"2452806.14"^^ . . . . . "\u30EC\u30C1\u30AF\u30EB\u5EA7\u03B2\u661F\uFF08\u30EC\u30C1\u30AF\u30EB\u3056\u30D9\u30FC\u30BF\u305B\u3044\u3001\u03B2 Reticuli\u3001\u03B2 Ret\uFF09\u306F\u3001\u30EC\u30C1\u30AF\u30EB\u5EA7\u306B\u3042\u308B\u4E09\u91CD\u661F\u7CFB\u3067\u3001\u5206\u5149\u9023\u661F\u3067\u3042\u308B\u3002\u4E3B\u661F\u306F\u3001\u6A59\u8272\u5DE8\u661F\u3067\u3042\u308B\u3002 \u30EC\u30C1\u30AF\u30EB\u5EA7\u03B2\u661F\u306F\u3001\u592A\u967D\u306B\u5BFE\u3057\u3066\u7D0469.2 km/s\u306E\u901F\u5EA6\u3067\u9280\u6CB3\u7CFB\u5185\u3092\u904B\u52D5\u3057\u3066\u3044\u308B\u3002\u9280\u6CB3\u7CFB\u306E\u4E2D\u5FC3\u304B\u3089\u306F\u300110,100\u5149\u5E74\u304B\u308924,200\u5149\u5E74\u96E2\u308C\u3066\u3044\u308B\u3002 31\u4E079000\u5E74\u524D\u306B\u592A\u967D\u306B\u6700\u3082\u8FD1\u304F67\u5149\u5E74\u307E\u3067\u8FD1\u3065\u304D\u3001\u305D\u306E\u6642\u306F2.98\u7B49\u7D1A\u307E\u3067\u660E\u308B\u304F\u306A\u3063\u305F\u3002"@ja . "+1.13"@en . . . . "\u03B2 Ret B"@en . "Beta Reticuli"@pt . . . . "K0IV SB"@en . "33.49"^^ . . . . . "Beta Reticuli (Beta Ret, \u03B2 Reticuli, \u03B2 Ret) \u00E8 una stella di magnitudine 3,85 situata nella costellazione australe del Reticolo. \u00C8 la seconda stella pi\u00F9 brillante della costellazione e si trova a circa 100 anni luce dal sistema solare."@it . "Beta Reticuli (\u03B2 Reticuli, f\u00F6rkortat Beta Ret, \u03B2 Ret) som \u00E4r stj\u00E4rnans Bayerbeteckning, \u00E4r en dubbelstj\u00E4rna bel\u00E4gen i den s\u00F6dra delen av stj\u00E4rnbilden Rombiska n\u00E4tet. Den har en skenbar magnitud p\u00E5 3,84 och \u00E4r synlig f\u00F6r blotta \u00F6gat d\u00E4r ljusf\u00F6roreningar ej f\u00F6rekommer. Baserat p\u00E5 parallaxm\u00E4tning inom Hipparcosuppdraget p\u00E5 ca 33,5 mas, ber\u00E4knas den befinna sig p\u00E5 ett avst\u00E5nd p\u00E5 ca 97 ljus\u00E5r (ca 30 parsek) fr\u00E5n solen. Beta Reticuli befann sig n\u00E4rmast solen f\u00F6r 319 000 \u00E5r sedan d\u00E5 den hade en skenbar magnitud p\u00E5 2,98 vid ett avst\u00E5nd av 67 ljus\u00E5r."@sv . . "8599"^^ . . . . . "+3.84"@en . . . "\u86C7\u9996\u4E8C(\u7F51\u7F5F\u5EA7\u03B2)\u662F\u4F4D\u4E8E\u7F51\u7F5F\u5EA7\u7684\u53CC\u661F\u7CFB\u7EDF\uFF0C\u5176\u89C6\u661F\u7B49\u4E3A3.84 \u3002"@zh . . . . . "\u30EC\u30C1\u30AF\u30EB\u5EA7\u30D9\u30FC\u30BF\u661F"@ja . . "Beta Reticuli"@en . . . . "Beta Reticuli (Beta Ret, \u03B2 Reticuli, \u03B2 Ret) is binary star system in southern constellation of Reticulum. It is visible to the naked eye with an apparent visual magnitude of +3.84. Based upon an annual parallax shift of 33.49 mas, it is located some 97 light years from the Sun. This is a single-lined spectroscopic binary with an