"Beta Serpentis (\u03B2 Ser / \u03B2 Serpentis) adalah bintang yang berada di rasi Serpens, berada di kepala \"sang ular\" (Serpens Caput). Komponen primernya, Beta Serpentis A, bintang katai putih tipe A (white A-type main sequence dwarf) dengan magnitudo +3.65. Komponen kedua, bintang bermagnitudo 9.9 B, terpisah pada jarak pada 31 arcsecond, dan bintang bermagnitudo 10.7 C, terpisah pada jarak 201 arcseconddari komponen utamanya. Beta Serpentis berada pada jarak 153 tahun cahaya dari Bumi."@id . "40"^^ . . . . . "Beta Serpentis"@es . . "153"^^ . . . "Beta Serpentis (\u03B2 Ser) ist die Bezeichnung f\u00FCr den f\u00FCnfthellsten Stern im Sternbild Schlange (lat: Serpens). In der klassischen chinesischen Astronomie tr\u00E4gt Beta Serpentis den Namen \u5468, dem Schriftzeichen, das f\u00FCr die Zhou-Dynastie steht. Beta Serpentis ist ein Mehrfachsternsystem, bestehend aus drei Sternen, die sich um einen gemeinsamen Schwerpunkt bewegen. Der Hauptstern besitzt eine scheinbare Helligkeit von 3,65m und geh\u00F6rt der Spektralklasse A3V an." . . "47"^^ . "+3.65"@fr . . . "Beta Serpentis (\u03B2 Ser / \u03B2 Serpentis / 28 Serpentis) \u00E8 un sistema stellare nella costellazione del Serpente. Si trova a 155 anni luce di distanza dal sistema solare e forma parte della corrente di stelle dell'associazione dell'Orsa Maggiore."@it . . . . "Beta Serpentis (Chow, 28 Serpentis) \u00E9 uma estrela na dire\u00E7\u00E3o da Serpens. Possui uma ascens\u00E3o reta de 15h 46m 11.21s e uma declina\u00E7\u00E3o de +15\u00B0 25\u2032 18.9\u2033. Sua magnitude aparente \u00E9 igual a 3.65. Considerando sua dist\u00E2ncia de 153 anos-luz em rela\u00E7\u00E3o \u00E0 Terra, sua magnitude absoluta \u00E9 igual a 0.29. Pertence \u00E0 classe espectral A3V."@pt . "Chow, 28 Serpentis, , , , , ,"@fr . . . "108073463"^^ . . "Beta Serpentis"@it . . . . . . . "Beta Serpentis" . "Coordonn\u00E9es : Sky map 15h 46m 11.3s, +15\u00B0 25\u2032 19\u2033Beta Serpentis (\u03B2 Ser, \u03B2 Serpentis) est une \u00E9toile multiple de la constellation du Serpent, dans sa t\u00EAte (Serpens Caput). Beta Serpentis est \u00E0 environ 150 ann\u00E9es-lumi\u00E8re de la Terre et est membre du courant d'\u00E9toiles de la Grande Ourse.La composante primaire, Beta Serpentis A, est une \u00E9toile blanche de la s\u00E9quence principale de type A avec une magnitude apparente de +3,65."@fr . . "\u3078\u3073\u5EA7\u30D9\u30FC\u30BF\u661F (\u03B2 Ser / \u03B2 