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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 Date
    July 13, 2026
  • Science Release
    NASA’s Hubble Discovers First of Star Cluster’s Missing Black Holes
  • Credit
    Animation: NASA, ESA, Matthew Whitaker (U of Utah), Joseph Olmsted (STScI)

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  • Video: Full res, 3840 × 2160, 60 FPS
    mp4 (2.61 MB)

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Details

Last Updated
Jul 13, 2026
Contact
Media

Claire Andreoli
NASA’s Goddard Space Flight Center
Greenbelt, Maryland
claire.andreoli@nasa.gov