Space

Companion for Betelgeuse update! A new image

Companion for Betelgeuse: Composite image showing the constellation of Orion outline, with a circle around Betelgeuse, an circle highlight with an line to an image of Betelgeuse and marks indicting a bright spot that could be the companion star to Betelgeuse.
Betelgeuse is a famous red supergiant star in the constellation Orion the Hunter. Astronomers had long suspected a companion for Betelgeuse, and a year ago, the companion was confirmed when furthest apart from Betelgeuse as seen from Earth. Now the European Southern Observatory (ESO) has confirmed the discovery, too, with a new image of the companion (inside crosshairs on far-left insert). Image via ESO/ M. Montargès et al.

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  • ESO’s Very Large Telescope has captured an image of the recently discovered companion to the famous red supergiant Betelgeuse at its expected location.
  • To confirm the object is Betelgeuse B astronomers will need to observe it in one year on the other side of the star.
  • The likely companion star is around 2 to 3 times the mass of our sun.

The European Southern Observatory shared this press release on July 28, 2026. Edits by EarthSky.

Image shows evidence of Betelgeuse companion star

A year ago, U.S. astronomers announced a companion for the red supergiant star Betelgeuse. This star is famous for being nearby and poised to explode. And now European astronomers have confirmed that important discovery. Using the European Southern Observatory’s Very Large Telescope (ESO’s VLT), a team led by French researcher Miguel Montargès obtained the clearest image ever of what is likely Betelgeuse B, the star orbiting Betelgeuse. He’s an astronomer at the Observatoire de Paris – PSL, France, and lead author of the study published today in Astronomy & Astrophysics. Montargès recalls:

I jumped from my chair when I saw the processed images.

Betelgeuse, in the constellation Orion the Hunter, is easily visible with the unaided eye. Want to see it? Read this article about the return of Orion before dawn at this time of year. Excitingly, the star is known to change in brightness. It has been observed for millennia. However, it still surprises astronomers.

The brightness of Betelgeuse varies

For a long time, astronomers have looked for the potential companion to Betelgeuse. It was originally proposed to explain Betelgeuse’s brightness changes. Then two studies published in 2024 predicted that in December that year, the companion would be furthest from Betelgeuse and hence easier to spot. Montargès and his team got to work, observing the star with ESO’s VLT in December 2024 and spending several months processing the data.

Originally the companion star was thought to be about as massive as the sun. However, the new observations reveal that Betelgeuse B has around two to three times the mass of the sun. Montargès explained:

Honestly, I thought we did not have the sensitivity to detect Betelgeuse B as it was predicted. Because it is more massive than predicted, we see it! The fact that we can still discover a nearby companion, more massive and brighter than the sun, around such a well-studied star is remarkable. These are among the best moments in science: seeing something new, unexpected.

The Betelgeuse companion imaged

Betelgeuse B was directly imaged, meaning the light from the star itself was detected, using the SPHERE instrument on ESO’s VLT. While there was evidence for the existence of this companion star, including a possible direct detection with the Gemini North Telescope in Hawaii, this is the strongest evidence for, and clearest image yet of, Betelgeuse B. Co-author Anthony Boccaletti, also an astronomer at the Observatoire de Paris said:

It is remarkable to see how SPHERE and advanced post-processing techniques, originally developed to find exoplanets, also excel at detecting a companion around a massive, evolved star like Betelgeuse.

Montargès added:

To be certain that the companion is really there, we still need to observe it in one year on the other side of the star. But there is very little space left for doubt.

Zoomed in view with a white circle in the middle where Betelgeuse would be and a highlighted bright spot to its lower left that is most likely the companion star to Betelgeuse.
This image, taken with ESO’s VLT, shows the clearest image ever of what likely is Betelgeuse B, a star orbiting Betelgeuse. The image was taken with the SPHERE instrument in December 2024, when the companion was predicted to be furthest apart from Betelgeuse. The circle indicates the size of Betelgeuse, which has been removed. Then the bright source to the left, marked with a crosshair, is consistent with being Betelgeuse B. Image via ESO/ M. Montargès et al.

Betelgeuse’s great dimming caught attention

A few years back, Betelgeuse was the subject of attention from astronomers and non-astronomers alike when it visibly started dimming. As an evolved supergiant star, Betelgeuse is expected to die in a supernova explosion. So the dramatic dimming of Betelgeuse led some to speculate it could be about to explode. A group of astronomers led by Montargès studied the star with ESO’s VLT, finding it was instead obscured by a cloud of dust.

The potential detection of Betelgeuse B will prompt astronomers to investigate how the companion could affect Betelgeuse’s anticipated supernova explosion. Montargès concluded:

The question is truly opened whether this companion is going to have an impact on the evolution of the red supergiant.

Starry sky with a bright sphere in the middle that is the star Betelgeuse.
This image is a color composite made from exposures from the Digitized Sky Survey 2 (DSS2). Image by Davide De Martin/ / Digitized Sky Survey 2/ ESO.

Bottom line: A recent image appears to show the companion star of Betelgeuse, know as Betelgeuse B. It’s the strongest evidence yet that the beloved red supergiant star has a companion star.

Via ESO

Read more: Betelgeuse’s companion star leaves detectable wake

Read more: New details about Betelbuddy, Betelgeuse’s companion star

Posted 
July 28, 2026
 in 
Space

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