Searching for Life-As-We-Don't-Know-It: Mission-relevant Application of Assembly Theory for Exoplanet Life Detection

Fuente: arXiv
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Autores principales: Walker, Sara, Janin, Estelle, Shkolnik, Evgenya, Slocombe, Louie, Cronin, Leroy
Formato: Preprint
Publicado: 2026
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author Walker, Sara
Janin, Estelle
Shkolnik, Evgenya
Slocombe, Louie
Cronin, Leroy
author_facet Walker, Sara
Janin, Estelle
Shkolnik, Evgenya
Slocombe, Louie
Cronin, Leroy
contents This white paper introduces a framework for applying Assembly Theory (AT) to planetary atmospheres as a biosignature framework suitable for the Habitable Worlds Observatory (HWO). AT quantifies the minimum combinatorial complexity required to co-construct an observed ensemble of molecular species, providing a measure of how much selection and evolution is encoded in a planetary atmosphere's chemical space, without assuming any specific biochemistry, kinetics nor metabolism. We outline some forthcoming results applying this framework and how it can be extended to population-level exoplanet studies, validated against existing spectroscopic data, and used to directly inform HWO instrumental requirements. Rather than imposing a binary alive/dead classification, AT-based atmospheric analysis would provide a continuous measure of planetary complexity, opening a path toward detecting life-as-we-don't-know-it.
format Preprint
id arxiv_https___arxiv_org_abs_2603_11086
institution arXiv
publishDate 2026
record_format arxiv
spellingShingle Searching for Life-As-We-Don't-Know-It: Mission-relevant Application of Assembly Theory for Exoplanet Life Detection
Walker, Sara
Janin, Estelle
Shkolnik, Evgenya
Slocombe, Louie
Cronin, Leroy
Instrumentation and Methods for Astrophysics
Earth and Planetary Astrophysics
This white paper introduces a framework for applying Assembly Theory (AT) to planetary atmospheres as a biosignature framework suitable for the Habitable Worlds Observatory (HWO). AT quantifies the minimum combinatorial complexity required to co-construct an observed ensemble of molecular species, providing a measure of how much selection and evolution is encoded in a planetary atmosphere's chemical space, without assuming any specific biochemistry, kinetics nor metabolism. We outline some forthcoming results applying this framework and how it can be extended to population-level exoplanet studies, validated against existing spectroscopic data, and used to directly inform HWO instrumental requirements. Rather than imposing a binary alive/dead classification, AT-based atmospheric analysis would provide a continuous measure of planetary complexity, opening a path toward detecting life-as-we-don't-know-it.
title Searching for Life-As-We-Don't-Know-It: Mission-relevant Application of Assembly Theory for Exoplanet Life Detection
topic Instrumentation and Methods for Astrophysics
Earth and Planetary Astrophysics
url https://arxiv.org/abs/2603.11086