Serpentis) \u306F\u3001\u3078\u3073\u5EA7\u306E\u982D\u90E8\u306B\u3042\u308B\u9023\u661F\u7CFB\u3067\u3042\u308B\u3002\u4E2D\u56FD\u306E\u5468\u738B\u671D\u306B\u7531\u6765\u3059\u308B\u30B7\u30E5\u30A6\uFF08Chow\uFF09\u3068\u3044\u3046\u56FA\u6709\u540D\u3092\u6301\u3064\u3002\u3078\u3073\u5EA7\u30D9\u30FC\u30BF\u661F\u306F\u5730\u7403\u304B\u3089\u7D04153\u5149\u5E74\u96E2\u308C\u3066\u304A\u308A\u3001\u304A\u304A\u3050\u307E\u5EA7\u904B\u52D5\u661F\u56E3\u306B\u5C5E\u3059\u308B\u3002\u4E3B\u661F\u3078\u3073\u5EA7\u30D9\u30FC\u30BF\u661FA\u306F\u767D\u8272\u306EA\u578B\u4E3B\u7CFB\u5217\u661F\u3067\u3001+3.65\u7B49\u7D1A\u3067\u3042\u308B\u3002\u3078\u3073\u5EA7\u30D9\u30FC\u30BF\u661FB\u306F+9.9\u7B49\u7D1A\u3067\u4E3B\u661F\u304B\u308931\u79D2\u96E2\u308C\u3066\u304A\u308A\u3001\u3078\u3073\u5EA7\u30D9\u30FC\u30BF\u661FC\u306F+10.7\u7B49\u7D1A\u3067201\u79D2\u96E2\u308C\u3066\u3044\u308B\u3002"@ja . . . . "Beta Serpentis (\u03B2 Ser, \u03B2 Serpentis) is a star system in the constellation Serpens, in its head (Serpens Caput)."@en . . "+15/25/19"@fr . "Coordonn\u00E9es : Sky map 15h 46m 11.3s, +15\u00B0 25\u2032 19\u2033Beta Serpentis (\u03B2 Ser, \u03B2 Serpentis) est une \u00E9toile multiple de la constellation du Serpent, dans sa t\u00EAte (Serpens Caput). Beta Serpentis est \u00E0 environ 150 ann\u00E9es-lumi\u00E8re de la Terre et est membre du courant d'\u00E9toiles de la Grande Ourse.La composante primaire, Beta Serpentis A, est une \u00E9toile blanche de la s\u00E9quence principale de type A avec une magnitude apparente de +3,65. Elle a deux compagnes, B de magnitude +9,9 \u00E0 31 arcsecondes, et C de magnitude +10,7 \u00E0 201 arcsecondes."@fr . . . . . . . "4764"^^ . . "Beta Serpentis"@id . "\u03B2 Serpentis"@fr . "7491064"^^ . "Beta Serpentis (\u03B2 Ser) ist die Bezeichnung f\u00FCr den f\u00FCnfthellsten Stern im Sternbild Schlange (lat: Serpens). In der klassischen chinesischen Astronomie tr\u00E4gt Beta Serpentis den Namen \u5468, dem Schriftzeichen, das f\u00FCr die Zhou-Dynastie steht. Beta Serpentis ist ein Mehrfachsternsystem, bestehend aus drei Sternen, die sich um einen gemeinsamen Schwerpunkt bewegen. Der Hauptstern besitzt eine scheinbare Helligkeit von 3,65m und geh\u00F6rt der Spektralklasse A3V an. Die Begleitsterne haben Helligkeiten von 9,9m und 10,7m und weisen Winkelabst\u00E4nde von 31\" bzw. 207\" auf. Das System Beta Serpentis ist 153 Lichtjahre von der Erde entfernt (Hipparcos Datenbank).Koordinaten (\u00C4quinoktium 2000)Rektaszension 15h 46m 11.3sDeklination\t+15\u00B0 25' 19\"" . "Beta Serpentis (Chow, 28 Serpentis) \u00E9 uma estrela na dire\u00E7\u00E3o da Serpens. Possui uma ascens\u00E3o reta de 15h 46m 11.21s e uma declina\u00E7\u00E3o de +15\u00B0 25\u2032 18.9\u2033. Sua magnitude aparente \u00E9 igual a 3.65. Considerando sua dist\u00E2ncia de 153 anos-luz em rela\u00E7\u00E3o \u00E0 Terra, sua magnitude absoluta \u00E9 igual a 0.29. Pertence \u00E0 classe espectral A3V."