. "\u0422\u0430\u0443 \u0410\u043D\u0434\u0440\u043E\u043C\u0435\u0434\u044B (\u043B\u0430\u0442. \u03C4 Andromedae), 53 \u0410\u043D\u0434\u0440\u043E\u043C\u0435\u0434\u044B (\u043B\u0430\u0442. 53 Andromedae), HD 10205 \u2014 \u0434\u0432\u043E\u0439\u043D\u0430\u044F \u0437\u0432\u0435\u0437\u0434\u0430 \u0432 \u0441\u043E\u0437\u0432\u0435\u0437\u0434\u0438\u0438 \u0410\u043D\u0434\u0440\u043E\u043C\u0435\u0434\u044B \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 663 \u0441\u0432\u0435\u0442\u043E\u0432\u044B\u0445 \u043B\u0435\u0442 (\u043E\u043A\u043E\u043B\u043E 203 \u043F\u0430\u0440\u0441\u0435\u043A\u043E\u0432) \u043E\u0442 \u0421\u043E\u043B\u043D\u0446\u0430. \u0412\u0438\u0434\u0438\u043C\u0430\u044F \u0437\u0432\u0451\u0437\u0434\u043D\u0430\u044F \u0432\u0435\u043B\u0438\u0447\u0438\u043D\u0430 \u0437\u0432\u0435\u0437\u0434\u044B \u2014 +4,942m."@ru . . . . . . . . . . . "\u22120.41"@en . . . . "Tau Andromedae (\u03C4 And / \u03C4 Andromedae) \u00E8 una stella gigante azzurra di magnitudine 4,96 situata nella costellazione di Andromeda. Dista 681 anni luce dal sistema solare."@it . "\uC548\uB4DC\uB85C\uBA54\uB2E4\uC790\uB9AC \uD0C0\uC6B0"@ko . . "Tau Andromedae"@es . . "\u0422\u0430\u0443 \u0410\u043D\u0434\u0440\u043E\u043C\u0435\u0434\u044B (\u043B\u0430\u0442. \u03C4 Andromedae), 53 \u0410\u043D\u0434\u0440\u043E\u043C\u0435\u0434\u044B (\u043B\u0430\u0442. 53 Andromedae), HD 10205 \u2014 \u0434\u0432\u043E\u0439\u043D\u0430\u044F \u0437\u0432\u0435\u0437\u0434\u0430 \u0432 \u0441\u043E\u0437\u0432\u0435\u0437\u0434\u0438\u0438 \u0410\u043D\u0434\u0440\u043E\u043C\u0435\u0434\u044B \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 663 \u0441\u0432\u0435\u0442\u043E\u0432\u044B\u0445 \u043B\u0435\u0442 (\u043E\u043A\u043E\u043B\u043E 203 \u043F\u0430\u0440\u0441\u0435\u043A\u043E\u0432) \u043E\u0442 \u0421\u043E\u043B\u043D\u0446\u0430. \u0412\u0438\u0434\u0438\u043C\u0430\u044F \u0437\u0432\u0451\u0437\u0434\u043D\u0430\u044F \u0432\u0435\u043B\u0438\u0447\u0438\u043D\u0430 \u0437\u0432\u0435\u0437\u0434\u044B \u2014 +4,942m."@ru . . . . "Tau Andromedae (\u03C4 Andromedae / \u03C4 And) est une \u00E9toile g\u00E9ante bleue de la constellation bor\u00E9ale d'Androm\u00E8de. Elle est visible \u00E0 l'\u0153il nu et sa magnitude apparente est de 4,94."@fr . . . . . "Tau Andromedae (53 Andromedae) \u00E9 uma estrela na dire\u00E7\u00E3o da constela\u00E7\u00E3o de Andromeda. Possui uma ascens\u00E3o reta de 01h 40m 34.80s e uma declina\u00E7\u00E3o de +40\u00B0 34\u2032 37.6\u2033. Sua magnitude aparente \u00E9 igual a 4.96. Considerando sua dist\u00E2ncia de 681 anos-luz em rela\u00E7\u00E3o \u00E0 Terra, sua magnitude absoluta \u00E9 igual a \u22121.64. Pertence \u00E0 classe espectral B8III. \u00C9 uma estrela vari\u00E1vel suspeita."