. "Beta del Cavallet (\u03B2 Equulei) \u00E9s una de la constel\u00B7laci\u00F3 del Cavallet. Malgrat la seva denominaci\u00F3 de Bayer \u00ABBeta\u00BB, \u00E9s nom\u00E9s la quarta estrella m\u00E9s brillant en la constel\u00B7laci\u00F3 amb magnitud aparent +5,16; \u00E9s superada en lluentor per Kitalpha (\u03B1 Equulei), \u03B4 Equulei i . S'hi troba a 329 anys llum del sistema solar. Diverses estrelles t\u00E8nues -entre magnitud 11,6 i 13,6- es localitzen visualment a una separaci\u00F3 compresa entre 30 i 90 segons d'arc de Beta Equulei. Cap d'elles est\u00E0 f\u00EDsicament vinculada amb ella, sent nom\u00E9s companyes \u00F2ptiques."@ca . . . . . . . . . . . . "Beta Equulei, Latinized from \u03B2 Equulei, is the Bayer designation for a solitary star in the northern constellation of Equuleus. It is faintly visible to the naked eye with an apparent visual magnitude of 5.16. The annual parallax shift is 11.27 mas, indicating a separation of around 289 light years from the Sun. It is drifting closer with a radial velocity of \u221211 km/s. \u03B2 Equulei has four optical companions. They are not physically associated with the star described above."@en . . . . . . . . "Beta Equulei (\u03B2 Equ / 10 Equulei / HD 203562)\u200B es una estrella en la constelaci\u00F3n de Equuleus.Pese a su denominaci\u00F3n de Bayer \u00ABBeta\u00BB, es solo la cuarta estrella m\u00E1s brillante en la constelaci\u00F3n con magnitud aparente +5,16; es superada en brillo por Kitalpha (\u03B1 Equulei), \u03B4 Equulei y \u03B3 Equulei.Se encuentra a 329 a\u00F1os luz del Sistema Solar. Beta Equulei es una estrella blanca de la secuencia principal de tipo espectral A3V con una temperatura superficial aproximada de 9000 K.Su luminosidad es 75 veces mayor que la luminosidad solar y tiene una masa entre 2,4 y 2,5 masas solares.Con un radio 3,6 veces m\u00E1s grande que el del Sol, gira sobre s\u00ED misma con una velocidad de rotaci\u00F3n proyectada de 49 km/s, implicando un per\u00EDodo de rotaci\u00F3n inferior a 4 d\u00EDas.Con una edad en torno a los 600 millones de a\u00F1os, est\u00E1 pr\u00F3xima a finalizar su etapa como estrella de la secuencia principal.Al igual que Vega (\u03B1 Lyrae) o Fomalhaut (\u03B1 Piscis Austrini), Beta Equulei est\u00E1 rodeada por un disco circunestelar de polvo, que puede ser el indicio de un posible sistema planetario.\u200B Varias estrellas tenues \u2014entre magnitud 11,6 y 13,6\u2014 se localizan visualmente a una separaci\u00F3n comprendida entre 30 y 90 segundos de arco de Beta Equulei. Ninguna de ellas est\u00E1 f\u00EDsicamente vinculada con ella, siendo solo compa\u00F1eras \u00F3pticas.