A team of researchers has discovered that winds generated by supermassive black holes are 100 times more powerful than previously thought, carrying energy across distances of approximately 300,000 light-years. The discovery demonstrates that these explosive winds affect the vast expanse of space beyond the galaxies they inhabit.
Details of the research are published in the journal Nature Astronomy on July 28, 2026.
“Black holes are largely known for sucking matter in, but they also eject gas in the form of powerful winds,” says Satoshi Yamada, assistant professor at Tohoku University’s Frontier Institute for Interdisciplinary Sciences (FRIS). “These winds were thought to be contained within the galaxy, but our study revealed that the force is immensely more powerful than previously understood.”
Yamada and his team, comprising colleagues from Kanazawa University and Tokyo Metropolitan University, harnessed the X-ray astronomy satellite XRISM to observe the activity of the quasar H1821+643, which is located in the constellation Draco, approximately 3.4 billion light-years from Earth. Quasars are extremely luminous objects powered by supermassive black holes that actively consume gas.
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X-ray image of the H1821+643 galaxy group obtained with the Chandra X-ray Observatory. The green dashed square indicates the observed region, corresponding to a physical scale of approximately 900,000 light-years on each side. The lower panel shows the energy distribution of X-ray emission lines from iron ions (e.g., at 6.7 keV) in the central region (within a radius of about 300,000 light-years), with observational data (white) overlaid with the best-fit model (red). Compared with a typical galaxy cluster such as the Perseus cluster, the line broadening is significantly more pronounced, indicating highly turbulent and dynamically active hot gas over a wide spatial extent. Credit: Yamada et al.
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Conceptual illustration showing a “blast” driven by a supermassive black hole hidden at the center of a galaxy, with its energy propagating beyond the galaxy and into the surrounding galaxy group environment. The illustration depicts the transport of an enormous amount of energy – equivalent to several billion supernova explosions – into the surrounding space, driving the violent motion of hot gas extending out to distances of approximately 300,000 light-years. Credit: Tohoku University
The rapidly growing black hole is located at the center of the galaxy cluster, where it drives turbulence in the surrounding hot gas that emits X-rays. The researchers precisely determined the motion of the gas by analyzing the emission lines of iron ions.
High-precision observations by XRISM revealed that the high-temperature gas surrounding the black hole does not remain static but violently disperses over a wide area because of turbulence. The researchers also confirmed that the gas flow extends beyond the host galaxy, reaching distances of about 300,000 light-years. The energy involved in the turbulence was approximately 100 times greater than previous estimates and equivalent to several billion supernova explosions—the explosions that occur when stars reach the end of their lives.
“For the first time, we have shown that black holes influence the broader cosmic environment through a shock wave of astonishing power,” Yamada adds. “Black holes are key drivers of gas flows and motion in space, transporting vast amounts of energy to different regions of the cosmos.”
Future observations are expected to further clarify the effects of black holes on their surrounding environment and how matter and elements circulate throughout the cosmos.
Publication details
Satoshi Yamada et al, Vigorous turbulence driven by quasar-mode feedback in a cluster core, Nature Astronomy (2026). DOI: 10.1038/s41550-026-02939-x
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Black hole ‘blast’ reaches 300,000 light-years (2026, July 29)
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