. . . . . . "Beta Hydrae, Latinized from \u03B2 Hydrae, is a double star in the equatorial constellation of Hydra. Historically, Beta Hydrae was designated 28 Crateris, but the latter fell out of use when the IAU defined the permanent constellation boundaries in 1930. The system is faintly visible to the naked eye with a combined apparent visual magnitude that ranges around 4.29. It is located at a distance of approximately 310 light years from the Sun based on parallax. The double nature of this system was first reported by English astronomer John Herschel in 1834. The brighter primary, designated component A, has an average visual magnitude of 4.67, while the secondary, component B, is of magnitude 5.47. As of 2002, the secondary is located at an angular separation of 0.65 arcseconds from the primary, along a position angle of 28.5\u00B0. The brighter component is an \u03B12 Canum Venaticorum variable that changes in brightness with a period of 2.344 days and an amplitude of 0.04 in visual magnitude. It is a magnetic chemically-peculiar star with an average quadratic field strength of (\u2212206\u00B168)\u00D710\u22124 T. The star is around 178 million years old with 3.4 times the mass of the Sun and 3.9 times the Sun's radius. On average, it is radiating 257 times the luminosity of the Sun from its photosphere at an effective temperature of 10,980 K. In 1972, M. R. Molnar found a stellar classification of B9IIIp Si for \u03B2 Hydrae A, showing an abundance anomaly for silicon. R. F. Garrison and R. O. Gray assigned it a class of kB8hB8HeA0VSi in 1994. This notation indicates the Calcium K line matches a star of class B8, the hydrogen lines also match a B8 spectrum, while the helium lines match an A-type main-sequence star of class A0V. They noted that the hydrogen lines have \"curious rounded profiles\". Later studies list abundance anomalies of silicon, chromium, and strontium."@en . . . . . "Beta Hydrae"@sv . . . . . . . . . . . . . "Beta Hydrae ( Hydrae) \u00E9 uma estrela na dire\u00E7\u00E3o da Hydra. Possui uma ascens\u00E3o reta de 11h 52m 54.56s e uma declina\u00E7\u00E3o de \u221233\u00B0 54\u2032 29.3\u2033. Sua magnitude aparente \u00E9 igual a 4.29. Considerando sua dist\u00E2ncia de 365 anos-luz em rela\u00E7\u00E3o \u00E0 Terra, sua magnitude absoluta \u00E9 igual a \u22120.96. Pertence \u00E0 classe espectral Ap Si. \u00C9 uma estrela vari\u00E1vel \u03B1\u00B2 Canum Venaticorum."@pt . "Beta Hydrae"@pt . . "Beta Hydrae"@en . . "1105422742"^^ . . "Beta Hydrae (Beta Hya, \u03B2 Hydrae, \u03B2 Hya) adalah bintang ganda yang ada di rasi bintang Hydra. Secara umum, magnitudonya bervariasi sebesar 0.04 magnitudo dengan periode 2.344 hari, dan pada saat paling terang magnitudoya sekitar 4.27. Bintang yang paling terang adalah bintang raksasa yang diklasifikasikan sebagai \u03B1\u00B2 Canum Venaticorum."