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Water contents of Earth-mass planets around M dwarfs
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“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)
In the citing paper
“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
In the citing paper
“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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Metadata
- 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 › Earth and Planetary Sciences › Space and Planetary Science › 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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