Alnilam (Epsilon Orionis)
Alnilam (Epsilon Orionis) is the central and brightest of the three stars in Orion's
Belt and the fourth brightest star in the whole of Orion.
Alnilam is a blue-white supergiant that
for many years has served as a standard star against which to compare others.
Its relatively simple spectrum also provides a useful background against
which to study the gases of the intervening interstellar
|Alnilam and surrounding nebulosity. Photo: Glen Youman
|To the left is Alnilam. Below it and next to the Horsehead Nebula is Alnitak.
In the upper right is the Orion Nebula.
Photo: Robert Gendler
Like most supergiants, Alnilam is rapidly shedding mass. A powerful stellar
wind blows from its surface at speeds up to 2,000 km/s, carrying way
about two millionths of a solar mass per year (20 million times the rate
lost by the Sun). Although only about four million years old, Alnilam is
already fusing heavy elements in its core and is doomed to explode, in the
next million years or so, as a supernova.
A molecular cloud, NGC 1990, surrounds Alnilam and is partly illuminated
as a reflection nebula by the star's
||1,300 light-years (400 pc)
||R.A. 05h 36m 12.8s,
Dec. -01° 12' 07"
||Alnihan, Alnitam, 46 Orionis,
HR 1903, BD -01°969, HD 37128,
SAO 132346, FK5 210, HIP 26311
• NOTABLE STARS