. . . . . . "HD 142415 is a single star in the southern constellation of Norma, positioned next to the southern constellation border with Triangulum Australe and less than a degree to the west of NGC 6025. With an apparent visual magnitude of 7.33, it is too faint to be visible to the naked eye. The distance to this star is 116 light years from the Sun based on parallax, but it is drifting closer with a radial velocity of \u221212 km/s. It is a candidate member of the NGC 1901 open cluster of stars."@en . . . . . . . . "28.1149"^^ . . . . . . . "HD 142415"@en . "0.0328"^^ . "HD 142415"@pt . . . . . . . . . . . "HD 142415 \u00E4r en ensam stj\u00E4rna bel\u00E4gen i den s\u00F6dra delen av stj\u00E4rnbilden Vinkelhaken mindre \u00E4n en grad v\u00E4ster om . Den har en skenbar magnitud av ca 7,33 och kr\u00E4ver \u00E5tminstone en stark handkikare eller ett mindre teleskop f\u00F6r att kunna observeras. Baserat p\u00E5 parallax enligt Gaia Data Release 2 p\u00E5 ca 28,1 mas, ber\u00E4knas den befinna sig p\u00E5 ett avst\u00E5nd p\u00E5 ca 116 ljus\u00E5r (ca 36 parsek) fr\u00E5n solen. Den r\u00F6r sig n\u00E4rmare solen med en heliocentrisk radialhastighet p\u00E5 ca -12 km/s. Stj\u00E4rnan ing\u00E5r m\u00F6jligen i den \u00F6ppna stj\u00E4rnhopen ."@sv . "7.33"^^ . . "HD 142415 \u2014 \u0437\u0432\u0435\u0437\u0434\u0430 \u0432 \u0441\u043E\u0437\u0432\u0435\u0437\u0434\u0438\u0438 \u041D\u0430\u0443\u0433\u043E\u043B\u044C\u043D\u0438\u043A\u0430 \u043D\u0430 \u0440\u0430\u0441\u0441\u0442\u043E\u044F\u043D\u0438\u0438 \u043E\u043A\u043E\u043B\u043E 113 \u0441\u0432\u0435\u0442\u043E\u0432\u044B\u0445 \u043B\u0435\u0442 \u043E\u0442 \u043D\u0430\u0441. \u0412\u043E\u043A\u0440\u0443\u0433 \u0437\u0432\u0435\u0437\u0434\u044B \u043E\u0431\u0440\u0430\u0449\u0430\u0435\u0442\u0441\u044F, \u043A\u0430\u043A \u043C\u0438\u043D\u0438\u043C\u0443\u043C, \u043E\u0434\u043D\u0430 \u043F\u043B\u0430\u043D\u0435\u0442\u0430."@ru . "HD 142415"@ru . . . . "386.3"^^ . . "HD 142415 is a single star in the southern constellation of Norma, positioned next to the southern constellation border with Triangulum Australe and less than a degree to the west of NGC 6025. With an apparent visual magnitude of 7.33, it is too faint to be visible to the naked eye. The distance to this star is 116 light years from the Sun based on parallax, but it is drifting closer with a radial velocity of \u221212 km/s. It is a candidate member of the NGC 1901 open cluster of stars. This is an ordinary G-type main-sequence star with a stellar classification of G1V. It has been identified as a solar twin by Datson et al. (2012), which means its physical properties are very similar to the Sun. It has 10% more mass than the Sun but only a 3% larger radius. The star is estimated to be 1.6 billion years old and is spinning with a projected rotational velocity of 4.2 km/s. It is radiating 1.16 times the luminosity of the Sun from its photosphere at an effective temperature of 5,869 K. The star is currently known to have one planet, designated HD 142415 b. This was detected via the radial velocity method and announced in 2004. The orbital period is just over a year, which made a determination of the orbital eccentricity more difficult due to undersampling over part of the orbit, in combination with jitter. The authors chose to pin the eccentricity value to 0.5, although solutions in the range 0.2\u20130.8 would be equally plausible."