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Phi Piscium information


Phi Piscium
Location of φ Piscium(circled)
Observation data
Epoch J2000.0      Equinox J2000.0
Constellation Pisces
Right ascension 01h 13m 44.94617s[1]
Declination +24° 35′ 01.3249″[1]
Apparent magnitude (V) 4.676 (A)/9.11 (B)
Characteristics
φ Psc A
Spectral type K0III[2]
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[1] mas/yr
Dec.: −21.415[1] mas/yr
Parallax (π)8.1541 ± 0.2028 mas[1]
Distance400 ± 10 ly
(123 ± 3 pc)
Absolute magnitude (MV)−0.67[3]
Orbit[4]
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
[1] R
Luminosity249.6±7.1[1] L
Surface gravity (log g)2.75[2] cgs
Temperature4,720+142
−65
[1] K
Metallicity [Fe/H]−0.08[3] 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[5]
Database references
SIMBADdata

Phi Piscium, Latinized from φ Piscium, is a quadruple star[6] 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.[5] 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.[7] The star system has a period of about 20½ years and has a notably high eccentricity of 0.815.[4]

  1. ^ a b c d e f g h Cite error: The named reference GaiaDR2 was invoked but never defined (see the help page).
  2. ^ a b Cite error: The named reference McWilliam1990 was invoked but never defined (see the help page).
  3. ^ a b Cite error: The named reference Ryon2009 was invoked but never defined (see the help page).
  4. ^ a b Cite error: The named reference b was invoked but never defined (see the help page).
  5. ^ a b Cite error: The named reference a was invoked but never defined (see the help page).
  6. ^ Cite error: The named reference Eggleton_Tokovinin_2008 was invoked but never defined (see the help page).
  7. ^ R.F. Griffin; G.H. Herbig (1991). "Spectroscopic binary orbits from photoelectric radial velocities. Paper 100: Phi PISCIUM B". The Observatory. 111: 201–219. Bibcode:1991Obs...111..201G.

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