. . . "0.8"^^ . "14.4"^^ . . "1.78"^^ . . . . . . . . "0.54"^^ . . . "Lambda Crateris ( \u03BB Crateris, f\u00F6rkortat Lambda Crt, \u03BB Crt) som \u00E4r stj\u00E4rnans Bayerbeteckning, \u00E4r en misst\u00E4nkt dubbelstj\u00E4rna bel\u00E4gen i den mellersta delen av stj\u00E4rnbilden B\u00E4garen. Den har en skenbar magnitud p\u00E5 5,02 och \u00E4r svagt synlig f\u00F6r blotta \u00F6gat d\u00E4r ljusf\u00F6roreningar ej f\u00F6rekommer. Baserat p\u00E5 parallaxm\u00E4tning inom Hipparcosuppdraget p\u00E5 ca 23,3 mas, ber\u00E4knas den befinna sig p\u00E5 ett avst\u00E5nd p\u00E5 ca 140 ljus\u00E5r (ca 43 parsek) fr\u00E5n solen."@sv . . . "5.08"^^ . . . . "\u2212305.37"@en . . "+1.92"@en . . "Lambda Crateris (13 Crateris) \u00E9 uma estrela bin\u00E1ria na dire\u00E7\u00E3o da constela\u00E7\u00E3o de Crater. Possui uma ascens\u00E3o reta de 11h 23m 22.07s e uma declina\u00E7\u00E3o de \u221218\u00B0 46\u2032 47.6\u2033. Sua magnitude aparente \u00E9 igual a 5.08. Considerando sua dist\u00E2ncia de 143 anos-luz em rela\u00E7\u00E3o \u00E0 Terra, sua magnitude absoluta \u00E9 igual a 1.87. Pertence \u00E0 classe espectral F3IV. \u00C9 um sistema bin\u00E1rio espetrosc\u00F3pico."@pt . "Lambda Crateris"@en . . . . . . . . "Lambda Crateris (13 Crateris) \u00E9 uma estrela bin\u00E1ria na dire\u00E7\u00E3o da constela\u00E7\u00E3o de Crater. Possui uma ascens\u00E3o reta de 11h 23m 22.07s e uma declina\u00E7\u00E3o de \u221218\u00B0 46\u2032 47.6\u2033. Sua magnitude aparente \u00E9 igual a 5.08. Considerando sua dist\u00E2ncia de 143 anos-luz em rela\u00E7\u00E3o \u00E0 Terra, sua magnitude absoluta \u00E9 igual a 1.87. Pertence \u00E0 classe espectral F3IV. \u00C9 um sistema bin\u00E1rio espetrosc\u00F3pico."@pt . "17"^^ . "32722"^^ . . . . . . . . "F5 III"@en . "Lambda Crateris ( \u03BB Crateris, f\u00F6rkortat Lambda Crt, \u03BB Crt) som \u00E4r stj\u00E4rnans Bayerbeteckning, \u00E4r en misst\u00E4nkt dubbelstj\u00E4rna bel\u00E4gen i den mellersta delen av stj\u00E4rnbilden B\u00E4garen. Den har en skenbar magnitud p\u00E5 5,02 och \u00E4r svagt synlig f\u00F6r blotta \u00F6gat d\u00E4r ljusf\u00F6roreningar ej f\u00F6rekommer. Baserat p\u00E5 parallaxm\u00E4tning inom Hipparcosuppdraget p\u00E5 ca 23,3 mas, ber\u00E4knas den befinna sig p\u00E5 ett avst\u00E5nd p\u00E5 ca 140 ljus\u00E5r (ca 43 parsek) fr\u00E5n solen."@sv . . "Lambda Crateris, Latinized from \u03BB Crateris, is the Bayer designation for a suspected binary star system in the southern constellation of Crater. With an annual parallax shift of 23.32 milliarcsecond as observed from Earth, it is located around 140 light years from the Sun. It is faintly visible to the naked eye with an apparent visual magnitude of 5.08."@en . "J2000.0"@en . . . "2.8"^^ . . . . "140.7"^^ . . . . . . . "1117372813"^^ . . "+27.56"@en . . . . . . . . . "23.32"^^ . . . . "Lambda Crateris"@sv . . . . "53328437"^^ . "Lambda Crateris"@pt . . "8657"^^ . "\u22120.04"@en . . . . . . . . "Lambda Crateris"@en . . . . . . "2.5"^^ . "Lambda Crateris, Latinized from \u03BB Crateris, is the Bayer designation for a suspected binary star system in the southern constellation of Crater. With an annual parallax shift of 23.32 milliarcsecond as observed from Earth, it is located around 140 light years from the Sun. It is faintly visible to the naked eye with an apparent visual magnitude of 5.08. This is a probable astrometric binary star system, with orbital elements first reported by Abt and Levy (1976). However, Morbey and Griffin (1987) later cast some doubt on the validity of these results, suggesting that further review is needed. The visible member of this system, component A, is an evolved F-type giant star with a stellar classification of F5 III. It has an estimated 1.78 times the mass of the Sun and 2.8 times the Sun's radius. The star is spinning with a projected rotational velocity of 17 km/s."@en . . . "+0.43"@en . . .