Recent modelling suggests that Earth-mass planets in the habitable zones of Sun-like stars could evolve into rocky worlds topped by helium-dominated atmospheres.
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Acknowledgements
The author thanks R. Wordsworth, C. Cherubim, I. Malsky, A. Bello-Arufe, and M. Zilinskas for helpful discussions. This article was written at the Jet Propulsion Laboratory, California Institute of Technology, under a contract with the National Aeronautics and Space Administration (80NM0018D0004).
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Hu, R. A new class of rocky exoplanets?. Nat Astron 9, 943–944 (2025). https://doi.org/10.1038/s41550-025-02607-6
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DOI: https://doi.org/10.1038/s41550-025-02607-6