science & techESA/Hubble

The Crab Nebula is the wreck of a star seen exploding in 1054, with a spinning neutron star at its heart

the gist

The Crab Nebula is the wreckage of a star that exploded as a supernova, an event Chinese and other astronomers recorded in 1054. At its centre sits a pulsar, a neutron star so dense that a teaspoon would weigh billions of tonnes, spinning once every 33 milliseconds and sweeping beams of radio waves and visible light like a lighthouse. Fast winds of particles from the pulsar energise the surrounding gas and dust. Combining radio, infrared, optical, ultraviolet and X-ray data reveals different layers of the nebula, about 6500 light-years away in Taurus.

so what

The Crab is one of the best-studied objects in the sky and a benchmark for how supernovae and pulsars work. Showing it in many wavelengths at once reveals structure that no single telescope could capture.

more on this

background

The Crab Nebula (catalogue designations M1, NGC 1952, Taurus A) is a supernova remnant and pulsar wind nebula in the constellation of Taurus. The common name comes from a drawing that somewhat resembled a crab with arms produced by William Parsons, 3rd Earl of Rosse, in 1842 or 1843 using a 36-inch (91 cm) telescope. The nebula was discovered by English astronomer John Bevis in 1731. It corresponds with a bright supernova observed in AD 1054 by Native American, Japanese, and Arab stargazers; this supernova was also recorded by Chinese astronomers as a guest star. The nebula was the first astronomical object identified that corresponds with a historically-observed supernova explosion.

From Wikipedia: Crab Nebula (CC BY-SA 4.0) ↗

ESA/Hubble · CC BY 4.0

Image: NASA, ESA, G. Dubner (IAFE, CONICET-University of Buenos Aires) et al.; A. Loll et al.; T. Temim et al.; F. Seward et al.; VLA/NRAO/AUI/NSF; Chandra/CXC; Spitze