. "Ross 614 \u00E8 uno dei sistemi binari pi\u00F9 vicino a noi ed \u00E8 formato da due piccole nane rosse. La coppia si trova ad una distanza di circa 13,3 anni luce \u00C8 una delle coppie di stelle pi\u00F9 piccole e leggere che si conoscono. Scoperte nel 1927 da F.E. Ross, entrambe sono di tipo spettrale M. Le due componenti, visualmente separate di 1,1 secondi d'arco, ruotano attorno al comune centro di massa in un periodo di 16,6 anni."@it . "Ross 614"@de . "\u0420\u043E\u0441\u0441 614"@ru . . . . . "B"@en . . . . . . "\u03A1\u03BF\u03C2 614"@el . . "K"@en . "Ross 614"@es . . "\u30ED\u30B9614\u306F\u3001\u592A\u967D\u7CFB\u304B\u308913.3\u5149\u5E74\u96E2\u308C\u305F\u8D64\u8272\u77EE\u661F\u306E\u9023\u661F\u3067\u3042\u308B\u3002\u3069\u3061\u3089\u3082\u5C0F\u3055\u304F\u6697\u3044\u8D64\u8272\u77EE\u661F\u306E\u305F\u3081\u3001\u5730\u7403\u304B\u3089\u8089\u773C\u3067\u898B\u308B\u3053\u3068\u306F\u3067\u304D\u306A\u3044\u3002\u96E2\u5FC3\u73870.38\u306E\u6955\u5186\u8ECC\u9053\u3067\u5171\u901A\u91CD\u5FC3\u306E\u5468\u308A\u309216.60\u5E74\u5468\u671F\u3067\u516C\u8EE2\u3057\u3066\u3044\u308B\u3002\u8ECC\u9053\u306E\u6E2C\u5B9A\u306B\u57FA\u3065\u304F\u8CEA\u91CF\u306F\u3001\u4E3B\u661F\u304C\u592A\u967D\u8CEA\u91CF\u306E0.2228\uFF08\u00B10.0055\uFF09\u500D\u3001\u4F34\u661F\u304C0.1107\uFF08\u00B10.0028\uFF09\u500D\u3068\u8A08\u7B97\u3055\u308C\u3066\u3044\u308B\u3002"@ja . . . . "Ross 614"@cs . . "~5.754/~7.38"@en . "1.19"^^ . . . "LHS 1850"@en . "Ross 614"@fr . "9281"^^ . . "A"@en . . . "11.15"^^ . . . . "Ross 614 je t\u011Bsn\u00E1 dvojhv\u011Bzda sest\u00E1vaj\u00EDc\u00ED ze dvou lehk\u00FDch \u010Derven\u00FDch trpasl\u00EDk\u016F. Orbit\u00E1ln\u00ED perioda je 16,6 let, vzd\u00E1lenost slo\u017Eek je 0,932\" a vzd\u00E1lenost syst\u00E9mu od Slunce je 13,3 sv\u011Bteln\u00FDch let."@cs . . . . "R"@en . "Ross 614"@it . . . . . . . "Ross 614 is een dubbelster van twee rode dwergen in het sterrenbeeld Monoceros op 13,42 lichtjaar van de zon."@nl . . . . . "Ross 614 (tamb\u00E9m conhecida por V577 Monocerotis e Gliese 234) \u00E9 um sistema estelar bin\u00E1rio formado por duas estrelas an\u00E3 vermelha localizado na constela\u00E7\u00E3o de Monoceros. Esta estrela tem uma magnitude de cerca de 11, sendo invis\u00EDvel a olho nu, embora seja uma das estrelas mais pr\u00F3ximas do Sol. Este sistema est\u00E1 entre os mais pr\u00F3ximos do nosso Sol a uma dist\u00E2ncia estimada de cerca de 13,3 anos-luz. Devido esta estrela est\u00E1 t\u00E3o perto da Terra ela \u00E9 muitas vezes objeto de estudo, da\u00ED o grande n\u00FAmero de designa\u00E7\u00F5es que ela conhecida."@pt . . . "Ross 614 ist ein Doppelsternsystem in 13,36 Lichtjahren Entfernung von der Sonne im Sternbild Einhorn und geh\u00F6rt damit zu den Sternen, die der Sonne am n\u00E4chsten sind. Es besteht aus zwei Roten Zwergen, die sich in ungef\u00E4hr 16,6 Jahren in einer Umlaufbahn mit einer Separation von \u00FCber 2,4 AU bewegen. Beide Sterne sind ver\u00E4nderlich und zeigen zuf\u00E4llige Flares. Ross 614 A ist ein UV-Ceti-Stern. Der gr\u00F6\u00DFere Prim\u00E4rstern tr\u00E4gt die Bezeichnung Ross 614 A (LHS 1849), der kleinere Sekund\u00E4rstern die Bezeichnung Ross 614 B (LHS 1850). Die Komponente A hat 22 % der Sonnenmasse und 25 % des Sonnenradius, die Komponente B etwa 11,7 % der Sonnenmasse und 13 % des Sonnenradius."