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RT Carinae, also known as CD-58 3538, is a variable star in the Carina Nebula in the constellation Carina. It has a mean apparent magnitude of +8.55. RT Carinae is a red supergiant with a spectral type of M2+ Iab and has a temperature of 3,660 K. With a diameter 861 times that of the Sun, it is one of the largest stars known. The luminosity is estimated to be 120,000 times more luminous than the Sun. It is close to the open cluster Trumpler 15, but is not thought to be a member. It appears to be surrounded by a dusty nebula, possibly material ejected from the star itself.

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  • RT Carinae (es)
  • RT Carinae (it)
  • りゅうこつ座RT星 (ja)
  • RT Carinae (en)
  • RT Киля (ru)
  • 船底座RT (zh)
rdfs:comment
  • りゅうこつ座RT星は、りゅうこつ座に位置する赤色超巨星で、8.2等と9.9等の間を変光する脈動変光星でもある。変光星総合カタログでは407.9日の周期で変光するSRC型の変光星に分類しているが、アメリカ変光星観測者協会ではLC型の変光星に分類している。半径は太陽の約1100倍あり、光度は太陽の約200,000倍あるとされている。 (ja)
  • RT Carinae è una stella di magnitudine +8,55 situata nella costellazione della Carena. Appartiene all'associazione stellare e questo consente di stimare la sua distanza in 8200 anni luce dal sistema solare. Con un raggio stimato superiore a 1000 volte quello del Sole è una delle stelle più grandi conosciute. (it)
  • 船底座RT(英語:RT Carinae),亦稱HD 303310、HIP 52562和SAO 238424,是一顆位於船底座中的變星。這顆恆星是至今人類已知體積最大的恆星之一,其半徑約為太陽半徑的1,090倍。 (zh)
  • RT Carinae (RT Car)​ es una estrella variable en la constelación de Carina, la quilla del Navío Argos.De magnitud aparente media +8,55, la medida de la paralaje realizada por el satélite Hipparcos lleva asociado un error de casi el 50%.Sin embargo, su pertenencia al cúmulo estelar -E —al igual que BO Carinae e IX Carinae—, permite estimar su distancia al Sistema Solar en 2500 pársecs (8200 años luz).​ (es)
  • RT Carinae, also known as CD-58 3538, is a variable star in the Carina Nebula in the constellation Carina. It has a mean apparent magnitude of +8.55. RT Carinae is a red supergiant with a spectral type of M2+ Iab and has a temperature of 3,660 K. With a diameter 861 times that of the Sun, it is one of the largest stars known. The luminosity is estimated to be 120,000 times more luminous than the Sun. It is close to the open cluster Trumpler 15, but is not thought to be a member. It appears to be surrounded by a dusty nebula, possibly material ejected from the star itself. (en)
  • RT Киля (RT Car) — переменная звезда в Туманности Киля созвездия Киля. Среднее значение видимой звёздной величины составляет +8,55m. RT Car является красным сверхгигантом спектрального класса M2I и обладает температурой 3625 K. Звезда является одной из крупнейших известных звёзд: диаметр приблизительно в тысячу раз превосходит солнечный. Оценки светимости лежат в интервале от 180 000 до 220 000 светимостей Солнца, среднее значение равно 200 000 светимостей Солнца. (ru)
foaf:name
  • RT Carinae (en)
foaf:depiction
  • http://commons.wikimedia.org/wiki/Special:FilePath/RTCarLightCurve.png
  • http://commons.wikimedia.org/wiki/Special:FilePath/Trumpler15.jpg
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