Martian volcanic glass could be hotspot for life

Martian Volcanic Glass Could Be Hotspot for Life
Dusty, glass-rich sand dunes like these found just south of the north polar ice cap could cover much of Mars. (False color image) Credit: NASA/JPL/University of Arizona

Water may have played a role in forming plains of volcanic glass that spread across nearly a third of Mars. The discovery of this volcanic glass could steer scientists toward subglacial lakes where martian life could thrive.

Glass sand on Mars may point the way to chemically-rich water ideal for hosting life. The newly discovered glass dune fields, spread across almost a third of the planet, likely formed from interactions between magma and ice or water - interactions that could create the perfect environments for microbial life.

A glassy sea of sand

The northern lowlands spread across millions of square miles in the red planet's . But dark sediments in the region have puzzled planetary scientists.

Briony Horgan and James Bell, both of Arizona State University, used the European Space Agency's Mars Express orbiter to re-examine light radiated from the martian plains. They determined that the strange readings were caused by sand composed of glass.

"We're actually seeing glass particles, like glass sand," Horgan said.

Such landforms are not unique to Mars. Iceland boasts thousands of square miles of desert dominated by glass sand.

The martian dunes don't just make an interesting vacation spot. They also provide tantalizing hints toward their formation.

"The only way to create an extensive glassy deposit like that is through explosive volcanism," Horgan said. "This is the first direct evidence on Mars for explosive volcanism on a planetary scale."

Martian Volcanic Glass Could Be Hotspot for Life
The Grímsvötn Volcano in Iceland sits beneath the Vatnajökull ice cap. As a result, most of its eruptions are subglacial, and the magma and meltwater interact much the way the two might interact on Mars. Credit: NASA/Jacques Descloitres

When a Martian volcano erupts, the thin atmosphere and difference in pressure should make for some great pyrotechnics. But a fiery eruption alone won't guarantee glass. It takes an interaction with water or ice to manage that.

"When lava or magma interacts with ice or water, it is quenched, which means it rapidly cools and solidifies," said Claire Cousins of the University of London. "This rapid cooling prevents any crystals from growing, and so a is produced."

Cousins, who was not involved in the new research, has studied volcanic environments in Iceland and Antarctica as martian analogues, and is investigating subglacial volcanoes on Earth as habitats for life.

The glassy plains also show evidence of water-related weathering. As ice melted across the lowlands, it mixed with the strange sand to form an acid. With enough exposure to the iron inside the sand, the chemicals would neutralize, which means that only a constantly renewed water source, like melting ice or snow, could cause the leaching the team saw.

Details on the new martian landforms were published online in the journal Geology.

A hotspot for life

The glassy expanse would not be the best location to search for life. But it could lead to more promising environments.

"We definitely know searching for organisms in the northern lowlands is difficult," Horgan said. "I think the better place to go would be those source regions, the ice-magma interactions."

Referring to hydrothermal systems and subglacial lakes, she said, "Those have been identified as places where biosignatures could have been preserved."

Cousins agreed.

"Regions of volcano-ice interactions on Earth provide a wide range of hydrothermal environments that can be exploited by microbial life," she said.

Martian Volcanic Glass Could Be Hotspot for Life
Covered with glass sand, the lava plain, Árskógar, in Iceland, could bear some similarity to regions on Mars. Credit: Hansueli Krap

If a volcano erupts beneath a glacier, the heat could form huge subglacial lakes.

"It's the perfect place for microbes," Horgan said. "A nice, warm, safe place for microbes to hang out, with lots of chemicals around to munch on."

Locating the lakes

Finding such water sources could prove to be a challenge. After a volcanic explosion, the newly-created sand could fall from the sky. But although scientists have modeled a number of possibilities, they haven't quite been able to make the sand spread across the lowlands.

"There's only a couple of ways to move this stuff around," Horgan said.

Sand-sized ash is too heavy to travel far from the vents. The northern highlands are hundreds to thousands of miles from known volcanoes, however, which has left scientists puzzled.

The glass sand could provide a valuable clue. Because it requires ice or water to form, the subglacial lakes they suggest could solve part of the distribution problem.

Though the water would initially be contained - and ripe for life - eventually it could break free of the walls containing it, creating enormous floods across the lowlands.

"This would be similar to some of the catastrophic floods people have talked about for Mars."

The presence of glass sand, and their requirement of water to form, bring a clearer understanding to the geology of the red planet, and a more concrete suggestion on where to look for life.

"It's the first time we've really seen evidence for ice-related alterations on ," Horgan said.

"It's something we're really excited to look into."

Explore further

Are gas-formed gullies the norm on Mars?

More information: Paper online: … /2012/03/23/G32755.1
Citation: Martian volcanic glass could be hotspot for life (2012, April 26) retrieved 24 July 2019 from
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User comments

Apr 26, 2012
Re: "The only way to create an extensive glassy deposit like that is through explosive volcanism"

Message to the editor:

This is a blatantly false statement which should be stricken from this article. You guys might want to tone down your rhetoric a little bit ...
"Evidence for a Lightning-Strike Origin of the Edeowie Glass"

Apr 27, 2012
@HannesAlfven, have you read the article you posted? It is talking about glass formed that is tens of centimeters wide. Whereas, this article is clearly discussing glass that is extensive and obviously much larger than that. Until you've read the paper available online (provided by the editor), how can you claim the information is blatantly false?

Apr 27, 2012
Making assumptions is not science, for all we know that area got struck by a CME.

Apr 27, 2012

Plasmas are known to scale over 14 orders of magnitude. Self-similar plasmas actually have a name: they are called heteromacs. What this means is that we can do experiments on plasmas in the laboratory, and those observations are indeed relevant to our observations of cosmic plasmas.

This is a very important point, for we observe space to be filamentary on MULTIPLE SCALES of existence. Dusty plasmas in tokamak devices can be observed to form filamentary and cellular structures which exhibit dramatic similarities to the dusty plasmas we see with telescopes in interstellar space.

Many people think that plasmas are too diffuse to maintain an E-field of any relevance. But, the plasma's self-similarity means that one need only scale up to a larger dimension to see that there is a larger, denser structure which includes that diffuse plasma, as a heteromac.

Plasma scaling offers us a whole new approach to cosmology and astrophysics, but it is largely ignored right now.

Apr 27, 2012
For more information on plasma's self-similarity, see the work of AB Kukushkin and VA Rantsev-Kartinov. These guys built artificial intelligence algorithms to detect skeletal structures in dusty plasmas in tokamak's, and then applied those algorithms to all sorts of natural phenomenon. The most dramatic illustrations of their work pertain to the application of those algorithms to our observations of interstellar HI hydrogen.

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