All-optical measurements of MORB-glass density at high pressure hint at a stiffness-composition relation in silicate glasses

The density of silicate melts at high pressure determined the efficiency of gravitational differentiation in the solidifying magma ocean and thus the starting conditions for the Earth's evolution. The denisty also controls the migration of melts in the lithosphere and their stabilization in the transition zone and near the core mantle boundary. Yet, no density systematic exists for melts across the pressure range of the mantle. This is primarily because of severe experimental difficulties associated with measuring the density of silicate liquids at mantle pressures and temperatures (tiny sample size, melt chemical reactivity, lack of crystalline structure). The use of glasses as proxies of melts at high pressure lifts some but not all of these challenges, and may prove important in developing theoretical models of melts physical behavior at high pressures. Here we report on the density of MORB glass up to 32.3 GPa at room temperature measured by the recently developed all-optical method in a diamond anvil cell. The comparison of the MORB glass density to that for other basaltic glasses reported in the literature reveals contradictions, similarly to those existing between data available for MORB-like melts, which underscore the need for consistent, systematic melt and glass density measurements at high pressure across a broad compositional space. More broadly, the compression behavior of MORB and other basaltic glasses, SiO 2 , MgSiO 3 , and Mg 2 SiO 4 glasses suggests that the incorporation of SiO 2 and/or large network-modifiers (larger than Mg) softens the glass (smaller isothermal bulk modulus and its pressure derivative). Future all-optical measurements of glass density may provide fundamental, critical input to develop models of complex glasses and melts physical properties, and help assessing the solidification of the primordial magma ocean, the initiation and development of physical and chemical heterogeneity in the mantle, and the migration or stabilization of melts at different levels in the deep Earth. • We report the refractive index of MORB-glass up to 134 GPa. • The density of MORB-glass is reported up to 32.3 GPa at room temperature. • SiO 2 and/or large network-modifiers soften the glass.

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Journal
Chemical Geology
Published
2025-09-21
DOI
https://doi.org/10.1016/j.chemgeo.2025.123066
Primary Topic
High-pressure geophysics and materials
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article
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article

All-optical measurements of MORB-glass density at high pressure hint at a stiffness-composition relation in silicate glasses

S. Speziale, Konstantin Solovev, Louis Hennet, Lukas Schifferle et al.
Chemical Geology
High-pressure geophysics and materials
article

All-optical measurements of MORB-glass density at high pressure hint at a stiffness-composition relation in silicate glasses

S. Speziale, Konstantin Solovev, Louis Hennet, Lukas Schifferle, Ilya Kupenko, Sergey S. Lobanov, Vladimir Roddatis, Séverine Brassamin
article en

Abstract

The density of silicate melts at high pressure determined the efficiency of gravitational differentiation in the solidifying magma ocean and thus the starting conditions for the Earth's evolution. The denisty also controls the migration of melts in the lithosphere and their stabilization in the transition zone and near the core mantle boundary. Yet, no density systematic exists for melts across the pressure range of the mantle. This is primarily because of severe experimental difficulties associated with measuring the density of silicate liquids at mantle pressures and temperatures (tiny sample size, melt chemical reactivity, lack of crystalline structure). The use of glasses as proxies of melts at high pressure lifts some but not all of these challenges, and may prove important in developing theoretical models of melts physical behavior at high pressures. Here we report on the density of MORB glass up to 32.3 GPa at room temperature measured by the recently developed all-optical method in a diamond anvil cell. The comparison of the MORB glass density to that for other basaltic glasses reported in the literature reveals contradictions, similarly to those existing between data available for MORB-like melts, which underscore the need for consistent, systematic melt and glass density measurements at high pressure across a broad compositional space. More broadly, the compression behavior of MORB and other basaltic glasses, SiO 2 , MgSiO 3 , and Mg 2 SiO 4 glasses suggests that the incorporation of SiO 2 and/or large network-modifiers (larger than Mg) softens the glass (smaller isothermal bulk modulus and its pressure derivative). Future all-optical measurements of glass density may provide fundamental, critical input to develop models of complex glasses and melts physical properties, and help assessing the solidification of the primordial magma ocean, the initiation and development of physical and chemical heterogeneity in the mantle, and the migration or stabilization of melts at different levels in the deep Earth. • We report the refractive index of MORB-glass up to 134 GPa. • The density of MORB-glass is reported up to 32.3 GPa at room temperature. • SiO 2 and/or large network-modifiers soften the glass.

Chemical GeologyVol. 695
Université d'Orléans (FR), Centre National de la Recherche Scientifique (FR), University of Potsdam (DE), European Synchrotron Radiation Facility (FR), Interfaces, Confinement, Matériaux et Nanostructures (FR), Conditions Extrêmes et Matériaux Haute Température et Irradiation (FR), GFZ Helmholtz Centre for Geosciences (DE)
Openalex Percentile: Top 64%
High-pressure geophysics and materials
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