"11 Puppis"@it . . . "11 Puppis \u00E8 una stella gigante brillante bianco-gialla di magnitudine 4,2 situata nella costellazione della Poppa. Dista 503 anni luce dal sistema solare."@it . . . . . "222 Puppis (j Puppis) \u00E9 uma estrela na dire\u00E7\u00E3o da Puppis. Possui uma ascens\u00E3o reta de 07h 56m 51.56s e uma declina\u00E7\u00E3o de \u221222\u00B0 52\u2032 48.5\u2033. Sua magnitude aparente \u00E9 igual a 4.20. Considerando sua dist\u00E2ncia de 502 anos-luz em rela\u00E7\u00E3o \u00E0 Terra, sua magnitude absoluta \u00E9 igual a \u22121.74. Pertence \u00E0 classe espectral F7/F8II."@pt . . . . "515"^^ . . . "222 Puppis"@pt . . . . . "11 Puppis \u00E8 una stella gigante brillante bianco-gialla di magnitudine 4,2 situata nella costellazione della Poppa. Dista 503 anni luce dal sistema solare."@it . "+0.44"@en . . . . . . . "11 Puppis is a single star in the southern constellation of Puppis, located approximately 522 light years away based on parallax. It has the Bayer designation j Puppis; 11 Puppis is the Flamsteed designation. This object is visible to the naked eye as a faint, yellow-white star with an apparent visual magnitude of 4.20. It is moving further from the Earth with a heliocentric radial velocity of +13.3 km/s. This is an evolved bright giant star with a stellar classification of F7/8 II. The spectrum displays a deficit of carbon, an excesses of nitrogen, and a high abundance of lithium. The first two anomalies suggest the giant has passed through a deep convection stage that would have also exhausted the lithium supply, indicating the current lithium abundance is of recent production. The star has 2.7 times the mass of the Sun and is radiating 515 times the Sun's luminosity from its enlarged photosphere at an effective temperature of 5,868 K."@en . . "J2000"@en . . . . "13.8"^^ . "F7/8 II"@en . . "4.2"^^ . "1079514985"^^ . . . . . . . . . . . . . "11 Puppis (11 Pup / j Puppis / HD 65228 / HR 3102)\u200B es una estrella en la constelaci\u00F3n de Puppis, la popa del Argo Navis.Duod\u00E9cima en brillo entre las estrellas de su constelaci\u00F3n, su magnitud aparente es +4,20.\u200B Se encuentra a unos 500 a\u00F1os luz del Sistema Solar. No existe unanimidad en lo referente a la metalicidad \u2014abundancia relativa de elementos m\u00E1s pesados que el helio\u2014 de 11 Puppis; un estudio se\u00F1ala una metalicidad igual a la solar,\u200B mientras que otro trabajo se\u00F1ala un contenido met\u00E1lico tres veces mayor que el de nuestra estrella.\u200B"@es . "11 Puppis"@en . . . "\u22121.82"@en . "11 Puppis (11 Pup / j Puppis / HD 65228 / HR 3102)\u200B es una estrella en la constelaci\u00F3n de Puppis, la popa del Argo Navis.Duod\u00E9cima en brillo entre las estrellas de su constelaci\u00F3n, su magnitud aparente es +4,20.\u200B Se encuentra a unos 500 a\u00F1os luz del Sistema Solar. 11 Puppis es una gigante luminosa blanco-amarilla de tipo espectral F7/F8 II con una temperatura superficial de 5932 K.Aunque las gigantes de tipo K y G-tard\u00EDo son abundantes, las de tipo F \u2014m\u00E1s calientes\u2014 no lo son tanto; 25 Monocerotis o \u03C1 Puppis pertenecen a esta clase, pero 11 Puppis es claramente m\u00E1s luminosa que cualquiera de ellas.11 Puppis brilla con una luminosidad 457 veces superior a la del Sol\u200B y 20 veces superior a la de \u03C1 Puppis.Tiene un radio 24 veces m\u00E1s grande que el radio solar\u200B y es una estrella masiva de 4,2 masas solares con una edad aproximada de 145 millones de a\u00F1os.