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SN 1054 and the Crab Nebula

1054MajorContested

A guest star appears near Tianguan in July 1054, bright enough to see by day for 23 days. Its remnant is the Crab Nebula, and a pulsar spins at its core.

The story

On July 4, 1054, Chinese astronomers in the Song capital noted a guest star near the star Tianguan, in the constellation Taurus. Official records say it was visible in daylight for 23 days and in the night sky for 653 days, until April 1056. Japanese sources also mention it, and some scholars think Arab observers did, but no clear European record has been found. To Chinese court astronomers it was an omen to be reported to the emperor.

Centuries later, in 1731, John Bevis found a faint nebula at the same place. In 1758 Charles Messier, hunting for Halley's Comet, mistook it for a comet and decided to list such objects so no one else would be fooled, making it the first entry in his catalog, M1. In 1844 Lord Rosse sketched it with tentacles and called it the Crab. In the 1920s astronomers measured that the Crab was expanding, and wound the motion back to about 900 years, pointing to 1054. In 1942 Jan Oort and Nicholas Mayall confirmed the link, and in 1968 radio astronomers found a pulsar in the Crab, a rapidly spinning neutron star left by the exploded star.

The explosion was a core-collapse supernova, the death of a massive star. The Crab is now one of the most studied objects in the sky and a standard calibration source for X-ray telescopes. It is also the clearest case where an ancient record, a nebula and a collapsed star all trace back to the same event.

Why it mattered

  • Proved that a historical guest star could be matched to a modern remnant, setting a method for dating supernova remnants.
  • Led to the identification of pulsars as spinning neutron stars, via the Crab pulsar found in 1968.
  • Inspired Messier's catalog, which began with the Crab Nebula, M1.
  • Made the Crab a standard light source that astronomers use to calibrate X-ray and gamma-ray instruments.

Contested history

Consensus: Chinese and Japanese records describe a supernova in 1054, and the Crab Nebula and its pulsar are its remnant; a few other claims about the star are less secure.

The Crab Nebula is the remnant of the 1054 supernovaEstablished
Its measured expansion, the position match and the pulsar all point to the Chinese record.
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Native American rock art at Chaco Canyon records the starSpeculation
A crescent and star image is suggestive, but it cannot be dated to 1054 or tied to the event.
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Europeans did not record it because of clouds or doctrineSpeculation
The absence of European records is real, but no study has shown whether weather, belief or poor survival explains it.
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