. . . . . "Sagittarius A* (w skr\u00F3cie Sgr A*) \u2013 obiekt astronomiczny, kt\u00F3ry jest jasnym i bardzo zwartym \u017Ar\u00F3d\u0142em radiowym w centrum Drogi Mlecznej, cz\u0119\u015Bci\u0105 wi\u0119kszej struktury astronomicznej (Sagittarius A). Odleg\u0142o\u015B\u0107 do \u017Ar\u00F3d\u0142a wynosi oko\u0142o 8 kpc (2,4\u00D71017 km). Radio\u017Ar\u00F3d\u0142o zawiera supermasywn\u0105 czarn\u0105 dziur\u0119 ci\u0119\u017Csz\u0105 od S\u0142o\u0144ca oko\u0142o 4,31\u00B10,06 miliona razy (masa S\u0142o\u0144ca to oko\u0142o 2\u00D71030 kg). Jej promie\u0144 oszacowano na oko\u0142o p\u00F3\u0142 minuty \u015Bwietlnej (0,06 j.a.) - trzynastokrotno\u015B\u0107 promienia S\u0142o\u0144ca. Badania wskazuj\u0105 r\u00F3wnie\u017C, \u017Ce czarna dziura zwi\u0119kszy\u0142a swoj\u0105 mas\u0119 2 do 4 razy w ci\u0105gu ostatnich 5-10 miliard\u00F3w lat, poprzez poch\u0142anianie pobliskich gwiazd."@pl . . . . "Sagittarius A* (diucapkan \"Sagittarius A-star\", biasa disingkat Sgr A*) adalah sebuah lubang hitam supermasif di Pusat Galaksi Bima Sakti. Sgr A* terletak dekat perbatasan rasi bintang Sagittarius dan Scorpius, kira-kira 5,6\u00B0 selatan ekliptika, dan tampak dekat Gugus Kupu-kupu (M6) dan . Reinhard Genzel dan Andrea Ghez menerima Penghargaan Nobel Fisika 2020 untuk menemukan bahwa Sgr A* adalah objek supermasif dan padat, dimana lubang hitam adalah satu-satunya penjelasan yang masuk akal pada saat itu."@in . . . . . . . . . . . . . . . . . . "\uAD81\uC218\uC790\uB9AC A*(\uC601\uC5B4: Sagittarius A*, Sgr A*, \"\uAD81\uC218\uC790\uB9AC A\uBCC4\"\uB85C \uBC1C\uC74C)\uC740 \uAD81\uC218\uC790\uB9AC\uC640 \uC804\uAC08\uC790\uB9AC \uACBD\uACC4 \uADFC\uCC98, \uC6B0\uB9AC \uC740\uD558\uC758 \uC911\uC2EC\uC5D0 \uC788\uB294 \uBC1D\uACE0 \uC791\uC740 \uC804\uD30C\uC6D0\uC774\uB2E4. \uC774\uB294 \uB85C \uC54C\uB824\uC838 \uC788\uB294 \uB354 \uD070 \uC804\uD30C\uC6D0\uC758 \uC77C\uBD80\uC774\uB2E4. \uAD81\uC218\uC790\uB9AC A*\uC740 \uC77C\uBC18\uC801\uC73C\uB85C \uB300\uBD80\uBD84\uC758 \uB098\uC120 \uC740\uD558\uC640 \uD0C0\uC6D0 \uC740\uD558\uC758 \uC911\uC2EC\uC5D0 \uC788\uC744 \uAC83\uC73C\uB85C \uBC1B\uC544\uB4E4\uC5EC\uC9C0\uB294, \uCD08\uB300\uC9C8\uB7C9 \uBE14\uB799\uD640\uC77C \uAC83\uC73C\uB85C \uC5EC\uACA8\uC9C0\uACE0 \uC788\uB2E4. \uAD81\uC218\uC790\uB9AC A* \uC8FC\uBCC0\uC744 \uACF5\uC804\uD558\uB294 \uBCC4 S2\uC758 \uAD00\uCE21\uC740 \uC6B0\uB9AC \uC740\uD558\uC758 \uC911\uC2EC \uBE14\uB799\uD640\uC758 \uC874\uC7AC\uB97C \uBCF4\uC5EC\uC8FC\uACE0, \uADF8\uC5D0 \uB300\uD55C \uB370\uC774\uD130\uB97C \uB9CC\uB4DC\uB294\uB370 \uC774\uC6A9\uB418\uBA70, \uC774\uB294 \uAD81\uC218\uC790\uB9AC A*\uC774 \uADF8 \uBE14\uB799\uD640\uC758 \uC704\uCE58\uB77C\uB294 \uACB0\uB860\uC73C\uB85C \uC720\uB3C4\uB41C\uB2E4."@ko . . . "Sagittarius A*"@pl . "Sagittarius A* (prononcata Sagittarius A stelo; mallongigite Sgr A*; la\u016D la latina nomo de la stela konstelacio Sagitario, do principe anka\u016D esperantigebla Sagitario A*) estas regiono de la kosmo en la konstelacio Sagitario. Temas pri fonto de radioondoj en la hipoteza centro de la galaksio Lakta Vojo. Sgr A*, estis malkovrita la 13-an kaj 15-an de februaro 1974 fare de astronomoj Bruce Balick kaj Robert Brown uzante la bazlinian interferometron (en Socorro) de la . La nomo Sgr A* estis elpensita fare de Brown en artikolo de 1982, \u0109ar la radiofonto estis \"ekscita\", kaj ekscititaj statoj de atomoj estas indikitaj per asteriskoj. Ekde la 1980-aj jaroj, ver\u015Dajnas ke la centra komponanto de Sgr A* estas nigra truo. En 1994, infraru\u011Daj kaj submilimetraj spektroskopiostudoj de Berkeley-teamo imp"@eo . . . . . . . . . "Sagittarius A* Esne Bidearen erdialdean dagoen zulo beltz supermasibo bat da."@eu . . . "Sagittarius A*"@nl . . . . . "A simulation of how a gas cloud that has been observed approaching the supermassive black hole at the centre of the galaxy.jpg"@en . . "Sagittarius A* (gesprochen: Sagittarius A Stern; abgek\u00FCrzt: Sgr A*; eine Region im Sternbild Sch\u00FCtze) ist eine Quelle von Radiowellen im Zentrum der Milchstra\u00DFe. Nach derzeitigem radioastronomischen Forschungsstand handelt es sich dabei um ein supermassereiches Schwarzes Loch von 4,154 \u00B1 0,014 Millionen Sonnenmassen, das 26.673 \u00B1 42 Lichtjahre (8.178 \u00B1 13 pc) von der Sonne entfernt ist. Der Durchmesser seines Ereignishorizonts (20 \u03BCas, Mikrobogensekunden) entspricht mit 24,5 Mio. km etwa 21 % des Bahndurchmessers des Merkur auf seiner Umlaufbahn um die Sonne. Mit der Entdeckung der Fermi-Blasen im Jahre 2010 und ihren m\u00F6glichen Pendants im R\u00F6ntgenlicht, den \u201EeROSITA-Blasen\u201C 2019 ergeben sich Hinweise darauf, dass Sagittarius A* vor langer Zeit aktiv gewesen war und die Milchstra\u00DFe somit eine aktive Galaxie gewesen sein k\u00F6nnte."@de . "center"@en . . . . . . . . "Sagittarius A*"@en . . "\u0421\u0442\u0440\u0435\u043B\u0435\u0446 A*"@ru . . . "15"^^ . . . . "Sagittarius A*, ook wel bekend als Sgr A*, is een superzwaar zwart gat en een radiobron in het centrum van de Melkweg. Het object bevindt zich in de samengestelde radiobron Sagittarius A op 26.673 lichtjaar van de Zon. Het bevat 4,15 miljoen zonsmassa's in een gebied met een radius van minder dan 6,25 lichtuur. Het is daarmee het zwaarste zwarte gat in de Melkweg (andere zwarte gaten in de Melkweg zijn stellair)."@nl . "\u3044\u3066\u5EA7A*\uFF08\u3044\u3066\u3056\u30A8\u30FC\u30FB\u30B9\u30BF\u30FC\u3001\u7565\u53F7Sgr A*\uFF09\u306F\u3001\u5929\u306E\u5DDD\u9280\u6CB3\u306E\u4E2D\u5FC3\u306B\u3042\u308B\u660E\u308B\u304F\u30B3\u30F3\u30D1\u30AF\u30C8\u306A\u5929\u6587\u96FB\u6CE2\u6E90\u3002\u3088\u308A\u5927\u898F\u6A21\u306A\u69CB\u9020\u306E\u96FB\u6CE2\u6E90\u9818\u57DF\u3067\u3042\u308B\u3044\u3066\u5EA7A\u306E\u4E00\u90E8\u3067\u3042\u308B\u3002\u3044\u3066\u5EA7A*\u306E\u4F4D\u7F6E\u306B\u306F\u8D85\u5927\u8CEA\u91CF\u30D6\u30E9\u30C3\u30AF\u30DB\u30FC\u30EB\u304C\u5B58\u5728\u3059\u308B\u3068\u8003\u3048\u3089\u308C\u3001\u591A\u304F\u306E\u6E26\u5DFB\u9280\u6CB3\u3084\u6955\u5186\u9280\u6CB3\u306E\u4E2D\u5FC3\u306B\u3082\u540C\u3058\u3088\u3046\u306B\u8D85\u5927\u8CEA\u91CF\u30D6\u30E9\u30C3\u30AF\u30DB\u30FC\u30EB\u304C\u3042\u308B\u3068\u3044\u3046\u306E\u304C\u5B9A\u8AAC\u3068\u306A\u3063\u3066\u3044\u308B\u3002\u3044\u3066\u5EA7A*\u306E\u5468\u56F2\u3092\u516C\u8EE2\u3057\u3066\u3044\u308B\u6052\u661FS2\u306E\u89B3\u6E2C\u306B\u3088\u3063\u3066\u3001\u9280\u6CB3\u7CFB\u4E2D\u5FC3\u306B\u8D85\u5927\u8CEA\u91CF\u30D6\u30E9\u30C3\u30AF\u30DB\u30FC\u30EB\u304C\u5B58\u5728\u3059\u308B\u8A3C\u62E0\u3068\u3001\u30D6\u30E9\u30C3\u30AF\u30DB\u30FC\u30EB\u306B\u95A2\u3059\u308B\u30C7\u30FC\u30BF\u304C\u3082\u305F\u3089\u3055\u308C\u3001\u3044\u3066\u5EA7A*\u304C\u305D\u306E\u5B58\u5728\u4F4D\u7F6E\u3067\u3042\u308B\u3068\u3044\u3046\u7D50\u8AD6\u306B\u306A\u3063\u3066\u3044\u305F\u304C\u30012022\u5E745\u670812\u65E5\u3001\u30D6\u30E9\u30C3\u30AF\u30DB\u30FC\u30EB\u306E\u76F4\u63A5\u89B3\u6E2C\u3092\u76EE\u6307\u3059\u56FD\u969B\u30D7\u30ED\u30B8\u30A7\u30AF\u30C8\u30A4\u30D9\u30F3\u30C8\u30DB\u30E9\u30A4\u30BA\u30F3\u30C6\u30EC\u30B9\u30B3\u30FC\u30D7 (EHT) \u306B\u3088\u308A\u3001\u3044\u3066\u5EA7A*\u306B\u5B58\u5728\u3059\u308B\u8D85\u5927\u8CEA\u91CF\u30D6\u30E9\u30C3\u30AF\u30DB\u30FC\u30EB\u306E\u76F4\u63A5\u89B3\u6E2C\u306B\u6210\u529F\u3057\u305F\u3068\u767A\u8868\u3055\u308C\u305F\u3002\u30D6\u30E9\u30C3\u30AF\u30DB\u30FC\u30EB\u306E\u76F4\u63A5\u89B3\u6E2C\u306B\u6210\u529F\u3057\u305F\u306E\u306FM87\u306E\u4E2D\u5FC3\u306B\u3042\u308B\u8D85\u5927\u8CEA\u91CF\u30D6\u30E9\u30C3\u30AF\u30DB\u30FC\u30EB\u306B\u6B21\u3044\u3067\u89B3\u6E2C\u53F2\u4E0A2\u4F8B\u76EE\u3067\u3042\u308B\u3002"@ja . . . . . . . . . . . . . . "Sagittarius A*"@eu . . . . . "Sagittarius A* (abr\u00E9g\u00E9 en Sgr A*) est une source intense d'ondes radio, situ\u00E9e dans la direction de la constellation zodiacale du Sagittaire (coordonn\u00E9es J2000 : ascension droite 17h 45m 40,045s, d\u00E9clinaison -29,00775\u00B0) et localis\u00E9e au centre de la Voie lact\u00E9e, \u00E0 environ 8 178 parsecs (26 673 ann\u00E9es-lumi\u00E8re) du Syst\u00E8me solaire. Initialement non r\u00E9solue au sein d'une zone d'\u00E9mission radio plus vaste d\u00E9nomm\u00E9e Sagittarius A, elle est par la suite distingu\u00E9e de l'ensemble des sources formant cette zone d'\u00E9mission, dont Sgr A Est et Sgr A Ouest. L'utilisation de l'ast\u00E9risque dans son nom signifie que, contrairement \u00E0 Sgr A Est et Sgr A Ouest, il s'agit d'une source quasi ponctuelle et non \u00E9tendue. La radiosource Sgr A* est aujourd'hui consid\u00E9r\u00E9e comme associ\u00E9e \u00E0 un trou noir supermassif d'environ 4,152 millions de masses solaires situ\u00E9 au centre de notre galaxie. Ce trou noir est l'objet primaire d'un amas stellaire. La douzaine d'\u00E9toiles connues composant cet amas est en orbite autour du trou noir."