Horsehead Nebula

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Horsehead Nebula
ESO-Horsehead Nebula.jpg
Observation data (Epoch J2000.0)
Type dark nebula/diffuse nebulae
Right ascension 05h 40m 59.0s
Declination −02° 27′ 30.0"
Distance (ly) 1,500 ly
Apparent dimensions (V) 8 × 6 arcmins
Constellation Orion
Physical characteristics
Notable features Resembles a horse's head
Other designations IC 434, Barnard 33,
LDN 1630, M3T 31,
[OS98] 52
See also: Dark nebula, Lists of nebulae

The Horsehead Nebula (also known as Barnard 33 in emission nebula IC 434) is a dark nebula in the constellation Orion.[1] The nebula is located just to the south of the star Alnitak, which is farthest east on Orion's Belt, and is part of the much larger Orion Molecular Cloud Complex. The nebula was first recorded in 1888 by Williamina Fleming on photographic plate B2312 taken at the Harvard College Observatory. The Horsehead Nebula is approximately 1500 light years from Earth. It is one of the most identifiable nebulae because of the shape of its swirling cloud of dark dust and gases, which is similar to that of a horse's head when viewed from Earth. [2]

The red or pinkish glow originates from hydrogen gas predominantly behind the nebula, ionized by the nearby bright star Sigma Orionis. The darkness of the Horsehead is caused mostly by thick dust, although the lower part of the Horsehead's neck casts a shadow to the left. Streams of gas leaving the nebula are funneled by a strong magnetic field. Bright spots in the Horsehead Nebula's base are young stars just in the process of forming.

[edit] External links

Media related to Horsehead Nebula at Wikimedia Commons

[edit] References

  1. ^ Arnett, Bill. http://astro.nineplanets.org/twn/b33x.html. Horsehead Nebula, 2000
  2. ^ Sharp, Nigel/NOAO. http://www.noao.edu/image_gallery/html/im0057.html.
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