THE POWER BEHIND A SUPERLUMINOUS BLAST.
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| Title: | THE POWER BEHIND A SUPERLUMINOUS BLAST. |
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| 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] |
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| Database: | Engineering Source |
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| 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] |
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| ISSN: | 00368423 |
