Crab Pulsar - Alchetron, The Free Social Encyclopedia
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Crab Pulsar - Alchetron, The Free Social Encyclopedia
The Crab Pulsar (PSR B053121) is a relatively young neutron star. The star is the central star in the Crab Nebula, a remnant of the supernova SN 1054, which was widely observed on Earth in the year 1054. Discovered in 1968, the pulsar was the first to be connected with a supernova remnant. The Crab
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The Crab Nebula is an expanding remnant of a star’s supernova explosion! 💥 Located about 6,500 light-years away, the orange filaments are the tattered remains of the star and consist mostly of hydrogen. Like a lighthouse, the neutron star embedded at the nebula’s center produces twin beams of radiation. From Earth, it appears to pulse 30 times a second due to the neutron star’s rotation sweeping the beams across our line of sight. It has the mass equivalent of our Sun crammed into a rapidly spi
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