@fr . . "\uAD81\uC218\uC790\uB9AC A*"@ko . "\u0421\u0442\u0440\u0435\u043B\u0435\u0446 A* (\u043B\u0430\u0442. Sagittarius A*, Sgr A*; \u043F\u0440\u043E\u0438\u0437\u043D\u043E\u0441\u0438\u0442\u0441\u044F \u00AB\u0421\u0442\u0440\u0435\u043B\u0435\u0301\u0446 \u0410 \u0441\u043E \u0437\u0432\u0451\u0437\u0434\u043E\u0447\u043A\u043E\u0439\u00BB) \u2014 \u043A\u043E\u043C\u043F\u0430\u043A\u0442\u043D\u044B\u0439 \u0440\u0430\u0434\u0438\u043E\u0438\u0441\u0442\u043E\u0447\u043D\u0438\u043A, \u043D\u0430\u0445\u043E\u0434\u044F\u0449\u0438\u0439\u0441\u044F \u0432 \u0446\u0435\u043D\u0442\u0440\u0435 \u041C\u043B\u0435\u0447\u043D\u043E\u0433\u043E \u041F\u0443\u0442\u0438, \u0432\u0445\u043E\u0434\u0438\u0442 \u0432 \u0441\u043E\u0441\u0442\u0430\u0432 \u0440\u0430\u0434\u0438\u043E\u0438\u0441\u0442\u043E\u0447\u043D\u0438\u043A\u0430 \u0421\u0442\u0440\u0435\u043B\u0435\u0446 \u0410. \u0418\u0437\u043B\u0443\u0447\u0430\u0435\u0442 \u0442\u0430\u043A\u0436\u0435 \u0432 \u0438\u043D\u0444\u0440\u0430\u043A\u0440\u0430\u0441\u043D\u043E\u043C, \u0440\u0435\u043D\u0442\u0433\u0435\u043D\u043E\u0432\u0441\u043A\u043E\u043C \u0438 \u0434\u0440\u0443\u0433\u0438\u0445 \u0434\u0438\u0430\u043F\u0430\u0437\u043E\u043D\u0430\u0445. \u041F\u0440\u0435\u0434\u0441\u0442\u0430\u0432\u043B\u044F\u0435\u0442 \u0441\u043E\u0431\u043E\u0439 \u0432\u044B\u0441\u043E\u043A\u043E\u043F\u043B\u043E\u0442\u043D\u044B\u0439 \u043E\u0431\u044A\u0435\u043A\u0442 \u2014 \u0441\u0432\u0435\u0440\u0445\u043C\u0430\u0441\u0441\u0438\u0432\u043D\u0443\u044E \u0447\u0451\u0440\u043D\u0443\u044E \u0434\u044B\u0440\u0443, \u043E\u043A\u0440\u0443\u0436\u0451\u043D\u043D\u0443\u044E \u0433\u043E\u0440\u044F\u0447\u0438\u043C \u0440\u0430\u0434\u0438\u043E\u0438\u0437\u043B\u0443\u0447\u0430\u044E\u0449\u0438\u043C \u0433\u0430\u0437\u043E\u0432\u044B\u043C \u043E\u0431\u043B\u0430\u043A\u043E\u043C \u0434\u0438\u0430\u043C\u0435\u0442\u0440\u043E\u043C \u043E\u043A\u043E\u043B\u043E 1,8 \u043F\u043A. \u0420\u0430\u0441\u0441\u0442\u043E\u044F\u043D\u0438\u0435 \u0434\u043E \u0440\u0430\u0434\u0438\u043E\u0438\u0441\u0442\u043E\u0447\u043D\u0438\u043A\u0430 \u0441\u043E\u0441\u0442\u0430\u0432\u043B\u044F\u0435\u0442 (27,00 \u00B1 0,10) \u0442\u044B\u0441. \u0441\u0432. \u043B\u0435\u0442, \u043C\u0430\u0441\u0441\u0430 \u0446\u0435\u043D\u0442\u0440\u0430\u043B\u044C\u043D\u043E\u0433\u043E \u043E\u0431\u044A\u0435\u043A\u0442\u0430 \u0440\u0430\u0432\u043D\u0430 (4,297 \u00B1 0,042) \u043C\u043B\u043D M\u2299. \u0414\u0430\u043D\u043D\u044B\u0435 \u0441 \u0440\u0430\u0434\u0438\u043E\u0442\u0435\u043B\u0435\u0441\u043A\u043E\u043F\u0430 VLBA \u0441\u0432\u0438\u0434\u0435\u0442\u0435\u043B\u044C\u0441\u0442\u0432\u0443\u044E\u0442, \u0447\u0442\u043E \u043D\u0435\u043F\u043E\u0441\u0440\u0435\u0434\u0441\u0442\u0432\u0435\u043D\u043D\u043E \u043D\u0430 \u0434\u043E\u043B\u044E \u0441\u0430\u043C\u043E\u0439 \u0447\u0451\u0440\u043D\u043E\u0439 \u0434\u044B\u0440\u044B \u043F\u0440\u0438\u0445\u043E\u0434\u0438\u0442\u0441\u044F \u043C\u0438\u043D\u0438\u043C\u0443\u043C \u0447\u0435\u0442\u0432\u0435\u0440\u0442\u044C \u043E\u0442 \u043E\u0431\u0449\u0435\u0439 \u043C\u0430\u0441\u0441\u044B \u043E\u0431\u044A\u0435\u043A\u0442\u0430 Sgr A*, \u0430 \u043E\u0441\u0442\u0430\u043B\u044C\u043D\u0430\u044F \u0447\u0430\u0441\u0442\u044C \u043C\u0430\u0441\u0441\u044B \u043F\u0440\u0438\u0445\u043E\u0434\u0438\u0442\u0441\u044F \u043D\u0430 \u043E\u043A\u0440\u0443\u0436\u0430\u044E\u0449\u0443\u044E \u0447\u0451\u0440\u043D\u0443\u044E \u0434\u044B\u0440\u0443 \u043C\u0430\u0442\u0435\u0440\u0438\u044E, \u0430 \u0442\u0430\u043A\u0436\u0435 \u0441\u043E\u0441\u0435\u0434\u043D\u0438\u0435 \u0441 \u043D\u0435\u0439 \u0437\u0432\u0451\u0437\u0434\u044B \u0438 \u043E\u0431\u043B\u0430\u043A\u0430 \u0433\u0430\u0437\u0430. 12 \u043C\u0430\u044F 2022 \u0433\u043E\u0434\u0430 \u0430\u0441\u0442\u0440\u043E\u043D\u043E\u043C\u044B, \u043F\u0440\u043E\u0432\u043E\u0434\u0438\u0432\u0448\u0438\u0435 \u043D\u0430\u0431\u043B\u044E\u0434\u0435\u043D\u0438\u044F \u0441 \u043F\u043E\u043C\u043E\u0449\u044C\u044E \u0422\u0435\u043B\u0435\u0441\u043A\u043E\u043F\u0430 \u0433\u043E\u0440\u0438\u0437\u043E\u043D\u0442\u0430 \u0441\u043E\u0431\u044B\u0442\u0438\u0439, \u043E\u043F\u0443\u0431\u043B\u0438\u043A\u043E\u0432\u0430\u043B\u0438 \u0444\u043E\u0442\u043E\u0433\u0440\u0430\u0444\u0438\u044E \u0421\u0442\u0440\u0435\u043B\u044C\u0446\u0430 \u0410*, \u043F\u043E\u0434\u0442\u0432\u0435\u0440\u0434\u0438\u0432, \u0447\u0442\u043E \u043E\u0431\u044A\u0435\u043A\u0442 \u0441\u043E\u0434\u0435\u0440\u0436\u0438\u0442 \u0447\u0451\u0440\u043D\u0443\u044E \u0434\u044B\u0440\u0443. \u042D\u0442\u043E \u0432\u0442\u043E\u0440\u043E\u0435 \u043F\u043E\u0434\u0442\u0432\u0435\u0440\u0436\u0434\u0451\u043D\u043D\u043E\u0435 \u0438\u0437\u043E\u0431\u0440\u0430\u0436\u0435\u043D\u0438\u0435 \u0447\u0451\u0440\u043D\u043E\u0439 \u0434\u044B\u0440\u044B."@ru . "Sagittarius A* (Sgr A*; i stj\u00E4rnbilden Skytten) \u00E4r en ljusstark och extremt kompakt radiok\u00E4lla i Vintergatans centrum, och \u00E4r en del av objektgruppen . Centrum f\u00F6r v\u00E5r galax befinner sig ca 26 000 ljus\u00E5r fr\u00E5n jorden."@sv . . . . . . . "Sagittarius A* (/\u02C8e\u026A st\u0251\u02D0r/ AY star), abbreviated Sgr A* (/\u02C8s\u00E6d\u0292 \u02C8e\u026A st\u0251\u02D0r/ SAJ AY star), is the supermassive black hole at the Galactic Center of the Milky Way. It is located near the border of the constellations Sagittarius and Scorpius, about 5.6\u00B0 south of the ecliptic, visually close to the Butterfly Cluster (M6) and Lambda Scorpii. The object is a bright and very compact astronomical radio source. The name Sagittarius A* follows from historical reasons. In 1954, John D. Kraus, Hsien-Ching Ko, and Sean Matt listed the radio sources they identified with the Ohio State University radio telescope at 250 MHz. The sources were arranged by constellation and the letter assigned to them was arbitrary, with A denoting the brightest radio source within the constellation. The asterisk * is because its discovery was considered \"exciting\", in parallel with the nomenclature for excited state atoms which are denoted with an asterisk (e.g. the excited state of Helium would be He*). The asterisk was assigned in 1982 by Robert L. Brown, who understood that the strongest radio emission from the center of the galaxy appeared to be due to a compact nonthermal radio object. The observations of several stars orbiting Sagittarius A*, particularly star S2, have been used to determine the mass and upper limits on the radius of the object. Based on mass and increasingly precise radius limits, astronomers have concluded that Sagittarius A* must be the Milky Way's central supermassive black hole. The current value of its mass is 4.154\u00B10.014 million solar masses. Reinhard Genzel and Andrea Ghez were awarded the 2020 Nobel Prize in Physics for their discovery that Sagittarius A* is a supermassive compact object, for which a black hole was the only plausible explanation at the time. On May 12, 2022, astronomers, using the Event Horizon Telescope, released the first image of the accretion disk around the horizon of Sagittarius A* produced using a world-wide network of radio observatories made in April 2017, confirming the object to be a black hole. This is the second confirmed image of a black hole, after Messier 87's supermassive black hole in 2019."