Horsehead Nebula
From Wikipedia, the free encyclopedia
| Dark nebula | Lists of nebulae |
|---|---|
| Horsehead Nebula. | |
| Observation data (Epoch J2000.0) |
|
| Type | Dark |
| Right ascension | 05h 40m 59.0s |
| Declination | -02° 27′ 30.0" |
| Distance | 1,500 ly |
| Apparent magnitude (V) | - |
| Apparent dimensions (V) | 8 × 6 arcmins |
| Constellation | Orion |
| Physical characteristics | |
| Radius | - |
| Absolute magnitude (V) | - |
| Notable features | - |
| Other designations | IC 434, Barnard 33, LDN 1630, M3T 31, [OS98] 52 |
| edit | |
The Horsehead Nebula (also known as Barnard 33' in bright nebula IC 434) is a dark nebula in the Orion constellation. The nebula is located just below Alnitak, the easternmost star of Orion's Belt, and is part of the much larger Orion Molecular Cloud Complex. It is approximately 1,500 light years from Earth, and is approximately 3.5 light years wide.
One of the most identifiable nebulae in the sky, it is part of a swirling cloud of dark dust and gases, shaped like a horse's head (hence its name). Also known as Barnard 33, the unusual shape was first discovered in 1888 by Mrs. Williamina Fleming on photographic plate B2312 taken at the Harvard College Observatory.
The red 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.
