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XUV-Exposed, Non-Hydrostatic Hydrogen-Rich Upper Atmospheres of Terrestrial Planets. Part I: Atmospheric Expansion and Thermal Escape
The recently discovered low-density “super-Earths” Kepler-11b, Kepler-11f, Kepler-11d, Kepler-11e, and planets such as GJ 1214b represent the most likely known planets that are surrounded by dense H/He envelopes or contain deep H(2)O oceans also surrounded by dense hydrogen envelopes. Although these...
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| Autori principali: | , , , , , , , , |
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| Natura: | Artigo |
| Lingua: | Inglês |
| Pubblicazione: |
Mary Ann Liebert, Inc.
2013
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| Soggetti: | |
| Accesso online: | https://ncbi.nlm.nih.gov/pmc/articles/PMC3865622/ https://ncbi.nlm.nih.gov/pubmed/24251443 https://ncbi.nlm.nih.govhttp://dx.doi.org/10.1089/ast.2012.0957 |
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