Astronomy:102 Herculis
| Observation data Equinox J2000.0]] (ICRS) | |
|---|---|
| Constellation | Hercules |
| Right ascension | 18h 08m 45.49142s[1] |
| Declination | +20° 48′ 52.4079″[1] |
| Apparent magnitude (V) | 4.37[2] |
| Characteristics | |
| Spectral type | B2 IV[3][4] or B2 V[5][6] |
| B−V color index | −0.164±0.013[2] |
| Astrometry | |
| Radial velocity (Rv) | −14.9±0.6[2] km/s |
| Proper motion (μ) | RA: −1.92[1] mas/yr Dec.: −5.89[1] mas/yr |
| Parallax (π) | 3.56 ± 0.19[1] mas |
| Distance | 920 ± 50 ly (280 ± 10 pc) |
| Absolute magnitude (MV) | −2.87[2] |
| Details | |
| Mass | 9.7±0.2[4] M☉ |
| Luminosity | 3,631.92[2] L☉ |
| Surface gravity (log g) | 3.54[7] cgs |
| Temperature | 22,420±1,440[8] K |
| Rotational velocity (v sin i) | 41[9] km/s |
| Age | 20.0±1.4[4] Myr |
| Other designations | |
| Database references | |
| SIMBAD | data |
102 Herculis is a single[11] star in the northern constellation of Hercules. It is visible to the naked eye as a faint, blue-white hued star with an apparent visual magnitude of 4.37.[2] Based upon parallax measurements, it is located around 920 light years away from the Sun.[1] The star is moving closer to the Earth with a heliocentric radial velocity of −15 km/s.[2]
The stellar classification of this object matches a massive, early B-type star with a luminosity class of IV[3] or V,[5] corresponding to a subgiant or main sequence star, respectively. It is 20[4] million years old with nearly ten[4] times the mass of the Sun and is spinning with a projected rotational velocity of 41 km/s.[9] The strength of the stellar magnetic field has been measured at (209.5±135.4)×10−4 T.[6] The star is radiating 3,632[2] times the Sun's luminosity from its photosphere at an effective temperature of 22,420 K.[8]
Etymology
In Chinese, 帛度 (Bó Dù), meaning Textile Ruler, refers to an asterism consisting of 102 Herculis and 95 Her[12].Consequently, 102 Herculis itself is known as 帛度二 (Bó Dù èr, English: the Second Star of Textile Ruler.)
This star, together with 93 Her, 95 Her, and 109 Her, formed the now obsolete constellation of Cerberus.[13]
References
- ↑ 1.0 1.1 1.2 1.3 1.4 1.5 van Leeuwen, F. (2007), "Validation of the new Hipparcos reduction", Astronomy and Astrophysics 474 (2): 653–664, doi:10.1051/0004-6361:20078357, Bibcode: 2007A&A...474..653V.
- ↑ 2.0 2.1 2.2 2.3 2.4 2.5 2.6 2.7 Anderson, E.; Francis, Ch. (2012), "XHIP: An extended hipparcos compilation", Astronomy Letters 38 (5): 331, doi:10.1134/S1063773712050015, Bibcode: 2012AstL...38..331A.
- ↑ 3.0 3.1 Lesh, Janet Rountree (December 1968), "The Kinematics of the Gould Belt: an Expanding Group?", Astrophysical Journal Supplement 17: 371, doi:10.1086/190179, Bibcode: 1968ApJS...17..371L.
- ↑ 4.0 4.1 4.2 4.3 4.4 Tetzlaff, N. et al. (January 2011), "A catalogue of young runaway Hipparcos stars within 3 kpc from the Sun", Monthly Notices of the Royal Astronomical Society 410 (1): 190–200, doi:10.1111/j.1365-2966.2010.17434.x, Bibcode: 2011MNRAS.410..190T.
- ↑ 5.0 5.1 Eggen, Olin J. (1961), "Space motions and distribution of the apparently bright B-type stars", Royal Observatory Bulletins 41: 245–287, Bibcode: 1961RGOB...41..245E.
- ↑ 6.0 6.1 Bychkov, V. D. et al. (August 2003), "Catalogue of averaged stellar effective magnetic fields. I. Chemically peculiar A and B type stars", Astronomy and Astrophysics 407 (2): 631–642, doi:10.1051/0004-6361:20030741, Bibcode: 2003A&A...407..631B.
- ↑ Lyubimkov, L. S. et al. (June 2004), "Surface abundances of light elements for a large sample of early B-type stars - III. An analysis of helium lines in spectra of 102 stars", Monthly Notices of the Royal Astronomical Society 351 (2): 745–767, doi:10.1111/j.1365-2966.2004.07825.x, Bibcode: 2004MNRAS.351..745L.
- ↑ 8.0 8.1 Zorec, J. et al. (July 2009), "Fundamental parameters of B supergiants from the BCD system. I. Calibration of the (λ_1, D) parameters into Teff", Astronomy and Astrophysics 501 (1): 297–320, doi:10.1051/0004-6361/200811147, Bibcode: 2009A&A...501..297Z.
- ↑ 9.0 9.1 Simón-Díaz, S. et al. (2017), "The IACOB project . III. New observational clues to understand macroturbulent broadening in massive O- and B-type stars", Astronomy and Astrophysics 597: A22, doi:10.1051/0004-6361/201628541, Bibcode: 2017A&A...597A..22S.
- ↑ "102 Her". SIMBAD. Centre de données astronomiques de Strasbourg. http://simbad.u-strasbg.fr/simbad/sim-basic?Ident=102+Her.
- ↑ 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, Bibcode: 2008MNRAS.389..869E.
- ↑ Ian Ridpath's Startales - Hercules
- ↑ Ian Ridpath's Star Tales - Cerberus
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