Metal-rich stars are less suitable for the evolution of life on their planets

Metal-rich stars are less suitable for the evolution of life on their planets

Abstract 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 hos...

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Bibliographic Details
Main Authors: Anna V. Shapiro, Christoph Brühl, Klaus Klingmüller, Benedikt Steil, Alexander I. Shapiro, Veronika Witzke, Nadiia Kostogryz, Laurent Gizon, Sami K. Solanki, Jos Lelieveld
Format: Article
Language:English
Published: Nature Portfolio 2023-04-01
Series:Nature Communications
Online Access:https://doi.org/10.1038/s41467-023-37195-4

Internet

https://doi.org/10.1038/s41467-023-37195-4

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