Star-planet interactions and dynamical evolution of exoplanetary systems
作者： Cilia Damiani
DOI: 10.1051/EPJCONF/201510104004
关键词:
摘要: The dynamical evolution of planetary systems, after the evaporation accretion disk, is result competition between tidal dissipation and net angular momentum loss system. description diversity orbital configurations, correlations parameters observed system (e.g. in case hot jupiters), still limited by our understanding transport within stars, its effective magnetic braking. After discussing challenges modelling for exoplanets, I will review recent results showing importance interactions to test models formation. This kind studies rely on determination stellar radii, masses ages. Major advances thus be obtained with PLATO 2.0 mission, selected as next M-class mission ESA’s Cosmic Vision plan, that allow complete characterisation host stars using asteroseismology.
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