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Universal Model of the Density of Deep Silicate Melts

Project description

Advanced laser technology helps identify how molten rock behaves inside Earth

The density of silicate melts plays a crucial role in shaping Earth’s evolution and mantle dynamics, influencing whether crystallising materials rise or sink, as well as controlling melt distribution and migration. However, measuring these densities under high pressure and temperature mantle conditions has been extremely difficult owing to tiny sample sizes, chemical reactivity and the lack of crystalline structure. The ERC-funded Glass2Melt project will leverage a novel class of white laser spectroscopy methods to analyse synthetic silicate glasses and melts across a wide compositional range and at pressure-temperature conditions ranging from Earth's crust to its core. The proposed approach aims to create a universal density model describing silicate melts, providing insights into magma ocean solidification, mantle heterogeneity, seismic velocity structures and magma behaviour in modern Earth.

Objective

The starting conditions for the Earth’s evolution were set by gravitational differentiation in the solidifying magma ocean. Yet, a thorough understanding of the magma ocean dynamics and thus of the primordial Earth is lacking. One key unknown is the density of silicate melts at high pressure, which determines whether the crystallizing phases rise or sink. Magma density also governs the storage, spatial distribution, and migration of melts in the present-day Earth. Densities of silicate liquids at mantle pressures and temperatures are extremely difficult to measure because of the tiny sample size, melt chemical reactivity, and its lack of crystalline structure. The use of glasses as proxies of melts lifts some but not all of these challenges. Albeit needed for a holistic picture of planet Earth, no density systematics exists for glasses or melts across the pressure range of the entire mantle.

Glass2Melt will employ and further a novel class of fast white laser spectroscopy methods to measure the density of multicomponent synthetic silicate glasses and melts at mantle pressure-temperature conditions. Our approach is ground-breaking because it allows to thoroughly explore a large compositional space and determine the density of any deep silicate melt. Our results will (i) parametrize a universal silicate melt density model applicable to the entire mantle, and (ii) quantify solid-liquid buoyancy throughout the whole crystallizing magma ocean.

Glass2Melt will have a broad, lasting impact on our understanding of the Earth’s interior and its evolution over geologic time. The new density model will provide critical input for future numerical simulations assessing fundamental questions about the solidification of the primordial magma ocean, as well as the initiation and development of physical and chemical heterogeneity in the mantle. It will also be crucial for deciphering deep low seismic velocity structures, and to modeling magma dynamics in the present-day Earth.

Fields of science (EuroSciVoc)

Keywords

Programme(s)

Topic(s)

Funding Scheme

HORIZON-ERC - HORIZON ERC Grants

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Call for proposal

(opens in new window) ERC-2023-COG

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Host institution

GFZ HELMHOLTZ-ZENTRUM FUR GEOFORSCHUNG
Net EU contribution
€ 1 998 856,00
Address
TELEGRAFENBERG
14473 POTSDAM
Germany
Region
Brandenburg Brandenburg Potsdam
Activity type
Research Organisations
Links
Total cost
€ 1 998 856,25

Beneficiaries (1)