@pt . "7810"^^ . . . . . "2781800"^^ . . . "Tau Andromedae"@in . . . . . "Tau Andromedae"@pt . . . . "Tau d'Andr\u00F2meda (Andromedae) \u00E9s una estrella bin\u00E0ria de la constel\u00B7laci\u00F3 d'Andr\u00F2meda. Est\u00E0 aproximadament a 681 anys-llum de la Terra. El component primari, \u03C4 d'Andr\u00F2meda A, \u00E9s una gegant blava-blanca del tipus B de la magnitud aparent +4,96. La seva companya, \u03C4 d'Andr\u00F2meda B, \u00E9s una estrella de la 12a magnitud, distant 52,3 segons d'arc."@ca . . . . "Tau Andromedae (\u03C4 Andromedae / \u03C4 And) est une \u00E9toile g\u00E9ante bleue de la constellation bor\u00E9ale d'Androm\u00E8de. Elle est visible \u00E0 l'\u0153il nu et sa magnitude apparente est de 4,94."@fr . "Tau Andromedae, Latinized from \u03C4 Andromedae, is the Bayer designation for a single star in the northern constellation of Andromeda. It has an apparent visual magnitude of +4.94, which is bright enough to be viewed from dark suburban skies. From parallax measurements made during the Gaia mission, the distance to this star can be estimated as roughly 680 light-years (210 parsecs) from Earth. The brightness of this star is diminished by 0.24 in magnitude due to extinction caused by intervening gas and dust. It is drifting closer to the Sun with a radial velocity of \u221214 km/s. The spectrum of this star matches a stellar classification of B5 III, with the luminosity class of III indicating that this is a giant star. It is radiating about 851 times the luminosity of the Sun from its photosphere at an effective temperature of 12,670 K. The star is an estimated 217 million years old and is spinning with a high projected rotational velocity of ~74 km/s."@en . "Tau Andromedae"@fr . . . . . . "851"^^ . . . . "Tau Andromedae (Tau And, \u03C4 Andromedae, \u03C4 And), som \u00E4r stj\u00E4rnans Bayerbeteckning, \u00E4r bel\u00E4gen i \u00F6stra delen av stj\u00E4rnbilden Andromeda. Den har en skenbar magnitud p\u00E5 ungef\u00E4r +4,94 och kan ses med blotta \u00F6gat fr\u00E5n m\u00F6rka platser utan ljusf\u00F6roreningar. Baserat p\u00E5 parallaxm\u00E4tningar under Hipparcosuppdraget befinner den sig p\u00E5 ett avst\u00E5nd av ca 710 ljus\u00E5r (220 parsek) fr\u00E5n solen. Ljusstyrkan minskar med 0,24 i magnitud p\u00E5 grund av skymning orsakad av mellanliggande gas och stoft."@sv . . "1119772947"^^ . . . "B5 III"@en . . "4.7804"^^ . . . "\u30A2\u30F3\u30C9\u30ED\u30E1\u30C0\u5EA7\u03C4\u661F\uFF08\u30A2\u30F3\u30C9\u30ED\u30E1\u30C0\u3056\u30BF\u30A6\u305B\u3044\u3001\u03C4 Andromedae\u3001\u03C4 