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33 Cygni is a single star located 159 light years away in the northern constellation Cygnus. It is visible to the naked eye as a white-hued star with an apparent visual magnitude of 4.28. The star is moving closer to the Earth with a heliocentric radial velocity of −16 km/s. Eggen (1995) listed it as a proper motion candidate for membership in the IC 2391 supercluster.

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  • 33 Cygni (en)
  • 33 Cygni (sv)
  • 奚仲增四 (zh)
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  • 33 Cygni, som är stjärnans Flamsteed-beteckning, är en ensam stjärna belägen i den norra delen av stjärnbilden Svanen. Den har en genomsnittlig skenbar magnitud på ca 4,28 och är svagt synlig för blotta ögat där ljusföroreningar ej förekommer. Baserat på parallaxmätning inom Hipparcosuppdraget på ca 20,5 mas, beräknas den befinna sig på ett avstånd av ca 159 ljusår (ca 49 parsek) från solen. Den rör sig närmare solen med en heliocentrisk radialhastighet av ca -16 km/s. Eggen (1995) listade den som en kandidat till att ingå i superhopen IC 2391. (sv)
  • 天鵝座33,又名BD+56 2376,HD 192696、SAO 32378、HR 7740,是天鵝座的一颗恒星,视星等为4.3,位于銀經91.08,銀緯12.06,其B1900.0坐标为赤經20h 11m 4.4s,赤緯+56° 12.06′ 42″。 (zh)
  • 33 Cygni is a single star located 159 light years away in the northern constellation Cygnus. It is visible to the naked eye as a white-hued star with an apparent visual magnitude of 4.28. The star is moving closer to the Earth with a heliocentric radial velocity of −16 km/s. Eggen (1995) listed it as a proper motion candidate for membership in the IC 2391 supercluster. (en)
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  • 33 Cygni (en)
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absmag v
age myr
appmag v
class
  • A3 IV–Vn (en)
constell
epoch
  • J2000 (en)
p error
parallax
prop mo dec
  • +82.18 (en)
prop mo ra
  • +61.82 (en)
radius
rotational velocity
type
  • main sequence (en)
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