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Habitability of Exo-Earths in various atmospheric oxidative conditions

Project description

More than water: characterising interactions with organic ingredients for the emergence of life

The evolution of life on Earth required water, a focus in our search for Earth-like planets within the ‘habitable zone’ of their host stars. Characterising the atmospheres of such planets to see if they also have the right organic ingredients for the emergence of life and whether their interactions with atmospheric water could fuel its emergence is the next step. The EU-funded OxyPlanets project will investigate this with a focus on organic aerosols and their reactivity with atmospheric water under a range of oxidative conditions. The project’s outcomes will shed light on the evolution of life on Earth and the habitability of other planets, informing the focus of future space missions.

Objective

Among the thousands of extrasolar planets discovered, Earth-like objects focus our attention to seek new habitable worlds. Eleven Earth-sized planets have already been discovered in the Habitable Zone (HZ) of their host-star, including three in the TRAPPIST-1 planetary system. Deciphering their atmospheres is the challenge of the next decade in exoplanetary science, stressing out urgent needs in fundamental data for these objects.

My aim is to investigate how the atmospheric organic reservoir forms and evolves in the frame of humid exoplanetary atmospheres in Habitable Zone. I will also quantify the impact of theses processes on the climate and on the potential for prebiotic chemistry on these planets. I propose to consider the role of organic aerosols as prebio-signature: those are nanoparticles chemically produced in the atmosphere. I will address the capacity of exo-Earths atmospheres to produce organic aerosols in various oxidative conditions, and their further physical and chemical interactions with atmospheric water.

To tackle these questions, I will combine experiments and models to discover the reactivity that occurs in atmospheres within an extensive range of oxidation conditions. I will experimentally determine the physical properties of the aerosols, and then model their radiative impact and their propensity to generate clouds in the atmosphere.
I will also experimentally identify the prebiotic molecules composing the aerosols that dissolve into clouds. This transfer from the dry organic reservoir towards liquid water is indeed critical for the emergence of life.

The ERC-AdG Oxyplanets project will contribute to interpret and suggest observations for the future NASA-JWST and ESA-ARIEL space missions. Furthermore, it will reinforce our knowledge of the habitability of Earth-like exo-worlds, potentially reappraising the conditions for life to appear on the early-Earth.

Fields of science (EuroSciVoc)

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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-ADG

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Host institution

UNIVERSITE DE VERSAILLES SAINT-QUENTIN EN YVELINES
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.

€ 2 412 601,00
Address
AVENUE DE PARIS 55
78035 VERSAILLES
France

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Region
Ile-de-France Ile-de-France Yvelines
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.

€ 2 412 601,00

Beneficiaries (1)

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