About: BI Cygni     Goto   Sponge   NotDistinct   Permalink

An Entity of Type : dbo:Star, within Data Space : dbpedia.demo.openlinksw.com associated with source document(s)
QRcode icon
http://dbpedia.demo.openlinksw.com/describe/?url=http%3A%2F%2Fdbpedia.org%2Fresource%2FBI_Cygni&invfp=IFP_OFF&sas=SAME_AS_OFF

BI Cygni (BI Cyg, IRC +40408, BD+36 4025) is a red supergiant in the constellation Cygnus. It is an irregular variable star with a maximum brightness of magnitude 8.4 and a minimum of magnitude 9.9. It is considered a member of the stellar Cygnus OB1 association, its distance is around 1,400 parsecs (4,500 light-years) of the Solar System. It is less than a degree south of another variable red supergiant, BC Cygni.

AttributesValues
rdf:type
rdfs:label
  • BI Cygni (es)
  • BI Cygni (en)
  • BI Cygni (it)
  • BI Лебедя (ru)
rdfs:comment
  • BI Cygni es una estrella supergigante roja en la constelación del Cisne. Tiene un radio de 1 240 veces el de nuestro Sol.​ Si se coloca en el centro de nuestro sistema solar, su superficie se extendería más allá de la órbita de Júpiter. Se encuentra a unos 5 153 años luz de la Tierra. (es)
  • BI Cygni è una stella supergigante rossa situata nella costellazione del Cigno. Ha un raggio che, a seconda delle fonti, va da 1000 volte quello del nostro Sole,, a 1240 R⊙ Se posta al centro del nostro sistema solare, la sua superficie si estenderebbe oltre l'orbita di Giove. Dista circa 5153 anni luce dalla Terra. (it)
  • BI Лебедя (IRC +40408 или BD+36 4025) — красный сверхгигант в созвездии Лебедя. Предположительно входит в состав звёздной ассоциации Лебедь OB1. Обладает радиусом в 916-1240 солнечных, что делает BI Лебедя одной из крупнейших известных звёзд. Масса звезды составляет 20 масс Солнца, а светимость больше солнечной в 123000-226000 раз. Эффективная температура поверхности звезды составляет 3575 K. Классифицируется как медленная неправильная переменная звезда. (ru)
  • BI Cygni (BI Cyg, IRC +40408, BD+36 4025) is a red supergiant in the constellation Cygnus. It is an irregular variable star with a maximum brightness of magnitude 8.4 and a minimum of magnitude 9.9. It is considered a member of the stellar Cygnus OB1 association, its distance is around 1,400 parsecs (4,500 light-years) of the Solar System. It is less than a degree south of another variable red supergiant, BC Cygni. (en)
foaf:name
  • BI Cygni (en)
foaf:depiction
  • http://commons.wikimedia.org/wiki/Special:FilePath/Red_circle.svg
  • http://commons.wikimedia.org/wiki/Special:FilePath/BICygLightCurve.png
  • http://commons.wikimedia.org/wiki/Special:FilePath/Sadr_Region_rgb.jpg
dcterms:subject
Wikipage page ID
Wikipage revision ID
Link from a Wikipage to another Wikipage
Link from a Wikipage to an external page
sameAs
dbp:wikiPageUsesTemplate
thumbnail
absmag v
  • –6.78 (en)
appmag v
caption
  • BI Cygni is the small very red dot right on the left edge of this image. The bright star at the centre is γ Cygni and north is to the right. (en)
class
  • M4 Iab (en)
component
constell
epoch
  • J2000 (en)
gravity
luminosity
mass
metal fe
  • +0.40 (en)
no heading
  • y (en)
Faceted Search & Find service v1.17_git139 as of Feb 29 2024


Alternative Linked Data Documents: ODE     Content Formats:   [cxml] [csv]     RDF   [text] [turtle] [ld+json] [rdf+json] [rdf+xml]     ODATA   [atom+xml] [odata+json]     Microdata   [microdata+json] [html]    About   
This material is Open Knowledge   W3C Semantic Web Technology [RDF Data] Valid XHTML + RDFa
OpenLink Virtuoso version 08.03.3330 as of Mar 19 2024, on Linux (x86_64-generic-linux-glibc212), Single-Server Edition (378 GB total memory, 67 GB memory in use)
Data on this page belongs to its respective rights holders.
Virtuoso Faceted Browser Copyright © 2009-2024 OpenLink Software