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We’ve found the best example yet of an enormous wandering black hole

Astronomers have caught a supermassive black hole straying far from the centre of its galaxy using light from a star being ripped apart
An artist’s impression of a supermassive black hole
Shutterstock/VisualMediaHub

Every massive galaxy astronomers have ever seen has a supermassive black hole at its centre. Some, though, ought to have so-called wandering supermassive black holes closer to their outskirts, too, and researchers have just spotted the most extreme example ever found.

True to their names, black holes don’t emit light, so at the University of Maryland and his team spotted this one only when it devoured a star in what’s known as a tidal disruption event, or TDE. A machine learning algorithm identified the burst of light as a possible TDE in data from the Zwicky Transient Facility (ZTF) in California, and the researchers performed follow-up observations with several other telescopes to confirm it.

This TDE, called TDE 2025abcr, is the most distant from the centre of its host galaxy that we’ve ever seen. “We have a couple of examples of a tidal disruption event that’s very close to the centre of a galaxy but a little offset, and then we have examples where there’s a big galaxy and a little dwarf galaxy merging with it, and that dwarf galaxy has a TDE. This is just an empty patch of sky as far as we can tell,” says Stein. It is more than 30,000 light years from the centre of its galaxy – for comparison, our solar system is about 26,000 light years from the centre of the Milky Way.

Wandering supermassive black holes usually begin their journeys away from a galactic centre due to a merger: two galaxies slam together, and one of their central black holes is flung away. Finding these black holes can tell us about the history and growth of their galaxies. “What’s exciting about this result is that we think it’s the tip of the iceberg,” says Stein. “If we can understand how many wandering supermassive black holes there are, then it can tell us about how many mergers the galaxy has been through and how it’s evolved over time.”

Black holes’ dark nature means that it is extremely difficult to find them; it is mostly accomplished by projects like ZTF that monitor the whole sky for flashes of light. The latest of these projects, the Legacy Survey of Space and Time (LSST) at the Vera Rubin Observatory in Chile, has just begun and is expected to find hundreds more in the coming years, Stein says.

In the meantime, there is a limit to how much we can learn about this particular black hole and its environs. The light from the star being devoured is still too bright to see much of anything else around it. “Some TDEs can last for years and years, so we might have to wait a long time to uncover what’s really going on here,” says Stein.  

Most likely there is a small cluster of stars that is gravitationally tied to the black hole, and one of those caused the TDE as it fell in, but we can’t confirm that until the light fades. At least we don’t have to worry about black holes lurking near Earth, because the sun isn’t in such a cluster, Stein says: “I think it’s very, very unlikely that this is going to happen to our star.”

Journal Reference:

The Astrophysical Journal Letters

Topics: Astronomy / Black holes / Galaxies