Low Hesperian P(CO2) constrained from in situ mineralogical analysis at Gale Crater, Mars

Carbon dioxide is an essential atmospheric component in martian climate models that attempt to reconcile a faint young sun with planetwide evidence of liquid water in the Noachian and Early Hesperian. In this study, we use mineral and contextual sedimentary environmental data measured by the Mars Sc...

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Detalhes bibliográficos
Publicado no:Proc Natl Acad Sci U S A
Main Authors: Bristow, Thomas F., Haberle, Robert M., Blake, David F., Des Marais, David J., Eigenbrode, Jennifer L., Fairén, Alberto G., Grotzinger, John P., Stack, Kathryn M., Mischna, Michael A., Rampe, Elizabeth B., Siebach, Kirsten L., Sutter, Brad, Vaniman, David T., Vasavada, Ashwin R.
Formato: Artigo
Idioma:Inglês
Publicado em: National Academy of Sciences 2017
Assuntos:
Physical Sciences
Acesso em linha:https://ncbi.nlm.nih.gov/pmc/articles/PMC5338541/
https://ncbi.nlm.nih.gov/pubmed/28167765
https://ncbi.nlm.nih.govhttp://dx.doi.org/10.1073/pnas.1616649114
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