@en . . . . . . . . . . . . "Sagittarius A* (diucapkan \"Sagittarius A-star\", biasa disingkat Sgr A*) adalah sebuah lubang hitam supermasif di Pusat Galaksi Bima Sakti. Sgr A* terletak dekat perbatasan rasi bintang Sagittarius dan Scorpius, kira-kira 5,6\u00B0 selatan ekliptika, dan tampak dekat Gugus Kupu-kupu (M6) dan . Observasi beberapa bintang yang mengorbit Sagittarius A*, terutama bintang , digunakan untuk mementukan massa dan batas maksimum radius objek. Berdasarkan massa dan batas radius yang semakin presisi, para astronom menarik kesimpulan bahwa Sagittarius A* adalah lubang hitam supermasif di pusat Bima Sakti. Nilai massanya saat ini adalah 4,154 (\u00B1 0,014) juta massa Matahari. Reinhard Genzel dan Andrea Ghez menerima Penghargaan Nobel Fisika 2020 untuk menemukan bahwa Sgr A* adalah objek supermasif dan padat, dimana lubang hitam adalah satu-satunya penjelasan yang masuk akal pada saat itu. Pada 12 Mei 2022, menggunakan Teleskop Event Horizon, para astronom merilis foto Sagittarius A* yang menggunakan data dari observasi radio pada April 2017, dan memastikan bahwa objek ini adalah lubang hitam. Ini adalah gambar terkonfirmasi lubang hitam kedua, setelah foto lubang hitam supermasif Messier 87 pada tahun 2019."@in . . . . . . . . "Sagittarius A*"@sv . . "Sagittarius A* (abbreviato in Sgr A*) \u00E8 una sorgente di onde radio molto luminosa, situata nel centro della Via Lattea, parte della grande struttura nota come Sagittarius A. Sgr A* \u00E8 il punto in cui si trova un buco nero supermassiccio, componente caratteristico dei centri di molte galassie ellittiche e spirali. Sagittarius A* avrebbe una massa di circa 4 milioni di volte quella del Sole e, trovandosi nel centro della nostra galassia, costituirebbe il corpo celeste attorno a cui tutte le stelle della Via Lattea, compresa la nostra, compiono il loro moto di rivoluzione."@it . . . . . . . "Sagittarius A* (abr\u00E9g\u00E9 en Sgr A*) est une source intense d'ondes radio, situ\u00E9e dans la direction de la constellation zodiacale du Sagittaire (coordonn\u00E9es J2000 : ascension droite 17h 45m 40,045s, d\u00E9clinaison -29,00775\u00B0) et localis\u00E9e au centre de la Voie lact\u00E9e, \u00E0 environ 8 178 parsecs (26 673 ann\u00E9es-lumi\u00E8re) du Syst\u00E8me solaire. Initialement non r\u00E9solue au sein d'une zone d'\u00E9mission radio plus vaste d\u00E9nomm\u00E9e Sagittarius A, elle est par la suite distingu\u00E9e de l'ensemble des sources formant cette zone d'\u00E9mission, dont Sgr A Est et Sgr A Ouest. L'utilisation de l'ast\u00E9risque dans son nom signifie que, contrairement \u00E0 Sgr A Est et Sgr A Ouest, il s'agit d'une source quasi ponctuelle et non \u00E9tendue."@fr . "\u4EBA\u99AC\u5EA7A*\uFF08Sagittarius A*\uFF0C\u7C21\u5BEB\u70BASgr A*\uFF0C\u661F\u865F*\u8B80\u4F5C\u300Cstar\u300D\u6216\u300C\u661F\u300D\uFF09\u662F\u500B\u4F4D\u65BC\u9280\u6CB3\u7CFB\u4E2D\u5FC3\u7684\u8D85\u5927\u8CEA\u91CF\u9ED1\u6D1E\u3002\u5B83\u4F4D\u65BC\u661F\u5EA7\u4EBA\u99AC\u5EA7\u548C\u5929\u880D\u5EA7\u7684\u908A\u754C\u9644\u8FD1\uFF0C\u5927\u7D04\u4F4D\u65BC\u9EC3\u9053\u4EE5\u53575.6\u00B0\uFF0C\u8996\u89BA\u4E0A\u63A5\u8FD1\u8774\u8776\u661F\u5718\uFF08M6\uFF09\u548C\u5C3E\u5BBF\u516B\uFF08\u5929\u880D\u5EA7\u03BB\uFF09\u3002 \u9019\u9846\u5929\u9AD4\u662F\u660E\u4EAE\u7DFB\u5BC6\u7684\u96FB\u6CE2\u6E90\u3002\u4EBA\u99AC\u5EA7A*\u7684\u540D\u5B57\u6709\u5176\u6B77\u53F2\u6DF5\u6E90\u3002\u5728 1954\u5E74\uFF0C\u7D04\u7FF0\u00B7\u4E39\u5C3C\u723E\u00B7\u514B\u52DE\u65AF\u3001\u67EF\u8CE2\u6E05\uFF08Hsien-Ching Ko\uFF09\u548C\u8096\u6069\u00B7\u99AC\u7279\uFF08Sean Matt\uFF09\u5217\u51FA\u4E86\u4ED6\u5011\u7528\u4FC4\u4EA5\u4FC4\u5DDE\u7ACB\u5927\u5B78\u96FB\u6CE2\u671B\u9060\u93E1\u5728250MHz\u4E0B\u78BA\u5B9A\u7684\u96FB\u6CE2\u6E90\u3002\u9019\u4E9B\u96FB\u6CE2\u6E90\u6309\u661F\u5EA7\u6392\u5217\uFF0C\u4E26\u96A8\u610F\u7684\u5206\u914D\u5B57\u6BCD\u4F86\u6A19\u793A\uFF0C\u4F46\u5B57\u6BCDA\u901A\u5E38\u8868\u793A\u661F\u5EA7\u5167\u6700\u4EAE\u7684\u96FB\u6CE2\u6E90\u3002\u661F\u865F * \u662F\u56E0\u70BA\u5B83\u7684\u767C\u73FE\u88AB\u8A8D\u70BA\u662F\"\u4EE4\u4EBA\u8208\u596E\u7684\"\u3002\u9019\u8207\u7528\u661F\u865F\u8868\u793A\u6FC0\u767C\u614B\u539F\u5B50\u7684\u547D\u540D\u6CD5\u4E00\u81F4\uFF08\u4F8B\u5982\uFF0C\u6C26\u7684\u6FC0\u767C\u614B\u70BAHe*\uFF09\u3002\u661F\u865F\u662F\u7F85\u4F2F\u7279\u00B7L\u00B7\u5E03\u6717\u65BC1982\u5E74\u8A2D\u7F6E\uFF0C\u4ED6\u77E5\u9053\uFF0C\u9280\u6CB3\u7CFB\u4E2D\u5FC3\u6700\u5F3A\u7684\u96FB\u6CE2\u767C\u5C04\u4F3C\u4E4E\u662F\u6E90\u81EA\u65BC\u4E00\u500B\u7DCA\u6E4A\u7684\u975E\u71B1\u5C04\u96FB\u9AD4\u3002 \u5B83\u662F\u975E\u5E38\u5149\u4EAE\u53CA\u7DFB\u5BC6\u7684\u7121\u7DDA\u96FB\u6CE2\u6E90\uFF0C\u5927\u7D04\u6BCF11\u5206\u9418\u81EA\u8F49\u4E00\u5708\u3002\u4EBA\u99AC\u5EA7A*\u662F\u76EE\u524D\u4EBA\u985E\u89C0\u6E2C\u5230\u79BB\u5730\u7403\u6700\u8FD1\uFF0C\u88AB\u8BA4\u4E3A\u662F\u7814\u7A76\u9ED1\u6D1E\u7269\u7406\u7684\u6700\u4F73\u76EE\u6807\u3002 \u5C0D\u570D\u7E5E\u4EBA\u99AC\u5EA7A*\u904B\u884C\u7684\u5E7E\u9846\u6046\u661F\u7684\u89C0\u6E2C\uFF0C\u7279\u5225\u662FS2\uFF0C\u5DF2\u88AB\u7528\u4F86\u78BA\u5B9A\u7269\u9AD4\u7684\u8CEA\u91CF\u548C\u534A\u5F91\u4E0A\u9650\u3002\u57FA\u65BC\u8CEA\u91CF\u548C\u65E5\u76CA\u7CBE\u78BA\u7684\u534A\u5F91\u503C\uFF0C\u5929\u6587\u5B78\u5BB6\u5F97\u51FA\u7D50\u8AD6\uFF1A\u4EBA\u99AC\u5EA7A*\u4E00\u5B9A\u662F\u9280\u6CB3\u7CFB\u4E2D\u592E\u7684\u8D85\u5927\u8CEA\u91CF\u9ED1\u6D1E\u3002\u5176\u8CEA\u91CF\u7684\u7576\u524D\u503C\u70BA4.154+0.014\u2212\u767E\u842C\u592A\u967D\u8CEA\u91CF\u3002 \u3002 \u8D56\u56E0\u54C8\u5FB7\u00B7\u6839\u7B56\u5C14\uFF08Reinhard Genzel\uFF09\u548C\u5B89\u5FB7\u70C8\u5A05\u00B7\u76D6\u5179\uFF08Andrea Ghez\uFF09\u56E0\u767C\u73FE\u4EBA\u99AC\u5EA7A*\u662F\u4E00\u500B\u8D85\u5927\u8CEA\u91CF\u7DFB\u5BC6\u5929\u9AD4\u800C\u7372\u5F972020\u5E74\u8AFE\u8C9D\u723E\u7269\u7406\u5B78\u734E\uFF0C\u800C\u9ED1\u6D1E\u662F\u7576\u6642\u552F\u4E00\u5408\u7406\u7684\u89E3\u91CB\u3002 2022\u5E745\u670812\u65E5\uFF0C\u5929\u6587\u5B78\u5BB6\u767C\u4F48\u65BC2017\u5E744\u6708\u4F7F\u7528\u5168\u7403\u5C04\u96FB\u5929\u6587\u81FA\u7DB2\u7D61\u4E8B\u4EF6\u8996\u754C\u671B\u9060\u93E1\u88FD\u4F5C\u7684\u4EBA\u99AC\u5EA7A*\u8996\u754C\u5468\u570D\u5438\u7A4D\u76E4\u7684\u7B2C\u4E00\u5F35\u5F71\u50CF\uFF0C\u78BA\u8A8D\u7269\u9AD4\u662F\u9ED1\u6D1E\u3002\u9019\u662F\u7E7C2019\u5E74M87\u7684\u8D85\u5927\u8CEA\u91CF\u9ED1\u6D1E\u4E4B\u5F8C\uFF0C\u78BA\u8A8D\u7684\u7B2C\u4E8C\u5F35\u9ED1\u6D1E\u5F71\u50CF\u3002\u3002"@zh . . . . . "Sagittarius A* Esne Bidearen erdialdean dagoen zulo beltz supermasibo bat da."@eu . . . . . . . . . . . "\u0645\u0646\u0637\u0642\u0629 \u0627\u0644\u0631\u0627\u0645\u064A \u0623* (\u0628\u0627\u0644\u0625\u0646\u062C\u0644\u064A\u0632\u064A\u0629: Sagittarius A*)\u200F \u0647\u064A \u0639\u0628\u0627\u0631\u0629 \u0639\u0646 \u0645\u0646\u0637\u0642\u0629 \u0644\u0627\u0645\u0639\u0629 \u0642\u0648\u064A \u062C\u062F\u0627\u064B \u062A\u0642\u0639 \u0641\u064A \u0645\u0631\u0643\u0632 \u0645\u062C\u0631\u0629 \u062F\u0631\u0628 \u0627\u0644\u062A\u0628\u0627\u0646\u0629\u060C \u0648\u0647\u064A \u062C\u0632\u0621 \u0645\u0646 \u0645\u0646\u0637\u0642\u0629 \u0623\u0643\u0628\u0631 \u062A\u0633\u0645\u0649 \u0627\u0644\u0631\u0627\u0645\u064A \u0623. \u062A\u062D\u062A\u0648\u064A \u0645\u0646\u0637\u0642\u0629 \u0627\u0644\u0631\u0627\u0645\u064A \u0623* \u0639\u0644\u0649 \u062B\u0642\u0628 \u0623\u0633\u0648\u062F \u0641\u0627\u0626\u0642 \u0627\u0644\u0636\u062E\u0627\u0645\u0629\u060C \u0648\u064A\u064F\u0639\u062A\u0642\u062F \u0623\u0646\u0647 \u062A\u0648\u062C\u062F \u062B\u0642\u0648\u0628 \u0633\u0648\u062F\u0627\u0621 \u0634\u0628\u064A\u0647\u0629 \u0641\u064A \u0645\u0631\u0627\u0643\u0632 \u0645\u0639\u0638\u0645 \u0627\u0644\u0645\u062C\u0631\u0627\u062A \u0627\u0644\u062D\u0644\u0632\u0648\u0646\u064A\u0629 \u0648\u0627\u0644\u0625\u0647\u0644\u064A\u062C\u064A\u0629."@ar . . . "May 2022"@en . . "Sagitario A*"@es . . . "Sagitario A* \u2014pronunciado Sagitario A estrella\u200B y abreviado Sgr A*\u2014 es el agujero negro supermasivo del centro gal\u00E1ctico de la V\u00EDa L\u00E1ctea. Es una fuente de radio muy compacta y brillante en el centro de la V\u00EDa L\u00E1ctea que forma parte de una estructura mayor llamada Sagitario A. Durante mucho tiempo se ha considerado que Sagitario A* contiene un agujero negro supermasivo,\u200B al igual que se supone sucede en los n\u00FAcleos de la mayor\u00EDa de galaxias de tipo espiral y el\u00EDptica. Observaciones de la \u00F3rbita de la estrella S2 alrededor de Sgr A* indican la presencia de dicho agujero negro.