Alnitak (Zeta Orionis)
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Alnitak is the left-hand star in Orion's Belt. Image: NASA
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The left hand star in Orion's Belt, the fifth brightest in the whole of Orion, and (in terms of apparent magnitude) the brightest O star in the sky. Its Arabic name comes from a phrase meaning "the belt of al Jauza." A B-type companion lies about 3 arc-seconds away, the pair orbiting each other with a period of several thousand years.
Like all O stars, Alnitak is a source of X-rays that seem to come from a stellar wind that blows from its surface at nearly 2,000 km/s. The X-rays are produced when blobs of gas in the wind crash violently into one another. Alnitak is probably only about 6 million years old and will eventually become a red supergiant before exploding as a supernova. In its vicinity are several dusty interstellar clouds, including, to the south, the Horsehead Nebula.
| visual magnitude |
1.74 |
| absolute magnitude |
-5.26 |
| spectral type |
O9.5Ib |
| surface temperature |
31,000 K |
| luminosity |
100,000 Lsun |
| mass |
20 Msun |
| distance |
817 light-years |
| position |
R.A. 05h 40m 45.5s,
Dec. -01° 56' 34" |
| other designations |
Al Nitak, 50 Ori, HR 1948/9,
BD -02°1338, HD 37742,
SAO 132444, HIP 26727 |
Related category
NOTABLE STARS
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