. "HD 114762 A b"@ru . . . . "HD 114762 b is a small red dwarf star, in the HD 114762 system, formerly thought to be a massive gaseous extrasolar planet, approximately 126 light-years (38.6 pc) away in the constellation of Coma Berenices. This optically undetected companion to the late F-type main-sequence star HD 114762 was discovered in 1989 by Latham, et al., and confirmed in an October 1991 paper by Cochran, et al. It was thought to be the first discovered exoplanet (although its existence was confirmed after those around PSR B1257+12.) The object orbits the primary star every 83.9 days at an approximate distance of 0.37 AU, with an orbital eccentricity of 0.57; for comparison, this orbit is similar to that of Mercury but with almost three times the eccentricity. Based on the radial velocity measurements alone, it was estimated to have a minimum mass of 11.069\u00B10.063 MJ (at 90\u00B0) and a probable mass of approximately 63.2 MJ (at 10\u00B0). However, analysis of its astrometric perturbation of its host star in 2019 found it to have an extremely low inclination of only 6.23+1.97\u22121.26 degrees, giving it a true mass of 107+20\u221227 MJ and putting it well outside of the range of planetary masses (less than 13 MJ). HD 114762 b was thought for a time to be the first extrasolar planet ever detected, predating the 1992 pulsar planets found around PSR B1257+12 and main-sequence yellow dwarf 51 Pegasi. However, now that it has been found to not be a planet, the planets found orbiting PRS B1257+12 were indeed the first exoplanets ever found. At an event celebrating the career of discoverer David Latham and attended by his colleagues and collaborators, the object was informally dubbed \"Latham's Planet\". However, this name has no official standing with the International Astronomical Union."@en . . . . "HD 114762 b"@in . . "HD 114762 A b \u2014 \u044D\u043A\u0437\u043E\u043F\u043B\u0430\u043D\u0435\u0442\u0430 \u0432 \u0434\u0432\u043E\u0439\u043D\u043E\u0439 \u0441\u0438\u0441\u0442\u0435\u043C\u0435 HD 114762 \u0432 \u0441\u043E\u0437\u0432\u0435\u0437\u0434\u0438\u0438 \u0412\u043E\u043B\u043E\u0441\u044B \u0412\u0435\u0440\u043E\u043D\u0438\u043A\u0438. \u0411\u044B\u043B\u0430 \u043E\u0442\u043A\u0440\u044B\u0442\u0430 \u0414. \u041B\u0430\u0442\u0430\u043C\u043E\u043C \u0432 1989 \u0433\u043E\u0434\u0443, \u043D\u043E \u043E\u043A\u043E\u043D\u0447\u0430\u0442\u0435\u043B\u044C\u043D\u043E \u043F\u043E\u0434\u0442\u0432\u0435\u0440\u0436\u0434\u0435\u043D\u0430 \u043B\u0438\u0448\u044C \u0432 1999 \u0433\u043E\u0434\u0443. HD 114762 A b \u043D\u0430\u0445\u043E\u0434\u0438\u0442\u0441\u044F \u0443 \u0437\u0432\u0435\u0437\u0434\u044B F-\u043A\u043B\u0430\u0441\u0441\u0430 \u043D\u0430 \u0440\u0430\u0441\u0441\u0442\u043E\u044F\u043D\u0438\u0438 132 \u0441\u0432\u0435\u0442\u043E\u0432\u044B\u0445 \u043B\u0435\u0442 \u043E\u0442 \u0421\u043E\u043B\u043D\u0446\u0430. \u041E\u0431\u043E\u0440\u043E\u0442 \u0432\u043E\u043A\u0440\u0443\u0433 \u0441\u0432\u043E\u0435\u0439 \u0437\u0432\u0435\u0437\u0434\u044B, \u0441\u043E\u0432\u0435\u0440\u0448\u0430\u0435\u0442 \u043F\u043E \u0432\u044B\u0442\u044F\u043D\u0443\u0442\u043E\u0439 \u043E\u0440\u0431\u0438\u0442\u0435 (\u044D\u043A\u0441\u0446\u0435\u043D\u0442\u0440\u0438\u0441\u0438\u0442\u0435\u0442 0,3359) \u043F\u043E\u0447\u0442\u0438 \u0437\u0430 \u0442\u0440\u0438 \u043C\u0435\u0441\u044F\u0446\u0430 (83 \u0434\u043D\u044F), \u043D\u0430 \u0440\u0430\u0441\u0441\u0442\u043E\u044F\u043D\u0438\u0438 0,363 (0,241\u20140,485) \u0430. \u0435. (\u0442\u043E \u0435\u0441\u0442\u044C, \u043F\u0440\u0438\u043C\u0435\u0440\u043D\u043E, \u043A\u0430\u043A \u041C\u0435\u0440\u043A\u0443\u0440\u0438\u0439 \u043E\u0442 \u0421\u043E\u043B\u043D\u0446\u0430). \u041F\u043E\u0441\u043A\u043E\u043B\u044C\u043A\u0443, \u0432\u0435\u0440\u0445\u043D\u044F\u044F \u043F\u043B\u0430\u043D\u043A\u0430 \u043C\u0430\u043A\u0441\u0438\u043C\u0430\u043B\u044C\u043D\u043E\u0439 \u043C\u0430\u0441\u0441\u044B \u043D\u0435 \u043E\u043F\u0440\u0435\u0434\u0435\u043B\u0435\u043D\u0430, HD 114762 A b \u043C\u043E\u0436\u0435\u0442 \u043E\u043A\u0430\u0437\u0430\u0442\u044C\u0441\u044F \u043D\u0435 \u044D\u043A\u0437\u043E\u043F\u043B\u0430\u043D\u0435\u0442\u043E\u0439, \u0430 \u043A\u043E\u0440\u0438\u0447\u043D\u0435\u0432\u044B\u043C \u043A\u0430\u0440\u043B\u0438\u043A\u043E\u043C. \u041C\u0438\u043D\u0438\u043C\u0430\u043B\u044C\u043D\u0430\u044F \u043C\u0430\u0441\u0441\u0430 HD 114762 A b \u2014 11 \u043C\u0430\u0441\u0441 \u042E\u043F\u0438\u0442\u0435\u0440\u0430. \u041E\u043F\u0442\u0438\u0447\u0435\u0441\u043A\u0438, \u044D\u0442\u043E\u0442 \u043A\u043E\u043C\u043F\u0430\u043D\u044C\u043E\u043D \u043D\u0435 \u043E\u0431\u043D\u0430\u0440\u0443\u0436\u0435\u043D. \u0415\u0441\u043B\u0438 \u043E\u043A\u0430\u0436\u0435\u0442\u0441\u044F, \u0447\u0442\u043E HD 114762 A b \u044D\u043A\u0437\u043E\u043F\u043B\u0430\u043D\u0435\u0442\u0430, \u0442\u043E \u043E\u043D\u0430 \u0431\u0443\u0434\u0435\u0442 \u0432\u0442\u043E\u0440\u043E\u0439, \u0432\u0441\u043B\u0435\u0434 \u0437\u0430 \u0413\u0430\u043C\u043C\u0430 \u0426\u0435\u0444\u0435\u044F A b, \u0432\u043D\u0435\u0441\u043E\u043B\u043D\u0435\u0447\u043D\u043E\u0439 \u043F\u043B\u0430\u043D\u0435\u0442\u043E\u0439, \u043E\u0431\u043D\u0430\u0440\u0443\u0436\u0435\u043D\u043D\u043E\u0439"@ru . "HD 114762 b"@en . "HD 114762 b\u662F\u4E00\u500B\u4F4D\u65BC\u540E\u9AEE\u5EA7\uFF0C\u8DDD\u96E2\u5730\u7403\u7D04132\u5149\u5E74\u7684\u5019\u9078\u7CFB\u5916\u884C\u661F\u6216\u68D5\u77EE\u661F\u3002"@zh . "1120695904"^^ . . . "HD 114762 b"@zh . "HD 114762 b\uB294 \uC9C0\uAD6C\uB85C\uBD80\uD130 \uBA38\uB9AC\uD138\uC790\uB9AC \uBC29\uD5A5\uC73C\uB85C \uC57D 132\uAD11\uB144 \uB5A8\uC5B4\uC9C4 \uACF3\uC5D0 \uC788\uB294 \uD56D\uC131 \uC8FC\uC704\uB97C \uB3C4\uB294 \uC678\uACC4 \uD589\uC131\uC774\uB2E4. \uC774 \uD589\uC131\uC758 \uCD5C\uC18C \uC9C8\uB7C9\uC740 \uBAA9\uC131\uC758 11\uBC30\uC5D0 \uC774\uB974\uB294\uB370, \uADA4\uB3C4\uACBD\uC0AC\uAC01\uC774 \uBC1D\uD600\uC9C8 \uACBD\uC6B0 \uC774 \uAC12\uC740 \uB354 \uCEE4\uC9C8 \uAC00\uB2A5\uC131\uC774 \uC788\uC73C\uBA70, \uAC08\uC0C9 \uC65C\uC131\uC77C \uD655\uB960\uC774 \uB192\uB2E4. 1989\uB144 \uB370\uC774\uBE44\uB4DC \uB77C\uC0BC \uC5F0\uAD6C\uC9C4\uC774 \uBC1C\uACAC\uD588\uB2E4. 2006\uB144 \uAE30\uC900\uC73C\uB85C \uC774 \uD589\uC131\uC774 \uC815\uD655\uD788 \uAC00\uC2A4 \uD589\uC131\uC778\uC9C0, \uAC08\uC0C9 \uC65C\uC131\uC778\uC9C0 \uC544\uB2C8\uBA74 \uC801\uC0C9 \uC65C\uC131\uC778\uC9C0\uB294 \uC815\uD655\uD788 \uBC1D\uD600\uC9C0\uC9C0 \uC54A\uC558\uB2E4. \uADF9\uB2E8\uC801\uC778 \uACBD\uC6B0 \uBAA9\uC131\uC9C8\uB7C9\uC758 145\uBC30\uAE4C\uC9C0 \uBB34\uAC70\uC6CC\uC9C8 \uC218 \uC788\uB294\uB370, \uC774 \uC815\uB3C4\uB77C\uBA74 \uC774\uBBF8 \uD56D\uC131\uC758 \uC601\uC5ED\uC5D0 \uB4E4\uC5B4\uAC04\uB2E4. b\uB294 \uC5B4\uBA38\uB2C8 \uD56D\uC131\uC744 83.89\uC77C \uC8FC\uAE30\uB85C 1\uD68C \uB3C8\uB2E4. \uACF5\uC804\uADA4\uB3C4 \uC774\uC2EC\uB960\uC740 0.34\uB85C \uC678\uACC4 \uD589\uC131\uB4E4 \uC911\uC5D0\uC11C\uB294 \uD3C9\uBC94\uD55C \uC218\uC900\uC774\uB2E4."@ko . "HD 114762 b"@ar . . "HD 114762 b adalah eksoplanet raksasa gas yang mengorbit bintang , di rasi bintang Coma Berenices, sekitar 126 tahun cahaya dari Bumi. Massanya adalah sekitar 10.69 Jupiter, dibutuhkan 83,9 hari untuk menyelesaikan satu orbit bintangnya, dan 0,35 AU dari bintangnya. Penemuannya diumumkan pada tahun 1989. Pada tahun 2012, statusnya sebagai eksoplanet dikonfirmasi. HD 114762 b adalah salah satu eksoplanet pertama yang pernah ditemukan, mendahului pulsar 1992 di sekitar PSR B1257+12 dan bintang katai kuning urutan pertama 51 Pegasi, meskipun Gamma Cephei Ab mendahului itu."