Xi Phoenicis

Xi Phoenicis

A light curve for Xi Phoenicis plotted from TESS data
Observation data
Epoch J2000.0      Equinox J2000.0 (ICRS)
Constellation Phoenix
Right ascension 00h 41m 46.30191s
Declination −56° 30 05.2370
Apparent magnitude (V) 5.70 + 9.98
Characteristics
Spectral type A3 Vp(SrCr v. st; K sn)
B−V color index +0.19
Variable type α2 CVn
Astrometry
ξ Phe A
Radial velocity (Rv)+9.8±2.9 km/s
Proper motion (μ) RA: +90.35 mas/yr
Dec.: +56.79 mas/yr
Parallax (π)14.6127±0.0903 mas
Distance223 ± 1 ly
(68.4 ± 0.4 pc)
Absolute bolometric
magnitude
 (Mbol)
1.64±0.079
ξ Phe B
Radial velocity (Rv)+9.19±0.28 km/s
Proper motion (μ) RA: +92.61 mas/yr
Dec.: +54.69 mas/yr
Parallax (π)14.7541 ± 0.0357 mas
Distance221.1 ± 0.5 ly
(67.8 ± 0.2 pc)
Details
ξ Phe A
Mass1.91±0.03 M
Radius2.04±0.26 R
Luminosity17.4+1.7
−1.6
 L
Surface gravity (log g)4.0±0.2 cgs
Temperature8,300±250 K
Rotation3.9516±0.0003 d
Rotational velocity (v sin i)22.5±2 km/s
Age680+100
−120
 Myr
ξ Phe B
Mass0.81 M
Radius0.76+0.04
−0.03
 R
Luminosity0.328±0.001 L
Temperature4,999+116
−100
 K
Other designations
ξ Phe, CD−57°137, HD 3980, HIP 3277, HR 183, SAO 232152, WDS J00418-5630A
Database references
SIMBADdata

Xi Phoenicis, Latinized from ξ Phoenicis, is a visual binary star system in the southern constellation of Phoenix. It is faintly visible to the naked eye, having an apparent visual magnitude of 5.70. Based upon an annual parallax shift of 14.61 mas as measured from Earth, it is located around 223 light years from the Sun. The system is moving away from the Sun with a radial velocity of about +10 km/s.