@en . "14667240"^^ . "HD 142415 \u00E9 uma estrela na constela\u00E7\u00E3o de Norma. Tem uma magnitude aparente visual de 7,33, portanto n\u00E3o \u00E9 vis\u00EDvel a olho nu. Com base em medi\u00E7\u00F5es de paralaxe, do segundo lan\u00E7amento do cat\u00E1logo Gaia, est\u00E1 localizada a uma dist\u00E2ncia de 116 anos-luz (35,6 parsecs) da Terra. Esta \u00E9 uma estrela de classe G da sequ\u00EAncia principal com um tipo espectral de G1V, sendo similar ao Sol por\u00E9m um pouco maior e mais brilhante. Estima-se que tenha uma massa 10% superior \u00E0 massa solar e um raio 4% maior que o do solar. Est\u00E1 irradiando 116% da luminosidade solar de sua fotosfera a uma temperatura efetiva de 5 870 K. Com uma idade estimada de 1,6 bilh\u00F5es de anos, esta estrela tem um n\u00EDvel moderado de atividade cromosf\u00E9rica e um per\u00EDodo de rota\u00E7\u00E3o de cerca de 10 dias. Sua metalicidade \u00E9 significativamente superior \u00E0 solar, com uma abund\u00E2ncia de ferro 62% maior que a do Sol. Em 2004, foi publicada a descoberta de um planeta extrassolar orbitando HD 142415, detectado pelo m\u00E9todo da velocidade radial a partir de observa\u00E7\u00F5es do espectr\u00F3grafo CORALIE. Esse planeta \u00E9 um gigante gasoso com uma massa m\u00EDnima de 1,62 vezes a massa de J\u00FApiter, orbitando a estrela a uma dist\u00E2ncia m\u00E9dia de 1,05 UA com um per\u00EDodo de 386 dias. O espa\u00E7o de tempo perto do m\u00EDnimo da curva de velocidade radial n\u00E3o possui observa\u00E7\u00F5es, o que significa que a excentricidade orbital do planeta n\u00E3o \u00E9 conhecida, podendo ser entre 0,2 e 0,8. Um valor arbitr\u00E1rio de 0,5 foi escolhido para a cria\u00E7\u00E3o da solu\u00E7\u00E3o final."@pt . . ">1.62"@en . . "HD 142415 \u00E4r en ensam stj\u00E4rna bel\u00E4gen i den s\u00F6dra delen av stj\u00E4rnbilden Vinkelhaken mindre \u00E4n en grad v\u00E4ster om . Den har en skenbar magnitud av ca 7,33 och kr\u00E4ver \u00E5tminstone en stark handkikare eller ett mindre teleskop f\u00F6r att kunna observeras. Baserat p\u00E5 parallax enligt Gaia Data Release 2 p\u00E5 ca 28,1 mas, ber\u00E4knas den befinna sig p\u00E5 ett avst\u00E5nd p\u00E5 ca 116 ljus\u00E5r (ca 36 parsek) fr\u00E5n solen. Den r\u00F6r sig n\u00E4rmare solen med en heliocentrisk radialhastighet p\u00E5 ca -12 km/s. Stj\u00E4rnan ing\u00E5r m\u00F6jligen i den \u00F6ppna stj\u00E4rnhopen ."@sv . . "1.05"^^ . . "4.66"^^ . "HD+142415"@en . . "J2000"@en . . . "HD 142415 \u00E9 uma estrela na constela\u00E7\u00E3o de Norma. Tem uma magnitude aparente visual de 7,33, portanto n\u00E3o \u00E9 vis\u00EDvel a olho nu. Com base em medi\u00E7\u00F5es de paralaxe, do segundo lan\u00E7amento do cat\u00E1logo Gaia, est\u00E1 localizada a uma dist\u00E2ncia de 116 anos-luz (35,6 parsecs) da Terra."@pt . "1121783395"^^ . . . . . . . . . . "HD 142415 \u2014 \u0437\u0432\u0435\u0437\u0434\u0430 \u0432 \u0441\u043E\u0437\u0432\u0435\u0437\u0434\u0438\u0438 \u041D\u0430\u0443\u0433\u043E\u043B\u044C\u043D\u0438\u043A\u0430 \u043D\u0430 \u0440\u0430\u0441\u0441\u0442\u043E\u044F\u043D\u0438\u0438 \u043E\u043A\u043E\u043B\u043E 113 \u0441\u0432\u0435\u0442\u043E\u0432\u044B\u0445 \u043B\u0435\u0442 \u043E\u0442 \u043D\u0430\u0441. \u0412\u043E\u043A\u0440\u0443\u0433 \u0437\u0432\u0435\u0437\u0434\u044B \u043E\u0431\u0440\u0430\u0449\u0430\u0435\u0442\u0441\u044F, \u043A\u0430\u043A \u043C\u0438\u043D\u0438\u043C\u0443\u043C, \u043E\u0434\u043D\u0430 \u043F\u043B\u0430\u043D\u0435\u0442\u0430."