R Carinae
http://dbpedia.org/resource/R_Carinae an entity of type: Thing
R Carinae est une étoile de la constellation de la Carène. Elle est située à environ 182 pc (∼594 a.l.) de la Terre. R Carinae est une géante rouge dont le type spectral varie entre M4e et M8e. Elle est classée comme une variable de type Mira et sa luminosité varie entre les magnitudes +3,9 et +10,5 sur une période de 305,6 jours.
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.HD 82901 è una stella gigante rossa di magnitudine 6,1 situata nella costellazione della Carena. Dista 416 anni luce dal sistema solare.
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R Carinae är en pulserande variabel av Mira Ceti-typ (M)i stjärnbilden Kölen. Stjärnan var den första i Kölen som fick en variabelbeteckning. R Carinae varierar mellan visuell magnitud +3,9 och 10,5 med en period av 307,0 dygn.
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船底座R，又名CP-62 1253，HD 82901、SAO 250614、HR 3816，是船底座的一颗恒星，视星等为6.1，位于銀經282.27，銀緯-8.21，其B1900.0坐标为赤經9h 29m 43.6s，赤緯-62° -8.21′ 46″。
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R Carinae is a double star in the southern constellation of Carina. The brighter component is a variable star that can be viewed with the naked eye at peak brightness, but is usually too faint to be seen without a telescope, having an apparent visual magnitude that fluctuates around 7.43. This star is located at a distance of approximately 1,300 light years from the Sun based on parallax, and is drifting further away with a radial velocity of +28 km/s. The companion is a magnitude 11.30 star at an angular separation of 2.10″ along a position angle of 132° from the main star, as of 2015.
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R Carinae
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HD 82901
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R Carinae
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R Carinae
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船底座R
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1.48
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M6/7pe
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J2000.0
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+22.232
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R Carinae est une étoile de la constellation de la Carène. Elle est située à environ 182 pc (∼594 a.l.) de la Terre. R Carinae est une géante rouge dont le type spectral varie entre M4e et M8e. Elle est classée comme une variable de type Mira et sa luminosité varie entre les magnitudes +3,9 et +10,5 sur une période de 305,6 jours.
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R Carinae is a double star in the southern constellation of Carina. The brighter component is a variable star that can be viewed with the naked eye at peak brightness, but is usually too faint to be seen without a telescope, having an apparent visual magnitude that fluctuates around 7.43. This star is located at a distance of approximately 1,300 light years from the Sun based on parallax, and is drifting further away with a radial velocity of +28 km/s. The main component is an aging red giant star on the asymptotic giant branch with a stellar classification of M6/7pe. It is classified as a pulsating Mira type variable star and its visual brightness varies with an average amplitude of 4.25 magnitudes over a period of 303.99±1.08 d. Its average maximum visual magnitude is 5.05±0.45, but the brightest observed maximum was magnitude 3.9 This star is surrounded by a dusty shell, with properties that are consistent with iron-poor silicates or corundum, extending from around three stellar radii outward. The companion is a magnitude 11.30 star at an angular separation of 2.10″ along a position angle of 132° from the main star, as of 2015.
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.HD 82901 è una stella gigante rossa di magnitudine 6,1 situata nella costellazione della Carena. Dista 416 anni luce dal sistema solare.
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R Carinae är en pulserande variabel av Mira Ceti-typ (M)i stjärnbilden Kölen. Stjärnan var den första i Kölen som fick en variabelbeteckning. R Carinae varierar mellan visuell magnitud +3,9 och 10,5 med en period av 307,0 dygn.
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船底座R，又名CP-62 1253，HD 82901、SAO 250614、HR 3816，是船底座的一颗恒星，视星等为6.1，位于銀經282.27，銀緯-8.21，其B1900.0坐标为赤經9h 29m 43.6s，赤緯-62° -8.21′ 46″。
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8008