@de . "J2000"@en . "B"@en . . "Ross 614"@sv . "Ross 614 A"@en . "\u0631\u0648\u0633 614"@ar . . "Ross 614 (HIP 30920 / GJ 234 A/B)\u200B es una estrella binaria situada a una distancia de 13,3 a\u00F1os luz del sistema solar en la constelaci\u00F3n de Monoceros. De magnitud aparente +11,15, no es observable a simple vista. El gran movimiento propio de esta estrella fue descubierto por Frank Elmore Ross en 1927. Ross 614 est\u00E1 compuesta por dos enanas rojas con una separaci\u00F3n en su semieje mayor de solo 0,932 segundos de arco, que corresponde a un per\u00EDodo orbital de 16,6 a\u00F1os. La estrella principal es de tipo espectral M4.5V y posee una masa de 0,22 veces masas solares; la estrella secundaria tiene una masa de 0,11 masas solares \u2014ligeramente mayor que Wolf 359, el tercer sistema m\u00E1s cercano al Sol\u2014 y superior a la inicialmente estimada.\u200B Asimismo, Ross 614 es una estrella fulgurante, recibiendo la denominaci\u00F3n de estrella variable V577 Monocerotis. Se han registrado llamaradas breves \u2014del orden de segundos\u2014 pero frecuentes. En un periodo de 4,3 horas se observaron cuatro llamaradas.\u200B"@es . "\u30ED\u30B9614"@ja . . "~8.06"@en . . . "UV CetiFlare star/"@en . . . . "J"@en . . "Ross 614 (HIP 30920 / GJ 234 A/B)\u200B es una estrella binaria situada a una distancia de 13,3 a\u00F1os luz del sistema solar en la constelaci\u00F3n de Monoceros. De magnitud aparente +11,15, no es observable a simple vista. El gran movimiento propio de esta estrella fue descubierto por Frank Elmore Ross en 1927. Asimismo, Ross 614 es una estrella fulgurante, recibiendo la denominaci\u00F3n de estrella variable V577 Monocerotis. Se han registrado llamaradas breves \u2014del orden de segundos\u2014 pero frecuentes. En un periodo de 4,3 horas se observaron cuatro llamaradas.\u200B"@es . . . . . . . . "0.1107"^^ . . . . "\u2212618.62"@en . . . . "\uB85C\uC2A4 614\uB294 \uC678\uBFD4\uC18C\uC790\uB9AC\uC5D0 \uC788\uB294 \uB450 \uAC1C\uC758 \uC801\uC0C9 \uC65C\uC131\uC73C\uB85C \uC774\uB8E8\uC5B4\uC838 \uC788\uB294 \uC30D\uC131\uC73C\uB85C, \uC9C0\uAD6C\uC5D0\uC11C 13.3\uAD11\uB144 \uB5A8\uC5B4\uC838 \uC788\uB2E4. \uB450 \uBCC4\uC758 \uACF5\uC804 \uC8FC\uAE30\uB294 16.6\uB144\uC73C\uB85C \uCC9C\uAD6C\uC0C1\uC5D0\uC11C \uC57D 0.932\" \uBD84\uB9AC\uB418\uC5B4 \uC788\uB2E4. \uB85C\uC2A4 614 A\uC640 B\uC758 \uAC89\uBCF4\uAE30 \uBC1D\uAE30\uB294 \uAC01\uAC01 11.25\uC640 14.23\uC73C\uB85C \uB9E8\uB208\uC73C\uB85C \uAD00\uCE21\uD558\uB294 \uAC83\uC740 \uBD88\uAC00\uB2A5\uD558\uB2E4."@ko . . . . . "0.73"^^ . "CCDM J06294-0249 B"@en . "H"@en . . "~12.77/~15.96"@en . "Ross 614 (HIP 30920 / GJ 234 A/B) \u00E9s un estel binari situat a una dist\u00E0ncia de 13,3 anys llum del sistema solar a la constel\u00B7laci\u00F3 de l'Unicorn, Monoceros. De magnitud aparent +11,15, no \u00E9s observable a ull nu. El gran moviment propi d'aquest estel va ser descobert per Frank Elmore Ross el 1927. Aix\u00ED mateix, Ross 614 \u00E9s un estel fulgurant, rebent la denominaci\u00F3 d'estel variable V577 Monocerotis. S'han registrat flamarades breus \u2014de l'ordre de segons\u2014 per\u00F2 freq\u00FCents. En un per\u00EDode de 4,3 hores es van observar quatre flamarades."