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An Entity of Type : dbo:Star, within Data Space : dbpedia.org associated with source document(s)
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K2-32 is a G9-type main sequence star slightly smaller and less massive than the sun. Four confirmed transiting exoplanets are known to orbit this star. A study of atmospheric escape from the planet K2-32b caused by high-energy stellar irradiation indicates that the star has always been a very slow rotator.

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  • K2-32 (en)
  • K2-32 (ja)
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  • K2-32 is a G9-type main sequence star slightly smaller and less massive than the sun. Four confirmed transiting exoplanets are known to orbit this star. A study of atmospheric escape from the planet K2-32b caused by high-energy stellar irradiation indicates that the star has always been a very slow rotator. (en)
  • K2-32とは、太陽よりわずかに小さく、質量が小さいスペクトル分類がG9型の主系列星である。4つの確認されたトランジットを起こす太陽系外惑星がK2-32の周囲を公転していることが知られている。高エネルギーのK2-32からの照射によって引き起こされた惑星からの大気散逸の研究は、K2-32が常に非常に遅く自転していたことを示している。 (ja)
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  • K2-32 (en)
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  • http://commons.wikimedia.org/wiki/Special:FilePath/K2-32_planetary_system.png
  • http://commons.wikimedia.org/wiki/Special:FilePath/K2-32_transit_light_curves.png
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  • J (en)
appmag 2 passband
  • H (en)
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  • K (en)
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  • G9V (en)
constell
eccentricity
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  • J2000 (en)
exoplanet
  • K2-32b (en)
  • K2-32c (en)
  • K2-32e (en)
  • -2764800.0 (second)
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  • K2-32 is a G9-type main sequence star slightly smaller and less massive than the sun. Four confirmed transiting exoplanets are known to orbit this star. A study of atmospheric escape from the planet K2-32b caused by high-energy stellar irradiation indicates that the star has always been a very slow rotator. (en)
  • K2-32とは、太陽よりわずかに小さく、質量が小さいスペクトル分類がG9型の主系列星である。4つの確認されたトランジットを起こす太陽系外惑星がK2-32の周囲を公転していることが知られている。高エネルギーのK2-32からの照射によって引き起こされた惑星からの大気散逸の研究は、K2-32が常に非常に遅く自転していたことを示している。 (ja)
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