\u200B El 12 de mayo de 2022, el Event Horizon Telescope, revel\u00F3 por primera vez una fotograf\u00EDa de Sagitario A*, confirmando que el objeto contiene un agujero negro.\u200B\u200B"@es . . . . . "\u0421\u0442\u0440\u0435\u043B\u0435\u0446 A* (\u043B\u0430\u0442. Sagittarius A*, Sgr A*; \u043F\u0440\u043E\u0438\u0437\u043D\u043E\u0441\u0438\u0442\u0441\u044F \u00AB\u0421\u0442\u0440\u0435\u043B\u0435\u0301\u0446 \u0410 \u0441\u043E \u0437\u0432\u0451\u0437\u0434\u043E\u0447\u043A\u043E\u0439\u00BB) \u2014 \u043A\u043E\u043C\u043F\u0430\u043A\u0442\u043D\u044B\u0439 \u0440\u0430\u0434\u0438\u043E\u0438\u0441\u0442\u043E\u0447\u043D\u0438\u043A, \u043D\u0430\u0445\u043E\u0434\u044F\u0449\u0438\u0439\u0441\u044F \u0432 \u0446\u0435\u043D\u0442\u0440\u0435 \u041C\u043B\u0435\u0447\u043D\u043E\u0433\u043E \u041F\u0443\u0442\u0438, \u0432\u0445\u043E\u0434\u0438\u0442 \u0432 \u0441\u043E\u0441\u0442\u0430\u0432 \u0440\u0430\u0434\u0438\u043E\u0438\u0441\u0442\u043E\u0447\u043D\u0438\u043A\u0430 \u0421\u0442\u0440\u0435\u043B\u0435\u0446 \u0410. \u0418\u0437\u043B\u0443\u0447\u0430\u0435\u0442 \u0442\u0430\u043A\u0436\u0435 \u0432 \u0438\u043D\u0444\u0440\u0430\u043A\u0440\u0430\u0441\u043D\u043E\u043C, \u0440\u0435\u043D\u0442\u0433\u0435\u043D\u043E\u0432\u0441\u043A\u043E\u043C \u0438 \u0434\u0440\u0443\u0433\u0438\u0445 \u0434\u0438\u0430\u043F\u0430\u0437\u043E\u043D\u0430\u0445. \u041F\u0440\u0435\u0434\u0441\u0442\u0430\u0432\u043B\u044F\u0435\u0442 \u0441\u043E\u0431\u043E\u0439 \u0432\u044B\u0441\u043E\u043A\u043E\u043F\u043B\u043E\u0442\u043D\u044B\u0439 \u043E\u0431\u044A\u0435\u043A\u0442 \u2014 \u0441\u0432\u0435\u0440\u0445\u043C\u0430\u0441\u0441\u0438\u0432\u043D\u0443\u044E \u0447\u0451\u0440\u043D\u0443\u044E \u0434\u044B\u0440\u0443, \u043E\u043A\u0440\u0443\u0436\u0451\u043D\u043D\u0443\u044E \u0433\u043E\u0440\u044F\u0447\u0438\u043C \u0440\u0430\u0434\u0438\u043E\u0438\u0437\u043B\u0443\u0447\u0430\u044E\u0449\u0438\u043C \u0433\u0430\u0437\u043E\u0432\u044B\u043C \u043E\u0431\u043B\u0430\u043A\u043E\u043C \u0434\u0438\u0430\u043C\u0435\u0442\u0440\u043E\u043C \u043E\u043A\u043E\u043B\u043E 1,8 \u043F\u043A. \u0420\u0430\u0441\u0441\u0442\u043E\u044F\u043D\u0438\u0435 \u0434\u043E \u0440\u0430\u0434\u0438\u043E\u0438\u0441\u0442\u043E\u0447\u043D\u0438\u043A\u0430 \u0441\u043E\u0441\u0442\u0430\u0432\u043B\u044F\u0435\u0442 (27,00 \u00B1 0,10) \u0442\u044B\u0441. \u0441\u0432. \u043B\u0435\u0442, \u043C\u0430\u0441\u0441\u0430 \u0446\u0435\u043D\u0442\u0440\u0430\u043B\u044C\u043D\u043E\u0433\u043E \u043E\u0431\u044A\u0435\u043A\u0442\u0430 \u0440\u0430\u0432\u043D\u0430 (4,297 \u00B1 0,042) \u043C\u043B\u043D M\u2299. \u0414\u0430\u043D\u043D\u044B\u0435 \u0441 \u0440\u0430\u0434\u0438\u043E\u0442\u0435\u043B\u0435\u0441\u043A\u043E\u043F\u0430 VLBA \u0441\u0432\u0438\u0434\u0435\u0442\u0435\u043B\u044C\u0441\u0442\u0432\u0443\u044E\u0442, \u0447\u0442\u043E \u043D\u0435\u043F\u043E\u0441\u0440\u0435\u0434\u0441\u0442\u0432\u0435\u043D\u043D\u043E \u043D\u0430 \u0434\u043E\u043B\u044E \u0441\u0430\u043C\u043E\u0439 \u0447\u0451\u0440\u043D\u043E\u0439 \u0434\u044B\u0440\u044B \u043F\u0440\u0438\u0445\u043E\u0434\u0438\u0442\u0441\u044F \u043C\u0438\u043D\u0438\u043C\u0443\u043C \u0447\u0435\u0442\u0432\u0435\u0440\u0442\u044C \u043E\u0442 \u043E\u0431\u0449\u0435\u0439 \u043C\u0430\u0441\u0441\u044B \u043E\u0431\u044A\u0435\u043A\u0442\u0430 Sgr A*, \u0430 \u043E\u0441\u0442\u0430\u043B\u044C\u043D\u0430\u044F \u0447\u0430\u0441\u0442\u044C \u043C\u0430\u0441\u0441\u044B \u043F\u0440\u0438\u0445\u043E\u0434\u0438\u0442\u0441\u044F \u043D\u0430 \u043E\u043A\u0440\u0443\u0436\u0430\u044E\u0449\u0443\u044E \u0447\u0451\u0440\u043D\u0443\u044E \u0434\u044B\u0440\u0443 \u043C\u0430\u0442\u0435\u0440\u0438\u044E, \u0430 \u0442\u0430\u043A\u0436\u0435 \u0441\u043E\u0441\u0435\u0434\u043D\u0438\u0435 \u0441 \u043D\u0435\u0439 \u0437\u0432\u0451\u0437\u0434\u044B \u0438 \u043E\u0431\u043B\u0430\u043A\u0430 \u0433\u0430\u0437\u0430."@ru . . . . "300"^^ . . . . "Artist impression of the accretion of gas cloud G2 onto Sgr A*. Credit: ESO"@en . . . . . . . . . "Sagittarius A* (zvan\u00FD \u201EA-star\u201C, standardn\u00ED zkratka Sgr A*) je velmi velk\u00FD, siln\u011B z\u00E1\u0159\u00EDc\u00ED a kompaktn\u00ED zdroj r\u00E1diov\u00E9ho z\u00E1\u0159en\u00ED nach\u00E1zej\u00EDc\u00ED se ve st\u0159edu galaxie Ml\u00E9\u010Dn\u00E1 dr\u00E1ha. Je sou\u010D\u00E1st\u00ED v\u011Bt\u0161\u00EDho uskupen\u00ED podobn\u00FDch t\u011Bles, kter\u00E9 nese n\u00E1zev Sagittarius A. Dne 16. \u0159\u00EDjna 2002 zve\u0159ejnil mezin\u00E1rodn\u00ED t\u00FDm z (Max-Planck-Institut f\u00FCr extraterrestrische Physik) veden\u00FD Rainerem Sch\u00F6delem v\u00FDsledky sv\u00FDch pozorov\u00E1n\u00ED, b\u011Bhem kter\u00FDch po dobu deseti let sledoval pohyb hv\u011Bzdy S2, kter\u00E1 se nach\u00E1z\u00ED v bl\u00EDzkosti Sgr A*. T\u00FDm R. Sch\u00F6dela dosp\u011Bl k z\u00E1v\u011Bru, \u017Ee se jedn\u00E1 o vysoce mas\u00EDvn\u00ED kompaktn\u00ED objekt. Po pr\u016Fzkumu ob\u011B\u017En\u00E9 dr\u00E1hy hv\u011Bzdy S2 byla ur\u010Dena hmotnost Sgr A* na 2,6 \u00B1 0,2 milion\u016F hmotnost\u00ED Slunce a polom\u011Br oblasti, ve kter\u00E9 se soustava nach\u00E1z\u00ED, nem\u011Bla b\u00FDt v\u011Bt\u0161\u00ED ne\u017E 120 AU. Pozd\u011Bj\u0161\u00ED pr\u016Fzkumy up\u0159esnily hmotnost objektu"@cs . "\u4EBA\u99AC\u5EA7A*"@zh . . . . "\u0397 \u03B1\u03C3\u03C4\u03C1\u03BF\u03BD\u03BF\u03BC\u03B9\u03BA\u03AE \u03C0\u03B7\u03B3\u03AE \u03A4\u03BF\u03BE\u03CC\u03C4\u03B7\u03C2 A* (Sagittarius A*, Sgr A*) \u03B5\u03AF\u03BD\u03B1\u03B9 \u03BC\u03AF\u03B1 \u03B9\u03C3\u03C7\u03C5\u03C1\u03AE \u03BA\u03B1\u03B9 \u03C0\u03BF\u03BB\u03CD \u03BC\u03B9\u03BA\u03C1\u03AE \u03C3\u03B5 \u03B4\u03B9\u03B1\u03C3\u03C4\u03AC\u03C3\u03B5\u03B9\u03C2 , \u03C0\u03BF\u03C5 \u03B2\u03C1\u03AF\u03C3\u03BA\u03B5\u03C4\u03B1\u03B9 \u03C3\u03C4\u03BF \u03BA\u03AD\u03BD\u03C4\u03C1\u03BF \u03C4\u03BF\u03C5 \u0393\u03B1\u03BB\u03B1\u03BE\u03AF\u03B1 \u03BC\u03B1\u03C2, \u03C3\u03C4\u03BF\u03BD \u03B1\u03C3\u03C4\u03B5\u03C1\u03B9\u03C3\u03BC\u03CC \u03A4\u03BF\u03BE\u03CC\u03C4\u03B7, \u03B1\u03C0\u03CC \u03CC\u03C0\u03BF\u03C5 \u03BA\u03B1\u03B9 \u03B7 \u03BF\u03BD\u03BF\u03BC\u03B1\u03C3\u03AF\u03B1 \u03C4\u03B7\u03C2, \u03BA\u03BF\u03BD\u03C4\u03AC \u03C3\u03C4\u03B1 \u03C3\u03CD\u03BD\u03BF\u03C1\u03B1 \u03BC\u03B5 \u03C4\u03BF\u03BD \u03A3\u03BA\u03BF\u03C1\u03C0\u03B9\u03CC. \u039F\u03B9 \u03C3\u03C5\u03BD\u03C4\u03B5\u03C4\u03B1\u03B3\u03BC\u03AD\u03BD\u03B5\u03C2 \u03C4\u03B7\u03C2 \u03B5\u03AF\u03BD\u03B1\u03B9 \u03BF\u03C1\u03B8\u03AE \u03B1\u03BD\u03B1\u03C6\u03BF\u03C1\u03AC 17:45:40,04 \u03BA\u03B1\u03B9 \u03B1\u03C0\u03CC\u03BA\u03BB\u03B9\u03C3\u03B7 \u221229\u00B0 0\u0384 28,1\u0384\u0384. \u0391\u03C0\u03BF\u03C4\u03B5\u03BB\u03B5\u03AF \u03C4\u03BC\u03AE\u03BC\u03B1 \u03B5\u03BD\u03CC\u03C2 \u03BC\u03B5\u03B3\u03B1\u03BB\u03CD\u03C4\u03B5\u03C1\u03BF\u03C5 \u03C7\u03B1\u03C1\u03B1\u03BA\u03C4\u03B7\u03C1\u03B9\u03C3\u03C4\u03B9\u03BA\u03BF\u03CD \u03C0\u03BF\u03C5 \u03B5\u03AF\u03BD\u03B1\u03B9 \u03B3\u03BD\u03C9\u03C3\u03C4\u03CC \u03C9\u03C2 . \u039F Sgr A* \u03C0\u03B9\u03C3\u03C4\u03B5\u03CD\u03B5\u03C4\u03B1\u03B9 \u03CC\u03C4\u03B9 \u03B1\u03BD\u03C4\u03B9\u03C3\u03C4\u03BF\u03B9\u03C7\u03B5\u03AF \u03C3\u03B5 \u03BC\u03AF\u03B1 , \u03CC\u03C0\u03C9\u03C2 \u03B1\u03C5\u03C4\u03AD\u03C2 \u03C0\u03BF\u03C5 \u03B2\u03C1\u03AF\u03C3\u03BA\u03BF\u03BD\u03C4\u03B1\u03B9 \u03C3\u03C4\u03B1 \u03BA\u03AD\u03BD\u03C4\u03C1\u03B1 \u03C0\u03BF\u03BB\u03BB\u03CE\u03BD (\u03AF\u03C3\u03C9\u03C2 \u03C4\u03C9\u03BD \u03C0\u03B5\u03C1\u03B9\u03C3\u03C3\u03CC\u03C4\u03B5\u03C1\u03C9\u03BD) \u03BC\u03B5\u03B3\u03AC\u03BB\u03C9\u03BD \u03B3\u03B1\u03BB\u03B1\u03BE\u03B9\u03CE\u03BD. \u03A0\u03B1\u03C1\u03B1\u03C4\u03B7\u03C1\u03AE\u03C3\u03B5\u03B9\u03C2 \u03C4\u03BF\u03C5 \u03B1\u03C3\u03C4\u03AD\u03C1\u03B1 S2 \u03C0\u03BF\u03C5 \u03B2\u03C1\u03AF\u03C3\u03BA\u03B5\u03C4\u03B1\u03B9 \u03C3\u03B5 \u03C4\u03C1\u03BF\u03C7\u03B9\u03AC \u03C0\u03AD\u03C1\u03B9\u03BE \u03C4\u03BF\u03C5 \u03A4\u03BF\u03BE\u03CC\u03C4\u03B7 