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72 Pegasi is a binary star system in the northern constellation of Pegasus. It is visible to the naked eye as a faint, orange-hued point of light with a combined apparent visual magnitude of 4.97. The system is located approximately 550 light years away from the Sun, based on parallax, but is drifting closer with a radial velocity of −25 km/s.

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  • 72 Pegasi (en)
  • 72 Pegasi (sv)
  • 壁宿增二 (zh)
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  • 72 Pegasi, som är stjärnans Flamsteed-beteckning, är en dubbelstjärna belägen i den norra delen av stjärnbilden Pegasus. Den har en genomsnittlig kombinerad skenbar magnitud på ca 4,97 och är svagt synlig för blotta ögat där ljusföroreningar ej förekommer. Baserat på parallaxmätning inom Hipparcosuppdraget på ca 5,9 mas, beräknas den befinna sig på ett avstånd på ca 550 ljusår (ca 170 parsek) från solen. Den rör sig närmare solen med en heliocentrisk radialhastighet av ca –25 km/s. (sv)
  • 飛馬座72,又名BD+30 4978,HD 221673、SAO 73341、HR 8943,是飛馬座的一颗恒星,视星等为4.98,位于銀經104.09,銀緯-28.69,其B1900.0坐标为赤經23h 28m 59.4s,赤緯+30° -28.69′ 24″。 (zh)
  • 72 Pegasi is a binary star system in the northern constellation of Pegasus. It is visible to the naked eye as a faint, orange-hued point of light with a combined apparent visual magnitude of 4.97. The system is located approximately 550 light years away from the Sun, based on parallax, but is drifting closer with a radial velocity of −25 km/s. (en)
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  • http://commons.wikimedia.org/wiki/Special:FilePath/Red_circle.svg
  • http://commons.wikimedia.org/wiki/Special:FilePath/Pegasus_constellation_map.svg
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absmag v
  • −1.15 (en)
appmag v
axis
b-v
  • +1.39 (en)
class
  • K4IIIb (en)
constell
eccentricity
epoch
  • J2000 (en)
gravity
inclination
luminosity
mass
metal fe
  • +0.06 (en)
node
p error
parallax
periarg
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