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ALMA Reveals 1.4-Light-Year Bubble Around Supergiant DFK 52

High-resolution ALMA data confirm the bubble’s expansion, challenging current models of red supergiant mass loss.

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Overview

  • The circumstellar bubble contains as much mass as the Sun and spans 1.4 light years around DFK 52 in the Stephenson 2 cluster.
  • ALMA observations traced gas velocities that indicate the material was expelled in a powerful eruption roughly 4,000 years ago.
  • Detailed imaging uncovered tangled filaments, nested loops and a ring-like bar preserved in cooled molecules such as CO and SiO.
  • The solar-mass scale and expansion dynamics contradict theories of steady, low-rate winds in the final stages of red supergiants.
  • Researchers led by Mark Siebert and Elvire De Beck plan follow-up observations to search for a hidden companion star and refine pre-supernova mass-loss models.