To understand exoplanet habitability, we need a better understanding of stellar flaring

One of the main questions in exoplanet science concerns M dwarfs (red dwarfs) and the habitability of exoplanets that orbit them. These stars are known for their prolific and energetic flaring, and that’s a problem. M dwarfs are so small that their habitable zones are in tight proximity to them, putting any potentially habitable planets in the direct line of fire of all this dangerous flaring.