A wet heterogeneous mantle creates a habitable world in the Hadean
- Creators
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Miyazaki, Yoshinori
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Korenaga, Jun
Abstract
The Hadean eon, following the global-scale melting of the mantle is expected to be a dynamic period, during which Earth experienced vastly different conditions. Geologic records, however, suggest that the surface environment of Earth was already similar to the present by the middle of the Hadean4,5. Under what conditions a harsh surface environment could turn into a habitable one remains uncertain6. Here we show that a hydrated mantle with small-scale chemical heterogeneity, created as a result of magma ocean solidification, is the key to ocean formation, the onset of plate tectonics and the rapid removal of greenhouse gases, which are all essential to create a habitable environment on terrestrial planets. When the mantle is wet and dominated by high-magnesium pyroxenites, the removal of carbon dioxide from the atmosphere is expected to be more than ten times faster than the case of a pyrolitic homogeneous mantle and could be completed within 160 million years. Such a chemically heterogeneous mantle would also produce oceanic crust rich in olivine, which is reactive with ocean water and promotes serpentinization. Therefore, conditions similar to the Lost City hydrothermal field may have existed globally in the Hadean seafloor.
Additional Information
© 2022 Springer Nature Limited. Received 03 August 2020. Accepted 20 December 2021. Published 02 March 2022. Issue Date 03 March 2022. This work was sponsored by the US National Aeronautics and Space Administration under Cooperative Agreement No. 80NSSC19M0069 issued through the Science Mission Directorate and the National Science Foundation under grant EAR-1753916. This work was also supported in part by the facilities and staff of the Yale University Faculty of Arts and Sciences High Performance Computing Center. Y.M. was supported by the Stanback Postdoctoral Fellowship from Caltech Center for Comparative Planetary Evolution. The authors thank N. Sleep and M. Hirschmann for providing constructive comments, which were helpful to substantially improve the accuracy of the manuscript. Contributions. Y.M. and J.K. designed the study, discussed the results, and wrote the manuscript. Y.M. performed calculations. Data availability. All relevant data are provided in the paper. Codes to reproduce the results are available at https://github.com/yoshi-miyazaki/Hadean-evolution/. The Gibbs energy minimization code is available at https://github.com/yoshi-miyazaki/GibbsE-minimization/. Source data are provided with this paper. The authors declare no competing financial interests. Peer review information. Nature thanks Marc Hirschmann and Norman Sleep for their contribution to the peer review of this work. Peer reviewer reports are available.Attached Files
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Additional details
- Eprint ID
- 113753
- Resolver ID
- CaltechAUTHORS:20220304-60865000
- Created
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2022-03-07Created from EPrint's datestamp field
- Updated
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2022-07-25Created from EPrint's last_modified field
- Caltech groups
- Caltech Center for Comparative Planetary Evolution