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Epsilon Orionis
From Wikipedia, the free encyclopedia
| Observation data Epoch J2000 |
|
|---|---|
| Constellation (pronunciation) |
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 × 106 years |
| Other designations | |
| Database references | |
| SIMBAD | data |
Epsilon Orionis (ε Ori / ε Orionis) is a large blue star in the constellation of Orion. It also has the traditional name Alnilam. Its Flamsteed designation is 46 Orionis.
It is the 30th brightest star in the sky (the 4th brightest in Orion) and as a blue-white supergiant it is one of the most luminous stars known. It is the middle star of Orion's belt.
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 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.
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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.
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 (traditional Chinese: 參宿; simplified Chinese: 参宿; 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]
These stars also allegedly influenced the construction of the Pyramids of Giza.
- ^ a b c Richard Hinckley Allen, Star-names and their meanings (1936), p. 314-15.
- ^ Schön, Ebbe. (2004). Asa-Tors hammare, Gudar och jättar i tro och tradition. Fält & Hässler, Värnamo. p. 228.
- ^ Moser, Mary B.; Stephen A. Marlett (2005). Comcáac quih yaza quih hant ihíip hac: Diccionario seri-español-inglés (in Spanish and English). Hermosillo, Sonora and Mexico City: Universidad de Sonora and Plaza y Valdés Editores.