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Mu Phoenicis
Location of μ Phoenicis (circled)
Observation data
Epoch J2000       Equinox J2000
Constellation Phoenix
Right ascension 00h 41m 19.55229s [1]
Declination −46° 05′ 06.0184″ [1]
Apparent magnitude (V) 4.59 [2]
Characteristics
Spectral type G8III [3]
U−B color index +0.72 [2]
B−V color index +0.97 [2]
Astrometry
Radial velocity (Rv)+17.41±0.16 [4] km/s
Proper motion (μ) RA: −28.20 [1]  mas/ yr
Dec.: +1.80 [1]  mas/ yr
Parallax (π)13.27 ± 0.23  mas [1]
Distance246 ± 4  ly
(75 ± 1  pc)
Absolute magnitude (MV)0.21 [5]
Details
Mass2.50 [6]  M
Radius13.15+2.59
−2.28
[4]  R
Luminosity96.6±2.4 [4]  L
Temperature4,900 [7]  K
Rotational velocity (v sin i)1.4 [8] km/s
Age1.4 [6]  Gyr
Other designations
μ Phe, CD−46°180, FK5 1015, GC 823, HD 3919, HIP 3245, HR 180, SAO 215194 [9]
Database references
SIMBAD data

μ Phoenicis, Latinized as Mu Phoenicis, is a suspected astrometric binary [10] star system in the southern constellation of Phoenix. It is visible to the naked eye as a faint, yellow-hued star with an apparent visual magnitude of 4.59. [2] This system is located approximately 246  light years distant from the Sun based on parallax, [1] and is drifting further away with a radial velocity of +17.4 km/s. [4]

The visible component is an aging G-type giant star with a stellar classification of G8III. [3] Having exhausted the supply of hydrogen at its core, this star cooled and expanded off the main sequence. At present it has 13 [4] times the girth of the Sun. It is 1.4 [6] billion years old with 2.5 [6] times the mass of the Sun. It is radiating 97 [4] times the luminosity of the Sun from its swollen photosphere at an effective temperature of 4,900 K. [7]

References

  1. ^ a b c d e f 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. Vizier catalog entry
  2. ^ a b c d Ducati, J. R. (2002). "VizieR Online Data Catalog: Catalogue of Stellar Photometry in Johnson's 11-color system". CDS/ADC Collection of Electronic Catalogues. 2237. Bibcode: 2002yCat.2237....0D.
  3. ^ a b Houk, Nancy (1978). Michigan catalogue of two-dimensional spectral types for the HD stars. Vol. 2. Ann Arbor: Dept. of Astronomy, University of Michigan. Bibcode: 1978mcts.book.....H.
  4. ^ a b c d e f 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.
  5. ^ Anderson, E.; Francis, Ch. (2012). "XHIP: An extended hipparcos compilation". Astronomy Letters. 38 (5): 331. arXiv: 1108.4971. Bibcode: 2012AstL...38..331A. doi: 10.1134/S1063773712050015. S2CID  119257644. Vizier catalog entry
  6. ^ a b c d Luck, R. Earle (2015). "Abundances in the Local Region. I. G and K Giants". The Astronomical Journal. 150 (3): 88. arXiv: 1507.01466. Bibcode: 2015AJ....150...88L. doi: 10.1088/0004-6256/150/3/88. S2CID  118505114.
  7. ^ a b Gontcharov, G. A. (2009). "Red giant clump in the Tycho-2 catalogue". Astronomy Letters. 34 (11): 785–796. arXiv: 1607.00619. Bibcode: 2008AstL...34..785G. doi: 10.1134/S1063773708110078. S2CID  73524157. Vizier catalog entry
  8. ^ De Medeiros, J. R.; Alves, S.; Udry, S.; Andersen, J.; Nordström, B.; Mayor, M. (2014). "A catalog of rotational and radial velocities for evolved stars". Astronomy & Astrophysics. 561: A126. arXiv: 1312.3474. Bibcode: 2014A&A...561A.126D. doi: 10.1051/0004-6361/201220762. S2CID  54046583. Vizier catalog entry
  9. ^ "mu Phe". SIMBAD. Centre de données astronomiques de Strasbourg.
  10. ^ 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.