Harman Patil (Editor)

Pi Cephei

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Primary
  
Pi Cephei Aa

Primary
  
Pi Cephei A (Aa + Ab)

Magnitude
  
4.419

Apparent magnitude (V)
  
4.419

Companion
  
Pi Cephei Ab

Companion
  
Pi Cephei B

Constellation
  
Cepheus

Eccentricity
  
0.58

People also search for
  
Omicron Cephei, Nu Cephei

Pi Cephei (π Cephei) is a trinary star located in the constellation Cepheus. With an apparent magnitude of about 4.4, the system is faintly visible to the naked eye. The inner pair of stars orbits in 1.5 years while the outer companion completes one orbit in about 160 years.

Stellar system

Pi Cephei was found to have a visual companion star by Otto Wilhelm von Struve in 1843. That the primary is itself a spectroscopic binary was first noticed by William Wallace Campbell in 1901 using photographic plates taken at Lick Observatory.

References

Pi Cephei Wikipedia