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47 Cygni is a triple star system in the northern constellation of Cygnus, and is located around 4,000 light years from the Earth. It is visible to the naked eye with a combined apparent visual magnitude of 4.61. The system is moving closer to the Earth with a heliocentric radial velocity of −4.6 km/s. The supergiant primary is a slow irregular variable with an amplitude of about 0.1 magnitudes. Its close companion has 57% of the mass of the Sun. The secondary is a hot B-type main-sequence star, but still 2.5 magnitudes fainter than the primary.

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  • 47 Cygni (en)
  • 47 Cygni (sv)
  • 天津增十三 (zh)
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  • 47 Cygni, som är stjärnans Flamsteed-beteckning, är en trippelstjärna belägen i den södra delen av stjärnbilden Svanen, som också har variabelbeteckningen V2125 Cygni. Den har en kombinerad skenbar magnitud på ca 4,61 och är svagt synlig för blotta ögat där ljusföroreningar ej förekommer. Baserat på parallax enligt Gaia Data Release 2 på ca 0,76 mas, beräknas den befinna sig på ett avstånd på ca 4 000 ljusår (ca 1 300 parsek) från solen. Den rör sig närmare solen med en heliocentrisk radialhastighet av ca -4,6 km/s. (sv)
  • 天鵝座47,又名BD+34 4079,HD 196093、SAO 70203、HR 7866,是天鵝座的一颗恒星,视星等为4.61,位于銀經75.43,銀緯-2.93,其B1900.0坐标为赤經20h 30m 0.7s,赤緯+34° -2.93′ 30″。 (zh)
  • 47 Cygni is a triple star system in the northern constellation of Cygnus, and is located around 4,000 light years from the Earth. It is visible to the naked eye with a combined apparent visual magnitude of 4.61. The system is moving closer to the Earth with a heliocentric radial velocity of −4.6 km/s. The supergiant primary is a slow irregular variable with an amplitude of about 0.1 magnitudes. Its close companion has 57% of the mass of the Sun. The secondary is a hot B-type main-sequence star, but still 2.5 magnitudes fainter than the primary. (en)
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  • 47 Cygni (en)
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  • http://commons.wikimedia.org/wiki/Special:FilePath/V2125CygLightCurve.png
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  • (en)
  • −4.1 (en)
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