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Millions come to EarthSky for night sky news and trusted science. Your donation keeps us free and accessible for all.<\/strong><\/p>\n Astronomers know of three different categories of black holes. There are the supermassive black holes, which are the beasts that lurk at the centers of galaxies. There are stellar-mass black holes, which form after huge stars die. And then there are intermediate-mass black holes that fill the gap between those two. <\/p>\n Astronomers think the Omega Centauri globular cluster \u2013 a huge collection of 10 million stars that orbits our Milky Way galaxy \u2013 should be home to some 10,000 stellar-mass black holes. But they\u2019d never found any stellar-mass black holes in the cluster \u2026 until now.<\/p>\n On July 13, 2026, ESA said observations with the Hubble and Webb space telescopes have revealed evidence for a stellar-mass black hole in the massive star cluster. The data from these two telescopes allowed astronomers to track a star orbiting a companion for more than 20 years in the cluster. And the star\u2019s invisible dance partner is so heavy that astronomers concluded it must be a black hole. They\u2019ve named the newly found black hole oMEGACat BH-2.<\/p>\n The researchers published their peer-reviewed paper in The Astrophysical Journal Letters<\/em> on July 13, 2026.<\/p>\n Astronomers had searched for stellar-mass black holes in the globular cluster before. Their previous methods of detection included looking for emissions from material falling into the black hole and something called the radial velocity method. This method looks at how fast stars are moving toward or away from us. It can reveal the presence of nearby objects. But these methods never turned up a black hole in Omega Centauri.<\/p>\n Enter astrometry. This is a method where astronomers measure precise locations and movements of stars over time. More than 20 years of data allowed astronomers to get a collection of the precise movements and wiggles of stars in Omega Centauri. And one star revealed it not only had a companion, but the companion was more massive than any star. <\/p>\n Astronomers calculated the companion was too heavy to be something like a neutron star (the dense core of a dead star). But at the same time, it was a bit lighter than they were expecting for a black hole. Co-author Anil Seth of the University of Utah said: <\/p>\n While we already knew that the star was 0.78 solar masses, we can now calculate the black hole\u2019s mass, which is 4.46 solar masses and therefore too heavy to be a neutron star. However, its mass is actually much lower than would be expected in a metal-poor environment like Omega Centauri. This is surprising and exciting. We now know that a metal-poor star should be able to form a black hole like this, and we need to figure out how that happens.<\/p>\n<\/blockquote>\n The astronomers learned that the visible star orbits the black hole \u2013 oMEGACat BH-2 \u2013 once every 94 years. That\u2019s the longest-known period for a star and its black hole.<\/p>\n But the star and black hole don\u2019t appear to be original dance partners. The astronomers said the binary pair likely found each other in the crowded environment of the cluster. <\/p>\n And they won\u2019t remain together forever. Calculations show the star and black hole will stay a pair for less than a billion years before other stars in the cluster tear them apart. It\u2019s not easy being on a packed dance floor.<\/p>\n This black hole and its stellar companion could give astronomers insight into gravitational waves. Gravitational waves are ripples in spacetime. They\u2019re triggered by explosive events in the universe, such as exploding stars or black hole mergers. And the formation of black holes and their influence on companions, like oMEGACat BH-2 and its star, could provide insight into the physics of these events. Seth said: <\/p>\n It\u2019s important to understand black hole populations in globular clusters, because there\u2019s uncertainty about their physics and formation. More specifically, understanding the process of forming black holes and then dynamically forming binaries is vital, because it affects our ability to interpret and understand gravitational wave events. Environments like Omega Centauri are the primary places where we think binaries are merging and creating these waves.<\/p>\n<\/blockquote>\n While this is the first detection of a stellar-mass black hole in Omega Centauri, astronomers believe they\u2019ve already identified an intermediate-mass black hole in the cluster. In 2024, a team of astronomers detected seven fast-moving stars in the innermost region of Omega Centauri. In fact, they\u2019re moving so fast they should escape the cluster. So their existence and speed suggests a massive object \u2013 an intermediate black hole \u2013 is pulling on them. Read more about the intermediate-mass black hole in Omega Centauri here.<\/p>\n10,000 black holes are missing from this star cluster<\/h3>\n
Finding a stellar-mass black hole<\/h3>\n
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More insights into the black hole<\/h3>\n
Insight into gravitational waves<\/h3>\n
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Not the only black hole in Omega Centauri<\/h3>\n