“The Exoplanet Paradox” -Worlds With Low Oxygen May Be Teeming with Life Based on Early Earth History

Early Earth

 

“Understanding how Earth regulates climate both in the modern era but also in the distant past is critical for our understanding of planetary habitability,” said Noah Planavsky, a biogeochemist at Yale University. “This will help guide our search for life beyond our solar system and is an example of how the evolution of complex life fundamentally changed our planet.”

Research by a UC Riverside-led astrobiology team suggests oxygen conditions in the early surface ocean were low and unstable for most of the history of Earth and possibly delayed the emergence of animals for hundreds of millions of years.

The fact that microbial life flourished amid such low oxygen levels presents a problem for scientists hunting for extraterrestrial life, reports Lucas Joel in Scientific American. The presence of the gas in the atmosphere of a planet is considered a telltale sign that it could harbor life, explains Planavsky, a co-author of a study, published in the Proceedings of the National Academy of Sciences USA.

“Milky Way’s Sweet Spot” –Earth at Center of Galactic Habitable Zone

May Appear as Dead Planets

But if environments with extremely low oxygen concentrations can still support life, space telescopes designed to detect an abundance of the gas may never find such life. “Even [if such planets are] teeming with complex life, they may appear—from a remote detectability point of view—as dead planets,” Planavsky says.

Planavsky and his team tested rocks for concentrations of the element cerium, which serves as a proxy for ancient oxygen levels 1.7 billion years ago . Oxygen binds to cerium in seawater and removes it, leaving less cerium behind to be deposited in sedimentary rock. The measured cerium levels correspond to oxygen concentrations of about 0.1 percent of present atmospheric levels, the team reported. Oxygen binds to cerium in seawater and removes it, leaving less cerium behind to be deposited in sedimentary rock. The measured cerium levels correspond to oxygen concentrations of about 0.1 percent of present atmospheric levels.

JWST Not Capable of Detecting Low Levels

This data, Planavsky says, could help guide the construction of the next generation of telescopes designed to hunt for life on other worlds.  But current technology, such as NASA’s James Webb Space Telescope (JWST) is not capable of detecting oxygen at such low concentrations, says Edward Schwieterman, an astrobiologist at the University of California, Riverside, who was not involved in the work.

Early Earth –A Model for Emerging Life on Alien Planets?

Records of the earliest animals on Earth extend to roughly 700 to 800 million years ago, despite much older traces of microbial life in rocks deposited 3.7 billion years ago. Multiple factors might have contributed to this delay — but not with equal effect and in ways that are often not well understood.

A 2018   study led by former University of California, Riverside graduate student Chris Reinhard, now an assistant professor at Georgia Tech University and member of the UC Riverside-based Alternative Earths Team of the NASA Astrobiology Institute, may have found the critical control.

Reinhard and coauthors — including Timothy Lyons, UC Riverside distinguished professor of biogeochemistry and leader of the Alternative Earths Team –use Earth’s long history of biologic and planetary interactions and evolution to build predictive models of other habitable worlds–and Stephanie Olson — suggest in a paper published  in the Proceedings of the National Academy of Sciences that oxygen in the surface ocean was either absent or highly variable for most of Earth history, and this combination likely disfavored the emergence of animals.

The Trigger: Increase in Oxygen in the Oceans

The paper, called “Earth’s oxygen cycle and the evolution of animal life,” further asserts that at about 700 to 800 million years ago, an increase in oxygen in the oceans was likely the principal trigger for the earliest evolution of animals. Understanding the significance of this result requires some context, Lyons said.

“As animals eventually became large and mobile and developed ecologies that included predator-prey relationships 500 to 600 million years ago the metabolic demands for energy rose — hand in hand with increasing needs for oxygen,” Lyons said.

There is widespread agreement on that front. But the earliest animals were small, immobile, and likely able to survive on very low levels of O2. “This resilience of our earliest ancestors has sparked a spirited debate about the importance of oxygen during the earliest chapters of animal evolution,” Lyons said.