A* \u03AD\u03C7\u03BF\u03C5\u03BD \u03C7\u03C1\u03B7\u03C3\u03B9\u03BC\u03BF\u03C0\u03BF\u03B9\u03B7\u03B8\u03B5\u03AF \u03B3\u03B9\u03B1 \u03BD\u03B1 \u03B1\u03C0\u03BF\u03B4\u03B5\u03B9\u03C7\u03B8\u03B5\u03AF \u03B7 \u03C0\u03B1\u03C1\u03BF\u03C5\u03C3\u03AF\u03B1 \u03C4\u03B7\u03C2 \u03BC\u03B1\u03CD\u03C1\u03B7\u03C2 \u03C4\u03C1\u03CD\u03C0\u03B1\u03C2 \u03C3\u03C4\u03BF \u03BA\u03AD\u03BD\u03C4\u03C1\u03BF \u03C4\u03BF\u03C5 \u0393\u03B1\u03BB\u03B1\u03BE\u03AF\u03B1 \u03BC\u03B1\u03C2 \u03BA\u03B1\u03B9 \u03BD\u03B1 \u03B4\u03B9\u03B1\u03BA\u03C1\u03B9\u03B2\u03C9\u03B8\u03BF\u03CD\u03BD \u03C4\u03B1 \u03C7\u03B1\u03C1\u03B1\u03BA\u03C4\u03B7\u03C1\u03B9\u03C3\u03C4\u03B9\u03BA\u03AC \u03C4\u03B7\u03C2. \u03A4\u03BF \u03C3\u03C5\u03BC\u03C0\u03AD\u03C1\u03B1\u03C3\u03BC\u03B1 \u03B5\u03AF\u03BD\u03B1\u03B9 \u03CC\u03C4\u03B9 \u03B7 \u03C0\u03B7\u03B3\u03AE Sagittarius A* \u03B5\u03AF\u03BD\u03B1\u03B9 \u03C0\u03C1\u03AC\u03B3\u03BC\u03B1\u03C4\u03B9 \u03B7 \u03B8\u03AD\u03C3\u03B7 \u03C4\u03B7\u03C2 \u03BC\u03B1\u03CD\u03C1\u03B7\u03C2 "@el . . "Is \u00E9ard is Sagittarius A* ann (fuaimnithe \"Sagittarius A-r\u00E9alt\", giorr\u00FAch\u00E1n caighde\u00E1nach Sgr A*) n\u00E1 foinse gheal an-dl\u00FAth raidi\u00F3 r\u00E9alteola\u00EDoch, ag l\u00E1r Bhealach na B\u00F3 Finne, in aice le teorainn na r\u00E9altbhu\u00EDonta Sagittarius agus Scorpius. Cuid de ghn\u00E9 r\u00E9alteola\u00EDoch is ea \u00E9,ar a dtugtar 'Sagittarius A'. Creidtear gur shu\u00EDomh dh\u00FAphoill sarollmh\u00F3ir \u00E9, cos\u00FAil le iad si\u00FAd a nglactar go ginear\u00E1lta anois a bheith ag l\u00E1ir an chuid is m\u00F3 de na an chuid is m\u00F3 de na r\u00E9altra\u00ED b\u00EDseacha agus \u00E9ilipseacha. D'\u00FAs\u00E1idt\u00ED grinnithe r\u00E9altacha ar an r\u00E9alta S2, i bithis timpeall ar Saighdeoir A*, chun l\u00E1ithreachta de, agus sonra\u00ED a th\u00E1irgeadh faoin dh\u00FAphoill sarollmh\u00F3r at\u00E1 i l\u00E1r Bhealach na B\u00F3 Finne, agus threora\u00EDt\u00ED ar an tuairim gur su\u00EDomh an dh\u00FAphoill sarollmh\u00F3ir \u00E9 Sagittarius A* ."@ga . . "Simulation of gas cloud being ripped apart by the black hole at the centre of the Milky Way.ogv"@en . . . "\u0645\u0646\u0637\u0642\u0629 \u0627\u0644\u0631\u0627\u0645\u064A \u0623* (\u0628\u0627\u0644\u0625\u0646\u062C\u0644\u064A\u0632\u064A\u0629: Sagittarius A*)\u200F \u0647\u064A \u0639\u0628\u0627\u0631\u0629 \u0639\u0646 \u0645\u0646\u0637\u0642\u0629 \u0644\u0627\u0645\u0639\u0629 \u0642\u0648\u064A \u062C\u062F\u0627\u064B \u062A\u0642\u0639 \u0641\u064A \u0645\u0631\u0643\u0632 \u0645\u062C\u0631\u0629 \u062F\u0631\u0628 \u0627\u0644\u062A\u0628\u0627\u0646\u0629\u060C \u0648\u0647\u064A \u062C\u0632\u0621 \u0645\u0646 \u0645\u0646\u0637\u0642\u0629 \u0623\u0643\u0628\u0631 \u062A\u0633\u0645\u0649 \u0627\u0644\u0631\u0627\u0645\u064A \u0623. \u062A\u062D\u062A\u0648\u064A \u0645\u0646\u0637\u0642\u0629 \u0627\u0644\u0631\u0627\u0645\u064A \u0623* \u0639\u0644\u0649 \u062B\u0642\u0628 \u0623\u0633\u0648\u062F \u0641\u0627\u0626\u0642 \u0627\u0644\u0636\u062E\u0627\u0645\u0629\u060C \u0648\u064A\u064F\u0639\u062A\u0642\u062F \u0623\u0646\u0647 \u062A\u0648\u062C\u062F \u062B\u0642\u0648\u0628 \u0633\u0648\u062F\u0627\u0621 \u0634\u0628\u064A\u0647\u0629 \u0641\u064A \u0645\u0631\u0627\u0643\u0632 \u0645\u0639\u0638\u0645 \u0627\u0644\u0645\u062C\u0631\u0627\u062A \u0627\u0644\u062D\u0644\u0632\u0648\u0646\u064A\u0629 \u0648\u0627\u0644\u0625\u0647\u0644\u064A\u062C\u064A\u0629."@ar . . . . "Sagitario A* \u2014pronunciado Sagitario A estrella\u200B y abreviado Sgr A*\u2014 es el agujero negro supermasivo del centro gal\u00E1ctico de la V\u00EDa L\u00E1ctea. Es una fuente de radio muy compacta y brillante en el centro de la V\u00EDa L\u00E1ctea que forma parte de una estructura mayor llamada Sagitario A. Durante mucho tiempo se ha considerado que Sagitario A* contiene un agujero negro supermasivo,\u200B al igual que se supone sucede en los n\u00FAcleos de la mayor\u00EDa de galaxias de tipo espiral y el\u00EDptica. Observaciones de la \u00F3rbita de la estrella S2 alrededor de Sgr A* indican la presencia de dicho agujero negro.\u200B"@es . "center"@en . . . . . . . . . . . . . . . . "\uAD81\uC218\uC790\uB9AC A*(\uC601\uC5B4: Sagittarius A*, Sgr A*, \"\uAD81\uC218\uC790\uB9AC A\uBCC4\"\uB85C \uBC1C\uC74C)\uC740 \uAD81\uC218\uC790\uB9AC\uC640 \uC804\uAC08\uC790\uB9AC \uACBD\uACC4 \uADFC\uCC98, \uC6B0\uB9AC \uC740\uD558\uC758 \uC911\uC2EC\uC5D0 \uC788\uB294 \uBC1D\uACE0 \uC791\uC740 \uC804\uD30C\uC6D0\uC774\uB2E4. \uC774\uB294 \uB85C \uC54C\uB824\uC838 \uC788\uB294 \uB354 \uD070 \uC804\uD30C\uC6D0\uC758 \uC77C\uBD80\uC774\uB2E4. \uAD81\uC218\uC790\uB9AC A*\uC740 \uC77C\uBC18\uC801\uC73C\uB85C \uB300\uBD80\uBD84\uC758 \uB098\uC120 \uC740\uD558\uC640 \uD0C0\uC6D0 \uC740\uD558\uC758 \uC911\uC2EC\uC5D0 \uC788\uC744 \uAC83\uC73C\uB85C \uBC1B\uC544\uB4E4\uC5EC\uC9C0\uB294, \uCD08\uB300\uC9C8\uB7C9 \uBE14\uB799\uD640\uC77C \uAC83\uC73C\uB85C \uC5EC\uACA8\uC9C0\uACE0 \uC788\uB2E4. \uAD81\uC218\uC790\uB9AC A* \uC8FC\uBCC0\uC744 \uACF5\uC804\uD558\uB294 \uBCC4 S2\uC758 \uAD00\uCE21\uC740 \uC6B0\uB9AC \uC740\uD558\uC758 \uC911\uC2EC \uBE14\uB799\uD640\uC758 \uC874\uC7AC\uB97C \uBCF4\uC5EC\uC8FC\uACE0, \uADF8\uC5D0 \uB300\uD55C \uB370\uC774\uD130\uB97C \uB9CC\uB4DC\uB294\uB370 \uC774\uC6A9\uB418\uBA70, \uC774\uB294 \uAD81\uC218\uC790\uB9AC A*\uC774 \uADF8 \uBE14\uB799\uD640\uC758 \uC704\uCE58\uB77C\uB294 \uACB0\uB860\uC73C\uB85C \uC720\uB3C4\uB41C\uB2E4."@ko . . . . . . "69242"^^ . . . . . "Supernova remnant ejecta producing planet-forming material"@en . "Sagittarius A* (zvan\u00FD \u201EA-star\u201C, standardn\u00ED zkratka Sgr A*) je velmi velk\u00FD, siln\u011B z\u00E1\u0159\u00EDc\u00ED a kompaktn\u00ED zdroj r\u00E1diov\u00E9ho z\u00E1\u0159en\u00ED nach\u00E1zej\u00EDc\u00ED se ve st\u0159edu galaxie Ml\u00E9\u010Dn\u00E1 dr\u00E1ha. Je sou\u010D\u00E1st\u00ED v\u011Bt\u0161\u00EDho uskupen\u00ED podobn\u00FDch t\u011Bles, kter\u00E9 nese n\u00E1zev Sagittarius A. Dne 16. \u0159\u00EDjna 2002 zve\u0159ejnil mezin\u00E1rodn\u00ED t\u00FDm z (Max-Planck-Institut f\u00FCr extraterrestrische Physik) veden\u00FD Rainerem Sch\u00F6delem v\u00FDsledky sv\u00FDch pozorov\u00E1n\u00ED, b\u011Bhem kter\u00FDch po dobu deseti let sledoval pohyb hv\u011Bzdy S2, kter\u00E1 se nach\u00E1z\u00ED v bl\u00EDzkosti Sgr A*. T\u00FDm R. Sch\u00F6dela dosp\u011Bl k z\u00E1v\u011Bru, \u017Ee se jedn\u00E1 o vysoce mas\u00EDvn\u00ED kompaktn\u00ED objekt. Po pr\u016Fzkumu ob\u011B\u017En\u00E9 dr\u00E1hy hv\u011Bzdy S2 byla ur\u010Dena hmotnost Sgr A* na 2,6 \u00B1 0,2 milion\u016F hmotnost\u00ED Slunce a polom\u011Br oblasti, ve kter\u00E9 se soustava nach\u00E1z\u00ED, nem\u011Bla b\u00FDt v\u011Bt\u0161\u00ED ne\u017E 120 AU. Pozd\u011Bj\u0161\u00ED pr\u016Fzkumy up\u0159esnily hmotnost objektu na 3,7 milion\u016F hmotnost\u00ED Slunce s polom\u011Brem p\u0159ibli\u017En\u011B 45 AU (6,7578 miliard kilometr\u016F). Pro porovn\u00E1n\u00ED, trpasli\u010D\u00ED planeta Pluto ob\u00EDh\u00E1 na\u0161e Slunce ve vzd\u00E1lenosti 39,68 AU, co\u017E je 5,9533 miliard kilometr\u016F. Tato zji\u0161t\u011Bn\u00ED tedy podporuj\u00ED hypot\u00E9zu, podle kter\u00E9 je Sagittarius A* ob\u0159\u00ED \u010Dernou d\u00EDrou. Je sice mo\u017En\u00E9 p\u0159i\u0159knout zji\u0161t\u011Bnou hmotnost b\u011B\u017En\u00FDm objekt\u016Fm, kter\u00E9 by se v dan\u00E9m prostoru mohly nach\u00E1zet, av\u0161ak \u017E\u00E1dn\u00E9 takov\u00E9 objekty o takov\u00E9 hmotnosti by v r\u00E1mci tak \u201Emal\u00E9\u201C oblasti nemohly odol\u00E1vat kolapsu sv\u00FDch vz\u00E1jemn\u00FDch orbit\u016F a n\u00E1sledn\u00E9mu neodvratiteln\u00E9mu \u201Ep\u00E1du\u201C do \u010Dern\u00E9 d\u00EDry d\u00E9le ne\u017E n\u011Bkolik stovek let, co\u017E je naprosto zanedbateln\u00E1 doba ve vztahu k d\u00E9lce \u201E\u017Eivota\u201C galaxie. N\u011Bkolik t\u00FDm\u016F v\u011Bdc\u016F, mimo jin\u00E9 i z nebo tak\u00E9 , se sna\u017Eily zobrazit Sgr A* pomoc\u00ED radioastronomick\u00E9 metody . Z\u00EDskan\u00E9 sn\u00EDmky byly shodn\u00E9 s r\u00E1diov\u00FDmi emisemi zp\u016Fsoben\u00FDmi gigantick\u00FDmi v\u00FDtrysky plazmatu z jin\u00FDch \u010Dern\u00FDch d\u011Br. V listopadu 2004 vydal t\u00FDm v\u011Bdc\u016F