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Epsilon Orionis
Epsilon Orionis
Alnilam lights up NGC 1990.
Photograph by Glen Youman.
Observation data
Epoch J2000      Equinox J2000
Constellation Orion
Right ascension 05h 36m 12.8s
Declination −01° 12′ 06.9″
Apparent magnitude (V) 1.70
Characteristics
Spectral type B0 Iab
U-B color index −1.03
B-V color index −0.19
Variable type Alp Cyg
Astrometry
Radial velocity (Rv) 25.9 km/s
Proper motion (μ) RA: 1.49 mas/yr
Dec.: −1.06 mas/yr
Parallax (π) 2.43 ± 0.91 mas
Distance approx. 1300 ly
(approx. 400 pc)
Absolute magnitude (MV) −6.4
Details
Mass 40 M
Radius 26 R
Luminosity 375,000 L
Temperature 25,000 K
Metallicity ?
Rotation ~87 km/s
Age 4,000,000 years
Other designations
Alnilam, Alnihan, Alnitam, 46 Orionis, HR 1903, BD -01°969, HD 37128, SAO 132346, FK5 210, HIP 26311, TD1 4963.
Database references
SIMBAD data

Alnilam is a large blue star in the constellation of Orion. It also has the modern name Epsilon Orionis (ε Ori / ε Orionis). Its Flamsteed designation is 46 Orionis.

It is the 30th brightest starrr in the sky (the 4th brightest in Orion) and as a blue-white supergiant it is the most powerful bright star in the sky. Together with Mintaka (Delta Orionis) and Alnitak (Zeta Orionis), the three stars make up the belt of Orion, known by many names across many ancient cultures. Alnilam is the middle star.

It is also one of the 57 stars used in celestial navigation. It is at its highest point in the sky around midnight on December 15.

Alnilam's relatively simple spectrum has made it useful for studying the interstellar medium. Within the next million years, this star may turn into a red supergiant and explode as a supernova. 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.

Contents

Other names and history

The name Alnilam derives from the Arabic النظام an-niżām, related to the word نظم nażm "string of pearls". Related spellings are Alnihan and Alnitam:[1] all three variants are evidently mistakes in transliteration or copy errors.

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Orion's belt

The three belt stars were collectively known by many names in many cultures. Arabic terms include Al Nijād 'the Belt', Al Nasak 'the Line', Al Alkāt 'the Golden Grains or Nuts' and, in modern Arabic, Al Mīzān al H•akk 'the Accurate Scale Beam'. In Chinese mythology they were also known as The Weighing Beam.[1] The belt was also the Three Stars mansion (simplified Chinese: 参宿traditional Chinese: 參宿pinyin: Shēn Xiù), one of the Twenty-eight mansions of the Chinese constellations. It is one of the western mansions of the White Tiger.

In pre-Christian Scandinavia, the belt was known as Frigg's Distaff (Friggerock) or Freyja's distaff[2]. Similarly Jacob's Staff and Peter's Staff were European biblical derived terms, as were the Three Magi, or the Three Kings. Väinämöinen's Scythe (Kalevala) and Kalevan Sword are terms from Finnish mythology.[1]

The Seri people of northwestern Mexico call the three belt stars Hapj (a name denoting a hunter) which consists of three stars: Hap (mule deer), Haamoja (pronghorn), and Mojet (bighorn sheep). Hap is in the middle and has been shot by the hunter; its blood has dripped onto Tiburón Island.[3]

References

  1. ^ a b c Richard Hinckley Allen, Star-names and their meanings (1936), p. 314-15.
  2. ^ Schön, Ebbe. (2004). Asa-Tors hammare, Gudar och jättar i tro och tradition. Fält & Hässler, Värnamo. p. 228.
  3. ^ Moser, Mary B.; Stephen A. Marlett (2005) (in Spanish and English). Comcáac quih yaza quih hant ihíip hac: Diccionario seri-español-inglés. Hermosillo, Sonora and Mexico City: Universidad de Sonora and Plaza y Valdés Editores. http://lengamer.org/admin/language_folders/seri/user_uploaded_files/links/File/DiccionarioSeri2005.pdf. 

See also

External links


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