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n Herculis

From Wikipedia, the free encyclopedia
Star in the Hercules constellation
n Herculis
Observation data
EpochJ2000.0      EquinoxJ2000.0
ConstellationHercules[1]
Right ascension16h 32m 35.7s[2]
Declination+5° 31′ 16″[2]
Apparent magnitude (V)5.63[3]
Characteristics
Evolutionary stagemain sequence[4]
Spectral typeB9.5III[5]
U−Bcolor index−0.18[6]
B−Vcolor index−0.06[6]
Astrometry
Radial velocity (Rv)−23.38±0.21[2] km/s
Proper motion (μ)RA: +15.556[2]mas/yr
Dec.: −0.282[2]mas/yr
Parallax (π)8.5519±0.1394 mas[2]
Distance381 ± 6 ly
(117 ± 2 pc)
Absolute magnitude (MV)+0.27[1]
Details
Mass2.75[7] M
Radius2.94[7] R
Luminosity99[7] L
Surface gravity (log g)3.94[7] cgs
Temperature10,623[7] K
Rotational velocity (v sin i)9.6[8] km/s
Age237[9] Myr
Other designations
28 Herculis,BD+05°3223,HD 149121,HIP 81007,HR 6158,SAO 121676[10]
Database references
SIMBADdata

n Herculis, also known as 28 Herculis, is amercury-manganese star[11] in the constellationHercules at a distance of approximately 381light-years (about 117parsecs) from theSun. Theapparent magnitude of the star is +5.6. Once in the constellationOphiuchus, it was also catalogued as 11 Ophiuchi.[10]

References

[edit]
  1. ^abAnderson, 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. XHIP record for this object atVizieR.
  2. ^abcdefVallenari, A.; et al. (Gaia collaboration) (2023)."Gaia Data Release 3. Summary of the content and survey properties".Astronomy and Astrophysics.674: A1.arXiv:2208.00211.Bibcode:2023A&A...674A...1G.doi:10.1051/0004-6361/202243940.S2CID 244398875. Gaia DR3 record for this source atVizieR.
  3. ^Ducati, J. R. (2002). "VizieR Online Data Catalog: Stellar Photometry in Johnson's 11-color system (Ducati, 2002)".Vizier Online Data Catalog.Bibcode:2002yCat.2237....0D.
  4. ^Takeda, Yoichi; Takada-Hidai, Masahide; Jugaku, Jun; Sakaue, Akihiko; Sadakane, Kozo (1999). "Oxygen 6156-8 Angstroms Triplet in Chemically Peculiar Stars of the Upper Main Sequence: Do HGMN Stars Show an Oxygen Anomaly?".Publications of the Astronomical Society of Japan.51: 961.Bibcode:1999PASJ...51..961T.doi:10.1093/pasj/51.6.961.
  5. ^"VizieR Detailed Page". Archived fromthe original on 2016-03-05. Retrieved2012-07-13.
  6. ^abHamdy, M. A.; Abo Elazm, M. S.; Saad, S. M. (1993). "A Catalogue of Spectral Classification and Photometric Data of B-Type Stars".Astrophysics and Space Science.203 (1): 53.Bibcode:1993Ap&SS.203...53H.doi:10.1007/BF00659414.
  7. ^abcdeStassun, Keivan G.; et al. (2019)."The Revised TESS Input Catalog and Candidate Target List".The Astronomical Journal.158 (4): 138.arXiv:1905.10694.Bibcode:2019AJ....158..138S.doi:10.3847/1538-3881/ab3467.
  8. ^Takeda, Yoichi; Han, Inwoo; Kang, Dong-Il; Lee, Byeong-Cheol; Kim, Kang-Min (2019)."Compositional differences between the component stars of eclipsing close binary systems showing chemical peculiarities".Monthly Notices of the Royal Astronomical Society.485 (1): 1067.arXiv:1902.04766.Bibcode:2019MNRAS.485.1067T.doi:10.1093/mnras/stz449.
  9. ^Gontcharov, G. A. (2012). "Dependence of kinematics on the age of stars in the solar neighborhood".Astronomy Letters.38 (12): 771.arXiv:1606.08814.Bibcode:2012AstL...38..771G.doi:10.1134/S1063773712120031.
  10. ^ab"28 Herculis".SIMBAD.Centre de données astronomiques de Strasbourg. Retrieved2025-10-16.
  11. ^Ghazaryan, S.; Alecian, G. (2016)."Statistical analysis from recent abundance determinations in HGMN stars".Monthly Notices of the Royal Astronomical Society.460 (2): 1912.Bibcode:2016MNRAS.460.1912G.doi:10.1093/mnras/stw911.
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