\u200B"@es . . . . . . . "Beta Equulei, (\u03B2 Equulei / \u03B2 Equ), est une \u00E9toile solitaire de la constellation bor\u00E9ale du Petit Cheval. Elle est faiblement visible \u00E0 l'oeil nu avec une magnitude apparente visuelle de 5,15. La parallaxe annuelle est de 24,55 mas, ce qui correspond \u00E0 une distance d'environ 133 ann\u00E9es-lumi\u00E8re du Soleil. \u03B2 Equulei poss\u00E8de quatre compagnons optiques. Ils ne sont pas physiquement associ\u00E9s avec l'\u00E9toile d\u00E9crite plus haut."@fr . . . . . . . . . . . . "78.3"^^ . . . "+0.10"@en . . . . "Beta del Cavallet (\u03B2 Equulei) \u00E9s una de la constel\u00B7laci\u00F3 del Cavallet. Malgrat la seva denominaci\u00F3 de Bayer \u00ABBeta\u00BB, \u00E9s nom\u00E9s la quarta estrella m\u00E9s brillant en la constel\u00B7laci\u00F3 amb magnitud aparent +5,16; \u00E9s superada en lluentor per Kitalpha (\u03B1 Equulei), \u03B4 Equulei i . S'hi troba a 329 anys llum del sistema solar. Beta del Cavallet \u00E9s un estel blanc de la seq\u00FC\u00E8ncia principal de tipus espectral A3V amb una temperatura superficial aproximada de 9000 K. La seva lluminositat \u00E9s 75 vegades major que la lluminositat solar i t\u00E9 una massa entre 2,4 i 2,5 masses solars. Amb un radi 3,6 vegades m\u00E9s gran que el del Sol, gira sobre si mateixa amb una velocitat de rotaci\u00F3 projectada de 49 km/s, implicant un per\u00EDode de rotaci\u00F3 inferior a 4 dies. Amb una edat al voltant dels 600 milions d'anys, est\u00E0 pr\u00F2xima a finalitzar la seva etapa com a estrella de la seq\u00FC\u00E8ncia principal. Igual que Vega (\u03B1 Lyrae) o Fomalhaut (\u03B1 Pisces Austrini), Beta Equulei est\u00E0 envoltada per un disc circumestel\u00B7lar de pols, que pot ser l'indici d'un possible sistema planetari. Diverses estrelles t\u00E8nues -entre magnitud 11,6 i 13,6- es localitzen visualment a una separaci\u00F3 compresa entre 30 i 90 segons d'arc de Beta Equulei. Cap d'elles est\u00E0 f\u00EDsicament vinculada amb ella, sent nom\u00E9s companyes \u00F2ptiques."@ca . "Beta Equulei (10 Equulei) \u00E9 uma estrela m\u00FAltipla na dire\u00E7\u00E3o da Equuleus. Possui uma ascens\u00E3o reta de 21h 22m 53.58s e uma declina\u00E7\u00E3o de +06\u00B0 48\u2032 40.0\u2033. Sua magnitude aparente \u00E9 igual a 5.16. Considerando sua dist\u00E2ncia de 360 anos-luz em rela\u00E7\u00E3o \u00E0 Terra, sua magnitude absoluta \u00E9 igual a \u22120.05. Pertence \u00E0 classe espectral A3V."@pt . . "Beta Equulei"@fr . "\u0411\u0435\u0442\u0430 \u041C\u0430\u043B\u043E\u0433\u043E \u041A\u043E\u043D\u044F (\u03B2 \u0411\u0435\u0442\u0430 \u041C\u0430\u043B\u043E\u0433\u043E \u041A\u043E\u043D\u044F, Beta Equulei, \u0441\u043E\u043A\u0440\u0430\u0449. Beta Equ, \u03B2 Equ) \u2014 \u0437\u0432\u0435\u0437\u0434\u0430 \u0432 \u0441\u0435\u0432\u0435\u0440\u043D\u043E\u043C \u0441\u043E\u0437\u0432\u0435\u0437\u0434\u0438\u0438 \u041C\u0430\u043B\u044B\u0439 \u041A\u043E\u043D\u044C. \u0417\u0432\u0435\u0437\u0434\u0430 \u0438\u043C\u0435\u0435\u0442 \u0432\u0438\u0434\u0438\u043C\u0443\u044E \u0437\u0432\u0451\u0437\u0434\u043D\u0443\u044E \u0432\u0435\u043B\u0438\u0447\u0438\u043D\u0443 5.15m, \u0438, \u0441\u043E\u0433\u043B\u0430\u0441\u043D\u043E \u0448\u043A\u0430\u043B\u0435 \u0411\u043E\u0440\u0442\u043B\u044F, \u0432\u0438\u0434\u043D\u0430 \u043D\u0435\u0432\u043E\u043E\u0440\u0443\u0436\u0435\u043D\u043D\u044B\u043C \u0433\u043B\u0430\u0437\u043E\u043C \u043A\u0430\u043A \u043C\u0438\u043D\u0438\u043C\u0443\u043C \u043D\u0430 \u0437\u0430\u0441\u0432\u0435\u0447\u0435\u043D\u043D\u043E\u043C \u043F\u0440\u0438\u0433\u043E\u0440\u043E\u0434\u043D\u043E\u043C \u043D\u0435\u0431\u0435 (\u0430\u043D\u0433\u043B. Bright suburban sky). \u0420\u0430\u0434\u0438\u0430\u043B\u044C\u043D\u0430\u044F \u0433\u0435\u043B\u0438\u043E\u0446\u0435\u043D\u0442\u0440\u0438\u0447\u0435\u0441\u043A\u0430\u044F \u0441\u043A\u043E\u0440\u043E\u0441\u0442\u044C \u0437\u0432\u0435\u0437\u0434\u044B \u0440\u0430\u0432\u043D\u0430 \u221211 \u043A\u043C/\u0441 \u0438 \u044D\u0442\u043E \u0437\u043D\u0430\u0447\u0438\u0442, \u0447\u0442\u043E \u0437\u0432\u0435\u0437\u0434\u0430 \u043F\u0440\u0438\u0431\u043B\u0438\u0436\u0430\u0435\u0442\u0441\u044F \u043A \u0421\u043E\u043B\u043D\u0446\u0443. \u0418\u0437 \u0438\u0437\u043C\u0435\u0440\u0435\u043D\u0438\u0439 \u043F\u0430\u0440\u0430\u043B\u043B\u0430\u043A\u0441\u0430, \u043F\u043E\u043B\u0443\u0447\u0435\u043D\u043D\u044B\u0445 \u0432\u043E \u0432\u0440\u0435\u043C\u044F \u043C\u0438\u0441\u0441\u0438\u0438 Hipparcos, \u0438\u0437\u0432\u0435\u0441\u0442\u043D\u043E, \u0447\u0442\u043E \u0437\u0432\u0435\u0437\u0434\u0430 \u0443\u0434\u0430\u043B\u0435\u043D\u0430 \u043F\u0440\u0438\u043C\u0435\u0440\u043D\u043E \u043D\u0430 133 \u00B1 4 \u0441\u0432. \u043B\u0435\u0442 (41 \u00B1 1 \u043F\u043A). \u0417\u0432\u0435\u0437\u0434\u0430 \u043D\u0430\u0431\u043B\u044E\u0434\u0430\u0435\u0442\u0441\u044F \u0441\u0435\u0432\u0435\u0440\u043D\u0435\u0435 84\u00B0 \u044E. \u0448., \u0442\u043E \u0435\u0441\u0442\u044C \u043F\u0440\u0430\u043A\u0442\u0438\u0447\u0435\u0441\u043A\u0438 \u043D\u0430 \u0432\u0441\u0435\u0439 \u0442\u0435\u0440\u0440\u0438\u0442\u043E\u0440\u0438\u0438 \u043E\u0431\u0438\u0442\u0430\u0435\u043C\u043E\u0439 \u0417\u0435\u043C\u043B\u0438, \u0437\u0430 \u0438\u0441\u043A\u043B\u044E\u0447\u0435\u043D\u0438\u0435\u043C \u0410\u043D\u0442\u0430\u0440\u043A\u0442\u0438\u0434\u044B. \u041B\u0443\u0447\u0448\u0435\u0435 \u0432\u0440\u0435\u043C\u044F \u043D\u0430\u0431\u043B\u044E\u0434\u0435\u043D\u0438\u044F \u2014 \u0430\u0432\u0433\u0443\u0441\u0442. \u0412 \u0442\u043E \u0432\u0440\u0435\u043C\u044F \u043A\u0430\u043A \u0411\u0435\u0442\u0430 \u0434\u043E\u043B\u0436\u043D\u0430 \u0431\u044B\u0442\u044C \u0432\u0442\u043E\u0440\u043E\u0439 \u043F\u043E \u044F\u0440\u043A\u043E\u0441\u0442\u0438 \u0437\u0432\u0435\u0437\u0434\u043E\u0439 \u0432 \u0441\u043E\u0437\u0432\u0435\u0437\u0434\u0438\u0438, \u043E\u043D\u0430 \u0442\u0430\u043A\u043E\u0432\u043E\u0439, \u043E\u0442\u043D\u044E\u0434\u044C, \u043D\u0435 \u044F\u0432\u043B\u044F\u0435\u0442\u0441\u044F. \u2014 \u0437\u0432\u0435\u0437\u0434\u0430 \u0447\u0435\u0442\u0432\u0451\u0440\u0442\u043E\u0439 \u0432\u0435\u043B\u0438\u0447\u0438\u043D\u044B, \u0434\u0435\u0439\u0441\u0442\u0432\u0438\u0442\u0435\u043B\u044C\u043D\u043E \u044F\u0432\u043B\u044F\u0435\u0442\u0441\u044F \u043F\u0435\u0440\u0432\u043E\u0439. \u041D\u043E\u043C\u0435\u0440 \u0434\u0432\u0430 \u2014 \u0414\u0435\u043B\u044C\u0442\u0430 \u041C\u0430\u043B\u043E\u0433\u043E \u041A\u043E\u043D\u044F, \u0437\u0430\u0442\u0435\u043C \u0441\u043B\u0435\u0434\u0443\u0435\u0442 \u0413\u0430\u043C\u043C\u0430 \u041C\u0430\u043B\u043E\u0433\u043E \u041A\u043E\u043D\u044F \u0438 \u0442\u043E\u043B\u044C\u043A\u043E \u043D\u0430 \u0447\u0435\u0442\u0432\u0451\u0440\u0442\u043E\u043C \u043C\u0435\u0441\u0442\u0435 \u0438\u0434\u0451\u0442 \u0411\u0435\u0442\u0430 \u2014 \u0437\u0432\u0435\u0437\u0434\u0430 \u043F\u044F\u0442\u043E\u0439 \u0432\u0435\u043B\u0438\u0447\u0438\u043D\u044B."@ru . . "Beta Equulei"@pt . . "600"^^ . "11.2696"^^ . "+10.136"@en . . "4.02"^^ . "+53.685"@en . . "9000"^^ . . . "Beta Equulei, (\u03B2 Equulei / \u03B2 Equ), est une \u00E9toile solitaire de la constellation bor\u00E9ale du Petit Cheval. Elle est faiblement visible \u00E0 l'oeil nu avec une magnitude apparente visuelle de 5,15. La parallaxe annuelle est de 24,55 mas, ce qui correspond \u00E0 une distance d'environ 133 ann\u00E9es-lumi\u00E8re du Soleil. C'est une \u00E9toile blanche de la s\u00E9quence principale de type spectral A3 V. Son rayon est \u00E9gal \u00E0 environ quatre fois celui du Soleil et sa temp\u00E9rature effective est d'environ 9000 K. Elle est \u00E2g\u00E9e d'environ 600 millions d'ann\u00E9es et elle tourne sur elle-m\u00EAme avec une vitesse de rotation projet\u00E9e de 58 km/s. L'\u00E9toile \u00E9met un exc\u00E8s d'infrarouge indiquant la pr\u00E9sence d'un disque de d\u00E9bris poussi\u00E9reux. La temp\u00E9rature moyenne de la poussi\u00E8re est de 85 K, indiquant que le demi-grand axe de son orbite vaut 104 ua. \u03B2 Equulei poss\u00E8de quatre compagnons optiques. Ils ne sont pas physiquement associ\u00E9s avec l'\u00E9toile d\u00E9crite plus haut."@fr . . . . . "Beta Equulei"@en . . "Beta Equulei, Latinized from \u03B2 Equulei, is the Bayer designation for a solitary star in the northern constellation of Equuleus. It is faintly visible to the naked eye with an apparent visual magnitude of 5.16. The annual parallax shift is 11.27 mas, indicating a separation of around 289 light years from the Sun. It is drifting closer with a radial velocity of \u221211 km/s. This is an ordinary A-type main sequence star with a stellar classification of A3 V. It has 2.7 times the mass of the Sun and about four times the Sun's