Beta Phoenicis

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Double star
β Phoenicis
AladinLite
Observation
dates equinoxJ2000.0 , epoch : J2000.0
Constellation Phoenix
Right ascension 01 h 06 m 5.04 s
declination -46 ° 43 ′ 6.3 ″
Apparent brightness 3.30 (3.22 to 3.32) mag
Typing
B − V color index (+0.89) 
U − B color index (+0.56) 
R − I index (+0.51) 
Spectral class G8 III / G8 III
Astrometry
Radial velocity (−1.10 ± 0.74) km / s
parallax (0.12 ± 14.62)  mas
distance (200)  ly  
Proper movement 
Rec. Share: (−80.81 ± 13.24)  mas / a
Dec. portion: (34.97 ± 9.51)  mas / a
Physical Properties
Dimensions (2.5 / 2.5)  M
Effective temperature (4950/4950)  K.
Other names
and catalog entries
Bayer name β Phoenicis
Cordoba Survey CD −47 ° 324
Bright Star Catalog HR 322 [1]
Henry Draper Catalog HD 6595 [2]
Hipparcos catalog HIP 5165 [3]
SAO catalog SAO 215365 [4]
2MASS catalog 2MASS J01060508-4643062 [5]

β Phoenicis is a double star in the constellation Phoenix . Both stars in the system are yellow giants of the spectral class G8 III and have almost the same level of development and the same properties. The two stars orbit each other on a very elliptical orbit with a period of 168 years. What is special about the system is that, despite the great brightness, it has not yet been possible to determine the distance using the parallax method . The data from the Hipparcos satellite result in an extremely large error range for parallax. Due to the spectral class of the two stars, a very rough determination of the distance to about 200 light years is possible.

Individual evidence

  1. a b c d e f g h bet Phe. In: SIMBAD . Center de Données astronomiques de Strasbourg , accessed on August 1, 2019 .
  2. a b NSV 400. In: VSX. AAVSO , accessed August 1, 2019 .
  3. a b c d Beta Phoenicis. Jim Kaler, accessed August 1, 2019 .