Astronomy:HD 176871

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Short description: Star in the constellation Lyra
HD 176871
Observation data
Equinox J2000.0]] (ICRS)
Constellation Lyra[1]
Right ascension  19h 01m 17.35683s[2]
Declination +26° 17′ 29.0764″[2]
Apparent magnitude (V) 5.69[1]
Characteristics
Spectral type B5V[3][1][4]
U−B color index −0.55[3]
B−V color index −0.086±0.002[1]
Astrometry
Radial velocity (Rv)−20.4±1.2[1] km/s
Proper motion (μ) RA: −0.489[2] mas/yr
Dec.: −9.207[2] mas/yr
Parallax (π)4.1038 ± 0.0835[2] mas
Distance790 ± 20 ly
(244 ± 5 pc)
Absolute magnitude (MV)−0.80[1]
Details
Mass4.1[5] M
Radius5.2[6] R
Luminosity394[5] L
Surface gravity (log g)4.5[4] cgs
Temperature11,688[6] K
Rotational velocity (v sin i)268±34[7] km/s
Age11[4] Myr
Other designations
BD+26°3429, FK5 3518, GC 26151, HD 176871, HIP 93393, HR 7202, SAO 86707[8]
Database references
SIMBADdata

HD 176871 is a single[9] star in the northern constellation of Lyra, positioned near the southern constellation border with Vulpecula. This object has a blue-white hue and is dimly visible to the naked eye with an apparent visual magnitude of 5.69.[1] It is located at a distance of approximately 790 light years from the Sun based on parallax, and has an absolute magnitude of −0.80.[1] The star is drifting closer with a radial velocity of −20 km/s.[1]

This is a normal B-type main-sequence star with a stellar classification of B5V,[3] which means it is generating energy via core hydrogen fusion. The star is around 11[4] million years old with 5.4[4] times the mass of the Sun and is spinning rapidly with a projected rotational velocity of 268 km/s.[7] It is radiating 233[10] times the luminosity of the Sun from its photosphere at an effective temperature of 10,540 K.[10]

References

  1. 1.0 1.1 1.2 1.3 1.4 1.5 1.6 1.7 1.8 Anderson, E.; Francis, Ch. (2012). "XHIP: An extended hipparcos compilation". Astronomy Letters 38 (5): 331. doi:10.1134/S1063773712050015. Bibcode2012AstL...38..331A.  XHIP record for this object at VizieR.
  2. 2.0 2.1 2.2 2.3 2.4 Brown, A. G. A. (August 2018). "Gaia Data Release 2: Summary of the contents and survey properties". Astronomy & Astrophysics 616: A1. doi:10.1051/0004-6361/201833051. Bibcode2018A&A...616A...1G.  Gaia DR2 record for this source at VizieR.
  3. 3.0 3.1 3.2 Hill, P. W.; Lynas-Gray, A. E. (September 1977), "UBV photometry and MK spectral classification of northern early-type stars at intermediate galactic latitudes.", Monthly Notices of the Royal Astronomical Society 180 (4): 691–702, doi:10.1093/mnras/180.4.691, Bibcode1977MNRAS.180..691H. 
  4. 4.0 4.1 4.2 4.3 4.4 Gullikson, Kevin et al. (2016), "The Close Companion Mass-ratio Distribution of Intermediate-mass Stars", The Astronomical Journal 152 (2): 40, doi:10.3847/0004-6256/152/2/40, Bibcode2016AJ....152...40G. 
  5. 5.0 5.1 Quintana, Alexis L.; Wright, Nicholas J.; Martínez García, Juan (2025), "A census of OB stars within 1 KPC and the star formation and core collapse supernova rates of the Milky Way", Monthly Notices of the Royal Astronomical Society 538 (3): 1367, doi:10.1093/mnras/staf083, Bibcode2025MNRAS.538.1367Q. 
  6. 6.0 6.1 Stassun, Keivan G. et al. (2019), "The Revised TESS Input Catalog and Candidate Target List", The Astronomical Journal 158 (4): 138, doi:10.3847/1538-3881/ab3467, Bibcode2019AJ....158..138S. 
  7. 7.0 7.1 Maestro, V. et al. (2013), "Optical interferometry of early-type stars with PAVO@CHARA - I. Fundamental stellar properties", Monthly Notices of the Royal Astronomical Society 434 (2): 1321, doi:10.1093/mnras/stt1092, Bibcode2013MNRAS.434.1321M. 
  8. "HD 176871". SIMBAD. Centre de données astronomiques de Strasbourg. http://simbad.u-strasbg.fr/simbad/sim-basic?Ident=HD+176871. 
  9. 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, doi:10.1111/j.1365-2966.2008.13596.x, Bibcode2008MNRAS.389..869E. 
  10. 10.0 10.1 McDonald, I. et al. (2012), "Fundamental parameters and infrared excesses of Hipparcos stars", Monthly Notices of the Royal Astronomical Society 427 (1): 343–357, doi:10.1111/j.1365-2966.2012.21873.x, Bibcode2012MNRAS.427..343M.