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Tracking Hydrates In Refined Sub-neptunes to Tackle their Emergence and Evolution

Project description

Searching for water on sub-Neptunes

Sub-Neptunes are a class of planets whose mass and size are between those of Earth and Neptune. Although they are among the most common planets in the galaxy, fundamental questions about their characteristics and origin remain unanswered. The most prevalent theory is that they are gas dwarfs with a rocky core and gaseous exosphere. However, recent evidence indicates that they may in fact be water worlds with rocks, ice and oceans. The ERC-funded THIRSTEE project aims to answer key questions concerning sub-Neptune formation and evolution and their atmospheres and demographic properties. With the help of leading-edge observational facilities, the project will use multiple approaches that combine transit, radial velocity and atmospheric characterisation data within a novel statistical framework.

Objective

"THIRSTEE is a ground-breaking project focusing on sub-Neptunes, a class of planets with masses and radii between those of Earth and Neptune. These planets are the most common in the Galaxy, especially around Sun-like stars, but the most basic questions about their origin and nature remain unanswered. Are sub-Neptunes ""gas dwarfs"" (Earth-like cores surrounded by large hydrogen-rich envelopes formed near their observed close-in locations) or ""water worlds"" (planets formed beyond the snow line composed of a 1:1 mixture of ice and rock)? If the latter exist, what are their demographic and individual properties and how do they depend on stellar host type? Do any of them harbour liquid water oceans below their atmospheres?

The gas dwarf hypothesis has the most traction in the field, but recent evidence suggests the existence of water worlds. The observations, however, can be explained by both scenarios due to the modelling degeneracies that surround these planets. THIRSTEE aims to solve this debate using a multi-technique approach combining transit, radial velocity and atmospheric characterization data with a novel statistical framework that accounts for observational biases. This dataset constitutes a valuable addition to the community, enlarging the known sample into unexplored regions of the parameter space and enabling a direct comparison with synthetic planet populations.

THIRSTEE is designed to mitigate all the shortcomings that have prevented previous studies from reaching conclusive results about this enigmatic population. For the first time, such an ambitious program can be pursued thanks to the simultaneous operation of state-of-the-art observational facilities. The project seeks to answer key questions about sub-Neptune formation and evolution, their atmospheres, and their demographic properties. Thanks to its unique approach, THIRSTEE will revolutionize our understanding of sub-Neptunes and their potential significance in the search for life beyond Earth."

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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-2024-STG

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Host institution

AGENCIA ESTATAL CONSEJO SUPERIOR DE INVESTIGACIONES CIENTIFICAS
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.

€ 1 478 665,00
Address
CALLE SERRANO 117
28006 MADRID
Spain

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Region
Comunidad de Madrid Comunidad de Madrid Madrid
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.

€ 1 478 665,00

Beneficiaries (1)

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