Red dwarf suns are the most common in the universe, and many of the exoplanets officially discovered so far orbit this type of “cool” star. Red dwarfs are much smaller and less powerful than the G type stars such as our own sun, and it is easier to detect exoplanets orbiting them because of their reduced size and energy.
As a result, a number of relatively nearby red dwarf stars — in the Trappist-1 system, Proxima Centauri and Barnard’s star, for instance — are avidly studied for their potential habitability. The exoplanets of red dwarfs tend to orbit much closer than around other larger stars, but the suns have that lower radiative power and so some are considered habitable candidates. And if they are indeed habitable, they could be for a very long time because red dwarfs live much longer than most other stars.
But there have been two (at least) problems with the habitable red dwarf exoplanet scenario. The first is that many of the planets so close to their star are tidally locked, meaning that only one side ever faces the sun. Some have argued a tidally locked planet can still be habitable, but it would not be easy.
More crucial, however, is that red dwarf stars are known for sending out many, many powerful solar flares, especially during their solar infancy and childhood. These high radiation and particle flares could and would potentially kill any life emerging on a dwarf exoplanet, and the stellar flares could even sterilize the planets’ atmosphere for all time. Although direct observations have not shown this deadly scenario to be inevitable or even present, the red dwarf flaring is well documented. And so potentially the flares have seemed to rule out, or make improbable, life on an estimated 75 percent of the stars in our galaxy.
This is why there is interest in the astrobiology world about a new paper that addresses a particular kind of stellar flare that would hit red dwarf exoplanets. Such studies of how the behavior of a star effects orbiting planets is one of the less well studied aspects of the exoplanet field, and so the paper is especially welcomed.
And the results suggests that the red dwarf flares would strike orbiting exoplanets from an angle rather than straight on, and therefore would land in a way that would theoretically minimize damage to potential atmospheres and life.… Read more