Zeta Orionis

From Wikipedia, the free encyclopedia

Zeta Orionis Aa/Ab/B
Observation data
Epoch J2000
Constellation Orion
Right ascension 05h 40m 45.5s
Declination −01° 56′ 34″
Apparent magnitude (V) 1.70/~4/4.21
Spectral Characteristics
Spectral type O9 Iab/O/B0 III
U-B color index −1.07
B-V color index 0.14 / ? / −0.01
Variable type
Astrometry
Radial velocity (Rv) 18 km/s
Proper motion (μ) RA: 3.99 mas/yr
Dec.: 2.54 mas/yr
Parallax (π) 3.99 ± 0.79 mas
Distance approx. 800 ly
(approx. 250 pc)
Absolute magnitude (MV) −5.25/−3/−2.8
Visual binary orbit
Companion Zeta Orionis B
Period (P) 1,500 years
Semimajor axis (a) 2.728"
Eccentricity (e) 0.07
Inclination (i) 72.0°
Node (Ω) 155.5°
Periastron epoch (T) 2070.6
Physical Characteristics
Mass 28/23/? M
Radius 20/? R
Luminosity 100,000/1,300/? L
Temperature 30,000/?/24,000 K
Metallicity  ?
Rotation 140 km/s / ?
Age  ? years
Other designations
Alnitak, Al Nitak, ζ Ori, 50 Ori, HR 1948/9, BD −02°1338, HD 37742, SAO 132444, HIP 26727.
Database references
SIMBAD data

Zeta Orionis (ζ Ori) is a star in the constellation Orion. It also has the traditional name Alnitak. The name is taken from the Arabic an-nitaq, "the belt".

Alnitak is a triple star system at the eastern end of Orion's belt. The primary is a blue supergiant that is also a close binary. The Alnitak system is bathed in the nebulosity of IC 434.


[edit] In fiction

The City on the Edge of Forever, an episode of Star Trek: The Original Series, Kirk mentions that in the year 2030 there is a famous novelist from "a planet circling the far left star in Orion's Belt".

[edit] References

  • C. A. Hummel et al, "ζ Orionis A Is a Double Star", The Astrophysical Journal, volume 540, 2, 2000.

[edit] External links