Can small, red dwarf stars (M class) really support extraterrestrial habitability? Red dwarf stars are much cooler (~10% brightness) and smaller (10 to 50%) than our Sun. This pushes the habitable zone for planets much closer to the parent star of the system which, in turn, causes planets to become tidally locked (one hemisphere always facing the star like the Moon is to Earth). Also, being closer the planets are more exposed to infrared and flaring radiation. Yet, they have incredible lifespans in trillions of years (vs. the Sun’s 10B year lifespan) and comprise about 75% of all stars in the galaxy.
Gale & Wandell (2017) argue that perhaps tidally locked planets orbiting red dwarfs may develop life in zones of “continuous illumination with a considerable component of photosynthetic 400-700 nm radiation. This is analogous to the lush summer growth of vegetation on Earth, at very high latitude.” You can read the paper here: The Potential of Planets Orbiting Red Dwarf Stars to Support Oxygenic Photosynthesis and Complex Life
With the large number of red dwarfs, maybe we’ll discover biotic markers in future missions!