@in . . . "Beta Hydrae"@cs . . . "HD103192 \u2014 \u043F\u043E\u0434\u0432\u0456\u0439\u043D\u0430 \u0437\u043E\u0440\u044F. \u0426\u044F \u043F\u043E\u0434\u0432\u0456\u0439\u043D\u0430 \u0441\u0438\u0441\u0442\u0435\u043C\u0430 \u043C\u0430\u0454 \u0432\u0438\u0434\u0438\u043C\u0443 \u0437\u043E\u0440\u044F\u043D\u0443 \u0432\u0435\u043B\u0438\u0447\u0438\u043D\u0443 \u0432 \u0441\u043C\u0443\u0437\u0456 V \u043F\u0440\u0438\u0431\u043B\u0438\u0437\u043D\u043E 4,7.\u0412\u043E\u043D\u0430 \u0440\u043E\u0437\u0442\u0430\u0448\u043E\u0432\u0430\u043D\u0430 \u043D\u0430 \u0432\u0456\u0434\u0441\u0442\u0430\u043D\u0456 \u0431\u043B\u0438\u0437\u044C\u043A\u043E 365,2 \u0441\u0432\u0456\u0442\u043B\u043E\u0432\u0438\u0445 \u0440\u043E\u043A\u0456\u0432 \u0432\u0456\u0434 \u0421\u043E\u043D\u0446\u044F."@uk . . "+0.19"@en . . . "Beta de l'Hidra Femella (\u03B2 Hydrae) \u00E9s un estel de magnitud aparent +4,29 a la constel\u00B7laci\u00F3 de l'Hidra Femella. Al costat de , a la Xina era coneguda com a Tsing Kew, \u2018el pujol verd'. S'hi troba a 365 anys llum de dist\u00E0ncia del sistema solar."@ca . "bet+hya+A"@en . . "4.29"^^ . "\u22120.59"@en . "B9IIIp Si + ?"@en . . . . . . "Beta Hydrae (\u03B2 Hydrae, f\u00F6rkortat Beta Hya, \u03B2 Hya) som \u00E4r stj\u00E4rnans Bayerbeteckning, \u00E4r en dubbelstj\u00E4rna bel\u00E4gen i den s\u00F6dra delen av stj\u00E4rnbilden Vattenormen. Den har en skenbar magnitud p\u00E5 4,67 och \u00E4r synlig f\u00F6r blotta \u00F6gat d\u00E4r ljusf\u00F6roreningar ej f\u00F6rekommer. Baserat p\u00E5 parallaxm\u00E4tning inom Hipparcosuppdraget p\u00E5 ca 8,9 mas, ber\u00E4knas den befinna sig p\u00E5 ett avst\u00E5nd p\u00E5 ca 370 ljus\u00E5r (ca 110 parsek) fr\u00E5n solen."@sv . . "\u0411\u0435\u0442\u0430 \u0413\u0438\u0434\u0440\u044B"@ru . . . "kB8hB8HeA0VSi"@en . . . "B"@en . "10.53"^^ . "Beta Hydrae"@fr . . "J2000.0"@en . . . . "Beta de l'Hidra Femella"@ca . "A"@en . . "\u221256.56"@en . "Beta de l'Hidra Femella (\u03B2 Hydrae) \u00E9s un estel de magnitud aparent +4,29 a la constel\u00B7laci\u00F3 de l'Hidra Femella. Al costat de , a la Xina era coneguda com a Tsing Kew, \u2018el pujol verd'. S'hi troba a 365 anys llum de dist\u00E0ncia del sistema solar. Beta Hydrae \u00E9s un estel binari les components del qual hi estan separades 1,7 segons d'arc. Beta Hydrae A, classificada com una gegant de tipus espectral B9IIIsp, t\u00E9 una temperatura efectiva de 11.100 K. 210 vegades m\u00E9s lluminosa que el Sol, el seu radi \u00E9s 4 vegades major que el radi solar. \u00C9s un estel peculiar de tipus Bp que exhibeix taques amb altes concentracions de silici, crom i estronci. Aix\u00F2 el converteix en un estel lleugerament variable -del tipus Variable Alpha\u00B2 Canum Venaticorum- amb un per\u00EDode equivalent al seu per\u00EDode de rotaci\u00F3 de 