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IC 434
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{{Short description|Emission nebula in the constellation Orion}} {{Infobox nebula | name = IC 434 | image = Barnard 33.jpg | image_scale = 1.3 | alt = | caption = IC 434 is found behind the [[Horsehead Nebula]] | credit = <!-- Per MOS:CREDITS, credits are discouraged --> | type = emission | type2 = <!-- can be wikilinked --> | epoch = [[J2000]] | subtype = H II region | class = | constellation = [[Orion (constellation)|Orion]] | ra = {{RA|05|40.9}}<ref name=Ruben_2009/> | dec = {{DEC|−02|27}}<ref name=Ruben_2009/> | dist_ly = {{cvt|385|pc|ly|order=flip}}<ref name=Ochsendorf_Tielens_2015/> | dist_pc = | dist_z = | appmag_v = 4.5<ref name=Ruben_2009/> | appdia = <!-- dd°mm'ss".mas --> | size_v = {{val|60|×|40|ul=arcminute}}<ref name=Ruben_2009/> | radius_ly = | radius_pc = | dimensions = | absmag_v = | notes = | names = }} '''IC 434''' is a bright [[emission nebula]] in the equatorial [[constellation]] of [[Orion (constellation)|Orion]]. It was discovered on February 1, 1786, by German-British astronomer [[William Herschel]].<ref name=Ochsendorf_Tielens_2015/> The nebula is located at a distance of approximately {{cvt|385|pc|ly|order=flip}} from the Sun and spans the interior of a [[neutral hydrogen]] shell with an [[angular size]] of {{val|2|×|4|u=°}}. At that distance, the dimensions correspond to a projected size of {{cvt|13|×|26|pc|ly|order=flip}}.<ref name=Ochsendorf_Tielens_2015/> This is an [[H II region]] that is being [[Ionization|ionized]] by [[Ultraviolet astronomy|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 {{cvt|4|pc|ly|order=flip}} and a mass of around {{val|100|ul=Solar mass|p=~ }} The mass displaced by the advancing ionization front of IC 434 is estimated at {{val|e=4|u=Solar mass}}.<ref name=Bally_et_al_2018/> The nebula includes [[Cosmic dust|dust]] with an estimated mass of {{val|2.3|u=Solar mass}}.<ref name=Ochsendorf_Tielens_2015/> 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]].<ref name=Ochsendorf_Tielens_2015/> The [[Horsehead Nebula]] is a [[dark nebula]] that is silhouetted 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]].<ref name=Bally_et_al_2018/> ==References== {{reflist|refs= <ref name=Bally_et_al_2018>{{cite journal | title=Kinematics of the Horsehead Nebula and IC 434 Ionization Front in CO and C+ | last1=Bally | first1=John | last2=Chambers | first2=Ed | last3=Guzman | first3=Viviana | last4=Keto | first4=Eric | last5=Mookerjea | first5=Bhaswati | last6=Sandell | first6=Goran | last7=Stanke | first7=Thomas | last8=Zinnecker | first8=Hans | display-authors=1 | journal=The Astronomical Journal | volume=155 | issue=2 | at=id. 80 | date=February 2018 | doi=10.3847/1538-3881/aaa248 | doi-access=free | bibcode=2018AJ....155...80B }}</ref> <ref name=Ochsendorf_Tielens_2015>{{cite journal | title=A bimodal dust grain distribution in the IC 434 H ii region | last1=Ochsendorf | first1=B. B. | last2=Tielens | first2=A. G. G. M. | journal=Astronomy & Astrophysics | volume=576 | at=id. A2 | date=April 2015 | doi=10.1051/0004-6361/201424799 | arxiv=1501.02256 | bibcode=2015A&A...576A...2O }}</ref> <ref name=Ruben_2009>{{cite book | title=The 100 Best Targets for Astrophotography: A Monthly Guide for CCD Imaging with Amateur Telescopes | first=Ruben | last=Kier | year=2009 | page=31 | publisher=Springer | isbn=978-1-4419-0603-8 | url=https://books.google.com/books?id=fCIYe_NZV08C&pg=PA31 }}</ref> }} ==External links== * {{cite APOD |date=21 February 2006 |title=Wisps Surrounding the Horsehead Nebula}} * [http://www.glyphweb.com/esky/nebulae/ic434.html IC 434] * {{cite simbad|title=IC 434}} {{Stars of Orion}} [[Category:Emission nebulae]] [[Category:IC objects|0434]] [[Category:Orion (constellation)]] [[Category:Orion molecular cloud complex]]
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