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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Detaylı Bibliyografya
Yayımlandı:Proc Natl Acad Sci U S A
Asıl Yazarlar: 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.
Materyal Türü: Artigo
Dil:Inglês
Baskı/Yayın Bilgisi: National Academy of Sciences 2017
Konular:
Physical Sciences
Online Erişim: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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