2,357 dies. Amb una massa de 3,3 masses solars, la seva edat s'estima en 200 milions d'anys. La component secund\u00E0ria del sistema, Beta Hydrae B, t\u00E9 magnitud 5,47. La meitat de lluminosa que la seva companya, probablement \u00E9s un estel de la seq\u00FC\u00E8ncia principal m\u00E9s calenta que Beta Hydrae A. L'\u00F2rbita del sistema no est\u00E0 determinada, per\u00F2 la seva separaci\u00F3 visual condueix a una dist\u00E0ncia real entre els dos estels d'almenys 190 unitats astron\u00F2miques, amb un per\u00EDode orbital de m\u00E9s de 1.000 anys."@ca . "19447362"^^ . "Beta Hydrae (\u03B2 Hya / HD 103192 / HR 4552) es una estrella de magnitud aparente +4,29 en la constelaci\u00F3n de Hidra.\u200B\u200B Junto a \u03BE Hydrae, en China era conocida como Tsing Kew, \u2018la colina verde\u2019.\u200BSe encuentra a 365 a\u00F1os luz de distancia del sistema solar."@es . . . . . . . . . . . . . . . "Beta Hydrae ( Hydrae) \u00E9 uma estrela na dire\u00E7\u00E3o da Hydra. Possui uma ascens\u00E3o reta de 11h 52m 54.56s e uma declina\u00E7\u00E3o de \u221233\u00B0 54\u2032 29.3\u2033. Sua magnitude aparente \u00E9 igual a 4.29. Considerando sua dist\u00E2ncia de 365 anos-luz em rela\u00E7\u00E3o \u00E0 Terra, sua magnitude absoluta \u00E9 igual a \u22120.96. Pertence \u00E0 classe espectral Ap Si. \u00C9 uma estrela vari\u00E1vel \u03B1\u00B2 Canum Venaticorum."@pt . . . "\u22120.08"@en . . . . . . . "Beta Hydrae (\u03B2 Hydrae / \u03B2 Hya) est une \u00E9toile binaire de la constellation de l'Hydre. Sa magnitude apparente combin\u00E9e varie de 0,04 magnitudes sur une p\u00E9riode de 2,344 jours, et vaut environ 4,27 \u00E0 sa luminosit\u00E9 maximale. L'\u00E9toile la plus brillante des deux est une \u00E9toile g\u00E9ante Bp qui a \u00E9t\u00E9 class\u00E9e comme variable de type \u03B12 Canum Venaticorum. Beta Hydrae porte la d\u00E9signation de Flamsteed de 28 Crateris. John Flamsteed, dans son catalogue d'\u00E9toiles, incluait parmi les constellations l'Hydre (Hydra) ainsi que \u00AB l'Hydre et la Coupe \u00BB (Hydra & Crater). Cette derni\u00E8re incluait indiff\u00E9remment les \u00E9toiles de la Coupe \u00E0 proprement parler et les \u00E9toiles de l'Hydre qui sont situ\u00E9es en dessous d'elle, Beta Hydrae \u00E9tant l'une d'entre-elles."@fr . "\u03B2 Hydrae"@en . "\u3046\u307F\u3078\u3073\u5EA7\u03B2\u661F\uFF08\u3046\u307F\u3078\u3073\u3056\u30D9\u30FC\u30BF\u305B\u3044\u3001\u03B2 Hydrae\u3001\u03B2 Hya\uFF09\u306F\u3001\u3046\u307F\u3078\u3073\u5EA7\u306E\u65B9\u89D2\u306B\u3001\u592A\u967D\u304B\u3089\u304A\u3088\u305D310\u5149\u5E74\u306E\u8DDD\u96E2\u306B\u3042\u308B\u3001\u4E8C\u91CD\u661F\u3067\u3042\u308B\u3002"@ja . "\uBC14\uB2E4\uBC40\uC790\uB9AC \uBCA0\uD0C0"@ko . . "Beta Hydrae (\u03B2 Hydrae, Beta Hya, \u03B2 Hya) je dvojhv\u011Bzda v souhv\u011Bzd\u00ED Hydry. Je od