Astronomers have found the first ever 'wandering' supermassive black hole at the edge of a galaxy

The black hole might've originated from the collision of two galaxies. Here's what we know about it.
Artwork of a black hole surrounded by an accretion disc of material, the light from which is warped by the strong gravity. (Representative Cover Image Source: Photo by MARK GARLICK / SCIENCE PHOTO LIBRARY / Getty Images)
Artwork of a black hole surrounded by an accretion disc of material, the light from which is warped by the strong gravity. (Representative Cover Image Source: Photo by MARK GARLICK / SCIENCE PHOTO LIBRARY / Getty Images)

Astronomers have discovered a supermassive black hole that, after lying dormant for a long time, just woke up to tear a star apart at the edge of a galaxy. While devouring the star, the black hole emitted light, helping the researchers to catch a glimpse of it. The discovery, led by researchers at the University of Maryland, has been reported in a paper published in The Astrophysical Journal Letters.

A supermassive black hole revealed itself with a flash of light, shown at the center of this image in blue, as it wandered the edge of a galaxy.
A supermassive black hole revealed itself with a flash of light, shown at the center of this image in blue, as it wandered the edge of a galaxy. (Image Source: Robert David Stein/University of Maryland/ edited in Canva)

Most galaxies, including the Milky Way, host a supermassive black hole at their centers. However, researchers have long predicted the existence of wandering black holes that might drift in the outer edges of galaxies. Such black holes possibly come from two merging galaxies. But because many of these black holes are not sucking in matter or giving off any light, they silently roam around, going undetected by human surveillance. But the Zwicky Transient Facility (ZTF), a public-private astronomical survey at the Palomar Observatory in California, provided the first evidence of such a wandering black hole.

Black Hole vs. Star: A Tidal Disruption Event (Artist's Concept) (Image Source: NASA Jet Propulsion Laboratory)
Black Hole vs. Star: A Tidal Disruption Event (Artist's Concept) (Image Source: NASA Jet Propulsion Laboratory)

ZTF rapidly scans the night sky to detect moving and exploding celestial objects, recording hundreds of thousands of celestial events each night. Detecting a black hole among such a huge number of objects is akin to finding a needle in a haystack. However, the research team overcame this hurdle by using an artificial intelligence (AI) program capable of detecting a black hole’s presence when it tears a star apart and emits light—a cosmic phenomenon called a tidal disruption event (TDE).

The first picture of a black hole was made using observations of the center of galaxy M87 taken by the Event Horizon Telescope (Image Source: NASA)
The first picture of a black hole was made using observations of the center of galaxy M87 taken by the Event Horizon Telescope (Image Source: NASA)

TDEs are typically documented at the centers of galaxies, but the AI can detect them even if they occur elsewhere in the sky. The UMD team launched its AI program in August 2025, and it detected the wandering black hole just three months later. “This discovery will have a huge impact,” said study co-author Suvi Gezari, an associate professor of astronomy at UMD, in a statement. “It means that we're going to find many more examples of wandering black holes, and we can understand how galaxies and their black holes merge and build up over time.”

Image of the Milky Way and a close-up of  Sagittarius A*. It was made by combining X-ray images from Chandra and infrared images from Hubble. (Resized and set against a black background by Starlust Staff) (Image Credits: X-ray: NASA/UMass/D.Wang et al., IR: NASA/STScI)
Image of the Milky Way and a close-up of Sagittarius A*. It was made by combining X-ray images from Chandra and infrared images from Hubble. (Resized and set against a black background by Starlust Staff) (Image Source: X-ray: NASA/UMass/D.Wang et al., IR: NASA/STScI)

The new black hole lies about 30,000 light-years away from the center of its host galaxy, and its mass is roughly equal to that of the supermassive black hole residing at the center of our galaxy. However, surprisingly, no galaxy has been found to be swirling around it. The researchers think that the black hole might have originated from two colliding galaxies, and offered two possible explanations. 

Binary Black Hole Merger (Image Source: Carl Knox, OzGrav, Swinburne University of Technology)
Illustration of a binary black hole merger (Image Source: Carl Knox, OzGrav, Swinburne University of Technology)

One of them is that during the collision, a larger galaxy cannibalized the smaller one and stripped away its stars, leaving behind only the black hole core. The other scenario indicates that one galaxy already had two black holes (a binary black hole) orbiting each other closely at its center. Now, if a third black hole enters the mix, a complex three-body interaction between the three black holes would oust the smallest one. Continuous monitoring of TDEs can help decide which of the two theories is correct. For the moment, the researchers continue to scan the horizons for further clues so that they can hunt down more wandering black holes, allowing them to better understand how galaxies form. “It is super exciting,” said Gezari. “It’s an example of machine learning opening up a whole new area of research.”

More on Starlust:

Scientists witness a black hole's point of no return for the first time ever 

Astronomers spent 6 years studying a supermassive black hole’s revival. Here’s what they found

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