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Encyclopedia > Alnilam

Alnilam, also known as ε Orionis or 46 Orionis, is a large blue star in the constellation of Orion. It is the 30th brightest star in the sky, the 4th brightest in Orion, and a blue-white supergiant. It is the middle star of Orion's belt.

Enlarge
Alnilam lights up NGC 1990. Photograph by Glen Youman.

It is also one of the 57 stars used in celestial navigation. For middle latitudes, it is at its highest point in the sky around 10 PM on December 10.


Alnilam's relatively simple spectrum has made it useful for studying the interstellar medium.


Other names and history

The name Alnilam derives from the Arabic Al Nitham or Al Nathm, which translates as "the String of Pearls". Related names also used to describe the star are Alnihan and Alnitam.


Various other names have been used to refer to Orion's belt, the line of three stars formed by Alnitak, Alnilam, and Mintaka. They include:

These stars also influenced the construction of the Pyramids of Giza.




Physical characteristics

Observation data
Right ascension (RA, α) (J2000,00) 05 h 36 m 12.8 s
Declination (Dec, δ) (J2000,00) -01 12' 6.91"
Distance from Earth 1340Ly 500 LY (410 pc)
Visual brightness (V)  +1.70m
Absolute magnitude -6.39m
Physical characteristics
Mean Diameter (dS = 1,392,000 km)
Surface area  
Volume  
Mass
Relative mass to the Sun
(mS = 1.9891 1030 kg)
~ 20 mS
Density  
Surface gravity  
Spectral type B0 Ia (Blue Supergiant)
Surface temperature 11000 K to 25000 K
Age ~ 4 million years
Color (B-V) -0.19 (Blue-white)
V-I
Luminosity (LS = 3.827 1026 J s-1) ~ 23 000 LS
Orbital characteristics
Period of rotation  
Period

Alnilam will eventually turn into red supergiant. Astronomers say that it then explode as a supernova, and this is expected to take place within the next million years. It is surrounded by a molecular cloud, NGC 1990, which it brightens to make a reflection nebula. Its stellar winds may reach up to 2000 km/s, causing it to lose mass about 20 million times more rapidly than the Sun.






  Results from FactBites:
 
Epsilon Orionis - Wikipedia, the free encyclopedia (254 words)
For middle latitudes, it is at its highest point in the sky around 10 PM on December 10.
Alnilam's relatively simple spectrum has made it useful for studying the interstellar medium.
The name Alnilam derives from the Arabic النظام an-niżām, related to the word نظم nażm "string of pearls".
Alnilam (Epsilon Orionis) (217 words)
Alnilam is a blue-white supergiant that for many years has served as a standard star against which to compare others.
Like most supergiants, Alnilam is rapidly shedding mass: a powerful stellar wind blowing from its surface at speeds up to 2,000 km/s and carrying way about two millionths of a solar mass per year (20 million times the rate lost by the Sun).
Though only about four million years old, Alnilam is already fusing heavy elements in its core and doomed to explode, in the next million years or so, as a supernova.
  More results at FactBites »


 

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