"4.75"^^ . . . . "Psi2 Lupi"@en . . . "2438252.97"^^ . "\u041F\u0441\u0438\u00B2 \u0412\u043E\u043B\u043A\u0430 (\u043B\u0430\u0442. \u03C8\u00B2 Lupi), 4 \u0412\u043E\u043B\u043A\u0430 (\u043B\u0430\u0442. 4 Lupi), HD 140008 \u2014 \u0442\u0440\u043E\u0439\u043D\u0430\u044F \u0437\u0432\u0435\u0437\u0434\u0430 \u0432 \u0441\u043E\u0437\u0432\u0435\u0437\u0434\u0438\u0438 \u0412\u043E\u043B\u043A\u0430 \u043D\u0430 \u0440\u0430\u0441\u0441\u0442\u043E\u044F\u043D\u0438\u0438 \u043F\u0440\u0438\u0431\u043B\u0438\u0437\u0438\u0442\u0435\u043B\u044C\u043D\u043E 378 \u0441\u0432\u0435\u0442\u043E\u0432\u044B\u0445 \u043B\u0435\u0442 (\u043E\u043A\u043E\u043B\u043E 116 \u043F\u0430\u0440\u0441\u0435\u043A\u043E\u0432) \u043E\u0442 \u0421\u043E\u043B\u043D\u0446\u0430. \u0412\u0438\u0434\u0438\u043C\u0430\u044F \u0437\u0432\u0451\u0437\u0434\u043D\u0430\u044F \u0432\u0435\u043B\u0438\u0447\u0438\u043D\u0430 \u0437\u0432\u0435\u0437\u0434\u044B \u2014 +4,721m. \u0412\u043E\u0437\u0440\u0430\u0441\u0442 \u0437\u0432\u0435\u0437\u0434\u044B \u043E\u043F\u0440\u0435\u0434\u0435\u043B\u0451\u043D \u043A\u0430\u043A \u043E\u043A\u043E\u043B\u043E 15,9 \u043C\u043B\u043D \u043B\u0435\u0442."@ru . . "Psi2 Lupi (\u03C82 Lup) is a triple star system in the constellation Lupus. It is visible to the naked eye with an apparent magnitude of 4.75. Based upon an annual parallax shift of 8.97 mas as seen from Earth, it is located around 360 light years from the Sun. At that distance, the visual magnitude is diminished by an extinction factor of 0.016\u00B10.009 due to interstellar dust. This system is a member of the Upper Centaurus\u2013Lupus subgroup of the Scorpius\u2013Centaurus association."@en . . "B5 V"@en . . . . . ""@en . "37692002"^^ . . . . . . . . . . . . "7187"^^ . . . . . . . "15135"^^ . . . . . . "Psi2 Lupi (125 Lupi) \u00E9 uma estrela na dire\u00E7\u00E3o da constela\u00E7\u00E3o de Lupus. Possui uma ascens\u00E3o reta de 15h 42m 41.04s e uma declina\u00E7\u00E3o de \u221234\u00B0 42\u2032 37.2\u2033. Sua magnitude aparente \u00E9 igual a 4.75. Considerando sua dist\u00E2ncia de 396 anos-luz em rela\u00E7\u00E3o \u00E0 Terra, sua magnitude absoluta \u00E9 igual a \u22120.67. Pertence \u00E0 classe espectral B5V."@pt . . . . . . "1059264.0"^^ . "Psi2 Lupi"@en . . . . "Psi2 Lupi (\u03C82 Lupi, f\u00F6rkortad Psi2 Lup, \u03C82 Lup), som \u00E4r stj\u00E4rnans Bayer-beteckning, \u00E4r en trippelstj\u00E4rna i norra delen av stj\u00E4rnbilden Vargen. Den har en skenbar magnitud av 4,75 och \u00E4r synlig f\u00F6r blotta \u00F6gat d\u00E4r ljusf\u00F6roreningar ej f\u00F6rekommer. Baserat p\u00E5 parallaxm\u00E4tning inom Hipparcosuppdraget p\u00E5 ca 9,0 mas, ber\u00E4knas den befinna sig p\u00E5 ett avst\u00E5nd av ca 360 ljus\u00E5r (111 parsek) fr\u00E5n solen. P\u00E5 det ber\u00E4knade avst\u00E5ndet minskar dess skenbara magnitud med 0,016 \u00B1 0009 enheter p\u00E5 grund av interstell\u00E4rt stoft. Stj\u00E4rnan ing\u00E5r i undergruppen \u00D6vre Centaurus-Lupus inom Scorpius-Centaurus-f\u00F6reningen."@sv . . . . "\u041F\u0441\u0438\u00B2 \u0412\u043E\u043B\u043A\u0430 (\u043B\u0430\u0442. \u03C8\u00B2 Lupi), 4 \u0412\u043E\u043B\u043A\u0430 (\u043B\u0430\u0442. 