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Mu1 Gruis

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Star in the constellation Grus For other stars with this Bayer designation, see μ Gruis.
Mu Gruis
Observation data
Epoch J2000.0      Equinox J2000.0 (ICRS)
Constellation Grus
Right ascension 22 15 36.93338
Declination −41° 20′ 48.3558″
Apparent magnitude (V) 4.79 (5.20 + 6.68)
Characteristics
Spectral type G8 III + G
U−B color index +0.47
B−V color index +0.80
Astrometry
Radial velocity (Rv)−4.82±1.54 km/s
Proper motion (μ) RA: +30.774 mas/yr
Dec.: +42.645 mas/yr
Parallax (π)13.5115 ± 0.2846 mas
Distance241 ± 5 ly
(74 ± 2 pc)
Absolute magnitude (MV)+0.17
Orbit
Period (P)19.04+0.16
−0.18 yr
Semi-major axis (a)0.168+0.003
−0.002″
Eccentricity (e)0.561+0.025
−0.020
Inclination (i)65.69+0.44
−0.53°
Longitude of the node (Ω)104.2+1.6
−1.8°
Periastron epoch (T)1996.35+0.17
−0.18
Argument of periastron (ω)
(secondary)
92.61+0.67
−0.54°
Details
A
Radius9.3+1.4
−1.3 R
Luminosity66.9+1.8
−1.6 L
Temperature5,422+423
−377 K
Other designations
μ Gru, CD−41° 14810, FK5 3777, HD 211088, HIP 109908, HR 8486, SAO 231055, WDS J22156-4121
Database references
SIMBADdata

Mu Gruis, Latinized from μ Gruis, is a binary star system in the southern constellation of Grus. It is visible to the naked eye with a combined apparent visual magnitude of 4.79. The distance to this system, as determined using an annual parallax shift of 11.44 mas as seen from the Earth, is around 275 light years. It is drifting closer with a heliocentric radial velocity of −5 km/s.

The pair orbit each other with a period of 19 years and an eccentricity of 0.56. The yellow-hued primary component is an evolved giant star with stellar classification of G III and visual magnitude 5.20. With the supply of hydrogen at its core exhausted, it cooled and expanded; at present it has nine times the girth of the Sun. The star is radiating 67 times the luminosity of the Sun from its enlarged photosphere at an effective temperature of 5,422 K.

The secondary component is magnitude 6.68 and classed as a G-type star, although its color index and absolute magnitude suggest it is of type A6.

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. ^ Johnson, H. L.; et al. (1966), "UBVRIJKL photometry of the bright stars", Communications of the Lunar and Planetary Laboratory, 4 (99): 99, Bibcode:1966CoLPL...4...99J.
  3. ^ 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.
  4. ^ Houk, N. (1978), Michigan catalogue of two-dimensional spectral types for the HD stars, vol. 2, Dept. of Astronomy, University of Michigan, Bibcode:1978mcts.book.....H.
  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.
  6. ^ Mendez, Rene A.; et al. (November 2017), "Orbits for 18 Visual Binaries and Two Double-line Spectroscopic Binaries Observed with HRCAM on the CTIO SOAR 4 m Telescope, Using a New Bayesian Orbit Code Based on Markov Chain Monte Carlo", The Astronomical Journal, 154 (5): 22, arXiv:1709.06582, Bibcode:2017AJ....154..187M, doi:10.3847/1538-3881/aa8d6f, S2CID 55695873, 187.
  7. "mu.01 Gru". SIMBAD. Centre de données astronomiques de Strasbourg. Retrieved 2017-06-26.{{cite web}}: CS1 maint: postscript (link)
  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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