Zem\u011B vzd\u00E1len\u00E1 370 \u00B1 40 sv\u011Bteln\u00FDch let. Jej\u00ED zd\u00E1nliv\u00E1 hv\u011Bzdn\u00E1 velikost se m\u011Bn\u00ED o 0,04 mag v period\u011B 2,344 dn\u00ED, p\u0159i\u010Dem\u017E dosahuje maxim\u00E1ln\u00ED hodnoty 4,27 mag. Jde o prom\u011Bnnou hv\u011Bzdu typu Alfa\u00B2 Canum Venaticorum. D\u0159\u00EDve byla za\u0159azena do souhv\u011Bzd\u00ED Poh\u00E1ru a ozna\u010Dov\u00E1na 28 Crateris"@cs . "\u9752\u4E18\u4E00\uFF08\u9577\u86C7\u5EA7\u03B2\uFF09\uFF0C\u53C8\u540DCD-33 8018\uFF0CHD 103192\u3001SAO 202901\u3001HR 4552\uFF0C\u662F\u9577\u86C7\u5EA7\u7684\u4E00\u9897\u6052\u661F\uFF0C\u89C6\u661F\u7B49\u4E3A4.28\uFF0C\u4F4D\u4E8E\u9280\u7D93289.27\uFF0C\u9280\u7DEF27.41\uFF0C\u5176B1900.0\u5750\u6807\u4E3A\u8D64\u7D9311h 47m 51.3s\uFF0C\u8D64\u7DEF-33\u00B0 27.41\u2032 6\u2033\u3002"@zh . . "HD103192"@uk . . . . . . "Beta Hydrae (\u03B2 Hydrae / \u03B2 Hya) est une \u00E9toile binaire de la constellation de l'Hydre. Sa magnitude apparente combin\u00E9e varie de 0,04 magnitudes sur une p\u00E9riode de 2,344 jours, et vaut environ 4,27 \u00E0 sa luminosit\u00E9 maximale. L'\u00E9toile la plus brillante des deux est une \u00E9toile g\u00E9ante Bp qui a \u00E9t\u00E9 class\u00E9e comme variable de type \u03B12 Canum Venaticorum."@fr . . . . . . . "~3"@en . . . "Beta Hydrae (\u03B2 Hydrae, Beta Hya, \u03B2 Hya) je dvojhv\u011Bzda v souhv\u011Bzd\u00ED Hydry. Je od Zem\u011B vzd\u00E1len\u00E1 370 \u00B1 40 sv\u011Bteln\u00FDch let. Jej\u00ED zd\u00E1nliv\u00E1 hv\u011Bzdn\u00E1 velikost se m\u011Bn\u00ED o 0,04 mag v period\u011B 2,344 dn\u00ED, p\u0159i\u010Dem\u017E dosahuje maxim\u00E1ln\u00ED hodnoty 4,27 mag. Jde o prom\u011Bnnou hv\u011Bzdu typu Alfa\u00B2 Canum Venaticorum. D\u0159\u00EDve byla za\u0159azena do souhv\u011Bzd\u00ED Poh\u00E1ru a ozna\u010Dov\u00E1na 28 Crateris"@cs . . "\u3046\u307F\u3078\u3073\u5EA7\u30D9\u30FC\u30BF\u661F"@ja . "\u3046\u307F\u3078\u3073\u5EA7\u03B2\u661F\uFF08\u3046\u307F\u3078\u3073\u3056\u30D9\u30FC\u30BF\u305B\u3044\u3001\u03B2 Hydrae\u3001\u03B2 Hya\uFF09\u306F\u3001\u3046\u307F\u3078\u3073\u5EA7\u306E\u65B9\u89D2\u306B\u3001\u592A\u967D\u304B\u3089\u304A\u3088\u305D310\u5149\u5E74\u306E\u8DDD\u96E2\u306B\u3042\u308B\u3001\u4E8C\u91CD\u661F\u3067\u3042\u308B\u3002"@ja . "\u9752\u4E18\u4E00"@zh . . . . . "Beta Hydrae (\u03B2 Hya / HD 103192 / HR 4552) es una estrella de magnitud aparente +4,29 en la constelaci\u00F3n de Hidra.\u200B\u200B Junto a \u03BE Hydrae, en China era conocida como Tsing Kew, \u2018la colina verde\u2019.