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Exoplanet secondary atmosphere loss and revival
The next step on the path toward another Earth is to find atmospheres similar to those of Earth and Venus—high–molecular-weight (secondary) atmospheres—on rocky exoplanets. Many rocky exoplanets are born with thick (>10 kbar) H(2)-dominated atmospheres but subsequently lose their H(2); this proce...
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| Publicat a: | Proc Natl Acad Sci U S A |
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| Autors principals: | , |
| Format: | Artigo |
| Idioma: | Inglês |
| Publicat: |
National Academy of Sciences
2020
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| Matèries: | |
| Accés en línia: | https://ncbi.nlm.nih.gov/pmc/articles/PMC7414166/ https://ncbi.nlm.nih.gov/pubmed/32694204 https://ncbi.nlm.nih.govhttp://dx.doi.org/10.1073/pnas.2006177117 |
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