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Phi Gruis

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Star in the constellation Grus
Phi Gruis
Observation data
Epoch J2000.0      Equinox J2000.0 (ICRS)
Constellation Grus
Right ascension 23 18 09.88466
Declination −40° 49′ 27.7034″
Apparent magnitude (V) 5.49
Characteristics
Evolutionary stage main sequence
Spectral type F4 V
U−B color index −0.05
B−V color index +0.47
Astrometry
Radial velocity (Rv)+15.15±0.29 km/s
Proper motion (μ) RA: +126.920 mas/yr
Dec.: −122.577 mas/yr
Parallax (π)29.3153 ± 0.1115 mas
Distance111.3 ± 0.4 ly
(34.1 ± 0.1 pc)
Absolute magnitude (MV)2.82
Details
Mass1.45+0.02
−0.01 M
Radius1.87+0.07
−0.04 R
Luminosity5.84±0.03 L
Surface gravity (log g)4.06±0.02 cgs
Temperature6,606±63 K
Metallicity 0.00±0.05 dex
Rotational velocity (v sin i)19.9±1.0 km/s
Age2.12+0.22
−0.16 Gyr
Other designations
φ Gru, CD−41°15211, GJ 4330, HD 219693, HIP 115054, HR 8859, SAO 231539
Database references
SIMBADdata

Phi Gruis, Latinised from φ Gruis, is a solitary, yellow-white hued star in the southern constellation of Grus, near the eastern constellation border with Phoenix. It is faintly visible to the naked eye with an apparent visual magnitude of +5.49. Based upon an annual parallax shift of 29.3 mas as seen from the Earth, it lies at a distance of 111 light years from the Sun. The star is drifting further away with a radial velocity of +15 km/s.

This object is an F-type main-sequence star with a stellar classification of F4 V, where the luminosity class of 'V' indicates it is currently generating energy through hydrogen fusion at its core. It is 2.12 billion years old and is spinning with a projected rotational velocity of 20 km/s. The star has 1.45 times the mass of the Sun and 1.87 times the Sun's radius. It is radiating 5.8 times as much luminosity as the Sun from its photosphere at an effective temperature of 6,606 km/s.

References

  1. ^ Brown, A. G. A.; et al. (Gaia collaboration) (August 2018). "Gaia Data Release 2: Summary of the contents and survey properties". Astronomy & Astrophysics. 616. A1. arXiv:1804.09365. Bibcode:2018A&A...616A...1G. doi:10.1051/0004-6361/201833051. Gaia DR2 record for this source at VizieR.
  2. ^ Przybylski, A.; Kennedy, P. M. (1965), "Radial velocities and three-colour photometry of 166 southern stars", Monthly Notices of the Royal Astronomical Society, 131: 95–104, Bibcode:1965MNRAS.131...95P, doi:10.1093/mnras/131.1.95.
  3. ^ Gray, R. O.; et al. (July 2006), "Contributions to the Nearby Stars (NStars) Project: spectroscopy of stars earlier than M0 within 40 pc-The Southern Sample", The Astronomical Journal, 132 (1): 161–170, arXiv:astro-ph/0603770, Bibcode:2006AJ....132..161G, doi:10.1086/504637, S2CID 119476992.
  4. ^ Ammler-von Eiff, Matthias; Reiners, Ansgar (June 2012), "New measurements of rotation and differential rotation in A-F stars: are there two populations of differentially rotating stars?", Astronomy & Astrophysics, 542: A116, arXiv:1204.2459, Bibcode:2012A&A...542A.116A, doi:10.1051/0004-6361/201118724, S2CID 53666672.
  5. ^ Aguilera-Gómez, Claudia; Ramírez, Iván; Chanamé, Julio (June 2018), "Lithium abundance patterns of late-F stars: an in-depth analysis of the lithium desert", Astronomy & Astrophysics, 614: 15, arXiv:1803.05922, Bibcode:2018A&A...614A..55A, doi:10.1051/0004-6361/201732209, S2CID 62799777, A55.
  6. "phi Gru -- Star", SIMBAD Astronomical Database, Centre de Données astronomiques de Strasbourg, retrieved 2017-06-19.
  7. 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, S2CID 14878976.
  8. 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, S2CID 18759600.
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