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Kepler-61 is a K-type main-sequence star approximately 1,100 light years from Earth in the constellation Cygnus. 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. On April 24, 2013 it was announced that the star has an extrasolar planet (a super-Earth) orbiting in the inner edge of the habitable zone, named Kepler-61b.

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  • Kepler-61 (en)
  • ケプラー61 (ja)
  • Kepler-61 (pt)
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  • Kepler-61 is a K-type main-sequence star approximately 1,100 light years from Earth in the constellation Cygnus. 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. On April 24, 2013 it was announced that the star has an extrasolar planet (a super-Earth) orbiting in the inner edge of the habitable zone, named Kepler-61b. (en)
  • ケプラー61(英語: Kepler-61)は、地球からはくちょう座の方向に約1,100光年離れた位置にあるK型主系列星である。NASAが打ち上げた通過を起こす惑星を発見するために打ち上げた、ケプラー宇宙望遠鏡の観測領域の中に位置している。2013年4月24日、この恒星のハビタブルゾーンの内縁付近を公転している太陽系外惑星を発見したと発表された。 (ja)
  • Kepler-61 é uma estrela anã vermelha de 15ª magnitude aparente na constelação de Cygnus. É uma estrela jovem com uma idade de 1 bilhão de anos. É ligeiramente mais densa do que o Sol com 63,5% de sua massa e 62% de raio. Por ser uma anã vermelha, é mais fria do que o Sol com uma temperatura de 4 017 K. Um exoplaneta chamado Kepler-61b, uma superterra, orbita na zona habitável. (pt)
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  • Kepler-61 (en)
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  • Kepler-61 (en)
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  • http://commons.wikimedia.org/wiki/Special:FilePath/LombergA1024.jpg
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  • >1 (en)
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  • K7V (en)
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  • <0.25 (en)
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  • Kepler-61 (en)
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  • J2000 (en)
exoplanet
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  • >89.80 (en)
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