22 Orionis
Binary star system in the constellation Orion
22 Orionis
Location of 22 Orionis (circled)
Observation dataEpoch J2000 Equinox ICRS
Constellation
Orion
Right ascension
05h 21m 45.74861s
Declination
−00° 22′ 56.9105″
Apparent magnitude (V)
4.74
Characteristics
Spectral type
B2 IV-V
U−B color index
−0.79
B−V color index
−0.16
Astrometry Radial velocity (Rv )+28.80 km/s Proper motion (μ) RA: −1.320 mas /yr Dec.: +3.457 mas /yr Parallax (π)2.8672± 0.3512 mas Distance approx. 1,100 ly (approx. 350 pc ) Absolute magnitude (MV )−2.98
Orbit Period (P)293 days Eccentricity (e)0.15 Periastron epoch (T) 2,442,175 JD Argument of periastron (ω) (secondary)234° Semi-amplitude (K1 ) (primary)4.1 km/s
Details 22 Ori A Mass 9.5 M ☉ Radius 6.6 R ☉ Luminosity 7,244 L ☉ Surface gravity (log g )3.56 cgs Temperature 22,646 K Metallicity [Fe/H] −0.06 dex Rotation 9.35 days Rotational velocity (v sin i )9 km/s Age 18.5 Myr
Other designations o Orionis , 22 Ori , NSV 16291 , BD −00°930 , FK5 1147 , GC 6579 , HD 35039 , HIP 25044 , HR 1765 , SAO 132028
Database references SIMBAD data
22 Orionis is a binary star in the equatorial constellation of Orion . It has the Bayer designation o Orionis , while 22 Orionis is the Flamsteed designation . This system is visible to the naked eye as a faint, blue-white hued star with an apparent visual magnitude of 4.74. It is located approximately 1,100 light years away from the Sun based on parallax . The system is moving further from the Earth with a heliocentric radial velocity of +28.80
A light curves for 22 Orionis, adapted from Balona and Engelbrecht (1985)
This is a single-lined spectroscopic binary with an orbital period of 293 days and an eccentricity of 0.15. The visible member, component A, has a stellar classification of B2 IV-V, matching a B-type star with a luminosity class that displays mixed traits of a main sequence star and a subgiant . It is a suspected Beta Cephei variable or a slowly pulsating B star . The star has about nine times the mass of the Sun and is radiating 7,244 times the Sun's luminosity from its photosphere at an effective temperature of 22,646 K .
References
1 2 3 4 5 6 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 .
1 2 3 4 Ducati, J. R. (2002). "VizieR Online Data Catalog: Catalogue of Stellar Photometry in Johnson's 11-color system". CDS/ADC Collection of Electronic Catalogues . 2237 . Bibcode :2002yCat.2237....0D .
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1 2 Hoffleit, D.; Warren, W. H. (1995). "VizieR Online Data Catalog: Bright Star Catalogue, 5th Revised Ed. (Hoffleit+, 1991)". VizieR On-line Data Catalog: V/50. Originally Published in: 1964BS....C......0H . 5050 . Bibcode :1995yCat.5050....0H .
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↑ McDonald, I.; Zijlstra, A. A.; Watson, R. A. (2017). "Fundamental parameters and infrared excesses of Tycho-Gaia stars" . Monthly Notices of the Royal Astronomical Society . 471 (1): 770. arXiv :1706.02208 . Bibcode :2017MNRAS.471..770M . doi :10.1093/mnras/stx1433 .
1 2 Soubiran, Caroline; Le Campion, Jean-François; Brouillet, Nathalie; Chemin, Laurent (2016). "The PASTEL catalogue: 2016 version" . Astronomy & Astrophysics . 591 : A118. arXiv :1605.07384 . Bibcode :2016A& A...591A.118S . doi :10.1051/0004-6361/201628497 . S2CID 119258214 .
↑ Oelkers, Ryan J.; Rodriguez, Joseph E.; Stassun, Keivan G.; Pepper, Joshua; Somers, Garrett; Kafka, Stella; Stevens, Daniel J.; Beatty, Thomas G.; Siverd, Robert J.; Lund, Michael B.; Kuhn, Rudolf B.; James, David; Gaudi, B. Scott (2018). "Variability Properties of Four Million Sources in the TESS Input Catalog Observed with the Kilodegree Extremely Little Telescope Survey" . The Astronomical Journal . 155 (1): 39. arXiv :1711.03608 . Bibcode :2018AJ....155...39O . doi :10.3847/1538-3881/aa9bf4 .
↑ Simón-Díaz, S.; Godart, M.; Castro, N.; Herrero, A.; Aerts, C.; Puls, J.; Telting, J.; Grassitelli, L. (2017). "The IACOB project . III. New observational clues to understand macroturbulent broadening in massive O- and B-type stars" . Astronomy and Astrophysics . 597 : A22. arXiv :1608.05508 . Bibcode :2017A& A...597A..22S . doi :10.1051/0004-6361/201628541 . S2CID 3478126 . Vizier catalog entry
↑ Tetzlaff, N.; Neuhäuser, R.; Hohle, M. M. (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 . Vizier catalog entry
↑ "22 Ori" . SIMBAD . Centre de données astronomiques de Strasbourg . Retrieved 2019-06-09 .
↑ Eggleton, P. P.; Tokovinin, A. A. (2008). "A catalogue of multiplicity among bright stellar systems" . Monthly Notices of the Royal Astronomical Society . 389 (2): 869. arXiv :0806.2878 . Bibcode :2008MNRAS.389..869E . doi :10.1111/j.1365-2966.2008.13596.x . S2CID 14878976 .
↑ Balona, L. A.; Engelbrecht, C. A. (June 1985). "Photometry and frequency analysis of line profile variables" . Monthly Notices of the Royal Astronomical Society . 214 (4): 559– 574. Bibcode :1985MNRAS.214..559B . doi :10.1093/mnras/214.4.559 .
↑ Samus, N. N.; Durlevich, O. V.; et al. (2009). "VizieR Online Data Catalog: General Catalogue of Variable Stars (Samus+ 2007-2013)". VizieR On-line Data Catalog: B/GCVS. Originally Published in: 2009yCat....102025S . 1 . Bibcode :2009yCat....102025S .
↑ Smith, M. A. (February 1980), "Nonradial m-mode changes in the 53 Persei variable 22 Orionis", Astrophysical Journal Supplement Series , 42 : 261– 281, Bibcode :1980ApJS...42..261S , doi :10.1086/190651