Flare-driven habitability: Expanding life’s potential around low-mass stars
Abstract
flaring stars, three planets are located within both the refined UV-HZ and the LW-HZ without causing ozone depletion. Our findings highlight the significant role of flares in expanding the potential for life around low-mass stars, offering a revised perspective on exoplanet habitability criteria.
Fields of Study & Subjects
Stellar
planetary
and galactic studies
Space Science and Extraterrestrial Life
Planetary Science and Exploration
Publication details
- Journal / source
- The Innovation
- Volume
- 7
- Issue
- 4
- Pages
- 101265–101265
- Publication date
- 15 January 2026
- Language
- EN