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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.
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:
“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 research, which has been published today [this will be live on Friday 27 October 2017] in the academic journal Nature Communications, is funded by the Europlanet 2020 Research Infrastructure through the European Union's Horizon 2020 Research and Innovation Programme [Grant Agreement No. 654208], and co-authored by academics* from the STFC Rutherford Appleton Laboratory, Universität Bern, and Université de Nantes. The initial research concept was developed by Susan J. Conway of Université de Nantes.
The research, ‘Water induced sediment levitation enhances downslope transport on Mars’, was developed in collaboration with the following academics:
Jan Raack (lead author), Manish R. Patel, Matthew R. Balme – School of Physical Sciences, Faculty of STEM, The Open University, Milton Keynes
Clémence Herny – Physikalisches Institut, Universität Bern, Switzerland
Sabrina Carpy, Susan J. Conway – Laboratoire de Planétologie et Géodynamique, Université de Nantes, France
To be published in Nature Communications on Friday 27 October 2017
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