\u200BSe encuentra a 365 a\u00F1os luz de distancia del sistema solar. Beta Hydrae es una estrella binaria cuyas componentes est\u00E1n separadas 1,7 segundos de arco. Beta Hydrae A, clasificada como una gigante de tipo espectral B9IIIsp, tiene una temperatura efectiva de 11 100 K. 210 veces m\u00E1s luminosa que el Sol, su radio es 4 veces mayor que el radio solar. Es una estrella peculiar de tipo Bp que exhibe manchas con altas concentraciones de silicio, cromo y estroncio. Esto la convierte en una estrella ligeramente variable \u2014del tipo Alfa2 Canum Venaticorum\u2014 con un per\u00EDodo equivalente a su periodo de rotaci\u00F3n de 2,357 d\u00EDas. Con una masa de 3,3 masas solares, su edad se estima en 200 millones de a\u00F1os.\u200B La componente secundaria del sistema, Beta Hydrae B, tiene magnitud 5,47. La mitad de luminosa que su compa\u00F1era, probablemente es una estrella de la secuencia principal m\u00E1s caliente que Beta Hydrae A. La \u00F3rbita del sistema no est\u00E1 determinada, pero su separaci\u00F3n visual conduce a una distancia real entre las dos estrellas de al menos 190 UA, con un per\u00EDodo orbital de m\u00E1s de 1000 a\u00F1os.\u200B"@es . . . "Beta Hydrae (\u03B2 Hydrae, f\u00F6rkortat Beta Hya, \u03B2 Hya) som \u00E4r stj\u00E4rnans Bayerbeteckning, \u00E4r en dubbelstj\u00E4rna bel\u00E4gen i den s\u00F6dra delen av stj\u00E4rnbilden Vattenormen. Den har en skenbar magnitud p\u00E5 4,67 och \u00E4r synlig f\u00F6r blotta \u00F6gat d\u00E4r ljusf\u00F6roreningar ej f\u00F6rekommer. Baserat p\u00E5 parallaxm\u00E4tning inom Hipparcosuppdraget p\u00E5 ca 8,9 mas, ber\u00E4knas den befinna sig p\u00E5 ett avst\u00E5nd p\u00E5 ca 370 ljus\u00E5r (ca 110 parsek) fr\u00E5n solen."@sv . . "\u9752\u4E18\u4E00\uFF08\u9577\u86C7\u5EA7\u03B2\uFF09\uFF0C\u53C8\u540DCD-33 8018\uFF0CHD 103192\u3001SAO 202901\u3001HR 4552\uFF0C\u662F\u9577\u86C7\u5EA7\u7684\u4E00\u9897\u6052\u661F\uFF0C\u89C6\u661F\u7B49\u4E3A4.28\uFF0C\u4F4D\u4E8E\u9280\u7D93289.27\uFF0C\u9280\u7DEF27.41\uFF0C\u5176B1900.0\u5750\u6807\u4E3A\u8D64\u7D9311h 47m 51.3s\uFF0C\u8D64\u7DEF-33\u00B0 27.41\u2032 6\u2033\u3002"@zh . . "13369"^^ . . . . "bet+hya"@en . . "HD103192 \u2014 \u043F\u043E\u0434\u0432\u0456\u0439\u043D\u0430 \u0437\u043E\u0440\u044F. \u0426\u044F \u043F\u043E\u0434\u0432\u0456\u0439\u043D\u0430 \u0441\u0438\u0441\u0442\u0435\u043C\u0430 \u043C\u0430\u0454 \u0432\u0438\u0434\u0438\u043C\u0443 \u0437\u043E\u0440\u044F\u043D\u0443 \u0432\u0435\u043B\u0438\u0447\u0438\u043D\u0443 \u0432 \u0441\u043C\u0443\u0437\u0456 V \u043F\u0440\u0438\u0431\u043B\u0438\u0437\u043D\u043E 4,7.\u0412\u043E\u043D\u0430 \u0440\u043E\u0437\u0442\u0430\u0448\u043E\u0432\u0430\u043D\u0430 \u043D\u0430 \u0432\u0456\u0434\u0441\u0442\u0430\u043D\u0456 \u0431\u043B\u0438\u0437\u044C\u043A\u043E 365,2 \u0441\u0432\u0456\u0442\u043B\u043E\u0432\u0438\u0445 \u0440\u043E\u043A\u0456\u0432 \u0432\u0456\u0434 \u0421\u043E\u043D\u0446\u044F."