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55 Cygni (55 Cyg) is a blue supergiant star in the constellation Cygnus. It is thought to be a member of the Cygnus OB7 stellar association at about 2,700 light years. Its apparent magnitude is 4.86, but this is slightly variable and the star is also called V1661 Cyg. When first analysed, it was classified as an irregular supergiant variable, but subsequent studies have treated it as an Alpha Cygni variable. It shows pulsations with multiple periods from a few hours to 22 days, and both p- and g-modes. Apart from p- and g-modes, strange mode and associated instabilities have also been found in models of this star. The spectrum also shows variation, leading to different classifications being given for the star.

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  • 55 del Cigne (ca)
  • 55 Cygni (en)
  • 55 Cygni (sv)
  • 天津增卅三 (zh)
rdfs:comment
  • 55 Cygni, som är stjärnans Flamsteed-beteckning, är en ensam stjärna belägen i den mellersta delen av stjärnbilden Svanen, som också har variabelbeteckningen V1661 Cygni. Den har en genomsnittlig skenbar magnitud på ca 4,86 och är svagt synlig för blotta ögat där ljusföroreningar ej förekommer. Baserat på parallaxmätning inom Hipparcosuppdraget på ca 1,4 mas, beräknas den befinna sig på ett avstånd av ca 830 parsek från solen. Den rör sig närmare solen med en heliocentrisk radialhastighet av ca -7 km/s. Stjärnan antas ingå i stjärnförening Cygnus OB7 vid ett avstånd av ungefär 2 700 ljusår från solen. (sv)
  • 天鵝座55,又名BD+45 3291,HD 198478、SAO 50099、HR 7977,是天鵝座的一颗恒星,视星等为4.84,位于銀經85.75,銀緯1.49,其B1900.0坐标为赤經20h 45m 31.8s,赤緯+45° 1.49′ 35″。 (zh)
  • 55 del Cigne (55 Cygni) és una estrella supergegant blava a la constel·lació del Cigne. Hom creu que és membre de l'associació estel·lar Cygnus OB7 al voltant d'aproximadament 2.700 anys llum. La seva magnitud aparent és de 4,86, però és lleugerament variable i l'estrella també s'anomena V1661 Cyg. Quan es va analitzar per primera vegada, es va classificar com una variable supergegant irregular, però estudis posteriors l'han tractat com una variable Alfa Cygni. Mostra pulsacions amb períodes múltiples d'unes poques hores a 22 dies, i amb modes p i g. A part dels modes p i g, també s'han trobat modes estranys i inestabilitats associades en els models d'aquesta estrella. L'espectre també mostra variacions, donant lloc a diferents classificacions per a l'estrella. (ca)
  • 55 Cygni (55 Cyg) is a blue supergiant star in the constellation Cygnus. It is thought to be a member of the Cygnus OB7 stellar association at about 2,700 light years. Its apparent magnitude is 4.86, but this is slightly variable and the star is also called V1661 Cyg. When first analysed, it was classified as an irregular supergiant variable, but subsequent studies have treated it as an Alpha Cygni variable. It shows pulsations with multiple periods from a few hours to 22 days, and both p- and g-modes. Apart from p- and g-modes, strange mode and associated instabilities have also been found in models of this star. The spectrum also shows variation, leading to different classifications being given for the star. (en)
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  • 55 Cygni (en)
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  • http://commons.wikimedia.org/wiki/Special:FilePath/V1661CygLightCurve.png
  • http://commons.wikimedia.org/wiki/Special:FilePath/Red_circle.svg
  • http://commons.wikimedia.org/wiki/Special:FilePath/Cygnus_constellation_map.svg
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absmag v
  • −6.93 - −7.26 (en)
appmag v
b-v
  • +0.42 (en)
class
  • B2.5Ia - B4Ia (en)
constell
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