Metal-Rich Stars Are Less Suitable for the Evolution of Life on Their Planets
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Metal-rich stars are less suitable for the evolution of life on their planets
Atmospheric ozone and oxygen protect the terrestrial biosphere against harmful ultraviolet (UV) radiation. Here, we model atmospheres of Earth-like planets hosted by stars with near-solar effective temperatures (5300 to 6300 K) and a broad range of metallicities covering known exoplanet host stars. We show that paradoxically, although metal-rich stars emit substantially less ultraviolet radiation than metal-poor stars, the surface of their plane…
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Leaning Left1Leaning Right0Center2Last UpdatedBias Distribution67% Center
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