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  2. Crab Nebula - Wikipedia

    en.wikipedia.org/wiki/Crab_Nebula

    The Crab Pulsar, a neutron star 28–30 kilometres (17–19 mi) across with a spin rate of 30.2 times per second, lies at the center of the Crab Nebula. The star emits pulses of radiation from gamma rays to radio waves .

  3. Near-Earth supernova - Wikipedia

    en.wikipedia.org/wiki/Near-Earth_supernova

    The Crab Nebula is a pulsar wind nebula associated with the 1054 supernova.It is located about 6,500 light-years from the Earth. [1]A near-Earth supernova is an explosion resulting from the death of a star that occurs close enough to the Earth (roughly less than 10 to 300 parsecs [30 to 1000 light-years] away [2]) to have noticeable effects on Earth's biosphere.

  4. Supernova - Wikipedia

    en.wikipedia.org/wiki/Supernova

    The pulsar in the Crab Nebula is travelling at 375 km/s relative to the nebula. [ 165 ] A long-standing puzzle surrounding type II supernovae is why the remaining compact object receives a large velocity away from the epicentre; [ 166 ] pulsars , and thus neutron stars, are observed to have high peculiar velocities , and black holes presumably ...

  5. NASA's Hubble captures stunning photos of the Crab Nebula's ...

    www.aol.com/article/2016/07/07/nasas-hubble...

    It spins at a rate of 30 times per second, spewing energy beams and taking on a decidedly pulsating appearance. NASA's Hubble captures stunning photos of the Crab Nebula's 'beating heart' Skip to ...

  6. Neutron star - Wikipedia

    en.wikipedia.org/wiki/Neutron_star

    Central neutron star at the heart of the Crab Nebula Radiation from the rapidly spinning pulsar PSR B1509-58 makes nearby gas emit X-rays (gold) and illuminates the rest of the nebula, here seen in infrared (blue and red). A neutron star is the collapsed core of a massive supergiant star.

  7. New Crab Nebula image captured by James Webb Space Telescope ...

    www.aol.com/news/crab-nebula-image-captured...

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  8. Pulsar - Wikipedia

    en.wikipedia.org/wiki/Pulsar

    The Crab pulsar 33-millisecond pulse period was too short to be consistent with other proposed models for pulsar emission. Moreover, the Crab pulsar is so named because it is located at the center of the Crab Nebula, consistent with the 1933 prediction of Baade and Zwicky. [23]

  9. Crab Pulsar - Wikipedia

    en.wikipedia.org/wiki/Crab_Pulsar

    Thomas Gold has shown that the pulsar's spin-down power is sufficient to power the Crab Nebula. A subsequent study by them, including William D. Brundage, also found that the NP 0532 source is located at the Crab Nebula. [20] A radio source was also reported coincident with the Crab Nebula in late 1968 by L. I. Matveenko in Soviet Astronomy. [21]