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The origin and evolution of a blastered Mercury

Project description

Peeling back the layers of Mercury’s origin and evolution

Mercury is the least explored terrestrial planet in our solar system, with many unresolved questions about how it has formed and evolved. Data collected from ongoing exploration of the planet by BepiColombo satellites will reveal much about its history. The ERC-funded IronHeart project theorises that Mercury was once a larger chondritic planet (proto-Mercury) whose mantle was stripped away in collisions. To validate this, IronHeart will conduct experiments to determine how the core and mantle compositions of proto-Mercury evolved into their current state. Further analysis of these compositions will elucidate phase equilibria of the inner layers, enabling calculation of their thermophysical properties. Finally, it will integrate empirical results with BepiColombo data to develop thermal and geophysical models of Mercury’s structure and evolution.

Objective

Mercury is a metal-rich planet from which Earth-based and spacecraft data were collected. Our understanding of its interior structure and thermochemical evolution is however still relatively poor. This is due to: (1) large uncertainties on its polar moment of inertia and surface composition; this will be largely improved by the BepiColombo mission; (2) an unknown bulk-planet composition; and (3) a poor knowledge of some key thermophysical properties (e.g. phase stability, temperature, density) of solid/liquid metals and silicates inside Mercury. This is because under Mercury’s reducing conditions, elements behave differently than on other planets. Currently available phase diagrams for the Moon and Mars are thus irrelevant for calculating the compositions and physical properties of Mercury’s core, mantle and crust. Improving such constraints is critical but requires new experiments under hitherto unexplored conditions; they will be done in IronHeart.
So far, it was largely neglected that many compositional features of Mercury are inconsistent with its direct accretion as a small, metal-rich planet. IronHeart’s working hypothesis is that Mercury is merely the remnant of a larger, Martian-sized, chondritic planet (which we call proto-Mercury) involved in collisions having stripped away much of its mantle. This process did eventually set the final composition of modern Mercury. For the first time, IronHeart will evaluate experimentally how proto-Mercury controlled the core and mantle compositions of modern Mercury. Further experiments on these compositions will provide phase equilibria of Mercury’s internal layers allowing us to calculate their thermophysical properties. By combining those with BepiColombo data into thermal and geophysical models, we will provide a clearer than ever picture of Mercury’s structure and evolution. IronHeart will also be critical to understanding dense exoplanets and the Earth, which accreted from similar building blocks as Mercury.

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Programme(s)

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Topic(s)

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HORIZON-ERC - HORIZON ERC Grants

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Call for proposal

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(opens in new window) ERC-2023-COG

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Host institution

KATHOLIEKE UNIVERSITEIT LEUVEN
Net EU contribution

Net EU financial contribution. The sum of money that the participant receives, deducted by the EU contribution to its linked third party. It considers the distribution of the EU financial contribution between direct beneficiaries of the project and other types of participants, like third-party participants.

€ 1 999 224,00
Address
OUDE MARKT 13
3000 LEUVEN
Belgium

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Region
Vlaams Gewest Prov. Vlaams-Brabant Arr. Leuven
Activity type
Higher or Secondary Education Establishments
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Total cost

The total costs incurred by this organisation to participate in the project, including direct and indirect costs. This amount is a subset of the overall project budget.

€ 1 999 224,00

Beneficiaries (1)

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