radius. The star is around 600 million years old \u2013 93% of the way through its main sequence lifetime \u2013 and is spinning with a projected rotational velocity of 58 km/s. It is radiating 78 times the luminosity of the Sun from its photosphere at an effective temperature of about 9,000 K. The star emits an infrared excess indicating the presence of a dusty debris disk. The mean temperature of the dust is 85 K, indicating the semimajor axis of its orbit is 104 AU. \u03B2 Equulei has four optical companions. They are not physically associated with the star described above."@en . "Beta Equulei (10 Equulei) \u00E9 uma estrela m\u00FAltipla na dire\u00E7\u00E3o da Equuleus. Possui uma ascens\u00E3o reta de 21h 22m 53.58s e uma declina\u00E7\u00E3o de +06\u00B0 48\u2032 40.0\u2033. Sua magnitude aparente \u00E9 igual a 5.16. Considerando sua dist\u00E2ncia de 360 anos-luz em rela\u00E7\u00E3o \u00E0 Terra, sua magnitude absoluta \u00E9 igual a \u22120.05. Pertence \u00E0 classe espectral A3V."@pt . . . "19268325"^^ . . "Beta Equulei (\u03B2 Equ / 10 Equulei / HD 203562)\u200B es una estrella en la constelaci\u00F3n de Equuleus.Pese a su denominaci\u00F3n de Bayer \u00ABBeta\u00BB, es solo la cuarta estrella m\u00E1s brillante en la constelaci\u00F3n con magnitud aparente +5,16; es superada en brillo por Kitalpha (\u03B1 Equulei), \u03B4 Equulei y \u03B3 Equulei.Se encuentra a 329 a\u00F1os luz del Sistema Solar. Varias estrellas tenues \u2014entre magnitud 11,6 y 13,6\u2014 se localizan visualmente a una separaci\u00F3n comprendida entre 30 y 90 segundos de arco de Beta Equulei. Ninguna de ellas est\u00E1 f\u00EDsicamente vinculada con ella, siendo solo compa\u00F1eras \u00F3pticas.\u200B"@es . . . . "\u5C0F\u99AC\u5EA7\u03B2\uFF0C\u53C8\u540DBD+06 4811\uFF0CHD 203562\u3001SAO 126749\u3001HR 8178\uFF0C\u662F\u5C0F\u99AC\u5EA7\u7684\u4E00\u9897\u6052\u661F\uFF0C\u89C6\u661F\u7B49\u4E3A5.16\uFF0C\u4F4D\u4E8E\u9280\u7D9359\uFF0C\u9280\u7DEF-29.23\uFF0C\u5176B1900.0\u5750\u6807\u4E3A\u8D64\u7D9321h 17m 55.8s\uFF0C\u8D64\u7DEF+6\u00B0 -29.23\u2032 1\u2033\u3002"@zh . . . "7251"^^ . . "J2000.0"@en . "0.2608"^^ . . "Beta Equulei (\u03B2 Equulei, f\u00F6rkortat Beta Equ, \u03B2 Equ) som \u00E4r stj\u00E4rnans Bayerbeteckning, \u00E4r en ensam stj\u00E4rna bel\u00E4gen i den \u00F6stra delen av stj\u00E4rnbilden Lilla h\u00E4sten. Den har en skenbar magnitud p\u00E5 5,15 och \u00E4r svagt synlig f\u00F6r blotta \u00F6gat d\u00E4r ljusf\u00F6roreningar ej f\u00F6rekommer. Baserat p\u00E5 parallaxm\u00E4tning inom Hipparcosuppdraget p\u00E5 ca 24,6 mas, ber\u00E4knas den befinna sig p\u00E5 ett avst\u00E5nd p\u00E5 ca 133 ljus\u00E5r (ca 41 parsek) fr\u00E5n solen."