Nasa James Webb Telescope - Crab Nebula (NIRCam and MIRI Compass Image) - Wall Art Photo Poster Print

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Nasa James Webb Telescope - Crab Nebula (NIRCam and MIRI Compass Image)

The Crab Nebula is a supernova remnant located in the constellation Taurus, about 6,500 light-years away from Earth. It is the result of a supernova explosion that was observed by Chinese astronomers in the year 1054 AD. The supernova, now known as SN 1054, was one of the brightest and most widely observed supernovae in human history.

The Crab Nebula is characterized by its intricate and filamentary structure, which is visible in both optical and radio wavelengths. At the heart of the nebula is a pulsar, a rapidly rotating neutron star formed in the aftermath of the supernova explosion. This pulsar, known as the Crab Pulsar or PSR B0531+21, rotates about 30 times per second and emits beams of radiation, including X-rays and gamma rays, which contribute to the nebula's overall appearance.

The Crab Nebula is a strong source of radiation across the electromagnetic spectrum, from radio waves to gamma rays. It is a popular target for astronomers and astrophysicists studying various aspects of astrophysics, including the behaviour of pulsars, the dynamics of supernova remnants, and the processes of cosmic ray acceleration. The Nasa James Webb Telescope and other observatories have provided stunning images of the Crab Nebula, revealing its intricate details and helping scientists better understand the aftermath of massive stellar explosions.