Whole-mantle convection with tectonic plates preserves long-term global patterns of upper mantle geochemistry

Abstract The evolution of the planetary interior during plate tectonics is controlled by slow convection within the mantle. Global-scale geochemical differences across the upper mantle are known, but how they are preserved during convection has not been adequately explained. We demonstrate that the...

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Main Authors: T. L. Barry, J. H. Davies, M. Wolstencroft, I. L. Millar, Z. Zhao, P. Jian, I. Safonova, M. Price
Format: Article
Language:English
Published: Nature Portfolio 2017-05-01
Series:Scientific Reports
Online Access:https://doi.org/10.1038/s41598-017-01816-y
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author T. L. Barry
J. H. Davies
M. Wolstencroft
I. L. Millar
Z. Zhao
P. Jian
I. Safonova
M. Price
author_facet T. L. Barry
J. H. Davies
M. Wolstencroft
I. L. Millar
Z. Zhao
P. Jian
I. Safonova
M. Price
author_sort T. L. Barry
collection DOAJ
description Abstract The evolution of the planetary interior during plate tectonics is controlled by slow convection within the mantle. Global-scale geochemical differences across the upper mantle are known, but how they are preserved during convection has not been adequately explained. We demonstrate that the geographic patterns of chemical variations around the Earth’s mantle endure as a direct result of whole-mantle convection within largely isolated cells defined by subducting plates. New 3D spherical numerical models embedded with the latest geological paleo-tectonic reconstructions and ground-truthed with new Hf-Nd isotope data, suggest that uppermost mantle at one location (e.g. under Indian Ocean) circulates down to the core-mantle boundary (CMB), but returns within ≥100 Myrs via large-scale convection to its approximate starting location. Modelled tracers pool at the CMB but do not disperse ubiquitously around it. Similarly, mantle beneath the Pacific does not spread to surrounding regions of the planet. The models fit global patterns of isotope data and may explain features such as the DUPAL anomaly and long-standing differences between Indian and Pacific Ocean crust. Indeed, the geochemical data suggests this mode of convection could have influenced the evolution of mantle composition since 550 Ma and potentially since the onset of plate tectonics.
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spelling doaj.art-8a936aaf38c44e769d50a672e6ff92662022-12-21T18:33:02ZengNature PortfolioScientific Reports2045-23222017-05-01711910.1038/s41598-017-01816-yWhole-mantle convection with tectonic plates preserves long-term global patterns of upper mantle geochemistryT. L. Barry0J. H. Davies1M. Wolstencroft2I. L. Millar3Z. Zhao4P. Jian5I. Safonova6M. Price7Department of Geology, University of LeicesterSchool of Earth and Ocean Sciences, Cardiff UniversityJBA Risk Management, Broughton HallNERC Isotope Geosciences Laboratory, British Geological Survey, KeyworthSchool of Earth Science and Resources, China University of GeosciencesBeijing SHRIMP Centre, Institute of Geology, Chinese Academy of Geological SciencesSobolev Institute of Geology and Mineralogy SB RASSchool of Earth and Ocean Sciences, Cardiff UniversityAbstract The evolution of the planetary interior during plate tectonics is controlled by slow convection within the mantle. Global-scale geochemical differences across the upper mantle are known, but how they are preserved during convection has not been adequately explained. We demonstrate that the geographic patterns of chemical variations around the Earth’s mantle endure as a direct result of whole-mantle convection within largely isolated cells defined by subducting plates. New 3D spherical numerical models embedded with the latest geological paleo-tectonic reconstructions and ground-truthed with new Hf-Nd isotope data, suggest that uppermost mantle at one location (e.g. under Indian Ocean) circulates down to the core-mantle boundary (CMB), but returns within ≥100 Myrs via large-scale convection to its approximate starting location. Modelled tracers pool at the CMB but do not disperse ubiquitously around it. Similarly, mantle beneath the Pacific does not spread to surrounding regions of the planet. The models fit global patterns of isotope data and may explain features such as the DUPAL anomaly and long-standing differences between Indian and Pacific Ocean crust. Indeed, the geochemical data suggests this mode of convection could have influenced the evolution of mantle composition since 550 Ma and potentially since the onset of plate tectonics.https://doi.org/10.1038/s41598-017-01816-y
spellingShingle T. L. Barry
J. H. Davies
M. Wolstencroft
I. L. Millar
Z. Zhao
P. Jian
I. Safonova
M. Price
Whole-mantle convection with tectonic plates preserves long-term global patterns of upper mantle geochemistry
Scientific Reports
title Whole-mantle convection with tectonic plates preserves long-term global patterns of upper mantle geochemistry
title_full Whole-mantle convection with tectonic plates preserves long-term global patterns of upper mantle geochemistry
title_fullStr Whole-mantle convection with tectonic plates preserves long-term global patterns of upper mantle geochemistry
title_full_unstemmed Whole-mantle convection with tectonic plates preserves long-term global patterns of upper mantle geochemistry
title_short Whole-mantle convection with tectonic plates preserves long-term global patterns of upper mantle geochemistry
title_sort whole mantle convection with tectonic plates preserves long term global patterns of upper mantle geochemistry
url https://doi.org/10.1038/s41598-017-01816-y
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