@sv . . . "Beta Equulei (\u03B2 Equulei, f\u00F6rkortat Beta Equ, \u03B2 Equ) som \u00E4r stj\u00E4rnans Bayerbeteckning, \u00E4r en ensam stj\u00E4rna bel\u00E4gen i den \u00F6stra delen av stj\u00E4rnbilden Lilla h\u00E4sten. Den har en skenbar magnitud p\u00E5 5,15 och \u00E4r svagt synlig f\u00F6r blotta \u00F6gat d\u00E4r ljusf\u00F6roreningar ej f\u00F6rekommer. Baserat p\u00E5 parallaxm\u00E4tning inom Hipparcosuppdraget p\u00E5 ca 24,6 mas, ber\u00E4knas den befinna sig p\u00E5 ett avst\u00E5nd p\u00E5 ca 133 ljus\u00E5r (ca 41 parsek) fr\u00E5n solen."@sv . "\u5C0F\u99AC\u5EA7\u03B2\uFF0C\u53C8\u540DBD+06 4811\uFF0CHD 203562\u3001SAO 126749\u3001HR 8178\uFF0C\u662F\u5C0F\u99AC\u5EA7\u7684\u4E00\u9897\u6052\u661F\uFF0C\u89C6\u661F\u7B49\u4E3A5.16\uFF0C\u4F4D\u4E8E\u9280\u7D9359\uFF0C\u9280\u7DEF-29.23\uFF0C\u5176B1900.0\u5750\u6807\u4E3A\u8D64\u7D9321h 17m 55.8s\uFF0C\u8D64\u7DEF+6\u00B0 -29.23\u2032 1\u2033\u3002"@zh . "\u0411\u0435\u0442\u0430 \u041C\u0430\u043B\u043E\u0433\u043E \u041A\u043E\u043D\u044F"@ru . . . . . . . . . . . . "A3 V"@en . "\u0411\u0435\u0442\u0430 \u041C\u0430\u043B\u043E\u0433\u043E \u041A\u043E\u043D\u044F (\u03B2 \u0411\u0435\u0442\u0430 \u041C\u0430\u043B\u043E\u0433\u043E \u041A\u043E\u043D\u044F, Beta Equulei, \u0441\u043E\u043A\u0440\u0430\u0449. Beta Equ, \u03B2 Equ) \u2014 \u0437\u0432\u0435\u0437\u0434\u0430 \u0432 \u0441\u0435\u0432\u0435\u0440\u043D\u043E\u043C \u0441\u043E\u0437\u0432\u0435\u0437\u0434\u0438\u0438 \u041C\u0430\u043B\u044B\u0439 \u041A\u043E\u043D\u044C. \u0417\u0432\u0435\u0437\u0434\u0430 \u0438\u043C\u0435\u0435\u0442 \u0432\u0438\u0434\u0438\u043C\u0443\u044E \u0437\u0432\u0451\u0437\u0434\u043D\u0443\u044E \u0432\u0435\u043B\u0438\u0447\u0438\u043D\u0443 5.15m, \u0438, \u0441\u043E\u0433\u043B\u0430\u0441\u043D\u043E \u0448\u043A\u0430\u043B\u0435 \u0411\u043E\u0440\u0442\u043B\u044F, \u0432\u0438\u0434\u043D\u0430 \u043D\u0435\u0432\u043E\u043E\u0440\u0443\u0436\u0435\u043D\u043D\u044B\u043C \u0433\u043B\u0430\u0437\u043E\u043C \u043A\u0430\u043A \u043C\u0438\u043D\u0438\u043C\u0443\u043C \u043D\u0430 \u0437\u0430\u0441\u0432\u0435\u0447\u0435\u043D\u043D\u043E\u043C \u043F\u0440\u0438\u0433\u043E\u0440\u043E\u0434\u043D\u043E\u043C \u043D\u0435\u0431\u0435 (\u0430\u043D\u0433\u043B. Bright suburban sky). \u0420\u0430\u0434\u0438\u0430\u043B\u044C\u043D\u0430\u044F \u0433\u0435\u043B\u0438\u043E\u0446\u0435\u043D\u0442\u0440\u0438\u0447\u0435\u0441\u043A\u0430\u044F \u0441\u043A\u043E\u0440\u043E\u0441\u0442\u044C \u0437\u0432\u0435\u0437\u0434\u044B \u0440\u0430\u0432\u043D\u0430 \u221211 \u043A\u043C/\u0441 \u0438 \u044D\u0442\u043E \u0437\u043D\u0430\u0447\u0438\u0442, \u0447\u0442\u043E \u0437\u0432\u0435\u0437\u0434\u0430 \u043F\u0440\u0438\u0431\u043B\u0438\u0436\u0430\u0435\u0442\u0441\u044F \u043A \u0421\u043E\u043B\u043D\u0446\u0443."@ru . "\u53F8\u5371\u4E00"@zh . . . . . . "1124785318"^^ . . . "Beta Equulei"@sv . . . . . . . . . "5.16"^^ . . "Main sequence"@en . . "+0.13"@en . "Beta Equulei"@en . . "Beta Equulei"@es . "Beta del Cavallet"@ca . . . .