Hidden in plain darkness
Astrophysicist Maximilian Häberle and his team at the Max Planck Institute forWhile most stars behaved predictably, seven of them, situated near the cluster's centre, moved suspiciously fast — too fast to be explained by the cluster's gravity alone. This indicated the possible influence of a massive, unseen object: a black hole.
50,000 times the size of our Sun!
The rogue velocities of these stars suggest they are being gravitationally tugged by an object between 8,200 and 50,000 solar masses. If true, this would place the candidate black hole in the elusive intermediate-mass range, filling a significant gap between stellar-mass black holes (weighing as much as a single large star) and supermassive black holes like the one at ourIntermediate-mass black holes remain enigmatic, with their existence often debated. Some past candidates for these "middleweight" black holes turned out to be neutron stars instead. However, a confirmed detection would bridge our understanding of how black holes grow, possibly suggesting a stepwise process from stellar-mass to supermassive giants.
Firing up the JWST
Häberle and his team aren’t resting on their laurels. They plan to use theThis cosmic detective story is far from over. As we push the boundaries of our telescopic capabilities, the possibility of uncovering new celestial phenomena keeps the universe as tantalising and mysterious as ever. Whether this candidate in Omega Centauri proves to be a true intermediate-mass black hole or another false alarm, the hunt itself drives our understanding of the cosmos to new heights
The findings of this research have been published in many journals, including Nature and Astronomy & Astrophysics.