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Extreme Water Loss and Abiotic O(2) Buildup on Planets Throughout the Habitable Zones of M Dwarfs
We show that terrestrial planets in the habitable zones of M dwarfs older than ∼1 Gyr could have been in runaway greenhouses for several hundred million years following their formation due to the star's extended pre-main sequence phase, provided they form with abundant surface water. Such prolo...
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| Publicado no: | Astrobiology |
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| Main Authors: | , |
| Formato: | Artigo |
| Idioma: | Inglês |
| Publicado em: |
Mary Ann Liebert, Inc.
2015
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| Assuntos: | |
| Acesso em linha: | https://ncbi.nlm.nih.gov/pmc/articles/PMC4323125/ https://ncbi.nlm.nih.gov/pubmed/25629240 https://ncbi.nlm.nih.govhttp://dx.doi.org/10.1089/ast.2014.1231 |
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