@uk . . . "0.6"^^ . "Beta Hydrae, Latinized from \u03B2 Hydrae, is a double star in the equatorial constellation of Hydra. Historically, Beta Hydrae was designated 28 Crateris, but the latter fell out of use when the IAU defined the permanent constellation boundaries in 1930. The system is faintly visible to the naked eye with a combined apparent visual magnitude that ranges around 4.29. It is located at a distance of approximately 310 light years from the Sun based on parallax."@en . "bet+hya+B"@en . . . "\u0411\u0435\u0442\u0430 \u0413\u0438\u0434\u0440\u044B (\u03B2 \u0413\u0438\u0434\u0440\u044B, Beta Hydrae, \u03B2 Hydrae, \u0441\u043E\u043A\u0440\u0430\u0449. Beta Hya, \u03B2 Hya) \u2014 \u0437\u0432\u0435\u0437\u0434\u0430 \u0432 \u044E\u0436\u043D\u043E\u043C \u0441\u043E\u0437\u0432\u0435\u0437\u0434\u0438\u0438 \u0413\u0438\u0434\u0440\u0430. \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 +4.276m, \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\u0451\u043D\u043D\u044B\u043C \u0433\u043B\u0430\u0437\u043E\u043C \u0434\u0430\u0436\u0435 \u043D\u0430 \u0433\u043E\u0440\u043E\u0434\u0441\u043A\u043E\u043C \u043D\u0435\u0431\u0435 (\u0430\u043D\u0433\u043B. City sky). \u0418\u0437 \u0438\u0437\u043C\u0435\u0440\u0435\u043D\u0438\u0439 \u0442\u0440\u0438\u0433\u043E\u043D\u043E\u043C\u0435\u0442\u0440\u0438\u0447\u0435\u0441\u043A\u043E\u0433\u043E \u043F\u0430\u0440\u0430\u043B\u043B\u0430\u043A\u0441\u0430 \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 370 \u00B1 40 \u0441\u0432. \u043B\u0435\u0442 (110 \u00B1 10 \u043F\u043A) \u043E\u0442 \u0417\u0435\u043C\u043B\u0438. \u0417\u0432\u0435\u0437\u0434\u0430 \u043D\u0430\u0431\u043B\u044E\u0434\u0430\u0435\u0442\u0441\u044F \u044E\u0436\u043D\u0435\u0435 57\u00B0 \u0441.\u0448., \u0442.\u0435. \u044E\u0436\u043D\u0435\u0435 \u0421\u0430\u043D\u043A\u0442-\u041F\u0435\u0442\u0435\u0440\u0431\u0443\u0440\u0433\u0430 (59\u00B0 \u0441.\u0448.), \u044E\u0436\u043D\u0435\u0435 \u041A\u043E\u043F\u0435\u043D\u0433\u0430\u0433\u0435\u043D\u0430 (55\u00B0 \u0441.\u0448.) \u0438 \u044E\u0436\u043D\u0435\u0435 \u042D\u0434\u043C\u043E\u043D\u0442\u043E\u043D\u0430. \u041B\u0443\u0447\u0448\u0435\u0435 \u0432\u0440\u0435\u043C\u044F \u043D\u0430\u0431\u043B\u044E\u0434\u0435\u043D\u0438\u044F \u2014 \u043C\u0430\u0440\u0442."@ru . "\u0411\u0435\u0442\u0430 \u0413\u0438\u0434\u0440\u044B (\u03B2 \u0413\u0438\u0434\u0440\u044B, Beta Hydrae, \u03B2 Hydrae, \u0441\u043E\u043A\u0440\u0430\u0449. Beta Hya, \u03B2 Hya) \u2014 \u0437\u0432\u0435\u0437\u0434\u0430 \u0432 \u044E\u0436\u043D\u043E\u043C \u0441\u043E\u0437\u0432\u0435\u0437\u0434\u0438\u0438 \u0413\u0438\u0434\u0440\u0430. \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 +4.276m, \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\u0451\u043D\u043D\u044B\u043C \u0433\u043B\u0430\u0437\u043E\u043C \u0434\u0430\u0436\u0435 \u043D\u0430 \u0433\u043E\u0440\u043E\u0434\u0441\u043A\u043E\u043C \u043D\u0435\u0431\u0435 (\u0430\u043D\u0433\u043B. City sky). \u0418\u0437 \u0438\u0437\u043C\u0435\u0440\u0435\u043D\u0438\u0439 \u0442\u0440\u0438\u0433\u043E\u043D\u043E\u043C\u0435\u0442\u0440\u0438\u0447\u0435\u0441\u043A\u043E\u0433\u043E \u043F\u0430\u0440\u0430\u043B\u043B\u0430\u043A\u0441\u0430 \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 370 \u00B1 40 \u0441\u0432. \u043B\u0435\u0442 (110 \u00B1 10 \u043F\u043A) \u043E\u0442 \u0417\u0435\u043C\u043B\u0438. \u0417\u0432\u0435\u0437\u0434\u0430 \u043D\u0430\u0431\u043B\u044E\u0434\u0430\u0435\u0442\u0441\u044F \u044E\u0436\u043D\u0435\u0435 57\u00B0 \u0441.\u0448., \u0442.\u0435. \u044E\u0436\u043D\u0435\u0435 \u0421\u0430\u043D\u043A\u0442-\u041F\u0435\u0442\u0435\u0440\u0431\u0443\u0440\u0433\u0430 (59\u00B0 \u0441.\u0448.), \u044E\u0436\u043D\u0435\u0435 \u041A\u043E\u043F\u0435\u043D\u0433\u0430\u0433\u0435\u043D\u0430 (55\u00B0 \u0441.\u0448.) \u0438 \u044E\u0436\u043D\u0435\u0435 \u042D\u0434\u043C\u043E\u043D\u0442\u043E\u043D\u0430. \u041B\u0443\u0447\u0448\u0435\u0435 \u0432\u0440\u0435\u043C\u044F \u043D\u0430\u0431\u043B\u044E\u0434\u0435\u043D\u0438\u044F \u2014 \u043C\u0430\u0440\u0442."@ru . . ""@en . . . . "\uBC14\uB2E4\uBC40\uC790\uB9AC \uBCA0\uD0C0\uB294 \uBC14\uB2E4\uBC40\uC790\uB9AC\uC758 \uCD5C\uB0A8\uB2E8\uC5D0 \uC704\uCE58\uD558\uACE0 \uC788\uB294 \uD56D\uC131\uC774\uB2E4. \uBCA0\uD0C0\uB294 \uC9C0\uAD6C\uC5D0\uC11C \uC57D 365\uAD11\uB144 \uB5A8\uC5B4\uC838 \uC788\uB2E4. \uBC14\uB2E4\uBC40\uC790\uB9AC \uBCA0\uD0C0\uB294 \uC30D\uC131\uC73C\uB85C, \uAD6C\uC131\uC6D0 \uBC14\uB2E4\uBC40\uC790\uB9AC A\uC640 B\uB294 \uCC9C\uAD6C\uC5D0\uC11C \uCD5C\uB300 1.7\uCD08\uAC01\uAE4C\uC9C0 \uC11C\uB85C \uB5A8\uC5B4\uC9C0\uB294\uB370, \uC5EC\uAE30\uC11C \uACC4\uC0B0\uD55C \uB450 \uBCC4 \uC0AC\uC774\uC758 \uCD5C\uB300 \uC774\uACA9 \uAC70\uB9AC\uB294 190 \uC218\uC900\uC774\uBA70 \uACF5\uC804 \uC8FC\uAE30\uB294 \uC57D 1\uCC9C \uB144\uC5D0 \uB2EC\uD560 \uAC83\uC73C\uB85C \uC608\uC0C1\uB41C\uB2E4. \uADF8\uB7EC\uB098 \uC774 \uC608\uC0C1\uAC12\uC740 \uD655\uC2E4\uD55C \uAC83\uC740 \uC544\uB2C8\uB2E4. \uC8FC\uC131 A\uB294 \uAC89\uBCF4\uAE30 \uB4F1\uAE09 4.67\uC5D0 \uBD84\uAD11\uD615\uC740 B9\uC758 \uB728\uAC70\uC6B4 \uCCAD\uBC31\uC0C9 \uBCC4\uC774\uBA70 \uBC18\uC131 B\uB294 \uC0C1\uB300\uC801\uC73C\uB85C \uC5B4\uB450\uC6B4 \uAC89\uBCF4\uAE30 \uB4F1\uAE09 5.47\uC774\uBA70 \uBD84\uAD11\uD615\uC740 \uC815\uD655\uD788 \uC54C\uB824\uC838 \uC788\uC9C0 \uC54A\uB2E4. \uBCA0\uD0C0 \uD56D\uC131\uACC4\uC758 \uB098\uC774\uB294 \uACE0\uC791 2\uC5B5 2\uCC9C\uB9CC \uB144\uC5D0 \uBD88\uACFC\uD558\uB2E4. \uD2B9\uAE30\uD560 \uC810\uC740 \uBC14\uB2E4\uBC40\uC790\uB9AC \uBCA0\uD0C0\uC758 \uBD84\uAD11\uD615\uC5D0\uB294 peculiar\uAC00 \uBD99\uC5B4 \uC788\uB294\uB370 \uC774\uB294 \uD56D\uC131\uC758 \uB300\uAE30\uC5D0 \uADDC\uC18C, \uD06C\uB85C\uBBB4, \uC2A4\uD2B8\uB860\uD2AC\uC774 \uD48D\uBD80\uD558\uB2E4\uB294 \uB73B\uC774\uB2E4. \uBCA0\uD0C0\uB294 \uC0AC\uB0E5\uAC1C\uC790\uB9AC \uC54C\uD30C2\uD615 \uBCC0\uAD11\uC131\uC758 \uD2B9\uC131\uC744 \uB760\uACE0 \uC788\uC73C\uBA70 \uBC1D\uAE30\uB294 0.04\uB4F1\uAE09\uC758 \uC9C4\uD3ED\uC73C\uB85C \uC694\uB3D9\uCE58\uBA70 \uCD5C\uB300 + 4.27 \uB4F1\uAE09\uAE4C\uC9C0 \uBC1D\uC544\uC9C4\uB2E4."