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Light elements in irons and metal-rich meteorites: Their isotopic distribution and evolution in the protoplanetary disk

Objective

Knowledge of the light element (H, C, N) characteristics of planetary building blocks is key to our understanding of the development of habitable conditions on Earth. Since 'magmatic' iron meteorites originate from the metallic cores of the earliest, differentiated planetesimals, they may preserve a record of H, C, and N isotopic variations in the inner and outer solar system during the first stages of planetary accretion. Based on novel multi-light-element isotopic analyses of irons and other Fe-Ni alloy-rich meteorites and experimental simulations, project IRONIS aims to answer the fundamental questions of (i) how the distributions of H, C, and N (and their carrier phases) evolved in space and time within the earliest stages of the protoplanetary disk, and (ii) how H, C, and N were distributed between metals and silicates during planetesimal accretion, differentiation, and subsequent evolution. A major objective is to develop novel secondary ion mass spectrometry protocols for analyzing H, C, and N in situ in Fe-Ni alloy, and to combine these with 'bulk' N-noble gas analyses by static noble gas mass spectrometry. The originality and uniqueness of project IRONIS thus lies in the coupling of two state-of the-art analytical techniques, which allow the quantification of any solar gas and cosmogenic nuclide contributions. Only once the effects of these secondary components are understood, can spatiotemporal isotopic variations in the protoplanetary disk be investigated. In parallel, new cross-calibrated N analyses of experimental run products will provide constraints on the degree of N isotopic fractionation during alloy-silicate partitioning, and will permit us to assess if the N isotopic compositions of irons represent a primary feature of their parent bodies. Ultimately, by investigating the remnants of the first planetesimal populations, project IRONIS will provide new fundamental insights into the cosmochemical history and evolution of life-forming light elements.

Fields of science (EuroSciVoc)

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Keywords

Project’s keywords as indicated by the project coordinator. Not to be confused with the EuroSciVoc taxonomy (Fields of science)

Programme(s)

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Topic(s)

Calls for proposals are divided into topics. A topic defines a specific subject or area for which applicants can submit proposals. The description of a topic comprises its specific scope and the expected impact of the funded project.

Funding Scheme

Funding scheme (or “Type of Action”) inside a programme with common features. It specifies: the scope of what is funded; the reimbursement rate; specific evaluation criteria to qualify for funding; and the use of simplified forms of costs like lump sums.

HORIZON-ERC - HORIZON ERC Grants

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Call for proposal

Procedure for inviting applicants to submit project proposals, with the aim of receiving EU funding.

(opens in new window) ERC-2022-COG

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Host institution

CENTRE NATIONAL DE LA RECHERCHE SCIENTIFIQUE CNRS
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.

€ 1 779 805,00
Address
RUE MICHEL ANGE 3
75794 PARIS
France

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Region
Ile-de-France Ile-de-France Hauts-de-Seine
Activity type
Research Organisations
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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.

€ 1 779 805,00

Beneficiaries (1)

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