. "Beta Scuti, Latinized from \u03B2 Scuti, is a binary star system in the southern constellation Scutum. Based upon an annual parallax shift of 3.56 mas as seen from Earth, it is located approximately 920 light years from the Sun. The primary component has an apparent visual magnitude of +4.22 and is radiating about 1,270 times the luminosity of the Sun from its outer atmosphere at an effective temperature of 4,622 K. This yellow-hued star is a G-type bright giant with a stellar classification of G4 IIa. Beta Scuti was a latter designation of 6 Aquilae."@en . "+1.09"@en . "\u03B2 \u0429\u0438\u0442\u0430 (\u043B\u0430\u0442. \u03B2 Scuti / \u03B2 Sct) \u2212 \u0441\u043F\u0435\u043A\u0442\u0440\u0430\u043B\u044C\u043D\u043E-\u0434\u0432\u043E\u0439\u043D\u0430\u044F \u0437\u0432\u0435\u0437\u0434\u0430, \u043A\u043E\u0442\u043E\u0440\u0430\u044F \u043D\u0430\u0445\u043E\u0434\u0438\u0442\u0441\u044F \u0432 \u0441\u043E\u0437\u0432\u0435\u0437\u0434\u0438\u0438 \u0429\u0438\u0442\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 690 \u0441\u0432\u0435\u0442\u043E\u0432\u044B\u0445 \u043B\u0435\u0442 \u043E\u0442 \u043D\u0430\u0441. \u042D\u0442\u043E \u0432\u0442\u043E\u0440\u0430\u044F \u043F\u043E \u044F\u0440\u043A\u043E\u0441\u0442\u0438 \u0437\u0432\u0435\u0437\u0434\u0430 \u0432 \u0441\u043E\u0437\u0432\u0435\u0437\u0434\u0438\u0438. \u0413\u043B\u0430\u0432\u043D\u044B\u0439 \u043A\u043E\u043C\u043F\u043E\u043D\u0435\u043D\u0442, \u03B2 \u0429\u0438\u0442\u0430 \u0410, \u2014 \u0436\u0451\u043B\u0442\u044B\u0439 \u044F\u0440\u043A\u0438\u0439 \u0433\u0438\u0433\u0430\u043D\u0442 \u043A\u043B\u0430\u0441\u0441\u0430 G. \u0415\u0433\u043E \u043A\u043E\u043C\u043F\u0430\u043D\u044C\u043E\u043D, \u03B2 \u0429\u0438\u0442\u0430 \u0412, \u2014 \u0431\u0435\u043B\u043E-\u0433\u043E\u043B\u0443\u0431\u0430\u044F \u0437\u0432\u0435\u0437\u0434\u0430 4 \u0437\u0432\u0451\u0437\u0434\u043D\u043E\u0439 \u0432\u0435\u043B\u0438\u0447\u0438\u043D\u044B. \u041E\u0440\u0431\u0438\u0442\u0430\u043B\u044C\u043D\u044B\u0439 \u043F\u0435\u0440\u0438\u043E\u0434 \u0441\u0438\u0441\u0442\u0435\u043C\u044B \u0441\u043E\u0441\u0442\u0430\u0432\u043B\u044F\u0435\u0442 834 \u0434\u043D\u044F."@ru . . . . . . "Beta Scuti (\u03B2 Sct / HD 173764 / HR 7063) \u00E9s una estrella a la constel\u00B7laci\u00F3 de l'Escut, Scutum, originalment Scutum Sobiescii, l'escut de Sobieski. \u00C9s la segona m\u00E9s brillant de la mateixa, despr\u00E9s d'\u03B1 Scuti, i la seva magnitud aparent \u00E9s +4,22. Es troba a 916 \u00B1 80 anys llum del sistema solar, d'acord amb la nova reducci\u00F3 de les dades de paral\u00B7laxi del sat\u00E8l\u00B7lit Hipparcos. Beta Scuti \u00E9s una geganta lluminosa groga de tipus espectral G4IIa amb una temperatura superficial de 4.700 K. \u00C9s unes 3.100 vegades m\u00E9s lluminosa que el Sol i el seu radi \u00E9s 84 vegades major que el radi solar, equivalent a 0,39 ua. La seva edat s'estima en uns 55 milions d'anys, quan va iniciar la seva vida com un estel calent B3 de la seq\u00FC\u00E8ncia principal. Actualment, esgotat ja l'hidrogen, en el seu nucli t\u00E9 lloc la fusi\u00F3 d'heli en carboni i oxigen. Beta Scuti \u00E9s a m\u00E9s una estrella bin\u00E0ria espectrosc\u00F2pica amb un per\u00EDode orbital de 834 dies. L'acompanyant, de magnitud +8,5, \u00E9s una estrella blanca de la seq\u00FC\u00E8ncia principal de tipus A0V amb una lluminositat 40 vegades superior a la del Sol."