zpr\u00E1vu, \u017Ee do\u0161lo k objevu prvn\u00ED, velmi dob\u0159e prokazateln\u00E9 \u010Dern\u00E9 d\u00EDry st\u0159edn\u00ED velikosti v na\u0161\u00ED galaxii, kter\u00E1 ob\u00EDh\u00E1 ve vzd\u00E1lenosti t\u0159\u00ED sv\u011Bteln\u00FDch let od Sagittaria A*. Tato \u010Dern\u00E1 d\u00EDra m\u00E1 hmotnost 1300 hmotnost\u00ED Slunce a \u201Evle\u010De\u201C s sebou shluk sedmi hv\u011Bzd, co\u017E je pravd\u011Bpodobn\u011B zbytek ob\u0159\u00EDho shluku hv\u011Bzd, kter\u00FD byl rozmet\u00E1n slapov\u00FDmi silami galaktick\u00E9ho st\u0159edu. Toto zji\u0161t\u011Bn\u00ED by mohlo podporovat teorii, \u017Ee gigantick\u00E9 \u010Dern\u00E9 d\u00EDry mohou \u201Er\u016Fst\u201C pot\u00E9, co absorbuj\u00ED men\u0161\u00ED \u010Dern\u00E9 d\u00EDry nebo hv\u011Bzdy. V srpnu 2008 t\u00FDm Andrey Ghezov\u00E9 z UCLA zve\u0159ejnil v\u00FDsledky m\u011B\u0159en\u00ED pohybu hv\u011Bzd v okol\u00ED Sagittaria A*. Zm\u011B\u0159ena byla p\u0159edev\u0161\u00EDm hmotnost objektu \u2013 nejm\u00E9n\u011B 4,1 milionu hmotnost\u00ED Slunce s nep\u0159esnost\u00ED m\u011B\u0159en\u00ED 15 %. P\u0159i p\u0159edpokladu, \u017Ee se s\u00E1m Sagittarius A* v\u016F\u010Di galaxii nepohybuje, hmotnost je 4,5 milionu hmotnost\u00ED Slunce s nep\u0159esnost\u00ED 9 %. Dal\u0161\u00EDm v\u00FDsledkem m\u011B\u0159en\u00ED bylo zp\u0159esn\u011Bn\u00ED vzd\u00E1lenosti Sagittaria A* od Slunce na 27 400 sv\u011Bteln\u00FDch let s odchylkou necel\u00FDch 5 %. V z\u00E1\u0159\u00ED 2008 t\u00FDm z MIT zve\u0159ejnil v\u00FDsledky v\u00FDzkumu Sagittaria A* pomoc\u00ED . Ten umo\u017Enil objekt sledovat s velk\u00FDm rozli\u0161en\u00EDm. Sagittarius A* je maxim\u00E1ln\u011B 50 milion\u016F km velk\u00FD, p\u0159i\u010Dem\u017E Schwarzschild\u016Fv polom\u011Br p\u0159edpokl\u00E1dan\u00E9 \u010Dern\u00E9 d\u00EDry by m\u011Bl b\u00FDt 13 milion\u016F km."@cs . . . "Sagitari A*"@ca . "The dusty cloud G2 passes the supermassive black hole at the centre of the Milky Way.webm"@en . . . . "Sagittarius A*"@eo . . . . . "Sagittarius A* (pronuncia-se Sagittarius A-estrela), tamb\u00E9m chamada de Sagit\u00E1rio A* (Sgr A* - sigla), \u00E9 uma fonte de r\u00E1dio astron\u00F4mica brilhante e muito compacta localizada no centro da Via L\u00E1ctea, perto da fronteira das constela\u00E7\u00F5es de Sagit\u00E1rio e Escorpi\u00E3o. \u00C9 parte de um objeto astron\u00F4mico maior conhecido como Sagittarius A. Acredita-se que Sagit\u00E1rio A* seja a localiza\u00E7\u00E3o de um buraco negro supermassivo, como aqueles que geralmente est\u00E3o nos centros da maioria das gal\u00E1xias espirais e el\u00EDpticas. As observa\u00E7\u00F5es da estrela S2 em \u00F3rbita ao redor de Sagit\u00E1rio A* foram usadas para mostrar sua presen\u00E7a e produzir dados sobre o buraco negro supermassivo central da Via L\u00E1ctea e levaram \u00E0 conclus\u00E3o de que Sagit\u00E1rio A* \u00E9 o local deste buraco negro. O buraco negro explodiu quase 3,5 milh\u00F5es de anos atr\u00E1s, devido a uma grande nuvem de hidrog\u00EAnio caindo no disco de material rodopiando perto do buraco negro central."@pt . . . . . . . . . . . . . "Sagitari A* (es pronuncia Sagitari A estel o Sagitari A asterisc, abreujat com Sgr A*) \u00E9s una font de r\u00E0dio molt compacta i brillant al centre de la Via L\u00E0ctia que forma part d'una estructura major anomenada Sagitari A. Hom considera que Sagitari A* cont\u00E9 un forat negre supermasiu, igual que se suposa succeeix als nuclis de la majoria de gal\u00E0xies de tipus espiral i el\u00B7l\u00EDptica. Observacions de l'\u00F2rbita de l'estel S2 al voltant de Sgr A* indiquen la pres\u00E8ncia d'aquest forat negre."@ca . . "Sagittarius A*"@pt . . "Sagitari A* (es pronuncia Sagitari A estel o Sagitari A asterisc, abreujat com Sgr A*) \u00E9s una font de r\u00E0dio molt compacta i brillant al centre de la Via L\u00E0ctia que forma part d'una estructura major anomenada Sagitari A. Hom considera que Sagitari A* cont\u00E9 un forat negre supermasiu, igual que se suposa succeeix als nuclis de la majoria de gal\u00E0xies de tipus espiral i el\u00B7l\u00EDptica. Observacions de l'\u00F2rbita de l'estel S2 al voltant de Sgr A* indiquen la pres\u00E8ncia d'aquest forat negre."@ca . "Sagittarius A*"@in . . . . . "Sagittarius A* (/\u02C8e\u026A st\u0251\u02D0r/ AY star), abbreviated Sgr A* (/\u02C8s\u00E6d\u0292 \u02C8e\u026A st\u0251\u02D0r/ SAJ AY star), is the supermassive black hole at the Galactic Center of the Milky Way. It is located near the border of the constellations Sagittarius and Scorpius, about 5.6\u00B0 south of the ecliptic, visually close to the Butterfly Cluster (M6) and Lambda Scorpii. Reinhard Genzel and Andrea Ghez were awarded the 2020 Nobel Prize in Physics for their discovery that Sagittarius A* is a supermassive compact object, for which a black hole was the only plausible explanation at the time."@en . . "Sagittarius A* (abbreviato in Sgr A*) \u00E8 una sorgente di onde radio molto luminosa, situata nel centro della Via Lattea, parte della grande struttura nota come Sagittarius A. Sgr A* \u00E8 il punto in cui si trova un buco nero supermassiccio, componente caratteristico dei centri di molte galassie ellittiche e spirali. Sagittarius A* avrebbe una massa di circa 4 milioni di volte quella del Sole e, trovandosi nel centro della nostra galassia, costituirebbe il corpo celeste attorno a cui tutte le stelle della Via Lattea, compresa la nostra, compiono il loro moto di rivoluzione."@it . . . . . . . . . "Sagittarius A* (w skr\u00F3cie Sgr A*) \u2013 obiekt astronomiczny, kt\u00F3ry jest jasnym i bardzo zwartym \u017Ar\u00F3d\u0142em radiowym w centrum Drogi Mlecznej, cz\u0119\u015Bci\u0105 wi\u0119kszej struktury astronomicznej (Sagittarius A). Odleg\u0142o\u015B\u0107 do \u017Ar\u00F3d\u0142a wynosi oko\u0142o 8 kpc (2,4\u00D71017 km). Radio\u017Ar\u00F3d\u0142o zawiera supermasywn\u0105 czarn\u0105 dziur\u0119 ci\u0119\u017Csz\u0105 od S\u0142o\u0144ca oko\u0142o 4,31\u00B10,06 miliona razy (masa S\u0142o\u0144ca to oko\u0142o 2\u00D71030 kg). Jej promie\u0144 oszacowano na oko\u0142o p\u00F3\u0142 minuty \u015Bwietlnej (0,06 j.a.) - trzynastokrotno\u015B\u0107 promienia S\u0142o\u0144ca. Badania wskazuj\u0105 r\u00F3wnie\u017C, \u017Ce czarna dziura zwi\u0119kszy\u0142a swoj\u0105 mas\u0119 2 do 4 razy w ci\u0105gu ostatnich 5-10 miliard\u00F3w lat, poprzez poch\u0142anianie pobliskich gwiazd."@pl . . . . . . "\u0421\u0442\u0440\u0456\u043B\u0435\u0446\u044C A* (Sagittarius A*, Sgr A*) \u2014 \u043D\u0430\u0434\u043C\u0430\u0441\u0438\u0432\u043D\u0430 \u0447\u043E\u0440\u043D\u0430 \u0434\u0456\u0440\u0430 \u0432 \u0446\u0435\u043D\u0442\u0440\u0456 \u043D\u0430\u0448\u043E\u0457 \u0413\u0430\u043B\u0430\u043A\u0442\u0438\u043A\u0438. \u0412\u0438\u043F\u0440\u043E\u043C\u0456\u043D\u044E\u0454 \u0432 \u0440\u0430\u0434\u0456\u043E, \u0456\u043D\u0444\u0440\u0430\u0447\u0435\u0440\u0432\u043E\u043D\u043E\u043C\u0443, \u0440\u0435\u043D\u0442\u0433\u0435\u043D\u0456\u0432\u0441\u044C\u043A\u043E\u043C\u0443 \u0442\u0430 \u0456\u043D\u0448\u0438\u0445 \u0434\u0456\u0430\u043F\u0430\u0437\u043E\u043D\u0430\u0445. \u0412\u043E\u043D\u0430 \u043E\u0442\u043E\u0447\u0435\u043D\u0430 \u0433\u0430\u0440\u044F\u0447\u043E\u044E \u0440\u0430\u0434\u0456\u043E\u0432\u0438\u043F\u0440\u043E\u043C\u0456\u043D\u044E\u0432\u0430\u043B\u044C\u043D\u043E\u044E \u0433\u0430\u0437\u043E\u0432\u043E\u044E \u0445\u043C\u0430\u0440\u043E\u044E \u0434\u0456\u0430\u043C\u0435\u0442\u0440\u043E\u043C \u0431\u043B\u0438\u0437\u044C\u043A\u043E 1,8 \u043F\u043A. \u0412\u0456\u0434\u0441\u0442\u0430\u043D\u044C \u0434\u043E \u043D\u0435\u0457 \u0441\u0442\u0430\u043D\u043E\u0432\u0438\u0442\u044C \u0431\u043B\u0438\u0437\u044C\u043A\u043E 27 \u0442\u0438\u0441. \u0441\u0432. \u0440\u043E\u043A\u0456\u0432, \u043C\u0430\u0441\u0430 \u043E\u0431'\u0454\u043A\u0442\u0430 \u2014 4,3 \u043C\u043B\u043D. M\u2609."