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Content archived on 2024-06-18

Exploring the physics of Proto-stars and Extra-solar PlanetS

Objective

The PEPS project is dedicated to the understanding of low-mass star, brown dwarf and giant planet formation and evolution and to the characterization of their internal structure and observable properties. The aim is to develop a sound theoretical foundation and a new generation of modelling tools, in close interaction with observing and experimental programs. The ultimate goal of the project is to provide a consistent description of the different stages from the very formation process to the long term evolution for these objects, characterizing the initial conditions of star/planet formation and exploring their impact on the subsequent mechanical (mass, radius, internal structure and composition), thermal (surface temperature, luminosity) and spectral properties. A dedicated part of the project will focus on exo-Earth planets and on the identification of bio-signatures in their atmosphere, opening an avenue to exobiology.

Fields of science (EuroSciVoc)

CORDIS classifies projects with EuroSciVoc, a multilingual taxonomy of fields of science, through a semi-automatic process based on NLP techniques. See: https://op.europa.eu/en/web/eu-vocabularies/euroscivoc.

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Call for proposal

ERC-2009-AdG
See other projects for this call

Host institution

CENTRE NATIONAL DE LA RECHERCHE SCIENTIFIQUE CNRS
EU contribution
€ 1 078 503,00
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
Links
Total cost
No data

Beneficiaries (2)

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