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...
Published in: | Proceedings of the National Academy of Sciences |
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Main Authors: | , , , , , , , , , , , , , |
Format: | Article in Journal/Newspaper |
Language: | English |
Published: |
National Academy of Sciences
2017
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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 |