Psi Andromedae

Psi Andromedae
Location of ψ Andromedae (circled)
Observation data
Epoch J2000      Equinox J2000
Constellation Andromeda
Right ascension 23h 46m 02.04703s
Declination +46° 25 12.9865
Apparent magnitude (V) 4.95
Characteristics
Spectral type G5 Ib + B9
U−B color index +0.83
B−V color index +1.085
Astrometry
Radial velocity (Rv)-23.62 km/s
Proper motion (μ) RA: 8.446(132) mas/yr
Dec.: −7.143(109) mas/yr
Parallax (π)1.6352±0.1627 mas
Distance2,000 ± 200 ly
(610 ± 60 pc)
Absolute magnitude (MV)–3.039
Details
ψ And A
Mass5.4 M
Radius59+8
−10
 R
Luminosity1,049±161 L
Surface gravity (log g)1.50 cgs
Temperature4,276±182 K
Metallicity [Fe/H]+0.10 dex
Age79 Myr
B
Mass2.6 M
Temperature11,000 K
Other designations
20 And, BD+45°4321, FK5 1622, HD 223047, HIP 117221, HR 9003, SAO 53355, PPM 64635
Database references
SIMBADdata

Psi Andromedae (ψ And, ψ Andromedae) is the Bayer designation for a triple star system in the northern constellation of Andromeda. The combined apparent visual magnitude of this system is 4.95. Based upon parallax measurements, is roughly 2,000 light-years (610 parsecs) from Earth.

The primary component has a stellar classification of G5 Ib, which matches the spectrum of an evolved supergiant star. It forms a pair with a star of type B9 with an unknown luminosity class separated by 0.28 arcseconds. A third component has a separation of 0.14 arcseconds. Details of the orbital arrangement remain uncertain.