The Reflection Nebula around the Trifid Nebula
AAO image reference UKS 7.    « Previous || Next »

The Reflection Nebula around the Trifid Nebula, M20, NGC 6514
Top left is NE. Image width is about 30 arc min
Image and text © 1979-2002, Anglo-Australian Observatory/Royal Obs. Edinburgh.
Photograph from UK Schmidt plates by David Malin.


The Trifid Nebula is a fine example of an object which combines emission and reflection nebulosity. The striking red emission nebula surrounds a small group of very hot stars. Energetic radiation from these stars causes part of the enveloping but otherwise invisible hydrogen cloud to fluoresce and emit its characteristic monochromatic red light. Beyond the limits of the emission nebula sufficient starlight escapes at longer wavelengths for it to be scattered by the dust grains associated with the gas. The scattering produces a faint blue reflection nebula around the irregular sphere of red emission. To the north, a star which is too cool to create an emission nebula is embedded in its own hazy blue reflection.

Related images
AAT 12.   The Trifid nebula, Messier 20
AAT 12a. The Trifid nebula, Messier 20 (wide field)
AAT 69.   Reflection nebula around M20
AAT 69a. Reflection nebula around M20 (wide field)
AAT 30.   The stars that excite the Trifid nebula
UKS 26.  The field of M8 and M20 in Sagittarius

For details of object position and photographic exposure, search technical table by UKS reference number.


galaxies | emission neb. | reflection neb. | dark neb. | planetaries | clusters | stars | supernovae
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