. "V520 \u041A\u0438\u043B\u044F (V520 Car / w Car / w Carinae) \u2014 \u043E\u0440\u0430\u043D\u0436\u0435\u0432\u044B\u0439 \u0433\u0438\u0433\u0430\u043D\u0442 \u0441\u043F\u0435\u043A\u0442\u0440\u0430\u043B\u044C\u043D\u043E\u0433\u043E \u043A\u043B\u0430\u0441\u0441\u0430 \u041A \u0432 \u0441\u043E\u0437\u0432\u0435\u0437\u0434\u0438\u0438 \u041A\u0438\u043B\u044F \u0441 \u0432\u0438\u0434\u0438\u043C\u043E\u0439 \u0437\u0432\u0451\u0437\u0434\u043D\u043E\u0439 \u0432\u0435\u043B\u0438\u0447\u0438\u043D\u043E\u0439 +4.58, \u0443\u0434\u0430\u043B\u0451\u043D \u043E\u0442 \u0417\u0435\u043C\u043B\u0438 \u043D\u0430 700 \u0441\u0432\u0435\u0442\u043E\u0432\u044B\u0445 \u043B\u0435\u0442. \u041A\u043B\u0430\u0441\u0441\u0438\u0444\u0438\u0446\u0438\u0440\u0443\u0435\u0442\u0441\u044F \u043A\u0430\u043A \u043D\u0435\u043F\u0440\u0430\u0432\u0438\u043B\u044C\u043D\u0430\u044F \u043F\u0435\u0440\u0435\u043C\u0435\u043D\u043D\u0430\u044F \u0437\u0432\u0435\u0437\u0434\u0430, \u0445\u0430\u043E\u0442\u0438\u0447\u0435\u0441\u043A\u0438 \u043C\u0435\u043D\u044F\u0435\u0442 \u0441\u0432\u043E\u0439 \u0431\u043B\u0435\u0441\u043A \u0432 \u0438\u043D\u0442\u0435\u0440\u0432\u0430\u043B\u0435 \u043E\u0442 +4.63 \u0434\u043E +4.70."@ru . . . . . . . . . . . . . . . "HD 93070"@it . . . . . . . "\u22123.63"@en . . . . . . "+3.10"@en . . . "5067754"^^ . "HD 93070"@zh . . . . . "J2000"@en . "V520 Carinae (en abr\u00E9g\u00E9 V520 Car) est une \u00E9toile variable de cinqui\u00E8me magnitude de la constellation australe de la Car\u00E8ne. Elle porte \u00E9galement la d\u00E9signation de Bayer de w Carinae, V520 Carinae \u00E9tant sa d\u00E9signation d'\u00E9toile variable. D'apr\u00E8s la mesure de sa parallaxe annuelle par le satellite Hipparcos, l'\u00E9toile est distante d'approximativement \u223C1 140 a.l. (\u223C350 pc) de la Terre. Elle s'\u00E9loigne du Syst\u00E8me solaire \u00E0 une vitesse radiale de +9 km/s. Elle est un membre propos\u00E9 du groupe mouvant d'\u00E9toiles d'IC 2391. V520 Carinae a \u00E9t\u00E9 class\u00E9e comme une \u00E9toile g\u00E9ante rouge de type spectral K4III par Houk & Cowley (1975), mais aussi comme une superg\u00E9ante de K3Ib par Humphreys (1970). C'est une variable irr\u00E9guli\u00E8re \u00E0 longue p\u00E9riode et sa magnitude apparente varie entre 4,50 et 4,59 sans p\u00E9riodicit\u00E9. Le rayon de l'\u00E9toile est actuellement 131 fois plus grand que le rayon solaire ; apr\u00E8s avoir \u00E9puis\u00E9 les r\u00E9serves en hydrog\u00E8ne qui \u00E9taient contenues dans son noyau, elle s'est refroidie et \u00E9tendue. Une comparaison de ses propri\u00E9t\u00E9s avec des trajectoires d'\u00E9volution th\u00E9oriques sugg\u00E8rent qu'elle est \u00E2g\u00E9e de 33 millions d'ann\u00E9es et que sa masse est 7,9 fois plus grande que celle du Soleil. L'\u00E9toile est environ 3 600 fois plus luminseuse que le Soleil et sa temp\u00E9rature de surface est de 3 903 K."