Scientists may have witnessed a massive, dying star split in two and then crash back together, triggering a never-before-seen double explosion. The explosion sent ripples through space-time and forged some of the universe's heaviest elements.
Most massive stars reach the ends of their lives by collapsing and exploding as supernovas, seeding the cosmos with elements such as carbon and iron. A different kind of cataclysm, known as a kilonova, occurs when the ultradense remnants of dead stars, called neutron stars, collide, forging even heavier elements like gold.
A two-in-one combo
AT2025ulz first caught astronomers' attention on Aug. 18, 2025, when gravitational wave detectors operated by the U.S.-based Laser Interferometer Gravitational-Wave Observatory (LIGO) and its European partner, Virgo, registered a subtle signal consistent with the merger of two compact objects.
Soon after, the Zwicky Transient Facility at Palomar Observatory in California spotted a rapidly fading red point of light in the same region of the sky, according to the statement. The event's behavior closely resembled that of GW170817 — the only confirmed kilonova, which was observed in 2017 — with its red glow consistent with freshly forged heavy elements such as gold and platinum.
Instead of fading as astronomers typically expect, AT2025ulz began to brighten again, the study reported. Follow-up observations from a dozen observatories around the world, including Hawaii's Keck Observatory, showed the light shifting toward bluer wavelengths and revealing fingerprints of hydrogen, a hallmark of a supernova rather than a kilonova.
That data helped researchers confirm the presence of hydrogen and helium, indicating that the massive star had shed most of its hydrogen-rich outer layers before detonating, the paper noted.
To explain the baffling sequence, the team proposed that a massive, rapidly spinning star collapsed and exploded as a supernova. But instead of forming a single neutron star, its core split into two smaller neutron stars. Those newborn remnants then spiraled together and collided within hours, triggering a kilonova inside of the expanding debris of the supernova.
The combined effect is a hybrid explosion in which the supernova initially masks the kilonova's signature, accounting for the unusual observations, the researchers wrote in the paper.
Clues from the gravitational-wave data bolster this idea. While the signal cannot precisely determine the individual masses of the two merging neutron stars, it does rule out scenarios in which both were heavier than the sun, the new paper noted.
The researchers find a 99% chance that at least one of the objects was less massive than the sun— an outcome that challenges conventional stellar physics, which predicts neutron stars should not weigh less than about 1.2 solar masses. Such lightweight neutron stars can form only when a very rapidly spinning star collapses, matching the scenario proposed for AT2025ulz, according to the statement.
However, the study noted that the complexity of the overlapping signals makes it difficult to rule out the possibility that the signals came from unrelated events that happened to occur close together. Ultimately, the only way to test the theory will be to find more such events using next-generation sky surveys such as those from Vera C. Rubin Observatory and NASA's upcoming Nancy Grace Roman Space Telescope, the researchers said.
"If superkilonovae are real, we'll eventually see more of them," study co-author Antonella Palmese, an assistant professor of astrophysics and cosmology at Carnegie Mellon University in Pennsylvania, said in a different statement. "And if we keep finding associations like this, then maybe this was the first."
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