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A PRECISE ASTEROSEISMIC AGE AND RADIUS FOR THE EVOLVED SUN-LIKE STAR KIC 11026764

Metcalfe, TS; Monteiro, MJPFG; Thompson, MJ; Molenda Zakowicz, J; Appourchaux, T; Chaplin, WJ; Dogan, G; Eggenberger, P; Bedding, TR; Bruntt, H

The primary science goal of the Kepler Mission is to provide a census of exoplanets in the solar neighborhood, including the identification and characterization of habitable Earth-like planets. The asteroseismic capabilities of the mission are being used to determine precise radii and ages for the target stars from their solar-like oscillations. Chaplin et al. published observations of three bright G-type stars...

Date: 2010   |   Origin: Repositório Aberto da Universidade do Porto
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