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First Direct Image Reveals Companion Star Orbiting Betelgeuse

High-resolution speckle imaging on Gemini North confirmed a 1.5-solar-mass pre–main-sequence star orbiting inside Betelgeuse’s outer atmosphere

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

Overview

  • The companion is six magnitudes dimmer than Betelgeuse in visible light, underscoring its faintness against the supergiant’s glare.
  • It follows a tight orbit of roughly four astronomical units, a separation newly accessible through advanced imaging techniques.
  • Discovery of this close-in star validates models attributing Betelgeuse’s six-year brightness cycle to a gravitational influence.
  • Strong tidal interactions are expected to draw the companion into Betelgeuse, leading to a merger within about 10,000 years.
  • Astronomers plan a follow-up observation in November 2027 when the star reaches its maximum apparent separation for detailed study.