Friday, February 28, 2020

How Mars May Have Once Hosted Oceans and Life

Scientists have devised new analytical tools to break down the enigmatic history of Mars’ atmosphere — and whether life was once possible there.

Jezero Crater, landing site for the upcoming Mars 2020 rover mission.
Credit: NASA/JPL/JHUAPL/MSSS/Brown University 

A paper detailing the work was published today in the journal Science Advances. It could help astrobiologists understand the alkalinity, pH and nitrogen content of ancient waters on Mars, and by extension, the carbon dioxide composition of the planet’s ancient atmosphere.

Mars of today is too cold to have liquid water on its surface, a requirement for hosting life as we know it.

“The question that drives our interests isn’t whether there’s life on present-day Mars,” said Tim Lyons, UCR distinguished professor of biogeochemistry. “We are driven instead by asking whether there was life on Mars billions of years ago, which seems significantly more likely.”

However, “Overwhelming evidence exists that Mars had liquid water oceans roughly 4 billion years ago,” Lyons noted.

The central question astrobiologists ask is how that was possible. The red planet is farther from the sun than Earth is, and billions of years ago the sun generated less heat than it does today.

“To have made the planet warm enough for liquid surface water, its atmosphere would likely have needed an immense amount of greenhouse gas, carbon dioxide specifically,” explained Chris Tino, a UCR graduate student and co-first-author of the paper along with Eva Stüeken, a lecturer at the University of St. Andrews in Scotland.

Since sampling Mars’ atmosphere from billions of years ago to learn its carbon dioxide content is impossible, the team concluded that a site on Earth whose geology and chemistry bear similarities to the Martian surface might provide some of the missing pieces. They found it in southern Germany’s Nordlinger Ries crater.

A sample of suevite rock formed nearly 15 million years ago by the Ries Crater meteorite impact. Similarly impact-generated rocks exist on the rims of ancient crater lakes on Mars.
Credit: NASA

Formed roughly 15 million years ago after being struck by a meteorite, Ries crater features layers of rocks and minerals better preserved than almost anywhere on Earth.

The Mars 2020 rover will land in a similarly structured, well-preserved ancient crater. Both places featured liquid water in their distant past, making their chemical compositions comparable.

According to Tino, it’s unlikely that ancient Mars had enough oxygen to have hosted complex life forms like humans or animals.

However, some microorganisms could have survived if ancient Martian water had both a neutral pH level and was highly alkaline. Those conditions imply sufficient carbon dioxide in the atmosphere — perhaps thousands of times more than what surrounds Earth today — to warm the planet and make liquid water possible.

While pH measures the concentration of hydrogen ions in a solution, alkalinity is a measure dependent on several ions and how they interact to stabilize pH.

“Ries crater rock samples have ratios of nitrogen isotopes that can best be explained by high pH,” Stüeken said. “What’s more, the minerals in the ancient sediments tell us that alkalinity was also very high.”

However, Martian samples with mineral indicators for high alkalinity and nitrogen isotope data pointing to relatively low pH would demand extremely high levels of carbon dioxide in the past atmosphere.

The resulting carbon dioxide estimates could help solve the long-standing mystery of how an ancient Mars located so far from a faint early sun could have been warm enough for surface oceans and perhaps life. How such high levels could have been maintained and what might have lived beneath them remain important questions.

“Before this study, it wasn’t clear that something as straightforward as nitrogen isotopes could be used to estimate the pH of ancient waters on Mars; pH is a key parameter in calculating the carbon dioxide in the atmosphere,” Tino said.

Funding for this study came from the NASA Astrobiology Institute, where Lyons leads the Alternative Earths team based at UCR.

Included in the study were Gernot Arp of the Georg-August University of Göttingen and Dietmar Jung of the Bavarian State Office for the Environment.

When samples from NASA’s Mars 2020 rover mission are brought back to Earth, they could be analyzed for their nitrogen isotope ratios. These data could confirm the team’s suspicion that very high levels of carbon dioxide made liquid water possible and maybe even some forms of microbial life long ago.

“It could be 10-20 years before samples are brought back to Earth,” Lyons said. “But I am delighted to know that we have perhaps helped to define one of the first questions to ask once these samples are distributed to labs in the U.S. and throughout the world.”

Contacts and sources:
Holly Ober
University of California Riverside (UCR)

Publication: Nitrogen isotope ratios trace high-pH conditions in a terrestrial Mars analog site
Eva E. Stüeken1,2,*,†, Christopher Tino3,*, Gernot Arp4, Dietmar Jung5 and Timothy W. Lyons2,3

1. School of Earth and Environmental Sciences, University of St. Andrews, St. Andrews, Fife, KY16 9AL Scotland, UK.
2. Virtual Planetary Laboratory, University of Washington, Seattle, WA 98195, USA.
3. Department of Earth Sciences, University of California, Riverside, CA 92521, USA.
4. Georg-August-Universität Göttingen, Geowissenschaftliches Zentrum, Goldschmidtstrasse 3, 3.7077 Göttingen, Germany.
5. Bayerisches Landesamt für Umwelt, Geologischer Dienst, Hans-Högn-Straße 12, 95030 Hof/Saale, Germany.
* These authors contributed equally to this work.
Science Advances 26 Feb 2020:
Vol. 6, no. 9, eaay3440 DOI: 10.1126/sciadv.aay3440


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