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Mu Ophiuchi
Location of μ Ophiuchi (circled)
Observation data
Epoch J2000       Equinox J2000
Constellation Ophiuchus
Right ascension 17h 37m 50.71308s [1]
Declination −8° 07′ 07.5749″ [1]
Apparent magnitude (V) 4.62 [2]
Characteristics
Spectral type B8II-IIIp:Mn [3]
U−B color index −0.20 [2]
B−V color index +0.11 [2]
Astrometry
Radial velocity (Rv)−18.50 [4] km/s
Proper motion (μ) RA: −11.31 [5]  mas/ yr
Dec.: −20.47 [5]  mas/ yr
Parallax (π)4.32 ± 0.20  mas [5]
Distance750 ± 30  ly
(230 ± 10  pc)
Absolute magnitude (MV)-2.24 [6]
Details
Radius11.1+2.1
−0.6
[1]  R
Luminosity398.7±26.8 [1]  L
Temperature7,748+210
−651
[1]  K
Metallicity [Fe/H]+0.00 [7]  dex
Rotational velocity (v sin i)95 [8] km/s
Other designations
μ Oph, 57 Ophiuchi, BD−08°4472, FK5 3399, GC 23889, HD 159975, HIP 86284, HR 6567, SAO 141772 [9]
Database references
SIMBAD data

μ Ophiuchi, Latinized as Mu Ophiuchi, is a solitary, [10] blue-white hued star in the equatorial constellation of Ophiuchus. It is visible to the naked as a faint point of light with an apparent visual magnitude of 4.62. [2] This object is located approximately 760  light years away from the Sun based on parallax, [5] but is drifting closer with a radial velocity of −18.5 km/s. [4]

This object has a stellar classification of B8II-IIIp:Mn, [3] showing a luminosity class with mixed traits of a giant or bright giant star. The suffix notation indicates it is a candidate chemically peculiar star with an overabundance of manganese in its spectrum. It may be a mercury-manganese star. [11] This object has 11 times the radius of the Sun and is radiating nearly 400 times the Sun's luminosity from its photosphere at an effective temperature of 7,748 K. [1] It is spinning with a projected rotational velocity of 95 km/s. [8]

In 2006, a new nearby star cluster, Mamajek 2 ( /ˈmæməɛk/), was discovered. Mu Ophiuchi is a candidate member. [12] The cluster has an estimated age of 120±25 million years. [13]

References

  1. ^ 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.
  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 Cowley, A. (November 1972). "Spectral classification of the bright B8 stars". Astronomical Journal. 77: 750–755. Bibcode: 1972AJ.....77..750C. doi: 10.1086/111348.
  4. ^ a b Gontcharov, G. A. (2006). "Pulkovo Compilation of Radial Velocities for 35 495 Hipparcos stars in a common system". Astronomy Letters. 32 (11): 759–771. arXiv: 1606.08053. Bibcode: 2006AstL...32..759G. doi: 10.1134/S1063773706110065. S2CID  119231169.
  5. ^ a b c d 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
  6. ^ 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
  7. ^ Gontcharov, G. A. (2012). "Dependence of kinematics on the age of stars in the solar neighborhood". Astronomy Letters. 38 (12): 771–782. arXiv: 1606.08814. Bibcode: 2012AstL...38..771G. doi: 10.1134/S1063773712120031. S2CID  118345778. Vizier catalog entry
  8. ^ a b Abt, Helmut A.; et al. (2002). "Rotational Velocities of B Stars". The Astrophysical Journal. 573 (1): 359–365. Bibcode: 2002ApJ...573..359A. doi: 10.1086/340590.
  9. ^ "mu. Oph". 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.
  11. ^ Renson, P.; Manfroid, J. (May 2009). "Catalogue of Ap, HgMn and Am stars". Astronomy and Astrophysics. 498 (3): 961–966. Bibcode: 2009A&A...498..961R. doi: 10.1051/0004-6361/200810788.
  12. ^ Mamajek, Eric E. (2006). "A New Nearby Candidate Star Cluster in Ophiuchus at d = 170 pc". Astronomical Journal. 132 (5): 2198–2205. arXiv: astro-ph/0609064. Bibcode: 2006AJ....132.2198M. doi: 10.1086/508205. S2CID  14070978.
  13. ^ Jilinski, E.; et al. (January 2009). "Dynamical Evolution and Spectral Characteristics of the Stellar Group Mamajek 2". The Astrophysical Journal. 691 (1): 212–218. arXiv: 0810.1198. Bibcode: 2009ApJ...691..212J. doi: 10.1088/0004-637X/691/1/212. S2CID  15570695.