\u200B No existe unanimidad en lo referente a la metalicidad \u2014abundancia relativa de elementos m\u00E1s pesados que el helio\u2014 de 11 Puppis; un estudio se\u00F1ala una metalicidad igual a la solar,\u200B mientras que otro trabajo se\u00F1ala un contenido met\u00E1lico tres veces mayor que el de nuestra estrella.\u200B Esta estrella no debe ser confundida con HD 64760, conocida tambi\u00E9n como J Puppis."@es . . "5868"^^ . "+13.30"@en . . . "\u8239\u5C3E\u5EA711\uFF0C\u53C8\u540DBD-22 2087\uFF0CHD 65228\u3001SAO 174852\u3001HR 3102\uFF0C\u662F\u8239\u5C3E\u5EA7\u7684\u4E00\u9897\u6052\u661F\uFF0C\u89C6\u661F\u7B49\u4E3A4.2\uFF0C\u4F4D\u4E8E\u9280\u7D93240.64\uFF0C\u9280\u7DEF3.07\uFF0C\u5176B1900.0\u5750\u6807\u4E3A\u8D64\u7D937h 52m 33.5s\uFF0C\u8D64\u7DEF-22\u00B0 3.07\u2032 47\u2033\u3002"@zh . . . "2.7"^^ . . . "6.25"^^ . . . . . . . . . "222 Puppis (j Puppis) \u00E9 uma estrela na dire\u00E7\u00E3o da Puppis. Possui uma ascens\u00E3o reta de 07h 56m 51.56s e uma declina\u00E7\u00E3o de \u221222\u00B0 52\u2032 48.5\u2033. Sua magnitude aparente \u00E9 igual a 4.20. Considerando sua dist\u00E2ncia de 502 anos-luz em rela\u00E7\u00E3o \u00E0 Terra, sua magnitude absoluta \u00E9 igual a \u22121.74. Pertence \u00E0 classe espectral F7/F8II."@pt . "11 Puppis"@sv . "11 Puppis (11 Pup), som \u00E4r stj\u00E4rnans Flamsteedbeteckning (eller Bayerbeteckning j Pup), \u00E4r en ensam stj\u00E4rna bel\u00E4gen i den norra delen av stj\u00E4rnbilden Akterskeppet. Den har en skenbar magnitud p\u00E5 4,20 och \u00E4r synlig f\u00F6r blotta \u00F6gat d\u00E4r ljusf\u00F6roreningar ej f\u00F6rekommer. Baserat p\u00E5 parallaxm\u00E4tning inom Hipparcosuppdraget p\u00E5 ca 6,3 mas, ber\u00E4knas den befinna sig p\u00E5 ett avst\u00E5nd p\u00E5 ca 520 ljus\u00E5r (ca 160 parsek) fr\u00E5n solen. Den r\u00F6r sig bort fr\u00E5n jorden med en heliocentrisk radiell hastighet av +13,3 km/s."@sv . . . "+11.49"@en . . "\u221230.42"@en . "38324402"^^ . . . . . "6272"^^ . . "11 Puppis is a single star in the southern constellation of Puppis, located approximately 522 light years away based on parallax. It has the Bayer designation j Puppis; 11 Puppis is the Flamsteed designation. This object is visible to the naked eye as a faint, yellow-white star with an apparent visual magnitude of 4.20. It is moving further from the Earth with a heliocentric radial velocity of +13.3 km/s."@en . . . . . . "1.99"^^ . "11 Puppis (11 Pup), som \u00E4r stj\u00E4rnans Flamsteedbeteckning (eller Bayerbeteckning j Pup), \u00E4r en ensam stj\u00E4rna bel\u00E4gen i den norra delen av stj\u00E4rnbilden Akterskeppet. Den har en skenbar magnitud p\u00E5 4,20 och \u00E4r synlig f\u00F6r blotta \u00F6gat d\u00E4r ljusf\u00F6roreningar ej f\u00F6rekommer. Baserat p\u00E5 parallaxm\u00E4tning inom Hipparcosuppdraget p\u00E5 ca 6,3 mas, ber\u00E4knas den befinna sig p\u00E5 ett avst\u00E5nd p\u00E5 ca 520 ljus\u00E5r (ca 160 parsek) fr\u00E5n solen. Den r\u00F6r sig bort fr\u00E5n jorden med en heliocentrisk radiell hastighet av +13,3 km/s."@sv . . . . . . . . . . . . "\u8239\u5C3E\u5EA711\uFF0C\u53C8\u540DBD-22 2087\uFF0CHD 65228\u3001SAO 174852\u3001HR 3102\uFF0C\u662F\u8239\u5C3E\u5EA7\u7684\u4E00\u9897\u6052\u661F\uFF0C\u89C6\u661F\u7B49\u4E3A4.2\uFF0C\u4F4D\u4E8E\u9280\u7D93240.64\uFF0C\u9280\u7DEF3.07\uFF0C\u5176B1900.0\u5750\u6807\u4E3A\u8D64\u7D937h 52m 33.5s\uFF0C\u8D64\u7DEF-22\u00B0 3.07\u2032 47\u2033\u3002"@zh . . . "+0.72"@en . . . "+0.09"@en . "0.23"^^ . "11 Puppis"@es . . . "\u5F27\u77E2\u589E\u5341\u4E94"@zh . .