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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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Detalhes bibliográficos
Publicado no:Proc Natl Acad Sci U S A
Main Authors: Kite, Edwin S., Barnett, Megan N.
Formato: Artigo
Idioma:Inglês
Publicado em: National Academy of Sciences 2020
Assuntos:
Acesso em linha: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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