The Earth is a rocky planet in the so-called classical habitable zone (HZ), with a surface ocean taking up just ~10–4 of its total mass. A study suggests that 5–10% of Earth-sized planets in the HZ around red dwarfs are ‘Earth-like’: rocky, with a small but non-zero amount of water on their surface.
References
Tian, F. & Ida, S. Nat. Geo. 8, 177–180 (2015).
Ramirez, R. & Kaltenegger, L. Astrophys. J. 2, L25 (2014).
Kimura, T. & Ikoma, M. Nat. Astron. https://doi.org/10.1038/s41550-022-01781-1 (2022).
Ida, S. & Lin, D. N. C. Astrophys. J. 604, 388–413 (2004).
Mordasini, C., Alibert, Y. & Benz, W. Astron. Astrophys. 501, 1139–1160 (2009).
Benz, W., Ida, S., Alibert, Y., Lin, D. N. C. & Mordasini, C. in Protostars and Planets VI (ed. Beuther, H. et al.) 691–713 (Univ. Arizona Press, 2014).
Fei, H. et al. Sci. Adv. 3, e1603024 (2017).
Nomura, R. et al. Science 343, 522–525 (2014).
Raymond, S. N., Quinn, T. & Lunine, J. I. Icarus 168, 1–17 (2004).
Cummings, A. et al. Publ. Astron. Soc. Pacific 120, 531–554 (2008).
Ikoma, M. & Genda, H. Astrophys. J. 648, 696–7062 (2006).
Lichtenberg, T. et al. Nat. Astron. 3, 307–313 (2019).
Author information
Authors and Affiliations
Corresponding author
Ethics declarations
Competing interests
The author declares no competing interests.
Rights and permissions
About this article
Cite this article
Ida, S. Predicting ‘Earth-like’ planets around red dwarfs. Nat Astron 6, 1231–1232 (2022). https://doi.org/10.1038/s41550-022-01822-9
Published:
Issue Date:
DOI: https://doi.org/10.1038/s41550-022-01822-9
- Springer Nature Limited