PEPS

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

Coordinatore	CENTRE NATIONAL DE LA RECHERCHE SCIENTIFIQUE    more Spiacenti, non ci sono informazioni su questo coordinatore. Contattare Fabio per maggiori infomrazioni, grazie.
Nazionalità Coordinatore	France [FR]
Totale costo	2˙376˙000 €
EC contributo	2˙376˙000 €
Programma	FP7-IDEAS-ERC Specific programme: "Ideas" implementing the Seventh Framework Programme of the European Community for research, technological development and demonstration activities (2007 to 2013)
Code Call	ERC-2009-AdG
Funding Scheme	ERC-AG
Anno di inizio	2010
Periodo (anno-mese-giorno)	2010-06-01   -   2016-05-31

 Partecipanti

#	participant	country	role	EC contrib. [€]
1	THE UNIVERSITY OF EXETER  Organization address address: Northcote House, The Queen's Drive city: EXETER postcode: EX4 4QJ contact info Titolo: Dr. Nome: Enda Cognome: Clarke Email: send email Telefono: +44 1392 263744 Fax: +44 1392 263686	UK (EXETER)	beneficiary	1˙297˙497.00
2	CENTRE NATIONAL DE LA RECHERCHE SCIENTIFIQUE  Organization address address: Rue Michel -Ange 3 city: PARIS postcode: 75794 contact info Titolo: Dr. Nome: Gilles Cognome: Chabrier Email: send email Telefono: -72728677 Fax: -72728758	FR (PARIS)	hostInstitution	1˙078˙503.00
3	CENTRE NATIONAL DE LA RECHERCHE SCIENTIFIQUE  Organization address address: Rue Michel -Ange 3 city: PARIS postcode: 75794 contact info Titolo: Dr. Nome: Pascaline Cognome: Toutois Email: send email Telefono: +33 4 72445641 Fax: +33 4 78890851	FR (PARIS)	hostInstitution	1˙078˙503.00

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 Obiettivo del progetto (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.'