Recent related studies published in the journals Science and Geology by the Alternative Earths Team suggest that oxygen in the atmosphere may have been very low during the billion-year interval leading up to the beginnings of animal life. At the same time, however, concentrations in the critical surface ocean, where the animals lived, could in theory have been high enough, particularly given that oxygen was produced in these shallow marine settings through the activity of photosynthetic bacteria. These details are essential fuel in the oxygen debate.

Now, in the light of the new paper, a clearer story has emerged, and it may reconcile all the previous observations.

“Our newest results based on numerical model simulations of the shallow ocean indicate that oxygen, although present, remained mostly low enough and sufficiently patchy in its distributions to make conditions inhospitable even for the earliest, low-oxygen-tolerant animals,” Olson said.

The model reveals that the highest oxygen levels occurred mostly along the margins of continents, and, most importantly, conditions in those often disconnected coastal environments varied dramatically on time scales as short as the seasons.

Olson added: “It was the overall instability of oxygen in the surface ocean that held animal evolution at bay prior to the major increase in oxygen availability about 700 to 800 million years ago.”

Lyons summarizes by noting: “The animal-oxygen debate is a bit like a tennis match that lasts for years. Recently, we provided evidence for low oxygen in the biosphere prior to the rise of animals, and those on the other side of the net countered by highlighting the likelihood of low oxygen requirements at the beginnings of animal life, suggesting that oxygen availability was not the critical factor.”

Disequilibrium –The Unmistakable Signal of Alien Biological Life

The Last Word

When asked about about oxygen detection via the JWST, which is not optimized for that gas, NASAs’ Eddie Schwieterman told The Daily Galaxy:  “The O2 levels would have to be equivalent to or higher than modern levels. For the TRAPPIST-1 system specifically, O2 would have to be more abundant in order to bring out the O2-O2 bands. For that scenario, we focused on the abiotic O2 case, which would be easier to detect.

“However,”  Schwieterman  explained, “we will be able to go after methane because of the biosignature build-up predicted for M dwarf stars (even given the same flux, or the higher flux from the Archean or even Proterozoic). JWST is much more likely to find CH4-CO2 disequilibrium if it exists in the atmospheres of the TRAPPIST-1 planets or similar systems. This would be an exciting early Earth biosignature.

In the paper Timothy Lyons observed that if environments with extremely low oxygen concentrations can still support life, space telescopes designed to detect an abundance of the gas may never find such life. Even [if such planets are] teeming with complex life, they may appear—from a remote detectability point of view—as dead planets.”

Fast Facts About Exoplanets

“Recent studies have shown that JWST can be used for oxygen (O2) detection using clever approaches that are particularly well suited for identifying relatively high levels, such as on modern Earth or those produced readily through non biological processes via some planet-star relationships, Lyons wrote in an email to The Daily Galaxy. ” Lessons from ancient Earth, however, teach us that oxygen levels in the atmosphere can be much lower when tied to life even when microbial photosynthetic organisms abound in the surface oceans,” he explained.  “As such, our hope is that next generation telescopes beyond JWST will be optimized for measurements of much lower levels of O2 and O3 (ozone) on distant planets, which will vastly improve our ability to explore for a wide range of possible biological levels, including those that dominated many chapters of Earth’s early history.  In the absence of those enhanced capabilities, distant planets teeming with life, even complex oxygen-requiring life, may appear dead when viewed remotely.”

If the Alternative Earths team’s results are correct, even our earliest, low-oxygen kin would have suffered in a world still very far removed from the one we enjoy today. Only when oxygen rose and stabilized did complex life find a clear path forward.

In addition to Lyons, Olson and Reinhard, Douglas Erwin of the Smithsonian National Museum of Natural History and Noah Planavsky of Yale University were co-authors of the paper.

Image credit top of page: Shutterstock License

Avi Shporer, Research Scientist, with the MIT Kavli Institute for Astrophysics and Space Research via Timothy Lyons, Eddie Schwieterman Yale University, UC Riverside and Scientific American 

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