@ca . "Ross 614 \u2013 jeden z najbli\u017Cszych uk\u0142ad\u00F3w podw\u00F3jnych gwiazd, para czerwonych kar\u0142\u00F3w o ma\u0142ej masie, typu widmowego M. Znajduje si\u0119 w gwiazdozbiorze Jednoro\u017Cca, w odleg\u0142o\u015Bci ok. 13,3 lat \u015Bwietlnych od S\u0142o\u0144ca."@pl . . . "\u0420\u043E\u0441\u0441 614 (GJ 234) \u2014 \u0434\u0432\u043E\u0439\u043D\u0430\u044F \u0437\u0432\u0435\u0437\u0434\u0430 \u0432 \u0441\u043E\u0437\u0432\u0435\u0437\u0434\u0438\u0438 \u0415\u0434\u0438\u043D\u043E\u0440\u043E\u0433. \u041D\u0430\u0445\u043E\u0434\u0438\u0442\u0441\u044F \u043D\u0430 \u0440\u0430\u0441\u0441\u0442\u043E\u044F\u043D\u0438\u0438 13,47 \u0441\u0432\u0435\u0442\u043E\u0432\u044B\u0445 \u043B\u0435\u0442 \u043E\u0442 \u0421\u043E\u043B\u043D\u0446\u0430."@ru . . . . . "Ross 614"@pl . . . . "\u039F \u03A1\u03BF\u03C2 614 (Ross 614) \u03AE Gliese 234 A \u03B5\u03AF\u03BD\u03B1\u03B9 \u03AD\u03BD\u03B1\u03C2 \u03B5\u03C1\u03C5\u03B8\u03C1\u03CC\u03C2 \u03BD\u03AC\u03BD\u03BF\u03C2 \u03B1\u03C3\u03C4\u03AD\u03C1\u03B1\u03C2 \u03B5\u03BA\u03BB\u03AC\u03BC\u03C8\u03B5\u03C9\u03BD \u03C4\u03CD\u03C0\u03BF\u03C5 \u03BA\u03B1\u03B9 \u03BF \u03C0\u03C1\u03C9\u03C4\u03B5\u03CD\u03C9\u03BD \u03B1\u03C3\u03C4\u03AD\u03C1\u03B1\u03C2 \u03B5\u03BD\u03CC\u03C2 \u03B3\u03B5\u03B9\u03C4\u03BF\u03BD\u03B9\u03BA\u03BF\u03CD \u03B4\u03B9\u03C0\u03BB\u03BF\u03CD \u03C3\u03C5\u03C3\u03C4\u03AE\u03BC\u03B1\u03C4\u03BF\u03C2 \u03B1\u03C3\u03C4\u03AD\u03C1\u03C9\u03BD \u03C3\u03C4\u03BF\u03BD \u03B1\u03C3\u03C4\u03B5\u03C1\u03B9\u03C3\u03BC\u03CC \u039C\u03BF\u03BD\u03CC\u03BA\u03B5\u03C1\u03C9. \u03A9\u03C2 \u03BC\u03B5\u03C4\u03B1\u03B2\u03BB\u03B7\u03C4\u03CC\u03C2 \u03B1\u03C3\u03C4\u03AD\u03C1\u03B1\u03C2 \u03B5\u03AF\u03BD\u03B1\u03B9 \u03B3\u03BD\u03C9\u03C3\u03C4\u03CC\u03C2 \u03C9\u03C2 V577 \u039C\u03BF\u03BD\u03BF\u03BA\u03AD\u03C1\u03C9\u03C4\u03BF\u03C2 (V577 Mon). \u039C\u03B5 \u03C6\u03B1\u03B9\u03BD\u03CC\u03BC\u03B5\u03BD\u03BF \u03BC\u03AD\u03B3\u03B5\u03B8\u03BF\u03C2 \u03C0\u03B5\u03C1\u03AF\u03C0\u03BF\u03C5 11, \u03B5\u03AF\u03BD\u03B1\u03B9 \u03B1\u03CC\u03C1\u03B1\u03C4\u03BF\u03C2 \u03BC\u03B5 \u03B3\u03C5\u03BC\u03BD\u03CC \u03BC\u03AC\u03C4\u03B9, \u03C0\u03B1\u03C1\u03CC\u03C4\u03B9 \u03B5\u03AF\u03BD\u03B1\u03B9 \u03AD\u03BD\u03B1\u03C2 \u03B1\u03C0\u03CC \u03C4\u03BF\u03C5\u03C2 \u03C0\u03BB\u03B7\u03C3\u03B9\u03AD\u03C3\u03C4\u03B5\u03C1\u03BF\u03C5\u03C2 \u03B1\u03C3\u03C4\u03AD\u03C1\u03B5\u03C2, \u03C3\u03B5 \u03B1\u03C0\u03CC\u03C3\u03C4\u03B1\u03C3\u03B7 13,3 \u03AD\u03C4\u03B7 \u03C6\u03C9\u03C4\u03CC\u03C2, \u03B3\u03B5\u03B3\u03BF\u03BD\u03CC\u03C2 \u03C0\u03BF\u03C5 \u03C3\u03C5\u03BD\u03AD\u03C4\u03B5\u03B9\u03BD\u03B5 \u03C3\u03C4\u03BF \u03BD\u03B1 \u03B1\u03C0\u03BF\u03C4\u03B5\u03BB\u03AD\u03C3\u03B5\u03B9 \u03C4\u03BF \u03B1\u03BD\u03C4\u03B9\u03BA\u03B5\u03AF\u03BC\u03B5\u03BD\u03BF \u03C0\u03BF\u03BB\u03BB\u03CE\u03BD \u03BC\u03B5\u03BB\u03B5\u03C4\u03CE\u03BD."