A team of astronomers led by Riccardo Middei from the INAF Astronomical Observatory of Rome has been monitoring the Seyfert galaxy ESO 511-G030, where a supermassive black hole has recently revived. Over a span of six years, the black hole brightened by a factor of 10 in ultraviolet and X-ray wavelengths. This revival followed a significant decrease in activity, with the accretion disk showing signs of recovery starting in 2021. The researchers noted that the X-ray emissions lagged behind the ultraviolet brightening, indicating a sequential recovery process. The study suggests that the transition occurred when the black hole was feeding at just below 1% of its maximum rate, aligning with observations in smaller black holes. These findings challenge existing models of accretion disks and emphasize the need for enhanced monitoring of such systems, particularly as the Vera Rubin Observatory prepares to expand the catalog of active galaxies.