Emission nebula in the constellation Orion
IC 434Emission nebula |
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![](//upload.wikimedia.org/wikipedia/commons/thumb/6/68/Barnard_33.jpg/290px-Barnard_33.jpg) IC 434 is found behind the Horsehead Nebula |
Observation data: J2000 epoch |
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Subtype | H II region |
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Right ascension | 05h 40.9m [1] |
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Declination | −02° 27′[1] |
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Distance | 1,260 ly (385 pc)[2] ly |
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Apparent magnitude (V) | 4.5[1] |
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Apparent dimensions (V) | 60′ × 40′[1] |
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Constellation | Orion |
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See also: Lists of nebulae |
IC 434 is a bright emission nebula in the equatorial constellation of Orion. It was discovered on February 1, 1786 by German-British astronomer William Herschel.[2] The nebula is located at a distance of approximately 1,260 ly (385 pc) from the Sun and spans the interior of a neutral hydrogen shell with an angular size of 2° × 4°. At that distance, the dimensions correspond to a projected size of 42 ly × 85 ly (13 pc × 26 pc).[2]
This is an H II region that is being ionized by ultraviolet radiation from the nearby Sigma Orionis (σ Ori) multi-star system. An additional half dozen stars provide further illumination of IC 434. This H II region is one of the youngest to form around members of the Orion OB1 association of hot stars. The region has a radius of about 13 ly (4 pc) and a mass of around ~ 100 M☉ The mass displaced by the advancing ionization front of IC 434 is estimated at 104 M☉.[3] The nebula includes dust with an estimated mass of 2.3 M☉.[2]
IC 434 is surrounded by a shell of neutral hydrogen gas with the identifier GS206-17+13. The primary driving energy behind this expanding shell was likely supplied by the blue supergiant Epsilon Orionis.[2] The Horsehead Nebula is a dark nebula that is silouetted against the diffuse background of IC 434. It is protruding from the Orion B molecular cloud, which is part of the Orion molecular cloud complex.[3]
References
- ^ a b c d Kier, Ruben (2009). The 100 Best Targets for Astrophotography: A Monthly Guide for CCD Imaging with Amateur Telescopes. Springer. p. 31. ISBN 978-1-4419-0603-8.
- ^ a b c d e Ochsendorf, B. B.; Tielens, A. G. G. M. (April 2015). "A bimodal dust grain distribution in the IC 434 H ii region". Astronomy & Astrophysics. 576. id. A2. arXiv:1501.02256. Bibcode:2015A&A...576A...2O. doi:10.1051/0004-6361/201424799.
- ^ a b Bally, John; et al. (February 2018). "Kinematics of the Horsehead Nebula and IC 434 Ionization Front in CO and C+". The Astronomical Journal. 155 (2). id. 80. Bibcode:2018AJ....155...80B. doi:10.3847/1538-3881/aaa248.
External links