@el . "The system"@en . . . . . "TYC+4789-3303-1"@en . . "Ross 614 (V577 Monocerotis) is a red dwarf UV Ceti flare star and it is the primary member of a nearby binary star system in the constellation of Monoceros. This star has a magnitude of about 11, making it invisible to the unaided eye even though it is one of the stars nearest to the Sun. This system is among the closest to the Sun at an estimated distance of about 13.3 light years. Because this star is so close to the Earth it is often the subject of study, hence the large number of designations by which it is known."@en . "Ross 614 is een dubbelster van twee rode dwergen in het sterrenbeeld Monoceros op 13,42 lichtjaar van de zon."@nl . . "Ross 614, CCDM J06294-0249, GJ 234, GCTP 1509.00, G 106-049, HIP 30920, LFT 473, LPM 239, LTT 2564, NLTT 16580, V577 Monocerotis"@en . "~5.486/~6.99"@en . . "Ross 614\uFF08V577 Monocerotis\uFF09\u662F\u4E00\u500B\u7D05\u77EE\u661F\u3002 \u5DF2\u96B1\u85CF\u90E8\u5206\u672A\u7FFB\u8B6F\u5185\u5BB9\uFF0C\u6B61\u8FCE\u53C3\u8207\u7FFB\u8B6F\u3002 flare star and it is the primary member of a nearby system in the constellation of . This star has a of about 11, making it invisible to the unaided eye even though it is one of the stars nearest to the Sun. \u8A72\u7D05\u77EE\u661F\u662F\u6700\u63A5\u8FD1\u592A\u967D\u7684\u7D05\u77EE\u661F\u4E4B\u4E00\uFF0C\u8DDD\u96E2\u7D0413.3\u5149\u5E74\u3002\u56E0\u70BA\u9019\u9846\u6046\u661F\u96E2\u5730\u7403\u5982\u6B64\u4E4B\u8FD1\uFF0C\u6240\u4EE5\u5B83\u7D93\u5E38\u6210\u70BA\u7814\u7A76\u7684\u4E3B\u984C\uFF0C\u800C\u4E14\u5B83\u6709\u591A\u7A2E\u7A31\u547C\u3002"@zh . . "Ross 614"@ca . "LHS 1849"@en . "1.72"^^ . "V"@en . . "Ross 614"@pt . . . . . . . "Ross 614"@en . . "\u0631\u0648\u0633 614 (V577 Monocerotis ) \u0647\u0648 \u0642\u0632\u0645 \u0623\u062D\u0645\u0631 UV Ceti \u0648\u0647\u0648 \u0639\u0636\u0648 \u0623\u0633\u0627\u0633\u064A \u0641\u064A \u0646\u0638\u0627\u0645 \u0646\u062C\u0645\u064A \u062B\u0646\u0627\u0626\u064A \u0642\u0631\u064A\u0628 \u0641\u064A \u0643\u0648\u0643\u0628\u0629 Monoceros . \u064A\u0628\u0644\u063A \u0627\u0644\u0642\u062F\u0631 \u0627\u0644\u0638\u0627\u0647\u0631\u064A \u0644\u0647\u0630\u0627 \u0627\u0644\u0646\u062C\u0645 \u062D\u0648\u0627\u0644\u064A 11 \u060C \u0645\u0645\u0627 \u064A\u062C\u0639\u0644\u0647 \u063A\u064A\u0631 \u0645\u0631\u0626\u064A \u0628\u0627\u0644\u0639\u064A\u0646 \u0627\u0644\u0645\u062C\u0631\u062F\u0629\u060C \u0639\u0644\u0649 \u0627\u0644\u0631\u063A\u0645 \u0645\u0646 \u0623\u0646\u0647 \u0623\u062D\u062F \u0627\u0644\u0646\u062C\u0648\u0645 \u0627\u0644\u0623\u0642\u0631\u0628 \u0625\u0644\u0649 \u0627\u0644\u0634\u0645\u0633. \u0647\u0630\u0627 \u0627\u0644\u0646\u0638\u0627\u0645 \u0647\u0648 \u0645\u0646 \u0628\u064A\u0646 \u0623\u0642\u0631\u0628 \u0627\u0644\u0646\u062C\u0648\u0645 \u0625\u0644\u0649 \u0627\u0644\u0634\u0645\u0633 \u0628\u0645\u0633\u0627\u0641\u0629 \u062A\u0642\u062F\u0631 \u0628\u062D\u0648\u0627\u0644\u064A 13.3 \u0633\u0646\u0629 \u0636\u0648\u0626\u064A\u0629 . \u0646\u0638\u0631\u064B\u0627 \u0644\u0623\u0646 \u0647\u0630\u0627 \u0627\u0644\u0646\u062C\u0645 \u0642\u0631\u064A\u0628 \u062C\u062F\u064B\u0627 \u0645\u0646 \u0627\u0644\u0623\u0631\u0636\u060C \u0641\u0625\u0646\u0647 \u063A\u0627\u0644\u0628\u064B\u0627 \u0645\u0627 \u064A\u0643\u0648\u0646 \u0645\u0648\u0636\u0648\u0639\u064B\u0627 \u0644\u0644\u062F\u0631\u0627\u0633\u0629\u061B \u0648\u0628\u0627\u0644\u062A\u0627\u0644\u064A \u0646\u0639\u0631\u0641 \u0639\u0646\u0647 \u0627\u0644\u0639\u062F\u062F \u0627\u0644\u0643\u0628\u064A\u0631 \u0645\u0646 \u0627\u0644\u0628\u064A\u0627\u0646\u0627\u062A \u0648\u062E\u0635\u0627\u0626\u0635\u0647."