Celestial hemisphere:  Northern  ·  Constellation: Lyra (Lyr)  ·  Contains:  IC 1296  ·  M 57  ·  NGC 6720  ·  Ring Nebula
M57 Ring Nebula, Joe Niemeyer
M57 Ring Nebula
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M57 Ring Nebula

M57 Ring Nebula, Joe Niemeyer
M57 Ring Nebula
Powered byPixInsight

M57 Ring Nebula

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This my image of the Ring Nebula (M57). It is in a class of deep sky objects called planetary nebulae. The term is a misnomer because they are totally unrelated to planets. The term originates from the planet-like round shape of these nebulae observed by astronomers through early telescopes. Such a nebula is formed when a medium-size star expels ionized gas during the last stages of its life before becoming a white dwarf. You can see the tiny white dwarf star in the center of this nebula surrounded by colorful gases it cast off thousands of years ago. Our own Sun will eventually meet the same fate as its hydrogen is consumed in the course of billions of years of nuclear fusion. It's been nice knowing you! 

M57 is about a light-year in diameter and is located some 2,500 light-years from Earth in the direction of the constellation Lyra below the bright star Vega. The deep blue central color is from very hot helium; the blue/green is from ionized oxygen; and the orange/red is from ionized nitrogen. These gases glow as they are bathed in ultraviolet radiation from the remnant central star, whose surface temperature is a white-hot 120,000 degrees Celsius. There is a bonus near the bottom of this image -- the barred spiral galaxy IC 1296.

I made this image from a stack of sixteen 300-second exposures shot at 2310mm focal length, calibrated with 20 each dark, flat, and dark flat frames. I highly cropped the image since the disk of M57 is only about one arcminute in size and then post-processed it with Photoshop, StarNet++, and DeNoise AI.

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M57 Ring Nebula, Joe Niemeyer