Horsehead Nebula
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The Horsehead Nebula (also known as Barnard 33 or B33) is a small dark nebula located about 1,375 light-years (422 pc)[1][2] from Earth in the constellation of Orion.[3] The nebula is located just to the south of Alnitak, the easternmost star of Orion's Belt, and is part of the much larger Orion molecular cloud complex. It appears within the southern region of the dense dust cloud known as Lynds 1630, along the edge of the much larger, active star-forming H II region called IC 434.[2] It is one of the most identifiable nebulae because of its resemblance to a horse's head.[4]
History
The nebula was discovered by Scottish astronomer Williamina Fleming in 1888 on a photographic plate taken at the Harvard College Observatory.[5][6] One of the first descriptions was made by E. E. Barnard, describing it as: "Dark mass, diam. 4′, on nebulous strip extending south from ζ Orionis", cataloguing the dark nebula as Barnard 33.[7]
Structure
It has an easily recognizable shape which resembles the head of a horse. Heavy concentrations of dust in the Horsehead Nebula region and the neighbouring Orion Nebula are localized into interstellar clouds resulting in alternating sections of nearly complete opacity and transparency.[8] The darkness of the Horsehead is caused mostly by thick dust blocking the light of stars behind it.[9] The lower part of the Horsehead's neck casts a shadow to the left.[10] The visible dark nebula emerging from the gaseous complex is an active site of the formation of "low-mass" stars. Bright spots in the Horsehead Nebula's base are young stars just in the process of forming.
The dark cloud of dust and gas is a region in the Orion molecular cloud complex, where star formation is taking place. It is located in the constellation of Orion, which is prominent in the winter evening sky in the Northern Hemisphere and the summer evening sky in the Southern Hemisphere.
Colour images reveal a red colour that originates from ionised hydrogen gas (Hα) predominantly behind the nebula, and caused by the nearby bright star Sigma Orionis. Magnetic fields channel the gases, leaving the nebula into streams, shown as foreground streaks against the background glow.[11] A glowing strip of hydrogen gas marks the edge of the enormous cloud, and the densities of nearby stars are noticeably different on either side.
See also
Notes
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References
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External links
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- SOFIA/upGREAT [C II] Velocity Resolved Map of the Horsehead Nebula
- The Horsehead Nebula @ The Electronic Sky
- Hubble Observes the Horsehead Nebula
- The discovery of early photographs of the Horsehead nebula, by Waldee and Hazen
- The Horsehead Nebula in the 19th Century, by Waldee
- Detection of new nebulae by photography, by Pickering
- Horsehead Nebula at ESA/Hubble
- The Horsehead Nebula at the Astro-Photography site of Mr. T. Yoshida.
- The Horsehead-Nebula and neighboring structures in a classical view
- The Horsehead Nebula on interactive astro-photography survey at Wikisky.org
- The Horsehead Nebula at Constellation Guide
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