Read Next
Discover
emission nebula
astronomy
verifiedCite
While every effort has been made to follow citation style rules, there may be some discrepancies.
Please refer to the appropriate style manual or other sources if you have any questions.
Select Citation Style
Feedback
Thank you for your feedback
Our editors will review what you’ve submitted and determine whether to revise the article.
External Websites
emission nebula, in astronomy, a bright, diffuse light sometimes associated with stars whose temperatures exceed 20,000 K. The excitation process necessary to provide observed optical and radio energies in such gaseous regions was long an astronomical puzzle. It was found that ultraviolet light from the star ionizes nearby hydrogen. The hydrogen atoms emit visible light after the electrons and nuclei recombine and the atoms drop to lower energy levels.