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WSU Undergrad Helps Develop Method For Detecting Water On Mars

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Provided by Eric Sorensen, Washington State University

A Washington State University undergraduate has helped develop a new method for detecting water on Mars. Her findings appear in Nature Communications, one of the most influential general science journals.

Kellie Wall, 21, of Port Orchard, Wash., looked for evidence that water influenced crystal formation in basalt, the dark volcanic rock that covers most of eastern Washington and Oregon. She then compared this with volcanic rock observations made by the rover Curiosity on Mars’ Gale Crater.

“This is really cool because it could potentially be useful for not only the study of rocks on Earth but on Mars and other planets,” said Wall.

She is the lead author of the article in Nature Communications. Among multidisciplinary science journals, it has the third-highest impact factor, a measure of its influence, after the journals Nature and Science, according to the 2013 Journal Citation Reports.

Co-authors include Michael Rowe, a former WSU research professor now at New Zealand’s University of Auckland, and Ben Ellis, a former WSU post-doctoral researcher now at the Institute of Geochemistry and Petrology in Zurich, Switzerland. The other authors are Mariek Schmidt of Brock University in Canada and Jennifer Eccles of the University of Auckland.

The researchers established a method to quantify the texture of volcanic rock using an index called “groundmass crystallinity.” Wall compares it to the texture of a chocolate chip cookie, which can vary according to how it is cooked and cooled.

“We were interested in the cookie dough part of the cookie,” she said.

Liquid volcanic rock cools rapidly as it hits water, flash-freezing to form mostly glass. Without water, it takes longer to cool and forms crystals within the groundmass, the cookie dough part.

Using an x-ray diffraction machine on the WSU campus, home to one of the most sophisticated basalt labs in the world, Wall analyzed rock samples from the Northwest, New Zealand and Italy’s Mount Etna and compared them to rocks analyzed by Curiosity’s x-ray diffractometer.

“The rocks that erupted and interacted with water, which we call phreatomagmatic, all had a groundmass crystallinity as low as 8 percent and ranging up to about 35 percent,” she said. “The rocks that erupted without interaction with water had groundmass crystallinities from about 45 percent upwards to almost totally crystalline.

“The analyses we did on the Mars soil samples fell in the range of the magmatic type eruptions, which are the ones erupted without water interaction,” she said.

Water is a key indicator for the potential of microbial life on the red planet. While Wall and her colleagues didn’t see evidence of it from two sites they studied, their method could look for water elsewhere.

“I think this quantification of volcanic textures is a new facet of the water story that hasn’t yet been explored,” Wall said. “Most of the studies searching for water have focused on either looking for sedimentary structures—large- and small-scale—for evidence of water, or looking for rocks like limestones that actually would have formed in a water-rich environment.

“But being able to determine the environment through the texture of a volcanic rock is something pretty cool and different,” she said. “I think it’s an interesting avenue for future research.”

The project was funded by the WSU College of Arts and Sciences’ Grants for Undergraduate Scholars and by the NASA Space Grant Undergraduate Scholarship in Science and Engineering.

> Continue reading…

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Source: http://www.redorbit.com/news/space/1113250760/mars-water-detection-wsu-kellie-wall-100714/


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