Chinese Astronomers Record Bright Supernova in Taurus

Summary

In the Song Dynasty capital of Kaifeng, court astronomers maintained detailed celestial logs of temporary 'guest stars.' On the morning of July 4, 1054, they noted a brilliant new object several degrees southeast of Zeta Tauri in the constellation Taurus. The star shone brightly enough to be visible in daylight for 23 days, rivaling Venus in intensity and appearing yellow at first. Contemporary records in the Sung-shih describe its gradual fading over the following months until it disappeared from view in April 1056 after roughly 653 days of naked-eye visibility. Modern astronomy identifies this event as the supernova SN 1054, whose remnant is the Crab Nebula, a pulsar-powered cloud of gas expanding at thousands of kilometers per second. The precise Chinese documentation provided one of the earliest reliable records of a galactic supernova visible from Earth.