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Atmospheric tracing of Earth's evolution

Project description

Tracing the origin and evolution of Earth’s atmospheric elements

Earth’s atmosphere consists of about 80 % nitrogen and 20 % oxygen. The interactions between the atmosphere and the continental crust play a major role in controlling nutrient bioavailability and composition in the atmosphere. However, there is no scientific consensus on how and why these two molecules emerged and persisted in the atmosphere. The EU-funded ATTRACTE project aims to enhance knowledge of the main drivers that underpinned the evolution of Earth’s atmosphere over the course of geological aeons. A variety of "proxies" (e.g. minerals containing geochemical signatures from the atmosphere) will be used to analyse new and past atmospheric gases.

Objective

Planetary atmospheres are fundamental reservoirs controlling the habitability of planets. The chemical and isotopic compositions of atmospheric constituents also hold clues on the geological evolution of the entire planetary body. Today, Earth's atmosphere contains about 80% dinitrogen and 20% dioxygen. Yet, there is no scientific consensus on how and why these two molecules emerged and persisted in the Earth's atmosphere. The interactions between the atmosphere and the continental crust also play a major role in controlling the bio-availability of nutrients and the composition of the atmosphere, and thus the climate. However, the evolution of the volume of continental crust over time is strongly debated. Project ATTRACTE will significantly improve our knowledge of the main drivers of atmospheric evolution over time. This will be achieved by going back in time and following the evolution of the composition of the Earth's atmosphere over geological eons. Analyses of gases contained in traditional and new paleo-atmospheric proxies, the post-impact hydrothermal minerals, will be carried out with innovative mass spectrometry techniques. The isotopic composition of paleo-atmospheric xenon will provide new constraints on the history of hydrogen escape for the Archean Earth. Coupled argon and nitrogen measurements will allow to determine, for the first time, the evolution of the partial pressure of atmospheric dinitrogen. Paleo-atmospheric data gathered during the project will be fed in numerical models of Earth's atmospheric and crustal evolution. This will allow to reconstruct how volatile elements have been exchanged between the silicate Earth and the atmosphere through time. Results gathered during project ATTRACTE will ultimately provide new datasets for climate studies of the ancient Earth but will also help building the scientific framework required to interpret future observations of exoplanetary atmospheres and to portray the geology of extrasolar planets.

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Keywords

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Programme(s)

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Topic(s)

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Funding Scheme

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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-2021-STG

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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.

€ 1 499 125,00
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.

€ 2 499 125,00

Beneficiaries (2)

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