"\u0421\u0438\u0433\u043C\u0430 \u0410\u043D\u0434\u0440\u043E\u043C\u0435\u0434\u044B"@ru . . . "2781073"^^ . . "\u5929\u5EC4\u4E09"@zh . "\uC548\uB4DC\uB85C\uBA54\uB2E4\uC790\uB9AC \uC2DC\uADF8\uB9C8(\u03C3 And / \u03C3 Andromedae)\uB294 \uC548\uB4DC\uB85C\uBA54\uB2E4\uC790\uB9AC\uC758 \uD56D\uC131\uC774\uB2E4. \uC9C0\uAD6C\uC5D0\uC11C 141 \uAD11\uB144 \uB5A8\uC5B4\uC838 \uC788\uB2E4. \uCCAD\uBC31\uC0C9 A\uD615 \uC8FC\uACC4\uC5F4\uC131\uC73C\uB85C \uAC89\uBCF4\uAE30 \uB4F1\uAE09\uC740 +4.51 \uB4F1\uAE09\uC774\uB2E4. \uC774\uB7EC\uD55C \uBC1D\uAE30\uB294 \uB300\uBD80\uBD84\uC758 \uC704\uCE58\uC5D0\uC11C \uB9E8\uB208\uC73C\uB85C \uBCFC \uC218 \uC788\uC744 \uC815\uB3C4\uC774\uB2E4."@ko . . . "Sigma Andromedae"@en . . . . . . . . . . . . "Sigma Andromedae"@fr . "\u03C3 Andromedae (Sigma Andromedae, kurz \u03C3 And) ist mit einer scheinbaren Helligkeit von 4,52m ein dem blo\u00DFen Auge recht lichtschwach erscheinender, wei\u00DF leuchtender Stern im Sternbild Andromeda. Nach Parallaxen-Messungen der Raumsonde Gaia ist er etwa 140 Lichtjahre von der Erde entfernt. Die Helligkeit des Sterns wird durch die Extinktion des interstellaren Gases und Staubs, die zwischen dem Stern und der Erde liegen, um circa 0,08m geschw\u00E4cht."@de . . "+4.51"@en . "Sigma Andromedae (Sig And, \u03C3 Andromedae, \u03C3 And), som \u00E4r stj\u00E4rnans Bayerbeteckning, \u00E4r en dv\u00E4rgstj\u00E4rna bel\u00E4gen i mellersta delen av stj\u00E4rnbilden Andromeda. Den har en skenbar magnitud p\u00E5 ungef\u00E4r +4,5, och \u00E4r tillr\u00E4ckligt ljus f\u00F6r att kunna ses med blotta \u00F6gat fr\u00E5n de flesta platser. Baserat p\u00E5 parallaxm\u00E4tningar gjorda under Hipparcosuppdraget befinner den sig p\u00E5 ett avst\u00E5nd av 135 ljus\u00E5r (41 parsek) fr\u00E5n solen. Stj\u00E4rnans magnitud minskar med 0,08 fr\u00E5n genom skymning orsakad av mellanliggande gas och stoft."@sv . . . . "Sigma Andromedae (25 Andromedae) \u00E9 uma estrela na dire\u00E7\u00E3o da constela\u00E7\u00E3o de Andromeda. Possui uma ascens\u00E3o reta de 00h 18m 19.71s e uma declina\u00E7\u00E3o de +36\u00B0 47\u2032 07.2\u2033. Sua magnitude aparente \u00E9 igual a 4.51. Considerando sua dist\u00E2ncia de 141 anos-luz em rela\u00E7\u00E3o \u00E0 Terra, sua magnitude absoluta \u00E9 igual a 1.33. Pertence \u00E0 classe espectral A2V. \u00C9 uma estrela vari\u00E1vel suspeita."