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93 Herculis

From Wikipedia, the free encyclopedia
Star in the constellation Hercules
93 Herculis
Location of 93 Herculis (circled)
Observation data
Epoch J2000      Equinox J2000
ConstellationHercules
Right ascension18h 00m 03.41611s[1]
Declination+16° 45′ 03.2855″[1]
Apparent magnitude (V)4.67[2]
Characteristics
Spectral typeK0.5IIb[3]
B−Vcolor index1.254±0.007[2]
Astrometry
Radial velocity (Rv)−24.47±0.20[4] km/s
Proper motion (μ)RA: −6.878[1]mas/yr
Dec.: −9.696[1]mas/yr
Parallax (π)4.5894±0.3311 mas[1]
Distance710 ± 50 ly
(220 ± 20 pc)
Absolute magnitude (MV)−1.85[2]
Details
Radius47[5] R
Luminosity868[5] L
Surface gravity (log g)1.74[6] cgs
Temperature4,594[5] K
Metallicity[Fe/H]−0.01[6] dex
Rotational velocity (v sin i)1.3[7] km/s
Other designations
93 Her,BD+16°3335,FK5 1469,HD 164349,HIP 88128,HR 6713,SAO 103285[8]
Database references
SIMBADdata

93 Herculis is astar located around 750[1] light years away from the Sun in the northernconstellation ofHercules.[8] It is visible to the naked eye as a faint, orange-hued star with anapparent visual magnitude of 4.67[2] The brightness of the star is diminished by anextinction of 0.21 due tointerstellar dust.[9] It is moving closer to the Earth with a heliocentricradial velocity of −24.5 km/s.[4] This star, together with95 Her,102 Her, and109 Her, made up the obsolete constellationCerberus.[10]

This object has astellar classification of K0.5IIb,[3] which indicates it is anevolvedbright giant. With the supply of hydrogen at itscore exhausted, the star has expanded to 47 times theSun's radius. It is radiating around 868 times theluminosity of the Sun from its enlargedphotosphere at aneffective temperature of4,594 K.[5] It is generally deficient inmetal elements, but appears weakly enhanced in barium and other heavier elements.[11] This is a suspectedbarium star and hence may have awhite dwarf companion in orbit.[12]

References

[edit]
  1. ^abcdefBrown, 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 atVizieR.
  2. ^abcdAnderson, 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.
  3. ^abKeenan, Philip C.; McNeil, Raymond C. (1989), "The Perkins catalog of revised MK types for the cooler stars",Astrophysical Journal Supplement Series,71: 245,Bibcode:1989ApJS...71..245K,doi:10.1086/191373.
  4. ^abde Bruijne, J. H. J.; Eilers, A.-C. (October 2012), "Radial velocities for the HIPPARCOS-Gaia Hundred-Thousand-Proper-Motion project",Astronomy & Astrophysics,546: 14,arXiv:1208.3048,Bibcode:2012A&A...546A..61D,doi:10.1051/0004-6361/201219219,S2CID 59451347, A61.
  5. ^abcdFetherolf, Tara; Pepper, Joshua; Simpson, Emilie; Kane, Stephen R.; Močnik, Teo; English, John Edward; Antoci, Victoria; Huber, Daniel; Jenkins, Jon M.; Stassun, Keivan; Twicken, Joseph D.; Vanderspek, Roland; Winn, Joshua N. (2023)."Variability Catalog of Stars Observed during the TESS Prime Mission".The Astrophysical Journal Supplement Series.268 (1): 4.arXiv:2208.11721.Bibcode:2023ApJS..268....4F.doi:10.3847/1538-4365/acdee5.
  6. ^abCoelho, Paula R. T.; Bruzual, Gustavo; Charlot, Stéphane (2020)."To use or not to use synthetic stellar spectra in population synthesis models?".Monthly Notices of the Royal Astronomical Society.491 (2): 2025.arXiv:1910.11902.Bibcode:2020MNRAS.491.2025C.doi:10.1093/mnras/stz3023.
  7. ^De Medeiros, J. R.; Alves, S.; Udry, S.; Andersen, J.; Nordström, B.; Mayor, M. (2014). "A catalog of rotational and radial velocities for evolved stars. V. Southern stars".Astronomy and Astrophysics.561: A126.arXiv:1312.3474.Bibcode:2014A&A...561A.126D.doi:10.1051/0004-6361/201220762.
  8. ^ab"93 Her".SIMBAD.Centre de données astronomiques de Strasbourg. Retrieved2019-06-16.
  9. ^Famaey, B.; et al. (January 2005), "Local kinematics of K and M giants from CORAVEL/Hipparcos/Tycho-2 data. Revisiting the concept of superclusters",Astronomy and Astrophysics,430 (1):165–186,arXiv:astro-ph/0409579,Bibcode:2005A&A...430..165F,doi:10.1051/0004-6361:20041272,S2CID 17804304.
  10. ^Ridpath, Ian,Ian Ridpath's Star Tales - Cerberus, retrieved2019-06-16.
  11. ^Smith, G. R.; Harmer, D. L. (January 1982), "A differential curve-of-growth analysis of the candidate barium star 93 Her",Monthly Notices of the Royal Astronomical Society,198:273–280,Bibcode:1982MNRAS.198..273S,doi:10.1093/mnras/198.1.273.
  12. ^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.
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