Get all your news in one place.
100’s of premium titles.
One app.
Start reading
Space
Space
Science
Stefanie Waldek

Giant star Betelgeuse has a 'Betelbuddy' — and it's very little indeed

This image of Betelgeuse is a color composite made from exposures from the Digitized Sky Survey 2 (DSS2). A bright ball of light glows in the middle of deep space.

Every superhero — or antihero — needs a sidekick. And it turns out that Beetlejuice Betelgeuse does indeed have one! The red supergiant star found in the constellation Orion has captivated stargazers for millennia, and while scientists have long theorized it had a companion of some sort due to its periodic dimming, no one had ever seen it. Until recently! World, meet Betelbuddy.

After the Gemini North Telescope in Hawaii imaged a faint potential companion to Betelgeuse, Carnegie Mellon University (CMU) researchers used NASA’s Chandra X-ray Observatory and the Hubble Space Telescope to examine Betelgeuse in more detail. And the timing was perfect — Betelbuddy, as the tiny companion is nicknamed — was at its maximum distance from its much larger, much brighter neighbor. (Betelgeuse is about 700 times the size of our sun and thousands of times brighter.) Finally, researchers made detailed, concrete observations.

"It turns out that there had never been a good observation where Betelbuddy wasn't behind Betelgeuse," Anna O’Grady, a postdoctoral fellow at CMU,"said in a statement. "This represents the deepest X-ray observations of Betelgeuse to date.”

Impressively, capturing an image of Betelbuddy was only the start of the discoveries. The researchers had anticipated the companion to be a white dwarf or a neutron star, but they saw no signs of accretion, a distinct signature of both types of objects. Instead, they suspect it might be a young stellar object about the size of our sun.

And herein lies the next major discovery. The size ratio between Betelgeuse and Betelbuddy challenges what we currently know about binary stars. Typically, binary stars have similar masses. But Betelgeuse is about 16 to 17 times the mass of our sun, whereas Betelbuddy has about the same mass as our sun.

"This opens up a new regime of extreme mass ratio binaries,” O’Grady said. "It's an area that hasn’t been explored much because it's so difficult to find them or to even identify them like we were able to do with Betelgeuse."

This is only the start of the tale of Betelgeuse and Betelbuddy, and we can't wait to see where it takes us next.

The team's research will be published in The Astrophysical Journal on Oct. 10.

Sign up to read this article
Read news from 100’s of titles, curated specifically for you.
Already a member? Sign in here
Related Stories
Top stories on inkl right now
One subscription that gives you access to news from hundreds of sites
Already a member? Sign in here
Our Picks
Fourteen days free
Download the app
One app. One membership.
100+ trusted global sources.