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The role of volatiles in reactive melt transport in the asthenosphere

The role of volatiles in reactive melt transport in the asthenosphere
The role of volatiles in reactive melt transport in the asthenosphere
Experimental studies of mantle petrology find that small concentrations of water and carbon dioxide have a large effect on the solidus temperature and distribution of melting in the upper mantle. However, it has remained unclear what effect small fractions of deep, volatile-rich melts have on melt transport and reactive melting in the shallow asthenosphere. Here we present theory and computations indicating that low-degree, reactive, volatile-rich melts cause channelization of magmatic flow at depths approximately corresponding to the anhydrous solidus temperature. These results are obtained with a novel method to simulate the thermochemical evolution of the upper mantle in the presence of volatiles. The method uses a thermodynamically consistent framework for reactive, disequilibrium, multi-component melting. It is coupled with a system of equations representing conservation of mass, momentum, and energy for a partially molten grain aggregate. Application of this method in two-phase, three-component upwelling-column models demonstrates that it reproduces leading-order features of hydrated and carbonated peridotite melting; in particular, it captures the production of low-degree, volatile-rich melt at depths far below the volatile-free solidus. The models predict that segregation of volatile-rich, deep melts promotes a reactive channelling instability that creates fast and chemically isolated pathways of melt extraction. Reactive channelling occurs where volatile-rich melts flux the base of the silicate melting region, enhancing dissolution of fusible components from the ambient mantle. We find this effect to be similarly expressed for models of both hydrated and carbonated mantle melting. These findings indicate that despite their small concentrations, water and carbon dioxide have an important control on the extent and style of magma genesis, as well as on the dynamics of melt transport.
0022-3530
1073–1108
Keller, Tobias
d8dfcfa5-89d1-4203-aa2d-8c142c00a169
Katz, Richard F.
01d7145d-41ad-44eb-9671-ac78313e82c2
Keller, Tobias
d8dfcfa5-89d1-4203-aa2d-8c142c00a169
Katz, Richard F.
01d7145d-41ad-44eb-9671-ac78313e82c2

Keller, Tobias and Katz, Richard F. (2016) The role of volatiles in reactive melt transport in the asthenosphere. Journal of Petrology, 57 (6), 1073–1108. (doi:10.1093/petrology/egw030).

Record type: Article

Abstract

Experimental studies of mantle petrology find that small concentrations of water and carbon dioxide have a large effect on the solidus temperature and distribution of melting in the upper mantle. However, it has remained unclear what effect small fractions of deep, volatile-rich melts have on melt transport and reactive melting in the shallow asthenosphere. Here we present theory and computations indicating that low-degree, reactive, volatile-rich melts cause channelization of magmatic flow at depths approximately corresponding to the anhydrous solidus temperature. These results are obtained with a novel method to simulate the thermochemical evolution of the upper mantle in the presence of volatiles. The method uses a thermodynamically consistent framework for reactive, disequilibrium, multi-component melting. It is coupled with a system of equations representing conservation of mass, momentum, and energy for a partially molten grain aggregate. Application of this method in two-phase, three-component upwelling-column models demonstrates that it reproduces leading-order features of hydrated and carbonated peridotite melting; in particular, it captures the production of low-degree, volatile-rich melt at depths far below the volatile-free solidus. The models predict that segregation of volatile-rich, deep melts promotes a reactive channelling instability that creates fast and chemically isolated pathways of melt extraction. Reactive channelling occurs where volatile-rich melts flux the base of the silicate melting region, enhancing dissolution of fusible components from the ambient mantle. We find this effect to be similarly expressed for models of both hydrated and carbonated mantle melting. These findings indicate that despite their small concentrations, water and carbon dioxide have an important control on the extent and style of magma genesis, as well as on the dynamics of melt transport.

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More information

Accepted/In Press date: 3 May 2016
Published date: 15 July 2016

Identifiers

Local EPrints ID: 488268
URI: http://eprints.soton.ac.uk/id/eprint/488268
ISSN: 0022-3530
PURE UUID: 19f15629-1e04-43e5-a389-ab6128cb36b7
ORCID for Tobias Keller: ORCID iD orcid.org/0000-0002-6121-5377

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Date deposited: 19 Mar 2024 17:49
Last modified: 21 Mar 2024 03:16

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Contributors

Author: Tobias Keller ORCID iD
Author: Richard F. Katz

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