@pt . . . . . . . . . . "\uC548\uB4DC\uB85C\uBA54\uB2E4\uC790\uB9AC \uC2DC\uADF8\uB9C8"@ko . . . "\u03C3 Andromedae (Sigma Andromedae, kurz \u03C3 And) ist mit einer scheinbaren Helligkeit von 4,52m ein dem blo\u00DFen Auge recht lichtschwach erscheinender, wei\u00DF leuchtender Stern im Sternbild Andromeda. Nach Parallaxen-Messungen der Raumsonde Gaia ist er etwa 140 Lichtjahre von der Erde entfernt. Die Helligkeit des Sterns wird durch die Extinktion des interstellaren Gases und Staubs, die zwischen dem Stern und der Erde liegen, um circa 0,08m geschw\u00E4cht. \u03C3 And ist ein Hauptreihenstern der Spektralklasse A2 V. Der Stern besitzt etwa 2,12 Sonnenmassen, 2,13 Sonnendurchmesser sowie 21 Sonnenleuchtkr\u00E4fte. Die effektive Temperatur seiner Photosph\u00E4re ist mit 8770 Kelvin deutlich h\u00F6her als jene der Sonne. \u03C3 And hat eine hohe projizierte Rotationsgeschwindigkeit von etwa 123 km/s und ist rund 450 Millionen Jahre alt. Der Stern zeigt de facto keine photometrische Ver\u00E4nderlichkeit und dient als Standardstern des UBV-Systems. Mit dem Spitzer-Weltraumteleskop wurde eine Tr\u00FCmmerscheibe um \u03C3 And entdeckt, die etwa 20,3 Astronomische Einheiten von dem Stern entfernt ist und eine mittlere Temperatur von 132, 9 K besitzt. 2009 wurde durch im Lick-Observatorium angestellte Beobachtungen ein 11,4m heller Begleiter, \u03C3 And B, entdeckt, der eine gemeinsame Eigenbewegung mit \u03C3 And A zeigt und von der Erde aus betrachtet im Jahr 2016 circa 7,0 Bogensekunden von diesem entfernt stand. Gaias Messungen ergaben f\u00FCr \u03C3 And B eine Parallaxe von (23,5181 \u00B1 0,0491) Millibogensekunden. Dies entspricht einer Entfernung von 139 Lichtjahren von der Erde, sodass hierdurch bei Ber\u00FCcksichtigung der Messunsicherheit die gravitative Bindung des Begleiters an \u03C3 And A best\u00E4tigt wird. Der Begleiter d\u00FCrfte ein Roter Zwerg des Spektraltyps M4 sein und eine reale Distanz von etwa 271 Astronomischen Einheiten zum Hauptstern aufweisen. \u03C3 And k\u00F6nnte der Ursa-Major-Gruppe, einem sog. Bewegungssternhaufen, angeh\u00F6ren, dessen Mitglieder \u00E4hnliche Eigenbewegungen besitzen und wahrscheinlich gemeinsam entstanden sind."@de . . "450"^^ . . "123"^^ . "A2 V"@en . . . . . . . "\u4ED9\u5973\u5EA7\u03C3\uFF0C\u53C8\u540DBD+35 44\uFF0CHD 1404\u3001SAO 53798\u3001HR 68\uFF0C\u662F\u4ED9\u5973\u5EA7\u7684\u4E00\u9897\u6052\u661F\uFF0C\u89C6\u661F\u7B49\u4E3A4.52\uFF0C\u4F4D\u4E8E\u9280\u7D93115.59\uFF0C\u9280\u7DEF-25.61\uFF0C\u5176B1900.0\u5750\u6807\u4E3A\u8D64\u7D930h 13m 6s\uFF0C\u8D64\u7DEF+36\u00B0 -25.61\u2032 51\u2033\u3002"@zh . "23.2542"^^ . . . "Sigma Andromedae"@it . "Sigma Andromedae (\u03C3 And / \u03C3 Andromedae) \u00E8 una stella bianca nella sequenza principale di magnitudine 4,52 situata nella costellazione di Andromeda. Dista 141 anni luce dal sistema solare."