@ca . "2.8"^^ . . . "Beta Scuti"@pl . . "Beta Scuti (\u03B2 Sct / HD 173764 / HR 7063)\u200B es una estrella en la constelaci\u00F3n de Scutum, originalmente Scutum Sobiescii, el escudo de Sobieski. Es la segunda m\u00E1s brillante de la misma, despu\u00E9s de \u03B1 Scuti, siendo su magnitud aparente +4,22.Se encuentra a 916 \u00B1 80 a\u00F1os luz del Sistema Solar, de acuerdo a la nueva reducci\u00F3n de los datos de paralaje del sat\u00E9lite Hipparcos.\u200B Beta Scuti es una gigante luminosa amarilla de tipo espectral G4IIa con una temperatura superficial de 4700 K.Es unas 3100 veces m\u00E1s luminosa que el Sol y su radio es 84 veces mayor que el radio solar, equivalente a 0,39 UA. Su edad se estima en unos 55 millones de a\u00F1os, cuando inici\u00F3 su vida como una estrella caliente B3 de la secuencia principal. Actualmente, agotado ya el hidr\u00F3geno, en su n\u00FAcleo tiene lugar la fusi\u00F3n de helio en carbono y ox\u00EDgeno.\u200B Beta Scuti es adem\u00E1s una estrella binaria espectrosc\u00F3pica con un per\u00EDodo orbital de 834 d\u00EDas. La acompa\u00F1ante, de magnitud +8,5, es una estrella blanca de la secuencia principal de tipo A0V con una luminosidad 40 veces superior a la del Sol.\u200B"@es . . . "Beta Scuti (\u03B2 Sct / \u03B2 Scuti) \u00E8 un sistema stellare binario nella costellazione dello Scudo. Dista approssimativamente 920 anni luce dalla Terra. La componente primaria, Beta Scuti \u00E8 una gigante luminosa gialla (classe spettrale G) con una magnitudine apparente di 4,22. La stella compagna, di magnitudine 8,5, appartiene alla classe spettrale B9,5. Il periodo orbitale della binaria \u00E8 di 834 giorni."@it . "\u03B2 Scuti"@en . . . "Beta Scuti"@pt . "\u03B2 \u0429\u0438\u0442\u0430 (\u043B\u0430\u0442. \u03B2 Scuti / \u03B2 Sct) \u2212 \u0441\u043F\u0435\u043A\u0442\u0440\u0430\u043B\u044C\u043D\u043E-\u0434\u0432\u043E\u0439\u043D\u0430\u044F \u0437\u0432\u0435\u0437\u0434\u0430, \u043A\u043E\u0442\u043E\u0440\u0430\u044F \u043D\u0430\u0445\u043E\u0434\u0438\u0442\u0441\u044F \u0432 \u0441\u043E\u0437\u0432\u0435\u0437\u0434\u0438\u0438 \u0429\u0438\u0442\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 690 \u0441\u0432\u0435\u0442\u043E\u0432\u044B\u0445 \u043B\u0435\u0442 \u043E\u0442 \u043D\u0430\u0441. \u042D\u0442\u043E \u0432\u0442\u043E\u0440\u0430\u044F \u043F\u043E \u044F\u0440\u043A\u043E\u0441\u0442\u0438 \u0437\u0432\u0435\u0437\u0434\u0430 \u0432 \u0441\u043E\u0437\u0432\u0435\u0437\u0434\u0438\u0438. \u0413\u043B\u0430\u0432\u043D\u044B\u0439 \u043A\u043E\u043C\u043F\u043E\u043D\u0435\u043D\u0442, \u03B2 \u0429\u0438\u0442\u0430 \u0410, \u2014 \u0436\u0451\u043B\u0442\u044B\u0439 \u044F\u0440\u043A\u0438\u0439 \u0433\u0438\u0433\u0430\u043D\u0442 \u043A\u043B\u0430\u0441\u0441\u0430 G. \u0415\u0433\u043E \u043A\u043E\u043C\u043F\u0430\u043D\u044C\u043E\u043D, \u03B2 \u0429\u0438\u0442\u0430 \u0412, \u2014 \u0431\u0435\u043B\u043E-\u0433\u043E\u043B\u0443\u0431\u0430\u044F \u0437\u0432\u0435\u0437\u0434\u0430 4 \u0437\u0432\u0451\u0437\u0434\u043D\u043E\u0439 \u0432\u0435\u043B\u0438\u0447\u0438\u043D\u044B. \u041E\u0440\u0431\u0438\u0442\u0430\u043B\u044C\u043D\u044B\u0439 \u043F\u0435\u0440\u0438\u043E\u0434 \u0441\u0438\u0441\u0442\u0435\u043C\u044B \u0441\u043E\u0441\u0442\u0430\u0432\u043B\u044F\u0435\u0442 834 \u0434\u043D\u044F."@ru . . "Beta Scuti A"@en . . . . "4.22"^^ . . "beta Scuti (\u03B2 Sct) \u2013 gwiazda podw\u00F3jna w gwiazdozbiorze Tarczy Sobieskiego. System ten jest oddalony o oko\u0142o 690 lat \u015Bwietlnych od Ziemi. G\u0142\u00F3wny sk\u0142adnik to pomara\u0144czowy jasny olbrzym typu widmowego G o jasno\u015Bci obserwowanej +4,22m. Jego towarzysz o jasno\u015Bci obserwowanej +8,5m to karze\u0142 o typie widmowym B9,5. Jest to uk\u0142ad spektroskopowo podw\u00F3jny o okresie obiegu oko\u0142o 834 dni."@pl . . . . . "Beta Scuti (24 Scuti) \u00E9 uma estrela na dire\u00E7\u00E3o da Scutum. Possui uma ascens\u00E3o reta de 18h 47m 10.48s e uma declina\u00E7\u00E3o de \u221204\u00B0 44\u2032 52.2\u2033. Sua magnitude aparente \u00E9 igual a 4.22. Considerando sua dist\u00E2ncia de 689 anos-luz em rela\u00E7\u00E3o \u00E0 Terra, sua magnitude absoluta \u00E9 igual a \u22122.41. Pertence \u00E0 classe espectral G5II...."@pt . "9562"^^ . "Beta Scuti"@es . "7.20576E7"^^ . "105.9"^^ . "Beta Scuti"@it . . . . . "Beta Scuti (\u03B2 Scuti, f\u00F6rkortad Beta Sct, \u03B2 Sct), som \u00E4r stj\u00E4rnans Bayer-beteckning, \u00E4r en dubbelstj\u00E4rna i nord\u00F6stra delen av stj\u00E4rnbilden Sk\u00F6lden. Den har en skenbar magnitud av 4,22 och \u00E4r synlig f\u00F6r blotta \u00F6gat d\u00E4r ljusf\u00F6roreningar ej f\u00F6rekommer. Baserat p\u00E5 parallaxm\u00E4tning inom Hipparcosuppdraget p\u00E5 ca 3,6 mas, ber\u00E4knas den befinna sig p\u00E5 ett avst\u00E5nd av ca 900 ljus\u00E5r (280 parsek) fr\u00E5n solen. Stj\u00E4rnan var ursprungligen en del av stj\u00E4rnbilden \u00D6rnen, d\u00E4r med beteckning 6 Aquilae."@sv . . . . . . . . . "7.8"^^ . . . "\u0411\u0435\u0442\u0430 \u0429\u0438\u0442\u0430"@ru . . . . . . . . . "Beta Scuti (\u03B2 Sct, \u03B2 Scuti) est une \u00E9toile binaire de la constellation de l'\u00C9cu de Sobieski. Elle est situ\u00E9e \u00E0 environ 690 ann\u00E9es-lumi\u00E8re de la Terre. L'\u00E9toile primaire est environ 1 270 fois plus lumineuse que le Soleil et sa temp\u00E9rature effective est de 4 622 K. C'est une g\u00E9ante lumineuse jaune de type spectral G0 et de magnitude apparente +4,22."