Phi Pegasi

φ Pegasi, Latinised as Phi Pegasi, is a solitary,[4] reddish hued star in the northern constellation of Pegasus. With an apparent visual magnitude of around 5.1,[2] it is a faint star that can be seen with the naked eye. Based upon an annual parallax shift of 7.05 mas as seen from Earth,[1] the system is located around 460 light years distant from the Sun. At that distance, the visual magnitude of the star is diminished by an extinction factor of 0.15 due to interstellar dust.[5]

Phi Pegasi
Observation data
Epoch J2000.0      Equinox J2000.0 (ICRS)
Constellation Pegasus
Right ascension  23h 52m 29.28762s[1]
Declination +19° 07′ 13.0218″[1]
Apparent magnitude (V) 5.107[2] (5.11−5.17)[3]
Characteristics
Spectral type M2.5 IIIb[4]
U−B color index +1.878[2]
B−V color index +1.599[2]
Astrometry
Radial velocity (Rv)−7.75±0.15[5] km/s
Proper motion (μ) RA: −7.27[1] mas/yr
Dec.: −35.40[1] mas/yr
Parallax (π)7.05 ± 0.27[1] mas
Distance460 ± 20 ly
(142 ± 5 pc)
Other designations
φ Peg, 81 Peg, CPD+18° 5231, FK5 898, HD 223768, HIP 117718, HR 9036, SAO 108878[6]
Database references
SIMBADdata

This is an evolved red giant star with a stellar classification of M2.5 IIIb.[4] It is a semiregular variable that ranges between magnitudes 5.11 and 5.17.[3] Hipparcos mission photometry gives an amplitude variation of 0.0148 in magnitude with a frequency of 11.4 cycles per day.[7]

In terms of its right ascension coordinates, φ Pegasi is located very near the line of the vernal equinox and will cross over around the year 3030, due to the precession of the Earth's axis.[8]

References
  1. van Leeuwen, F. (2007), "Validation of the new Hipparcos reduction", Astronomy and Astrophysics, 474 (2): 653–664, arXiv:0708.1752, Bibcode:2007A&A...474..653V, doi:10.1051/0004-6361:20078357.
  2. Gutierrez-Moreno, Adelina; et al. (1966), A System of photometric standards, 1, Publicaciones Universidad de Chile, Department de Astronomy, pp. 1–17, Bibcode:1966PDAUC...1....1G.
  3. Watson, Christopher (4 January 2010), "Phi Pegasi", AAVSO Website, American Association of Variable Star Observers, retrieved 15 February 2014.
  4. Eggleton, P. P.; Tokovinin, A. A. (September 2008), "A catalogue of multiplicity among bright stellar systems", Monthly Notices of the Royal Astronomical Society, 389 (2): 869–879, arXiv:0806.2878, Bibcode:2008MNRAS.389..869E, doi:10.1111/j.1365-2966.2008.13596.x.
  5. Famaey, B.; et al. (January 2005), "Local kinematics of K and M giants from CORAVEL/Hipparcos/Tycho-2 data. Revisiting the concept of superclusters", Astronomy and Astrophysics, 430: 165–186, arXiv:astro-ph/0409579, Bibcode:2005A&A...430..165F, doi:10.1051/0004-6361:20041272.
  6. "phi Peg". SIMBAD. Centre de données astronomiques de Strasbourg. Retrieved 2017-08-10.
  7. Koen, Chris; Eyer, Laurent (2002), "New periodic variables from the Hipparcos epoch photometry", Monthly Notices of the Royal Astronomical Society, 331: 45, arXiv:astro-ph/0112194, Bibcode:2002MNRAS.331...45K, doi:10.1046/j.1365-8711.2002.05150.x.
  8. Kaler, James B. (December 2, 2016), "PHI PEG (Phi Pegasi)", STARS, University of Illinois, retrieved 2017-08-10.
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