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emission nebula

noun

Astronomy.
  1. a bright diffuse nebula that emits light as a result of ionization of its gas atoms by ultraviolet radiation, as the Orion Nebula, planetary nebulae, and supernova remnants, as the Crab Nebula.


emission nebula

noun

  1. a type of nebula that emits visible radiation See nebula
“Collins English Dictionary — Complete & Unabridged” 2012 Digital Edition © William Collins Sons & Co. Ltd. 1979, 1986 © HarperCollins Publishers 1998, 2000, 2003, 2005, 2006, 2007, 2009, 2012

emission nebula

/ ĭ-ĭə /

  1. A nebula that absorbs ionizing ultraviolet radiation from nearby hot stars or star remnants and reemits it as visible light. HII regions , planetary nebulae , and nebulae created by the explosion of supernovae are different kinds of emission nebulae.
  2. See more at nebula
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Example Sentences

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This image features the California Nebula - also known as NGC 1499 - an emission nebula in the constellation of Perseus.

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Known as the Bubble Nebula, or NGC 7635, it is an emission nebula located 8 000 light-years away; emission nebulas are interstellar clouds which are comprised of ionized gases.

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The Bubble Nebula, also known as NGC 7635, is an emission nebula located 8 000 light-years away.

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The Flame Nebula, designated as NGC 2024 and Sh2-277, is an emission nebula in the constellation Orion, lying some 900 to 1,500 light years away from Earth.

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