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κ Pictoris, Latinised as Kappa Pictoris, is a star in the constellation Pictor. It is close to the lower limit of stars that are visible to the naked eye having an apparent visual magnitude of +6.11. Based upon an annual parallax shift of 5.14 mas as seen from Earth, this star is located around 630 light years from the Sun. At that distance, the visual magnitude is diminished by an extinction factor of 0.10 due to interstellar dust.

AttributesValues
rdf:type
rdfs:label
  • Kappa Pictoris (en)
  • Kappa Pictoris (pt)
  • Kappa Pictoris (sv)
  • 繪架座κ (zh)
rdfs:comment
  • Kappa Pictoris (κ Pictoris, förkortat Kappa Pic, κ Pic) som är stjärnans Bayerbeteckning, är en ensam stjärna belägen i den södra delen av stjärnbilden Målaren. Den har en skenbar magnitud på 6,11 och är svagt synlig för blotta ögat där ljusföroreningar ej förekommer. Baserat på parallaxmätning inom Hipparcosuppdraget på ca 5,1 mas, beräknas den befinna sig på ett avstånd på ca 630 ljusår (ca 30 parsek) från solen. På det beräknade avståndet minskas dess skenbara magnitud med 0,10 enheter beroende på mellanliggande interstellärt stoft. (sv)
  • Kappa Pictoris (κ Pic, κ Pictoris) é uma estrela na constelação de Pictor. Com uma magnitude aparente visual de 6,09, só é visível a olho nu em excelentes condições de visualização. De acordo com sua paralaxe, está localizada a aproximadamente 670 anos-luz (206 parsecs) da Terra. É uma estrela de classe B da sequência principal com um tipo espectral de B8.5 V e temperatura efetiva 11 640 K, portanto possui coloração azul-branca. Possui uma massa de 3,42 vezes a massa solar e está brilhando com 210 vezes a luminosidade solar. (pt)
  • 繪架座κ,又名CP-56 840,HD 35580、SAO 233952、HR 1801,是繪架座的一颗恒星,视星等为6.11,位于銀經264.19,銀緯-34.51,其B1900.0坐标为赤經5h 20m 31.5s,赤緯-56° -34.51′ 42″。 (zh)
  • κ Pictoris, Latinised as Kappa Pictoris, is a star in the constellation Pictor. It is close to the lower limit of stars that are visible to the naked eye having an apparent visual magnitude of +6.11. Based upon an annual parallax shift of 5.14 mas as seen from Earth, this star is located around 630 light years from the Sun. At that distance, the visual magnitude is diminished by an extinction factor of 0.10 due to interstellar dust. (en)
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  • Kappa Pictoris (en)
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absmag v
  • +0.34 (en)
age myr
appmag v
  • +6.11 (en)
b-v
  • −0.10 (en)
class
  • B8/9 V (en)
constell
epoch
equinox
  • J2000.0 (en)
luminosity
p error
parallax
prop mo dec
  • +22.01 (en)
prop mo ra
  • −5.03 (en)
rotational velocity
temperature
has abstract
  • κ Pictoris, Latinised as Kappa Pictoris, is a star in the constellation Pictor. It is close to the lower limit of stars that are visible to the naked eye having an apparent visual magnitude of +6.11. Based upon an annual parallax shift of 5.14 mas as seen from Earth, this star is located around 630 light years from the Sun. At that distance, the visual magnitude is diminished by an extinction factor of 0.10 due to interstellar dust. This is a B-type main sequence star with a stellar classification of B8/9 V. It is about 76.4% of the way through its main sequence lifespan. The star is spinning rapidly with a projected rotational velocity of 264 km/s. It has an estimated 3.4 times the mass of the Sun and is radiating 210 times the Sun's luminosity from its photosphere at an effective temperature of 11,641 K. (en)
  • Kappa Pictoris (κ Pictoris, förkortat Kappa Pic, κ Pic) som är stjärnans Bayerbeteckning, är en ensam stjärna belägen i den södra delen av stjärnbilden Målaren. Den har en skenbar magnitud på 6,11 och är svagt synlig för blotta ögat där ljusföroreningar ej förekommer. Baserat på parallaxmätning inom Hipparcosuppdraget på ca 5,1 mas, beräknas den befinna sig på ett avstånd på ca 630 ljusår (ca 30 parsek) från solen. På det beräknade avståndet minskas dess skenbara magnitud med 0,10 enheter beroende på mellanliggande interstellärt stoft. (sv)
  • Kappa Pictoris (κ Pic, κ Pictoris) é uma estrela na constelação de Pictor. Com uma magnitude aparente visual de 6,09, só é visível a olho nu em excelentes condições de visualização. De acordo com sua paralaxe, está localizada a aproximadamente 670 anos-luz (206 parsecs) da Terra. É uma estrela de classe B da sequência principal com um tipo espectral de B8.5 V e temperatura efetiva 11 640 K, portanto possui coloração azul-branca. Possui uma massa de 3,42 vezes a massa solar e está brilhando com 210 vezes a luminosidade solar. (pt)
  • 繪架座κ,又名CP-56 840,HD 35580、SAO 233952、HR 1801,是繪架座的一颗恒星,视星等为6.11,位于銀經264.19,銀緯-34.51,其B1900.0坐标为赤經5h 20m 31.5s,赤緯-56° -34.51′ 42″。 (zh)
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