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Kepler-14 is a binary star system targeted by the Kepler spacecraft. It is host to one known planet: the Jupiter-like Kepler-14b. The star system was identified by Kepler as a possible planetary host, but when imaging revealed that Kepler-14 was a binary star system and not a single star, the confirmation process became protracted. The stars are separated by at least 280 AU, and the stars complete an orbit around a common center of mass every 2800 years. Both stars are larger than the Sun. They are of similar absolute magnitudes; however, the primary star is brighter as seen from Earth.

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  • Kepler-14 (in)
  • Kepler-14 (en)
  • Kepler-14 (fr)
  • 케플러-14 (ko)
  • ケプラー14 (ja)
  • Kepler-14 (ru)
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  • Kepler-14 is a binary star system targeted by the Kepler spacecraft. It is host to one known planet: the Jupiter-like Kepler-14b. The star system was identified by Kepler as a possible planetary host, but when imaging revealed that Kepler-14 was a binary star system and not a single star, the confirmation process became protracted. The stars are separated by at least 280 AU, and the stars complete an orbit around a common center of mass every 2800 years. Both stars are larger than the Sun. They are of similar absolute magnitudes; however, the primary star is brighter as seen from Earth. (en)
  • Kepler-14 est une étoile binaire située à environ ∼3 200 a.l. (∼981 pc) du Système solaire, dans la constellation de la Lyre. Les deux composantes de ce système binaire sont deux étoiles distantes l'une de l'autre d'au moins 280 UA et orbitant l'une autour de l'autre en 2 800 ans environ. Trop proches l'une de l'autre pour pouvoir être étudiées séparément, leurs propriétés résultantes ont été analysées ensemble et correspondent à un astre unique de 1,512 masse solaire et 2,048 rayons solaires de type spectral F et ayant une température effective de 6 395 K. (fr)
  • ケプラー14 (英: Kepler-14) とは、地球から見てこと座の方向、約3,196光年(約980パーセク)先にある連星系である。2011年に、太陽系外惑星が発見された。 (ja)
  • 케플러-14는 케플러 탐사선이 관측목표로 삼은 쌍성이다. 이 별은 목성형 외계 행성 케플러-14b를 거느리고 있다. 원래 케플러 관측선은 이 별을 외계 행성을 거느릴 가능성이 있는 후보로 인식했으나, 사진촬영으로 케플러 14가 쌍성계임을 알게 된 후 검증절차는 지연되었다. 쌍성 구성원 둘은 최소 280 천문단위 떨어져 있으며 서로의 질량중심을 2800년에 1회 돌고 있다. 둘 다 태양보다 크고 밝으며 절대 등급은 비슷한 수준이다. 그러나 지구에서 볼 때는 주인별 쪽이 좀 더 밝다. (ko)
  • Kepler-14 — звезда в созвездии Лиры на расстоянии около 3196 световых лет от нас. Вокруг звезды обращается как минимум одна планета. (ru)
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  • Kepler-14 (en)
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  • Kepler-14B (en)
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  • http://commons.wikimedia.org/wiki/Special:FilePath/PalomarObservatory.jpg
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