Observation data Epoch J2000 Equinox J2000 | |
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Constellation | Lacerta |
Right ascension | 22 30 29.26005 |
Declination | +43° 07′ 24.1565″ |
Apparent magnitude (V) | 4.52 |
Characteristics | |
Spectral type | B2 IV |
B−V color index | −0.086±0.018 |
Astrometry | |
Radial velocity (Rv) | −8.7±0.9 km/s |
Proper motion (μ) | RA: −4.800 mas/yr Dec.: −2.598 mas/yr |
Parallax (π) | 1.7577 ± 0.2697 mas |
Distance | approx. 1,900 ly (approx. 570 pc) |
Absolute magnitude (MV) | −2.62 |
Orbit | |
Period (P) | 880 days |
Eccentricity (e) | 0.30 |
Periastron epoch (T) | 2,416,300 JD |
Argument of periastron (ω) (secondary) | 190° |
Semi-amplitude (K1) (primary) | 9 km/s |
Details | |
Mass | 12.5±0.6 M☉ |
Radius | 6.9 R☉ |
Luminosity (bolometric) | 34,590 L☉ |
Surface gravity (log g) | 3.56 cgs |
Temperature | 21,150 K |
Metallicity | −0.04 dex |
Rotational velocity (v sin i) | 70 km/s |
Age | 15.7±0.1 Myr |
Other designations | |
6 Lac, BD+42° 4420, FK5 3800, HD 213420, HIP 111104, HR 8579, SAO 52079 | |
Database references | |
SIMBAD | data |
6 Lacertae is a binary star system in the northern constellation of Lacerta, located around 1,900 light years from the Sun. It is visible to the naked eye as a dim, blue-white hued star with a combined apparent visual magnitude of 4.52. The system is moving closer to the Earth with a heliocentric radial velocity of −9 km/s, and is a suspected member of the Lac OB1 association.
This system forms a single-lined spectroscopic binary with an orbital period of 880 days and an eccentricity of 0.3. The visible component has a stellar classification of B2 IV, matching a B-type subgiant star. It is about 16 million years old with a relatively high projected rotational velocity of 70 km/s. The star has 12.5 times the mass of the Sun and about 7 times the Sun's radius. It is radiating a net 34,590 times the Sun's luminosity from its photosphere at an effective temperature of 21,150 K.
References
- ^ Brown, 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 at VizieR.
- ^ Anderson, 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.
- ^ Lesh, Janet Rountree (December 1968), "The Kinematics of the Gould Belt: an Expanding Group?", Astrophysical Journal Supplement, 17: 371, Bibcode:1968ApJS...17..371L, doi:10.1086/190179
- ^ Kaltcheva, Nadia (October 2009), "Lacerta OB1 Revisited", Publications of the Astronomical Society of the Pacific, 121 (884): 1045–1053, Bibcode:2009PASP..121.1045K, doi:10.1086/606037, S2CID 120329065.
- ^ Beardsley, Wallace R. (1969), "The Radial Velocities of 129 Stars in the Years 1906 to 1917", Publications of the Allegheny Observatory of the University of Pittsburgh, 7: 91–263, Bibcode:1969PAllO...8...91B.
- ^ 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, arXiv:1007.4883, Bibcode:2011MNRAS.410..190T, doi:10.1111/j.1365-2966.2010.17434.x, S2CID 118629873.
- ^ Pasinetti Fracassini, L. E.; et al. (February 2001), "Catalogue of Apparent Diameters and Absolute Radii of Stars (CADARS)", Astronomy and Astrophysics, 367 (Third ed.): 521–524, arXiv:astro-ph/0012289, Bibcode:2001A&A...367..521P, doi:10.1051/0004-6361:20000451, S2CID 425754.
- ^ Hohle, M. M.; et al. (April 2010), "Masses and luminosities of O- and B-type stars and red supergiants", Astronomische Nachrichten, 331 (4): 349, arXiv:1003.2335, Bibcode:2010AN....331..349H, doi:10.1002/asna.200911355, S2CID 111387483.
- ^ Gies, Douglas R.; Lambert, David L. (March 1992), "Carbon, Nitrogen, and Oxygen Abundances in Early B-Type Stars", Astrophysical Journal, 387: 673, Bibcode:1992ApJ...387..673G, doi:10.1086/171116.
- ^ Strom, Stephen E.; et al. (2005), "B Star Rotational Velocities in h and χ Persei: A Probe of Initial Conditions during the Star Formation Epoch?", The Astronomical Journal, 129 (2): 809–828, arXiv:astro-ph/0410337, Bibcode:2005AJ....129..809S, doi:10.1086/426748, S2CID 15059129.
- "6 Lac". SIMBAD. Centre de données astronomiques de Strasbourg. Retrieved 2019-01-28.
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