Astronomers report an extremely rapid transformation of one of the largest known stars in the Universe – WOH G64. The object located in the Large Magellanic Cloud has transitioned from the red supergiant phase to the yellow hypergiant stage in just a few years, a clear signal of an impending cosmic catastrophe. Scientists from the team led by Gonzalo Muñoz-Sanchez believe the star is preparing to explode as a supernova or collapse into a black hole. This process, described in the journal "Nature Astronomy," provides a unique opportunity to observe the final stages of a massive star's life in real time.
Rapid Evolutionary Transformation
Star WOH G64 transitioned in a surprisingly short time, within a few years, from the red supergiant phase to the rare yellow hypergiant stage. The observed rapid heating of the object and intense shedding of its outer layers of matter indicate an accelerated countdown to the end of its life.
Harbinger of a Cosmic Catastrophe
Scientists agree that the observed changes are a clear prelude to the final act in the star's life. The most likely scenario is a supernova explosion of unimaginable scale, although a quiet collapse into a black hole is also possible. The explosion would occur in our galactic neighborhood.
Unique Research Opportunity
Direct observation of such an advanced stage in the evolution of a massive star is an extremely rare event. These processes usually occur over thousands or millions of years, whereas now scientists can track them on a human timescale, providing invaluable data for astrophysical models.
Cosmic Colossus with Record Parameters
WOH G64 is one of the largest known objects in the Universe, with a radius exceeding 1500 solar radii. Despite its gigantic size, on a cosmic timescale it is a relatively young star, estimated to be only about five million years old.
Astronomers are witnessing an extremely rare and accelerated cosmic spectacle – the final moments in the life of one of the largest known stars, WOH G64. The object located in the neighboring galaxy of the Large Magellanic Cloud is undergoing a dramatic evolutionary transformation from the red supergiant phase to the yellow hypergiant stage. The key is the speed of this change – a process that, according to standard stellar evolution models, should take thousands of years is unfolding here in just a few years. Observations, particularly clear since around 2014, show the star rapidly heating up and violently ejecting its outer layers into space. A team of scientists led by Gonzalo Muñoz-Sanchez from the National Observatory of Athens presented the research results in the prestigious journal "Nature Astronomy." According to the researchers, the observed transformation is a clear signal that the massive star is preparing for the final act of its existence. For an object with the parameters of WOH G64, this most likely means the explosion of a supernova on an unimaginable energy scale. However, an alternative scenario cannot be ruled out, in which the star collapses without a spectacular explosion, directly forming a black hole. Regardless of the finale, this event will take place in our cosmic neighborhood. Studying the final stages of massive stars' lives is a cornerstone of modern astrophysics. Theory predicts that stars significantly more massive than the Sun end their lives in spectacular supernova explosions, which scatter heavy elements essential for planet and life formation throughout the cosmos. However, direct observations of these processes are extremely rare due to their cosmic timescale. WOH G64 thus provides a unique opportunity to verify theoretical models. The phenomenon is all the more valuable because it concerns a star with nearly record-breaking parameters. Its radius, exceeding 1500 solar radii, makes it one of the largest known celestial bodies. Paradoxically, this cosmic colossus is, from an evolutionary perspective, an infant – it is estimated to have ignited only about five million years ago. For comparison, the Sun has existed for about 4.6 billion years and is only halfway through its life. Observations of WOH G64 are being conducted by a network of telescopes worldwide, allowing for continuous monitoring of its state. The coming months and years may bring decisive moments in its evolution, offering astronomers an unprecedented insight into the mechanisms governing the death of the largest stars. „„It's like watching a slow-motion countdown to an explosion. Changes we usually think of as static over millennia are happening right before our eyes.”” (This event does not pose a direct threat to Earth, but its observation will be of fundamental importance for science. A supernova explosion in our galactic neighborhood would be visible to the naked eye in the sky for many months, even years, becoming one of the brightest points in the night sky.) — Gonzalo Muñoz-Sanchez This event does not pose a direct threat to Earth, but its observation will be of fundamental importance for science. A supernova explosion in our galactic neighborhood would be visible to the naked eye in the sky for many months, even years, becoming one of the brightest points in the night sky.
Mentioned People
- Gonzalo Muñoz-Sanchez — Astronomer from the National Observatory of Athens, leading the research team analyzing the transformation of star WOH G64.