@it . . . . "Sigma Andromedae (\u03C3 And / \u03C3 Andromedae) adalah bintang yang berada di rasi bintang Andromeda. Sigma Andromedae adalah bintang katai putih kelas A dengan magnitudo +4.51. Bintang ini berada pada jarak 141 tahun cahaya dari Bumi."@in . . "Sigma Andromedae (Sig And, \u03C3 Andromedae, \u03C3 And), som \u00E4r stj\u00E4rnans Bayerbeteckning, \u00E4r en dv\u00E4rgstj\u00E4rna bel\u00E4gen i mellersta delen av stj\u00E4rnbilden Andromeda. Den har en skenbar magnitud p\u00E5 ungef\u00E4r +4,5, och \u00E4r tillr\u00E4ckligt ljus f\u00F6r att kunna ses med blotta \u00F6gat fr\u00E5n de flesta platser. Baserat p\u00E5 parallaxm\u00E4tningar gjorda under Hipparcosuppdraget befinner den sig p\u00E5 ett avst\u00E5nd av 135 ljus\u00E5r (41 parsek) fr\u00E5n solen. Stj\u00E4rnans magnitud minskar med 0,08 fr\u00E5n genom skymning orsakad av mellanliggande gas och stoft."@sv . "Sigma Andromedae (\u03C3 And / \u03C3 Andromedae) \u00E8 una stella bianca nella sequenza principale di magnitudine 4,52 situata nella costellazione di Andromeda. Dista 141 anni luce dal sistema solare."@it . "+0.07"@en . "21.23"^^ . . . . "0.1809"^^ . "Sigma Andromedae (25 Andromedae) \u00E9 uma estrela na dire\u00E7\u00E3o da constela\u00E7\u00E3o de Andromeda. Possui uma ascens\u00E3o reta de 00h 18m 19.71s e uma declina\u00E7\u00E3o de +36\u00B0 47\u2032 07.2\u2033. Sua magnitude aparente \u00E9 igual a 4.51. Considerando sua dist\u00E2ncia de 141 anos-luz em rela\u00E7\u00E3o \u00E0 Terra, sua magnitude absoluta \u00E9 igual a 1.33. Pertence \u00E0 classe espectral A2V. \u00C9 uma estrela vari\u00E1vel suspeita."@pt . . "Sigma d'Andr\u00F2meda (\u03C3 Andromedae) \u00E9s una estrella de la constel\u00B7laci\u00F3 d'Andr\u00F2meda. Sigma d'Andr\u00F2meda \u00E9s una nana de la seq\u00FC\u00E8ncia principal blanca del tipus A de la magnitud aparent +4,51. Est\u00E0 aproximadament a 141 anys-llum de la Terra."@ca . . . "2.13"^^ . . "Sigma Andromedae (\u03C3 And / \u03C3 Andromedae) adalah bintang yang berada di rasi bintang Andromeda. Sigma Andromedae adalah bintang katai putih kelas A dengan magnitudo +4.51. Bintang ini berada pada jarak 141 tahun cahaya dari Bumi."@in . "12261"^^ . "Sigma Andromedae"@in . . . "Sigma Andromedae"@sv . . . . "Sigma Andromedae, Latinized from \u03C3 Andromedae, is the Bayer designation for a single star in the northern constellation of Andromeda. It has an apparent visual magnitude of +4.5, which is bright enough to be seen with the naked eye from most locations. Parallax measurements made during the Gaia mission place it at a distance of about 140 light-years (43 parsecs). The magnitude of the star is diminished by 0.08 from