Space / crab-pulsar
Facts about Crab Pulsar
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Younger and more energetic than most pulsars, the Crab Pulsar continuously powers the surrounding Crab Nebula by converting rotational energy into radiation and particle winds.
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Optical pulses from the Crab Pulsar were first detected in 1969, confirming it as the first pulsar identified at visible wavelengths.
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Discovered as a radio pulsar in 1968, the Crab Pulsar is the collapsed stellar core left behind after a massive star exploded.
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Remnants of the supernova that created the Crab Pulsar were observed by Chinese astronomers in 1054 AD and recorded as a guest star visible in daylight.
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The Crab Pulsar rotates approximately 30 times per second, making it one of the fastest-spinning and most energetic pulsars known.