"44 Ophiuchi, som \u00E4r stj\u00E4rnans Flamsteed-beteckning, \u00E4r en ensam stj\u00E4rna i den s\u00F6dra delen av stj\u00E4rnbilden Ormb\u00E4raren, som ocks\u00E5 har Bayer-beteckningen b Ophiuchi. Den har en genomsnittlig skenbar magnitud p\u00E5 ca 4,16 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 39,2 mas, ber\u00E4knas den befinna sig p\u00E5 ett avst\u00E5nd p\u00E5 ca 83 ljus\u00E5r (ca 26 parsek) fr\u00E5n solen. Den r\u00F6r sig n\u00E4rmare solen med en heliocentrisk radialhastighet av ca \u201337 km/s. och ber\u00E4knas komma inom ett avst\u00E5nd av 30 ljus\u00E5r fr\u00E5n solen inom 550 000 \u00E5r."@sv . "1.77"^^ . . "kA5hA9mF1III"@en . . . . . . "44 Ophiuchi"@en . "78"^^ . "39.22"^^ . "44 Ophiuchi (b Ophiuchi) \u00E9 uma estrela na dire\u00E7\u00E3o da Ophiuchus. Possui uma ascens\u00E3o reta de 17h 26m 22.22s e uma declina\u00E7\u00E3o de \u221224\u00B0 10\u2032 30.1\u2033. Sua magnitude aparente \u00E9 igual a 4.16. Considerando sua dist\u00E2ncia de 84 anos-luz em rela\u00E7\u00E3o \u00E0 Terra, sua magnitude absoluta \u00E9 igual a 2.11. Pertence \u00E0 classe espectral A3IV:m."@pt . "J2000"@en . . "44 Ophiuchi is a single star in the constellation Ophiuchus. It has the Bayer designation b Ophiuchi, while 44 Ophiuchi is the Flamsteed designation. It is visible to the naked eye as a faint, white-hued star with an apparent visual magnitude of 4.16. The distance to this object is approximately 83.2 light years based on parallax. It is drifting closer to the Earth with a heliocentric radial velocity of -37.2 km/s, and is predicted to come within 30 light-years around 585,000 years from now."@en . "44 Ophiuchi is a single star in the constellation Ophiuchus. It has the Bayer designation b Ophiuchi, while 44 Ophiuchi is the Flamsteed designation. It is visible to the naked eye as a faint, white-hued star with an apparent visual magnitude of 4.16. The distance to this object is approximately 83.2 light years based on parallax. It is drifting closer to the Earth with a heliocentric radial velocity of -37.2 km/s, and is predicted to come within 30 light-years around 585,000 years from now. This is an Am star with a stellar classification of kA5hA9mF1III, indicating it has the luminosity class of a giant star with a spectrum that matches an A5 star based on the calcium K line, and an A9 star from the hydrogen and metal lines. It is around a billion years old with 1.77 times the mass of the Sun and 1.9 times the Sun's girth. The star is radiating 13 times the Sun's luminosity from its photosphere at an effective temperature of 7,559 K. It retains a moderately high rotation rate, showing a projected rotational velocity of 78 km/s."@en . . . "HD157792 \u2014 \u0445\u0456\u043C\u0456\u0447\u043D\u043E \u043F\u0435\u043A\u0443\u043B\u044F\u0440\u043D\u0430 \u0437\u043E\u0440\u044F \u0441\u043F\u0435\u043A\u0442\u0440\u0430\u043B\u044C\u043D\u043E\u0433\u043E \u043A\u043B\u0430\u0441\u0443 A3, \u0449\u043E \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 4,2.\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 83,7 \u0441\u0432\u0456\u0442\u043B\u043E\u0432\u0438\u0445 \u0440\u043E\u043A\u0456\u0432 \u0432\u0456\u0434 \u0421\u043E\u043D\u0446\u044F."@uk . . "+0.28"@en . "HD157792 \u2014 \u0445\u0456\u043C\u0456\u0447\u043D\u043E \u043F\u0435\u043A\u0443\u043B\u044F\u0440\u043D\u0430 \u0437\u043E\u0440\u044F \u0441\u043F\u0435\u043A\u0442\u0440\u0430\u043B\u044C\u043D\u043E\u0433\u043E \u043A\u043B\u0430\u0441\u0443 A3, \u0449\u043E \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 4,2.