extinction caused by intervening gas and dust. It is drifting closer to the Sun with a radial velocity of \u20138 km/s. This star has a stellar classification of A2 V, which matches the spectrum of an A-type main sequence star. It is about 450 million years old and is spinning rapidly with a projected rotational velocity of 123 km/s. The star has 2.12 times the mass of the Sun and 2.13 times the Sun's girth. It is radiating 21 times the luminosity of the Sun from its photosphere at an effective temperature of 8,929 K, giving it the white-hued glow of an A-type star. In the past, radial velocity variations have been reported, but this remains unconfirmed. The star does not show any significant photometric variations and is used as an ubvy standard star. A debris disk of warm dust around this star has been detected by Spitzer Space Telescope. A model fit to the data yields an orbital distance of 20.3 AU from the host star with a mean temperature of 132.9 K. Sigma Andromedae is a candidate for membership in the stream of stars associated with the Ursa Major Moving Group. This is a set of stars that share a common motion through space, which suggests they originated together."@en . "Sigma Andromedae"@pt . . . . . "\uC548\uB4DC\uB85C\uBA54\uB2E4\uC790\uB9AC \uC2DC\uADF8\uB9C8(\u03C3 And / \u03C3 Andromedae)\uB294 \uC548\uB4DC\uB85C\uBA54\uB2E4\uC790\uB9AC\uC758 \uD56D\uC131\uC774\uB2E4. \uC9C0\uAD6C\uC5D0\uC11C 141 \uAD11\uB144 \uB5A8\uC5B4\uC838 \uC788\uB2E4. \uCCAD\uBC31\uC0C9 A\uD615 \uC8FC\uACC4\uC5F4\uC131\uC73C\uB85C \uAC89\uBCF4\uAE30 \uB4F1\uAE09\uC740 +4.51 \uB4F1\uAE09\uC774\uB2E4. \uC774\uB7EC\uD55C \uBC1D\uAE30\uB294 \uB300\uBD80\uBD84\uC758 \uC704\uCE58\uC5D0\uC11C \uB9E8\uB208\uC73C\uB85C \uBCFC \uC218 \uC788\uC744 \uC815\uB3C4\uC774\uB2E4."@ko . . . . "\u0421\u0438\u0433\u043C\u0430 \u0410\u043D\u0434\u0440\u043E\u043C\u0435\u0434\u044B (\u043B\u0430\u0442. \u03C3 Andromedae) \u2014 \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. \u0412\u0438\u0434\u0438\u043C\u0430\u044F \u0437\u0432\u0451\u0437\u0434\u043D\u0430\u044F \u0432\u0435\u043B\u0438\u0447\u0438\u043D\u0430 \u0440\u0430\u0432\u043D\u0430 +4.5, \u0437\u0432\u0435\u0437\u0434\u0430 \u0432\u0438\u0434\u043D\u0430 \u043D\u0435\u0432\u043E\u043E\u0440\u0443\u0436\u0451\u043D\u043D\u044B\u043C \u0433\u043B\u0430\u0437\u043E\u043C. \u0418\u0437\u043C\u0435\u0440\u0435\u043D\u0438\u044F \u043F\u0430\u0440\u0430\u043B\u043B\u0430\u043A\u0441\u0430 \u0434\u0430\u043B\u043E \u043E\u0446\u0435\u043D\u043A\u0443 \u0440\u0430\u0441\u0441\u0442\u043E\u044F\u043D\u0438\u044F \u0434\u043E \u0437\u0432\u0435\u0437\u0434\u044B 135 \u0441\u0432\u0435\u0442\u043E\u0432\u044B\u0445 \u043B\u0435\u0442. \u0412\u0438\u0434\u0438\u043C\u044B\u0439 \u0431\u043B\u0435\u0441\u043A \u0437\u0432\u0435\u0437\u0434\u044B \u043E\u0441\u043B\u0430\u0431\u043B\u044F\u0435\u0442\u0441\u044F \u043D\u0430 0,08 \u0432\u0441\u043B\u0435\u0434\u0441\u0442\u0432\u0438\u0435 \u043C\u0435\u0436\u0437\u0432\u0451\u0437\u0434\u043D\u043E\u0439 \u044D\u043A\u0441\u0442\u0438\u043D\u043A\u0446\u0438\u0438. \u0417\u0432\u0435\u0437\u0434\u0443 \u043E\u0442\u043D\u043E\u0441\u044F\u0442 \u043A \u0441\u043F\u0435\u043A\u0442\u0440\u0430\u043B\u044C\u043D\u043E\u043C\u0443 \u043A\u043B\u0430\u0441\u0441\u0443 A2 V, \u0447\u0442\u043E \u0441\u043E\u043E\u0442\u0432\u0435\u0442\u0441\u0442\u0432\u0443\u0435\u0442 \u0441\u043F\u0435\u043A\u0442\u0440\u0443 \u0437\u0432\u0435\u0437\u0434\u044B \u0433\u043B\u0430\u0432\u043D\u043E\u0439 \u043F\u043E\u0441\u043B\u0435\u0434\u043E\u0432\u0430\u0442\u0435\u043B\u044C\u043D\u043E\u0441\u0442\u0438. \u0412\u043E\u0437\u0440\u0430\u0441\u0442 \u043E\u0446\u0435\u043D\u0438\u0432\u0430\u0435\u0442\u0441\u044F \u0432 450 \u043C\u0438\u043B\u043B\u0438\u043E\u043D\u043E\u0432 \u043B\u0435\u0442, \u043E\u0431\u044A\u0435\u043A\u0442 \u0431\u044B\u0441\u0442\u0440\u043E \u0432\u0440\u0430\u0449\u0430\u0435\u0442\u0441\u044F, \u043F\u0440\u043E\u0435\u043A\u0446\u0438\u044F \u0441\u043A\u043E\u0440\u043E\u0441\u0442\u0438 \u0432\u0440\u0430\u0449\u0435\u043D\u0438\u044F \u0440\u0430\u0432\u043D\u0430 123 \u043A\u043C/\u0441. \u041F\u043E \u0434\u0430\u043D\u043D\u044B\u043C \u0438\u043D\u0442\u0435\u0440\u0444\u0435\u0440\u043E\u043C\u0435\u0442\u0440\u0438\u0447\u0435\u0441\u043A\u043E\u0433\u043E \u0438\u0437\u043C\u0435\u0440\u0435\u043D\u0438\u044F \u0443\u0433\u043B\u043E\u0432\u043E\u0439 \u0434\u0438\u0430\u043C\u0435\u0442\u0440 \u0437\u0432\u0435\u0437\u0434\u044B \u0441\u043E\u0441\u0442\u0430\u0432\u043B\u044F\u0435\u0442 0,465 \u043C\u0441\u0434, \u0447\u0442\u043E \u043F\u0440\u0438 \u0438\u0437\u0432\u0435\u0441\u0442\u043D\u043E\u043C \u0440\u0430\u0441\u0441\u0442\u043E\u044F\u043D\u0438\u0438 \u0441\u043E\u043E\u0442\u0432\u0435\u0442\u0441\u0442\u0432\u0443\u0435\u0442 \u0440\u0430\u0434\u0438\u0443\u0441\u0443 2,1 \u0440\u0430\u0434\u0438\u0443\u0441\u0430 \u0421\u043E\u043B\u043D\u0446\u0430. \u0421\u0432\u0435\u0442\u0438\u043C\u043E\u0441\u0442\u044C \u0441\u043E\u0441\u0442\u0430\u0432\u043B\u044F\u0435\u0442 26 \u0441\u0432\u0435\u0442\u0438\u043C\u043E\u0441\u0442\u0435\u0439 \u0421\u043E\u043B\u043D\u0446\u0430, \u0442\u0435\u043C\u043F\u0435\u0440\u0430\u0442\u0443\u0440\u0430 \u0432\u043D\u0435\u0448\u043D\u0438\u0445 \u0441\u043B\u043E\u0451\u0432 \u0430\u0442\u043C\u043E\u0441\u0444\u0435\u0440\u044B \u0441\u043E\u0441\u0442\u0430\u0432\u043B\u044F\u0435\u0442 8929 K, \u043F\u0440\u0438 \u044D\u0442\u043E\u043C \u0446\u0432\u0435\u0442 \u0437\u0432\u0435\u0437\u0434\u044B \u044F\u0432\u043B\u044F\u0435\u0442\u0441\u044F \u0431\u0435\u043B\u043E-\u0436\u0451\u043B\u0442\u044B\u043C. \u0412 \u043F\u0440\u043E\u0448\u043B\u043E\u043C \u0431\u044B\u043B\u0438 \u0437\u0430\u043C\u0435\u0447\u0435\u043D\u044B \u0432\u0430\u0440\u0438\u0430\u0446\u0438\u0438 \u043B\u0443\u0447\u0435\u0432\u043E\u0439 \u0441\u043A\u043E\u0440\u043E\u0441\u0442\u0438, \u043D\u043E \u043F\u043E\u0434\u0442\u0432\u0435\u0440\u0436\u0434\u0435\u043D\u0438\u0435 \u043D\u0435 \u0431\u044B\u043B\u043E \u043F\u043E\u043B\u0443\u0447\u0435\u043D\u043E. \u0423 \u0437\u0432\u0435\u0437\u0434\u044B \u043D\u0435\u0442 \u0437\u043D\u0430\u0447\u0438\u0442\u0435\u043B\u044C\u043D\u043E\u0439 \u043F\u0435\u0440\u0435\u043C\u0435\u043D\u043D\u043E\u0441\u0442\u0438 \u0444\u043E\u0442\u043E\u043C\u0435\u0442\u0440\u0438\u0447\u0435\u0441\u043A\u0438\u0445 \u0441\u0432\u043E\u0439\u0441\u0442\u0432, \u043E\u043D\u0430 \u0438\u0441\u043F\u043E\u043B\u044C\u0437\u0443\u0435\u0442\u0441\u044F \u043A\u0430\u043A \u0441\u0442\u0430\u043D\u0434\u0430\u0440\u0442 \u0432 \u0441\u0438\u0441\u0442\u0435\u043C\u0435 UBV. \u041F\u043E \u0434\u0430\u043D\u043D\u044B\u043C \u043D\u0430\u0431\u043B\u044E\u0434\u0435\u043D\u0438\u0439 \u043D\u0430 \u0442\u0435\u043B\u0435\u0441\u043A\u043E\u043F\u0435 Spitzer \u0431\u044B\u043B \u043E\u0431\u043D\u0430\u0440\u0443\u0436\u0435\u043D \u043E\u0441\u0442\u0430\u0442\u043E\u0447\u043D\u044B\u0439 \u0434\u0438\u0441\u043A. \u0421\u0438\u0433\u043C\u0430 \u0410\u043D\u0434\u0440\u043E\u043C\u0435\u0434\u044B \u044F\u0432\u043B\u044F\u0435\u0442\u0441\u044F \u0432\u0435\u0440\u043E\u044F\u0442\u043D\u044B\u043C \u043F\u0440\u0435\u0434\u0441\u0442\u0430\u0432\u0438\u0442\u0435\u043B\u0435\u043C \u043F\u043E\u0442\u043E\u043A\u0430 \u0437\u0432\u0451\u0437\u0434, \u0430\u0441\u0441\u043E\u0446\u0438\u0438\u0440\u0443\u0435\u043C\u043E\u0433\u043E \u0441 \u0434\u0432\u0438\u0436\u0443\u0449\u0435\u0439\u0441\u044F \u0433\u0440\u0443\u043F\u043F\u043E\u0439 \u0437\u0432\u0451\u0437\u0434 \u0411\u043E\u043B\u044C\u0448\u043E\u0439 \u041C\u0435\u0434\u0432\u0435\u0434\u0438\u0446\u044B. \u042D\u0442\u043E \u0433\u0440\u0443\u043F\u043F\u0430 \u0437\u0432\u0451\u0437\u0434, \u043E\u0431\u043B\u0430\u0434\u0430\u044E\u0449\u0438\u0445 \u043F\u043E\u0445\u043E\u0436\u0438\u043C\u0438 \u043F\u0430\u0440\u0430\u043C\u0435\u0442\u0440\u0430\u043C\u0438 \u0434\u0432\u0438\u0436\u0435\u043D\u0438\u044F \u0438, \u0432\u043E\u0437\u043C\u043E\u0436\u043D\u043E, \u043E\u0431\u0449\u0438\u043C \u043F\u0440\u043E\u0438\u0441\u0445\u043E\u0436\u0434\u0435\u043D\u0438\u0435\u043C."