Expanding wreckage of a supernova recorded in AD 1054, with the Crab Pulsar at its centre.
Worth knowing about the Crab Nebula
You see the Crab Nebula as it was about 6,200 years ago.
What it is
The expanding wreckage of a massive star’s supernova, gas still blasting outwards at thousands of km/s, with the Crab Pulsar left at its centre.
How we know: Photographs decades apart show the gas visibly spreading; run the expansion backwards and it starts around AD 1130 — close to 1054, and the gap shows the gas has been speeding up, pushed by the pulsar’s wind.
Its name and its story
Recorded by Chinese, Japanese and Arab astronomers in AD 1054 as a “guest star” visible in daylight for weeks. A Chaco Canyon petroglyph is a debated possible Native American record.
The numbers
Across
about 11 light-years
Distance from us
about 6,200 light-years
How big it looks
about 6 arcminutes — the full Moon is about 30
We use about 6,200 light-years, from a radio parallax of the pulsar at its centre (Lin et al. 2023). The long-quoted 6,500 is the older 2.0 kiloparsecs.