About: Nu Microscopii

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ν Microscopii, Latinized as Nu Microscopii, is a star in the constellation Microscopium. It is an orange hued star that is visible to the naked eye as a faint point of light with an apparent visual magnitude of 4.76. It was first catalogued as Nu Indi by the French explorer and astronomer Nicolas Louis de Lacaille in 1756, before being reclassified in Microscopium and given its current Bayer designation of Nu Microscopii by Gould. The object is located at a distance of around 252 light-years from the Sun, based on parallax, and is drifting further away with a radial velocity of about +9 km/s.

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  • ν Microscopii, Latinized as Nu Microscopii, is a star in the constellation Microscopium. It is an orange hued star that is visible to the naked eye as a faint point of light with an apparent visual magnitude of 4.76. It was first catalogued as Nu Indi by the French explorer and astronomer Nicolas Louis de Lacaille in 1756, before being reclassified in Microscopium and given its current Bayer designation of Nu Microscopii by Gould. The object is located at a distance of around 252 light-years from the Sun, based on parallax, and is drifting further away with a radial velocity of about +9 km/s. It is an aging giant star with a stellar classification of K0 III. It has expanded to 10.6 times the girth of the Sun after exhausting the supply of hydrogen at its core and evolving off the main sequence. The star has 2.46 times the mass of the Sun. It is radiating 59.5 times the Sun's luminosity from its swollen photosphere at an effective temperature of 4,925 K. (en)
  • Nu Microscopii (6 Microscopii) é uma estrela na direção da constelação de Microscopium. Possui uma ascensão reta de 20h 33m 55.06s e uma declinação de −44° 30′ 57.5″. Sua magnitude aparente é igual a 5.12. Considerando sua distância de 216 anos-luz em relação à Terra, sua magnitude absoluta é igual a 1.01. Pertence à classe espectral K0III. (pt)
  • Ny Microscopii (ν Microscopii, förkortat Ny Mic, ν Mic) som är stjärnans Bayerbeteckning, är en ensam stjärna belägen i den sydvästra delen av stjärnbilden Mikroskopet. Den har en skenbar magnitud på 5,13 och är synlig för blotta ögat där ljusföroreningar ej förekommer. Baserat på parallaxmätning inom Hipparcosuppdraget på ca 13,9 mas, beräknas den befinna sig på ett avstånd på ca 234 ljusår (ca 72 parsek) från solen. (sv)
  • 顯微鏡座ν，又名CD-4414020，HD 195569、SAO 230276、HR 7846，是顯微鏡座的一颗恒星，视星等为5.11，位于銀經356，銀緯-36.45，其B1900.0坐标为赤經20h 27m 2.8s，赤緯-44° -36.45′ 18″。 (zh)
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  • +0.84 (en)
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  • 4.760000 (xsd:double)
dbp:class
  • K0 III (en)
dbp:constell
dbp:epoch
dbp:equinox
  • J2000.0 (en)
dbp:gravity
  • 2.780000 (xsd:double)
dbp:mass
  • 2.460000 (xsd:double)
dbp:pError
  • 0.108100 (xsd:double)
dbp:parallax
  • 12.948000 (xsd:double)
dbp:propMoDec
  • -35.224000 (xsd:double)
dbp:propMoRa
  • +11.727 (en)
dbp:rotationalVelocity
  • 2.020000 (xsd:double)
dbp:uB
  • +1.009 (en)
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rdfs:comment
  • Nu Microscopii (6 Microscopii) é uma estrela na direção da constelação de Microscopium. Possui uma ascensão reta de 20h 33m 55.06s e uma declinação de −44° 30′ 57.5″. Sua magnitude aparente é igual a 5.12. Considerando sua distância de 216 anos-luz em relação à Terra, sua magnitude absoluta é igual a 1.01. Pertence à classe espectral K0III. (pt)
  • Ny Microscopii (ν Microscopii, förkortat Ny Mic, ν Mic) som är stjärnans Bayerbeteckning, är en ensam stjärna belägen i den sydvästra delen av stjärnbilden Mikroskopet. Den har en skenbar magnitud på 5,13 och är synlig för blotta ögat där ljusföroreningar ej förekommer. Baserat på parallaxmätning inom Hipparcosuppdraget på ca 13,9 mas, beräknas den befinna sig på ett avstånd på ca 234 ljusår (ca 72 parsek) från solen. (sv)
  • 顯微鏡座ν，又名CD-4414020，HD 195569、SAO 230276、HR 7846，是顯微鏡座的一颗恒星，视星等为5.11，位于銀經356，銀緯-36.45，其B1900.0坐标为赤經20h 27m 2.8s，赤緯-44° -36.45′ 18″。 (zh)
  • ν Microscopii, Latinized as Nu Microscopii, is a star in the constellation Microscopium. It is an orange hued star that is visible to the naked eye as a faint point of light with an apparent visual magnitude of 4.76. It was first catalogued as Nu Indi by the French explorer and astronomer Nicolas Louis de Lacaille in 1756, before being reclassified in Microscopium and given its current Bayer designation of Nu Microscopii by Gould. The object is located at a distance of around 252 light-years from the Sun, based on parallax, and is drifting further away with a radial velocity of about +9 km/s. (en)
rdfs:label
  • Nu Microscopii (en)
  • Nu Microscopii (pt)
  • 顯微鏡座ν (zh)
  • Ny Microscopii (sv)
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foaf:name
  • ν Microscopii (en)
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