@pt . . . . . . "Beta Serpentis"@en . . . . . . "Beta Serpentis (\u03B2 Ser / \u03B2 Serpentis / 28 Serpentis) es un sistema estelar en la constelaci\u00F3n de Serpens.Recibe el nombre tradicional de Chow, del mandar\u00EDn \u5468, zh\u014Du, en referencia a la dinast\u00EDa Zhou.Se encuentra a 155 a\u00F1os luz del Sistema Solar y forma parte de la corriente de estrellas de la Asociaci\u00F3n estelar de la Osa Mayor.La estrella principal, Beta Serpentis A, es una subgigante blanca de tipo espectral A2IV de magnitud aparente de +3,65.Su temperatura superficial alcanza los 8549 K y su luminosidad es 61 veces superior a la luminosidad solar.Gira sobre s\u00ED misma a gran velocidad \u2014su velocidad de rotaci\u00F3n es de al menos 189 km/s\u2014, siendo su per\u00EDodo de rotaci\u00F3n inferior a 23 horas.Tiene una masa entre 2,4 y 2,5 masas solares.Acompa\u00F1a a la subgigante Beta Serpentis B, una enana naranja de tipo K3V y magnitud +9,9.Separada de ella al menos 1500 UA, emplea m\u00E1s de 31.000 a\u00F1os en completar una \u00F3rbita.Una tercera estrella de magnitud +10,7, Beta Serpentis C, tambi\u00E9n forma parte del sistema; es asimismo una enana naranja cuyo radio orbital alrededor del par AB es igual o mayor de 9500 UA, lo que implica un amplio per\u00EDodo superior a 500.000 a\u00F1os."@es . . "Beta Serpentis (\u03B2 Ser / \u03B2 Serpentis / 28 Serpentis) \u00E8 un sistema stellare nella costellazione del Serpente. Si trova a 155 anni luce di distanza dal sistema solare e forma parte della corrente di stelle dell'associazione dell'Orsa Maggiore."@it . "Beta Serpentis"@fr . . . "Beta Serpentis (\u03B2 Ser, \u03B2 Serpentis) is a star system in the constellation Serpens, in its head (Serpens Caput). It was a member of indigenous Arabic asterism al-Nasaq al-Sha'\u0101m\u012B, \"the Northern Line\" of al-Nasaq\u0101n \"the Two Lines\", along with \u03B2 Her (Kornephoros), \u03B3 Her (Hejian, Ho Keen) and \u03B3 Ser (Zheng, Ching).According to the catalogue of stars in the Technical Memorandum 33-507 - A Reduced Star Catalog Containing 537 Named Stars, al-Nasaq al-Sha'\u0101m\u012B or Nasak Shamiya were the title for three stars :\u03B2 Ser as Nasak Shamiya I, \u03B3 Ser as Nasak Shamiya II, \u03B3 Her as Nasak Shamiya III (exclude \u03B2 Her)In Chinese, \u5929\u5E02\u53F3\u57A3 (Ti\u0101n Sh\u00EC Y\u00F2u Yu\u00E1n), meaning Right Wall of Heavenly Market Enclosure, refers to an asterism which is represent eleven old states in China which is marking the right borderline of the enclosure, consisting of \u03B2 Serpentis, \u03B2 Herculis, \u03B3 Herculis, \u03BA Herculis, \u03B3 Serpentis, \u03B4 Serpentis, \u03B1 Serpentis, \u03B5 Serpentis, \u03B4 Ophiuchi, \u03B5 Ophiuchi and \u03B6 Ophiuchi. Consequently, \u03B2 Serpentis itself is known as \u5929\u5E02\u53F3\u57A3\u4E94 (Ti\u0101n Sh\u00EC Y\u00F2u Yu\u00E1n wu, English: the Fifth Star of Right Wall of Heavenly Market Enclosure), represent Zhou (\u912D) (possibly Chow, the dynasty in China), together with \u03B7 Capricorni and 21 Capricorni in Twelve States (asterism)."