orbital period of 5.25 years and an eccentricity of 0.33. The primary, component A, is an evolved K-type giant star with a stellar classification of K0 IVSB:. It is between 5 and 6 billion years old, with 1.2 times the mass of the Sun and 9.3 times the Sun's radius. The companion, component B, is most likely a red dwarf with a classification in the range M0\u2013M4. During the mid-20th century, the Dutch-American astronomer Willem Jacob Luyten proposed that the G3V star HD 24293 formed a third component of this system, based upon similar proper motions. However, this was subsequently ruled out based on more accurate measurements, since their actual distances, radial velocities, and proper motions do not match. Beta Reticuli is moving through the Galaxy at a speed of 69.2 km/s relative to the Sun. Its projected Galactic orbit carries it between 10,100 and 24,200 light years from the center of the Galaxy. Beta Reticuli came closest to the Sun 319,000 years ago when it had brightened to magnitude 2.98 from a distance of 67 light years."@en . . . . . . . "Beta Reticuli (14 Reticuli) \u00E9 uma estrela tripla na dire\u00E7\u00E3o da Reticulum. Possui uma ascens\u00E3o reta de 03h 44m 11.55s e uma declina\u00E7\u00E3o de \u221264\u00B0 48\u2032 25.5\u2033. Sua magnitude aparente \u00E9 igual a 3.84. Considerando sua dist\u00E2ncia de 100 anos-luz em rela\u00E7\u00E3o \u00E0 Terra, sua magnitude absoluta \u00E9 igual a 1.41. Pertence \u00E0 classe espectral K0IV SB. \u00C9 um sistema bin\u00E1rio espetrosc\u00F3pico."@pt . "\u30EC\u30C1\u30AF\u30EB\u5EA7\u03B2\u661F\uFF08\u30EC\u30C1\u30AF\u30EB\u3056\u30D9\u30FC\u30BF\u305B\u3044\u3001\u03B2 Reticuli\u3001\u03B2 Ret\uFF09\u306F\u3001\u30EC\u30C1\u30AF\u30EB\u5EA7\u306B\u3042\u308B\u4E09\u91CD\u661F\u7CFB\u3067\u3001\u5206\u5149\u9023\u661F\u3067\u3042\u308B\u3002\u4E3B\u661F\u306F\u3001\u6A59\u8272\u5DE8\u661F\u3067\u3042\u308B\u3002 \u30EC\u30C1\u30AF\u30EB\u5EA7\u03B2\u661F\u306F\u3001\u592A\u967D\u306B\u5BFE\u3057\u3066\u7D0469.2 km/s\u306E\u901F\u5EA6\u3067\u9280\u6CB3\u7CFB\u5185\u3092\u904B\u52D5\u3057\u3066\u3044\u308B\u3002\u9280\u6CB3\u7CFB\u306E\u4E2D\u5FC3\u304B\u3089\u306F\u300110,100\u5149\u5E74\u304B\u308924,200\u5149\u5E74\u96E2\u308C\u3066\u3044\u308B\u3002 31\u4E079000\u5E74\u524D\u306B\u592A\u967D\u306B\u6700\u3082\u8FD1\u304F67\u5149\u5E74\u307E\u3067\u8FD1\u3065\u304D\u3001\u305D\u306E\u6642\u306F2.98\u7B49\u7D1A\u307E\u3067\u660E\u308B\u304F\u306A\u3063\u305F\u3002"@ja . . . . . . . . . "Beta Reticuli (\u03B2 Reticuli / \u03B2 Ret) est une \u00E9toile binaire de la constellation du R\u00E9ticule, avec une magnitude apparente de +3,84. La composante primaire est une g\u00E9ante orange de type K. Le syst\u00E8me est distant d'environ \u223C102 a.l. (\u223C31,3 pc) de la Terre."