@fr . . . . . . . . . "HD 93070\uFF0C\u53C8\u540DCP-59 2532\uFF0CSAO 251090\u3001HR 4200\uFF0C\u662F\u4E00\u9897\u6052\u661F\uFF0C\u89C6\u661F\u7B49\u4E3A4.57\uFF0C\u4F4D\u4E8E\u9280\u7D93287.84\uFF0C\u9280\u7DEF-1.5\uFF0C\u5176B1900.0\u5750\u6807\u4E3A\u8D64\u7D9310h 39m 43.8s\uFF0C\u8D64\u7DEF-60\u00B0 -1.5\u2032 32\u2033\u3002"@zh . "+4.58"@en . . . ""@en . "V520 \u041A\u0438\u043B\u044F (V520 Car / w Car / w Carinae) \u2014 \u043E\u0440\u0430\u043D\u0436\u0435\u0432\u044B\u0439 \u0433\u0438\u0433\u0430\u043D\u0442 \u0441\u043F\u0435\u043A\u0442\u0440\u0430\u043B\u044C\u043D\u043E\u0433\u043E \u043A\u043B\u0430\u0441\u0441\u0430 \u041A \u0432 \u0441\u043E\u0437\u0432\u0435\u0437\u0434\u0438\u0438 \u041A\u0438\u043B\u044F \u0441 \u0432\u0438\u0434\u0438\u043C\u043E\u0439 \u0437\u0432\u0451\u0437\u0434\u043D\u043E\u0439 \u0432\u0435\u043B\u0438\u0447\u0438\u043D\u043E\u0439 +4.58, \u0443\u0434\u0430\u043B\u0451\u043D \u043E\u0442 \u0417\u0435\u043C\u043B\u0438 \u043D\u0430 700 \u0441\u0432\u0435\u0442\u043E\u0432\u044B\u0445 \u043B\u0435\u0442. \u041A\u043B\u0430\u0441\u0441\u0438\u0444\u0438\u0446\u0438\u0440\u0443\u0435\u0442\u0441\u044F \u043A\u0430\u043A \u043D\u0435\u043F\u0440\u0430\u0432\u0438\u043B\u044C\u043D\u0430\u044F \u043F\u0435\u0440\u0435\u043C\u0435\u043D\u043D\u0430\u044F \u0437\u0432\u0435\u0437\u0434\u0430, \u0445\u0430\u043E\u0442\u0438\u0447\u0435\u0441\u043A\u0438 \u043C\u0435\u043D\u044F\u0435\u0442 \u0441\u0432\u043E\u0439 \u0431\u043B\u0435\u0441\u043A \u0432 \u0438\u043D\u0442\u0435\u0440\u0432\u0430\u043B\u0435 \u043E\u0442 +4.63 \u0434\u043E +4.70."@ru . . . . . . . . . "V520 Carinae is a single star in the southern constellation of Carina. It has the Bayer designation w Carinae, while V520 Carinae is a variable star designation. The star has an orange hue and is faintly visible to the naked eye with an apparent visual magnitude that fluctuates around +4.58. It is located at a distance of approximately 1,140 light years from the Sun based on parallax, and it is drifting further away with a radial velocity of +9 km/s. It is a candidate member of the IC 2391 moving group of co-moving stars. This is an aging giant star with a stellar classification of K4III, although Humphreys (1970) found a supergiant class of K3Ib. It is a suspected slow irregular variable of type Lc and its brightness varies from magnitude +4.50 to +4.59 with no periodicity. The star now has 131 times the girth of the Sun, having exhausted the supply of hydrogen at its core then cooled and expanded. Comparison with theoretical evolutionary tracks suggests it is 33 million years old with 7.9 times the mass of the Sun, although analysis of its motion suggests it may be an astrometric binary with a mass of 1.014 M\u2609. The star is radiating 3,600 times the luminosity of the Sun from its enlarged photosphere at an effective temperature of 3,903 K."