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The missing stellar physics component for atmospheric evaporation of exoplanets

Objective

The aim of this ambitious project is to use stellar physics to overcome a roadblock in our understanding of how exoplanets lose their primary hydrogen-helium atmospheres and make space for secondary, life-enabling ones. The best observing window for evaporating primary atmospheres are transit observations in the near-infrared metastable helium lines. However, correctly interpreting the observed absorption is extremely challenging. How much of the planetary helium is in the metastable state is controlled by a very small, but incredibly hard to observe part of the host star's extreme-ultraviolet spectrum. Not knowing this controlling factor makes quantitative estimates of the planet's evaporating atmosphere currently impossible. In this project my team and I will put helium triplet spectroscopy on a solid stellar physics footing for the first time, leveraging my extensive background in stellar X-ray astronomy. We will develop a procedure to reconstruct the crucial part of the stellar extreme-UV spectrum accurately from observed coronal X-ray spectra of stars, vastly outperforming the current highly uncertain estimation methods. We will model the outflowing planetary atmosphere to predict helium absorption as a function of stellar extreme-UV irradiation, and for the first time add accurate physics of X-ray bright stellar flares. We will use an unprecedented approach to test our predictions: We will conduct transit observations of exoplanetary helium during different phases of a host star's activity cycle, i.e. observationally isolating the changing stellar extreme-UV irradiation as a driver of helium absorption for the first time. This high risk - high gain project will turn the phenomenology of the helium window to the exoplanetary atmosphere into true understanding, by paying equal attention to the stellar window in the extreme-UV that controls how much we can see of the planet's escaping atmosphere.

Fields of science (EuroSciVoc)

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Keywords

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Programme(s)

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Topic(s)

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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-2024-COG

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Host institution

LEIBNIZ-INSTITUT FUR ASTROPHYSIK POTSDAM (AIP)
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.

€ 2 034 375,00
Address
AN DER STERNWARTE 16
14482 Potsdam
Germany

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Region
Brandenburg Brandenburg Potsdam
Activity type
Research Organisations
Links
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.

€ 2 034 375,00

Beneficiaries (1)

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