The haunted atmosphere of Betelguese distrupted by a shadowy companion(Image credit: NSF/AUI/NSF NRAO/M. Weiss)
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Something spooky is stirring in the shadows of the infamous star Betelgeuse, a cosmic poltergeist that is disrupting the atmosphere of the red supergiant.

New radio observations have shown Betelgeuse's smaller stellar companion,Siwarha(not Betelguese Betelguese, unfortunately), cutting through the supergiant's extended atmosphere and leaving a wake in its path, like a jet boat slicing through a lake.

Because the name of this red supergiant star located about 650 light-years away from Earth, marking the shoulder of constellation Orion, is Betelgeuse, which means "the hand of al-Jawza" in Arabic, the companion was namedSiwarha, meaning "her bracelet."

"This companion is orbiting so close to the star that it actually passes through its extended atmosphere," Lynn Matthews, the principal research scientist at Massachusetts Institute of Technology (MIT) Haystack Observatory who led the new observations, said in astatement.

Astronomers turn cosmic ghost hunters

Using data collected from 2021 to 2026 using the Karl G. JanskyVery Large Arrayin New Mexico and the Atacama Large Millimeter/submillimeter Array (ALMA) in Chile, Matthews and colleagues found that Betelgeuse's atmosphere stretches into an egg shape when the companion star is farthest away and rounds out when the companion passes in front of or behind it.

The same data also showed that Betelgeuse itself has largely recovered from the "Great Dimming" that made headlines in 2020. This recovery comes after the red supergiant "sneezed" in 2020, dramatically ejecting tons of gas and dust and fading to its dimmest in more than a century.

ALMA captures a stunning image of the doomed star Betelgeuse(Image credit: ALMA(ESO/NAOJ/NRAO)/W. Dent et al.)

Among the long-standing mysteries of Betelgeuse, scientists have puzzled over a brightening and dimming cycle that lasts roughly 2,100 days. Recent studies pointed to a low-mass companion orbiting deep inside the star's atmosphere, and its existence was confirmed inearly 2026.

Though Siwarha itself istoo faint to detect directlyat radio wavelengths, its influence shows up in the star's shape, the new study found. To confirm the effect, the researchers say, they will need to observe more of the companion's orbit, especially at radio frequencies that have so far been sparsely sampled.

TheNext Generation Very Large Array, a planned telescope, should make this kind of monitoring far more routine, according to the team. With sharper vision, researchers could see how red supergiants like Betelgeuse shed their material as they near the end of their lives, and how a close companion might affect that process by tugging on that ejected matter.

This research is described in apaperpublished in The Astronomical Journal.

Sharmila Kuthunur

Contributing Writer

Sharmila Kuthunur is an independent space journalist based in Bengaluru, India. Her work has also appeared in Scientific American, Science, Astronomy and Live Science, among other publications. She holds a master's degree in journalism from Northeastern University in Boston.

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