. . . . "S0-102"@ru . . . "S0-102\uB294 \uC6B0\uB9AC \uC740\uD558 \uC911\uC2EC\uBD80\uC5D0 \uC788\uB294 \uAC15\uB825\uD55C \uC804\uD30C\uC6D0 \uAD81\uC218\uC790\uB9AC A*\uC640 \uC544\uC8FC \uAC00\uAE4C\uC774 \uC788\uB294 \uD56D\uC131\uC774\uB2E4."@ko . "S0-102 ou S-55 est une \u00E9toile qui se trouve situ\u00E9e tr\u00E8s pr\u00E8s du centre de la Voie lact\u00E9e, en orbite pr\u00E8s de la source radio Sagittarius A*, avec une p\u00E9riode orbitale de 11,5 ans ou de 12,8 ans suivant les sources."@fr . . . . "S0-102"@fr . . . . . . . . "S0-102\uFF0C\u662F\u4E00\u9897\u6052\u661F\uFF0C\u5341\u5206\u9760\u8FD1\u94F6\u6CB3\u7CFB\u4E2D\u5FC3\uFF0C\u5E76\u63A5\u8FD1\u65E0\u7EBF\u7535\u6CE2\u6E90\u4EBA\u9A6C\u5EA7A*\uFF0C\u73AF\u7ED5\u5176\u8FD0\u884C\u7684\u5468\u671F\u4E3A11.5\u5E74\u3002 \u8BE5\u6052\u661F\u4E8E2012\u5E74\u53D1\u73B0\uFF0C\u4E3A\u8FC4\u4ECA\u5DF2\u53D1\u73B0\u7684\u8DDD\u94F6\u6CB3\u7CFB\u4E2D\u5FC3\u9ED1\u6D1E\u6700\u8FD1\u7684\u6052\u661F\uFF0C\u662F\u7531\u6D1B\u6749\u77F6\u52A0\u5DDE\u5927\u5B66\u6559\u6388\uFF08Andrea M. Ghez\uFF09\u9886\u5BFC\u7684\u5C0F\u7EC4\u53D1\u73B0\u7684\u3002 \u51F1\u514B\u5929\u6587\u53F0\u81EA2000\u52302012\u5E74\u9593\u89C0\u6E2CS0-102\u7684\u904B\u52D5\uFF0C\u4E26\u5F97\u77E5\u4E86\u5B83\u4EE5\u9806\u6642\u91DD\u65B9\u5411\u74B0\u7E5E\u4EBA\u9A6C\u5EA7A* \u7684\u5B8C\u6574\u8ECC\u9053\u3002\u89C0\u6E2C\u4EBA\u9A6C\u5EA7A*\u4E2D\u5FC3\u9644\u8FD1\u5169\u9846\u6046\u661F\u5B8C\u6574\u9031\u671F\u7684\u8ECC\u9053\u904B\u52D5\u53EF\u4EE5\u6C42\u5F97\u4EBA\u9A6C\u5EA7A*\u7684\u91CD\u529B\u4F4D\u3002\u800C\u9019\u4E9B\u6046\u661F\u5468\u570D\u53EF\u80FD\u6709\u5927\u91CF\u6697\u7269\u8CEA\u5B58\u5728\u3002\u901A\u8FC7\u7814\u7A76\u8BE5\u6052\u661F\uFF0C\u53EF\u4EE5\u89C2\u5BDF\u8BE5\u6052\u661F\u53D7\u5230\u9ED1\u6D1E\u9644\u8FD1\u626D\u66F2\u65F6\u7A7A\u7684\u5F71\u54CD\uFF0C\u6709\u52A9\u4E8E\u9A8C\u8BC1\u5E7F\u4E49\u76F8\u5BF9\u8BBA\u3002"@zh . . . "S0-102"@de . . . . . . . . "S0-102 ist ein Stern im Galaktischen Zentrum. Er befindet sich in einer Umlaufbahn um die Radioquelle Sagittarius A* und uml\u00E4uft diese einmal in 11,5 \u00B1 0,3 Jahren. Damit unterbietet er den bisherigen Rekordhalter S0-2 um 5 Jahre. Auf seiner Umlaufbahn n\u00E4hert er sich dem Mittelpunkt der Milchstra\u00DFe auf 39 Milliarden Kilometer (260 AE, bzw. 36 Lichtstunden) an und erreicht dabei ca. 1 % der Lichtgeschwindigkeit."@de . . . . . . . "S55 (also known as S0\u2013102) is a star that is located very close to the centre of the Milky Way, near the radio source Sagittarius A*, orbiting it with an orbital period of 12.8 years. Until 2019, when the star S62 became the new record holder, it was the star with the shortest known period orbiting the black hole at the centre of the Milky Way. This beat the record of 16 years previously set by S2. The star was identified by a University of California, Los Angeles team headed by Andrea M. Ghez. At its