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EI2GYB > ASTRO 13.10.25 14:39l 84 Lines 5012 Bytes #999 (0) @ WW
BID : 46533_EI2GYB
Subj: Betelgeuse's Secret Companion Finally Revealed
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Betelgeuse's Secret Companion Finally Revealed
Betelgeuse, the brilliant red star marking Orion's shoulder, has long been
suspected of harbouring 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 theorised 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, the findings 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 realised 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 whilst its companion barely reaches one
solar mass. This massive mass ratio opens up a new the possibility of extreme
mass ratio binaries, an area that remains largely unexplored simply because
such systems are extraordinarily difficult to detect.
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