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Key FactsNewborn magnetar explains superluminous supernovae’s brightness
Mar 11, 2026 · Reading time: ~45 sec.
Summary created with AI assistance · Source: scientificamerican.com
  • Superluminous supernovae can shine longer and more than ten times brighter than ordinary supernovae.

  • SN 2024afav, about one billion light-years away, showed periodic dips over 200 days, with intervals becoming shorter.

  • The study identifies a newly formed, rapidly spinning magnetar as the energy source, documenting its birth for the first time.

  • The Lense-Thirring effect made the tilted matter disk precess; its shrinking made the dips more frequent.
  • It means we can test one of our fundamental theories of reality in one of the most extreme environments in the universe.
    — Joseph Farah, a graduate student at the Las Cumbres Observatory (LCO) and the University of California, Santa Barbara, discussing testing general relativity in extreme environments.
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