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The Crab Nebula is a supernova remnant in the constellation Taurus, formed from a massive star explosion observed in 1054 AD. It contains the Crab Pulsar, a neutron star that emits radiation and powers the nebula, making it significant for astrophysical studies, including the life cycle of stars and particle acceleration. The nebula serves as a cosmic laboratory and is used to calibrate X-ray telescopes due to its strong emissions.

Author

Anindya Biswas

Language

EN