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Communication Dans Un Congrès Année : 2011

PLATO : PLAnetary Transits and Oscillations of stars

Résumé

PLATO is a M-class candidate in the ESA Cosmic Vision program. PLATO's objective is to characterize exoplanets and their host stars in the solar neighbourhood. While it builds on the heritage from CoRoT and Kepler, the major breakthrough will come from its strong focus on bright targets (mV

Dates et versions

hal-03733857 , version 1 (21-07-2022)

Identifiants

Citer

Claude Catala, Thierry Appourchaux. PLATO : PLAnetary Transits and Oscillations of stars. GONG-SoHO 24: A new era of seismology of the sun and solar-like stars, Jun 2010, Aix-en-Provence, France, France. pp.2084, ⟨10.1088/1742-6596/271/1/012084⟩. ⟨hal-03733857⟩
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