@uk . . "horizontal"@en . . "840191"^^ . . . . . "\u0421\u0442\u0440\u0456\u043B\u0435\u0446\u044C A* (Sagittarius A*, Sgr A*) \u2014 \u043D\u0430\u0434\u043C\u0430\u0441\u0438\u0432\u043D\u0430 \u0447\u043E\u0440\u043D\u0430 \u0434\u0456\u0440\u0430 \u0432 \u0446\u0435\u043D\u0442\u0440\u0456 \u043D\u0430\u0448\u043E\u0457 \u0413\u0430\u043B\u0430\u043A\u0442\u0438\u043A\u0438. \u0412\u0438\u043F\u0440\u043E\u043C\u0456\u043D\u044E\u0454 \u0432 \u0440\u0430\u0434\u0456\u043E, \u0456\u043D\u0444\u0440\u0430\u0447\u0435\u0440\u0432\u043E\u043D\u043E\u043C\u0443, \u0440\u0435\u043D\u0442\u0433\u0435\u043D\u0456\u0432\u0441\u044C\u043A\u043E\u043C\u0443 \u0442\u0430 \u0456\u043D\u0448\u0438\u0445 \u0434\u0456\u0430\u043F\u0430\u0437\u043E\u043D\u0430\u0445. \u0412\u043E\u043D\u0430 \u043E\u0442\u043E\u0447\u0435\u043D\u0430 \u0433\u0430\u0440\u044F\u0447\u043E\u044E \u0440\u0430\u0434\u0456\u043E\u0432\u0438\u043F\u0440\u043E\u043C\u0456\u043D\u044E\u0432\u0430\u043B\u044C\u043D\u043E\u044E \u0433\u0430\u0437\u043E\u0432\u043E\u044E \u0445\u043C\u0430\u0440\u043E\u044E \u0434\u0456\u0430\u043C\u0435\u0442\u0440\u043E\u043C \u0431\u043B\u0438\u0437\u044C\u043A\u043E 1,8 \u043F\u043A. \u0412\u0456\u0434\u0441\u0442\u0430\u043D\u044C \u0434\u043E \u043D\u0435\u0457 \u0441\u0442\u0430\u043D\u043E\u0432\u0438\u0442\u044C \u0431\u043B\u0438\u0437\u044C\u043A\u043E 27 \u0442\u0438\u0441. \u0441\u0432. \u0440\u043E\u043A\u0456\u0432, \u043C\u0430\u0441\u0430 \u043E\u0431'\u0454\u043A\u0442\u0430 \u2014 4,3 \u043C\u043B\u043D. M\u2609."@uk . . . "This simulation shows a gas cloud, discovered in 2011, as it passes close to the supermassive black hole at the center of the Milky Way"@en . "Sagittarius A*"@it . . . . . . "\u4EBA\u99AC\u5EA7A*\uFF08Sagittarius A*\uFF0C\u7C21\u5BEB\u70BASgr A*\uFF0C\u661F\u865F*\u8B80\u4F5C\u300Cstar\u300D\u6216\u300C\u661F\u300D\uFF09\u662F\u500B\u4F4D\u65BC\u9280\u6CB3\u7CFB\u4E2D\u5FC3\u7684\u8D85\u5927\u8CEA\u91CF\u9ED1\u6D1E\u3002\u5B83\u4F4D\u65BC\u661F\u5EA7\u4EBA\u99AC\u5EA7\u548C\u5929\u880D\u5EA7\u7684\u908A\u754C\u9644\u8FD1\uFF0C\u5927\u7D04\u4F4D\u65BC\u9EC3\u9053\u4EE5\u53575.6\u00B0\uFF0C\u8996\u89BA\u4E0A\u63A5\u8FD1\u8774\u8776\u661F\u5718\uFF08M6\uFF09\u548C\u5C3E\u5BBF\u516B\uFF08\u5929\u880D\u5EA7\u03BB\uFF09\u3002 \u9019\u9846\u5929\u9AD4\u662F\u660E\u4EAE\u7DFB\u5BC6\u7684\u96FB\u6CE2\u6E90\u3002\u4EBA\u99AC\u5EA7A*\u7684\u540D\u5B57\u6709\u5176\u6B77\u53F2\u6DF5\u6E90\u3002\u5728 1954\u5E74\uFF0C\u7D04\u7FF0\u00B7\u4E39\u5C3C\u723E\u00B7\u514B\u52DE\u65AF\u3001\u67EF\u8CE2\u6E05\uFF08Hsien-Ching Ko\uFF09\u548C\u8096\u6069\u00B7\u99AC\u7279\uFF08Sean Matt\uFF09\u5217\u51FA\u4E86\u4ED6\u5011\u7528\u4FC4\u4EA5\u4FC4\u5DDE\u7ACB\u5927\u5B78\u96FB\u6CE2\u671B\u9060\u93E1\u5728250MHz\u4E0B\u78BA\u5B9A\u7684\u96FB\u6CE2\u6E90\u3002\u9019\u4E9B\u96FB\u6CE2\u6E90\u6309\u661F\u5EA7\u6392\u5217\uFF0C\u4E26\u96A8\u610F\u7684\u5206\u914D\u5B57\u6BCD\u4F86\u6A19\u793A\uFF0C\u4F46\u5B57\u6BCDA\u901A\u5E38\u8868\u793A\u661F\u5EA7\u5167\u6700\u4EAE\u7684\u96FB\u6CE2\u6E90\u3002\u661F\u865F * \u662F\u56E0\u70BA\u5B83\u7684\u767C\u73FE\u88AB\u8A8D\u70BA\u662F\"\u4EE4\u4EBA\u8208\u596E\u7684\"\u3002\u9019\u8207\u7528\u661F\u865F\u8868\u793A\u6FC0\u767C\u614B\u539F\u5B50\u7684\u547D\u540D\u6CD5\u4E00\u81F4\uFF08\u4F8B\u5982\uFF0C\u6C26\u7684\u6FC0\u767C\u614B\u70BAHe*\uFF09\u3002\u661F\u865F\u662F\u7F85\u4F2F\u7279\u00B7L\u00B7\u5E03\u6717\u65BC1982\u5E74\u8A2D\u7F6E\uFF0C\u4ED6\u77E5\u9053\uFF0C\u9280\u6CB3\u7CFB\u4E2D\u5FC3\u6700\u5F3A\u7684\u96FB\u6CE2\u767C\u5C04\u4F3C\u4E4E\u662F\u6E90\u81EA\u65BC\u4E00\u500B\u7DCA\u6E4A\u7684\u975E\u71B1\u5C04\u96FB\u9AD4\u3002 \u5B83\u662F\u975E\u5E38\u5149\u4EAE\u53CA\u7DFB\u5BC6\u7684\u7121\u7DDA\u96FB\u6CE2\u6E90\uFF0C\u5927\u7D04\u6BCF11\u5206\u9418\u81EA\u8F49\u4E00\u5708\u3002\u4EBA\u99AC\u5EA7A*\u662F\u76EE\u524D\u4EBA\u985E\u89C0\u6E2C\u5230\u79BB\u5730\u7403\u6700\u8FD1\uFF0C\u88AB\u8BA4\u4E3A\u662F\u7814\u7A76\u9ED1\u6D1E\u7269\u7406\u7684\u6700\u4F73\u76EE\u6807\u3002 \u5C0D\u570D\u7E5E\u4EBA\u99AC\u5EA7A*\u904B\u884C\u7684\u5E7E\u9846\u6046\u661F\u7684\u89C0\u6E2C\uFF0C\u7279\u5225\u662FS2\uFF0C\u5DF2\u88AB\u7528\u4F86\u78BA\u5B9A\u7269\u9AD4\u7684\u8CEA\u91CF\u548C\u534A\u5F91\u4E0A\u9650\u3002\u57FA\u65BC\u8CEA\u91CF\u548C\u65E5\u76CA\u7CBE\u78BA\u7684\u534A\u5F91\u503C\uFF0C\u5929\u6587\u5B78\u5BB6\u5F97\u51FA\u7D50\u8AD6\uFF1A\u4EBA\u99AC\u5EA7A*\u4E00\u5B9A\u662F\u9280\u6CB3\u7CFB\u4E2D\u592E\u7684\u8D85\u5927\u8CEA\u91CF\u9ED1\u6D1E\u3002\u5176\u8CEA\u91CF\u7684\u7576\u524D\u503C\u70BA4.154+0.014\u2212\u767E\u842C\u592A\u967D\u8CEA\u91CF\u3002 \u3002"@zh . "Sagittarius A*"@ga . . "Sagittarius A* (Sgr A*; i stj\u00E4rnbilden Skytten) \u00E4r en ljusstark och extremt kompakt radiok\u00E4lla i Vintergatans centrum, och \u00E4r en del av objektgruppen . Centrum f\u00F6r v\u00E5r galax befinner sig ca 26 000 ljus\u00E5r fr\u00E5n jorden."@sv . "Sagittarius A*"@en . "Is \u00E9ard is Sagittarius A* ann (fuaimnithe \"Sagittarius A-r\u00E9alt\", giorr\u00FAch\u00E1n caighde\u00E1nach Sgr A*) n\u00E1 foinse gheal an-dl\u00FAth raidi\u00F3 r\u00E9alteola\u00EDoch, ag l\u00E1r Bhealach na B\u00F3 Finne, in aice le teorainn na r\u00E9altbhu\u00EDonta Sagittarius agus Scorpius. Cuid de ghn\u00E9 r\u00E9alteola\u00EDoch is ea \u00E9,ar a dtugtar 'Sagittarius A'. Creidtear gur shu\u00EDomh dh\u00FAphoill sarollmh\u00F3ir \u00E9, cos\u00FAil le iad si\u00FAd a nglactar go ginear\u00E1lta anois a bheith ag l\u00E1ir an chuid is m\u00F3 de na an chuid is m\u00F3 de na r\u00E9altra\u00ED b\u00EDseacha agus \u00E9ilipseacha. D'\u00FAs\u00E1idt\u00ED grinnithe r\u00E9altacha ar an r\u00E9alta S2, i bithis timpeall ar Saighdeoir A*, chun l\u00E1ithreachta de, agus sonra\u00ED a th\u00E1irgeadh faoin dh\u00FAphoill sarollmh\u00F3r at\u00E1 i l\u00E1r Bhealach na B\u00F3 Finne, agus threora\u00EDt\u00ED ar an tuairim gur su\u00EDomh an dh\u00FAphoill sarollmh\u00F3ir \u00E9 Sagittarius A* ."@ga . . . "Sagittarius A* (gesprochen: Sagittarius A Stern; abgek\u00FCrzt: Sgr A*; eine Region im Sternbild Sch\u00FCtze) ist eine Quelle von Radiowellen im Zentrum der Milchstra\u00DFe. Nach derzeitigem radioastronomischen Forschungsstand handelt es sich dabei um ein supermassereiches Schwarzes Loch von 4,154 \u00B1 0,014 Millionen Sonnenmassen, das 26.673 \u00B1 42 Lichtjahre (8.178 \u00B1 13 pc) von der Sonne entfernt ist. Der Durchmesser seines Ereignishorizonts (20 \u03BCas, Mikrobogensekunden) entspricht mit 24,5 Mio. km etwa 21 % des Bahndurchmessers des Merkur auf seiner Umlaufbahn um die Sonne. Mit der Entdeckung der Fermi-Blasen im Jahre 2010 und ihren m\u00F6glichen Pendants im R\u00F6ntgenlicht, den \u201EeROSITA-Blasen\u201C 2019 ergeben sich Hinweise darauf, dass Sagittarius A* vor langer Zeit aktiv gewesen war und die Milchstra\u00DFe somit ei"@de . . "\u0627\u0644\u0631\u0627\u0645\u064A A*"@ar . . . . . . . . "\u3044\u3066\u5EA7A*\uFF08\u3044\u3066\u3056\u30A8\u30FC\u30FB\u30B9\u30BF\u30FC\u3001\u7565\u53F7Sgr A*\uFF09\u306F\u3001\u5929\u306E\u5DDD\u9280\u6CB3\u306E\u4E2D\u5FC3\u306B\u3042\u308B\u660E\u308B\u304F\u30B3\u30F3\u30D1\u30AF\u30C8\u306A\u5929\u6587\u96FB\u6CE2\u6E90\u3002\u3088\u308A\u5927\u898F\u6A21\u306A\u69CB\u9020\u306E\u96FB\u6CE2\u6E90\u9818\u57DF\u3067\u3042\u308B\u3044\u3066\u5EA7A\u306E\u4E00\u90E8\u3067\u3042\u308B\u3002\u3044\u3066\u5EA7A*\u306E\u4F4D\u7F6E\u306B\u306F\u8D85\u5927\u8CEA\u91CF\u30D6\u30E9\u30C3\u30AF\u30DB\u30FC\u30EB\u304C\u5B58\u5728\u3059\u308B\u3068\u8003\u3048\u3089\u308C\u3001\u591A\u304F\u306E\u6E26\u5DFB\u9280\u6CB3\u3084\u6955\u5186\u9280\u6CB3\u306E\u4E2D\u5FC3\u306B\u3082\u540C\u3058\u3088\u3046\u306B\u8D85\u5927\u8CEA\u91CF\u30D6\u30E9\u30C3\u30AF\u30DB\u30FC\u30EB\u304C\u3042\u308B\u3068\u3044\u3046\u306E\u304C\u5B9A\u8AAC\u3068\u306A\u3063\u3066\u3044\u308B\u3002\u3044\u3066\u5EA7A*\u306E\u5468\u56F2\u3092\u516C\u8EE2\u3057\u3066\u3044\u308B\u6052\u661FS2\u306E\u89B3\u6E2C\u306B\u3088\u3063\u3066\u3001\u9280\u6CB3\u7CFB\u4E2D\u5FC3\u306B\u8D85\u5927\u8CEA\u91CF\u30D6\u30E9\u30C3\u30AF\u30DB\u30FC\u30EB\u304C\u5B58\u5728\u3059\u308B\u8A3C\u62E0\u3068\u3001\u30D6\u30E9\u30C3\u30AF\u30DB\u30FC\u30EB\u306B\u95A2\u3059\u308B\u30C7\u30FC\u30BF\u304C\u3082\u305F\u3089\u3055\u308C\u3001\u3044\u3066\u5EA7A*\u304C\u305D\u306E\u5B58\u5728\u4F4D\u7F6E\u3067\u3042\u308B\u3068\u3044\u3046\u7D50\u8AD6\u306B\u306A\u3063\u3066\u3044\u305F\u304C\u30012022\u5E745\u670812\u65E5\u3001\u30D6\u30E9\u30C3\u30AF\u30DB\u30FC\u30EB\u306E\u76F4\u63A5\u89B3\u6E2C\u3092\u76EE\u6307\u3059\u56FD\u969B\u30D7\u30ED\u30B8\u30A7\u30AF\u30C8\u30A4\u30D9\u30F3\u30C8\u30DB\u30E9\u30A4\u30BA\u30F3\u30C6\u30EC\u30B9\u30B3\u30FC\u30D7 (EHT) \u306B\u3088\u308A\u3001\u3044\u3066\u5EA7A*\u306B\u5B58\u5728\u3059\u308B\u8D85\u5927\u8CEA\u91CF\u30D6\u30E9\u30C3\u30AF\u30DB\u30FC\u30EB\u306E\u76F4\u63A5\u89B3\u6E2C\u306B\u6210\u529F\u3057\u305F\u3068\u767A\u8868\u3055\u308C\u305F\u3002\u30D6\u30E9\u30C3\u30AF\u30DB\u30FC\u30EB\u306E\u76F4\u63A5\u89B3\u6E2C\u306B\u6210\u529F\u3057\u305F\u306E\u306FM87\u306E\u4E2D\u5FC3\u306B\u3042\u308B\u8D85\u5927\u8CEA\u91CF\u30D6\u30E9\u30C3\u30AF\u30DB\u30FC\u30EB\u306B\u6B21\u3044\u3067\u89B3\u6E2C\u53F2\u4E0A2\u4F8B\u76EE\u3067\u3042\u308B\u3002"@ja . "Sagittarius A*"@cs . . "\u3044\u3066\u5EA7A*"@ja . . . . . . . "1119064178"^^ . . . . . "This video sequence shows the motion of the dusty cloud G2 as it closes in on, and then passes, the supermassive black hole at the center of the Milky Way."