Gamma Pegasi

γ Pegasi
Observation data
Epoch J2000.0      Equinox J2000.0
Constellation Pegasus
Right ascension 00h 13m 14.2s
Declination +15° 11' 01"
Apparent magnitude (V) +2.83
Distance 335 ly
(103 pc)
Spectral type B2IV
Other designations
Algeneb, Algenib, 88 Peg, HR 39, HD 886, FK5 7, SAO 91781, HIP 1067

Gamma Pegasi (γ Peg) is a star in the constellation of Pegasus. It also has the traditional name Algenib; confusingly however, this name is also used for Alpha Persei.

The asterism of γ Pegasi and α Andromedae, in Hindu astronomy, is called Uttara Bhādrapadā (उत्तरभाद्रपदा) or Uttṛṭṭāti. It is the 26th nakshatra. In Chinese, 壁宿 (Bì Sù), meaning Wall (asterism) refers to an asterism consisting of γ Pegasi and α Andromedae .[1] Consequently, γ Pegasi itself is known as 壁宿一 (Bì Sù yī, English: the First Star of Wall.)[2]

Gamma Pegasi is a Beta Cephei variable star that lies at the lower left-hand corner of the Great Square of Pegasus. Its magnitude varies between +2.78 and +2.89 with a period of 3.6 hours. It is 335 light-years distant and belongs to spectral type B2. It has a total luminosity of 4000 times that of the Sun with a radius of 4.5 times solar. The mass of γ Pegasi is 7 to 10 solar masses.

References

  1. ^ (Chinese) p. 170, 中國星座神話, written by 陳久金. Published by 台灣書房出版有限公司, 2005, ISBN 978-986-7332-25-7.
  2. ^ (Chinese) 香港太空館 - 研究資源 - 亮星中英對照表, Hong Kong Space Museum. Accessed on line November 23, 2010.

External links