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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Bibliographic Details
Published in:Proceedings of the National Academy of Sciences
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.
Format: Article in Journal/Newspaper
Language:English
Published: National Academy of Sciences 2017
Subjects:
Online Access:https://authors.library.caltech.edu/74131/
https://authors.library.caltech.edu/74131/3/PNAS-2017-Bristow-2166-70.pdf
https://authors.library.caltech.edu/74131/2/pnas.201616649SI.pdf
https://resolver.caltech.edu/CaltechAUTHORS:20170207-103345859