A black hole named LID-568, previously thought to be consuming matter at an incredible rate, is now seen as more ordinary than once believed. Researchers using the James Webb Space Telescope (JWST) had found this black hole from the early universe, just 1.5 billion years after the Big Bang, apparently feeding 40 times faster than expected. This raised eyebrows among scientists, who questioned if it was really possible for such a black hole to grow so large in such a short time.
However, a recent study published in The Astrophysical Journal corrects these earlier assumptions. The new research indicates that the initial calculations were off due to heavy dust obscuring the black hole. This dust can absorb and scatter light, making objects behind it appear dimmer than they truly are. Myungshin Im, an astrophysicist at Seoul National University, emphasized the importance of addressing dust extinction in measurements. Without proper corrections, scientists risk miscalculating a black hole’s mass and, consequently, its brightness.
In their revised measurements, researchers found LID-568’s mass is just under a billion solar masses, about 40 times less than what was previously thought. They used infrared light to measure the mass. This type of light is less affected by dust than visible light, allowing for more accurate calculations. With the revised mass, LID-568’s luminosity now aligns with established limits known as the Eddington limit, which describes the maximum brightness a black hole can reach based on its mass.
The implications of this study reach beyond LID-568. Astronomers often encounter similar dust issues when studying distant galaxies. Im noted that while adjustments for dust extinction are commonly made in general measurements, they haven’t been sufficiently applied in studies of active galactic nuclei (AGN), where massive black holes dominate the galaxies’ brightness.
Interestingly, this refinement in observing techniques could reshape our understanding of other black holes hidden by dust. The JWST has recently discovered a new category of galaxies referred to as "little red dots," which may reveal even more about dust-obscured black holes.
As researchers build on these findings, they can improve how they study these cosmic giants. This helps bridge different fields and might provide us with a clearer picture of early universe conditions and black hole formation, enhancing our knowledge of how they evolve over cosmic time.