Habitability of Tidally Locked Planets Around Red Dwarfs: Climate Boundaries and Biosignature Prospects
To the point
A. Wandel and J. Gale argue that planets around red dwarfs, even when tidally locked, can maintain climates with liquid water and potential life across a range of atmospheres, might support oxygenic photosynthesis, and offer detectable biosignatures, with upcoming data from TESS and JWST helping to test these ideas.
