Observation data Epoch J2000.0 Equinox J2000.0 (ICRS)
Constellation
Orion
Right ascension
06h 11m 56.39693s[1]
Declination
+14° 12′ 31.5555″[1]
Apparent magnitude (V)
4.47[2]
Characteristics
Spectral type
B3 IV[3]
U−B color index
−0.65[2]
B−V color index
−0.19[2]
Astrometry
Radial velocity (Rv)
+19.30[4] km/s
Proper motion (μ)
RA: +0.29[1] mas/yr Dec.: −20.12[1] mas/yr
Parallax (π)
5.37 ± 0.23 mas[1]
Distance
610 ± 30 ly (186 ± 8 pc)
Orbit[5]
Period (P)
45.1 d
Eccentricity (e)
0.26
Periastron epoch (T)
2,441,962.3 JD
Argument of periastron (ω) (secondary)
205°
Semi-amplitude (K1) (primary)
22.4 km/s
Details
ξ Ori A
Mass
6.7±0.1[3]M☉
Luminosity
1,390[6]L☉
Temperature
15,476[6] K
Rotational velocity (v sin i)
160[7] km/s
Age
32.1±4.3[3] Myr
Other designations
ξ Ori, 70 Orionis, BD+14° 1187, HD 42560, HIP 29426, HR 2199, SAO 95362[8]
Database references
SIMBAD
data
Xi Orionis (ξ Orionis) is a binary star system in the northeastern part of the constellation of Orion, well above the red giant star Betelgeuse in the sky. It lies next to another blue main-sequence star, Nu Orionis, which is somewhat closer at 520 light-years' distance. The apparent visual magnitude of Xi Orionis is 4.47,[2] which is bright enough to be seen with the naked eye. The distance to this star, as determined using the parallax method, is roughly 610 light-years.[1]
This is a spectroscopic binary star system with an orbital period of 45.1 days and an eccentricity of 0.26.[5] The primary component is a B-type subgiant star with a stellar classification of B3 IV.[3] With an estimated age of just 32 million years,[3] it has a relatively high rate of spin, showing a projected rotational velocity of 160 km/s.[7] Xi Orionis has about 6.7 times the mass of the Sun,[3] and shines with 1,390 times the solar luminosity from its outer atmosphere at an effective temperature of 15,476 K.[6]
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^ abcdCite error: The named reference Crawford1971 was invoked but never defined (see the help page).
^ abcdefCite error: The named reference Tetzlaff2011 was invoked but never defined (see the help page).
^Cite error: The named reference deBruijne2012 was invoked but never defined (see the help page).
^ abCite error: The named reference pourbaix2004 was invoked but never defined (see the help page).
^ abcCite error: The named reference Mcdonald2012 was invoked but never defined (see the help page).
^ abCite error: The named reference Abt2002 was invoked but never defined (see the help page).
^Cite error: The named reference SIMBAD was invoked but never defined (see the help page).
XiOrionis (ξ Orionis) is a binary star system in the northeastern part of the constellation of Orion, well above the red giant star Betelgeuse in the...
APIN, this name was also applied to the pairs of Pi3 and Pi4 Orionis and Zeta and XiOrionis. The meaning of MASH.TAB.BA evolved as well, becoming the twin...
degrees to the north of Xi Orionis. It has the Bayer designation f1 Orionis; 69 Orionis is the Flamsteed designation. The star is visible to the naked eye...
University Press. p. 170. ISBN 0-521-44921-9. Kaler, James B. "Saiph (Kappa Orionis)". Stars. University of Illinois. Archived from the original on 2012-02-02...
are some exceptions such as the chain of stars π1, π2, π3, π4, π5 and π6 Orionis. The most stars given the same Bayer designation but with an extra number...
constellation of Pegasus. Menkab, traditional name for the star Alpha Orionis or Betelgeuse in the constellation of Orion Markab, the proper name approved...
study of mass loss from the mid-ultraviolet spectrum of α Cygni (A2 Ia), β Orionis (B8 Ia), and η Leonis (A0 Ib)". The Astrophysical Journal. 223: 207. Bibcode:1978ApJ...
et al. (2006). "A search for substellar members in the Praesepe and Sigma Orionis clusters". Astronomy & Astrophysics. 460 (3): 799–810. arXiv:astro-ph/0609283...
of the zodiac, and 15 to the south. For instance, the stars nu Orionis and 62 Orionis which are now around ecliptic longitude 91° are attributed longitudes...
; Zavala, R. T. (2013). "Dynamical mass of the O-type supergiant in ζ Orionis A". Astronomy & Astrophysics. 554: A52. arXiv:1306.0330. Bibcode:2013A&A...
31 Eta Orionis Quadruple star system 3.35 Theta Leonis Star 3.35 Omicron Ursae Majoris Star 3.35 Zeta Cephei Star Suspected variable star 3.36 Xi Geminorum...
297, been found to have a dusty disk surrounding it, and is also a UX Orionis star, meaning that it shows irregular variations in its brightness. The...
; Zavala, R. T. (2013). "Dynamical mass of the O-type supergiant in ζ Orionis A". Astronomy & Astrophysics. 554: A52. arXiv:1306.0330. Bibcode:2013A&A...
a mere 300,000 years old composed of two pre-main-sequence stars—a FU Orionis star and a Herbig Ae/Be star, which has brightened episodically by two...
Olivier; Pueyo, Laurent; Robin, Annie C.; Doyon, René (March 2018). "BANYAN. XI. The BANYAN Σ Multivariate Bayesian Algorithm to Identify Members of Young...
eclipsing binaries - Into the G stars with HS Aurigae, FL Lyrae, and EW Orionis". The Astronomical Journal. 91: 383. Bibcode:1986AJ.....91..383P. doi:10...
Netherlands and eventually becomes part of Belgium. March 28 – The nova V529 Orionis is discovered by Polish astronomer Johannes Hevelius (Jan Heweliusz). April...
Brown Dwarfs. Astrophysics and Space Science Library. Vol. 401. SpringerLink. XI, 168. doi:10.1007/978-3-319-01162-2. eISSN 2214-7985. ISBN 978-3-319-01162-2...
Netherlands and eventually becomes part of Belgium. March 28 – The nova V529 Orionis is discovered by Polish astronomer Johannes Hevelius (Jan Heweliusz). April...