Hubble Discovers Intermediate-Mass Black Hole in Omega Centauri

NASA's Hubble Space Telescope has found compelling evidence for an intermediate-mass black hole in the star cluster Omega Centauri.

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This discovery suggests the presence of an intermediate-mass black hole, filling the gap between stellar-mass and supermassive black holes.

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Omega Centauri is the largest and brightest globular cluster in the Milky Way, located about 16,000 light-years away.

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Hubble detected the black hole through precise measurements of star movements within Omega Centauri, indicating the gravitational influence of a massive unseen object.

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Stars near the core of Omega Centauri exhibit rapid movements, a key indicator of the black hole's presence.

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This discovery impacts our understanding of how black holes merge and grow, providing insights into cosmic phenomena.

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Future Observations

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