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Star Orbiting Black Hole Animation
The precise data collected by NASA’s Hubble and James Webb space telescopes enabled a team of astronomers to chart the visible star’s orbital path over a 20 year-plus period. Researchers recorded this segment of the star’s orbit during its closest approach to its stellar-mass black hole companion, oMEGACat BH-2.
Based on the timespan covered by the Hubble-Webb dataset, the team calculated the remainder of the visible star’s orbital path and found that it orbits oMEGACat BH-2 once every 94 years. This makes it the longest-period black hole binary ever known and gives a clue to the pair’s origin. The duo probably formed dynamically, meaning the visible star and its stellar-mass black hole companion found each other in the crowded globular star cluster Omega Centauri.
- Release DateJuly 13, 2026
- Science ReleaseNASA’s Hubble Discovers First of Star Cluster’s Missing Black Holes
- CreditAnimation: NASA, ESA, Matthew Whitaker (U of Utah), Joseph Olmsted (STScI)
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Omega Centauri Context Image
Astronomers found Omega Centauri’s first stellar-mass black hole, which has a visible star companion that is shown in greater detail. They used 20-plus years of data from NASA’s Hubble Space Telescope and recent data from NASA’s James Webb Space Telescope to make the discovery.
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Claire Andreoli
NASA’s Goddard Space Flight Center
Greenbelt, Maryland
claire.andreoli@nasa.gov




