
In this artist’s concept, X-ray and extreme ultraviolet light from a young red dwarf star cause ions to escape from an exoplanet’s atmosphere. Scientists have developed a model that estimates the oxygen ion escape rate on planets around red dwarfs, which plays an important role in determining an exoplanet’s habitability. (screen shot from video) Credit: NASA Goddard/Conceptual Image Lab; Michael Lentz, animator/Genna Duberstein, producer
The search for life beyond Earth starts in habitable zones could potentially allow liquid water to pool on a planet’s surface. New NASA research suggests some of these zones might not actually be able to support life due to frequent stellar eruptions from young red dwarf stars...
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