About: Chi Pegasi     Goto   Sponge   NotDistinct   Permalink

An Entity of Type : yago:WikicatFlamsteedObjects, within Data Space : dbpedia.demo.openlinksw.com associated with source document(s)
QRcode icon
http://dbpedia.demo.openlinksw.com/c/7zzugETVPV

Chi Pegasi, Latinised from χ Pegasi, is a single star in the northern constellation of Pegasus, along the eastern constellation border with Pisces. It has a reddish hue and is faintly visible to the naked eye with an apparent visual magnitude of 4.80. The distance to this star is approximately 368 light-years based on parallax, but it is drifting closer with a radial velocity of −46 km/s. Chi Pegasi is a suspected small-amplitude variable. Koen and Eyer examined the Hipparcos data for Chi Pegasi, and found that its brightness varied by 0.0094 magnitudes, with a period of 5.9641 days.

AttributesValues
rdf:type
rdfs:label
  • Chi Pegasi (en)
  • Chi Pegasi (pt)
  • Chi Pegasi (sv)
  • 壁宿增十九 (zh)
rdfs:comment
  • Chi Pegasi (χ Pegasi, förkortat Chi Peg, χ Peg) som är stjärnans Bayerbeteckning, är en ensam stjärna belägen i den östra delen av stjärnbilden Pegasus. Den har en skenbar magnitud på 4,80 och är synlig för blotta ögat där ljusföroreningar ej förekommer. Baserat på parallaxmätning inom Hipparcosuppdraget på ca 8,9 mas, beräknas den befinna sig på ett avstånd på ca 368 ljusår (ca 113 parsek) från solen. (sv)
  • Chi Pegasi (89 Pegasi) é uma estrela na direção da constelação de Pegasus. Possui uma ascensão reta de 00h 14m 36.11s e uma declinação de +20° 12′ 24.1″. Sua magnitude aparente é igual a 4.80. Considerando sua distância de 326 anos-luz em relação à Terra, sua magnitude absoluta é igual a −0.21. Pertence à classe espectral M2III. (pt)
  • 飛馬座χ,又名BD+19 27,HD 1013、SAO 91792、HR 45,是飛馬座的一颗恒星,视星等为4.8,位于銀經111.3,銀緯-41.83,其B1900.0坐标为赤經0h 9m 25.6s,赤緯+19° -41.83′ 2″。 (zh)
  • Chi Pegasi, Latinised from χ Pegasi, is a single star in the northern constellation of Pegasus, along the eastern constellation border with Pisces. It has a reddish hue and is faintly visible to the naked eye with an apparent visual magnitude of 4.80. The distance to this star is approximately 368 light-years based on parallax, but it is drifting closer with a radial velocity of −46 km/s. Chi Pegasi is a suspected small-amplitude variable. Koen and Eyer examined the Hipparcos data for Chi Pegasi, and found that its brightness varied by 0.0094 magnitudes, with a period of 5.9641 days. (en)
foaf:depiction
  • http://commons.wikimedia.org/wiki/Special:FilePath/ChiPegLightCurve.png
  • http://commons.wikimedia.org/wiki/Special:FilePath/Red_circle.svg
  • http://commons.wikimedia.org/wiki/Special:FilePath/Pegasus_constellation_map.svg
dct: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
Faceted Search & Find service v1.17_git147 as of Sep 06 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 08.03.3331 as of Sep 2 2024, on Linux (x86_64-generic-linux-glibc212), Single-Server Edition (378 GB total memory, 55 GB memory in use)
Data on this page belongs to its respective rights holders.
Virtuoso Faceted Browser Copyright © 2009-2024 OpenLink Software