Mars Craters Tell Story of Water and Ice

Mars Craters Tell Story of Water and Ice
Ice core from Antarctica with an aggregation of soil grains. (Image credit: Hans Paerl, University of North Carolina at Chapel Hill)

Enigmatic 'Meridiani Planum' deposits on Mars -- deep salty areas found by NASA's Opportunity rover -- have attracted several theories to explain their existence in recent years.

Add another one to the list: the Martian deposits could be remnants of a massive ancient ice-field, a new study suggests.

This new icy theory better explains some of the odd signatures of the deposits, its authors say. The finding, detailed in the Feb. 15 online version of the journal Nature Geoscience, "advances a new idea for how the sedimentology of Mars developed," said study co-author Paul Niles of NASA's Johnson Space Center in Houston.

On Earth, ocean evaporate deposits are purely calcium sulfates, because magnesium stays dissolved in the water. But on Mars, there are "mixtures of minerals that don't really seem to go together," Niles told Space.com. "It's an interesting thing to try to explain."

The theory put forward by Niles and his co-author Joseph Michalski, of the Université Paris Sud in France, provides an explanation for the discrepancy.

The new theory draws on the mechanism that scientists think is responsible for forming the ice that currently tops Mars' polar caps.

"It's kind of like acid rain on Earth," he said.

All that ice and dust and aerosol eventually gets incorporated into a large ice field. While the ice reflects incoming sunlight, the dust grains absorb it and "get warmer than the ice," Niles explained. The ice around the grains melts, creating little pockets where the trapped materials can react with the water.

Because the acidic water is kept in small pockets, the minerals in the silicate dust grains don't separate out like they would in a larger space. Such aggregates of grains have been seen in Antarctic ice cores.

The case of how the deposits came to be still isn't closed though, and it may take a rover exploring these or similar deposits to nail their origin down.

"There's a lot more work to be done to figure out how this happened," Niles said.

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Andrea Thompson
Contributor

Andrea Thompson is an associate editor at Scientific American, where she covers sustainability, energy and the environment. Prior to that, she was a senior writer covering climate science at Climate Central and a reporter and editor at Live Science, where she primarily covered Earth science and the environment. She holds a graduate degree in science health and environmental reporting from New York University, as well as a bachelor of science and and masters of science in atmospheric chemistry from the Georgia Institute of Technology.