Zeta Phoenicis
From Infogalactic: the planetary knowledge core
Observation data Epoch J2000 Equinox J2000 |
|
---|---|
Constellation | Phoenix |
Right ascension | 01h 08m 23.08s[1] |
Declination | –55° 14′ 44.7″[1] |
Apparent magnitude (V) | 3.9 to 4.4 |
Characteristics | |
Spectral type | B6 V + B9 V |
B−V color index | –0.12 |
Variable type | Algol |
Astrometry | |
Radial velocity (Rv) | +15.4 km/s |
Proper motion (μ) | RA: 20.87 ± 0.36[1] mas/yr Dec.: 30.64 ± 0.38[1] mas/yr |
Parallax (π) | 10.92 ± 0.39[1] mas |
Distance | 300 ± 10 ly (92 ± 3 pc) |
Absolute magnitude (MV) | -0.37/0.90[2] |
Details | |
Mass | 3.92/2.55[2] M☉ |
Radius | 2.85/1.85[2] R☉ |
Luminosity | 316/65[2] L☉ |
Surface gravity (log g) | 4.12/4.31[2] cgs |
Temperature | 14,400/12,000[2] K |
Other designations | |
Zeta Phoenicis (ζ Phe, ζ Phoenicis) is a 280 light-year distant star in the constellation Phoenix. It is an Algol-type eclipsing binary star and its apparent magnitude fluctuates between 3.9 and 4.4 with a period of 1.66977 days. Zeta Phoenicis is most likely a four-star system: it has two other telescopic components with an apparent magnitude of 7.2 and 8.2 at an angular separation of 0.8 and 6.4 arcseconds from the main pair.[3]
References
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- Der Brockhaus. Astronomie. 2006, p. 334.