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science14 March 2026

🌀The Cosmic Collision That Broke the Rules

A black hole and a neutron star were caught spiraling into each other on an oval-shaped orbit — the first time this has ever been seen. It suggests the universe is far more chaotic and surprising in how it births these extreme objects than scientists had assumed.

When two of the universe's most extreme objects — a black hole and a neutron star — fall toward each other, physics has always predicted they should settle into a near-perfect circle before the final collision. Gravity, over time, smooths out any irregularities. That was the assumption.

Then came GW200105.

In March 2026, an international team from the University of Birmingham, the Universidad Autónoma de Madrid, and the Max Planck Institute for Gravitational Physics published a startling re-analysis of a gravitational wave signal first detected in 2020. The signal, ripples in the very fabric of spacetime, told a different story. This neutron star and black hole were orbiting each other on an oval — an ellipse — right up until they merged into a single black hole about 13 times the mass of the Sun.

What are gravitational waves?

When massive objects accelerate through space, they send out ripples in spacetime itself — like the waves a stone makes in a pond, but through the fabric of the universe. These ripples travel at the speed of light and can be detected on Earth by instruments called LIGO (in the United States) and Virgo (in Europe), which measure distortions in space smaller than a fraction of a proton.

Why does an oval orbit matter?

An oval orbit means the two objects did not form quietly and evolve in isolation. Something stirred them — another star nearby, a third companion, gravitational chaos in a dense stellar neighborhood like a globular cluster. The shape of the orbit, researcher Geraint Pratten noted, gives the game away: it tells you the system had a turbulent past before its final, violent end.

Previous analyses of this same event had assumed a circular orbit — and as a result, they got the masses wrong. The black hole was underestimated; the neutron star overestimated. Correcting the assumption corrected the numbers.

A wider lesson

This discovery doesn't just change one data point. It challenges the idea that all neutron star–black hole mergers follow the same quiet story of formation. Some are born in chaos. And that diversity — that messiness — may turn out to be the norm rather than the exception.

As more gravitational wave detections accumulate in the years ahead, scientists expect to find even stranger systems. The universe, it seems, has more ways to make things collide than our models had imagined.

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In loving memory of Saroj Singh