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Magnetar-Powered Kilonova Blast

This animation shows the sequence for forming a magnetar-powered kilonova, whose peak brightness reaches up to 10,000 times that of a classical nova. In this sequence, two orbiting neutron stars spiral closer and closer together before colliding and merging. This triggers an explosion that unleashes more energy in a half-second than the Sun will produce over its entire 10-billion-year lifetime. The merger forms an even more massive neutron star called a magnetar, which has an extraordinarily powerful magnetic field. The magnetar deposits energy into the ejected material, causing it to glow unexpectedly bright at infrared wavelengths.
  • Release Date
    November 12, 2020
  • Science Release
    NASA’s Hubble Sees Unexplained Brightness from Colossal Explosion
  • Credit
    NASA, ESA, and D. Player (STScI)

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    mp4 (7.2 MB)
  • 1920 × 1080, 30 FPS
    mp4 (9.58 MB)
  • 3840 × 2160, 30 FPS
    mp4 (34.01 MB)

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Details

Last Updated
Mar 28, 2025
Contact
Media

Claire Andreoli
NASA’s Goddard Space Flight Center
Greenbelt, Maryland
claire.andreoli@nasa.gov