A recent preprint study has shed new light on Betelgeuse, the famous red giant in the constellation Orion. Astronomers have long observed Betelgeuse’s fluctuations in brightness, but new interpretations of these patterns suggest that the star is currently in the carbon-burning phase of its evolution. This stage indicates that Betelgeuse is nearing the end of its life cycle, with potentially explosive consequences in the relatively near future.
If you happened to catch a glimpse of Orion before it disappeared behind the Sun earlier this year, you might have noticed Betelgeuse’s unusual brightness. This phenomenon has puzzled astronomers, but the latest research suggests that it aligns with Betelgeuse’s advanced stage of stellar evolution. According to the preprint study, authored by Dr. Hideyuki Saio and colleagues from Tohoku University, Betelgeuse is not only actively fusing carbon in its core but is also approaching the depletion of this crucial element.
Stars like Betelgeuse begin their lives by fusing hydrogen into helium, a process that sustains them for the majority of their existence. As hydrogen supplies diminish in the core, helium fusion ensues, eventually leading to the production of heavier elements like carbon. The preprint argues that Betelgeuse’s current state suggests it is progressing through these stages rapidly.
The study focuses on Betelgeuse’s pulsations, which cause the star to expand and contract cyclically, resulting in fluctuations in its luminosity. These pulsation periods, including cycles of 185, 230, 420, and notably 2,200 days, have been closely monitored by astronomers. The interpretation hinges on identifying the fundamental mode among these pulsations, which directly correlates with the star’s radius. According to the authors, if the 2,200-day cycle indeed represents the radial fundamental mode, Betelgeuse must be significantly larger than previously estimated.
Estimating the exact timeline until Betelgeuse reaches the end of its life and explodes as a supernova remains challenging. However, the authors suggest that given Betelgeuse’s current stage, this cataclysmic event could unfold within a few decades—potentially within the lifetime of those alive today.
Betelgeuse’s impending supernova, while a spectacular astronomical event, poses no direct threat to Earth. Even at its closest estimated distance of 530 light-years or potentially much farther, Betelgeuse is far enough away to ensure that any impact on our planet would be negligible. Instead, it promises a breathtaking celestial display—a cosmic spectacle that could rival the brightness of the full Moon and serve as a rare astronomical event not witnessed since 1604.
As astronomers continue to unravel the mysteries surrounding Betelgeuse’s evolution and anticipate its eventual supernova, one thing remains certain: humanity stands poised to witness one of the most dramatic events in the cosmos—a celestial fireworks display that will illuminate the night sky and captivate observers worldwide.
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