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Direct Imaging Confirms Betelgeuse’s Long-Sought Companion Star

Astronomers used the Alopeke speckle imager on Gemini North to identify a 1.5-solar-mass blue-white star orbiting within Betelgeuse’s extended atmosphere.

Image
Credit: International Gemini Observatory/NOIRLab/NSF/AURA/M. Zamani (NSF NOIRLab)

Overview

  • Observers identified a blue-white A/B-type pre-main-sequence companion with an estimated mass of 1.5 solar masses and a brightness six magnitudes below Betelgeuse.
  • The star orbits at approximately four astronomical units—about 52 milliarcseconds from Betelgeuse—placing it within the red supergiant’s outer atmosphere.
  • Speckle imaging with the Alopeke instrument on the Gemini North telescope used millisecond exposures to freeze atmospheric turbulence, delivering the high angular resolution required for the discovery.
  • The peer-reviewed results published in The Astrophysical Journal Letters on July 21, 2025, confirm long-standing predictions linking a close companion to Betelgeuse’s six-year brightness variations.
  • Models predict that friction from Betelgeuse’s extended atmosphere will drag the companion inward, leading to its consumption within about 10,000 years.