\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 83,7 \u0441\u0432\u0456\u0442\u043B\u043E\u0432\u0438\u0445 \u0440\u043E\u043A\u0456\u0432 \u0432\u0456\u0434 \u0421\u043E\u043D\u0446\u044F."@uk . . . . "\u86C7\u592B\u5EA744\uFF0C\u53C8\u540DCD-2413337\uFF0CHD 157792\u3001SAO 185401\u3001HR 6486\uFF0C\u662F\u86C7\u592B\u5EA7\u7684\u4E00\u9897\u6052\u661F\uFF0C\u89C6\u661F\u7B49\u4E3A4.17\uFF0C\u4F4D\u4E8E\u9280\u7D931.71\uFF0C\u9280\u7DEF6.19\uFF0C\u5176B1900.0\u5750\u6807\u4E3A\u8D64\u7D9317h 20m 15.7s\uFF0C\u8D64\u7DEF-24\u00B0 6.19\u2032 0\u2033\u3002"@zh . . . . . . . . "7559"^^ . . . . . . "44 Ophiuchi (b Ophiuchi) \u00E9 uma estrela na dire\u00E7\u00E3o da Ophiuchus. Possui uma ascens\u00E3o reta de 17h 26m 22.22s e uma declina\u00E7\u00E3o de \u221224\u00B0 10\u2032 30.1\u2033. Sua magnitude aparente \u00E9 igual a 4.16. Considerando sua dist\u00E2ncia de 84 anos-luz em rela\u00E7\u00E3o \u00E0 Terra, sua magnitude absoluta \u00E9 igual a 2.11. Pertence \u00E0 classe espectral A3IV:m."@pt . . "\u221237.20"@en . . . . . . . . "7932"^^ . . . . "+0.12"@en . . . . . "b Ophiuchi(\nNe doit pas \u00EAtre confondu avec Beta Ophiuchi. ) 44 Ophiuchi(b Ophiuchi) Autres d\u00E9signations b Oph, 44 Oph (Flamsteed), HR 6486, HD 157792, HIP 85340, GJ 673.1, GJ 9591, CD-24 13337, CPD-24 5895, FK5 1457, SAO 185401, NSV 8640 44 Ophiuchi (en abr\u00E9g\u00E9 44 Oph) est une \u00E9toile Am de la constellation d'Ophiuchus. Elle porte \u00E9galement la d\u00E9signation de Bayer de b Ophiuchi, 44 Ophiuchi \u00E9tant sa d\u00E9signation de Flamsteed. Elle est visible \u00E0 l'\u0153il nu avec une magnitude apparente de 4,16."@fr . . . "0.24"^^ . . . . . . . . . . . . . "\u5929\u6C5F\u56DB"@zh . . "4.15"^^ . "44 Ophiuchi"@sv . . "44 Ophiuchi"@en . . . . "13"^^ . "+0.10"@en . "+0.30"@en . . "44 Ophiuchi"@pt . . . . "38042045"^^ . "44 Ophiuchi"@fr . . . . . . "\u86C7\u592B\u5EA744\uFF0C\u53C8\u540DCD-2413337\uFF0CHD 157792\u3001SAO 185401\u3001HR 6486\uFF0C\u662F\u86C7\u592B\u5EA7\u7684\u4E00\u9897\u6052\u661F\uFF0C\u89C6\u661F\u7B49\u4E3A4.17\uFF0C\u4F4D\u4E8E\u9280\u7D931.71\uFF0C\u9280\u7DEF6.19\uFF0C\u5176B1900.0\u5750\u6807\u4E3A\u8D64\u7D9317h 20m 15.7s\uFF0C\u8D64\u7DEF-24\u00B0 6.19\u2032 0\u2033\u3002"@zh . . "1.028"^^ . . . "2.13"^^ . . . "44 Ophiuchi, som \u00E4r stj\u00E4rnans Flamsteed-beteckning, \u00E4r en ensam stj\u00E4rna i den s\u00F6dra delen av stj\u00E4rnbilden Ormb\u00E4raren, som ocks\u00E5 har Bayer-beteckningen b Ophiuchi. Den har en genomsnittlig skenbar magnitud p\u00E5 ca 4,16 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 39,2 mas, ber\u00E4knas den befinna sig p\u00E5 ett avst\u00E5nd p\u00E5 ca 83 ljus\u00E5r (ca 26 parsek) fr\u00E5n solen. Den r\u00F6r sig n\u00E4rmare solen med en heliocentrisk radialhastighet av ca \u201337 km/s. och ber\u00E4knas komma inom ett avst\u00E5nd av 30 ljus\u00E5r fr\u00E5n solen inom 550 000 \u00E5r."@sv . . . . . . . . . . "HD157792"@uk . . "4.16"^^ . "1079519278"^^ . "\u2212118.18"@en . . . . . "1.9"^^ . . . "b Ophiuchi(\nNe doit pas \u00EAtre confondu avec Beta Ophiuchi. ) 44 Ophiuchi(b Ophiuchi) Autres d\u00E9signations b Oph, 44 Oph (Flamsteed), HR 6486, HD 157792, HIP 85340, GJ 673.1, GJ 9591, CD-24 13337, CPD-24 5895, FK5 1457, SAO 185401, NSV 8640 44 Ophiuchi (en abr\u00E9g\u00E9 44 Oph) est une \u00E9toile Am de la constellation d'Ophiuchus. Elle porte \u00E9galement la d\u00E9signation de Bayer de b Ophiuchi, 44 Ophiuchi \u00E9tant sa d\u00E9signation de Flamsteed. Elle est visible \u00E0 l'\u0153il nu avec une magnitude apparente de 4,16."@fr . . . . . . . .