Scientists harness plasma clumps trapped in stellar magnetospheres to assess habitability around M dwarf stars
How does a star affect the makeup of its planets? And what does this mean for the habitability of distant worlds? Carnegie's Luke Bouma is exploring a new way to probe this critical question—using naturally occurring space weather stations that orbit at least 10% of M dwarf stars during their early lives. He presented his work at the American Astronomical Society meeting (AAS 247) held in Phoenix in January.
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