@ru . "HD 142415"@zh . . . . . . . . . . . . . "HD 142415\u306F\u3001\u3058\u3087\u3046\u304E\u5EA7\u306E\u65B9\u89D2\u306B\u7D04116\u5149\u5E74\u306E\u8DDD\u96E2\u306B\u3042\u308B\u30017\u7B49\u7D1A\u306E\u9EC4\u8272\u4E3B\u7CFB\u5217\u661F\u3067\u3042\u308B\u3002\u592A\u967D\u3068\u6BD4\u3079\u3001\u8CEA\u91CF\u306F1.15\u500D\u3001\u534A\u5F84\u306F0.98\u500D\u3001\u5149\u5EA6\u306F1.1\u500D\u3001\u8868\u9762\u6E29\u5EA6\u306F1.03\u500D\u3001\u91D1\u5C5E\u91CF\u306F1.4\u500D\u3068\u826F\u304F\u4F3C\u3066\u3044\u308B\u3002\u5E74\u9F62\u306F10\u5104\u6B73\u7A0B\u5EA6\u3067\u3042\u308B\u3002"@ja . . "HD 142415\u662F\u4E00\u9846\u4F4D\u65BC\u77E9\u5C3A\u5EA7\u7684\u9EC3\u77EE\u661F\uFF0C\u8996\u661F\u7B497\u7B49\uFF0C\u8DDD\u96E2\u5730\u7403\u7D04113\u5149\u5E74\u3002\u8A72\u8861\u661F\u76F8\u7576\u985E\u4F3C\u592A\u967D\uFF0C\u8CEA\u91CF\u662F\u592A\u967D\u76841.09\u500D\uFF0C\u534A\u5F91\u662F\u592A\u967D\u76841.03\u500D\uFF0C\u5149\u5EA6\u662F\u592A\u967D\u76841.1\u500D\uFF0C\u6EAB\u5EA6\u5247\u662F\u592A\u967D\u76841.01\u500D\uFF0C\u91D1\u5C6C\u91CF1.62\u500D\u3002\u5B83\u7684\u5E74\u9F61\u53EA\u670915\u5104\u5E74\u3002 \u76EE\u524D\u5DF2\u77E5\u8A72\u6046\u661F\u65C1\u6709\u4E00\u9846\u7CFB\u5916\u884C\u661F\u3002"@zh . . . "HD 142415 ist ein 112 Lichtjahre von der Erde entfernter Gelber Zwerg mit einer Rektaszension von 15h 57m 40s und einer Deklination von \u221260\u00B0 12' 00\". Er besitzt eine scheinbare Helligkeit von 7,34 mag. Im Jahre 2003 entdeckte Michel Mayor einen extrasolaren Planeten, der diesen Stern umkreist.Dieser tr\u00E4gt den Namen HD 142415 b."@de . . . . . "HD 142415"@ja . . . . "HD 142415 ist ein 112 Lichtjahre von der Erde entfernter Gelber Zwerg mit einer Rektaszension von 15h 57m 40s und einer Deklination von \u221260\u00B0 12' 00\". Er besitzt eine scheinbare Helligkeit von 7,34 mag. Im Jahre 2003 entdeckte Michel Mayor einen extrasolaren Planeten, der diesen Stern umkreist.Dieser tr\u00E4gt den Namen HD 142415 b."@de . . . . "HD+142415"@en . . . . . "HD 142415"@sv . . "HD 142415\u306F\u3001\u3058\u3087\u3046\u304E\u5EA7\u306E\u65B9\u89D2\u306B\u7D04116\u5149\u5E74\u306E\u8DDD\u96E2\u306B\u3042\u308B\u30017\u7B49\u7D1A\u306E\u9EC4\u8272\u4E3B\u7CFB\u5217\u661F\u3067\u3042\u308B\u3002\u592A\u967D\u3068\u6BD4\u3079\u3001\u8CEA\u91CF\u306F1.15\u500D\u3001\u534A\u5F84\u306F0.98\u500D\u3001\u5149\u5EA6\u306F1.1\u500D\u3001\u8868\u9762\u6E29\u5EA6\u306F1.03\u500D\u3001\u91D1\u5C5E\u91CF\u306F1.4\u500D\u3068\u826F\u304F\u4F3C\u3066\u3044\u308B\u3002\u5E74\u9F62\u306F10\u5104\u6B73\u7A0B\u5EA6\u3067\u3042\u308B\u3002"@ja . . "HD 142415\u662F\u4E00\u9846\u4F4D\u65BC\u77E9\u5C3A\u5EA7\u7684\u9EC3\u77EE\u661F\uFF0C\u8996\u661F\u7B497\u7B49\uFF0C\u8DDD\u96E2\u5730\u7403\u7D04113\u5149\u5E74\u3002\u8A72\u8861\u661F\u76F8\u7576\u985E\u4F3C\u592A\u967D\uFF0C\u8CEA\u91CF\u662F\u592A\u967D\u76841.09\u500D\uFF0C\u534A\u5F91\u662F\u592A\u967D\u76841.03\u500D\uFF0C\u5149\u5EA6\u662F\u592A\u967D\u76841.1\u500D\uFF0C\u6EAB\u5EA6\u5247\u662F\u592A\u967D\u76841.01\u500D\uFF0C\u91D1\u5C6C\u91CF1.62\u500D\u3002\u5B83\u7684\u5E74\u9F61\u53EA\u670915\u5104\u5E74\u3002 \u76EE\u524D\u5DF2\u77E5\u8A72\u6046\u661F\u65C1\u6709\u4E00\u9846\u7CFB\u5916\u884C\u661F\u3002"@zh . . . "G1V"@en . "HD 142415"@de . . . "7993"^^ . . "0.5"^^ . . .