23 Orionis
Double star in the constellation Orion
23 Orionis
Observation dataEpoch J2000 Equinox ICRS
Constellation
Orion
Right ascension
05h 22m 50.00474s
Declination
+03° 32′ 39.9770″
Apparent magnitude (V)
4.99 (4.95 + 6.76)
Characteristics
Evolutionary stage
main sequence
Spectral type
B1Ⅴ + B3Ⅴn
B−V color index
−0.096± 0.004
Astrometry Absolute magnitude (MV )−2.93
23 Ori A Radial velocity (Rv ) +18.0± 3.7 km/s Proper motion (μ) RA: −2.414 mas /yr Dec.: +1.230 mas /yr Parallax (π)2.7199± 0.3155 mas Distance approx. 1,200 ly (approx. 370 pc ) 23 Ori B Radial velocity (Rv )28 km/s Proper motion (μ) RA: +1.275 mas /yr Dec.: −0.552 mas /yr Parallax (π)2.5579± 0.0864 mas Distance 1,280 ± 40 ly (390 ± 10 pc )
Details 23 Ori A Mass 12.5± 0.6 M ☉ Radius 6.97 R ☉ Luminosity 26,546 L ☉ Surface gravity (log g ) 4.078± 0.045 cgs Temperature 25,400 K Rotational velocity (v sin i )350 km/s Age 15.4± 0.6 Myr 23 Ori B Mass 6.6± 0.1 M ☉ Radius 4.71 R ☉ Luminosity 1,620 L ☉ Temperature 18,700 K Rotational velocity (v sin i )370 km/s Age 22.8± 2.3 Myr
Other designations 23 Ori , SAO 112697 , WDS J05228+0333A : BD +03°871 , HD 35149 , HIP 25142 , HR 1770 , SAO 112697B : BD +03°872 , HD 35148 , HIP 25145 , SAO 112699
Database references SIMBAD data B
23 Orionis is a double star located around 1,200 light-years (370 parsecs ) away from the Sun in the equatorial constellation of Orion . It is visible to the naked eye as a dim, blue-white-hued point of light with a combined apparent visual magnitude of 4.99. The pair are moving away from the Earth with a heliocentric radial velocity of +18 km/s, and they are members of the Orion OB1 association , subgroup 1a.
Howe and Clarke (2009) catalog this as a double-lined spectroscopic binary star system with a wide projected separation of 9,460 AU . As of 2018, they had an angular separation of 31.9″ along a position angle of 30°. The brighter member, component A, is a B-type main-sequence star with a stellar classification of B1V. The secondary, component B, is of class B3V. Both stars are spinning rapidly.
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 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 .
1 2 Mason, B. D.; et al. (2014), "The Washington Visual Double Star Catalog", The Astronomical Journal , 122 (6): 3466, Bibcode :2001AJ....122.3466M , doi :10.1086/323920 .
1 2 3 4 5 6 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 .
1 2 de 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.
↑ Morrell, Nidia; Levato, Hugo (1991), "Spectroscopic Binaries in the Orion OB1 Association", The Astrophysical Journal Supplement Series , 75 : 965, Bibcode :1991ApJS...75..965M , doi :10.1086/191556 .
1 2 3 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 Howe, K. S.; Clarke, C. J. (January 2009), "An analysis of v sin (i) correlations in early-type binaries", Monthly Notices of the Royal Astronomical Society , 392 (1): 448– 454, Bibcode :2009MNRAS.392..448H , doi :10.1111/j.1365-2966.2008.14073.x .
1 2 3 4 Hohle, M. M.; et al. (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 .
↑ Huang, Wenjin; et al. (October 2010), "A Stellar Rotation Census of B Stars: From ZAMS to TAMS", The Astrophysical Journal , 722 (1): 605– 619, arXiv :1008.1761 , Bibcode :2010ApJ...722..605H , doi :10.1088/0004-637X/722/1/605 , S2CID 118532653 .
1 2 3 4 Levato, H. (1975), "Rotational velocities and spectral types for a sample of binary systems", Astronomy and Astrophysics , 19 : 91, Bibcode :1975A& AS...19...91L .
1 2 "23 Ori" . SIMBAD . Centre de données astronomiques de Strasbourg . Retrieved 2019-06-08 .
↑ Welty, Daniel E.; et al. (October 1999), "The Diffuse Interstellar Clouds toward 23 Orionis", The Astrophysical Journal Supplement Series , 124 (2): 465– 501, arXiv :astro-ph/9905234 , Bibcode :1999ApJS..124..465W , doi :10.1086/313263 , S2CID 13966185 .
↑ Chini, R.; et al. (2012), "A spectroscopic survey on the multiplicity of high-mass stars", Monthly Notices of the Royal Astronomical Society , 424 (3): 1925– 1929, arXiv :1205.5238 , Bibcode :2012MNRAS.424.1925C , doi :10.1111/j.1365-2966.2012.21317.x , S2CID 119120749 .