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Betelgeuse, the brilliant red star marking Orion's shoulder, has long been suspected of harboring a secret. I have to confess, Betelgeuse holds a special place in my heart as the first star I ever looked at through a telescope as a child, so learning that astronomers theorized this massive supergiant wasn't alone made it even more intriguing.

Proving it, however, required catching a fleeting alignment and deploying some of our most powerful space telescopes in a race against time. Now, researchers from Carnegie Mellon University have finally confirmed what many suspected: Betelgeuse does indeed have a companion star, though not quite the type anyone expected.

The challenge of detecting anything near Betelgeuse cannot be overstated. The star is roughly 700 times larger than our sun and thousands of times brighter, making it extraordinarily difficult to spot nearby objects. It's rather like trying to photograph a firefly hovering next to a car headlight, perhaps worse! The brightness difference between Betelgeuse and its tiny companion is, as Anna O'Grady, a McWilliams Postdoctoral Fellow at Carnegie Mellon, put it, "absolutely insane."

The breakthrough came during a critical observational window around 6th December, when the companion, affectionately nicknamed "Betelbuddy," reached its maximum separation from the supergiant before disappearing behind it for another two years. The timing demanded swift action. O'Grady and her team secured Director's Discretionary Time on both NASA's Chandra X-ray Observatory and the Hubble Space Telescope, reserved time typically granted only for the most exceptional research opportunities. Having two such proposals accepted simultaneously speaks to the significance of the discovery.

Using Chandra's X-ray observations, the deepest ever taken of Betelgeuse, O'Grady's team searched for evidence of accretion, the telltale signature of compact objects like neutron stars or white dwarfs pulling material from their surroundings. They found nothing. No accretion signature appeared in the data, ruling out these possibilities. Instead, published in the Astrophysical Journal point to something more ordinary yet equally fascinating, a young stellar object roughly the size of our sun.

The discovery emerged from a rather wonderfully spontaneous circumstance. The idea to propose for observing time arose during a discussion at the McWilliams Center for Cosmology at Carnegie Mellon University. Professor Katelyn Breivik recalled how what seemed like an extreme longshot gradually coalesced into a genuine opportunity as the team realized their unique combination of expertise and the perfect timing might actually succeed in securing Director's time. It's quite satisfying when a casual conversation transforms into an exciting discovery.

Beyond confirming Betelbuddy's existence, the findings help explain Betelgeuse's puzzling six-year cycle of brightening and dimming. A previous 2024 study proposed that an orbiting companion clears away light blocking dust, allowing Betelgeuse to appear brighter from Earth. Now that theory finally has observational support. It does, however, challenge current binary star formation process models.

Typically, binary pairs form with similar masses, but Betelgeuse weighs in at 16 or 17 solar masses while its companion barely reaches one solar mass. This massive mass ratio opens up a new possibility of extreme mass ratio binaries, an area that remains largely unexplored simply because such systems are extraordinarily difficult to detect.