NASA's Hubble Space Telescope has uncovered compelling evidence of a rare intermediate-mass black hole (IMBH) residing in Omega Centauri.
Unlike the more common supermassive black holes found in galaxy cores or lighter stellar-mass black holes, IMBHs are elusive "missing links" crucial to understanding black hole evolution.
An international team of astronomers has used over 500 images from Hubble to search for evidence of the intermediate-mass black hole.
In a monumental discovery, NASA’s Hubble Space Telescope has uncovered compelling evidence of a rare intermediate-mass black hole (IMBH) residing in Omega Centauri, a massive globular star cluster visible from Earth’s southern hemisphere. Unlike the more common supermassive black holes found in galaxy cores or lighter stellar-mass black holes, IMBHs are elusive “missing links” crucial to understanding black hole evolution.
Let’s delve into the details.
An international team of astronomers has used more than 500 images from NASA’s Hubble Space Telescope — spanning two decades of observations — to search for evidence of the intermediate-mass black hole by following the motion of seven fast-moving stars in the innermost region of the globular star cluster Omega Centauri. These stars exhibited velocities suggesting they were influenced by an exceptionally massive object, estimated to be at least 8,200 times the mass of our Sun—likely an IMBH exerting gravitational pull.
Also read: 5 crazy solar system images captured by NASA’s Hubble Space Telescope
Omega Centauri itself is a colossal cluster containing approximately 10 million stars, nearly rivalling a small galaxy in mass. The discovery of these high-velocity stars supports the hypothesis of an IMBH’s presence, challenging previous theories that suggested a cluster of smaller black holes could account for similar gravitational effects.
“We discovered seven stars that should not be there,” explained Maximilian Haberle of the Max Planck Institute for Astronomy in Germany, who led this investigation. “They are moving so fast that they would escape the cluster and never come back. The most likely explanation is that a very massive object is gravitationally pulling on these stars and keeping them close to the centre. The only object that can be so massive is a black hole, with a mass at least 8,200 times that of our sun.”
Also read: Hubble Space Telescope: What is it and How Does it Work?
Located just 17,700 light-years away, closer than the supermassive black hole at the centre of our Milky Way, this IMBH discovery opens new avenues for studying the formation and behaviour of black holes. Omega Centauri’s visibility to the naked eye has long made it a favourite among stargazers, with its appearance nearly as large as a full Moon when observed from rural areas.
Since its launch over three decades ago, the Hubble Space Telescope, a collaboration between NASA and ESA (European Space Agency), continues to redefine our knowledge of the universe.
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Ayushi Jain
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