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ケプラー17 (英: Kepler-17) とは、はくちょう座の方向に2400光年離れた位置にあるG型主系列星である。
, Kepler-17 ou KOI-203 est une étoile de la constellation du Cygne située à environ ∼2 400 a.l. (∼736 pc) de la Terre. Cette naine jaune de type spectral G5V est une étoile variable par rotation autour de laquelle la planète Kepler-17 b orbite.
, Kepler-17 is a main-sequence yellow dwarf star that is much more active than the Sun with starspots covering roughly 6% of its surface. Starspots are long-lived, with at least one persisting for 1400 days.
, Kepler-17 — звезда, которая находится в созвездии Лебедь на расстоянии около 2283 световых лет от нас. Вокруг звезды обращается, как минимум, одна планета.
, Kepler-17 — зірка, яка знаходиться в сузір'ї Лебедя на відстані близько 2 283 світлових років (800 парсек) від нас. Навколо зірки обертається, як мінімум, одна планета.
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| rdfs:comment |
ケプラー17 (英: Kepler-17) とは、はくちょう座の方向に2400光年離れた位置にあるG型主系列星である。
, Kepler-17 is a main-sequence yellow dwarf star that is much more active than the Sun with starspots covering roughly 6% of its surface. Starspots are long-lived, with at least one persisting for 1400 days.
, Kepler-17 — зірка, яка знаходиться в сузір'ї Лебедя на відстані близько 2 283 світлових років (800 парсек) від нас. Навколо зірки обертається, як мінімум, одна планета.
, Kepler-17 — звезда, которая находится в созвездии Лебедь на расстоянии около 2283 световых лет от нас. Вокруг звезды обращается, как минимум, одна планета.
, Kepler-17 ou KOI-203 est une étoile de la constellation du Cygne située à environ ∼2 400 a.l. (∼736 pc) de la Terre. Cette naine jaune de type spectral G5V est une étoile variable par rotation autour de laquelle la planète Kepler-17 b orbite.
|
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Kepler-17
, ケプラー17
|
