NGC 7027

1,890 billion kmmaximum extent

Updated

1,890billion km0.20ly
Visual creditHubble 2020 / NASA, ESA, and J. Kastner (RIT) / CC BY 2.0Source: Wikimedia Commons

Details

NGC 7027 is a young planetary nebula in Cygnus with a compact bright inner region wrapped in fainter outer shells of gas. Recent Hubble observations show a remnant still changing shape, where newer, more directed outflows are running into older material shed by the dying central star.

NGC 7027 is a young planetary nebula with a bright, compact inner region surrounded by fainter shells of material expelled earlier by its central star. Its maximum visible extent depends on which outer emission is included, so the 0.2-light-year value is a boundary of the imaged structure rather than a solid edge.

Hubble observations reveal narrow outflows cutting through the older envelope. Their collisions with previously shed gas help explain why the nebula is asymmetric and still changing instead of forming a single smooth shell.

Key facts

Category
Nebulae
Object class
Planetary nebula
Host
Milky Way
Scale fact
1,890 billion km0.2 lymaximum extent
Composition
Gas, dust, and stellar ejecta
Embed

Size neighbors

Objects near NGC 7027 on the scale

On the logarithmic size axis, NGC 7027 falls between Phoenix A* and Cat's Eye Nebula. The band uses nearby Planetary nebula records.

Shared physical scale
4.28ly
NGC 70271,890 billion km
Cat's Eye Nebula3,800 billion km
Ring Nebula2.6 ly
Helix Nebula5.6 ly

Sources

References for NGC 7027

Measurements and descriptive context are compiled by the Scale of Space team from the references below. If you find an error, please let us know.

Continue with nearby objects or open the full scale.

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