Double Blast: ESO Telescope captures rare double-star explosion supernova

But a new idea suggests some white dwarfs blow up early. In this model, they collect helium that erupts in a smaller blast first. That shockwave then causes a second, deeper explosion—the real supernova.

Until now, this idea lacked visual proof. But researchers have now found exactly what they predicted: two calcium shells in the remnant, like smoke rings left by the twin explosions. The discovery was made using MUSE, an advanced instrument on the European Southern Observatory’s VLT.

“This is the clearest sign of a double detonation,” said Ivo Seitenzahl, one of the lead scientists. “It shows that white dwarfs don’t need to reach maximum mass before exploding.”

Measuring the Universe with Stellar Clues

Type Ia supernovae aren’t just cosmic light shows. They’ve helped scientists map the universe’s expansion. Their consistent brightness—even across vast distances—acts like a cosmic measuring tape. It was by studying them that astronomers discovered the universe is expanding faster over time, a Nobel-winning revelation.

Priyam Das, a PhD student leading the study, said these explosions shape our view of the cosmos. “They tell us how stars die, how elements form, and even how fast the universe grows,” he said.

His team’s find brings more than just answers—it offers beauty. “The layers left behind are stunning,” Das added. “They’re a window into a star’s final moments.”

Uncovering the Past, Shaping the Future

The star that became SNR 0509-67.5 may be long gone. But what it left behind is rewriting how we understand stellar death. With tools like MUSE and the sharp eyes of astronomers, these ancient explosions are giving up their secrets—one shell at a time.