M57 - Ring Nebula




M57 is a planetary nebula, so named because in a small telescope the disk resembles a planet. The material forming the nebula has been ejected from the central star and is slowly moving outward. This gas is energized by the hot central star (notice it is blue in colour) and radiates at a variety of wavelengths, hence the multiple colours.

You may have to adjust your monitor's brightness and contrast to get the best view.
 

This image is a composite of three individual exposures, each taken through a different coloured filter. The size and structure of the gas is very different at different wavelengths as is the brightness of the central star....

Individual exposures through the red, green and blue filters

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