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Lead Story · Cosmology
A Supernova That Exploded Five Times
Two foreground galaxies bent the light from one supernova into five separate images. The tiny gaps between when each one arrives are now the cleanest measurement we have of how fast the Universe is expanding.
A team led by Sherry Suyu at TU Munich and the Max Planck Institute for Astrophysics has caught a single supernova showing up five times in the same patch of sky. They nicknamed it SN Winny (formally, SN 2025wny). It went off ten billion years ago.
Between us and the blast sit two foreground galaxies. Their gravity warps spacetime, so the supernova's light bends around them along five different paths. Each path is a slightly different length, which means the same explosion reaches Earth at five slightly different moments. One supernova. Five arrival times.
Nobody has caught a superluminous supernova lensed like this before. The team puts the odds lower than one in a million.
Those lags are a clock. Measure them, drop them into a model of how the two foreground galaxies bend the light, and the Hubble constant — the rate at which the Universe is expanding — falls out directly. It sidesteps the cosmic distance ladder entirely; the catch is that the answer is only as good as the lens model.
Two existing methods disagree about that rate. The mismatch is called the Hubble tension, and it has been cosmology's open wound for a decade. SN Winny is one of the few measurements clean enough to settle which side is right.
Source · TU Munich
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