January 6, 2026
2 min read
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Astronomers May Have Unlocked the Reason for Betelgeuse’s Bizarre Dimming
Researchers found evidence that a companion star may be influencing Betelgeuse, explaining why the latter star’s brightness changes over time
NASA/ESA/Elizabeth Wheatley/STScI (artwork); Andrea Dupree/CfA (science)
Astronomers may have finally solved one of the weirdest mysteries of our night sky: why Betelgeuse, a massive star in the constellation Orion, seems to fade and brighten as if it were operated by a heavenly dimmer switch.
Using the Hubble Space Telescope and ground-based observatories, scientists observed Betelgeuse for almost eight years and found patterns in the star’s light and atmosphere that suggested it was passing through the wake of another, unseen star.
“It’s a bit like a boat moving through water. The companion star creates a ripple effect in Betelgeuse’s atmosphere that we can actually see in the data,” said Andrea Dupree, an astronomer at the Center for Astrophysics | Harvard & Smithsonian, in a statement.
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The other star appears to pass in front of Betelgeuse every six years or so. If the findings are confirmed by follow-up observations, they will help explain why Betelgeuse, a bright, nearby star that is more massive than 400 million suns, periodically seems to be on the point of vanishing before our eyes. That’s what happened in 2020: at that time, Betelgeuse appeared so faint that it fed rumors that it was possibly about to explode into a supernova. (Astronomers, in general, did not think that such a cataclysm was imminent. But they were mightily confused.)
Scientists had predicted the existence of a companion star, dubbed Siwarha, before. But the evidence was lacking, Dupree said in the recent statement.
“With this new direct evidence, Betelgeuse gives us a front-row seat to watch how a giant star changes over time,” she said. “Finding the wake from its companion means we can now understand how stars like this evolve, shed material, and eventually explode as supernovae.”
The research was presented on Monday at the annual meeting of the American Astronomical Society and will be published in the Astrophysical Journal.
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