In 2024, astronomers made an exciting discovery about Betelgeuse. They speculated that this famous red supergiant star might have a companion star, and it turns out they were right. After much research and a few false alarms, scientists at NASA’s Ames Research Center confirmed that Betelgeuse does have a smaller “buddy” star nearby.
This companion star is about 1.5 times the mass of our Sun. Its presence likely influences Betelgeuse’s unusual dimming patterns. Astronomers had noticed an extended dimming phase occurring roughly every six years, which was a mystery until this discovery.
Steve Howell, the leading astronomer in this research, shared, “Papers that predicted Betelgeuse’s companion believed that no one would likely ever be able to image it. This now opens the door for other observational pursuits of a similar nature.” This hints at more exciting discoveries ahead.
The researchers used the Gemini North telescope in Hawaii, employing a technique called speckle imaging. This method minimizes distortions caused by Earth’s atmosphere, allowing for a clear view of the companion star. They gathered crucial data about its mass and temperature.
Affectionately dubbed “BetelBuddy” by the researchers, this companion star is younger than Betelgeuse. While the red supergiant is nearing the end of its life, the buddy star is still in its early stages of evolution. Betelgeuse, which is 10 to 20 times the mass of our Sun, has a far shorter lifespan, suggesting a fascinating contrast between the two stars.
For centuries, astronomers have closely studied Betelgeuse due to its proximity to Earth. They observed that its brightness changes in cycles, with a prominent period lasting about 400 days and another lasting around six years. The longer dimming phase was puzzling until now.
It’s important to note that this discovery is separate from the “Great Dimming” observed from 2019 to 2020. Scientists believe that phenomenon was caused by a large cloud of dust being expelled from Betelgeuse, affecting its brightness. Now, the recent findings provide clarity on why Betelgeuse has these unusual brightness patterns.
Moving forward, astronomers expect Betelgeuse’s gravitational pull to eventually draw in its companion star within the next 10,000 years. Fortunately, BetelBuddy won’t disappear quietly; it will pass into a range observable by telescopes again in November 2027, giving us another chance to study this unique stellar relationship.
Overall, this discovery deepens our understanding of not just Betelgeuse but stellar evolution as a whole. It also reflects a growing trend in astronomy, where advanced imaging techniques allow scientists to uncover more details about the cosmos than ever before.
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Astronomy,Stellar astronomy,Stellar evolution