@en . . . "\u3078\u3073\u5EA7\u30D9\u30FC\u30BF\u661F (\u03B2 Ser / \u03B2 Serpentis) \u306F\u3001\u3078\u3073\u5EA7\u306E\u982D\u90E8\u306B\u3042\u308B\u9023\u661F\u7CFB\u3067\u3042\u308B\u3002\u4E2D\u56FD\u306E\u5468\u738B\u671D\u306B\u7531\u6765\u3059\u308B\u30B7\u30E5\u30A6\uFF08Chow\uFF09\u3068\u3044\u3046\u56FA\u6709\u540D\u3092\u6301\u3064\u3002\u3078\u3073\u5EA7\u30D9\u30FC\u30BF\u661F\u306F\u5730\u7403\u304B\u3089\u7D04153\u5149\u5E74\u96E2\u308C\u3066\u304A\u308A\u3001\u304A\u304A\u3050\u307E\u5EA7\u904B\u52D5\u661F\u56E3\u306B\u5C5E\u3059\u308B\u3002\u4E3B\u661F\u3078\u3073\u5EA7\u30D9\u30FC\u30BF\u661FA\u306F\u767D\u8272\u306EA\u578B\u4E3B\u7CFB\u5217\u661F\u3067\u3001+3.65\u7B49\u7D1A\u3067\u3042\u308B\u3002\u3078\u3073\u5EA7\u30D9\u30FC\u30BF\u661FB\u306F+9.9\u7B49\u7D1A\u3067\u4E3B\u661F\u304B\u308931\u79D2\u96E2\u308C\u3066\u304A\u308A\u3001\u3078\u3073\u5EA7\u30D9\u30FC\u30BF\u661FC\u306F+10.7\u7B49\u7D1A\u3067201\u79D2\u96E2\u308C\u3066\u3044\u308B\u3002"@ja . "A3V"@fr . . . . "Beta Serpentis (\u03B2 Ser / \u03B2 Serpentis) adalah bintang yang berada di rasi Serpens, berada di kepala \"sang ular\" (Serpens Caput). Komponen primernya, Beta Serpentis A, bintang katai putih tipe A (white A-type main sequence dwarf) dengan magnitudo +3.65. Komponen kedua, bintang bermagnitudo 9.9 B, terpisah pada jarak pada 31 arcsecond, dan bintang bermagnitudo 10.7 C, terpisah pada jarak 201 arcseconddari komponen utamanya. Beta Serpentis berada pada jarak 153 tahun cahaya dari Bumi."@id . . "15"^^ . "\u3078\u3073\u5EA7\u30D9\u30FC\u30BF\u661F"@ja . . . "Beta Serpentis (\u03B2 Ser / \u03B2 Serpentis / 28 Serpentis) es un sistema estelar en la constelaci\u00F3n de Serpens.Recibe el nombre tradicional de Chow, del mandar\u00EDn \u5468, zh\u014Du, en referencia a la dinast\u00EDa Zhou.Se encuentra a 155 a\u00F1os luz del Sistema Solar y forma parte de la corriente de estrellas de la Asociaci\u00F3n estelar de la Osa Mayor.La estrella principal, Beta Serpentis A, es una subgigante blanca de tipo espectral A2IV de magnitud aparente de +3,65.Su temperatura superficial alcanza los 8549 K y su luminosidad es 61 veces superior a la luminosidad solar.Gira sobre s\u00ED misma a gran velocidad \u2014su velocidad de rotaci\u00F3n es de al menos 189 km/s\u2014, siendo su per\u00EDodo de rotaci\u00F3n inferior a 23 horas.Tiene una masa entre 2,4 y 2,5 masas solares.Acompa\u00F1a a la subgigante Beta Serpentis B, una enana naranja de tipo K3V y magnitud +9,9.Separada de ella al menos 1500 UA, emplea m\u00E1s de 31.000 a\u00F1os en completar una \u00F3rbita.Una tercera estrella de magnitud +10,7, Beta Serpentis C, tambi\u00E9n forma parte del sistema; es asimismo una enana naranja cuyo radio orbital alrededor del par AB es igual o mayor de 9500 UA, lo que implica un amplio per\u00EDodo superior a 500.000 a\u00F1os."@es . "Beta Serpentis"@pt .