Unraveling the Mysteries of Supermassive Black Holes: A Glimpse into the Early Universe
In a groundbreaking discovery, astronomers have identified a supermassive black hole located in the galaxy LID-568 that is challenging our understanding of black hole formation and growth. This black hole, observed just 1.5 billion years after the Big Bang, is consuming material at an astonishing rate—more than 40 times the Eddington limit, a theoretical threshold that governs the maximum rate at which black holes can accrete matter.
The Eddington limit plays a crucial role in black hole accretion theory. As black holes consume surrounding material, it forms an accretion disk that spirals around the event horizon. The radiation pressure generated by this infalling matter eventually becomes strong enough to counterbalance further accretion, effectively capping the growth rate of the black hole. However, the black hole in LID-568 is defying this limit, exhibiting a luminosity far exceeding expectations for its size. This remarkable behavior was confirmed through observations from the James Webb Space Telescope (JWST) and the Chandra X-ray Observatory.