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Tidal Heating of Earth-like Exoplanets around M Stars: Thermal, Magnetic, and Orbital Evolutions
The internal thermal and magnetic evolution of rocky exoplanets is critical to their habitability. We focus on the thermal-orbital evolution of Earth-mass planets around low-mass M stars whose radiative habitable zone overlaps with the “tidal zone,” where tidal dissipation is expected to be a signif...
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| Publicado en: | Astrobiology |
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| Main Authors: | , |
| Formato: | Artigo |
| Idioma: | Inglês |
| Publicado: |
Mary Ann Liebert, Inc.
2015
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| Assuntos: | |
| Acceso en liña: | https://ncbi.nlm.nih.gov/pmc/articles/PMC4582693/ https://ncbi.nlm.nih.gov/pubmed/26393398 https://ncbi.nlm.nih.govhttp://dx.doi.org/10.1089/ast.2015.1325 |
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