The Vela Pulsar is a neutron star located in the Vela constellation, about 1,000 light-years from Earth. It is the remnant of a supernova that occurred around 11,000 years ago. The Vela Pulsar is known for its rapid rotation, spinning approximately 11 times per second, and emits powerful beams of radio waves and X-rays, which are observed as regular pulses. This makes it one of the most well-studied and brightest pulsars in the sky. Its study provides valuable insights into the nature of neutron stars and the aftermath of supernova explosions.

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