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Alnilam

HIP 26311; Epsilon Ori; 46 Ori

HIP 26311; Epsilon Ori; 46 Ori DoubleStar Ori Visible Level 3 Medium telescope (6-8") - Requires steady seeing
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Physical Properties

Magnitude 1.70
Spectral Type B0Ib
Star Color Blue (B-V -0.19)
Temperature 27526 K
Radius 32.4 R☉
Distance 1341.2 ly

Position & Identifiers

RA 05h 36m 12.8s
Dec -01° 12' 07.0"
Constellation Ori
HR 1903
HIP 26311
Bayer Epsilon
Flamsteed 46 Ori
Variable ID f

Visibility

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Multiple Star System

Separation 179.5″
Companion Mag 11.3
Position Angle 58°
Star Colors A: Blue
Discoverer BUP 81

Eyepiece View

32x Dawes: 1.9″ TFOV: 1.6°
Realistic = true angular size
N E 58° A (1.7) B (11.3)

Sep: 179.5″ · PA: 58° · N up, E left

Resolved · Rayleigh: 2.3″ · Dawes: 1.9″ · Eff: 3.1″

Size Comparison

Stellar Lifecycle

Spectral Classification

Hertzsprung-Russell Diagram

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Blackbody Spectrum

Stellar Absorption Spectrum

Simulated absorption spectrum based on spectral type. Hover over lines to identify elements.

Stellar Notes

Alpha Cyg 1.64 - 1.74V.
In both infrared survey and UV CELESCOPE. Color excess E(B-V) = +0.08.
Ori OB1b2; Orion belt; cluster NGC 1980; nebulosity.
Nitrogen deficient. Interstellar Lyman alpha absorption observed by AEROBEE rocket. Walborn declares "no e", but | Merrill found H alpha emission.
UV AEROBEE spectra indicate mass ejection at velocity up to 1800k/s.
ALNILAM; Alnihan; Alnitam.
Diam. = 0.00067 - 0.00069".

Survey Image

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About Alnilam

Description

Alnilam is a blue supergiant of spectral type B0Ia, the middle and brightest star of Orion's Belt at magnitude 1.70. Located about 2,000 light-years from Earth, it is one of the most distant bright stars visible to the naked eye. Alnilam is extraordinarily luminous — roughly 275,000 times the luminosity of the Sun — and has about 40 times the Sun's mass. It is losing mass rapidly through powerful stellar winds.

Observing Tips

Alnilam is the middle star of Orion's famous Belt, flanked by Alnitak to the east and Mintaka to the west. The three Belt stars are one of the most recognizable patterns in the night sky. Through binoculars, the surrounding region is rich with nebulosity — the emission nebula NGC 1990 surrounds Alnilam itself. The Belt points downward to Sirius and upward to Aldebaran, making it an excellent starting point for star-hopping. Best observed from November through March.

History

The name Alnilam comes from the Arabic 'al-Nilam' meaning 'string of pearls,' referring to the line of Belt stars. Orion's Belt is one of the most universally recognized star patterns across human cultures — it has been identified with three kings, three sisters, a celestial bridge, and many other mythological figures worldwide. The ancient Egyptians aligned the three Great Pyramids of Giza to mirror the Belt stars.

Fun Facts

At roughly 275,000 solar luminosities, Alnilam is one of the most luminous stars known in the Milky Way. Its powerful stellar wind blows at over 2,000 km/s, and it is losing mass at a rate millions of times greater than the Sun's solar wind. The alignment of the three Pyramids of Giza with Orion's Belt (the Orion Correlation Theory) is one of the most popular — and debated — claims in archaeoastronomy.