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Nebulae · Lyra

Ring Nebula

NGC 6720 · M57

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Details

Magnitude

8.80

Angular size

1.4′ × 1′

Messier

M57

NGC

6720

What you can realistically expect

A small faint grey smoke-ring in a small scope; the ring shape is obvious at 100× or more. Colour is not visible visually. An OIII filter darkens the background.

A tiny smoke-ring in Lyra — the classic amateur planetary nebula.

Intermediate

What is it?

The Ring Nebula is a planetary nebula: gas ejected by a dying star, glowing under the ultraviolet light of the tiny hot remnant at its centre. It lies about 2,300 light-years away.

What will I see?

Binoculars

A tiny fuzzy 'star' — difficult to identify without knowing exactly where to look.

Small telescope

A small but distinctly ring-shaped smoke ring at moderate magnification. Central hole is visible.

Medium telescope

The ring's shape is unmistakable. Very hard to detect the extremely faint central star visually.

Astrophotography

Photography

Photographs reveal delicate structure and colour: blue-green in the interior, red-pink at the edges.

Reference imagery from long-exposure photography usually shows far more colour and structure than the human eye can see through a telescope.

Reference image

Processed image
Reference image of the Ring Nebula (M57) from Hubble, showing the classic ring-shaped shell of gas from a dying star

NASA, ESA and the Hubble Heritage (STScI/AURA)-ESA/Hubble Collaboration · NASA Science / Hubble Messier catalog

Long-exposure or processed astronomy images can show much more colour and structure than you may see through an eyepiece.

Observing tips

  • Use higher magnification than typical for deep-sky objects — the nebula is small.
  • An O-III filter dramatically improves visibility under light-polluted skies.
  • Located between the two southern stars of Lyra's parallelogram.

Interesting facts

  • About 1 light-year across.
  • The central star will eventually cool into a white dwarf.
Ring Nebula (M57): Observing Guide | Starbital