‘Behemoth star,’ previously thought to be dying, is ‘rising from the ashes’ like a pheonix
One of the universe’s largest stars, previously predicted to be in the throes of a violent supernova death, may not imminently explode after all, a new study suggests. The surprise finding also hints that the stellar “behemoth” is slowly being cannibalized by a smaller, hidden partner.
WOH G64, often dubbed the “behemoth star,” is a red supergiant located around 163,000 light-years from Earth, in the Large Magellanic Cloud — a dwarf galaxy that closely orbits the Milky Way. The stellar giant is around 1,500 times wider than the sun, making it one of the largest stars ever discovered. It also shines up to 282,000 times brighter than our home star.
In recent years, WOH G64 had become significantly dimmer, suggesting that the gigantic star was transitioning into a smaller and hotter yellow hypergiant by shedding its outermost layers of gas. When this happens to a red supergiant, it is usually a sign that the star is about to go supernova. Given that the star is around 5 million years old — around the maximum lifespan for red supergiants, which burn up their fuel much more quickly than sunlike stars do — it seemed likely that this was happening.
Further proof of an imminent explosion came in November 2024, when researchers took a highly detailed photo of WOH G64 with the Very Large Telescope in Chile — the first image of its kind for an object outside our galaxy — and detected an “egg-shaped cocoon” of gas and dust around the star. This was proof that the star had shed its outer layers and become a yellow hypergiant, experts assumed.
But in the new study, published Jan. 7 in the journal Monthly Notices of the Royal Astronomical Society, researchers took another look at WOH G64, using the Southern African Large Telescope (SALT) — and they found a “smoking gun” that challenges the widely accepted supernova hypothesis.
The team’s data, collected by SALT’s powerful spectroscope between November 2024 and December 2025, revealed titanium oxide — which is normally found only in red supergiants — within WOH G64’s atmosphere.
“This implies that WOH G64 is currently a red supergiant and may never have ceased to be,” study co-lead author Jacco van Loon, an astrophysicist at Keele University in England, said in a statement. “We are essentially witnessing a ‘phoenix’ rising from the ashes,” he added.
But if WOH G64 isn’t turning into a yellow hypergiant, why is it behaving so strangely?
The research team suspects the giant star is part of a binary system that includes a smaller star. In this case, its diminutive partner, which likely shines blue, is probably pulling WOH G64’s outer layers into a circumstellar disk.
“The atmosphere of the red supergiant is being stretched out by the approach of the companion star, but it has not been stripped altogether,” van Loon said. “It persists.”
This theory was also raised when the star’s dusty cocoon was photographed in 2024, but it failed to gain traction.
All eyes are now on WOH G64 for more clues as to when the stellar behemoth will eventually blow its top.
Van Loon, J. T., & Ohnaka, K. (2026). A phoenix rises from the ashes: WOH G64 is still a red supergiant, for now. Monthly Notices of the Royal Astronomical Society, 546(2). https://doi.org/10.1093/mnras/stag012
