Crab Nebula

11 lydiameter

Updated

11.0ly
Visual creditNASA's Great Observatories 2006 / X-ray: NASA/CXC/J. Hester (ASU); Optical: NASA/ESA/J. Hester & A. Loll (ASU); Infrared: NASA/JPL-Caltech/R. Gehrz (Univ. Minn.) / Public domainSource: Wikimedia Commons

Details

The Crab Nebula is the expanding supernova remnant created by the stellar explosion recorded in 1054. Its tangled filaments are still being energized from within by the Crab Pulsar, the neutron star left by the explosion.

Astronomers in 1054 recorded the new star whose debris we now call the Crab Nebula. Nearly a millennium later, repeated images still show its gas and dust expanding, so the historical observation and the changing remnant can be studied as one event across time.

At the center, the Crab Pulsar rotates about 30 times per second and drives a wind of high-energy particles. Its synchrotron emission fills the interior, while filaments trace material expelled by the supernova. The nebula is therefore both explosion debris and a pulsar-powered system.

Key facts

Category
Nebulae
Object class
Supernova remnant
Composition
Ionized gas and supernova ejecta
Scale fact
11 lydiameter
Estimated age
~970 years
Embed

Size neighbors

Objects near Crab Nebula on the scale

On the logarithmic size axis, Crab Nebula falls between Helix Nebula and Orion Nebula. The band uses nearby Nebulae records.

Shared physical scale
230ly

Sources

References for Crab 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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