@in . . . . . . . "HD 114762 b\uB294 \uC9C0\uAD6C\uB85C\uBD80\uD130 \uBA38\uB9AC\uD138\uC790\uB9AC \uBC29\uD5A5\uC73C\uB85C \uC57D 132\uAD11\uB144 \uB5A8\uC5B4\uC9C4 \uACF3\uC5D0 \uC788\uB294 \uD56D\uC131 \uC8FC\uC704\uB97C \uB3C4\uB294 \uC678\uACC4 \uD589\uC131\uC774\uB2E4. \uC774 \uD589\uC131\uC758 \uCD5C\uC18C \uC9C8\uB7C9\uC740 \uBAA9\uC131\uC758 11\uBC30\uC5D0 \uC774\uB974\uB294\uB370, \uADA4\uB3C4\uACBD\uC0AC\uAC01\uC774 \uBC1D\uD600\uC9C8 \uACBD\uC6B0 \uC774 \uAC12\uC740 \uB354 \uCEE4\uC9C8 \uAC00\uB2A5\uC131\uC774 \uC788\uC73C\uBA70, \uAC08\uC0C9 \uC65C\uC131\uC77C \uD655\uB960\uC774 \uB192\uB2E4. 1989\uB144 \uB370\uC774\uBE44\uB4DC \uB77C\uC0BC \uC5F0\uAD6C\uC9C4\uC774 \uBC1C\uACAC\uD588\uB2E4. 2006\uB144 \uAE30\uC900\uC73C\uB85C \uC774 \uD589\uC131\uC774 \uC815\uD655\uD788 \uAC00\uC2A4 \uD589\uC131\uC778\uC9C0, \uAC08\uC0C9 \uC65C\uC131\uC778\uC9C0 \uC544\uB2C8\uBA74 \uC801\uC0C9 \uC65C\uC131\uC778\uC9C0\uB294 \uC815\uD655\uD788 \uBC1D\uD600\uC9C0\uC9C0 \uC54A\uC558\uB2E4. \uADF9\uB2E8\uC801\uC778 \uACBD\uC6B0 \uBAA9\uC131\uC9C8\uB7C9\uC758 145\uBC30\uAE4C\uC9C0 \uBB34\uAC70\uC6CC\uC9C8 \uC218 \uC788\uB294\uB370, \uC774 \uC815\uB3C4\uB77C\uBA74 \uC774\uBBF8 \uD56D\uC131\uC758 \uC601\uC5ED\uC5D0 \uB4E4\uC5B4\uAC04\uB2E4. b\uB294 \uC5B4\uBA38\uB2C8 \uD56D\uC131\uC744 83.89\uC77C \uC8FC\uAE30\uB85C 1\uD68C \uB3C8\uB2E4. \uACF5\uC804\uADA4\uB3C4 \uC774\uC2EC\uB960\uC740 0.34\uB85C \uC678\uACC4 \uD589\uC131\uB4E4 \uC911\uC5D0\uC11C\uB294 \uD3C9\uBC94\uD55C \uC218\uC900\uC774\uB2E4."@ko . . . "HD 114762 b \u00E8 stato il nome di un pianeta extrasolare gassoso, attestato falso positivo nel 2022, che orbita intorno alla stella HD 114762. Essendo che dista dalla Terra 91,3 anni luce non si pu\u00F2 sapere con certezza il colore; sul sito ufficiale della NASA \u00E8 rappresentato con diverse gradazioni di rosso e arancione.. Venne scoperto nel 1989 da David Latham che us\u00F2 uno spettroscopio Doppler."@it . . . . . . . . "HD 114762 b"@it . "HD 114762 b"@pl . "HD 114762 b"@es . "HD 114762 b \u00E9 um planeta extrassolar massivo gasoso, localizado a cerca de 132 anos-luz (40,6 pc) de dist\u00E2ncia a partir da Terra na constela\u00E7\u00E3o de Coma Berenices. Ele orbita a estrela HD 114762. Dependendo do \u00E2ngulo de inclina\u00E7\u00E3o sua menor massa poss\u00EDvel \u00E9 11 vezes a massa de J\u00FApiter, e sua maior massa cerca de 145 vezes a de J\u00FApiter. HD 114762 b pode ter sido o primeiro planeta extrassolar a ser detectado, antecedendo os planetas de pulsar encontrados em torno de PSR B1257+12 em 1992 e da an\u00E3 amarela da 51 Pegasi. O companheiro orbita sua estrela a cada 83,9 dias e tem uma excentricidade orbital de 0,34; para compara\u00E7\u00E3o, esta \u00F3rbita \u00E9 semelhante a de Merc\u00FArio, mas com o dobro da excentricidade."@pt . "d"@en . "11151"^^ . . . "HD 114762 A b \u2014 \u044D\u043A\u0437\u043E\u043F\u043B\u0430\u043D\u0435\u0442\u0430 \u0432 \u0434\u0432\u043E\u0439\u043D\u043E\u0439 \u0441\u0438\u0441\u0442\u0435\u043C\u0435 HD 114762 \u0432 \u0441\u043E\u0437\u0432\u0435\u0437\u0434\u0438\u0438 \u0412\u043E\u043B\u043E\u0441\u044B \u0412\u0435\u0440\u043E\u043D\u0438\u043A\u0438. \u0411\u044B\u043B\u0430 \u043E\u0442\u043A\u0440\u044B\u0442\u0430 \u0414. \u041B\u0430\u0442\u0430\u043C\u043E\u043C \u0432 1989 \u0433\u043E\u0434\u0443, \u043D\u043E \u043E\u043A\u043E\u043D\u0447\u0430\u0442\u0435\u043B\u044C\u043D\u043E \u043F\u043E\u0434\u0442\u0432\u0435\u0440\u0436\u0434\u0435\u043D\u0430 \u043B\u0438\u0448\u044C \u0432 1999 \u0433\u043E\u0434\u0443. HD 114762 A b \u043D\u0430\u0445\u043E\u0434\u0438\u0442\u0441\u044F \u0443 \u0437\u0432\u0435\u0437\u0434\u044B F-\u043A\u043B\u0430\u0441\u0441\u0430 \u043D\u0430 \u0440\u0430\u0441\u0441\u0442\u043E\u044F\u043D\u0438\u0438 132 \u0441\u0432\u0435\u0442\u043E\u0432\u044B\u0445 \u043B\u0435\u0442 \u043E\u0442 \u0421\u043E\u043B\u043D\u0446\u0430. \u041E\u0431\u043E\u0440\u043E\u0442 \u0432\u043E\u043A\u0440\u0443\u0433 \u0441\u0432\u043E\u0435\u0439 \u0437\u0432\u0435\u0437\u0434\u044B, \u0441\u043E\u0432\u0435\u0440\u0448\u0430\u0435\u0442 \u043F\u043E \u0432\u044B\u0442\u044F\u043D\u0443\u0442\u043E\u0439 \u043E\u0440\u0431\u0438\u0442\u0435 (\u044D\u043A\u0441\u0446\u0435\u043D\u0442\u0440\u0438\u0441\u0438\u0442\u0435\u0442 0,3359) \u043F\u043E\u0447\u0442\u0438 \u0437\u0430 \u0442\u0440\u0438 \u043C\u0435\u0441\u044F\u0446\u0430 (83 \u0434\u043D\u044F), \u043D\u0430 \u0440\u0430\u0441\u0441\u0442\u043E\u044F\u043D\u0438\u0438 0,363 (0,241\u20140,485) \u0430. \u0435. (\u0442\u043E \u0435\u0441\u0442\u044C, \u043F\u0440\u0438\u043C\u0435\u0440\u043D\u043E, \u043A\u0430\u043A \u041C\u0435\u0440\u043A\u0443\u0440\u0438\u0439 \u043E\u0442 \u0421\u043E\u043B\u043D\u0446\u0430). \u041F\u043E\u0441\u043A\u043E\u043B\u044C\u043A\u0443, \u0432\u0435\u0440\u0445\u043D\u044F\u044F \u043F\u043B\u0430\u043D\u043A\u0430 \u043C\u0430\u043A\u0441\u0438\u043C\u0430\u043B\u044C\u043D\u043E\u0439 \u043C\u0430\u0441\u0441\u044B \u043D\u0435 \u043E\u043F\u0440\u0435\u0434\u0435\u043B\u0435\u043D\u0430, HD 114762 A b \u043C\u043E\u0436\u0435\u0442 \u043E\u043A\u0430\u0437\u0430\u0442\u044C\u0441\u044F \u043D\u0435 \u044D\u043A\u0437\u043E\u043F\u043B\u0430\u043D\u0435\u0442\u043E\u0439, \u0430 \u043A\u043E\u0440\u0438\u0447\u043D\u0435\u0432\u044B\u043C \u043A\u0430\u0440\u043B\u0438\u043A\u043E\u043C. \u041C\u0438\u043D\u0438\u043C\u0430\u043B\u044C\u043D\u0430\u044F \u043C\u0430\u0441\u0441\u0430 HD 114762 A b \u2014 11 \u043C\u0430\u0441\u0441 \u042E\u043F\u0438\u0442\u0435\u0440\u0430. \u041E\u043F\u0442\u0438\u0447\u0435\u0441\u043A\u0438, \u044D\u0442\u043E\u0442 \u043A\u043E\u043C\u043F\u0430\u043D\u044C\u043E\u043D \u043D\u0435 \u043E\u0431\u043D\u0430\u0440\u0443\u0436\u0435\u043D. \u0415\u0441\u043B\u0438 \u043E\u043A\u0430\u0436\u0435\u0442\u0441\u044F, \u0447\u0442\u043E HD 114762 A b \u044D\u043A\u0437\u043E\u043F\u043B\u0430\u043D\u0435\u0442\u0430, \u0442\u043E \u043E\u043D\u0430 \u0431\u0443\u0434\u0435\u0442 \u0432\u0442\u043E\u0440\u043E\u0439, \u0432\u0441\u043B\u0435\u0434 \u0437\u0430 \u0413\u0430\u043C\u043C\u0430 \u0426\u0435\u0444\u0435\u044F A b, \u0432\u043D\u0435\u0441\u043E\u043B\u043D\u0435\u0447\u043D\u043E\u0439 \u043F\u043B\u0430\u043D\u0435\u0442\u043E\u0439, \u043E\u0431\u043D\u0430\u0440\u0443\u0436\u0435\u043D\u043D\u043E\u0439 (\u043D\u043E \u043D\u0435\u043F\u043E\u0434\u0442\u0432\u0435\u0440\u0436\u0434\u0451\u043D\u043D\u043E\u0439) \u0434\u043E \u043E\u0442\u043A\u0440\u044B\u0442\u0438\u044F \u044D\u043A\u0437\u043E\u043F\u043B\u0430\u043D\u0435\u0442 \u0432 1991 \u0433\u043E\u0434\u0443 \u0443 \u043F\u0443\u043B\u044C\u0441\u0430\u0440\u0430 PSR B1257+12 \u0438 \u0432 1995 \u0433\u043E\u0434\u0443 \u0443 \u0437\u0432\u0435\u0437\u0434\u044B 51 \u041F\u0435\u0433\u0430\u0441\u0430."@ru . . . . . . . . "HD 114762 b es un planeta extrasolar, a unos 132 a\u00F1os luz de distancia en la constelaci\u00F3n de Coma Berenices. Aunque posteriormente ha sido incluida en los cat\u00E1logos de los planetas extrasolares.\u200B\u200B Confirmado en octubre de 1991 en un papel de Cochran, et al.\u200B"@es . . . . "HD 114762 b \u2013 gwiazda w gwiazdozbiorze Warkocza Bereniki. Kr\u0105\u017Cy wok\u00F3\u0142 masywniejszej gwiazdy HD 114762; przez wiele lat by\u0142a uznawana za jedn\u0105 z pierwszych odkrytych planet pozas\u0142onecznych lub br\u0105zowych kar\u0142\u00F3w. P\u00F3\u017Aniejsze oceny masy wykluczaj\u0105 jej planetarn\u0105 natur\u0119."