffered from erosion, indicating they were formed during ancient times.
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Notable features in the Sirenum Fossae region of Mars.
There is an impact crater with a diameter of about 28 km to the left of the image. In contrast to other craters in its vicinity, it has experienced less erosion – its crater rim and central peak are still preserved. There are three other craters nearby: to the west is a large crater with a diameter of 56 km, to the northeast one that stretches 34 km across and a smaller crater of only 9 km diameter to the south.
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Craters in the Sirenum Fossae region of Mars
On the basis of their appearances, the craters can be placed in age order. The largest two are the oldest because they have been partially destroyed by the mid-sized crater. The smallest is the youngest because it has impacted into the rim of the mid-sized crater.
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Elevation of the Sirenum Fossae region in the Southern Highlands of Mars.
In the central part of the image, a plateau is recognisable and shows evidence of further erosion. In particular, there is a broad valley system on the western slope.
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Part of the Sirenum Fossae region in high resolution.
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Part of the Sirenum Fossae region in 3D.
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Traces of Martian life
Mars Express close flybys of martian moon Phobos
Mars Express has returned images from the Phobos flyby of 9 January 2011. Mars Express passed Mars’ largest moon at a distance of 100km.
Wind and water have shaped Schiaparelli on Mars
The small crater embedded in the northwestern rim of the Schiaparelli impact basin features prominently in this new image from ESA’s Mars Express. All around is evidence for past water and the great martian winds that periodically blow.
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Related links
HRSC at DLR
Behind the lens...
This is the camera behind the stunning European imagery from Mars. The High Resolution Stereo Camera on ESA’s Mars Express is now mapping most of the Martian surface with unprecedented detail.
Mars Express HRSC images Frequently Asked Questions (FAQs)
We get lots of questions regarding Mars and Mars Express. Before posting your question, please go through the following FAQs to see if your question has already been answered.
ESA Planetary Science archive (PSA)
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