4 Lupi), HD 140008 \u2014 \u0442\u0440\u043E\u0439\u043D\u0430\u044F \u0437\u0432\u0435\u0437\u0434\u0430 \u0432 \u0441\u043E\u0437\u0432\u0435\u0437\u0434\u0438\u0438 \u0412\u043E\u043B\u043A\u0430 \u043D\u0430 \u0440\u0430\u0441\u0441\u0442\u043E\u044F\u043D\u0438\u0438 \u043F\u0440\u0438\u0431\u043B\u0438\u0437\u0438\u0442\u0435\u043B\u044C\u043D\u043E 378 \u0441\u0432\u0435\u0442\u043E\u0432\u044B\u0445 \u043B\u0435\u0442 (\u043E\u043A\u043E\u043B\u043E 116 \u043F\u0430\u0440\u0441\u0435\u043A\u043E\u0432) \u043E\u0442 \u0421\u043E\u043B\u043D\u0446\u0430. \u0412\u0438\u0434\u0438\u043C\u0430\u044F \u0437\u0432\u0451\u0437\u0434\u043D\u0430\u044F \u0432\u0435\u043B\u0438\u0447\u0438\u043D\u0430 \u0437\u0432\u0435\u0437\u0434\u044B \u2014 +4,721m. \u0412\u043E\u0437\u0440\u0430\u0441\u0442 \u0437\u0432\u0435\u0437\u0434\u044B \u043E\u043F\u0440\u0435\u0434\u0435\u043B\u0451\u043D \u043A\u0430\u043A \u043E\u043A\u043E\u043B\u043E 15,9 \u043C\u043B\u043D \u043B\u0435\u0442."@ru . . "Psi2 Lupi (125 Lupi) \u00E9 uma estrela na dire\u00E7\u00E3o da constela\u00E7\u00E3o de Lupus. Possui uma ascens\u00E3o reta de 15h 42m 41.04s e uma declina\u00E7\u00E3o de \u221234\u00B0 42\u2032 37.2\u2033. Sua magnitude aparente \u00E9 igual a 4.75. Considerando sua dist\u00E2ncia de 396 anos-luz em rela\u00E7\u00E3o \u00E0 Terra, sua magnitude absoluta \u00E9 igual a \u22120.67. Pertence \u00E0 classe espectral B5V."@pt . . "Psi2 Lupi (\u03C82 Lupi, f\u00F6rkortad Psi2 Lup, \u03C82 Lup), som \u00E4r stj\u00E4rnans Bayer-beteckning, \u00E4r en trippelstj\u00E4rna i norra delen av stj\u00E4rnbilden Vargen. Den har en skenbar magnitud av 4,75 och \u00E4r synlig f\u00F6r blotta \u00F6gat d\u00E4r ljusf\u00F6roreningar ej f\u00F6rekommer. Baserat p\u00E5 parallaxm\u00E4tning inom Hipparcosuppdraget p\u00E5 ca 9,0 mas, ber\u00E4knas den befinna sig p\u00E5 ett avst\u00E5nd av ca 360 ljus\u00E5r (111 parsek) fr\u00E5n solen. P\u00E5 det ber\u00E4knade avst\u00E5ndet minskar dess skenbara magnitud med 0,016 \u00B1 0009 enheter p\u00E5 grund av interstell\u00E4rt stoft. Stj\u00E4rnan ing\u00E5r i undergruppen \u00D6vre Centaurus-Lupus inom Scorpius-Centaurus-f\u00F6reningen."@sv . . "0.19"^^ . . "Psi2 Lupi"@pt . . "\u22121.44"@en . . "\u22120.570"@en . . . . . . . "\u041F\u0441\u0438\u00B2 \u0412\u043E\u043B\u043A\u0430"@ru . "4.29"^^ . . . . . "\u22120.146"@en . "82.8"^^ . . . "Microvariable"@en . "\u221229.98"@en . . . "Psi2 Lupi"@sv . . . . . . . . . . . . . . . . . . "66.40000000000001"^^ . . "0.27"^^ . "8.970000000000001"^^ . . . . . . . "63.3"^^ . "Psi2 Lupi (\u03C82 Lup) is a triple star system in the constellation Lupus. It is visible to the naked eye with an apparent magnitude of 4.75. Based upon an annual parallax shift of 8.97 mas as seen from Earth, it is located around 360 light years from the Sun. At that distance, the visual magnitude is diminished by an extinction factor of 0.016\u00B10.009 due to interstellar dust. This system is a member of the Upper Centaurus\u2013Lupus subgroup of the Scorpius\u2013Centaurus association. The inner pair of stars in this system form a double-lined spectroscopic binary with an orbital period of 12.26 days and an eccentricity of 0.19. The two components are described as similar in appearance. They have the spectrum of a B-type main sequence star with a stellar classification of B5 V. The luminosity has a micro-variability with a frequency of 0.94483 cycles per day and an amplitude of 0.0067 in magnitude. The third component is a magnitude 10 star at an angular separation of 0.51 arc seconds."@en . "\u221221.37"@en . "1086505592"^^ . . "J2000.0"@en . . . .