Solid-state mantle convection coupled with a crystallising basal magma ocean

Fractional crystallisation of a basal magma ocean (BMO) has been proposed to explain the formation of large scale compositional variations in the mantle and the persistence of partially molten patches in the lowermost mantle. We present a complete set of equations for the thermal and compositional e...

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Main Authors: Labrosse, Stéphane, Morison, Adrien, Tackley, Paul James
Format: Article
Language:English
Published: Académie des sciences 2024-11-01
Series:Comptes Rendus. Géoscience
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Online Access:https://comptes-rendus.academie-sciences.fr/geoscience/articles/10.5802/crgeos.275/
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author Labrosse, Stéphane
Morison, Adrien
Tackley, Paul James
author_facet Labrosse, Stéphane
Morison, Adrien
Tackley, Paul James
author_sort Labrosse, Stéphane
collection DOAJ
description Fractional crystallisation of a basal magma ocean (BMO) has been proposed to explain the formation of large scale compositional variations in the mantle and the persistence of partially molten patches in the lowermost mantle. We present a complete set of equations for the thermal and compositional evolution of the BMO and show that it can be implemented in a mantle convection code to solve the long term mantle evolution problem. The presence of the BMO modifies the dynamics of the mantle in several ways. The phase equilibrium at the bottom of the solid mantle implies a change of mechanical boundary condition, which helps solid state convection. The net freezing of the BMO implies a change of computational domain, which is treated by mapping the radial coordinate on a constant thickness domain. Fractional melting and freezing at the boundary makes the composition of the BMO and the solid mantle evolve, which is treated using Lagrangian tracers. A sample calculation shows that the persistence of the BMO and its long term evolution drastically changes the dynamics of the solid mantle by promoting downwelling currents and large scale flow. The gradual increase of the FeO content in the BMO and in the solid that crystallises from it leads to the stabilisation of large scale thermo-compositional piles at the bottom of the mantle, possibly explaining the observations from seismology.
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series Comptes Rendus. Géoscience
spelling doaj-art-1aace429ff534cec827613535e1dd8e52025-02-07T10:41:28ZengAcadémie des sciencesComptes Rendus. Géoscience1778-70252024-11-01356S152110.5802/crgeos.27510.5802/crgeos.275Solid-state mantle convection coupled with a crystallising basal magma oceanLabrosse, Stéphane0https://orcid.org/0000-0002-7620-4363Morison, Adrien1https://orcid.org/0000-0002-8261-9143Tackley, Paul James2https://orcid.org/0000-0003-4878-621XLGLTPE, ENS de Lyon, Université de Lyon, 46 allée d’Italie, 69003 Lyon, FranceUniv Exeter, Phys & Astron, Exeter, Devon, EnglandDepartment of Earth and Planetary Sciences, ETH Zürich, Sonneggstrasse 5, Zürich, 8092, SwitzerlandFractional crystallisation of a basal magma ocean (BMO) has been proposed to explain the formation of large scale compositional variations in the mantle and the persistence of partially molten patches in the lowermost mantle. We present a complete set of equations for the thermal and compositional evolution of the BMO and show that it can be implemented in a mantle convection code to solve the long term mantle evolution problem. The presence of the BMO modifies the dynamics of the mantle in several ways. The phase equilibrium at the bottom of the solid mantle implies a change of mechanical boundary condition, which helps solid state convection. The net freezing of the BMO implies a change of computational domain, which is treated by mapping the radial coordinate on a constant thickness domain. Fractional melting and freezing at the boundary makes the composition of the BMO and the solid mantle evolve, which is treated using Lagrangian tracers. A sample calculation shows that the persistence of the BMO and its long term evolution drastically changes the dynamics of the solid mantle by promoting downwelling currents and large scale flow. The gradual increase of the FeO content in the BMO and in the solid that crystallises from it leads to the stabilisation of large scale thermo-compositional piles at the bottom of the mantle, possibly explaining the observations from seismology.https://comptes-rendus.academie-sciences.fr/geoscience/articles/10.5802/crgeos.275/Thermal evolutionMantle convectionCore coolingBasal magma ocean
spellingShingle Labrosse, Stéphane
Morison, Adrien
Tackley, Paul James
Solid-state mantle convection coupled with a crystallising basal magma ocean
Comptes Rendus. Géoscience
Thermal evolution
Mantle convection
Core cooling
Basal magma ocean
title Solid-state mantle convection coupled with a crystallising basal magma ocean
title_full Solid-state mantle convection coupled with a crystallising basal magma ocean
title_fullStr Solid-state mantle convection coupled with a crystallising basal magma ocean
title_full_unstemmed Solid-state mantle convection coupled with a crystallising basal magma ocean
title_short Solid-state mantle convection coupled with a crystallising basal magma ocean
title_sort solid state mantle convection coupled with a crystallising basal magma ocean
topic Thermal evolution
Mantle convection
Core cooling
Basal magma ocean
url https://comptes-rendus.academie-sciences.fr/geoscience/articles/10.5802/crgeos.275/
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AT morisonadrien solidstatemantleconvectioncoupledwithacrystallisingbasalmagmaocean
AT tackleypauljames solidstatemantleconvectioncoupledwithacrystallisingbasalmagmaocean