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THE POWER BEHIND A SUPERLUMINOUS BLAST.

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Title: THE POWER BEHIND A SUPERLUMINOUS BLAST.
Authors: Bennett, Jay (AUTHOR)
Source: Science News. May2026, Vol. 208 Issue 5, p10-11. 2p. 1 Color Photograph.
Subjects: Supernovae, Magnetars, Light intensity, Neutron stars, Circumstellar matter, Astronomical observations, Stars
Abstract: The article focuses on the observation of a superluminous supernova detected about a billion light-years from Earth in 2024, which shone approximately 30 times brighter than typical supernovas formed from collapsed stellar cores. Astronomers report a unique "chirp" in the supernova's light—a fluctuation that accelerated over time—suggesting the presence of a fast-spinning magnetar, a highly magnetized neutron star. This magnetar may have continuously energized the surrounding debris, sustaining the explosion's brightness, while a wobbling disk of debris could have caused the observed chirp. [Extracted from the article]
Copyright of Science News is the property of Society for Science & the Public and its content may not be copied or emailed to multiple sites without the copyright holder's express written permission. Additionally, content may not be used with any artificial intelligence tools or machine learning technologies. However, users may print, download, or email articles for individual use. This abstract may be abridged. No warranty is given about the accuracy of the copy. Users should refer to the original published version of the material for the full abstract. (Copyright applies to all Abstracts.)
Database: Engineering Source
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  Availability: 1
Header DbId: egs
DbLabel: Engineering Source
An: 192715575
AccessLevel: 6
PubType: Periodical
PubTypeId: serialPeriodical
PreciseRelevancyScore: 0
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  Data: THE POWER BEHIND A SUPERLUMINOUS BLAST.
– Name: Author
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  Data: <searchLink fieldCode="AR" term="%22Bennett%2C+Jay%22">Bennett, Jay</searchLink> (AUTHOR)
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  Data: <searchLink fieldCode="JN" term="%22Science+News%22">Science News</searchLink>. May2026, Vol. 208 Issue 5, p10-11. 2p. 1 Color Photograph.
– Name: Subject
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  Data: <searchLink fieldCode="DE" term="%22Supernovae%22">Supernovae</searchLink><br /><searchLink fieldCode="DE" term="%22Magnetars%22">Magnetars</searchLink><br /><searchLink fieldCode="DE" term="%22Light+intensity%22">Light intensity</searchLink><br /><searchLink fieldCode="DE" term="%22Neutron+stars%22">Neutron stars</searchLink><br /><searchLink fieldCode="DE" term="%22Circumstellar+matter%22">Circumstellar matter</searchLink><br /><searchLink fieldCode="DE" term="%22Astronomical+observations%22">Astronomical observations</searchLink><br /><searchLink fieldCode="DE" term="%22Stars%22">Stars</searchLink>
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  Label: Abstract
  Group: Ab
  Data: The article focuses on the observation of a superluminous supernova detected about a billion light-years from Earth in 2024, which shone approximately 30 times brighter than typical supernovas formed from collapsed stellar cores. Astronomers report a unique "chirp" in the supernova's light—a fluctuation that accelerated over time—suggesting the presence of a fast-spinning magnetar, a highly magnetized neutron star. This magnetar may have continuously energized the surrounding debris, sustaining the explosion's brightness, while a wobbling disk of debris could have caused the observed chirp. [Extracted from the article]
– Name: AbstractSuppliedCopyright
  Label:
  Group: Ab
  Data: <i>Copyright of Science News is the property of Society for Science & the Public and its content may not be copied or emailed to multiple sites without the copyright holder's express written permission. Additionally, content may not be used with any artificial intelligence tools or machine learning technologies. However, users may print, download, or email articles for individual use. This abstract may be abridged. No warranty is given about the accuracy of the copy. Users should refer to the original published version of the material for the full abstract.</i> (Copyright applies to all Abstracts.)
PLink https://search.ebscohost.com/login.aspx?direct=true&site=eds-live&db=egs&AN=192715575
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      – Code: eng
        Text: English
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        PageCount: 2
        StartPage: 10
    Subjects:
      – SubjectFull: Supernovae
        Type: general
      – SubjectFull: Magnetars
        Type: general
      – SubjectFull: Light intensity
        Type: general
      – SubjectFull: Neutron stars
        Type: general
      – SubjectFull: Circumstellar matter
        Type: general
      – SubjectFull: Astronomical observations
        Type: general
      – SubjectFull: Stars
        Type: general
    Titles:
      – TitleFull: THE POWER BEHIND A SUPERLUMINOUS BLAST.
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              M: 05
              Text: May2026
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              Y: 2026
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