Water contents of Earth-mass planets around M dwarfs
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Earth-mass planets with Earth-like water contents orbiting M-dwarfs have a 10-100 times reduced likelihood than around G dwarfs.
“Particularly, Tian & Ida (2015) argued that Earth-mass planets with Earth-like water contents orbiting M-dwarfs have a 10-100 times reduced likelihood than around G dwarfs.”
From ABOUT EXOBIOLOGY: THE CASE FOR DWARF K STARS (2016) · cites this paper as Tian & Ida (2015)
Accreting planets in the CLI-HZ around stars cooler than K5 (including M-dwarfs) are most likely subjected to runaway greenhouse processes.
“It has also been pointed out that accreting planets, if formed, subsequently located in the CLI-HZ around stars cooler than K5 (including the full range of M-dwarfs) are most likely subjected to runaway greenhouse processes”
From ABOUT EXOBIOLOGY: THE CASE FOR DWARF K STARS (2016) · cites this paper as Tian & Ida 2015
Such planets may lose substantial amounts of initially delivered water and emerge as almost certainly uninhabitable dry planets ('desert worlds').
“and thus may lose substantial amounts of water initially delivered to them (Ramirez & Kaltenegger 2014; Luger & Barnes 2015; Tian & Ida 2015), thus emerging as (almost certainly) uninhabitable dry planets ('desert worlds').”
From ABOUT EXOBIOLOGY: THE CASE FOR DWARF K STARS (2016) · cites this paper as Tian & Ida 2015
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“…of M-dwarfs) are most likely subjected to runaway greenhouse processes, and thus may lose substantial amounts of water initially delivered to them (Ramirez & Kaltenegger 2014; Luger & Barnes 2015; Tian & Ida 2015), thus emerging as (almost certainly) uninhabitable dry planets (“desert worlds”).”
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New Insights into Cosmic-Ray-induced Biosignature Chemistry in Earth-like Atmospheres
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Dependence of Biological Activity on the Surface Water Fraction of Planets
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Near-infrared transmission spectrum of TRAPPIST-1 h usingHubbleWFC3 G141 observations
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- Authors
- Tian, F., & Ida, S.
- Affiliations
- Tsinghua University (CN)
- Tokyo Institute of Technology (JP)
- Corresponding author
- Tian, Feng
- Venue
- Nature Geoscience
- Published
- 2015-02-16
- Volume
- 8
- Issue
- 3
- Pages
- 177-180
- ISSN
- 1752-0894 (ISSN-L)
- 1752-0908
- OpenAlex
- W2035144479
- Cited by
- 162
- References
- 38
- Citations by year
- 2026: 4 · 2025: 7 · 2024: 11 · 2023: 7 · 2022: 16 · 2021: 16 · 2020: 19 · 2019: 24 · 2018: 22 · 2017: 10 · 2016: 11 · 2015: 14
- FWCI
- 10.81
- Type
- journal article
- Language
- en
- Open access
- closed
- Licence
- www.springer.com/tdm (tdm)
- Locations
- Nature Geoscience (publishedVersion)
- Topics
- Physical Sciences › Physics and Astronomy › Astronomy and Astrophysics › Stellar, planetary, and galactic studies
- Physical Sciences › Physics and Astronomy › Astronomy and Astrophysics › Space Science and Extraterrestrial Life
- Physical Sciences › Physics and Astronomy › Astronomy and Astrophysics › Astro and Planetary Science
- Keywords
- M dwarfs, habitable planets, moisture content, Earth-mass planets, water loss, hydrodynamic escape, planet population synthesis, ocean planets, habitability, G dwarfs
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