New Evidence for a Water-Rich History on Mars

Mars may have been a wetter place than previously thought, according to research on simulated Martian meteorites conducted, in part, at the Department of Energy’s Lawrence Berkeley National Laboratory (Berkeley Lab).

In a study published today in the journal Nature Communications, researchers found evidence that a mineral found in Martian meteorites—which had been considered as proof of an ancient dry environment on Mars—may have originally been a hydrogen-containing mineral that could indicate a more water-rich history for the Red Planet.

Photo - Naturally formed crystals of the mineral whitlockite, which is rare on Earth, are visible in this sample on display at Canada's Royal Ontario Museum. (Credit: Wikimedia Commons)

Naturally formed crystals of the mineral whitlockite, which is rare on Earth, are visible in this sample on display at Canada’s Royal Ontario Museum. (Credit: Wikimedia Commons)

Scientists at the University of Nevada, Las Vegas (UNLV), who led an international research team in the study, created a synthetic version of a hydrogen-containing mineral known as whitlockite.

After shock-compression experiments on whitlockite samples that simulated

the conditions of ejecting meteorites from Mars, the researchers studied their microscopic makeup with X-ray experiments at Berkeley Lab’s Advanced Light Source (ALS) and at Argonne National Laboratory’s Advanced Photon Source (APS).

The X-ray experiments showed that whitlockite can become dehydrated from such shocks, forming merrillite, a mineral that is commonly found in Martian meteorites but does not occur naturally on Earth.

“This is important for deducing how much water could have been on Mars, and whether the water was from Mars itself rather than comets or meteorites,” said Martin Kunz, a staff scientist at Berkeley Lab’s ALS who participated in X-ray studies of the shocked whitlockite samples.

Image - This image of Mars was created from about 1,000 Viking Orbiter images. (Credit: NASA Jet Propulsion Laboratory, U.S. Geological Survey)

This image of Mars was created from about 1,000 Viking Orbiter images. (Credit: NASA Jet Propulsion Laboratory, U.S. Geological Survey)

“If even a part of merrillite had been whitlockite before, it changes the water budget of Mars dramatically,” said Oliver Tschauner, a professor of research in the Department of Geoscience at UNLV who co-led the study with Christopher Adcock, an assistant research professor at UNLV.

And because whitlockite can be dissolved in water and contains phosphorous, an essential element for life on Earth—and merrillite appears to be common to many Martian meteorites—the study could also have implications for the possibility of life on Mars.

“The overarching question here is about water on Mars and its early history on Mars: Had there ever been an environment that enabled a generation of life on Mars?” Tschauner said.

This animation simulates a fly-around look at one of the places on Mars, within Hale Crater, where dark streaks advance down slopes during warm seasons, possibly involving liquid water. The streaks are roughly the length of a football field. (Credit: NASA JPL)

The pressures and temperatures generated in the shock experiments, while comparable to those of a meteorite impact, lasted for only about 100 billionths of a second, or about one-tenth to one-hundredth as long as an actual meteorite impact.

The fact that experiments showed even partial conversion to merrillite in these lab-created conditions, a longer duration impact would likely have produced “almost full conversion” to merrillite, Tschauner said.

He added that this latest study appears to be one of the first of its kind to detail the shock effects on synthetic whitlockite, which is rare on Earth.

Researchers blasted the synthetic whitlockite samples with metal plates fired from a gas-pressurized gun at speeds of up to about half a mile per second, or about 1,678 miles per hour, and at pressures of up to about 363,000 times greater than the air pressure in a basketball.

“You need a very severe impact to accelerate material fast enough to escape the gravitational pull of Mars,” Tschauner said.

Image - The Mojave Crater on Mars, which is believed to be the source of some Martian meteorites found on Earth, is pictured here in an image produced by the HIRISE camera on NASA's Mars Reconnaissance Orbiter. (Credit: NASA JPL-Caltech, University of Arizona)

The Mojave Crater on Mars, which is believed to be the source of some Martian meteorites found on Earth, is pictured here in a rendering produced by the HIRISE camera on NASA’s Mars Reconnaissance Orbiter. (Credit: NASA JPL-Caltech, University of Arizona)

 

Content retrieved from: https://newscenter.lbl.gov/2017/03/06/new-evidence-water-rich-mars/.