. . . "\u22120.18"@en . . "B"@en . "HD 119124 \u00E4r en gles dubbelstj\u00E4rna bel\u00E4gen i den mellersta delen av stj\u00E4rnbilden Stora bj\u00F6rnen. Den har en skenbar magnitud av ca 6,32 och kr\u00E4ver \u00E5tminstone en handkikare f\u00F6r att kunna observeras. Baserat p\u00E5 parallax enligt Gaia Data Release 2 p\u00E5 ca 39,2 mas, ber\u00E4knas den befinna sig p\u00E5 ett avst\u00E5nd p\u00E5 ca 83 ljus\u00E5r (ca 25 parsek) fr\u00E5n solen. Den r\u00F6r sig n\u00E4rmare solen med en heliocentrisk radialhastighet p\u00E5 ca -12 km/s. Stj\u00E4rnan \u00E4r en trolig medlem i Castor r\u00F6relsegrupp."@sv . . "HD 119124 is a wide binary star system in the circumpolar constellation of Ursa Major. With an apparent visual magnitude of 6.3, it lies below the normal brightness limit of stars that are visible with the naked eye under most viewing conditions. An annual parallax shift of 39.24 mas for the A component provides a distance estimate of 83 light years. The pair are candidate members of the Castor Moving Group, which implies a relatively youthful age of around 200 million years. HD 119124 is moving closer to the Sun with a radial velocity of \u221212 km/s. This system was first identified as a double star by Friedrich von Struve (1793\u22121864) and catalogued as the 1774th entry in his list. As of 2015, the magnitude 10.5 K-type companion star was located at an angular separation of 18.10 arc seconds along a position angle of 135\u00B0 from the brighter primary. They appear to be gravitationally bound with an estimated orbital period of around 7,000 years and a linear projected separation of 444.6 AU. The primary, component A, is a Sun-like star with a stellar classification of F8 V, indicating it is an F-type main-sequence star that is generating energy via hydrogen fusion at its core. It is slightly larger and more massive than the Sun and appears mildly variable. The star is radiating 1.5 times the Sun's luminosity from its photosphere at an effective temperature of 6,149 K. HD 119124 A displays a strong infrared excess at a wavelength of 70 \u03BCm, indicating an orbiting circumstellar disk of cold dust. The emission fits a model with a grain temperature of 40 K, indicating a minimum orbital radius of 60 AU from the host star. The estimated grain lifetimes are 84,000 years \u2013 much shorter than the star's lifespan. This suggests the grains are being replenished via collisions between some number of larger bodies totaling around 1\u22126 times the mass of the Moon. This system is a likely (80.4% chance) source of the strong X-ray emission coming from these coordinates."@en . . "+0.52"@en . "0.0354"^^ . "HD 119124"@sv . "39.3513"^^ . . "1.1"^^ . . . . . "10.51"^^ . . "1.15"^^ . . . "6149"^^ . . . . . . . . "39.2353"^^ . . . . . . . . . . . . . "HD 119124"@zh . . . . . . . . . "4.3"^^ . . . . . "10.2"^^ . "4130"^^ . . "6.32"^^ . . "56400051"^^ . . . "12442"^^ . . "1.5"^^ . . "F8 V + K7"@en . . "1079517585"^^ . . . . . . . "HD 119124\uFF0C\u53C8\u540DBD+51 1859\uFF0CSAO 28836\u3001HR 5148\uFF0C\u662F\u4E00\u9897\u6052\u661F\uFF0C\u89C6\u661F\u7B49\u4E3A6.32\uFF0C\u4F4D\u4E8E\u9280\u7D93104.46\uFF0C\u9280\u7DEF64.82\uFF0C\u5176B1900.0\u5750\u6807\u4E3A\u8D64\u7D9313h 36m 25.3s\uFF0C\u8D64\u7DEF+51\u00B0 64.82\u2032 26\u2033\u3002"@zh . . . "0.0326"^^ . "HD 119124 \u00E4r en gles dubbelstj\u00E4rna bel\u00E4gen i den mellersta delen av stj\u00E4rnbilden Stora bj\u00F6rnen. Den har en skenbar magnitud av ca 6,32 och kr\u00E4ver \u00E5tminstone en handkikare f\u00F6r att kunna observeras. Baserat p\u00E5 parallax enligt Gaia Data Release 2 p\u00E5 ca 39,2 mas, ber\u00E4knas den befinna sig p\u00E5 ett avst\u00E5nd p\u00E5 ca 83 ljus\u00E5r (ca 25 parsek) fr\u00E5n solen. Den r\u00F6r sig n\u00E4rmare solen med en heliocentrisk radialhastighet p\u00E5 ca -12 km/s. Stj\u00E4rnan \u00E4r en trolig medlem i Castor r\u00F6relsegrupp."@sv . . . . . . . "J2000"@en . . . "0.63"^^ . . . . . "HD 119124 is a wide binary star system in the circumpolar constellation of Ursa Major. With an apparent visual magnitude of 6.3, it lies below the normal brightness limit of stars that are visible with the naked eye under most viewing conditions. An annual parallax shift of 39.24 mas for the A component provides a distance estimate of 83 light years. The pair are candidate members of the Castor Moving Group, which implies a relatively youthful age of around 200 million years. HD 119124 is moving closer to the Sun with a radial velocity of \u221212 km/s."@en . . "HD 119124"@en . . "\u22120.01"@en . "HD 119124\uFF0C\u53C8\u540DBD+51 1859\uFF0CSAO 28836\u3001HR 5148\uFF0C\u662F\u4E00\u9897\u6052\u661F\uFF0C\u89C6\u661F\u7B49\u4E3A6.32\uFF0C\u4F4D\u4E8E\u9280\u7D93104.46\uFF0C\u9280\u7DEF64.82\uFF0C\u5176B1900.0\u5750\u6807\u4E3A\u8D64\u7D9313h 36m 25.3s\uFF0C\u8D64\u7DEF+51\u00B0 64.82\u2032 26\u2033\u3002"@zh . . . "A"@en . . . .