The host stars of Kepler 's habitable exoplanets: superflares, rotation and activity
The host stars of Kepler 's habitable exoplanets: superflares, rotation and activity
复制标题
开普勒宜居系外行星的主恒星:超级耀斑、自转和活动
DOI:
10.1093/mnras/stv2419
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发表时间:
2015
影响因子:
4.8
通讯作者:
Armstrong D
中科院分区:
文献类型:
--
作者:
Armstrong D
We embark on a detailed study of the light curves ofKepler's most Earth-like exoplanet host stars using the full length ofKeplerdata. We derive rotation periods, photometric activity indices, flaring energies, mass-loss rates, gyrochronological ages, X-ray luminosities and consider implications for the planetary magnetospheres and habitability. Furthermore, we present the detection of superflares in the light curve of Kepler-438, the exoplanet with the highest Earth Similarity Index to date. Kepler-438b orbits at a distance of 0.166 au to its host star, and hence may be susceptible to atmospheric stripping. Our sample is taken from the Habitable Exoplanet Catalogue, and consists of the stars Kepler-22, Kepler-61, Kepler-62, Kepler-174, Kepler-186, Kepler-283, Kepler-296, Kepler-298, Kepler-438, Kepler-440, Kepler-442, Kepler-443 and KOI-4427, between them hosting 15 of the most habitable transiting planets known to date fromKepler.