Cat's Eye Nebula

3,800 billion kmmaximum extent

Updated

3,800billion km0.40ly
Visual creditHubble 2026 / ESA/Hubble & NASA, Z. Tsvetanov / CC BY 4.0Source: Wikimedia Commons

Details

The Cat's Eye Nebula is a planetary nebula in Draco whose bright inner core folds shells, jets, and dense knots around a dying central star. Hubble resolves that compact center as a layered record of repeated mass loss, distinct from the much fainter halo beyond it.

The Cat's Eye Nebula contains nested shells, knots and jets around the exposed core of a dying star. The bright inner region spans about 0.4 light-years, while a much fainter halo extends farther and is not included in this record's displayed size.

The overlapping structures trace separate episodes of mass loss. Later, faster winds ran into older material, compressing and reshaping it rather than producing one uniformly expanding sphere.

Key facts

Category
Nebulae
Object class
Planetary nebula
Host
Milky Way
Scale fact
3,800 billion km0.4 lymaximum extent
Composition
Ionized gas, dust, stellar ejecta
Temperature
~8,000 K ionized gas
Embed

Size neighbors

Objects near Cat's Eye Nebula on the scale

On the logarithmic size axis, Cat's Eye Nebula falls between NGC 7027 and Homunculus 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 Cat's Eye Nebula

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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