@pl . . . . . . . . . . . . "HD 114762 b (\u0628\u0627\u0644\u0625\u0646\u062C\u0644\u064A\u0632\u064A\u0629: HD 114762 b)\u200F \u0627\u0644\u0630\u064A \u064A\u0631\u0645\u0632 \u0644\u0647 \u0628\u0627\u0644\u0631\u0645\u0632 HD 114762b\u060C \u0647\u0648 \u0639\u0645\u0644\u0627\u0642 \u063A\u0627\u0632\u064A\u060C \u0641\u064A \u0643\u0648\u0643\u0628\u0629 \u0627\u0644\u0647\u0644\u0628\u0629\u060C \u064A\u062A\u0628\u0639 HD 114762 \u200F."@ar . . . "HD 114762 A b \u2014 \u0441\u0443\u043F\u0443\u0442\u043D\u0438\u043A \u0437\u043E\u0440\u0456 \u0443 \u043F\u043E\u0434\u0432\u0456\u0439\u043D\u0456\u0439 \u0441\u0438\u0441\u0442\u0435\u043C\u0456 HD 114762 \u0432 \u0441\u0443\u0437\u0456\u0440'\u0457 \u0412\u043E\u043B\u043E\u0441\u0441\u044F \u0412\u0435\u0440\u043E\u043D\u0456\u043A\u0438, \u0432\u0456\u0440\u043E\u0433\u0456\u0434\u043D\u043E \u0454 \u0435\u043A\u0437\u043E\u043F\u043B\u0430\u043D\u0435\u0442\u043E\u044E. \u0412\u0456\u0434\u043A\u0440\u0438\u0442\u0438\u0439 \u0414. \u041B\u0430\u0442\u0430\u043C\u043E\u043C 1989 \u0440\u043E\u043A\u0443, \u0430\u043B\u0435 \u043E\u0441\u0442\u0430\u0442\u043E\u0447\u043D\u043E \u043F\u0456\u0434\u0442\u0432\u0435\u0440\u0434\u0436\u0435\u043D\u0438\u0439 \u043B\u0438\u0448\u0435 1999 \u0440\u043E\u043A\u0443. \u0421\u0443\u043F\u0443\u0442\u043D\u0438\u043A \u043E\u0431\u0435\u0440\u0442\u0430\u0454\u0442\u044C\u0441\u044F \u043D\u0430\u0432\u043A\u043E\u043B\u043E \u0437\u043E\u0440\u0456 F-\u043A\u043B\u0430\u0441\u0443 HD 114762 A, \u044F\u043A\u0430 \u043F\u0435\u0440\u0435\u0431\u0443\u0432\u0430\u0454 \u043D\u0430 \u0432\u0456\u0434\u0441\u0442\u0430\u043D\u0456 132 \u0441\u0432\u0456\u0442\u043B\u043E\u0432\u0438\u0445 \u0440\u043E\u043A\u0456\u0432 \u0432\u0456\u0434 \u0421\u043E\u043D\u0446\u044F. \u041E\u0440\u0431\u0456\u0442\u0430 \u0441\u0443\u043F\u0443\u0442\u043D\u0438\u043A\u0430 \u0432\u0438\u0442\u044F\u0433\u043D\u0443\u0442\u0430 (\u0435\u043A\u0441\u0446\u0435\u043D\u0442\u0440\u0438\u0441\u0438\u0442\u0435\u0442 \u2014 0,3359), \u043F\u0435\u0440\u0456\u043E\u0434 \u043E\u0431\u0435\u0440\u0442\u0430\u043D\u043D\u044F \u0441\u0442\u0430\u043D\u043E\u0432\u0438\u0442\u044C 83 \u0434\u043E\u0431\u0438 (\u043C\u0430\u0439\u0436\u0435 \u0442\u0440\u0438 \u043C\u0456\u0441\u044F\u0446\u0456), \u0441\u0435\u0440\u0435\u0434\u043D\u044F \u0432\u0456\u0434\u0441\u0442\u0430\u043D\u044C \u2014 0,363 \u0430.\u043E. (\u0437\u043C\u0456\u043D\u044E\u0454\u0442\u044C\u0441\u044F \u0432 \u043C\u0435\u0436\u0430\u0445 0,241-0,485, \u0442\u043E\u0431\u0442\u043E, \u043F\u0440\u0438\u0431\u043B\u0438\u0437\u043D\u043E \u044F\u043A \u0432\u0456\u0434\u0441\u0442\u0430\u043D\u044C \u041C\u0435\u0440\u043A\u0443\u0440\u0456\u044F \u0432\u0456\u0434 \u0421\u043E\u043D\u0446\u044F). \u041E\u0446\u0456\u043D\u0435\u043D\u0430 \u043C\u0456\u043D\u0456\u043C\u0430\u043B\u044C\u043D\u0430 \u043C\u0430\u0441\u0430 HD 114762 A b \u2014 11 \u043C\u0430\u0441 \u042E\u043F\u0456\u0442\u0435\u0440\u0430. \u041E\u0441\u043A\u0456\u043B\u044C\u043A\u0438 \u0432\u0435\u0440\u0445\u043D\u044E \u043C\u0435\u0436\u0443 \u043C\u0430\u0441\u0438 \u043D\u0435 \u0432\u0438\u0437\u043D\u0430\u0447\u0435\u043D\u043E, \u043D\u0435 \u0432\u0438\u043A\u043B\u044E\u0447\u0435\u043D\u043E, \u0449\u043E HD 114762 A b \u043C\u043E\u0436\u0435 \u0431\u0443\u0442\u0438 \u043A\u043E\u0440\u0438\u0447\u043D\u0435\u0432\u0438\u043C \u043A\u0430\u0440\u043B\u0438\u043A\u043E\u043C, \u0430 \u043D\u0435 \u0435\u043A\u0437\u043E\u043F\u043B\u0430\u043D\u0435\u0442\u043E\u044E. \u041E\u043F\u0442\u0438\u0447\u043D\u043E \u0446\u0435\u0439 \u0441\u0443\u043F\u0443\u0442\u043D\u0438\u043A \u043D\u0435 \u0432\u0438\u044F\u0432\u043B\u0435\u043D\u043E. \u042F\u043A\u0449\u043E \u043E\u0441\u0442\u0430\u0442\u043E\u0447\u043D\u043E \u0437'\u044F\u0441\u0443\u0454\u0442\u044C\u0441\u044F, \u0449\u043E HD 114762 A b \u2014 \u0441\u043F\u0440\u0430\u0432\u0434\u0456 \u0435\u043A\u0437\u043E\u043F\u043B\u0430\u043D\u0435\u0442\u0430, \u0442\u043E \u0432\u043E\u043D\u0430 \u0431\u0443\u0434\u0435 \u0434\u0440\u0443\u0433\u043E\u044E \u0437\u0430 \u043B\u0456\u043A\u043E\u043C \u0432\u0438\u044F\u0432\u043B\u0435\u043D\u043E\u044E \u0435\u043A\u0437\u043E\u043F\u043B\u0430\u043D\u0435\u0442\u043E\u044E (\u043F\u0456\u0441\u043B\u044F \u0413\u0430\u043C\u043C\u0430 \u0426\u0435\u0444\u0435\u044F A b), \u0445\u043E\u0447\u0430 \u043F\u0456\u0434\u0442\u0432\u0435\u0440\u0434\u0436\u0435\u043D\u043E\u044E \u0457\u0457 \u0432\u0456\u0434\u043A\u0440\u0438\u0442\u0442\u044F \u0431\u0443\u043B\u043E \u043F\u0456\u0437\u043D\u0456\u0448\u0435 \u0435\u043A\u0437\u043E\u043F\u043B\u0430\u043D\u0435\u0442 \u043F\u0443\u043B\u044C\u0441\u0430\u0440\u0430 PSR B1257+12 (1991 \u0440\u0456\u043A) \u0456 \u0437\u043E\u0440\u0456 51 \u041F\u0435\u0433\u0430\u0441\u0430 (1995 \u0440\u0456\u043A)."@uk . "HD 114762 b\u306F\u3001\u304B\u307F\u306E\u3051\u5EA7\u306E\u5929\u4F53\u3067\u3042\u308B\u30021989\u5E74\u306BDavid W. Latham\u3089\u306B\u3088\u3063\u3066\u767A\u898B\u3055\u308C\u305F\u3002\u592A\u967D\u7CFB\u5916\u60D1\u661F\u5019\u88DC\u306E\u4E00\u3064\u3060\u304C\u3001\u8910\u8272\u77EE\u661F\u306B\u5206\u985E\u3055\u308C\u308B\u53EF\u80FD\u6027\u3082\u3042\u308B\u3002\u592A\u967D\u7CFB\u304B\u3089\u306F126\u5149\u5E74\u96E2\u308C\u3066\u3044\u308B\u3002"@ja . . . "HD 114762 b"@en . "HD 114762 b\u306F\u3001\u304B\u307F\u306E\u3051\u5EA7\u306E\u5929\u4F53\u3067\u3042\u308B\u30021989\u5E74\u306BDavid W. Latham\u3089\u306B\u3088\u3063\u3066\u767A\u898B\u3055\u308C\u305F\u3002\u592A\u967D\u7CFB\u5916\u60D1\u661F\u5019\u88DC\u306E\u4E00\u3064\u3060\u304C\u3001\u8910\u8272\u77EE\u661F\u306B\u5206\u985E\u3055\u308C\u308B\u53EF\u80FD\u6027\u3082\u3042\u308B\u3002\u592A\u967D\u7CFB\u304B\u3089\u306F126\u5149\u5E74\u96E2\u308C\u3066\u3044\u308B\u3002"@ja . . "HD 114762 b"@pt . "AU"@en . "HD 114762 b, formellement HD 114762 Ab, est un objet en orbite autour de l'\u00E9toile HD 114762 A, la naine (classe de luminosit\u00E9 V) jaune-blanc (type spectral F) composante principale de la binaire spectroscopique HD 114762. D\u00E9couverte en 1992 par la m\u00E9thode des vitesses radiales, sa masse minimale de 11 masses joviennes laissait penser qu'il pourrait s'agir d'une naine brune voire d'une plan\u00E8te extrasolaire (exoplan\u00E8te), ce qui en aurait fait la premi\u00E8re connue. Les mesures d'astrom\u00E9trie obtenues pr\u00E8s de 30 ans apr\u00E8s semblent cependant montrer que l'orbite est vue de fa\u00E7on quasi-polaire et que HD 114762 Ab est donc probablement une petite \u00E9toile naine rouge. Elle se situe \u00E0 une distance d'environ 40,6 parsecs (132 ann\u00E9es-lumi\u00E8re) du Soleil, dans la constellation de la Chevelure de B\u00E9r\u00E9nice."@fr . "HD 114762 Ab"@fr . . . "12447263"^^ . "HD 114762 A b \u2014 \u0441\u0443\u043F\u0443\u0442\u043D\u0438\u043A \u0437\u043E\u0440\u0456 \u0443 \u043F\u043E\u0434\u0432\u0456\u0439\u043D\u0456\u0439 \u0441\u0438\u0441\u0442\u0435\u043C\u0456 HD 114762 \u0432 \u0441\u0443\u0437\u0456\u0440'\u0457 \u0412\u043E\u043B\u043E\u0441\u0441\u044F \u0412\u0435\u0440\u043E\u043D\u0456\u043A\u0438, \u0432\u0456\u0440\u043E\u0433\u0456\u0434\u043D\u043E \u0454 \u0435\u043A\u0437\u043E\u043F\u043B\u0430\u043D\u0435\u0442\u043E\u044E. \u0412\u0456\u0434\u043A\u0440\u0438\u0442\u0438\u0439 \u0414. \u041B\u0430\u0442\u0430\u043C\u043E\u043C 1989 \u0440\u043E\u043A\u0443, \u0430\u043B\u0435 \u043E\u0441\u0442\u0430\u0442\u043E\u0447\u043D\u043E \u043F\u0456\u0434\u0442\u0432\u0435\u0440\u0434\u0436\u0435\u043D\u0438\u0439 \u043B\u0438\u0448\u0435 1999 \u0440\u043E\u043A\u0443. \u0421\u0443\u043F\u0443\u0442\u043D\u0438\u043A \u043E\u0431\u0435\u0440\u0442\u0430\u0454\u0442\u044C\u0441\u044F \u043D\u0430\u0432\u043A\u043E\u043B\u043E \u0437\u043E\u0440\u0456 F-\u043A\u043B\u0430\u0441\u0443 HD 114762 A, \u044F\u043A\u0430 \u043F\u0435\u0440\u0435\u0431\u0443\u0432\u0430\u0454 \u043D\u0430 \u0432\u0456\u0434\u0441\u0442\u0430\u043D\u0456 132 \u0441\u0432\u0456\u0442\u043B\u043E\u0432\u0438\u0445 \u0440\u043E\u043A\u0456\u0432 \u0432\u0456\u0434 \u0421\u043E\u043D\u0446\u044F. \u041E\u0440\u0431\u0456\u0442\u0430 \u0441\u0443\u043F\u0443\u0442\u043D\u0438\u043A\u0430 \u0432\u0438\u0442\u044F\u0433\u043D\u0443\u0442\u0430 (\u0435\u043A\u0441\u0446\u0435\u043D\u0442\u0440\u0438\u0441\u0438\u0442\u0435\u0442 \u2014 0,3359), \u043F\u0435\u0440\u0456\u043E\u0434 \u043E\u0431\u0435\u0440\u0442\u0430\u043D\u043D\u044F \u0441\u0442\u0430\u043D\u043E\u0432\u0438\u0442\u044C 83 \u0434\u043E\u0431\u0438 (\u043C\u0430\u0439\u0436\u0435 \u0442\u0440\u0438 \u043C\u0456\u0441\u044F\u0446\u0456), \u0441\u0435\u0440\u0435\u0434\u043D\u044F \u0432\u0456\u0434\u0441\u0442\u0430\u043D\u044C \u2014 0,363 \u0430.\u043E. (\u0437\u043C\u0456\u043D\u044E\u0454\u0442\u044C\u0441\u044F \u0432 \u043C\u0435\u0436\u0430\u0445 0,241-0,485, \u0442\u043E\u0431\u0442\u043E, \u043F\u0440\u0438\u0431\u043B\u0438\u0437\u043D\u043E \u044F\u043A \u0432\u0456\u0434\u0441\u0442\u0430\u043D\u044C \u041C\u0435\u0440\u043A\u0443\u0440\u0456\u044F \u0432\u0456\u0434 \u0421\u043E\u043D\u0446\u044F). \u041E\u0446\u0456\u043D\u0435\u043D\u0430 \u043C\u0456\u043D\u0456\u043C\u0430\u043B\u044C\u043D\u0430 \u043C\u0430\u0441\u0430 HD 114762 A b \u2014 11 \u043C\u0430\u0441 \u042E\u043F\u0456\u0442\u0435\u0440\u0430. \u041E\u0441\u043A\u0456\u043B\u044C\u043A\u0438 \u0432\u0435\u0440\u0445\u043D\u044E \u043C\u0435\u0436\u0443 \u043C\u0430\u0441\u0438 \u043D\u0435 \u0432\u0438\u0437\u043D\u0430\u0447\u0435\u043D\u043E, \u043D\u0435 \u0432\u0438\u043A\u043B\u044E\u0447\u0435\u043D\u043E, \u0449\u043E HD 114762 A b \u043C\u043E\u0436\u0435 \u0431\u0443\u0442\u0438 \u043A\u043E\u0440\u0438\u0447\u043D\u0435\u0432\u0438\u043C \u043A\u0430\u0440\u043B\u0438\u043A\u043E\u043C, \u0430 \u043D\u0435 \u0435\u043A\u0437\u043E\u043F\u043B\u0430\u043D\u0435\u0442\u043E\u044E. \u041E\u043F\u0442\u0438\u0447\u043D\u043E \u0446\u0435\u0439 \u0441\u0443\u043F\u0443\u0442\u043D\u0438\u043A \u043D\u0435 \u0432\u0438\u044F\u0432\u043B\u0435\u043D\u043E. \u042F\u043A\u0449\u043E \u043E\u0441\u0442\u0430\u0442\u043E\u0447\u043D\u043E \u0437'\u044F\u0441\u0443\u0454\u0442\u044C\u0441\u044F, \u0449\u043E HD 114762 A b \u2014 \u0441\u043F\u0440\u0430\u0432\u0434\u0456 \u0435\u043A\u0437\u043E\u043F\u043B\u0430\u043D\u0435\u0442\u0430"@uk . . . "HD 114762 b \u00E8 stato il nome di un pianeta extrasolare gassoso, attestato falso positivo nel 2022, che orbita intorno alla stella HD 114762. Essendo che dista dalla Terra 91,3 anni luce non si pu\u00F2 sapere con certezza il colore; sul sito ufficiale della NASA \u00E8 rappresentato con diverse gradazioni di rosso e arancione.. Venne scoperto nel 1989 da David Latham che us\u00F2 uno spettroscopio Doppler."@it . . "HD 114762 b \u2013 gwiazda w gwiazdozbiorze Warkocza Bereniki. Kr\u0105\u017Cy wok\u00F3\u0142 masywniejszej gwiazdy HD 114762; przez wiele lat by\u0142a uznawana za jedn\u0105 z pierwszych odkrytych planet pozas\u0142onecznych lub br\u0105zowych kar\u0142\u00F3w. P\u00F3\u017Aniejsze oceny masy wykluczaj\u0105 jej planetarn\u0105 natur\u0119."