Kepler-138 (original) (raw)

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Kepler-138 (auch KOI-314) ist ein Roter Zwerg im Sternbild Leier, der rund 217 Lichtjahre von der Sonne entfernt ist. Der Stern besitzt ein Planetensystem mit drei bekannten Exoplaneten. (de)
Kepler-138, also known as KOI-314, is a red dwarf located in the constellation Lyra, 218 light years from Earth. It is located within the field of vision of the Kepler spacecraft, the satellite that NASA's Kepler Mission used to detect planets that may be transiting their stars. The star hosts three confirmed planets, including the lowest-mass planet with a measured mass and size discovered to date, Kepler-138b, with a mass comparable to that of Mars. Kepler-138d is remarkable for being a gas dwarf despite being only slightly heavier than Earth. (en)
ケプラー138（英語: Kepler-138）または KOI-314 は、地球から見てこと座の方向に約219光年離れたところにある赤色矮星である。2022年12月時点で、周囲に3つの太陽系外惑星が存在していることが知られており、さらに低質量の惑星候補の存在が示されている。 (ja)
Kepler-138 é uma anã vermelha localizada na constelação Lyra, há 200 anos-luz da Terra. Ela está localizada no campo de visão do telescópio espacial Kepler. Quatro planetas orbitam a estrela, sendo eles: Kepler-138b, Kepler-138c, Kepler-138d. e Kepler-138e (pt)
克卜勒138（Kepler-138），舊稱KOI-314，是一顆位於天琴座的紅矮星，距離地球約200光年。該恆星位於克卜勒太空望遠鏡的觀測視野內，因此如有行星在恆星盤面通過時有機會被觀測到。克卜勒138已確認有3顆行星存在，其中一顆是經測量後確認為發現時體積和質量最低的，它的質量幾乎和地球相等。KOI-314c因為密度過低，被認為是氣體行星，而非岩石行星，即使它的質量與地球大約相等。 (zh)
Kepler-138 (KOI-314) — звезда, которая находится в созвездии Лиры на расстоянии около 217 световых лет от Солнца. Вокруг звезды обращаются, как минимум, три планеты. (ru)

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Kepler-138 (auch KOI-314) ist ein Roter Zwerg im Sternbild Leier, der rund 217 Lichtjahre von der Sonne entfernt ist. Der Stern besitzt ein Planetensystem mit drei bekannten Exoplaneten. (de)
Kepler-138, also known as KOI-314, is a red dwarf located in the constellation Lyra, 218 light years from Earth. It is located within the field of vision of the Kepler spacecraft, the satellite that NASA's Kepler Mission used to detect planets that may be transiting their stars. The star hosts three confirmed planets, including the lowest-mass planet with a measured mass and size discovered to date, Kepler-138b, with a mass comparable to that of Mars. Kepler-138d is remarkable for being a gas dwarf despite being only slightly heavier than Earth. (en)
ケプラー138（英語: Kepler-138）または KOI-314 は、地球から見てこと座の方向に約219光年離れたところにある赤色矮星である。2022年12月時点で、周囲に3つの太陽系外惑星が存在していることが知られており、さらに低質量の惑星候補の存在が示されている。 (ja)
Kepler-138 é uma anã vermelha localizada na constelação Lyra, há 200 anos-luz da Terra. Ela está localizada no campo de visão do telescópio espacial Kepler. Quatro planetas orbitam a estrela, sendo eles: Kepler-138b, Kepler-138c, Kepler-138d. e Kepler-138e (pt)
克卜勒138（Kepler-138），舊稱KOI-314，是一顆位於天琴座的紅矮星，距離地球約200光年。該恆星位於克卜勒太空望遠鏡的觀測視野內，因此如有行星在恆星盤面通過時有機會被觀測到。克卜勒138已確認有3顆行星存在，其中一顆是經測量後確認為發現時體積和質量最低的，它的質量幾乎和地球相等。KOI-314c因為密度過低，被認為是氣體行星，而非岩石行星，即使它的質量與地球大約相等。 (zh)
Kepler-138 (KOI-314) — звезда, которая находится в созвездии Лиры на расстоянии около 217 световых лет от Солнца. Вокруг звезды обращаются, как минимум, три планеты. (ru)

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Kepler-138 (de)
Kepler-138 (en)
ケプラー138 (ja)
Kepler-138 (pt)
Kepler-138 (ru)
克卜勒138 (zh)

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