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V399 Carinae (V399 Car, P Carinae, P Car, 195 G. Carinae) is a variable star in the constellation Carina. The spectral type of V399 Carinae has been variously assigned between A5 and F0, being a bright, luminous supergiant. Its spectrum is described as having a non-photospheric continuum and silicon absorption lines, indicative of high mass loss. V399 lies amongst the stars of the open cluster IC 2581, by far the brightest member of the cluster. It is about 7,500 light years from Earth assuming it is a member of IC 2581, which is given a 62.9% probability.

AttributesValues
rdf:type
rdfs:label
  • V393 Carinae (es)
  • P Carinae (in)
  • V399 Carinae (fr)
  • HD 90772 (it)
  • 195 Carinae (pt)
  • V399 Carinae (en)
  • P Киля (ru)
  • 船底座V399 (zh)
rdfs:comment
  • V393 Carinae (HD 66260 / 2MASS J07590267-6135009) es una estrella variable en la constelación de Carina a 652 años luz del sistema solar y dentro del perímetro de la Vía Láctea.​ La estrella es una gigante luminosa y brillante con un rango espectral que varía entre A5 y F0. Se describe que su espectro tiene un continuo no fotosférico con líneas de absorción de silicio, lo que indica una gran pérdida de masa por parte de la estrella. (es)
  • P Carinae (P Car) adalah salah satu bintang di rasi Carina. P Carinae adalah bintang supraraksasa putih tipe A (white A-type supergiant) dengan rata-rata magnitudo 4.65. Bintang ini berada pada jarak sekitar 2000 tahun cahaya dari Bumi. (in)
  • HD 90772 (P Carinae) è una stella supergigante bianca di magnitudine 4,66 situata nella costellazione della Carena. Dista 8000 anni luce circa dal sistema solare. (it)
  • 195 Carinae (P Carinae) é uma estrela na direção da Carina. Possui uma ascensão reta de 10h 27m 24.48s e uma declinação de −57° 38′ 19.7″. Sua magnitude aparente é igual a 4.65. Sua magnitude absoluta é igual a . Pertence à classe espectral A6Ia. É uma estrela variável cefeida. (pt)
  • О звезде p Киля см. PP Киля P Киля (P Car, V399 Киля, V399 Car) — звезда в созвездии Киля. P Киля — белый сверхгигант класса А с видимой звёздной величиной +4,65. Расстояние до Земли составляет около 2308 парсек. является переменной класса цефеид, и её блеск меняется в пределах от +4,63 до +4,72 с периодом в 88,3 дня. (ru)
  • 船底座V399,又名CP-57 3256,HD 90772、SAO 238077、HR 4110,是船底座的一颗恒星,视星等为4.66,位于銀經284.59,銀緯0.01,其B1900.0坐标为赤經10h 23m 40.9s,赤緯-57° 0.01′ 43″。 (zh)
  • V399 Carinae (en abrégé V399 Car), aussi connue comme P Carinae (P Car) et 195 G. Carinae, est une étoile variable de la constellation de la Carène. Il s'agit d'une supergéante lumineuse, à qui l'on a attribué divers types spectraux compris entre A5 et F0. L'étoile est plus de 300 000 fois plus lumineuse que le Soleil et sa magnitude absolue est estimée à -8,8. Son spectre est décrit comme possédant un continuum non-photosphérique et des raies d'absorption du silicium, ce qui indique que l'étoile perd de la masse à un taux élevé. (fr)
  • V399 Carinae (V399 Car, P Carinae, P Car, 195 G. Carinae) is a variable star in the constellation Carina. The spectral type of V399 Carinae has been variously assigned between A5 and F0, being a bright, luminous supergiant. Its spectrum is described as having a non-photospheric continuum and silicon absorption lines, indicative of high mass loss. V399 lies amongst the stars of the open cluster IC 2581, by far the brightest member of the cluster. It is about 7,500 light years from Earth assuming it is a member of IC 2581, which is given a 62.9% probability. (en)
foaf:name
  • V399 Carinae (en)
foaf:depiction
  • http://commons.wikimedia.org/wiki/Special:FilePath/V399CarLightCurve.png
  • http://commons.wikimedia.org/wiki/Special:FilePath/Red_circle.svg
  • http://commons.wikimedia.org/wiki/Special:FilePath/Carina_constellation_map.svg
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