SETI Talks: Is Oxygen Really a Biosignature?

SETI Talks

Tags: SETI Talks, Outreach, Astrobiology

Time: Wednesday, Jun 23, 2021 -

Location: Online

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Biosignatures, the footprint of life on other planets, or exoplanets, could be the easiest way for astronomers to prove that we are not alone, and oxygen has been for decades the top contenders in proving that life exists elsewhere. But how truly useful is oxygen as a biosignature?

In Earth’s history, oxygen is the byproduct of photosynthesizers such as plants, algae and cyanobacteria. With the fast growth of the field of exoplanets and the arrival of future extremely large telescopes and space-based telescopes that could soon find oxygen signatures, or its light-modified form, ozone, are we on the verge of finding life on an exoplanet?

Scientists have been busy modeling exoplanet formations, chemistry and their atmosphere, and as a byproduct of this work, they succeeded in poking holes in the atmospheric oxygen-means-life scenario. We invited two scientists to discuss the discovery of potential false positives for atmospheric oxygen as a biosignature. Jade Checlair is a planetary scientist at the University of Chicago who models the atmosphere and climate of habitable exoplanets and will show how the observation of oxygen on a large number of exoplanets would allow astronomers to discover true Earth-like exoplanets. Joshua Krissansen-Totton, an astrobiologist at the University of California, Santa Cruz, models the atmospheric evolution of rocky planets to anticipate exoplanet biosignatures and their false positives.

Hypothetical scenarios have been proposed for non-biological oxygen accumulation on exoplanets, especially around M-dwarf stars, as oxygen remains behind as hydrogen escapes the atmosphere of their planets. The researchers will also discuss numerous other ways that planet atmospheres can be filled with oxygen from a non-biological source.

In this bleak environment, there is still hope. Oxygen false positives could, in principle, be distinguished from inhabited planets using contextual clues and corroborating signs of life. But the task may not be straightforward, and proving beyond reasonable doubt that there is life on exoplanets could require telescopes much more advanced than anything currently being built.

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Jade Checlair

Jade Checlair is a planetary scientist at the University of Chicago, where she is currently completing her PhD. Her research interests broadly include modeling the atmosphere and climate of habitable exoplanets and simulating future observations to detect extraterrestrial life. Her current work focuses on developing statistical tests of habitability that could be carried out with future NASA direct imaging instruments. In particular, she is interested in testing the concept of the habitable zone and its boundaries by using large numbers of exoplanets. Previously, she also worked on studying the climate of tidally locked planets orbiting M-stars. Notably, she showed that they are not expected to jump in and out of globally glaciated states as Earth-like planets do.

Joshua Krissansen-Totton

Dr. Joshua Krissansen-Totton is a planetary scientist and astrobiologist at the University of California, Santa Cruz. His research focuses on modeling the atmospheric evolution of rocky planets to anticipate exoplanet biosignatures and false positives. Joshua's research interests also encompass modeling the coevolution of life and the environment to better understand the early Earth. In 2019 he was selected as a NASA Sagan Fellow.