Celestial hemisphere:  Northern  ·  Constellation: Lyra (Lyr)  ·  Contains:  IC 1296  ·  M 57  ·  NGC 6720  ·  PK063+13.1  ·  Ring nebula  ·  Ring nebula in Lyra
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The Ring Nebula: M57, Richard Francis
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The Ring Nebula: M57

Getting plate-solving status, please wait...
The Ring Nebula: M57, Richard Francis
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The Ring Nebula: M57

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Description

The Ring Nebula is a so-called Planetary Nebula, called this because their relatively small, round shapes can be confused for planets. In fact they are the expanding gas shells, roughly spherical, of exploded stars. In this case the shells is not symmetric and has an equatorial bulge, so it appears elliptical as we see it. The "crust" of the shell of expanding material is denser than the interior so it takes the form of a ring with a "hollow" interior -- it's not really hollow but the optical depth of material is less than at the edge. It's estimates that the ring has been expanding for just over 1600 years. The central star, a white dwarf, which can be seen in this image, has magnitude 14.8 and difficult to see visually, though the first reported observation dates back to 1800.

The Ring Nebula is about 2300 light years away and is a popular object in small telescopes.

This image is part of the on-going commissioning process of my observatory. In particular the scope collimation is not yet adequate and close examination will show the stars have a consistent elongated shape. What's more, my auto guiding still has unacceptable random errors. Finally, the image is a bit over-processed

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The Ring Nebula: M57, Richard Francis