Scientific American - USA (2019-12)

(Antfer) #1
BLAST SCENE
DEEP IN THE HEART of the Crab Nebula lies a highly mag-
netized, rapidly rotating neutron star that was produced
when a massive star exploded as a supernova in the year


  1. This multiwavelength image reveals the debris from
    the blast: x-rays are shown in purple, ultraviolet light in blue,
    visible in green, infrared in yellow and radio light in red. The
    x-ray emission, closest to the neutron star, is dominated by
    light released by charged particles that were accelerated to
    high energies by the star’s rotation.
    X-RAY: NASA, CXC AND SAO; OPTICAL: NASA AND STSCI; INFRARED: NASA, JPL AND CALTECH; RADIO: NSF,
    NRAO AND VLA; ULTRAVIOLET: ESA AND XMM-NEWTON


© 2019 Scientific American

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