Geoscience and the Search for Life Beyond the Solar System
Rory Barnes, Anat Shahar, Cayman Unterborn, Hilairy Hartnett, Ariel, Anbar, Brad Foley, Peter Driscoll, S.-H. Dan Shim, Thomas Quinn, Kayla, Iacovino, Stephen Kane, Steven Desch, Norman Sleep, David Catling

TL;DR
This paper discusses how geophysical and geochemical insights are crucial for interpreting potential biosignatures on exoplanets, emphasizing the need for models to distinguish biological signals from abiotic features in upcoming observations.
Contribution
It highlights the importance of integrating geophysical and geochemical models to interpret exoplanet biosignatures and identifies key areas for future research in this interdisciplinary field.
Findings
Exoplanet interior properties can be constrained by atmospheric and stellar observations.
Plausible models are needed to interpret biosignatures and rule out abiotic explanations.
Understanding Earth's biogeochemical evolution informs exoplanet habitability assessments.
Abstract
How can scientists conclude with high confidence that an exoplanet hosts life? As telescopes come on line over the next 20 years that can directly observe photons from terrestrial exoplanets, this question will dictate the activities of many scientists across many fields. The expected data will be sparse and with low signal-to-noise, which will make disentangling biosignatures from abiotic features challenging. Our Earth is not just unique in that it hosts life, it is also the only terrestrial planet with direct observations of its interior through seismic waves, and compositional evolution through field and laboratory measurements. This extensive research reveals a planet born from collisions between worlds, followed by a complicated biogeochemical evolution. Exoplanet interiors, on the other hand, can only be constrained by the following observations: 1) photometric and spectroscopic…
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Taxonomy
TopicsAstro and Planetary Science · Stellar, planetary, and galactic studies · Astrophysics and Star Formation Studies