periapsis, its speed reaches 1.7% of the speed of light. At that point it is 246 astronomical units (34 light hours, 36.7 billion km) from the centre, while the black hole radius is only a small fraction of that size (the Schwarzschild radius is about 0.082 au). It passed that point in 2009 and will be there again in 2022. Its position in the sky has been monitored from 2000 to 2012 using the W. M. Keck telescope and from 2002 to 2016 with the VLT. One complete orbit has been observed. From Earth's current perspective, it travels in a clockwise direction. Having observed two stars orbiting through complete periods around the centre (S55 and S2), the gravitational potential of SgrA* could be established. It is also possible that there is a great deal of dark matter around the orbits of these stars. Also general relativistic effects due to gravitational redshift should become observable."@en . "S0-102"@it . . "S0-102 \u00E8 una stella situata vicino al centro della Via Lattea, in prossimit\u00E0 della radiosorgente e probabile buco nero supermassiccio Sagittarius A*, attorno al quale orbita con un periodo di 11,5 \u00B1 0,3 anni. Il suo cambiamento di posizione apparente \u00E8 stato monitorato dal 2000 al 2012 dai Telescopi Keck, che ne hanno osservato una rivoluzione completa attorno a Sagittarius A*. S0-102 \u00E8, al febbraio 2013, la stella col minimo periodo di rivoluzione attorno al centro galattico (circa 11,5 anni), minore anche di quello della stella S2 (circa 16 anni). Come termine di paragone il Sole ha un periodo di rivoluzione di circa 225 milioni di anni (periodo detto anno galattico)."@it . "S55 (star)"@en . . . . . "S55"@en . . . "S0-102 \u2014 \u0437\u0432\u0435\u0437\u0434\u0430 S-\u043A\u043B\u0430\u0441\u0441\u0430, \u043E\u0431\u0440\u0430\u0449\u0430\u044E\u0449\u0430\u044F\u0441\u044F \u0432\u043E\u043A\u0440\u0443\u0433 \u0440\u0430\u0434\u0438\u043E\u0438\u0441\u0442\u043E\u0447\u043D\u0438\u043A\u0430 \u0421\u0442\u0440\u0435\u043B\u0435\u0446 A* \u2014 \u0441\u0432\u0435\u0440\u0445\u043C\u0430\u0441\u0441\u0438\u0432\u043D\u043E\u0439 \u0447\u0451\u0440\u043D\u043E\u0439 \u0434\u044B\u0440\u044B \u0432 \u0446\u0435\u043D\u0442\u0440\u0435 \u041C\u043B\u0435\u0447\u043D\u043E\u0433\u043E \u041F\u0443\u0442\u0438. \u0417\u0432\u0435\u0437\u0434\u0430, \u043E\u0442\u043A\u0440\u044B\u0442\u0430\u044F \u0432 2012 \u0433\u043E\u0434\u0443, \u0441\u043E\u0432\u0435\u0440\u0448\u0430\u0435\u0442 \u043F\u043E\u043B\u043D\u044B\u0439 \u043E\u0431\u043E\u0440\u043E\u0442 \u0432\u043E\u043A\u0440\u0443\u0433 \u0421\u0442\u0440\u0435\u043B\u044C\u0446\u0430 A* \u0437\u0430 11,5 \u00B1 0,3 \u0433\u043E\u0434\u0430. \u042D\u0442\u043E \u0437\u0432\u0435\u0437\u0434\u0430 \u0438\u043C\u0435\u0435\u0442 \u043E\u0434\u0438\u043D \u0438\u0437 \u0441\u0430\u043C\u044B\u0445 \u043C\u0430\u043B\u044B\u0445 \u043F\u0435\u0440\u0438\u043E\u0434\u043E\u0432 \u043E\u0431\u0440\u0430\u0449\u0435\u043D\u0438\u044F \u0432\u043E\u043A\u0440\u0443\u0433 \u0447\u0451\u0440\u043D\u043E\u0439 \u0434\u044B\u0440\u044B."