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72 Cygni is a star in the northern constellation of Cygnus, located 299 light years from the Sun and a member of the Hercules stream. It is visible to the naked eye as a faint, orange-hued star with an apparent visual magnitude of 4.87. 72 Cyg is moving closer to the Earth with a heliocentric radial velocity of −68 km/s. It has a relatively high proper motion, traversing the celestial sphere at the rate of 0.154″ per year.

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  • 72 Cygni (en)
  • 72 Cygni (sv)
  • 車府增八 (zh)
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  • 72 Cygni, som är stjärnans Flamsteed-beteckning, är en ensam stjärna belägen i den mellersta delen av stjärnbilden Svanen. Den har skenbar magnitud på ca 4,87 och är svagt synlig för blotta ögat där ljusföroreningar ej förekommer. Baserat på parallax enligt Gaia Data Release 2 på ca 14,2 mas, beräknas den befinna sig på ett avstånd på ca 229 ljusår (ca 70 parsek) från solen. Den rör sig närmare solen med en heliocentrisk radialhastighet av ca –68 km/s. Stjärnan har en relativt stor egenrörelse och förflyttar sig över himlavalvet med en hastighet av 0,154 bågsekunder per år. Den antas ingå i Herculesströmmen. (sv)
  • 天鵝座72(车府增八),又名BD+37 4359,HD 205512、SAO 71480、HR 8255,是天鵝座的一颗恒星,视星等为4.9,位于銀經86.01,銀緯-9.85,其B1900.0坐标为赤經21h 30m 41.4s,赤緯+38° -9.85′ 8″。 (zh)
  • 72 Cygni is a star in the northern constellation of Cygnus, located 299 light years from the Sun and a member of the Hercules stream. It is visible to the naked eye as a faint, orange-hued star with an apparent visual magnitude of 4.87. 72 Cyg is moving closer to the Earth with a heliocentric radial velocity of −68 km/s. It has a relatively high proper motion, traversing the celestial sphere at the rate of 0.154″ per year. (en)
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  • 72 Cygni (en)
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absmag v
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  • or (en)
  • + M5 (en)
  • K0.5 III CN 0.5 (en)
  • K0.5 III Fe0.5 (en)
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  • J2000 (en)
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