This artist’s concept shows the red supergiant star Betelgeuse and an orbiting companion star. The companion, which is orbiting clockwise from this point of view, generates a dense wake of gas that expands outward. It is so close to Betelgeuse that it is passing through the extended outer atmosphere of the supergiant. The companion star is not to scale; it would be a pinprick compared to Betelgeuse, which is hundreds of times larger. The companion’s distance from Betelgeuse is to scale relative to the diameter of Betelgeuse. (Image credit: NASA, ESA, Elizabeth Wheatley (STScI); Science: Andrea Dupree (CfA))

Astronomers and scientists love Betelgeuse because it shines so brightly. While most stars appear as tiny points of light, Betelgeuse is large enough, and close enough, that we can study it in much greater detail. But this red supergiant star is strange, often shifting, dimming and brightening in our night sky.

In July 2025, scientists found a companion star in Betelgeuse's outer atmosphere, which could account for the red supergiant star's odd appearance. Now, using new observations from the Hubble Space Telescope, as well as data from observatories here on Earth, scientists have detected the wake of Betelgeuse's companion star, which is named Siwarha. This new study confirms Siwarha's existence.

"With this new direct evidence, Betelgeuse gives us a front-row seat to watch how a giant star changes over time," she added. "Finding the wake from its companion means we can now understand how stars like this evolve, shed material and eventually explode as supernovae."

With the combined observations of Hubble and telescopes at the Fred Lawrence Whipple Observatory in Arizona and Roque de Los Muchachos Observatory in the Canary Islands, the researchers spotted a "pattern of changes" in Betelgeuse. They could recognize Siwarha's wake, or trail, because it's composed of material that's denser than the outer-atmospheric gases that surround it.

Scientists used NASA’s Hubble Space Telescope to look for evidence of a wake being generated by a companion star orbiting Betelgeuse. The team found a noticeable difference in light shown in the lefthand peak when the companion star was at different points in its orbit. (Image credit: NASA, ESA, Elizabeth Wheatley (STScI); Science: Andrea Dupree (CfA))