@pl . "HD 114762 b, formellement HD 114762 Ab, est un objet en orbite autour de l'\u00E9toile HD 114762 A, la naine (classe de luminosit\u00E9 V) jaune-blanc (type spectral F) composante principale de la binaire spectroscopique HD 114762. D\u00E9couverte en 1992 par la m\u00E9thode des vitesses radiales, sa masse minimale de 11 masses joviennes laissait penser qu'il pourrait s'agir d'une naine brune voire d'une plan\u00E8te extrasolaire (exoplan\u00E8te), ce qui en aurait fait la premi\u00E8re connue. Les mesures d'astrom\u00E9trie obtenues pr\u00E8s de 30 ans apr\u00E8s semblent cependant montrer que l'orbite est vue de fa\u00E7on quasi-polaire et que HD 114762 Ab est donc probablement une petite \u00E9toile naine rouge. Elle se situe \u00E0 une distance d'environ 40,6 parsecs (132 ann\u00E9es-lumi\u00E8re) du Soleil, dans la constellation de la Chevelure de B\u00E9r\u00E9nice."@fr . . . . . . "HD 114762 A b"@uk . . "HD 114762 b"@ko . . . "HD 114762 b \u00E9 um planeta extrassolar massivo gasoso, localizado a cerca de 132 anos-luz (40,6 pc) de dist\u00E2ncia a partir da Terra na constela\u00E7\u00E3o de Coma Berenices. Ele orbita a estrela HD 114762. Dependendo do \u00E2ngulo de inclina\u00E7\u00E3o sua menor massa poss\u00EDvel \u00E9 11 vezes a massa de J\u00FApiter, e sua maior massa cerca de 145 vezes a de J\u00FApiter. HD 114762 b pode ter sido o primeiro planeta extrassolar a ser detectado, antecedendo os planetas de pulsar encontrados em torno de PSR B1257+12 em 1992 e da an\u00E3 amarela da 51 Pegasi. O companheiro orbita sua estrela a cada 83,9 dias e tem uma excentricidade orbital de 0,34; para compara\u00E7\u00E3o, esta \u00F3rbita \u00E9 semelhante a de Merc\u00FArio, mas com o dobro da excentricidade."@pt . . . "HD 114762 b\u662F\u4E00\u500B\u4F4D\u65BC\u540E\u9AEE\u5EA7\uFF0C\u8DDD\u96E2\u5730\u7403\u7D04132\u5149\u5E74\u7684\u5019\u9078\u7CFB\u5916\u884C\u661F\u6216\u68D5\u77EE\u661F\u3002"@zh . . . . "HD 114762 b (\u0628\u0627\u0644\u0625\u0646\u062C\u0644\u064A\u0632\u064A\u0629: HD 114762 b)\u200F \u0627\u0644\u0630\u064A \u064A\u0631\u0645\u0632 \u0644\u0647 \u0628\u0627\u0644\u0631\u0645\u0632 HD 114762b\u060C \u0647\u0648 \u0639\u0645\u0644\u0627\u0642 \u063A\u0627\u0632\u064A\u060C \u0641\u064A \u0643\u0648\u0643\u0628\u0629 \u0627\u0644\u0647\u0644\u0628\u0629\u060C \u064A\u062A\u0628\u0639 HD 114762 \u200F."@ar . . . . . . "HD 114762 b es un planeta extrasolar, a unos 132 a\u00F1os luz de distancia en la constelaci\u00F3n de Coma Berenices. Aunque posteriormente ha sido incluida en los cat\u00E1logos de los planetas extrasolares.\u200B\u200B Confirmado en octubre de 1991 en un papel de Cochran, et al.\u200B"@es . "HD 114762 b is a small red dwarf star, in the HD 114762 system, formerly thought to be a massive gaseous extrasolar planet, approximately 126 light-years (38.6 pc) away in the constellation of Coma Berenices. This optically undetected companion to the late F-type main-sequence star HD 114762 was discovered in 1989 by Latham, et al., and confirmed in an October 1991 paper by Cochran, et al. It was thought to be the first discovered exoplanet (although its existence was confirmed after those around PSR B1257+12.)"@en . . . . . . . "HD 114762 b"@ja . "HD 114762 b adalah eksoplanet raksasa gas yang mengorbit bintang , di rasi bintang Coma Berenices, sekitar 126 tahun cahaya dari Bumi. Massanya adalah sekitar 10.69 Jupiter, dibutuhkan 83,9 hari untuk menyelesaikan satu orbit bintangnya, dan 0,35 AU dari bintangnya. Penemuannya diumumkan pada tahun 1989. Pada tahun 2012, statusnya sebagai eksoplanet dikonfirmasi. HD 114762 b adalah salah satu eksoplanet pertama yang pernah ditemukan, mendahului pulsar 1992 di sekitar PSR B1257+12 dan bintang katai kuning urutan pertama 51 Pegasi, meskipun Gamma Cephei Ab mendahului itu."@in .