The Case for a Gaian Bottleneck: The Biology of Habitability
Abstract
The prerequisites and ingredients for life seem to be abundantly available in the Universe. However, the Universe does not seem to be teeming with life. The most common explanation for this is a low probability for the emergence of life (an emergence bottleneck), notionally due to the intricacies of the molecular recipe. Here, we present an alternative Gaian bottleneck explanation: If life emerges on a planet, it only rarely evolves quickly enough to regulate greenhouse gases and albedo, thereby maintaining surface temperatures compatible with liquid water and habitability. Such a Gaian bottleneck suggests that (i) extinction is the cosmic default for most life that has ever emerged on the surfaces of wet rocky planets in the Universe and (ii) rocky planets need to be inhabited to remain habitable. In the Gaian bottleneck model, the maintenance of planetary habitability is a property more associated with an unusually rapid evolution of biological regulation of surface volatiles than with the luminosity and distance to the host star.
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These effects and other factors could greatly diminish the likelihood of development of multicellular complex life.
“These effects as well as other factors (including biological and chemical bottlenecks, asteroid bombardments, among others), as recently discussed by Chopra & Lineweaver (2016) and references therein, could greatly diminish the likelihood of development of multicellular complex life.”
From ABOUT EXOBIOLOGY: THE CASE FOR DWARF K STARS (2016) · cites this paper as Chopra & Lineweaver (2016)
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ABOUT EXOBIOLOGY: THE CASE FOR DWARF K STARS
Cuntz, M., & Guinan, E. F. (2016) · The Astrophysical Journal · doi:10.3847/0004-637x/827/1/79 · Cited by 77 · see citing works
“The lack of evidence of technologically advanced civilizations such as radio signals and other modes of one-way communication are referred to as the Fermi’s Paradox, which continues to remain unresolved (see Chopra & Lineweaver 2016).”
BackgroundInfluentialHarrison, T. M. (2020) · doi:10.1007/978-3-030-46687-9 · Cited by 53 · see citing works
- Authors
- Chopra, A., & Lineweaver, C. H.
- Affiliations
- Australian National University (AU)
- Venue
- Astrobiology
- Publisher
- SAGE Publications
- Published
- 2016-01
- Volume
- 16
- Issue
- 1
- Pages
- 7-22
- ISSN
- 1531-1074 (ISSN-L)
- 1557-8070
- OpenAlex
- W2267142438
- Cited by
- 115
- References
- 21
- Citations by year
- 2026: 5 · 2025: 11 · 2024: 9 · 2023: 28 · 2022: 13 · 2021: 7 · 2020: 7 · 2019: 5 · 2018: 12 · 2017: 13 · 2016: 5
- FWCI
- 5.58
- Type
- journal article
- Language
- en
- Open access
- closed
- Locations
- Astrobiology (publishedVersion)
- PubMed (publishedVersion)
- ANU Open Research (Australian National University) (submittedVersion)
- Funders
- Australian National University
- Topics
- Physical Sciences › Physics and Astronomy › Astronomy and Astrophysics › Space Science and Extraterrestrial Life
- Physical Sciences › Earth and Planetary Sciences › Atmospheric Science › Earth Systems and Cosmic Evolution
- Physical Sciences › Physics and Astronomy › Astronomy and Astrophysics › Origins and Evolution of Life
- Keywords
- habitability, surface temperature, liquid water, extinction, evolution of life, origin of life
- MeSH terms
- Carbonates, Extraterrestrial Environment, Models, Theoretical, Time Factors, Water, Planets, Silicates, Exobiology, Extinction, Biological
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