@ru . "S0-102\uFF0C\u662F\u4E00\u9897\u6052\u661F\uFF0C\u5341\u5206\u9760\u8FD1\u94F6\u6CB3\u7CFB\u4E2D\u5FC3\uFF0C\u5E76\u63A5\u8FD1\u65E0\u7EBF\u7535\u6CE2\u6E90\u4EBA\u9A6C\u5EA7A*\uFF0C\u73AF\u7ED5\u5176\u8FD0\u884C\u7684\u5468\u671F\u4E3A11.5\u5E74\u3002 \u8BE5\u6052\u661F\u4E8E2012\u5E74\u53D1\u73B0\uFF0C\u4E3A\u8FC4\u4ECA\u5DF2\u53D1\u73B0\u7684\u8DDD\u94F6\u6CB3\u7CFB\u4E2D\u5FC3\u9ED1\u6D1E\u6700\u8FD1\u7684\u6052\u661F\uFF0C\u662F\u7531\u6D1B\u6749\u77F6\u52A0\u5DDE\u5927\u5B66\u6559\u6388\uFF08Andrea M. Ghez\uFF09\u9886\u5BFC\u7684\u5C0F\u7EC4\u53D1\u73B0\u7684\u3002 \u51F1\u514B\u5929\u6587\u53F0\u81EA2000\u52302012\u5E74\u9593\u89C0\u6E2CS0-102\u7684\u904B\u52D5\uFF0C\u4E26\u5F97\u77E5\u4E86\u5B83\u4EE5\u9806\u6642\u91DD\u65B9\u5411\u74B0\u7E5E\u4EBA\u9A6C\u5EA7A* \u7684\u5B8C\u6574\u8ECC\u9053\u3002\u89C0\u6E2C\u4EBA\u9A6C\u5EA7A*\u4E2D\u5FC3\u9644\u8FD1\u5169\u9846\u6046\u661F\u5B8C\u6574\u9031\u671F\u7684\u8ECC\u9053\u904B\u52D5\u53EF\u4EE5\u6C42\u5F97\u4EBA\u9A6C\u5EA7A*\u7684\u91CD\u529B\u4F4D\u3002\u800C\u9019\u4E9B\u6046\u661F\u5468\u570D\u53EF\u80FD\u6709\u5927\u91CF\u6697\u7269\u8CEA\u5B58\u5728\u3002\u901A\u8FC7\u7814\u7A76\u8BE5\u6052\u661F\uFF0C\u53EF\u4EE5\u89C2\u5BDF\u8BE5\u6052\u661F\u53D7\u5230\u9ED1\u6D1E\u9644\u8FD1\u626D\u66F2\u65F6\u7A7A\u7684\u5F71\u54CD\uFF0C\u6709\u52A9\u4E8E\u9A8C\u8BC1\u5E7F\u4E49\u76F8\u5BF9\u8BBA\u3002"@zh . . "1096961465"^^ . . . "S55 (also known as S0\u2013102) is a star that is located very close to the centre of the Milky Way, near the radio source Sagittarius A*, orbiting it with an orbital period of 12.8 years. Until 2019, when the star S62 became the new record holder, it was the star with the shortest known period orbiting the black hole at the centre of the Milky Way. This beat the record of 16 years previously set by S2. The star was identified by a University of California, Los Angeles team headed by Andrea M. Ghez. At its periapsis, its speed reaches 1.7% of the speed of light. At that point it is 246 astronomical units (34 light hours, 36.7 billion km) from the centre, while the black hole radius is only a small fraction of that size (the Schwarzschild radius is about 0.082 au). It passed that point in 2009 a"@en . "S0-102"@zh . "S0-102 ist ein Stern im Galaktischen Zentrum. Er befindet sich in einer Umlaufbahn um die Radioquelle Sagittarius A* und uml\u00E4uft diese einmal in 11,5 \u00B1 0,3 Jahren. Damit unterbietet er den bisherigen Rekordhalter S0-2 um 5 Jahre. Auf seiner Umlaufbahn n\u00E4hert er sich dem Mittelpunkt der Milchstra\u00DFe auf 39 Milliarden Kilometer (260 AE, bzw. 36 Lichtstunden) an und erreicht dabei ca. 1 % der Lichtgeschwindigkeit. Die Beobachtung von S0-102 erfolgte \u00FCber mehr als einen Umlaufzyklus von 1995 bis 2012 am Keck-Observatorium mit Hilfe von adaptiver Optik und Speckle-Interferometrie. Da er 16-mal lichtschw\u00E4cher ist als der (ohnehin schwer zu beobachtende) Stern S0-2, konnte man ihn erst sp\u00E4t vom Infrarothintergrund unterscheiden. Er war nach S0-2 der zweite Stern, dessen Orbit um das supermassereiche Schwarze Loch Sagittarius A* sehr genau vermessen werden konnte."