@ar . "\u30ED\u30B9614\u306F\u3001\u592A\u967D\u7CFB\u304B\u308913.3\u5149\u5E74\u96E2\u308C\u305F\u8D64\u8272\u77EE\u661F\u306E\u9023\u661F\u3067\u3042\u308B\u3002\u3069\u3061\u3089\u3082\u5C0F\u3055\u304F\u6697\u3044\u8D64\u8272\u77EE\u661F\u306E\u305F\u3081\u3001\u5730\u7403\u304B\u3089\u8089\u773C\u3067\u898B\u308B\u3053\u3068\u306F\u3067\u304D\u306A\u3044\u3002\u96E2\u5FC3\u73870.38\u306E\u6955\u5186\u8ECC\u9053\u3067\u5171\u901A\u91CD\u5FC3\u306E\u5468\u308A\u309216.60\u5E74\u5468\u671F\u3067\u516C\u8EE2\u3057\u3066\u3044\u308B\u3002\u8ECC\u9053\u306E\u6E2C\u5B9A\u306B\u57FA\u3065\u304F\u8CEA\u91CF\u306F\u3001\u4E3B\u661F\u304C\u592A\u967D\u8CEA\u91CF\u306E0.2228\uFF08\u00B10.0055\uFF09\u500D\u3001\u4F34\u661F\u304C0.1107\uFF08\u00B10.0028\uFF09\u500D\u3068\u8A08\u7B97\u3055\u308C\u3066\u3044\u308B\u3002"@ja . "694.73"^^ . . . . . "Ross 614 \u00E8 uno dei sistemi binari pi\u00F9 vicino a noi ed \u00E8 formato da due piccole nane rosse. La coppia si trova ad una distanza di circa 13,3 anni luce \u00C8 una delle coppie di stelle pi\u00F9 piccole e leggere che si conoscono. Scoperte nel 1927 da F.E. Ross, entrambe sono di tipo spettrale M. Le due componenti, visualmente separate di 1,1 secondi d'arco, ruotano attorno al comune centro di massa in un periodo di 16,6 anni."@it . . . . . "13.09"^^ . . . . . "I"@en . "\u0420\u043E\u0441\u0441 614 (GJ 234) \u2014 \u0434\u0432\u043E\u0439\u043D\u0430\u044F \u0437\u0432\u0435\u0437\u0434\u0430 \u0432 \u0441\u043E\u0437\u0432\u0435\u0437\u0434\u0438\u0438 \u0415\u0434\u0438\u043D\u043E\u0440\u043E\u0433. \u041D\u0430\u0445\u043E\u0434\u0438\u0442\u0441\u044F \u043D\u0430 \u0440\u0430\u0441\u0441\u0442\u043E\u044F\u043D\u0438\u0438 13,47 \u0441\u0432\u0435\u0442\u043E\u0432\u044B\u0445 \u043B\u0435\u0442 \u043E\u0442 \u0421\u043E\u043B\u043D\u0446\u0430."@ru . . . "\u0631\u0648\u0633 614 (V577 Monocerotis ) \u0647\u0648 \u0642\u0632\u0645 \u0623\u062D\u0645\u0631 UV Ceti \u0648\u0647\u0648 \u0639\u0636\u0648 \u0623\u0633\u0627\u0633\u064A \u0641\u064A \u0646\u0638\u0627\u0645 \u0646\u062C\u0645\u064A \u062B\u0646\u0627\u0626\u064A \u0642\u0631\u064A\u0628 \u0641\u064A \u0643\u0648\u0643\u0628\u0629 Monoceros . \u064A\u0628\u0644\u063A \u0627\u0644\u0642\u062F\u0631 \u0627\u0644\u0638\u0627\u0647\u0631\u064A \u0644\u0647\u0630\u0627 \u0627\u0644\u0646\u062C\u0645 \u062D\u0648\u0627\u0644\u064A 11 \u060C \u0645\u0645\u0627 \u064A\u062C\u0639\u0644\u0647 \u063A\u064A\u0631 \u0645\u0631\u0626\u064A \u0628\u0627\u0644\u0639\u064A\u0646 \u0627\u0644\u0645\u062C\u0631\u062F\u0629\u060C \u0639\u0644\u0649 \u0627\u0644\u0631\u063A\u0645 \u0645\u0646 \u0623\u0646\u0647 \u0623\u062D\u062F \u0627\u0644\u0646\u062C\u0648\u0645 \u0627\u0644\u0623\u0642\u0631\u0628 \u0625\u0644\u0649 \u0627\u0644\u0634\u0645\u0633. \u0647\u0630\u0627 \u0627\u0644\u0646\u0638\u0627\u0645 \u0647\u0648 \u0645\u0646 \u0628\u064A\u0646 \u0623\u0642\u0631\u0628 \u0627\u0644\u0646\u062C\u0648\u0645 \u0625\u0644\u0649 \u0627\u0644\u0634\u0645\u0633 \u0628\u0645\u0633\u0627\u0641\u0629 \u062A\u0642\u062F\u0631 \u0628\u062D\u0648\u0627\u0644\u064A 13.3 \u0633\u0646\u0629 \u0636\u0648\u0626\u064A\u0629 . \u0646\u0638\u0631\u064B\u0627 \u0644\u0623\u0646 \u0647\u0630\u0627 \u0627\u0644\u0646\u062C\u0645 \u0642\u0631\u064A\u0628 \u062C\u062F\u064B\u0627 \u0645\u0646 \u0627\u0644\u0623\u0631\u0636\u060C \u0641\u0625\u0646\u0647 \u063A\u0627\u0644\u0628\u064B\u0627 \u0645\u0627 \u064A\u0643\u0648\u0646 \u0645\u0648\u0636\u0648\u0639\u064B\u0627 \u0644\u0644\u062F\u0631\u0627\u0633\u0629\u061B \u0648\u0628\u0627\u0644\u062A\u0627\u0644\u064A \u0646\u0639\u0631\u0641 \u0639\u0646\u0647 \u0627\u0644\u0639\u062F\u062F \u0627\u0644\u0643\u0628\u064A\u0631 \u0645\u0646 \u0627\u0644\u0628\u064A\u0627\u0646\u0627\u062A \u0648\u062E\u0635\u0627\u0626\u0635\u0647."@ar . . "\u039F \u03A1\u03BF\u03C2 614 (Ross 614) \u03AE Gliese 234 A \u03B5\u03AF\u03BD\u03B1\u03B9 \u03AD\u03BD\u03B1\u03C2 \u03B5\u03C1\u03C5\u03B8\u03C1\u03CC\u03C2 \u03BD\u03AC\u03BD\u03BF\u03C2 \u03B1\u03C3\u03C4\u03AD\u03C1\u03B1\u03C2 \u03B5\u03BA\u03BB\u03AC\u03BC\u03C8\u03B5\u03C9\u03BD \u03C4\u03CD\u03C0\u03BF\u03C5 \u03BA\u03B1\u03B9 \u03BF \u03C0\u03C1\u03C9\u03C4\u03B5\u03CD\u03C9\u03BD \u03B1\u03C3\u03C4\u03AD\u03C1\u03B1\u03C2 \u03B5\u03BD\u03CC\u03C2 \u03B3\u03B5\u03B9\u03C4\u03BF\u03BD\u03B9\u03BA\u03BF\u03CD \u03B4\u03B9\u03C0\u03BB\u03BF\u03CD \u03C3\u03C5\u03C3\u03C4\u03AE\u03BC\u03B1\u03C4\u03BF\u03C2 \u03B1\u03C3\u03C4\u03AD\u03C1\u03C9\u03BD \u03C3\u03C4\u03BF\u03BD \u03B1\u03C3\u03C4\u03B5\u03C1\u03B9\u03C3\u03BC\u03CC \u039C\u03BF\u03BD\u03CC\u03BA\u03B5\u03C1\u03C9. \u03A9\u03C2 \u03BC\u03B5\u03C4\u03B1\u03B2\u03BB\u03B7\u03C4\u03CC\u03C2 \u03B1\u03C3\u03C4\u03AD\u03C1\u03B1\u03C2 \u03B5\u03AF\u03BD\u03B1\u03B9 \u03B3\u03BD\u03C9\u03C3\u03C4\u03CC\u03C2 \u03C9\u03C2 V577 \u039C\u03BF\u03BD\u03BF\u03BA\u03AD\u03C1\u03C9\u03C4\u03BF\u03C2 (V577 Mon). \u039C\u03B5 \u03C6\u03B1\u03B9\u03BD\u03CC\u03BC\u03B5\u03BD\u03BF \u03BC\u03AD\u03B3\u03B5\u03B8\u03BF\u03C2 \u03C0\u03B5\u03C1\u03AF\u03C0\u03BF\u03C5 11, \u03B5\u03AF\u03BD\u03B1\u03B9 \u03B1\u03CC\u03C1\u03B1\u03C4\u03BF\u03C2 \u03BC\u03B5 \u03B3\u03C5\u03BC\u03BD\u03CC \u03BC\u03AC\u03C4\u03B9, \u03C0\u03B1\u03C1\u03CC\u03C4\u03B9 \u03B5\u03AF\u03BD\u03B1\u03B9 \u03AD\u03BD\u03B1\u03C2 \u03B1\u03C0\u03CC \u03C4\u03BF\u03C5\u03C2 \u03C0\u03BB\u03B7\u03C3\u03B9\u03AD\u03C3\u03C4\u03B5\u03C1\u03BF\u03C5\u03C2 \u03B1\u03C3\u03C4\u03AD\u03C1\u03B5\u03C2, \u03C3\u03B5 \u03B1\u03C0\u03CC\u03C3\u03C4\u03B1\u03C3\u03B7 13,3 \u03AD\u03C4\u03B7 \u03C6\u03C9\u03C4\u03CC\u03C2, \u03B3\u03B5\u03B3\u03BF\u03BD\u03CC\u03C2 \u03C0\u03BF\u03C5 \u03C3\u03C5\u03BD\u03AD\u03C4\u03B5\u03B9\u03BD\u03B5 \u03C3\u03C4\u03BF \u03BD\u03B1 \u03B1\u03C0\u03BF\u03C4\u03B5\u03BB\u03AD\u03C3\u03B5\u03B9 \u03C4\u03BF \u03B1\u03BD\u03C4\u03B9\u03BA\u03B5\u03AF\u03BC\u03B5\u03BD\u03BF \u03C0\u03BF\u03BB\u03BB\u03CE\u03BD \u03BC\u03B5\u03BB\u03B5\u03C4\u03CE\u03BD."