An international team of astronomers co-led by an IAS scholar has identified what appears to be a universal rule governing one of the most dramatic behaviors of black holes: the production of powerful jets. The researchers found that black holes can launch jets at the same critical stage of their feeding cycle, regardless of their size. That includes "stellar-mass" black holes about ten times the mass of our sun as well as supermassive black holes that are millions of times heavier.
The work was carried out by Andrew Mummery, Martin A. and Helen Chooljian Member (2025-30) in the School of Natural Sciences at the Institute for Advanced Study, and Adelle Goodwin, a Forrest Research Foundation Fellow at Curtin University's International Centre of Radio Astronomy Research in Western Australia. Published in Nature Astronomy under the title "A universal critical accretion rate for black hole jet formation," the study brings together years of observations across multiple wavelengths. The researchers combined data from telescopes in America, Australia, India, South Africa, and space.
Their focus was on tidal disruption events, which occur when a star passes so close to a supermassive black hole that intense gravitational forces rip it apart. These events gave the team a rare opportunity to watch how a black hole behaves after suddenly receiving a large supply of stellar material. "We really wanted to figure out this massive puzzle," said Mummery.
"Why do some supermassive black holes blast out radio jets right after shredding a star, while others just sit there looking completely dormant, only to suddenly fire up their jets months or even years later?" Black holes are often compared with cosmic vacuum cleaners, but their feeding behavior is much messier. "When a black hole tears apart a star, it does not swallow everything neatly," Goodwin stated. Some of the stellar material falls toward the black hole, while much of it can be violently expelled into space through powerful outflows.
These enormous cosmic "burps" can carry material across vast distances and can significantly affect the evolution of the galaxies that contain them. A Faster Way to Study Supermassive Black Holes Astronomers have long suspected that black holes obey the same basic physical rules even when their masses differ enormously. Confirming that idea has been difficult because changes around supermassive black holes can normally unfold over thousands or even millions of years.
Tidal disruption events offer a way around that problem. When a star is destroyed, the resulting feeding episode around a supermassive black hole can evolve over just a few years. That gives scientists a much faster view of processes that would otherwise be extremely difficult to track in real time.
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