Astronomers report finding the first evidence of a “missing” black hole in the Omega Centauri globular star cluster, using data from the Hubble and James Webb space telescopes. The object is described as a black hole candidate that was previously not directly observed, despite expectations that many black holes could remain bound within dense star clusters like Omega Centauri. Both outlets describe the discovery as the first of what researchers anticipate could be up to about 10,000 smaller black holes within the cluster. The reports emphasize that the identification is based on space-based observations that reveal clues consistent with an embedded compact object, rather than a previously detected, obvious black hole source. The discovery is framed as an initial step in a larger search, with researchers suggesting that additional candidates may be found as they analyze more data and refine their methods. While the exact number of black holes remains an estimate, the detection supports the idea that a substantial population of stellar-mass black holes may persist in Omega Centauri even if they are difficult to observe directly.