Quasars are powered by supermassive black holes that devour surrounding matter at incredible rates, releasing tremendous energy across the electromagnetic spectrum.
Recent observations of billion-solar-mass black holes challenge conventional growth models in astrophysics, as they were observed at redshifts when the universe was less than a billion years old.
Studies suggest that these early quasars have surprisingly short active lifetimes of less than a million years, prompting researchers to explore alternative growth mechanisms like episodic super-Eddington accretion and black hole mergers.
Observations using the Very Large Telescope's MUSE reveal that distant quasars have only recently started intense accretion, challenging current understanding of supermassive black hole growth in the early universe.