And\uFF09\u306F\u3001\u30A2\u30F3\u30C9\u30ED\u30E1\u30C0\u5EA7\u306E\u6052\u661F\u3067\u3042\u308B\u3002\u898B\u304B\u3051\u306E\u7B49\u7D1A\u306F4.95\u3067\u3001\u90CA\u5916\u306E\u7A7A\u4EE5\u4E0A\u306E\u6697\u3044\u591C\u7A7A\u3067\u306F\u3001\u8089\u773C\u3067\u307F\u308B\u3053\u3068\u304C\u3067\u304D\u308B\u3002\u30D2\u30C3\u30D1\u30EB\u30B3\u30B9\u885B\u661F\u304C\u6E2C\u5B9A\u3057\u305F\u5E74\u5468\u8996\u5DEE\u3092\u57FA\u306B\u8A08\u7B97\u3057\u305F\u592A\u967D\u304B\u3089\u306E\u8DDD\u96E2\u306F\u3001\u304A\u3088\u305D710\u5149\u5E74\u3067\u3042\u308B\u3002"@ja . . . "Tau Andromedae"@de . "\uC548\uB4DC\uB85C\uBA54\uB2E4\uC790\uB9AC \uD0C0\uC6B0(\u03C4 And / \u03C4 Andromedae)\uB294 \uC548\uB4DC\uB85C\uBA54\uB2E4\uC790\uB9AC\uC758 \uD56D\uC131\uC774\uB2E4. \uC9C0\uAD6C\uC5D0\uC11C 681 \uAD11\uB144 \uB5A8\uC5B4\uC838 \uC788\uB2E4. \uCCAD\uBC31\uC0C9 B\uD615 \uAC70\uC131\uC73C\uB85C \uAC89\uBCF4\uAE30 \uB4F1\uAE09\uC740 +4.96 \uB4F1\uAE09\uC774\uB2E4."@ko . . "0.1304"^^ . "Tau d'Andr\u00F2meda (Andromedae) \u00E9s una estrella bin\u00E0ria de la constel\u00B7laci\u00F3 d'Andr\u00F2meda. Est\u00E0 aproximadament a 681 anys-llum de la Terra. El component primari, \u03C4 d'Andr\u00F2meda A, \u00E9s una gegant blava-blanca del tipus B de la magnitud aparent +4,96. La seva companya, \u03C4 d'Andr\u00F2meda B, \u00E9s una estrella de la 12a magnitud, distant 52,3 segons d'arc."@ca . "Tau Andromedae (\u03C4 And / \u03C4 Andromedae) adalah salah satu bintang di rasi bintang Andromeda. Bintang ini berada pada jarak 681 tahun cahaya dari Bumi. Bintang ini tergolong bintang raksasa biru keputihan tipe B dengan magnitudo +4.96."@in . . . . "Tau Andromedae (53 Andromedae) \u00E9 uma estrela na dire\u00E7\u00E3o da constela\u00E7\u00E3o de Andromeda. Possui uma ascens\u00E3o reta de 01h 40m 34.80s e uma declina\u00E7\u00E3o de +40\u00B0 34\u2032 37.6\u2033. Sua magnitude aparente \u00E9 igual a 4.96. Considerando sua dist\u00E2ncia de 681 anos-luz em rela\u00E7\u00E3o \u00E0 Terra, sua magnitude absoluta \u00E9 igual a \u22121.64. Pertence \u00E0 classe espectral B8III. \u00C9 uma estrela vari\u00E1vel suspeita."@pt . . . . . . . . "\u03C4 Andromedae (Tau Andromedae, kurz \u03C4 And) ist ein dem blo\u00DFen Auge sehr lichtschwach erscheinender Stern im Sternbild Andromeda. Die scheinbare Helligkeit dieses blauwei\u00DF schimmernden Sterns betr\u00E4gt 4,94m. Nach Parallaxen-Messungen der Raumsonde Gaia ist er etwa 682 Lichtjahre von der Erde entfernt."@de . "Tau Andromedae (Tau And, \u03C4 Andromedae, \u03C4 And), som \u00E4r stj\u00E4rnans Bayerbeteckning, \u00E4r bel\u00E4gen i \u00F6stra delen av stj\u00E4rnbilden Andromeda. Den har en skenbar magnitud p\u00E5 ungef\u00E4r +4,94 och kan ses med blotta \u00F6gat fr\u00E5n m\u00F6rka platser utan ljusf\u00F6roreningar. Baserat p\u00E5 parallaxm\u00E4tningar under Hipparcosuppdraget befinner den sig p\u00E5 ett avst\u00E5nd av ca 710 ljus\u00E5r (220 parsek) fr\u00E5n solen. Ljusstyrkan minskar med 0,24 i magnitud p\u00E5 grund av skymning orsakad av mellanliggande gas och stoft."