| http://dbpedia.org/ontology/abstract
|
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。
, K2-32 is a G9-type main sequence star slig … 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. star has always been a very slow rotator.
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http://commons.wikimedia.org/wiki/Special:FilePath/K2-32_transit_light_curves.png?width=300 +
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http://exoplanet.eu/catalog/k2-32_d/ +
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, http://exoplanet.eu/catalog/k2-32_c/ +
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61899876
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15316
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1119035886
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J
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H
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K
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G9V
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http://dbpedia.org/resource/Ophiuchus +
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0.05
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J2000
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K2-32c
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89
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8.1
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0.0153
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6.3939
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31.71701
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2.134
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0.7
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0.18422
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http://dbpedia.org/resource/Variable_star +
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http://dbpedia.org/resource/Category:Planetary_systems_with_four_confirmed_planets +
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http://en.wikipedia.org/wiki/K2-32?oldid=1119035886&ns=0 +
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http://commons.wikimedia.org/wiki/Special:FilePath/K2-32_planetary_system.png +
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http://en.wikipedia.org/wiki/K2-32 +
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K2-32
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https://global.dbpedia.org/id/AtxX2 +
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|
| rdfs:comment |
K2-32 is a G9-type main sequence star slig … 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. star has always been a very slow rotator.
, 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。
|
| rdfs:label |
K2-32
|
