
TL;DR
The paper proposes that many habitable exoplanets may lack detectable signs of life due to various scenarios, emphasizing the importance of understanding these possibilities in the search for extraterrestrial life.
Contribution
It introduces the hypothesis that most habitable worlds may show no detectable signs of life and discusses scenarios and implications for exoplanet biosignature detection.
Findings
Many habitable worlds could lack detectable biosignatures
Detection of life depends on specific biological and planetary conditions
Rejecting the hypothesis requires life to produce detectable biosignatures
Abstract
'Most habitable worlds in the cosmos will have no remotely detectable signs of life' is proposed as a biological hypothesis to be tested in studies of exoplanets. Habitable planets could be discovered elsewhere in the Universe, yet there are many hypothetical scenarios whereby the search for life on them could yield negative results. Scenarios for habitable worlds with no remotely detectable signatures of life include: planets that are habitable, but have no biosphere (Uninhabited Habitable Worlds); planets with life, but lacking any detectable surface signatures of that life (laboratory examples are provided) and planets with life, where the concentration of atmospheric gases produced or removed by biota are impossible to disentangle from abiotic processes because of the lack of detailed knowledge of planetary conditions (the 'problem of exoplanet thermodynamic uncertainty'). A…
Peer Reviews
No public reviews on file for this paper yet. If you reviewed it on a platform where reviews are public (OpenReview, ICLR, NeurIPS, ICML), you can paste yours below so the community can read it here.
Videos
No videos yet. Explain this paper in a talk, walkthrough, or lecture? Add one.