@sv . . "\u5929\u5927\u5C07\u8ECD\u4E03"@zh . "Tau Andromedae (\u03C4 And / 53 Andromedae)\u200B es una estrella de la constelaci\u00F3n de Andr\u00F3meda.De magnitud aparente +4,96, se encuentra a 712 a\u00F1os luz de distancia del Sistema Solar."@es . "\u03C4 Andromedae (Tau Andromedae, kurz \u03C4 And) ist ein dem blo\u00DFen Auge sehr lichtschwach erscheinender Stern im Sternbild Andromeda. Die scheinbare Helligkeit dieses blauwei\u00DF schimmernden Sterns betr\u00E4gt 4,94m. Nach Parallaxen-Messungen der Raumsonde Gaia ist er etwa 682 Lichtjahre von der Erde entfernt. \u03C4 And ist wohl ein Riesenstern der Spektralklasse B5 III, doch wird er in anderen Studien als ein vom Unterriesen- ins Riesenstadium \u00FCbergehender B8 IV-III-Stern klassifiziert. In letzterem Fall w\u00E4re aus seiner Farbe zu schlie\u00DFen, dass kein zwischen der Erde und dem Stern liegender interstellarer Staub seine Helligkeit schw\u00E4cht. Er h\u00E4tte dann etwa 4,5 bis 4,6 Sonnenmassen, 6 Sonnendurchmesser und circa die 910-fache Sonnenleuchtkraft. Falls \u03C4 And aber ein B5-Riesenstern ist, deutet seine Farbe auf eine Verdunkelung seiner scheinbaren Helligkeit um knapp 0,3m infolge der Extinktion dazwischenliegenden interstellaren Staubs hin. Seine Leuchtkraft entspr\u00E4che dann rund 1200 Sonnenleuchtkr\u00E4ften, seine Masse w\u00E4re aber nur geringf\u00FCgig gr\u00F6\u00DFer. Aus der projizierten Rotationsgeschwindigkeit von 74 km/s geht hervor, dass \u03C4 And sich in weniger als 4,1 Tagen um seine eigene Achse dreht. \u03C4 And ist ein Einzelstern. Zwar wird im Washington Double Star Catalog ein 11,5m heller Begleiter mit der Katalogbezeichnung UCAC2 45921715 verzeichnet, der von der Erde aus gesehen im Jahr 2014 etwa 52,9 Bogensekunden von \u03C4 And entfernt stand, doch handelt es sich hierbei nur um einen optischen Doppelstern. Der scheinbare Begleiter steht nur zuf\u00E4llig in der gleichen Sichtlinie am Himmel. Gaias Parallaxenmessungen ergaben, dass er mit circa 1120 Lichtjahren Abstand wesentlich weiter als \u03C4 And von der Erde entfernt ist."@de . . . "Tau Andromedae"@en . . "217"^^ . . "Tau Andromedae, Latinized from \u03C4 Andromedae, is the Bayer designation for a single star in the northern constellation of Andromeda. It has an apparent visual magnitude of +4.94, which is bright enough to be viewed from dark suburban skies. From parallax measurements made during the Gaia mission, the distance to this star can be estimated as roughly 680 light-years (210 parsecs) from Earth. The brightness of this star is diminished by 0.24 in magnitude due to extinction caused by intervening gas and dust. It is drifting closer to the Sun with a radial velocity of \u221214 km/s."