@fr . . "Beta Reticuli (\u03B2 Reticuli, f\u00F6rkortat Beta Ret, \u03B2 Ret) som \u00E4r stj\u00E4rnans Bayerbeteckning, \u00E4r en dubbelstj\u00E4rna bel\u00E4gen i den s\u00F6dra delen av stj\u00E4rnbilden Rombiska n\u00E4tet. Den har en skenbar magnitud p\u00E5 3,84 och \u00E4r synlig f\u00F6r blotta \u00F6gat d\u00E4r ljusf\u00F6roreningar ej f\u00F6rekommer. Baserat p\u00E5 parallaxm\u00E4tning inom Hipparcosuppdraget p\u00E5 ca 33,5 mas, ber\u00E4knas den befinna sig p\u00E5 ett avst\u00E5nd p\u00E5 ca 97 ljus\u00E5r (ca 30 parsek) fr\u00E5n solen. Beta Reticuli befann sig n\u00E4rmast solen f\u00F6r 319 000 \u00E5r sedan d\u00E5 den hade en skenbar magnitud p\u00E5 2,98 vid ett avst\u00E5nd av 67 ljus\u00E5r."@sv . . "36735683"^^ . "Beta Reticuli"@fr . "Beta Reticuli (\u03B2 Reticuli / \u03B2 Ret) est une \u00E9toile binaire de la constellation du R\u00E9ticule, avec une magnitude apparente de +3,84. La composante primaire est une g\u00E9ante orange de type K. Le syst\u00E8me est distant d'environ \u223C102 a.l. (\u223C31,3 pc) de la Terre."@fr . . . . . . "J2000.0"@en . . . "5"^^ . . "0.53"^^ . . "\u86C7\u9996\u4E8C(\u7F51\u7F5F\u5EA7\u03B2)\u662F\u4F4D\u4E8E\u7F51\u7F5F\u5EA7\u7684\u53CC\u661F\u7CFB\u7EDF\uFF0C\u5176\u89C6\u661F\u7B49\u4E3A3.84 \u3002"@zh . . . "\u86C7\u9996\u4E8C"@zh . "1079512532"^^ . "+77.50"@en . . . . . . . "Beta Reticuli (14 Reticuli) \u00E9 uma estrela tripla na dire\u00E7\u00E3o da Reticulum. Possui uma ascens\u00E3o reta de 03h 44m 11.55s e uma declina\u00E7\u00E3o de \u221264\u00B0 48\u2032 25.5\u2033. Sua magnitude aparente \u00E9 igual a 3.84. Considerando sua dist\u00E2ncia de 100 anos-luz em rela\u00E7\u00E3o \u00E0 Terra, sua magnitude absoluta \u00E9 igual a 1.41. Pertence \u00E0 classe espectral K0IV SB. \u00C9 um sistema bin\u00E1rio espetrosc\u00F3pico."@pt . ""@en . . . . "+307.13"@en . "\u03B2 Ret A"@en . . . "Beta Reticuli"@en . "Beta Reticuli (Beta Ret, \u03B2 Reticuli, \u03B2 Ret) \u00E8 una stella di magnitudine 3,85 situata nella costellazione australe del Reticolo. \u00C8 la seconda stella pi\u00F9 brillante della costellazione e si trova a circa 100 anni luce dal sistema solare."@it . . "Beta Reticuli (Beta Ret, \u03B2 Reticuli, \u03B2 Ret) is binary star system in southern constellation of Reticulum. It is visible to the naked eye with an apparent visual magnitude of +3.84. Based upon an annual parallax shift of 33.49 mas, it is located some 97 light years from the Sun."@en . . . . . . . . . . . . . . . . . . . . . "+1.11"@en . ""@en . . . . . . "Beta Reticuli"@sv . "Beta Reticuli"@it . . . . . . . . . . . . . . .