@ru . . . "J2000.0"@en . . . . . "1.33"^^ . . . . "main sequence"@en . . "Sigma Andromedae"@de . . . . . . . . . "4.02"^^ . . . "8929"^^ . . . . "\u4ED9\u5973\u5EA7\u03C3\uFF0C\u53C8\u540DBD+35 44\uFF0CHD 1404\u3001SAO 53798\u3001HR 68\uFF0C\u662F\u4ED9\u5973\u5EA7\u7684\u4E00\u9897\u6052\u661F\uFF0C\u89C6\u661F\u7B49\u4E3A4.52\uFF0C\u4F4D\u4E8E\u9280\u7D93115.59\uFF0C\u9280\u7DEF-25.61\uFF0C\u5176B1900.0\u5750\u6807\u4E3A\u8D64\u7D930h 13m 6s\uFF0C\u8D64\u7DEF+36\u00B0 -25.61\u2032 51\u2033\u3002"@zh . . "Sigma Andromedae (\u03C3 Andromedae / \u03C3 And) est une \u00E9toile binaire de la constellation bor\u00E9ale d'Androm\u00E8de. Elle est visible \u00E0 l\u2019\u0153il nu avec une magnitude apparente de 4,51. L'\u00E9toile primaire, Sigma Andromedae A, est une \u00E9toile blanche de la s\u00E9quence principale qui poss\u00E8de un disque de d\u00E9bris en orbite. Son compagnon, Sigma Andromedae B, est une probable naine rouge d\u00E9couverte en 2009."@fr . "1079510782"^^ . . . . . . . "\u20138.0"@en . . . . "\u0421\u0438\u0433\u043C\u0430 \u0410\u043D\u0434\u0440\u043E\u043C\u0435\u0434\u044B (\u043B\u0430\u0442. \u03C3 Andromedae) \u2014 \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. \u0412\u0438\u0434\u0438\u043C\u0430\u044F \u0437\u0432\u0451\u0437\u0434\u043D\u0430\u044F \u0432\u0435\u043B\u0438\u0447\u0438\u043D\u0430 \u0440\u0430\u0432\u043D\u0430 +4.5, \u0437\u0432\u0435\u0437\u0434\u0430 \u0432\u0438\u0434\u043D\u0430 \u043D\u0435\u0432\u043E\u043E\u0440\u0443\u0436\u0451\u043D\u043D\u044B\u043C \u0433\u043B\u0430\u0437\u043E\u043C. \u0418\u0437\u043C\u0435\u0440\u0435\u043D\u0438\u044F \u043F\u0430\u0440\u0430\u043B\u043B\u0430\u043A\u0441\u0430 \u0434\u0430\u043B\u043E \u043E\u0446\u0435\u043D\u043A\u0443 \u0440\u0430\u0441\u0441\u0442\u043E\u044F\u043D\u0438\u044F \u0434\u043E \u0437\u0432\u0435\u0437\u0434\u044B 135 \u0441\u0432\u0435\u0442\u043E\u0432\u044B\u0445 \u043B\u0435\u0442. \u0412\u0438\u0434\u0438\u043C\u044B\u0439 \u0431\u043B\u0435\u0441\u043A \u0437\u0432\u0435\u0437\u0434\u044B \u043E\u0441\u043B\u0430\u0431\u043B\u044F\u0435\u0442\u0441\u044F \u043D\u0430 0,08 \u0432\u0441\u043B\u0435\u0434\u0441\u0442\u0432\u0438\u0435 \u043C\u0435\u0436\u0437\u0432\u0451\u0437\u0434\u043D\u043E\u0439 \u044D\u043A\u0441\u0442\u0438\u043D\u043A\u0446\u0438\u0438. \u0412 \u043F\u0440\u043E\u0448\u043B\u043E\u043C \u0431\u044B\u043B\u0438 \u0437\u0430\u043C\u0435\u0447\u0435\u043D\u044B \u0432\u0430\u0440\u0438\u0430\u0446\u0438\u0438 \u043B\u0443\u0447\u0435\u0432\u043E\u0439 \u0441\u043A\u043E\u0440\u043E\u0441\u0442\u0438, \u043D\u043E \u043F\u043E\u0434\u0442\u0432\u0435\u0440\u0436\u0434\u0435\u043D\u0438\u0435 \u043D\u0435 \u0431\u044B\u043B\u043E \u043F\u043E\u043B\u0443\u0447\u0435\u043D\u043E. \u0423 \u0437\u0432\u0435\u0437\u0434\u044B \u043D\u0435\u0442 \u0437\u043D\u0430\u0447\u0438\u0442\u0435\u043B\u044C\u043D\u043E\u0439 \u043F\u0435\u0440\u0435\u043C\u0435\u043D\u043D\u043E\u0441\u0442\u0438 \u0444\u043E\u0442\u043E\u043C\u0435\u0442\u0440\u0438\u0447\u0435\u0441\u043A\u0438\u0445 \u0441\u0432\u043E\u0439\u0441\u0442\u0432, \u043E\u043D\u0430 \u0438\u0441\u043F\u043E\u043B\u044C\u0437\u0443\u0435\u0442\u0441\u044F \u043A\u0430\u043A \u0441\u0442\u0430\u043D\u0434\u0430\u0440\u0442 \u0432 \u0441\u0438\u0441\u0442\u0435\u043C\u0435 UBV. \u041F\u043E \u0434\u0430\u043D\u043D\u044B\u043C \u043D\u0430\u0431\u043B\u044E\u0434\u0435\u043D\u0438\u0439 \u043D\u0430 \u0442\u0435\u043B\u0435\u0441\u043A\u043E\u043F\u0435 Spitzer \u0431\u044B\u043B \u043E\u0431\u043D\u0430\u0440\u0443\u0436\u0435\u043D \u043E\u0441\u0442\u0430\u0442\u043E\u0447\u043D\u044B\u0439 \u0434\u0438\u0441\u043A."@ru . . . "Sigma Andromedae, Latinized from \u03C3 Andromedae, is the Bayer designation for a single star in the northern constellation of Andromeda. It has an apparent visual magnitude of +4.5, which is bright enough to be seen with the naked eye from most locations. Parallax measurements made during the Gaia mission place it at a distance of about 140 light-years (43 parsecs). The magnitude of the star is diminished by 0.08 from extinction caused by intervening gas and dust. It is drifting closer to the Sun with a radial velocity of \u20138 km/s."@en . . "Sigma d'Andr\u00F2meda"@ca . . . "Sigma d'Andr\u00F2meda (\u03C3 Andromedae) \u00E9s una estrella de la constel\u00B7laci\u00F3 d'Andr\u00F2meda. Sigma d'Andr\u00F2meda \u00E9s una nana de la seq\u00FC\u00E8ncia principal blanca del tipus A de la magnitud aparent +4,51. Est\u00E0 aproximadament a 141 anys-llum de la Terra."@ca . . "+0.05"@en . . "Sigma Andromedae (\u03C3 Andromedae / \u03C3 And) est une \u00E9toile binaire de la constellation bor\u00E9ale d'Androm\u00E8de. Elle est visible \u00E0 l\u2019\u0153il nu avec une magnitude apparente de 4,51. L'\u00E9toile primaire, Sigma Andromedae A, est une \u00E9toile blanche de la s\u00E9quence principale qui poss\u00E8de un disque de d\u00E9bris en orbite. Son compagnon, Sigma Andromedae B, est une probable naine rouge d\u00E9couverte en 2009."@fr . .