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....

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Detalles Bibliográficos
Autores principales: Shapiro, Anna V., Brühl, Christoph, Klingmüller, Klaus, Steil, Benedikt, Shapiro, Alexander I., Witzke, Veronika, Kostogryz, Nadiia, Gizon, Laurent, Solanki, Sami K., Lelieveld, Jos
Formato: Online Artículo Texto
Lenguaje:English
Publicado: Nature Publishing Group UK 2023
Materias:
Article
Acceso en línea:https://www.ncbi.nlm.nih.gov/pmc/articles/PMC10113254/
https://www.ncbi.nlm.nih.gov/pubmed/37072387
http://dx.doi.org/10.1038/s41467-023-37195-4

Internet

https://www.ncbi.nlm.nih.gov/pmc/articles/PMC10113254/
https://www.ncbi.nlm.nih.gov/pubmed/37072387
http://dx.doi.org/10.1038/s41467-023-37195-4

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