Observation data Epoch J2000.0 Equinox J2000.0 (ICRS)
Constellation
Orion
Right ascension
06h 07m 34.32588s[1]
Declination
+14° 46′ 06.5061″[1]
Apparent magnitude (V)
4.42[2]
Characteristics
Spectral type
B3 V[3] or B3 IV[4]
U−B color index
−0.67[2]
B−V color index
−0.18[2]
Astrometry
Radial velocity (Rv)
+24.1[5] km/s
Proper motion (μ)
RA: +6.78[1] mas/yr Dec.: −20.23[1] mas/yr
Parallax (π)
6.32 ± 0.33 mas[1]
Distance
520 ± 30 ly (158 ± 8 pc)
Orbit[6]
Period (P)
131.211 d
Eccentricity (e)
0.64
Periastron epoch (T)
2436475.852 JD
Argument of periastron (ω) (secondary)
6.6°
Semi-amplitude (K1) (primary)
33.3 km/s
Details
ν Ori A
Mass
6.7±0.1[4]M☉
Radius
4.3[7]R☉
Luminosity
1,965[3]L☉
Surface gravity (log g)
4.06[8] cgs
Temperature
17,880[8] K
Metallicity [Fe/H]
−0.05[8] dex
Rotational velocity (v sin i)
30[9] km/s
Age
26.3±5.3[4] Myr
Other designations
ν Ori, 67 Orionis, BD+14° 1152, FK5 232, HD 41753, HIP 29038, HR 2159, SAO 95259.[10]
Database references
SIMBAD
data
Nu Orionis (ν Orionis) is a binary star[11] system in the northeastern part of the constellation Orion. It should not be confused with the variable star NU Orionis.[12] Nu Orionis has an apparent visual magnitude of 4.42,[2] which is bright enough to be seen with the naked eye. Based upon an annual parallax shift of 0.00632 arcseconds,[1] the distance to this system is roughly 520 light years.
This is a single-lined spectroscopic binary system,[9] which means that only the absorption line features of one of the components can be distinguished. The components orbit each other with a period of 131.2 days and an eccentricity of 0.64.[6] Depending on the source, the primary is either a B-type main sequence star with a stellar classification of B3 V,[3] or a more evolved B-type subgiant star of class B3 IV.[4] It has an angular diameter of 0.251 mas,[13] which, at the estimated distance of this system, yields a physical size of about 4.3 times the radius of the Sun.[7] The mass is 6.7[4] times that of the Sun and it shines with 1,965[3] times the solar luminosity from its outer atmosphere at an effective temperature of 17,880 K.[8]
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NuOrionis (ν Orionis) is a binary star system in the northeastern part of the constellation Orion. It should not be confused with the variable star NU...
main-sequence star, NuOrionis, which is somewhat closer at 520 light-years' distance. The apparent visual magnitude of Xi Orionis is 4.47, which is bright...
X-Ray, Astrophoto, Sky Map, Articles and images On March 4 Full name: NUOrionis Gaia Data Release 2 gives a parallax that would place it 1,706 ± 36 light-years...
north of the zodiac, and 15 to the south. For instance, the stars nuOrionis and 62 Orionis which are now around ecliptic longitude 91° are attributed longitudes...
O4I(n)fp Alnilam (Epsilon Orionis) B-type supergiant, spectral type B0Ia, central star of Orion's Belt Saiph (Kappa Orionis) B-type supergiant, spectral...
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...
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...
Mrigashira - मृगशिर "the deer's head". Also known as āgrahāyaṇī λ "Meissa", φ Orionis Lord: Mangala (Mars) Symbol: Deer's head Deity: Soma, Chandra, the Moon...
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...
(1981). "The near ultraviolet stellar spectra of alpha Lyrae and beta Orionis". Monthly Notices of the Royal Astronomical Society. 197: 57–74. Bibcode:1981MNRAS...
Detail for NSV 4456". www.aavso.org. Retrieved 2022-09-01. "VSX : Detail for nu. Pup". www.aavso.org. Retrieved 2022-09-03. "VSX : Detail for NSV 14656"....
19°20′ Gemini 5 Mṛgaśīrā "the deer's head". Also known as āgrahāyaṇī λ, φ Orionis Astrological leader: Mangala (Mars) Symbol: Deer's head Rigvedic name:...
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...
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...
Abraham; Pease, Francis G. (1921). "Measurement of the diameter of alpha Orionis with the interferometer". Astrophysical Journal. 53 (5): 249–59. Bibcode:1921ApJ...
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...
light FUOR – (celestial object) FU Orionis objects, a class of variable pre–main sequence stars named after FU Orionis, the archetype for the class also...