@en . . "Tau d'Andr\u00F2meda"@ca . . . "\uC548\uB4DC\uB85C\uBA54\uB2E4\uC790\uB9AC \uD0C0\uC6B0(\u03C4 And / \u03C4 Andromedae)\uB294 \uC548\uB4DC\uB85C\uBA54\uB2E4\uC790\uB9AC\uC758 \uD56D\uC131\uC774\uB2E4. \uC9C0\uAD6C\uC5D0\uC11C 681 \uAD11\uB144 \uB5A8\uC5B4\uC838 \uC788\uB2E4. \uCCAD\uBC31\uC0C9 B\uD615 \uAC70\uC131\uC73C\uB85C \uAC89\uBCF4\uAE30 \uB4F1\uAE09\uC740 +4.96 \uB4F1\uAE09\uC774\uB2E4."@ko . . "Tau Andromedae (\u03C4 And / \u03C4 Andromedae) adalah salah satu bintang di rasi bintang Andromeda. Bintang ini berada pada jarak 681 tahun cahaya dari Bumi. Bintang ini tergolong bintang raksasa biru keputihan tipe B dengan magnitudo +4.96."@in . "J2000"@en . . . . "Tau Andromedae (\u03C4 And / \u03C4 Andromedae) \u00E8 una stella gigante azzurra di magnitudine 4,96 situata nella costellazione di Andromeda. Dista 681 anni luce dal sistema solare."@it . . . . "Tau Andromedae"@it . "\u4ED9\u5973\u5EA7\u03C4\uFF0C\u53C8\u540DBD+39 378\uFF0CHD 10205\u3001SAO 37418\u3001HR 477\uFF0C\u662F\u4ED9\u5973\u5EA7\u7684\u4E00\u9897\u6052\u661F\uFF0C\u89C6\u661F\u7B49\u4E3A4.94\uFF0C\u4F4D\u4E8E\u9280\u7D93132.92\uFF0C\u9280\u7DEF-21.34\uFF0C\u5176B1900.0\u5750\u6807\u4E3A\u8D64\u7D931h 34m 40.4s\uFF0C\u8D64\u7DEF+40\u00B0 -21.34\u2032 14\u2033\u3002"@zh . . . . . "\u30A2\u30F3\u30C9\u30ED\u30E1\u30C0\u5EA7\u03C4\u661F\uFF08\u30A2\u30F3\u30C9\u30ED\u30E1\u30C0\u3056\u30BF\u30A6\u305B\u3044\u3001\u03C4 Andromedae\u3001\u03C4 And\uFF09\u306F\u3001\u30A2\u30F3\u30C9\u30ED\u30E1\u30C0\u5EA7\u306E\u6052\u661F\u3067\u3042\u308B\u3002\u898B\u304B\u3051\u306E\u7B49\u7D1A\u306F4.95\u3067\u3001\u90CA\u5916\u306E\u7A7A\u4EE5\u4E0A\u306E\u6697\u3044\u591C\u7A7A\u3067\u306F\u3001\u8089\u773C\u3067\u307F\u308B\u3053\u3068\u304C\u3067\u304D\u308B\u3002\u30D2\u30C3\u30D1\u30EB\u30B3\u30B9\u885B\u661F\u304C\u6E2C\u5B9A\u3057\u305F\u5E74\u5468\u8996\u5DEE\u3092\u57FA\u306B\u8A08\u7B97\u3057\u305F\u592A\u967D\u304B\u3089\u306E\u8DDD\u96E2\u306F\u3001\u304A\u3088\u305D710\u5149\u5E74\u3067\u3042\u308B\u3002"@ja . . . . "+4.94"@en . . . . . . . . . . "\u4ED9\u5973\u5EA7\u03C4\uFF0C\u53C8\u540DBD+39 378\uFF0CHD 10205\u3001SAO 37418\u3001HR 477\uFF0C\u662F\u4ED9\u5973\u5EA7\u7684\u4E00\u9897\u6052\u661F\uFF0C\u89C6\u661F\u7B49\u4E3A4.94\uFF0C\u4F4D\u4E8E\u9280\u7D93132.92\uFF0C\u9280\u7DEF-21.34\uFF0C\u5176B1900.0\u5750\u6807\u4E3A\u8D64\u7D931h 34m 40.4s\uFF0C\u8D64\u7DEF+40\u00B0 -21.34\u2032 14\u2033\u3002"@zh . "Tau Andromedae"@sv . . . . . . . . . . . . "\u22120.09"@en . . "\u0422\u0430\u0443 \u0410\u043D\u0434\u0440\u043E\u043C\u0435\u0434\u044B"@ru . "Tau Andromedae (\u03C4 And / 53 Andromedae)\u200B es una estrella de la constelaci\u00F3n de Andr\u00F3meda.De magnitud aparente +4,96, se encuentra a 712 a\u00F1os luz de distancia del Sistema Solar."@es . . . . . . "\u30A2\u30F3\u30C9\u30ED\u30E1\u30C0\u5EA7\u30BF\u30A6\u661F"@ja . . . . . .