@en . . . . . . "V520 \u041A\u0438\u043B\u044F"@ru . "0.17"^^ . . . . . . "HD 93070\uFF0C\u53C8\u540DCP-59 2532\uFF0CSAO 251090\u3001HR 4200\uFF0C\u662F\u4E00\u9897\u6052\u661F\uFF0C\u89C6\u661F\u7B49\u4E3A4.57\uFF0C\u4F4D\u4E8E\u9280\u7D93287.84\uFF0C\u9280\u7DEF-1.5\uFF0C\u5176B1900.0\u5750\u6807\u4E3A\u8D64\u7D9310h 39m 43.8s\uFF0C\u8D64\u7DEF-60\u00B0 -1.5\u2032 32\u2033\u3002"@zh . . . . "V520 Carinae"@en . . . "\u221214.75"@en . . "8184"^^ . . "HD 93070, nota anche come V520 Carinae, \u00E8 una stella gigante arancione di magnitudine 4,58 situata nella costellazione della Carena. Dista 1433 anni luce dal sistema solare."@it . . "1083875443"^^ . . . . "V520 Carinae (en abr\u00E9g\u00E9 V520 Car) est une \u00E9toile variable de cinqui\u00E8me magnitude de la constellation australe de la Car\u00E8ne. Elle porte \u00E9galement la d\u00E9signation de Bayer de w Carinae, V520 Carinae \u00E9tant sa d\u00E9signation d'\u00E9toile variable. D'apr\u00E8s la mesure de sa parallaxe annuelle par le satellite Hipparcos, l'\u00E9toile est distante d'approximativement \u223C1 140 a.l. (\u223C350 pc) de la Terre. Elle s'\u00E9loigne du Syst\u00E8me solaire \u00E0 une vitesse radiale de +9 km/s. Elle est un membre propos\u00E9 du groupe mouvant d'\u00E9toiles d'IC 2391."@fr . . . . . . . . . . "HD 93070, nota anche come V520 Carinae, \u00E8 una stella gigante arancione di magnitudine 4,58 situata nella costellazione della Carena. Dista 1433 anni luce dal sistema solare."@it . . . . . . . "2.86"^^ . . . . "224 Carinae (w Carinae) \u00E9 uma estrela na dire\u00E7\u00E3o da Carina. Possui uma ascens\u00E3o reta de 10h 43m 32.31s e uma declina\u00E7\u00E3o de \u221260\u00B0 33\u2032 59.9\u2033. Sua magnitude aparente \u00E9 igual a 4.58. Considerando sua dist\u00E2ncia de 1065 anos-luz em rela\u00E7\u00E3o \u00E0 Terra, sua magnitude absoluta \u00E9 igual a \u22122.99. Pertence \u00E0 classe espectral K3Ib. \u00C9 uma estrela vari\u00E1vel irregular."@pt . . . "K4III"@en . "224 Carinae"@pt . "V520 Carinae is a single star in the southern constellation of Carina. It has the Bayer designation w Carinae, while V520 Carinae is a variable star designation. The star has an orange hue and is faintly visible to the naked eye with an apparent visual magnitude that fluctuates around +4.58. It is located at a distance of approximately 1,140 light years from the Sun based on parallax, and it is drifting further away with a radial velocity of +9 km/s. It is a candidate member of the IC 2391 moving group of co-moving stars."@en . "V520 Carinae"@fr . . . "224 Carinae (w Carinae) \u00E9 uma estrela na dire\u00E7\u00E3o da Carina. Possui uma ascens\u00E3o reta de 10h 43m 32.31s e uma declina\u00E7\u00E3o de \u221260\u00B0 33\u2032 59.9\u2033. Sua magnitude aparente \u00E9 igual a 4.58. Considerando sua dist\u00E2ncia de 1065 anos-luz em rela\u00E7\u00E3o \u00E0 Terra, sua magnitude absoluta \u00E9 igual a \u22122.99. Pertence \u00E0 classe espectral K3Ib. \u00C9 uma estrela vari\u00E1vel irregular."@pt . . . . . . .