@fr . . . . . "\u221221.30"@en . "0.43"^^ . . . . . . . "Beta Scuti (\u03B2 Scuti, f\u00F6rkortad Beta Sct, \u03B2 Sct), som \u00E4r stj\u00E4rnans Bayer-beteckning, \u00E4r en dubbelstj\u00E4rna i nord\u00F6stra delen av stj\u00E4rnbilden Sk\u00F6lden. Den har en skenbar magnitud av 4,22 och \u00E4r synlig f\u00F6r blotta \u00F6gat d\u00E4r ljusf\u00F6roreningar ej f\u00F6rekommer. Baserat p\u00E5 parallaxm\u00E4tning inom Hipparcosuppdraget p\u00E5 ca 3,6 mas, ber\u00E4knas den befinna sig p\u00E5 ett avst\u00E5nd av ca 900 ljus\u00E5r (280 parsek) fr\u00E5n solen. Stj\u00E4rnan var ursprungligen en del av stj\u00E4rnbilden \u00D6rnen, d\u00E4r med beteckning 6 Aquilae."@sv . . . . . "Beta Scuti"@en . . . . "Beta Scuti"@sv . "beta Scuti (\u03B2 Sct) \u2013 gwiazda podw\u00F3jna w gwiazdozbiorze Tarczy Sobieskiego. System ten jest oddalony o oko\u0142o 690 lat \u015Bwietlnych od Ziemi. G\u0142\u00F3wny sk\u0142adnik to pomara\u0144czowy jasny olbrzym typu widmowego G o jasno\u015Bci obserwowanej +4,22m. Jego towarzysz o jasno\u015Bci obserwowanej +8,5m to karze\u0142 o typie widmowym B9,5. Jest to uk\u0142ad spektroskopowo podw\u00F3jny o okresie obiegu oko\u0142o 834 dni."@pl . . "3.56"^^ . . "Beta Scuti (\u03B2 Sct, \u03B2 Scuti) est une \u00E9toile binaire de la constellation de l'\u00C9cu de Sobieski. Elle est situ\u00E9e \u00E0 environ 690 ann\u00E9es-lumi\u00E8re de la Terre. L'\u00E9toile primaire est environ 1 270 fois plus lumineuse que le Soleil et sa temp\u00E9rature effective est de 4 622 K. C'est une g\u00E9ante lumineuse jaune de type spectral G0 et de magnitude apparente +4,22."@fr . . "0.9399999999999999"^^ . . . . . . "Beta Scuti"@fr . . . "G4IIa"@en . . "Beta Scuti"@ca . "Beta Scuti (\u03B2 Sct / \u03B2 Scuti) \u00E8 un sistema stellare binario nella costellazione dello Scudo. Dista approssimativamente 920 anni luce dalla Terra. La componente primaria, Beta Scuti \u00E8 una gigante luminosa gialla (classe spettrale G) con una magnitudine apparente di 4,22. La stella compagna, di magnitudine 8,5, appartiene alla classe spettrale B9,5. Il periodo orbitale della binaria \u00E8 di 834 giorni."@it . . "4622"^^ . . . "288.1"^^ . . "J2000"@en . . . "Bet Scuti B"@en . "1079519964"^^ . . . . "\u305F\u3066\u5EA7\u30D9\u30FC\u30BF\u661F"@ja . . "\u22128.44"@en . . . "2422480.9"^^ . . "-0.16"^^ . "\u221216.37"@en . "\u305F\u3066\u5EA7\u03B2\u661F\uFF08\u305F\u3066\u3056\u30D9\u30FC\u30BF\u305B\u3044\u3001\u03B2 Scuti\u3001\u03B2 Sct\uFF09\u306F\u3001\u305F\u3066\u5EA7\u306B\u3042\u308B\u9023\u661F\u3067\u3042\u308B\u3002\u5E74\u5468\u8996\u5DEE\u306B\u57FA\u3065\u3044\u3066\u8A08\u7B97\u3057\u305F\u3001\u592A\u967D\u304B\u3089\u306E\u8DDD\u96E2\u306F\u3001\u304A\u3088\u305D690\u5149\u5E74\u3067\u3042\u308B\u3002\u898B\u304B\u3051\u306E\u7B49\u7D1A\u306F4.22\u3067\u3001\u8089\u773C\u3067\u307F\u308B\u3053\u3068\u304C\u3067\u304D\u308B\u3002"@ja . . . "Beta Scuti (24 Scuti) \u00E9 uma estrela na dire\u00E7\u00E3o da Scutum. Possui uma ascens\u00E3o reta de 18h 47m 10.48s e uma declina\u00E7\u00E3o de \u221204\u00B0 44\u2032 52.2\u2033. Sua magnitude aparente \u00E9 igual a 4.22. Considerando sua dist\u00E2ncia de 689 anos-luz em rela\u00E7\u00E3o \u00E0 Terra, sua magnitude absoluta \u00E9 igual a \u22122.41. Pertence \u00E0 classe espectral G5II...."