These prominent trenches were formed by faults that pulled the planet's surface apart less than 10 million years ago.
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| Mars Express view of Cerberus Fossae [Credit: ESA/DLR/FU Berlin, CC BY-SA 3.0 IGO] |
The fossae – meaning 'ditches' or 'trenches' in Latin – stretch for more than 1000 kilometres from the northwest to the southeast.
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| Cerberus Fossae in context [Credit: European Space Agency] |
They vary in width, typically from a few tens of metres to over a kilometre wide, and are thought to be tectonic features originating from faults that stretch the upper layers of the surface apart.
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| Perspective view of Cerberus Fossae [Credit: European Space Agency] |
Rounded collapse pits observed in the northern part (north is to the right in the main colour image) indicate an early stage of surface sinking; in other places rounded features can be seen connecting up to create longer cracks.
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| Perspective view of Cerberus Fossae [Credit: European Space Agency] |
To the west, as seen in the context image, the Athabasca Valles outflow channel links with the fossae system.
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| Topographic view of Cerberus Fossae [Credit: European Space Agency] |
During its mission lifetime it has taken over 40,000 images of Mars and its two moons with the high resolution stereo camera, as well as context images with its Visual Monitoring Camera. It has also collected a vast dataset with its suite of scientific instruments that are analysing the planet from its ionosphere, atmosphere, and interaction with the solar wind, through to its subsurface with radar.
Source: ESA [September 20, 2018]











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