About: Kappa Aurigae

An Entity of Type: star, from Named Graph: http://dbpedia.org, within Data Space: dbpedia.org:8891

Kappa Aurigae, Latinised from κ Aurigae, is the Bayer designation for a star in the northern constellation of Auriga. It is visible to the naked eye with an apparent visual magnitude of 4.3. Based upon an annual parallax shift of 18.43 mas, it is approximately 177 light-years (54 parsecs) distant from Earth.

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  • Kappa Aurigae, Latinised from κ Aurigae, is the Bayer designation for a star in the northern constellation of Auriga. It is visible to the naked eye with an apparent visual magnitude of 4.3. Based upon an annual parallax shift of 18.43 mas, it is approximately 177 light-years (54 parsecs) distant from Earth. This is an evolved giant star with a stellar classification of G8.5 IIIb. It is a red clump star, which means it is towards the cool end of the horizontal branch and is generating energy through the fusion of helium at its core. Kappa Aurigae has expanded to 11 times the radius of the Sun and shines with 54 times the Sun's luminosity. This energy is radiated into outer space from the outer envelope at an effective temperature of 4,732 K. At this heat, the star glows with the orange hue of a G-type star. (en)
  • Kappa Aurigae (κ Aur / κ Aurigae) è una stella gigante gialla di magnitudine 4,35 situata nella costellazione dell'Auriga. Dista 169 anni luce dal sistema solare. (it)
  • Каппа Возничего (лат. κ Aurigae), 44 Возничего (лат. 44 Aurigae), HD 43039 — одиночная звезда в созвездии Возничего на расстоянии приблизительно 159 световых лет (около 49 парсеков) от Солнца. Видимая звёздная величина звезды — +4,35m. Возраст звезды оценивается как около 4,7 млрд лет. (ru)
  • Kappa Aurigae (κ Aurigae, förkortat Kappa Aur, κ Aur) som är stjärnans Bayerbeteckning, är en ensam stjärna belägen i den sydöstra delen av stjärnbilden Kusken. Den har en skenbar magnitud på 4,33 och är synlig för blotta ögat där ljusföroreningar ej förekommer. Baserat på parallaxmätning inom Hipparcosuppdraget på ca 19,3 mas, beräknas den befinna sig på ett avstånd på ca 169 ljusår (ca 52 parsek) från solen. (sv)
  • Kappa Aurigae (44 Aurigae) é uma estrela na direção da constelação de Auriga. Possui uma ascensão reta de 06h 15m 22.74s e uma declinação de +29° 29′ 55.4″. Sua magnitude aparente é igual a 4.32. Considerando sua distância de 169 anos-luz em relação à Terra, sua magnitude absoluta é igual a 0.75. Pertence à classe espectral G8IIIvar. (pt)
  • 井宿增一，即拜耳命名法的御夫座κ，是御夫座中的一顆恆星。它的視星等為裸眼可見的4.3等。基於19.31mas的周年視差，它與地球的距離為169光年（52秒差距）。 這是顆演化成巨星的恆星，恆星分類為G8.5 IIIb ，是顆通過氦在核心的核融合產生能量的紅群聚恆星。井宿增一的半徑約為太陽的11倍，亮度約為太陽的54倍。這些能量經由外層傳送進太空，使得表面的有效溫度為4732K。在這種炙熱的情況下，這顆恆星的表面呈現橙色，是一顆G型星 。 (zh)
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  • +0.65 (en)
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dbp:bV
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  • G8.5 IIIb (en)
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  • J2000 (en)
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  • 54 (xsd:integer)
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dbp:metalFe
  • −0.33 (en)
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  • −261.42 (en)
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  • −70.88 (en)
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  • (en)
  • +20.69 ± 0.15 (en)
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  • 11 (xsd:integer)
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dbp:uB
  • +0.812 (en)
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rdfs:comment
  • Kappa Aurigae (κ Aur / κ Aurigae) è una stella gigante gialla di magnitudine 4,35 situata nella costellazione dell'Auriga. Dista 169 anni luce dal sistema solare. (it)
  • Каппа Возничего (лат. κ Aurigae), 44 Возничего (лат. 44 Aurigae), HD 43039 — одиночная звезда в созвездии Возничего на расстоянии приблизительно 159 световых лет (около 49 парсеков) от Солнца. Видимая звёздная величина звезды — +4,35m. Возраст звезды оценивается как около 4,7 млрд лет. (ru)
  • Kappa Aurigae (κ Aurigae, förkortat Kappa Aur, κ Aur) som är stjärnans Bayerbeteckning, är en ensam stjärna belägen i den sydöstra delen av stjärnbilden Kusken. Den har en skenbar magnitud på 4,33 och är synlig för blotta ögat där ljusföroreningar ej förekommer. Baserat på parallaxmätning inom Hipparcosuppdraget på ca 19,3 mas, beräknas den befinna sig på ett avstånd på ca 169 ljusår (ca 52 parsek) från solen. (sv)
  • Kappa Aurigae (44 Aurigae) é uma estrela na direção da constelação de Auriga. Possui uma ascensão reta de 06h 15m 22.74s e uma declinação de +29° 29′ 55.4″. Sua magnitude aparente é igual a 4.32. Considerando sua distância de 169 anos-luz em relação à Terra, sua magnitude absoluta é igual a 0.75. Pertence à classe espectral G8IIIvar. (pt)
  • 井宿增一，即拜耳命名法的御夫座κ，是御夫座中的一顆恆星。它的視星等為裸眼可見的4.3等。基於19.31mas的周年視差，它與地球的距離為169光年（52秒差距）。 這是顆演化成巨星的恆星，恆星分類為G8.5 IIIb ，是顆通過氦在核心的核融合產生能量的紅群聚恆星。井宿增一的半徑約為太陽的11倍，亮度約為太陽的54倍。這些能量經由外層傳送進太空，使得表面的有效溫度為4732K。在這種炙熱的情況下，這顆恆星的表面呈現橙色，是一顆G型星 。 (zh)
  • Kappa Aurigae, Latinised from κ Aurigae, is the Bayer designation for a star in the northern constellation of Auriga. It is visible to the naked eye with an apparent visual magnitude of 4.3. Based upon an annual parallax shift of 18.43 mas, it is approximately 177 light-years (54 parsecs) distant from Earth. (en)
rdfs:label
  • Kappa Aurigae (it)
  • Kappa Aurigae (en)
  • Каппа Возничего (ru)
  • Kappa Aurigae (pt)
  • Kappa Aurigae (sv)
  • 井宿增一 (zh)
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foaf:name
  • κ Aurigae (en)
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