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HAT-P-23 is a G-type main-sequence star about 1200 light-years away. It has a rapid rotation (rotation period equal to 7 days) for its advanced age of 4 billion years, and exhibits a strong starspot activity. The star may be in the process of being spun up by the giant planet on close orbit. The star is enriched in heavy elements, having about 140% amount of metals compared to solar abundance.

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  • HAT-P-23 (en)
  • HAT-P-23 (ja)
  • HAT-P-23 (ru)
  • HAT-P-23 (sv)
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  • HAT-P-23 is a G-type main-sequence star about 1200 light-years away. It has a rapid rotation (rotation period equal to 7 days) for its advanced age of 4 billion years, and exhibits a strong starspot activity. The star may be in the process of being spun up by the giant planet on close orbit. The star is enriched in heavy elements, having about 140% amount of metals compared to solar abundance. (en)
  • HAT-P-23は、いるか座の方角におよそ1,200光年の距離にある恒星である。周囲に1つの太陽系外惑星が発見されている。 (ja)
  • HAT-P-23 — звезда, которая находится в созвездии Дельфина на расстоянии около 1281 светового года от нас. Вокруг звезды обращается, как минимум, одна планета. (ru)
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  • HAT-P-23 (en)
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  • http://commons.wikimedia.org/wiki/Special:FilePath/Exoplanet_Comparison_HAT-P-23_b.png
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  • J (en)
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  • G0V (en)
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  • J2000 (en)
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  • HAT-P-23 is a G-type main-sequence star about 1200 light-years away. It has a rapid rotation (rotation period equal to 7 days) for its advanced age of 4 billion years, and exhibits a strong starspot activity. The star may be in the process of being spun up by the giant planet on close orbit. The star is enriched in heavy elements, having about 140% amount of metals compared to solar abundance. (en)
  • HAT-P-23は、いるか座の方角におよそ1,200光年の距離にある恒星である。周囲に1つの太陽系外惑星が発見されている。 (ja)
  • HAT-P-23 — звезда, которая находится в созвездии Дельфина на расстоянии около 1281 светового года от нас. Вокруг звезды обращается, как минимум, одна планета. (ru)
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