@el . . . "Ross+614"@en . . . . . "Ross 614"@nl . "M4.5V/M8V"@en . . . . "244.07"^^ . "+18.2"@en . "1107393508"^^ . "14.23"^^ . . "1.1012"^^ . "GJ+234+B"@en . "2484274"^^ . . "~6.376/~8.17"@en . . . "Ross 614 ist ein Doppelsternsystem in 13,36 Lichtjahren Entfernung von der Sonne im Sternbild Einhorn und geh\u00F6rt damit zu den Sternen, die der Sonne am n\u00E4chsten sind. Es besteht aus zwei Roten Zwergen, die sich in ungef\u00E4hr 16,6 Jahren in einer Umlaufbahn mit einer Separation von \u00FCber 2,4 AU bewegen. Beide Sterne sind ver\u00E4nderlich und zeigen zuf\u00E4llige Flares. Ross 614 A ist ein UV-Ceti-Stern."@de . . "Ross 614 (V577 Monocerotis) is a red dwarf UV Ceti flare star and it is the primary member of a nearby binary star system in the constellation of Monoceros. This star has a magnitude of about 11, making it invisible to the unaided eye even though it is one of the stars nearest to the Sun. This system is among the closest to the Sun at an estimated distance of about 13.3 light years. Because this star is so close to the Earth it is often the subject of study, hence the large number of designations by which it is known."@en . . "CCDM J06294-0249 A"@en . "\u7F85\u65AF614"@zh . "Ross 614 est la premi\u00E8re \u00E9toile binaire dont la binarit\u00E9 a \u00E9t\u00E9 d\u00E9couverte par astrom\u00E9trie photographique. Elle est constitu\u00E9e de deux naines rouges de faible masse, situ\u00E9e dans la constellation de la Licorne. La p\u00E9riode orbitale est d'environ 16,6 ans et le demi-grand axe a une s\u00E9paration angulaire de seulement 0,932\". Ce syst\u00E8me est parmi les plus proches de notre Soleil, \u00E0 une distance de 13,4 ann\u00E9es-lumi\u00E8re. L'\u00E9toile primaire a \u00E9t\u00E9 d\u00E9couverte en 1927 par Frank E. Ross (1874-1960) avec le t\u00E9lescope de 40 pouces de l'observatoire Yerkes. L'\u00E9toile secondaire a \u00E9t\u00E9 d\u00E9tect\u00E9e en 1936 par (en) (1906-1972) \u00E0 partir de photographies prises avec le t\u00E9lescope de 26 pouces de l'observatoire McCormick."@fr . "Ross 614 est la premi\u00E8re \u00E9toile binaire dont la binarit\u00E9 a \u00E9t\u00E9 d\u00E9couverte par astrom\u00E9trie photographique. Elle est constitu\u00E9e de deux naines rouges de faible masse, situ\u00E9e dans la constellation de la Licorne. La p\u00E9riode orbitale est d'environ 16,6 ans et le demi-grand axe a une s\u00E9paration angulaire de seulement 0,932\". Ce syst\u00E8me est parmi les plus proches de notre Soleil, \u00E0 une distance de 13,4 ann\u00E9es-lumi\u00E8re."@fr . "\uB85C\uC2A4 614\uB294 \uC678\uBFD4\uC18C\uC790\uB9AC\uC5D0 \uC788\uB294 \uB450 \uAC1C\uC758 \uC801\uC0C9 \uC65C\uC131\uC73C\uB85C \uC774\uB8E8\uC5B4\uC838 \uC788\uB294 \uC30D\uC131\uC73C\uB85C, \uC9C0\uAD6C\uC5D0\uC11C 13.3\uAD11\uB144 \uB5A8\uC5B4\uC838 \uC788\uB2E4. \uB450 \uBCC4\uC758 \uACF5\uC804 \uC8FC\uAE30\uB294 16.6\uB144\uC73C\uB85C \uCC9C\uAD6C\uC0C1\uC5D0\uC11C \uC57D 0.932\" \uBD84\uB9AC\uB418\uC5B4 \uC788\uB2E4. \uB85C\uC2A4 614 A\uC640 B\uC758 \uAC89\uBCF4\uAE30 \uBC1D\uAE30\uB294 \uAC01\uAC01 11.25\uC640 14.23\uC73C\uB85C \uB9E8\uB208\uC73C\uB85C \uAD00\uCE21\uD558\uB294 \uAC83\uC740 \uBD88\uAC00\uB2A5\uD558\uB2E4."