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BC Cygni (BC Cyg, HIP 100404, BD + 37 3903) is a red supergiant and pulsating variable star of spectral type M3.5Ia in the constellation Cygnus. It is considered a member of the stellar Cygnus OB1 association, and within it the open cluster Berkeley 87.2 which would place at a distance of 1,500 parsecs (4,890 light-years) of the Solar System; however, according to the measure of the parallax by the satellite Hipparcos (1.20 milliarcseconds). It is less than a degree north of another variable red supergiant, BI Cygni.

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rdf:type
rdfs:label
  • BC Cygni (es)
  • BC Cygni (en)
  • BC Cygni (it)
  • BC Cygni (fr)
  • BC Лебедя (ru)
rdfs:comment
  • BC Cygni (BC Cyg, HIP 100404, BD + 37 3903) is a red supergiant and pulsating variable star of spectral type M3.5Ia in the constellation Cygnus. It is considered a member of the stellar Cygnus OB1 association, and within it the open cluster Berkeley 87.2 which would place at a distance of 1,500 parsecs (4,890 light-years) of the Solar System; however, according to the measure of the parallax by the satellite Hipparcos (1.20 milliarcseconds). It is less than a degree north of another variable red supergiant, BI Cygni. (en)
  • BC Cygni (BC Cyg / HIP 100404 / BD+37 3903)​ es una estrella variable en la constelación del Cisne de magnitud aparente media +9,97.Se la ha considerado miembro de la Asociación estelar , y dentro de ésta del cúmulo abierto ,​ lo que la situaría a una distancia de 1500 pársecs (4890 años luz) del Sistema Solar;sin embargo, de acuerdo a la medida de la paralaje realizada por el satélite Hipparcos (1,20 milisegundos de arco),​ BC Cygni se halla a poco más de 2700 años luz. (es)
  • BC Cygni (BC Cyg / HIP 100404 / BD +37 3903) est une étoile variable de la constellation du Cygne de magnitude apparente 9,97. Elle est considérée comme un membre de l'association stellaire Cygnus OB1, et en son sein de l'amas ouvert Berkeley 87, ce qui la placerait à une distance d'environ 1 500 pc (∼4 890 a.l.) du système solaire ; cependant, selon la mesure de la parallaxe par le satellite Hipparcos (1,20 milliarcsecondes), BC Cygni est à un peu plus de ∼2 700 a.l. (∼828 pc). Gaia DR2 fournit une parallaxe de 0,75 ± 0,10 mas, ce qui correspond à une distance d'environ 1 330 pc (∼4 340 a.l.). (fr)
  • BC Cygni è una stella supergigante rossa di tipo spettrale M3Iab situata nella costellazione del Cigno. È una delle stelle più grandi conosciute: con un diametro di oltre 1100 volte più grande di quello solare, essa supera ampiamente in raggio supergiganti come Betelgeuse e Antares e, se fosse al posto del Sole, si estenderebbe fin oltre l'orbita di Giove, a 5,7 U.A. dal suo centro. La misura della parallasse effettuata dal satellite Hipparcos la pone ad una distanza dal sistema solare di circa 2700 anni luce. (it)
  • BC Лебедя (BC Cyg, HIP 100404, BD + 37 3903) — переменная звезда в созвездии Лебедя. Среднее значение видимой звёздной величины составляет +9,97m. Предположительно входит в состав звёздной ассоциации Лебедь OB1 и принадлежащего ей рассеянного скопления , находящегося на расстоянии около 1500 пк (4890 св. лет) от Солнца. BC Лебедя считается пульсирующей переменной звездой, видимая звёздная величина меняется от +9,0 до +10,8 с периодом 720 ± 40 дней. Вероятно, между 1900 г и 2000 г звезда увеличила видимую яркость на 0,5m. (ru)
foaf:name
  • BC Cygni (en)
foaf:depiction
  • http://commons.wikimedia.org/wiki/Special:FilePath/Red_circle.svg
  • http://commons.wikimedia.org/wiki/Special:FilePath/BCCygLightCurve.png
  • http://commons.wikimedia.org/wiki/Special:FilePath/Sadr_Region_rgb.jpg
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absmag v
  • –7.71 (en)
appmag v
b-v
  • +3.13 - +3.21 (en)
caption
  • BC Cygni is visible as a red star . The bright star at the centre is γ Cygni and north is to the right. (en)
class
  • (en)
  • M3.5 Ia (en)
component
  • Maximum (en)
  • Minimum (en)
constell
epoch
  • J2000 (en)
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