The Milky Way's supermassive black hole is spinning incredibly fast and at the wrong angle. Scientists may finally know why.

Observations from the Event Horizon Telescope may reveal a secret merger in our supermassive black hole's past, potentially explaining the cosmic monster's unusual spin.

A swirling ring of orange light
A recent photo of Sagittarius A* from the Event Horizon Telescope provides the first glimpse of the supermassive black hole’s spiraling magnetic field lines.
(Image credit: EHT Collaboration)

Astronomers studying the Milky Way's supermassive black hole have found "compelling evidence" that could finally help explain its mysterious past.

Located 26,000 light-years away in the center of our galaxy, Sagittarius A* is a gargantuan tear in space-time that is 4 million times the mass of our sun and 14.6 million miles (23.5 million kilometers) wide.

Ben Turner
Features Editor

Ben Turner is the features editor at Live Science. He covers physics and astronomy, among other topics such as tech and climate change. He graduated from University College London with a degree in particle physics before training as a journalist. When he's not writing, Ben enjoys reading literature, playing the guitar and losing at chess.