Scientists have detected the first direct evidence of a coronal mass ejection from a star beyond our Sun, specifically the M dwarf StKM1-1262. This massive expulsion of plasma, observed as a Type II radio burst, offers crucial insights into the space weather experienced by exoplanets, particularly those orbiting M dwarfs, and their potential for habitability.from Science News: Fresh Discoveries, Research & Breakthroughs https://ift.tt/sWxr29b
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