Exoplanet Biosignatures: A Review of Remotely Detectable Signs of Life
Edward W. Schwieterman, Nancy Y. Kiang, Mary N. Parenteau, Chester E., Harman, Shiladitya DasSarma, Theresa M. Fisher, Giada N. Arney, Hilairy E., Hartnett, Christopher T. Reinhard, Stephanie L. Olson, Victoria S. Meadows,, Charles S. Cockell, Sara I. Walker, John Lee Grenfell

TL;DR
This review paper summarizes current knowledge on potential biosignatures for detecting life on exoplanets, emphasizing advances since 2002 and discussing methods to assess biosignature plausibility from remote observations.
Contribution
It provides a comprehensive overview of exoplanet biosignatures, integrating recent advances and highlighting areas for future research without proposing new strategies.
Findings
Compiled a state-of-the-art overview of biosignatures
Reviewed methods for assessing chemical disequilibrium
Discussed tools for estimating minimum biomass
Abstract
In the coming years and decades, advanced space- and ground-based observatories will allow an unprecedented opportunity to probe the atmospheres and surfaces of potentially habitable exoplanets for signatures of life. Life on Earth, through its gaseous products and reflectance and scattering properties, has left its fingerprint on the spectrum of our planet. Aided by the universality of the laws of physics and chemistry, we turn to Earth's biosphere, both in the present and through geologic time, for analog signatures that will aid in the search for life elsewhere. Considering the insights gained from modern and ancient Earth, and the broader array of hypothetical exoplanet possibilities, we have compiled a state-of-the-art overview of our current understanding of potential exoplanet biosignatures including gaseous, surface, and temporal biosignatures. We additionally survey biogenic…
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