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Martian landscapes formed from sand 'levitating' on a little boiling water


Scientists from The Open University (OU) have discovered a process that could explain the long-debated mystery of how land features on Mars are formed in the absence of significant amounts of water.

Martian landscapes formed from sand 'levitating' on a little boiling water
A view from the "Kimberley" formation on Mars taken by NASA's Curiosity rover. The strata in the foreground dip 
towards the base of Mount Sharp, indicating flow of water toward a basin that existed before the larger bulk 
of the mountain formed [Credit: NASA/JPL-Caltech/MSSS]
Experiments carried out in the OU Mars Simulation Chamber -- specialised equipment, which is able to simulate the atmospheric conditions on Mars -- reveal that Mars' thin atmosphere (about 7 mbar -- compared to 1,000 mbar on Earth) combined with periods of relatively warm surface temperatures causes water flowing on the surface to violently boil. This process can then move large amounts of sand and other sediment, which effectively 'levitates' on the boiling water.

This means that, in comparison to Planet Earth, relatively small amounts of liquid water moving across Mars' surface could form the large dune flows, gullies and other features, which characterise the Red Planet.

Dr Jan Raack, Marie Skłodowska-Curie Research Fellow at The Open University, is lead author of the research; he said:

Martian landscapes formed from sand 'levitating' on a little boiling water
The Cliffs of Rover resembling an ocean beating against cliffs [Credit: NASA/JPL-Caltech/MSSS]
"Whilst planetary scientists already know that the surface of Mars has 'mass-wasting' features -- such as dune flows, gullies, and recurring slope lineae -- which occur as a result of sediment transportation down a slope, the debate about what is forming them continues.

"Our research has discovered that this levitation effect caused by boiling water under low pressure enables the rapid transport of sand and sediment across the surface. This is a new geological phenomenon, which doesn't happen on Earth, and could be vital to understanding similar processes on other planetary surfaces."

Dr Raack conducted these experiments in the Hypervelocity Impact (HVI) Laboratory based at the OU. He added:

"The sources of this liquid water will require more observational studies; however, the research shows that the effects of relatively small amounts of water on Mars in forming features on the surface may have been widely underestimated.

"We need to carry out more research into how water levitates on Mars, and missions such as the ESA ExoMars 2020 Rover will provide vital insight to help us better understand our closest neighbour."

The study is published in Nature Communications.

Source: Open University [October 27, 2017]
TANN

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