Phi Piscium

Phi Piscium, Latinized from φ Piscium, is a quadruple star system approximately 380 light years away in the constellation Pisces. It consists of Phi Piscium A, with a spectral type of K0III, and Phi Piscium B. Phi Piscium A possesses a surface temperature of 3,500 to 5,000 kelvins. Some suggest the only visible companion in the Phi Piscium B sub-system is a late F dwarf star, while others suggest it is a K0 star. The invisible component of the Phi Piscium B sub-system is proposed to have a spectral type of M2V. The star system has a period of about 20½ years and has a notably high eccentricity of 0.815.

Phi Piscium
Location of φ Piscium(circled)
Observation data
Epoch J2000.0      Equinox J2000.0
Constellation Pisces
Right ascension 01h 13m 44.94617s
Declination +24° 35 01.3249
Apparent magnitude (V) 4.676 (A)/9.11 (B)
Characteristics
φ Psc A
Spectral type K0III
U−B color index +0.
B−V color index +1.03
φ Psc B
Spectral type K0
U−B color index +0.25
B−V color index +0.92
Astrometry
Radial velocity (Rv)5.9 km/s
Proper motion (μ) RA: 16.901 mas/yr
Dec.: −21.415 mas/yr
Parallax (π)8.1541 ± 0.2028 mas
Distance400 ± 10 ly
(123 ± 3 pc)
Absolute magnitude (MV)−0.67
Orbit
Companionφ Psc B
Period (P)7473±3 d yr
Eccentricity (e)0.815±0.005
Argument of periastron (ω)
(secondary)
71.9±1.7°
Details
A
Radius23.63+0.66
−1.36
 R
Luminosity249.6±7.1 L
Surface gravity (log g)2.75 cgs
Temperature4,720+142
−65
 K
Metallicity [Fe/H]−0.08 dex
Other designations
Phi Psc, φ Psc, 85 Piscium, BD+23° 158, FK5 2082, GC 1474, HD 7318, HIP 5742, HR 360, SAO 74571, PPM 90580, CCDM J01137+2435A, WDS J01137+2435A
Database references
SIMBADdata
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