@en . "200"^^ . "l"@en . . "Sagittarius A* (pronuncia-se Sagittarius A-estrela), tamb\u00E9m chamada de Sagit\u00E1rio A* (Sgr A* - sigla), \u00E9 uma fonte de r\u00E1dio astron\u00F4mica brilhante e muito compacta localizada no centro da Via L\u00E1ctea, perto da fronteira das constela\u00E7\u00F5es de Sagit\u00E1rio e Escorpi\u00E3o. \u00C9 parte de um objeto astron\u00F4mico maior conhecido como Sagittarius A. Acredita-se que Sagit\u00E1rio A* seja a localiza\u00E7\u00E3o de um buraco negro supermassivo, como aqueles que geralmente est\u00E3o nos centros da maioria das gal\u00E1xias espirais e el\u00EDpticas. As observa\u00E7\u00F5es da estrela S2 em \u00F3rbita ao redor de Sagit\u00E1rio A* foram usadas para mostrar sua presen\u00E7a e produzir dados sobre o buraco negro supermassivo central da Via L\u00E1ctea e levaram \u00E0 conclus\u00E3o de que Sagit\u00E1rio A* \u00E9 o local deste buraco negro. O buraco negro explodiu quase 3,5 milh\u00F5es de anos "@pt . . . . . "Sagittarius A*"@fr . . "Sagittarius A* (prononcata Sagittarius A stelo; mallongigite Sgr A*; la\u016D la latina nomo de la stela konstelacio Sagitario, do principe anka\u016D esperantigebla Sagitario A*) estas regiono de la kosmo en la konstelacio Sagitario. Temas pri fonto de radioondoj en la hipoteza centro de la galaksio Lakta Vojo. Sgr A*, estis malkovrita la 13-an kaj 15-an de februaro 1974 fare de astronomoj Bruce Balick kaj Robert Brown uzante la bazlinian interferometron (en Socorro) de la . La nomo Sgr A* estis elpensita fare de Brown en artikolo de 1982, \u0109ar la radiofonto estis \"ekscita\", kaj ekscititaj statoj de atomoj estas indikitaj per asteriskoj. Ekde la 1980-aj jaroj, ver\u015Dajnas ke la centra komponanto de Sgr A* estas nigra truo. En 1994, infraru\u011Daj kaj submilimetraj spektroskopiostudoj de Berkeley-teamo implicanta Nobel-premiiton Charles Hard Townes kaj estontan Nobelpremiiton Reinhard Genzel montris, ke la maso de Sgr A* estis ege koncentrita kaj je \u0109irka\u016D 3 milionoj da Sunoj. La\u016D la nuntempa stato de radioastronomiaj esploroj temas pri hipoteza supermasa Nigra Truo de proksimume 4,3 milionoj da sunaj masoj.. \u011Ci markas la lokon kiu estu la mezo de la Lakta Vojo. En majo 2022, astronomoj, uzante la internacian kunlaboron , publikigis foton de Sagittarius A* produktitan uzante datumojn de radio-observa\u0135oj en aprilo 2017 , tiele konfirmante ke la objekton estas nigra truo. \u0108i tiu estas la dua konfirmita bildo de nigra truo, post la supermasiva nigra truo de Messier 87 en 2019."@eo . . . . . . . . . "Sagittarius A*"@de . "\u0397 \u03B1\u03C3\u03C4\u03C1\u03BF\u03BD\u03BF\u03BC\u03B9\u03BA\u03AE \u03C0\u03B7\u03B3\u03AE \u03A4\u03BF\u03BE\u03CC\u03C4\u03B7\u03C2 A* (Sagittarius A*, Sgr A*) \u03B5\u03AF\u03BD\u03B1\u03B9 \u03BC\u03AF\u03B1 \u03B9\u03C3\u03C7\u03C5\u03C1\u03AE \u03BA\u03B1\u03B9 \u03C0\u03BF\u03BB\u03CD \u03BC\u03B9\u03BA\u03C1\u03AE \u03C3\u03B5 \u03B4\u03B9\u03B1\u03C3\u03C4\u03AC\u03C3\u03B5\u03B9\u03C2 , \u03C0\u03BF\u03C5 \u03B2\u03C1\u03AF\u03C3\u03BA\u03B5\u03C4\u03B1\u03B9 \u03C3\u03C4\u03BF \u03BA\u03AD\u03BD\u03C4\u03C1\u03BF \u03C4\u03BF\u03C5 \u0393\u03B1\u03BB\u03B1\u03BE\u03AF\u03B1 \u03BC\u03B1\u03C2, \u03C3\u03C4\u03BF\u03BD \u03B1\u03C3\u03C4\u03B5\u03C1\u03B9\u03C3\u03BC\u03CC \u03A4\u03BF\u03BE\u03CC\u03C4\u03B7, \u03B1\u03C0\u03CC \u03CC\u03C0\u03BF\u03C5 \u03BA\u03B1\u03B9 \u03B7 \u03BF\u03BD\u03BF\u03BC\u03B1\u03C3\u03AF\u03B1 \u03C4\u03B7\u03C2, \u03BA\u03BF\u03BD\u03C4\u03AC \u03C3\u03C4\u03B1 \u03C3\u03CD\u03BD\u03BF\u03C1\u03B1 \u03BC\u03B5 \u03C4\u03BF\u03BD \u03A3\u03BA\u03BF\u03C1\u03C0\u03B9\u03CC. \u039F\u03B9 \u03C3\u03C5\u03BD\u03C4\u03B5\u03C4\u03B1\u03B3\u03BC\u03AD\u03BD\u03B5\u03C2 \u03C4\u03B7\u03C2 \u03B5\u03AF\u03BD\u03B1\u03B9 \u03BF\u03C1\u03B8\u03AE \u03B1\u03BD\u03B1\u03C6\u03BF\u03C1\u03AC 17:45:40,04 \u03BA\u03B1\u03B9 \u03B1\u03C0\u03CC\u03BA\u03BB\u03B9\u03C3\u03B7 \u221229\u00B0 0\u0384 28,1\u0384\u0384. \u0391\u03C0\u03BF\u03C4\u03B5\u03BB\u03B5\u03AF \u03C4\u03BC\u03AE\u03BC\u03B1 \u03B5\u03BD\u03CC\u03C2 \u03BC\u03B5\u03B3\u03B1\u03BB\u03CD\u03C4\u03B5\u03C1\u03BF\u03C5 \u03C7\u03B1\u03C1\u03B1\u03BA\u03C4\u03B7\u03C1\u03B9\u03C3\u03C4\u03B9\u03BA\u03BF\u03CD \u03C0\u03BF\u03C5 \u03B5\u03AF\u03BD\u03B1\u03B9 \u03B3\u03BD\u03C9\u03C3\u03C4\u03CC \u03C9\u03C2 . \u039F Sgr A* \u03C0\u03B9\u03C3\u03C4\u03B5\u03CD\u03B5\u03C4\u03B1\u03B9 \u03CC\u03C4\u03B9 \u03B1\u03BD\u03C4\u03B9\u03C3\u03C4\u03BF\u03B9\u03C7\u03B5\u03AF \u03C3\u03B5 \u03BC\u03AF\u03B1 , \u03CC\u03C0\u03C9\u03C2 \u03B1\u03C5\u03C4\u03AD\u03C2 \u03C0\u03BF\u03C5 \u03B2\u03C1\u03AF\u03C3\u03BA\u03BF\u03BD\u03C4\u03B1\u03B9 \u03C3\u03C4\u03B1 \u03BA\u03AD\u03BD\u03C4\u03C1\u03B1 \u03C0\u03BF\u03BB\u03BB\u03CE\u03BD (\u03AF\u03C3\u03C9\u03C2 \u03C4\u03C9\u03BD \u03C0\u03B5\u03C1\u03B9\u03C3\u03C3\u03CC\u03C4\u03B5\u03C1\u03C9\u03BD) \u03BC\u03B5\u03B3\u03AC\u03BB\u03C9\u03BD \u03B3\u03B1\u03BB\u03B1\u03BE\u03B9\u03CE\u03BD. \u03A0\u03B1\u03C1\u03B1\u03C4\u03B7\u03C1\u03AE\u03C3\u03B5\u03B9\u03C2 \u03C4\u03BF\u03C5 \u03B1\u03C3\u03C4\u03AD\u03C1\u03B1 S2 \u03C0\u03BF\u03C5 \u03B2\u03C1\u03AF\u03C3\u03BA\u03B5\u03C4\u03B1\u03B9 \u03C3\u03B5 \u03C4\u03C1\u03BF\u03C7\u03B9\u03AC \u03C0\u03AD\u03C1\u03B9\u03BE \u03C4\u03BF\u03C5 \u03A4\u03BF\u03BE\u03CC\u03C4\u03B7 A* \u03AD\u03C7\u03BF\u03C5\u03BD \u03C7\u03C1\u03B7\u03C3\u03B9\u03BC\u03BF\u03C0\u03BF\u03B9\u03B7\u03B8\u03B5\u03AF \u03B3\u03B9\u03B1 \u03BD\u03B1 \u03B1\u03C0\u03BF\u03B4\u03B5\u03B9\u03C7\u03B8\u03B5\u03AF \u03B7 \u03C0\u03B1\u03C1\u03BF\u03C5\u03C3\u03AF\u03B1 \u03C4\u03B7\u03C2 \u03BC\u03B1\u03CD\u03C1\u03B7\u03C2 \u03C4\u03C1\u03CD\u03C0\u03B1\u03C2 \u03C3\u03C4\u03BF \u03BA\u03AD\u03BD\u03C4\u03C1\u03BF \u03C4\u03BF\u03C5 \u0393\u03B1\u03BB\u03B1\u03BE\u03AF\u03B1 \u03BC\u03B1\u03C2 \u03BA\u03B1\u03B9 \u03BD\u03B1 \u03B4\u03B9\u03B1\u03BA\u03C1\u03B9\u03B2\u03C9\u03B8\u03BF\u03CD\u03BD \u03C4\u03B1 \u03C7\u03B1\u03C1\u03B1\u03BA\u03C4\u03B7\u03C1\u03B9\u03C3\u03C4\u03B9\u03BA\u03AC \u03C4\u03B7\u03C2. \u03A4\u03BF \u03C3\u03C5\u03BC\u03C0\u03AD\u03C1\u03B1\u03C3\u03BC\u03B1 \u03B5\u03AF\u03BD\u03B1\u03B9 \u03CC\u03C4\u03B9 \u03B7 \u03C0\u03B7\u03B3\u03AE Sagittarius A* \u03B5\u03AF\u03BD\u03B1\u03B9 \u03C0\u03C1\u03AC\u03B3\u03BC\u03B1\u03C4\u03B9 \u03B7 \u03B8\u03AD\u03C3\u03B7 \u03C4\u03B7\u03C2 \u03BC\u03B1\u03CD\u03C1\u03B7\u03C2 \u03C4\u03C1\u03CD\u03C0\u03B1\u03C2. \u0397 \u03C0\u03B1\u03C1\u03BF\u03C5\u03C3\u03AF\u03B1 \u03C4\u03B7\u03C2 \u03BC\u03B1\u03CD\u03C1\u03B7\u03C2 \u03C4\u03C1\u03CD\u03C0\u03B1\u03C2 \u03B5\u03C0\u03B9\u03B2\u03B5\u03B2\u03B1\u03B9\u03CE\u03B8\u03B7\u03BA\u03B5 \u03BC\u03B5 \u03B1\u03C0\u03B5\u03B9\u03BA\u03CC\u03BD\u03B9\u03C3\u03AE \u03C4\u03B7\u03C2 \u03B1\u03C0\u03CC \u03C4\u03BF \u03A4\u03B7\u03BB\u03B5\u03C3\u03BA\u03CC\u03C0\u03B9\u03BF \u039F\u03C1\u03AF\u03B6\u03BF\u03BD\u03C4\u03B1 \u0393\u03B5\u03B3\u03BF\u03BD\u03CC\u03C4\u03C9\u03BD \u03C4\u03BF 2022."@el . . . "\u0421\u0442\u0440\u0456\u043B\u0435\u0446\u044C A*"@uk . "Sagittarius A*, ook wel bekend als Sgr A*, is een superzwaar zwart gat en een radiobron in het centrum van de Melkweg. Het object bevindt zich in de samengestelde radiobron Sagittarius A op 26.673 lichtjaar van de Zon. Het bevat 4,15 miljoen zonsmassa's in een gebied met een radius van minder dan 6,25 lichtuur. Het is daarmee het zwaarste zwarte gat in de Melkweg (andere zwarte gaten in de Melkweg zijn stellair)."@nl . . . . . . . "\u03A4\u03BF\u03BE\u03CC\u03C4\u03B7\u03C2 A*"@el .