Doctoral student explores formation of martian gullies

Doctoral student explores formation of martian gullies
Matthew Sylvest, a doctoral student in space and planetary sciences the the University of Arkansas, adjusts the placement of thermocouples to measure the temperature distribution in the simulated Martian regolith last fall at the Open University in England.

The gullies of Mars have fascinated scientists since they were first identified through high-definition images transmitted to Earth by the Mars Global Surveyor in the late 1990s.

"On Earth, gullies are formed by erosion due to water flow," said Matthew Sylvest, a doctoral candidate in the Arkansas Center for Space and Planetary Sciences at the University of Arkansas. "Under conditions on Mars, water can't exist in its liquid form – at least not in quantities to erode and form those features. So the question becomes: If it isn't water, what could it be that is making this happen?"

Sylvest is investigating the potential role of dry ice in the creation of the gullies on Mars. Dry ice – the solid form of – exists on the Martian surface, and carbon dioxide constitutes more than 85 percent of the planet's atmosphere.

Sylvest recently returned from the Open University in England, where, as a fellow of the U of A's Roy and Christine Sturgis International Honors Program, he worked with a research group to develop experimental planetary surface simulations.

"Plenty of people have begun supposing this is carbon dioxide frost causing the surface to move, but nobody had done a laboratory simulation to see if that could really happen," Sylvest said. "This opportunity at the Open University was very special. They had the facilities and a group of people that represent the cutting edge of experimental planetary surface simulations. We built an apparatus and the process to see if dry ice would move the simulated Martian soil. We discovered that it does, and at reduced atmospheric pressure very surprisingly and dramatically."

The next step, Sylvest said, is to analyze the results and attempt to explain why the dry ice moves the soil.

"There are quite a few parameters that could be affecting this to varying degrees," he said. "I'm looking forward to getting more data and looking at the mechanisms up close and understand what makes that work. The fact that we see move the soil, we're not in a position to say that's what caused the , just that we've shown we can't rule it out."


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Citation: Doctoral student explores formation of martian gullies (2015, February 6) retrieved 4 April 2020 from https://phys.org/news/2015-02-doctoral-student-explores-formation-martian.html
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