H2020Individual fellowship2019–2023

HAMA · New insights on Earth’s formation and differentiation processes from in situ analyses of halogens (F, Cl, Br and I) in meteorites and mantle samples

Horizon 2020 — Marie Skłodowska-Curie Actions

Duration
2019-09-01 → 2023-07-01
EU contribution
€304,724
Participants
1
Scheme
MSCA-IF

Lines connect the coordinator with its partners.

Results in brief

New insights on Earth’s formation and differentiation processes from in situ analyses of halogens (F, Cl, Br and I) in meteorites and mantle samples

The transport of volatiles, in particular sulfur and halogens (F, Cl, Br and I), from surface reservoirs to the inner Earth and back in volcanic emissions is suggested by geochemical studies of magmas and volatile measurements on volcanoes. Furthermore, the widespread presence of sulfur-rich liquid phases has been proposed in the inner Earth by geophysical methods. However, the physicochemical properties of these liquids are poorly understood. In particular, the coupling between volatiles and metals, which controls geochemical transport processes from the inner Earth to the surface through porous and focused liquid migration, and then volcanic processes is not well known. Understanding the behaviour of halogens and sulfur through magmatic processes is key for our society since volcanic emissions of these elements can locally or globally trigger environmental issues. This can happen, for instance, through climatic cooling by sulfur-bearing aerosols or metal pollution of agricultural areas, since these chemical compounds are produced during explosive volcanic eruptions triggered by magma degassing processes. However, highly precious metals also occur among those which can be concentrated by halogens and sulfur in magmas. These chemical elements include ‘base’ metals (e.g. Cu) and ‘noble’ metals, the latter of which encompass Au, Re and platinum group elements (PGE’s) (Os, Ir, Ru, Rh, Pt, Pd). PGE’s are extremely rare in the earth's crust (<10-9 g.g-1 on average) and their use covers a wide field of applications in medicine, electronics and chemistry. These elements also play a key role in sustainable development, whether it involves reducing emissions of atmospheric pollutants or producing and managing clean and/or renewable energy. Due to the ever-increasing demands of our society, PGE’s are notably classified as critical and strategic resources by the European Union. The overall objectives of the project HAMA were to investigate the behaviours of halogens and sulfur, together with precious metals, in natural samples from intra-oceanic subduction zones. For this to be achieved, several analytical and methodological developments needed to be undertaken. In parallel, a geochemical model (e.g. involving solubility and mineral/liquid partitioning properties) needed to be developed. The aim of this model is to simulate and predict the couplings between volatile compounds and metals in the mantle and the crust of the Earth. Combining data from natural samples with the results of numerical simulations during the project HAMA aimed at providing new insights into two fundamental processes involved in the coupled mobilizations of volatiles and precious metals in the inner Earth: (i) partial melting in the deep Earth’s mantle to produce magmas; and (ii), physicochemical evolution of magmas during their emplacement in the upper part of the Earth’s mantle and in the Earth’s crust.

Data: CORDIS, © European Union

Project objective

Halogens (F, Cl, Br and I) are involved in key processes of the Earth and Planetary sciences. However, some crucial challenges of halogens’ geochemistry are unsolved. They include (i) halogen abundances in the Earth’s primitive mantle (PM) with implications on their origin and evolution during Earth formation and early differentiation; (ii) their behaviour during subduction to the Earth’s mantle; and (iii), their magmatic-volcanogenic fluxes from the mantle to the crust at subduction zones (SZ). Halogen geochemistry is currently hampered by analytical and sampling limitations. The suitability of reference halogen values in glass standards for in situ analysis is disputed. It has been also shown that indirect inferences from the whole-rock compositions of magmas are limited for fully assessing the chemical geodynamics of halogens. Technique and methodology leaps are needed to allow the in situ analysis (i.e. in minerals) of mantle and crust rocks, and to address fundamental questions in halogen geochemistry. I propose to analyse halogens in the minerals of meteorites, and unique PM-like intraplate, SZ and cratonic mantle rocks. This research will enable to define new benchmark values for meteorites and PM and determine how halogens are recycled to SZ magmas and to the deeper mantle. I will produce new standards, which in combination with analytical developments, will provide unique data about the volumetrically important mantle reservoir. In the final phase of the project, I will study halogens in the mineral-hosted melt inclusions of magma-percolated mantle and crust rocks to derive partitioning coefficients and model their SZ magmatic-volcanogenic fluxes. The research will settle in an interdisciplinary, collaborative network to stimulate breakthrough outcomes in geochemistry, cosmochemistry, volcanology and economic geology. It will significant upgrade my technical and scientific capabilities and will allow me to reach a leading position in volatile geochemistry.

Original text from CORDIS.

Participants

  • UNIVERSITE DE LAUSANNE · LAUSANNECoordinatorSwitzerland

Links

Data: CORDIS, © European Union