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ο Pegasi, Latinized as Omicron Pegasi, is a suspected astrometric binary star system in the northern constellation of Pegasus. It is white in hue and visible to the naked eye as a faint point of light with an apparent visual magnitude of +4.80. The distance to this system is approximately 290 light years based on parallax, and it is drifting further away from the Sun with a radial velocity of +8.5 km/s.

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rdf:type
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  • Ómicron Pegasi (es)
  • Omicron Pegasi (in)
  • Omicron Pegasi (en)
  • Omicron Pegasi (pt)
  • Omikron Pegasi (sv)
  • HD214994 (uk)
  • 離宮三 (zh)
rdfs:comment
  • Omicron Pegasi (ο Peg) adalah salah satu bintang di rasi Pegasus. Omicron Pegasi termasuk bintang kelas A1IV dan bermagnitudo +4.8. Bintang ini berada pada jarak 305 tahun cahaya dari Earth. (in)
  • Omikron Pegasi (ο Pegasi, förkortat Omikron Peg, ο Peg) som är stjärnans Bayerbeteckning, är en ensam stjärna belägen i den norra delen av stjärnbilden Pegasus. Den har en skenbar magnitud på 4,79 och är synlig för blotta ögat där ljusföroreningar ej förekommer. Baserat på parallaxmätning inom Hipparcosuppdraget på ca 10,9 mas, beräknas den befinna sig på ett avstånd på ca 300 ljusår (ca 92 parsek) från solen. (sv)
  • Omicron Pegasi (43 Pegasi) é uma estrela na direção da constelação de Pegasus. Possui uma ascensão reta de 22h 41m 45.41s e uma declinação de +29° 18′ 27.7″. Sua magnitude aparente é igual a 4.82. Considerando sua distância de 305 anos-luz em relação à Terra, sua magnitude absoluta é igual a −0.05. Pertence à classe espectral A1IV. (pt)
  • HD214994 — хімічно пекулярна зоря спектрального класу A0, що має видиму зоряну величину в смузі V приблизно 4,8.Вона розташована на відстані близько 304,8 світлових років від Сонця. (uk)
  • 离宫三(飛馬座ο),又名BD+28 4436,HD 214994、SAO 90717、HR 8641,是飛馬座的一颗恒星,视星等为4.79,位于銀經91.71,銀緯-25.59,其B1900.0坐标为赤經22h 37m 3.6s,赤緯+28° -25.59′ 8″。 (zh)
  • Ómicron Pegasi (ο Peg / 43 Pegasi)​​ es una estrella en la constelación de Pegaso.Tiene magnitud aparente +4,80 y está situada a 299 años luz del Sistema Solar. Ómicron Pegasi es una subgigante blanca de tipo espectral A1IV.Tiene una temperatura efectiva entre 9453 y 9506 K y es 106 veces más luminosa que el Sol.​​Diversos estudios indican un valor de su radio entre 1,8 y 2,5 radios solares​​ y gira sobre sí misma con una velocidad de rotación de 14 km/s, si bien éste es un valor mínimo.Tiene una masa de 2,8 masas solares y, en cuanto a su estado evolutivo, está abandonando la secuencia principal.​ (es)
  • ο Pegasi, Latinized as Omicron Pegasi, is a suspected astrometric binary star system in the northern constellation of Pegasus. It is white in hue and visible to the naked eye as a faint point of light with an apparent visual magnitude of +4.80. The distance to this system is approximately 290 light years based on parallax, and it is drifting further away from the Sun with a radial velocity of +8.5 km/s. (en)
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