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- Betelgeuse is a famous red supergiant star<\/strong>, located some 650-700 light-years from Earth. Its fame stems in part from the fact it\u2019ll someday explode and become visibly brighter in our sky! Astronomers have long thought Betelgeuse might have a smaller, fainter companion star.<\/li>\n
- Betelgeuse does indeed have a buddy,<\/strong> astronomers have now confirmed using the Gemini North telescope in Hawaii. The companion star is blue-white and orbits within Betelgeuse\u2019s outer atmosphere.<\/li>\n
- Both stars likely formed at the same time,<\/strong> only about 10 million years ago. The fate of the companion isn\u2019t entirely known, but it may eventually be consumed by Betelgeuse.<\/li>\n<\/ul>\n
A companion for Betelgeuse<\/h3>\n
It\u2019s confirmed! The beloved red supergiant star Betelgeuse has a companion! Astronomers using the \u2018Alopeke instrument on the Gemini North telescope in Hawaii found the companion star. The researchers said on July 21, 2025 that the companion has an estimated mass of around 1.5 times that of our sun. It appears to be an A- or B-type pre-main-sequence star \u2014 a hot, young, blue-white star that has not yet initiated hydrogen burning in its core.<\/p>\n
The companion is 6 magnitudes fainter than Betelgeuse and orbits close to Betelgeuse itself, within<\/em> the supergiant star\u2019s extended outer atmosphere.<\/p>\n
So \u2026 wow! What an incredible example of stellar evolution in action. Both Betelgeuse and its companion are relatively young stars, only about 10 million years old. Both are massive stars, of the sort that burn their fuel quickly. In accordance with what astronomers have learned about how stars evolve, Betelgeuse started out more massive than its companion. It probably started with about 15 to 20 times the sun\u2019s mass. Betelgeuse has already spent the hydrogen fuel in its core and evolved to the red giant stage. It\u2019ll famously explode as a supernova someday soon, anytime between now and 10,000 years from now. <\/p>\n
The companion \u2013 at only 1.5 times the sun\u2019s mass \u2013 appears to be still forming. It\u2019s not massive enough to become a supernova itself someday, but, in any case, its life will be cut short by Betelgeuse. It may eventually spiral into Betelgeuse. <\/p>\n
Several astronomers in recent decades have suggested a companion for Betelgeuse. A previous study from last year strongly suggested it. But now, the new observations have confirmed it.<\/p>\n
The researchers published their peer-reviewed findings in The Astrophysical Journal Letters<\/em> on July 21, 2025.<\/p>\n
![\"Bright](\"https:\/\/earthsky.org\/upl\/2025\/07\/Betelgeuse-companion-Orion-Gemini-North-July-21-2025.jpg\")
View larger. | Betelgeuse and its companion in the constellation Orion. Image via International Gemini Observatory\/ NOIRLab\/ NSF\/ AURA; Image Processing: M. Zamani (NSF NOIRLab).<\/figcaption><\/figure>\n Higher-resolution images reveal Betelgeuse\u2019s buddy<\/h3>\n
Astrophysicist Steve Howell at NASA Ames Research Center in California led the team that made the discovery. The researchers used a speckle imager on Gemini North called \u2018Alopeke<\/em> (\u2018fox\u2019 in Hawaiian). Speckle imaging uses very short exposure times to freeze out the distortions in astronomical images caused by Earth\u2019s atmosphere. The astronomers combined it with the power of Gemini North\u2019s 8.1-meter mirror to produce higher-resolution images.<\/p>\n
The researchers analyzed the light of the fainter companion star to determine its characteristics. It is an A- or B-type pre-main-sequence star: young, hot and blue-white in color, in contrast to Betelegeuse\u2019s fiery red. In addition, it is also much smaller and less massive than Betelgeuse, only 1.5 times as massive as our sun. Betelgeuse itself is enormous, about 1,400 times larger in size than the sun.<\/p>\n
Optically, the companion star is 6 magnitudes fainter than Betelgeuse.<\/p>\n
The researchers say that both stars likely formed at the same time. The companion, however, will probably have a sorter lifetime. It will eventually be consumed by Betelgeuse after it spirals into the red supergiant.<\/p>\n
An impressive accomplishment<\/h3>\n
The detection of the companion star is an impressive achievement, to be sure. Howell said:<\/p>\n
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Gemini North\u2019s ability to obtain high angular resolutions and sharp contrasts allowed the companion of Betelgeuse to be directly detected. Papers that predicted Betelgeuse\u2019s companion believed that no one would likely ever be able to image it.<\/p>\n
This detection was at the very extremes of what can be accomplished with Gemini in terms of high-angular resolution imaging, and it worked. This now opens the door for other observational pursuits of a similar nature.<\/p>\n<\/blockquote>\n
Martin Still, the National Science Foundation program director for the International Gemini Observatory, added:<\/p>\n
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The speckle capabilities provided by the International Gemini Observatory continue to be a spectacular tool, open to all astronomers for a wide range of astronomy applications. Delivering the solution to the Betelgeuse problem that has stood for hundreds of years will stand as an evocative highlight achievement.<\/p>\n<\/blockquote>\n
![\"Bright](\"https:\/\/earthsky.org\/upl\/2020\/10\/Betelgeuse-ALMA-hot-gas-extended-atmosphere-e1603162702351.jpg\")
The red supergiant star Betelgeuse is a beloved star, bright and easy to see in the famous constellation Orion the Hunter. See the \u201cbump\u201d on the left side in this submillimeter-wavelength image of the star? It\u2019s hot gas from the red giant star\u2019s extended atmosphere. Image via the ALMA telescope in Chile in 2020\/ ESO\/ NAOJ\/ NRAO)\/ E. O\u2019Gorman\/ P. Kervella.<\/figcaption><\/figure>\n ![\"Smiling](\"https:\/\/earthsky.org\/upl\/2025\/07\/Steve-Howell-NASA-Ames-Research-Center.jpeg\")
Steve Howell at NASA\u2019s Ames Research Center led the team that discovered the companion star to Betelgeuse. Image via NASA.<\/figcaption><\/figure>\n The Great Dimming of Betelgeuse<\/h3>\n
Betelgeuse is a variable star, but also experiences periods of even more significant dimming in brightness. It most recently did so in 2019-2020 and again in 2024. In fact, these dimming episodes have sparked speculation that Betelgeuse might explode soon (and astronomers say that indeed it will do so one day).<\/p>\n
In 2021, scientists said that massive amounts of hot gas and dust was being expelled from Betelgeuse\u2019s atmosphere. This, consequently, caused the dimming, as the dust temporarily blocked some of the star\u2019s light.<\/p>\n
Interestingly, the previous study from 2024 also suggested that if Betelgeuse did have a companion, then it probably won\u2019t<\/em> go boom anytime soon. So we might be waiting a long time yet!<\/p>\n
Bottom line: Astronomers using the Gemini North telescope in Hawaii have confirmed a companion for Betelgeuse!<\/p>\n
Source: Probable Direct Imaging Discovery of the Stellar Companion to Betelgeuse<\/p>\n
Via NOIRLab.<\/p>\n
Read more: Betelgeuse will explode someday, but WHEN?<\/p>\n
Read more: How far is Betelgeuse, the famous red supergiant star?<\/p>\n
<\/div>\n
\n - Betelgeuse does indeed have a buddy,<\/strong> astronomers have now confirmed using the Gemini North telescope in Hawaii. The companion star is blue-white and orbits within Betelgeuse\u2019s outer atmosphere.<\/li>\n