@ko . . . . "~11.08/~14.23"@en . . "Ross 614 je t\u011Bsn\u00E1 dvojhv\u011Bzda sest\u00E1vaj\u00EDc\u00ED ze dvou lehk\u00FDch \u010Derven\u00FDch trpasl\u00EDk\u016F. Orbit\u00E1ln\u00ED perioda je 16,6 let, vzd\u00E1lenost slo\u017Eek je 0,932\" a vzd\u00E1lenost syst\u00E9mu od Slunce je 13,3 sv\u011Bteln\u00FDch let."@cs . "Ross 614 \u2013 jeden z najbli\u017Cszych uk\u0142ad\u00F3w podw\u00F3jnych gwiazd, para czerwonych kar\u0142\u00F3w o ma\u0142ej masie, typu widmowego M. Znajduje si\u0119 w gwiazdozbiorze Jednoro\u017Cca, w odleg\u0142o\u015Bci ok. 13,3 lat \u015Bwietlnych od S\u0142o\u0144ca."@pl . . "Ross 614 B"@en . . "Ross 614 (HIP 30920 / GJ 234 A/B) \u00E9s un estel binari situat a una dist\u00E0ncia de 13,3 anys llum del sistema solar a la constel\u00B7laci\u00F3 de l'Unicorn, Monoceros. De magnitud aparent +11,15, no \u00E9s observable a ull nu. El gran moviment propi d'aquest estel va ser descobert per Frank Elmore Ross el 1927. Ross 614 est\u00E0 composta per dues nanes vermelles amb una separaci\u00F3 en el seu semieix major de sols 0,932 segons d'arc, que correspon a un per\u00EDode orbital de 16,6 anys. L'estel principal \u00E9s de tipus espectral M4.5V i posseeix una massa de 0,22 vegades masses solars; l'estel secundari t\u00E9 una massa de 0,11 masses solars \u2014lleugerament major que Wolf 359, el tercer sistema m\u00E9s proper al Sol\u2014 i superior a la inicialment estimada. Aix\u00ED mateix, Ross 614 \u00E9s un estel fulgurant, rebent la denominaci\u00F3 d'estel variable V577 Monocerotis. S'han registrat flamarades breus \u2014de l'ordre de segons\u2014 per\u00F2 freq\u00FCents. En un per\u00EDode de 4,3 hores es van observar quatre flamarades."@ca . "Ross 614 (tamb\u00E9m conhecida por V577 Monocerotis e Gliese 234) \u00E9 um sistema estelar bin\u00E1rio formado por duas estrelas an\u00E3 vermelha localizado na constela\u00E7\u00E3o de Monoceros. Esta estrela tem uma magnitude de cerca de 11, sendo invis\u00EDvel a olho nu, embora seja uma das estrelas mais pr\u00F3ximas do Sol. Este sistema est\u00E1 entre os mais pr\u00F3ximos do nosso Sol a uma dist\u00E2ncia estimada de cerca de 13,3 anos-luz. Devido esta estrela est\u00E1 t\u00E3o perto da Terra ela \u00E9 muitas vezes objeto de estudo, da\u00ED o grande n\u00FAmero de designa\u00E7\u00F5es que ela conhecida."@pt . "0.2228"^^ . "~9.78"@en . . "Ross 614\uFF08V577 Monocerotis\uFF09\u662F\u4E00\u500B\u7D05\u77EE\u661F\u3002 \u5DF2\u96B1\u85CF\u90E8\u5206\u672A\u7FFB\u8B6F\u5185\u5BB9\uFF0C\u6B61\u8FCE\u53C3\u8207\u7FFB\u8B6F\u3002 flare star and it is the primary member of a nearby system in the constellation of . This star has a of about 11, making it invisible to the unaided eye even though it is one of the stars nearest to the Sun. \u8A72\u7D05\u77EE\u661F\u662F\u6700\u63A5\u8FD1\u592A\u967D\u7684\u7D05\u77EE\u661F\u4E4B\u4E00\uFF0C\u8DDD\u96E2\u7D0413.3\u5149\u5E74\u3002\u56E0\u70BA\u9019\u9846\u6046\u661F\u96E2\u5730\u7403\u5982\u6B64\u4E4B\u8FD1\uFF0C\u6240\u4EE5\u5B83\u7D93\u5E38\u6210\u70BA\u7814\u7A76\u7684\u4E3B\u984C\uFF0C\u800C\u4E14\u5B83\u6709\u591A\u7A2E\u7A31\u547C\u3002"@zh . . . . "\uB85C\uC2A4 614"@ko . . "Ross 614"@en .