An exploration of origin of life for exoplanetary science

The factors that enable life to begin define the difference between an inhabited planet and one that is simply habitable. While used extensively in Origins, Worlds, and Life: A Decadal Strategy for Planetary Science and Astrobiology 2023–2032 (abbreviated “OWL” in this paper), the term origin of lif...

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Main Authors: Finnegan Keller, Tiffany Kataria, Laura M. Barge, Pin Chen, Yuk Yung, Jessica M. Weber
Format: Article
Language:English
Published: Frontiers Media S.A. 2025-03-01
Series:Frontiers in Astronomy and Space Sciences
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Online Access:https://www.frontiersin.org/articles/10.3389/fspas.2025.1544426/full
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author Finnegan Keller
Tiffany Kataria
Laura M. Barge
Pin Chen
Yuk Yung
Jessica M. Weber
author_facet Finnegan Keller
Tiffany Kataria
Laura M. Barge
Pin Chen
Yuk Yung
Jessica M. Weber
author_sort Finnegan Keller
collection DOAJ
description The factors that enable life to begin define the difference between an inhabited planet and one that is simply habitable. While used extensively in Origins, Worlds, and Life: A Decadal Strategy for Planetary Science and Astrobiology 2023–2032 (abbreviated “OWL” in this paper), the term origin of life is never mentioned in Pathways to Discovery in Astronomy and Astrophysics for the 2020s (notated as “Astro2020” in this paper). While the chapters on the search for life in the solar system in OWL treat the origin of life as a central concept, the exoplanet focused chapters of the OWL and Astro2020 reports mostly do not mention origin of life science, particularly with respect to how it intersects with biosignature identification and interpretation. To begin to fill this gap, we describe the set of conditions that are required for life to begin and suggest that they may be distinct from those that make an environment habitable. Finally, we present a putative list of origin of life processes that may be observable on exoplanets and outline the relevance of future planetary science and astrophysics missions to this topic. Given the complexity of detecting these conditions beyond the solar system, we argue that while looking for signs of the origin of life on exoplanets could be fruitful in determining which are worthy of further study, the concept is likely more appropriate for distinguishing true biosignatures from false positives. Ensuring that future facilities like the Large Interferometer For Exoplanets (LIFE) and the Habitable Worlds Observatory (HWO) can constrain origin of life conditions is necessary for life detection searches beyond the solar system.
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spelling doaj-art-edc3c62cb5cf4a05b4c8258bc7743ac12025-08-20T02:51:53ZengFrontiers Media S.A.Frontiers in Astronomy and Space Sciences2296-987X2025-03-011210.3389/fspas.2025.15444261544426An exploration of origin of life for exoplanetary scienceFinnegan Keller0Tiffany Kataria1Laura M. Barge2Pin Chen3Yuk Yung4Jessica M. Weber5Department of Physics, Brown University, Providence, RI, United StatesJet Propulsion Laboratory, California Institute of Technology, Pasadena, CA, United StatesJet Propulsion Laboratory, California Institute of Technology, Pasadena, CA, United StatesJet Propulsion Laboratory, California Institute of Technology, Pasadena, CA, United StatesDivision of Geological and Planetary Sciences, California Institute of Technology, Pasadena, CA, United StatesJet Propulsion Laboratory, California Institute of Technology, Pasadena, CA, United StatesThe factors that enable life to begin define the difference between an inhabited planet and one that is simply habitable. While used extensively in Origins, Worlds, and Life: A Decadal Strategy for Planetary Science and Astrobiology 2023–2032 (abbreviated “OWL” in this paper), the term origin of life is never mentioned in Pathways to Discovery in Astronomy and Astrophysics for the 2020s (notated as “Astro2020” in this paper). While the chapters on the search for life in the solar system in OWL treat the origin of life as a central concept, the exoplanet focused chapters of the OWL and Astro2020 reports mostly do not mention origin of life science, particularly with respect to how it intersects with biosignature identification and interpretation. To begin to fill this gap, we describe the set of conditions that are required for life to begin and suggest that they may be distinct from those that make an environment habitable. Finally, we present a putative list of origin of life processes that may be observable on exoplanets and outline the relevance of future planetary science and astrophysics missions to this topic. Given the complexity of detecting these conditions beyond the solar system, we argue that while looking for signs of the origin of life on exoplanets could be fruitful in determining which are worthy of further study, the concept is likely more appropriate for distinguishing true biosignatures from false positives. Ensuring that future facilities like the Large Interferometer For Exoplanets (LIFE) and the Habitable Worlds Observatory (HWO) can constrain origin of life conditions is necessary for life detection searches beyond the solar system.https://www.frontiersin.org/articles/10.3389/fspas.2025.1544426/fullexoplanetsorigin of lifehabitabilitybiosignatureslife detection
spellingShingle Finnegan Keller
Tiffany Kataria
Laura M. Barge
Pin Chen
Yuk Yung
Jessica M. Weber
An exploration of origin of life for exoplanetary science
Frontiers in Astronomy and Space Sciences
exoplanets
origin of life
habitability
biosignatures
life detection
title An exploration of origin of life for exoplanetary science
title_full An exploration of origin of life for exoplanetary science
title_fullStr An exploration of origin of life for exoplanetary science
title_full_unstemmed An exploration of origin of life for exoplanetary science
title_short An exploration of origin of life for exoplanetary science
title_sort exploration of origin of life for exoplanetary science
topic exoplanets
origin of life
habitability
biosignatures
life detection
url https://www.frontiersin.org/articles/10.3389/fspas.2025.1544426/full
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