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Statements

Subject Item
dbr:Rho_Cet
dbo:wikiPageWikiLink
dbr:Rho_Ceti
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dbr:Rho_Ceti
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Rho Ceti Rho Ceti 蒭藁一 Rho Ceti Rho Ceti Rho Ceti Rho Ceti
rdfs:comment
Rho Ceti (72 Ceti) é uma estrela na direção da constelação de Cetus. Possui uma ascensão reta de 02h 25m 57.01s e uma declinação de −12° 17′ 25.6″. Sua magnitude aparente é igual a 4.88. Considerando sua distância de 528 anos-luz em relação à Terra, sua magnitude absoluta é igual a −1.17. Pertence à classe espectral A0V. Sigma Ceti (σ Cet / σ Ceti) adalah salah satu bintang di rasi Cetus. Sigma Cetus tergolong bintang dengan kelas A0V dan magnitudo 4.88. Bintang ini berada pada jarak 528 tahun cahaya dari Bumi. Rho Ceti (ρ Cet / ρ Ceti) è una stella bianca nella sequenza principale di magnitudine 4,87 situata nella costellazione della Balena. Dista 529 anni luce dal sistema solare. Rho Ceti (ρ Ceti / ρ Cet) est une étoile de la constellation équatoriale de la Baleine. Elle est visible à l'œil nu et sa magnitude apparente est de 4,89. L'étoile présente une parallaxe annuelle de 5,81 mas telle que mesurée par le satellite Gaia, ce qui permet d'en déduire qu'elle est distante d'environ 172 pc (∼561 a.l.) de la Terre. Elle s'éloigne du Système solaire à une vitesse radiale de +19 km/s. 鯨魚座ρ，又名BD-12 451，HD 15130、SAO 148385、HR 708，是鯨魚座的一颗恒星，视星等为4.89，位于銀經183.75，銀緯-63.35，其B1900.0坐标为赤經2h 21m 7.1s，赤緯-12° -63.35′ 29″。 Rho Ceti , Latinized from ρ Ceti, is the Bayer designation for a star in the equatorial constellation of Cetus. It is faintly visible to the naked eye with an apparent visual magnitude of 4.885. The distance to this star, based upon an annual parallax shift of 7.15 mas, is around 460 light years. Rho Ceti (ρ Ceti, förkortat Rho Cet, ρ Cet) som är stjärnans Bayerbeteckning, är en ensam stjärna belägen i den östra delen av stjärnbilden Valfisken (stjärnbild). Den har en skenbar magnitud på 4,89 och är svagt synlig för blotta ögat där ljusföroreningar ej förekommer. Baserat på parallaxmätning inom Hipparcosuppdraget på ca 7,2 mas, beräknas den befinna sig på ett avstånd av ca 460 ljusår (ca 140 parsek) från solen.
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Rho Ceti
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dbp:absmagV
−0.85
dbp:appmagV
4.885
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3.1
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219
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8905
dbp:uB
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dbo:abstract
Rho Ceti (72 Ceti) é uma estrela na direção da constelação de Cetus. Possui uma ascensão reta de 02h 25m 57.01s e uma declinação de −12° 17′ 25.6″. Sua magnitude aparente é igual a 4.88. Considerando sua distância de 528 anos-luz em relação à Terra, sua magnitude absoluta é igual a −1.17. Pertence à classe espectral A0V. 鯨魚座ρ，又名BD-12 451，HD 15130、SAO 148385、HR 708，是鯨魚座的一颗恒星，视星等为4.89，位于銀經183.75，銀緯-63.35，其B1900.0坐标为赤經2h 21m 7.1s，赤緯-12° -63.35′ 29″。 Rho Ceti (ρ Ceti, förkortat Rho Cet, ρ Cet) som är stjärnans Bayerbeteckning, är en ensam stjärna belägen i den östra delen av stjärnbilden Valfisken (stjärnbild). Den har en skenbar magnitud på 4,89 och är svagt synlig för blotta ögat där ljusföroreningar ej förekommer. Baserat på parallaxmätning inom Hipparcosuppdraget på ca 7,2 mas, beräknas den befinna sig på ett avstånd av ca 460 ljusår (ca 140 parsek) från solen. Rho Ceti (ρ Cet / ρ Ceti) è una stella bianca nella sequenza principale di magnitudine 4,87 situata nella costellazione della Balena. Dista 529 anni luce dal sistema solare. Sigma Ceti (σ Cet / σ Ceti) adalah salah satu bintang di rasi Cetus. Sigma Cetus tergolong bintang dengan kelas A0V dan magnitudo 4.88. Bintang ini berada pada jarak 528 tahun cahaya dari Bumi. Rho Ceti (ρ Ceti / ρ Cet) est une étoile de la constellation équatoriale de la Baleine. Elle est visible à l'œil nu et sa magnitude apparente est de 4,89. L'étoile présente une parallaxe annuelle de 5,81 mas telle que mesurée par le satellite Gaia, ce qui permet d'en déduire qu'elle est distante d'environ 172 pc (∼561 a.l.) de la Terre. Elle s'éloigne du Système solaire à une vitesse radiale de +19 km/s. Rho Ceti , Latinized from ρ Ceti, is the Bayer designation for a star in the equatorial constellation of Cetus. It is faintly visible to the naked eye with an apparent visual magnitude of 4.885. The distance to this star, based upon an annual parallax shift of 7.15 mas, is around 460 light years. This is an A-type main sequence star with a stellar classification of A0 V. It is spinning rapidly with a projected rotational velocity of 219 km/s, giving the star an oblate shape with an equatorial bulge that is 10% larger than the polar radius. The star has an estimated size 3.1 times the radius of the Sun and is radiating 178 times the solar luminosity from its outer atmosphere at an effective temperature of 8,905 K.
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