@ko . . . "A"@en . . . . "Beta Hydrae"@in . "\u2212"@en . . . . . . . "\uBC14\uB2E4\uBC40\uC790\uB9AC \uBCA0\uD0C0\uB294 \uBC14\uB2E4\uBC40\uC790\uB9AC\uC758 \uCD5C\uB0A8\uB2E8\uC5D0 \uC704\uCE58\uD558\uACE0 \uC788\uB294 \uD56D\uC131\uC774\uB2E4. \uBCA0\uD0C0\uB294 \uC9C0\uAD6C\uC5D0\uC11C \uC57D 365\uAD11\uB144 \uB5A8\uC5B4\uC838 \uC788\uB2E4. \uBC14\uB2E4\uBC40\uC790\uB9AC \uBCA0\uD0C0\uB294 \uC30D\uC131\uC73C\uB85C, \uAD6C\uC131\uC6D0 \uBC14\uB2E4\uBC40\uC790\uB9AC A\uC640 B\uB294 \uCC9C\uAD6C\uC5D0\uC11C \uCD5C\uB300 1.7\uCD08\uAC01\uAE4C\uC9C0 \uC11C\uB85C \uB5A8\uC5B4\uC9C0\uB294\uB370, \uC5EC\uAE30\uC11C \uACC4\uC0B0\uD55C \uB450 \uBCC4 \uC0AC\uC774\uC758 \uCD5C\uB300 \uC774\uACA9 \uAC70\uB9AC\uB294 190 \uC218\uC900\uC774\uBA70 \uACF5\uC804 \uC8FC\uAE30\uB294 \uC57D 1\uCC9C \uB144\uC5D0 \uB2EC\uD560 \uAC83\uC73C\uB85C \uC608\uC0C1\uB41C\uB2E4. \uADF8\uB7EC\uB098 \uC774 \uC608\uC0C1\uAC12\uC740 \uD655\uC2E4\uD55C \uAC83\uC740 \uC544\uB2C8\uB2E4. \uC8FC\uC131 A\uB294 \uAC89\uBCF4\uAE30 \uB4F1\uAE09 4.67\uC5D0 \uBD84\uAD11\uD615\uC740 B9\uC758 \uB728\uAC70\uC6B4 \uCCAD\uBC31\uC0C9 \uBCC4\uC774\uBA70 \uBC18\uC131 B\uB294 \uC0C1\uB300\uC801\uC73C\uB85C \uC5B4\uB450\uC6B4 \uAC89\uBCF4\uAE30 \uB4F1\uAE09 5.47\uC774\uBA70 \uBD84\uAD11\uD615\uC740 \uC815\uD655\uD788 \uC54C\uB824\uC838 \uC788\uC9C0 \uC54A\uB2E4. \uBCA0\uD0C0 \uD56D\uC131\uACC4\uC758 \uB098\uC774\uB294 \uACE0\uC791 2\uC5B5 2\uCC9C\uB9CC \uB144\uC5D0 \uBD88\uACFC\uD558\uB2E4. \uD2B9\uAE30\uD560 \uC810\uC740 \uBC14\uB2E4\uBC40\uC790\uB9AC \uBCA0\uD0C0\uC758 \uBD84\uAD11\uD615\uC5D0\uB294 peculiar\uAC00 \uBD99\uC5B4 \uC788\uB294\uB370 \uC774\uB294 \uD56D\uC131\uC758 \uB300\uAE30\uC5D0 \uADDC\uC18C, \uD06C\uB85C\uBBB4, \uC2A4\uD2B8\uB860\uD2AC\uC774 \uD48D\uBD80\uD558\uB2E4\uB294 \uB73B\uC774\uB2E4. \uBCA0\uD0C0\uB294 \uC0AC\uB0E5\uAC1C\uC790\uB9AC \uC54C\uD30C2\uD615 \uBCC0\uAD11\uC131\uC758 \uD2B9\uC131\uC744 \uB760\uACE0 \uC788\uC73C\uBA70 \uBC1D\uAE30\uB294 0.04\uB4F1\uAE09\uC758 \uC9C4\uD3ED\uC73C\uB85C \uC694\uB3D9\uCE58\uBA70 \uCD5C\uB300 + 4.27 \uB4F1\uAE09\uAE4C\uC9C0 \uBC1D\uC544\uC9C4\uB2E4."@ko . . "\u22120.34"@en . . . . . . "B"@en . . . . . . "Beta Hydrae"@es . . "Beta Hydrae (Beta Hya, \u03B2 Hydrae, \u03B2 Hya) adalah bintang ganda yang ada di rasi bintang Hydra. Secara umum, magnitudonya bervariasi sebesar 0.04 magnitudo dengan periode 2.344 hari, dan pada saat paling terang magnitudoya sekitar 4.27. Bintang yang paling terang adalah bintang raksasa yang diklasifikasikan sebagai \u03B1\u00B2 Canum Venaticorum."@in . . .