@pt . "\u22122.99"@en . . . . . . "Beta Scuti (\u03B2 Sct / HD 173764 / HR 7063) \u00E9s una estrella a la constel\u00B7laci\u00F3 de l'Escut, Scutum, originalment Scutum Sobiescii, l'escut de Sobieski. \u00C9s la segona m\u00E9s brillant de la mateixa, despr\u00E9s d'\u03B1 Scuti, i la seva magnitud aparent \u00E9s +4,22. Es troba a 916 \u00B1 80 anys llum del sistema solar, d'acord amb la nova reducci\u00F3 de les dades de paral\u00B7laxi del sat\u00E8l\u00B7lit Hipparcos. Beta Scuti \u00E9s una geganta lluminosa groga de tipus espectral G4IIa amb una temperatura superficial de 4.700 K."@ca . . "0.35"^^ . . "1270"^^ . . "2673933"^^ . . . "Beta Scuti (\u03B2 Sct / HD 173764 / HR 7063)\u200B es una estrella en la constelaci\u00F3n de Scutum, originalmente Scutum Sobiescii, el escudo de Sobieski. Es la segunda m\u00E1s brillante de la misma, despu\u00E9s de \u03B1 Scuti, siendo su magnitud aparente +4,22.Se encuentra a 916 \u00B1 80 a\u00F1os luz del Sistema Solar, de acuerdo a la nueva reducci\u00F3n de los datos de paralaje del sat\u00E9lite Hipparcos.\u200B"@es . . . "+0.84"@en . . . "33.9"^^ . "Beta Scuti, Latinized from \u03B2 Scuti, is a binary star system in the southern constellation Scutum. Based upon an annual parallax shift of 3.56 mas as seen from Earth, it is located approximately 920 light years from the Sun. The primary component has an apparent visual magnitude of +4.22 and is radiating about 1,270 times the luminosity of the Sun from its outer atmosphere at an effective temperature of 4,622 K. This yellow-hued star is a G-type bright giant with a stellar classification of G4 IIa. This is a spectroscopic binary with an orbital period of 2.3 years and eccentricity around 0.35. The secondary is about 3.3 magnitudes dimmer than the primary and estimated as type B9 based on the flux of far-ultraviolet radiation. The secondary was directly detected with a magnitude difference of 3.6 at a separation of about 17 milli-arcseconds using observations from the Navy Precision Optical Interferometer. This detection was significant as observations with the Hubble Space Telescope which indicated a companion star was present were not definitive. With an orbit and a parallax the sum of the masses of the two stars can be determined via a dynamical parallax. This eventually can yield a precise mass for the evolved giant primary star. Beta Scuti was a latter designation of 6 Aquilae."@en . . . . . . . . . "\u305F\u3066\u5EA7\u03B2\u661F\uFF08\u305F\u3066\u3056\u30D9\u30FC\u30BF\u305B\u3044\u3001\u03B2 Scuti\u3001\u03B2 Sct\uFF09\u306F\u3001\u305F\u3066\u5EA7\u306B\u3042\u308B\u9023\u661F\u3067\u3042\u308B\u3002\u5E74\u5468\u8996\u5DEE\u306B\u57FA\u3065\u3044\u3066\u8A08\u7B97\u3057\u305F\u3001\u592A\u967D\u304B\u3089\u306E\u8DDD\u96E2\u306F\u3001\u304A\u3088\u305D690\u5149\u5E74\u3067\u3042\u308B\u3002\u898B\u304B\u3051\u306E\u7B49\u7D1A\u306F4.22\u3067\u3001\u8089\u773C\u3067\u307F\u308B\u3053\u3068\u304C\u3067\u304D\u308B\u3002"@ja . .