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Mu Sagittarii information


μ Sagittarii
Location of μ Sgr(circled)
Observation data
Epoch J2000.0      Equinox J2000.0
Constellation Sagittarius
Right ascension 18h 13m 45.8s[1]
Declination −21° 03′ 32″[1]
Apparent magnitude (V) +3.85[2]
Characteristics
μ Sgr A
Spectral type B8Iap[3] + B1.5V[4]
U−B color index −0.52[5]
B−V color index +0.22[5]
Variable type EA + α Cyg[6]
μ Sgr B
Spectral type B9III[4]
U−B color index −0.11[5]
B−V color index −0.04[5]
μ Sgr C
U−B color index −0.30[5]
B−V color index +0.23[5]
μ Sgr D
Spectral type B2IV[7]
U−B color index −0.57[5]
B−V color index +0.11[5]
μ Sgr E
Spectral type B2.5V[7]
U−B color index −0.67[5]
B−V color index +0.04[5]
Astrometry
Parallax (π)A: 0.09 ± 0.28 mas[1]
Distance920[8] pc
Absolute magnitude (MV)A: −7.1[7]
B: −1.2[9]
D: −3.3[7]
E: −2.1[7]
Details
μ Sgr Aa
Mass14.1 - 30[10] M
Radius67.9[10] R
Luminosity200 000 L
Surface gravity (log g)2.0[10] cgs
Temperature12,000[10] K
μ Sgr Ab
Mass9.8 - 15[10] M
Radius12.2[10] R
Surface gravity (log g)4.0[10] cgs
Temperature23,000[10] K
Age10[7] Myr
μ Sgr B
Luminosity603[8] L
Temperature18,200[8] K
μ Sgr D
Luminosity1,660[8] L
Temperature20,400[8] K
μ Sgr E
Luminosity2,450[8] L
Temperature20,900[8] K
Other designations
Polis, μ Sagittarii, μ Sgr, Mu Sgr, 13 Sagittarii, CCDM J18210-2950, IDS 18078-2105, SAO 186497, WDS J18138-2104
μ Sgr A: HD 166937, HIP 89341, HR 6812, PPM 268080, BD−21°4908, FK5 682, GC 24856
μ Sgr D: HD 314059, BD−21°4907
μ Sgr E: HD 314057, BD−21°4909, 2MASS J18134906-2103528
Database references
SIMBADμ Sgr AB
μ Sgr D
μ Sgr E

Mu Sagittarii (μ Sagittarii, abbreviated Mu Sgr, μ Sgr) is a multiple star system in the constellation of Sagittarius. The brightest component, designated Mu Sagittarii Aa, is formally named Polis /ˈpɒlɪs/.[11] The system is 3,000 light-years from the Sun and is part of the Sgr OB1 stellar association.

  1. ^ a b c 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.
  2. ^ 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. ^ Fraser, M.; Dufton, P. L.; Hunter, I.; Ryans, R. S. I. (2010). "Atmospheric parameters and rotational velocities for a sample of Galactic B-type supergiants". Monthly Notices of the Royal Astronomical Society. 404 (3): 1306. arXiv:1001.3337. Bibcode:2010MNRAS.404.1306F. doi:10.1111/j.1365-2966.2010.16392.x. S2CID 118674151.
  4. ^ a b Cite error: The named reference zasche was invoked but never defined (see the help page).
  5. ^ a b c d e f g h i j Echevarria, J.; Roth, M.; Warman, J. (1979). "Photometric Study of Trapezium-Type Systems". Revista Mexicana de Astronomía y Astrofísica. 4: 287. Bibcode:1979RMxAA...4..287E.
  6. ^ Samus, N. N.; Durlevich, O. V.; et al. (2009). "VizieR Online Data Catalog: General Catalogue of Variable Stars (Samus+ 2007-2013)". VizieR On-line Data Catalog: B/GCVS. Originally Published in: 2009yCat....102025S. 1. Bibcode:2009yCat....102025S.
  7. ^ a b c d e f Abt, H. A.; Cardona, O. (1983). "Confirmation among visual multiples of an increase of AP stars with age". Astrophysical Journal. 272: 182. Bibcode:1983ApJ...272..182A. doi:10.1086/161276.
  8. ^ a b c d e f g Lindroos, K. P. (1986). "A study of visual double stars with early-type primaries. V - Post-T Tauri secondaries". Astronomy and Astrophysics. 156: 223. Bibcode:1986A&A...156..223L.
  9. ^ Cite error: The named reference lindroos1985 was invoked but never defined (see the help page).
  10. ^ a b c d e f g h Cite error: The named reference polidan was invoked but never defined (see the help page).
  11. ^ "Naming Stars". IAU.org. Retrieved 16 December 2017.

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Astronomical naming conventions

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