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Toward a better understanding of planet MErcury's Redox conditions: implications for its bulk Composition and Internal structure

Project description

Decoding the mysteries of Mercury’s hidden interior

Mercury, our Solar System’s smallest and most enigmatic planet, boasts a very large metallic core and a surface rich in sulfur but poor in iron. As the joint ESA/JAXA BepiColombo mission prepares to orbit the planet in late 2026, with the support of the Marie Skłodowska-Curie Actions programme, the MERCI project provides the essential experimental groundwork needed to decode the coming data. The project will simulate the extreme pressure, high temperature and highly reduced conditions of Mercury’s depths in order to map iron distribution and silicon partitioning from core to crust. This research will refine thermodynamic models of the planet’s bulk composition and internal structure, ensuring that Europe’s investment in BepiColombo yields a new understanding of Mercury’s unique evolution.

Objective

Mercury is the innermost and smallest planet in our Solar System, having unique chemical and structural characteristics. Past NASA space missions have revealed Mercury’s exceptionally high density and surface lavas with high S and low, but measurable, Fe content. These observations point to two key features: i) an extremely reduced interior (very low oxygen fugacity) and ii) a large metallic core, where most of the Fe is hosted. Over the past decade, the integration of geophysical data and modelling with high-pressure and -temperature experiments has helped to develop a picture of Mercury’s interior, although very large uncertainties remain. BepiColombo, a new space mission led by ESA and JAXA, will begin orbiting Mercury in November 2026 and is expected to deliver new high spatiotemporal-resolution data (2027-2028). However, to fully interpret them, new experiments simulating Mercury’s interior conditions are necessary. In this context, the MERCI project aims to provide more accurate experimental and thermodynamic constraints on the redox conditions of Mercury’s interior, with implications for its bulk composition and internal structure. The main objectives are i) understanding Fe distribution from the mantle to the surface lavas and ii) to constrain Si partitioning behaviour under reducing conditions and, thus, determine mantle and core bulk compositions. MERCI will provide a fundamental reference dataset that I will use for the analysis and interpretation of the mission spectroscopic and geophysical observations. This will help to maximize BepiColombo scientific impact and return, since it was largely financed by the European Union. The MERCI timeline and multidisciplinary approach, along with the supervisor’s key scientific role in the mission and significant contributions to the topic, combined with my experimental and scientific background, will ensure a highly effective contribution to understanding Mercury’s origin and evolution.

Fields of science (EuroSciVoc)

Keywords

Programme(s)

Topic(s)

Funding Scheme

HORIZON-TMA-MSCA-PF-EF - HORIZON TMA MSCA Postdoctoral Fellowships - European Fellowships

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Call for proposal

(opens in new window) HORIZON-MSCA-2025-PF

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Coordinator

KATHOLIEKE UNIVERSITEIT LEUVEN
Net EU contribution
€ 200 400,00
Address
OUDE MARKT 13
3000 Leuven
Belgium
Region
Vlaams Gewest Prov. Vlaams-Brabant Arr. Leuven
Activity type
Higher or Secondary Education Establishments
Links
Total cost
No data

Partners (1)