@de . "17.2"^^ . . "S0-102 \u00E8 una stella situata vicino al centro della Via Lattea, in prossimit\u00E0 della radiosorgente e probabile buco nero supermassiccio Sagittarius A*, attorno al quale orbita con un periodo di 11,5 \u00B1 0,3 anni. Il suo cambiamento di posizione apparente \u00E8 stato monitorato dal 2000 al 2012 dai Telescopi Keck, che ne hanno osservato una rivoluzione completa attorno a Sagittarius A*. S0-102 \u00E8, al febbraio 2013, la stella col minimo periodo di rivoluzione attorno al centro galattico (circa 11,5 anni), minore anche di quello della stella S2 (circa 16 anni)."@it . . . "S0-102"@ko . . . . . . "S0-102 ou S-55 est une \u00E9toile qui se trouve situ\u00E9e tr\u00E8s pr\u00E8s du centre de la Voie lact\u00E9e, en orbite pr\u00E8s de la source radio Sagittarius A*, avec une p\u00E9riode orbitale de 11,5 ans ou de 12,8 ans suivant les sources."@fr . "37240862"^^ . . . "5474"^^ . . "S0-102\uB294 \uC6B0\uB9AC \uC740\uD558 \uC911\uC2EC\uBD80\uC5D0 \uC788\uB294 \uAC15\uB825\uD55C \uC804\uD30C\uC6D0 \uAD81\uC218\uC790\uB9AC A*\uC640 \uC544\uC8FC \uAC00\uAE4C\uC774 \uC788\uB294 \uD56D\uC131\uC774\uB2E4."@ko . . "Sagittarius A*"@en . "S0-102 \u2014 \u0437\u0432\u0435\u0437\u0434\u0430 S-\u043A\u043B\u0430\u0441\u0441\u0430, \u043E\u0431\u0440\u0430\u0449\u0430\u044E\u0449\u0430\u044F\u0441\u044F \u0432\u043E\u043A\u0440\u0443\u0433 \u0440\u0430\u0434\u0438\u043E\u0438\u0441\u0442\u043E\u0447\u043D\u0438\u043A\u0430 \u0421\u0442\u0440\u0435\u043B\u0435\u0446 A* \u2014 \u0441\u0432\u0435\u0440\u0445\u043C\u0430\u0441\u0441\u0438\u0432\u043D\u043E\u0439 \u0447\u0451\u0440\u043D\u043E\u0439 \u0434\u044B\u0440\u044B \u0432 \u0446\u0435\u043D\u0442\u0440\u0435 \u041C\u043B\u0435\u0447\u043D\u043E\u0433\u043E \u041F\u0443\u0442\u0438. \u0417\u0432\u0435\u0437\u0434\u0430, \u043E\u0442\u043A\u0440\u044B\u0442\u0430\u044F \u0432 2012 \u0433\u043E\u0434\u0443, \u0441\u043E\u0432\u0435\u0440\u0448\u0430\u0435\u0442 \u043F\u043E\u043B\u043D\u044B\u0439 \u043E\u0431\u043E\u0440\u043E\u0442 \u0432\u043E\u043A\u0440\u0443\u0433 \u0421\u0442\u0440\u0435\u043B\u044C\u0446\u0430 A* \u0437\u0430 11,5 \u00B1 0,3 \u0433\u043E\u0434\u0430. \u042D\u0442\u043E \u0437\u0432\u0435\u0437\u0434\u0430 \u0438\u043C\u0435\u0435\u0442 \u043E\u0434\u0438\u043D \u0438\u0437 \u0441\u0430\u043C\u044B\u0445 \u043C\u0430\u043B\u044B\u0445 \u043F\u0435\u0440\u0438\u043E\u0434\u043E\u0432 \u043E\u0431\u0440\u0430\u0449\u0435\u043D\u0438\u044F \u0432\u043E\u043A\u0440\u0443\u0433 \u0447\u0451\u0440\u043D\u043E\u0439 \u0434\u044B\u0440\u044B."@ru . . .