Gargantuan Black Hole Jets Are Biggest Seen Yet

Astronomers have spotted the biggest pair of black hole jets ever seen, spanning 23 million light-years in total length. That's equivalent to lining up 140 Milky Way galaxies back to back.

"This pair is not just the size of a solar system, or a Milky Way; we are talking about 140 Milky Way diameters in total," says Martijn Oei, a Caltech postdoctoral scholar and lead author of a new Nature paper reporting the findings. "The Milky Way would be a little dot in these two giant eruptions."

The jet megastructure, nicknamed Porphyrion after a giant in Greek mythology, dates to a time when our universe was 6.3 billion years old, or less than half its present age of 13.8 billion years. These fierce outflows—with a total power output equivalent to trillions of suns—shoot out from above and below a supermassive black hole at the heart of a remote galaxy.

Prior to Porphyrion's discovery, the largest confirmed jet system was Alcyoneus, also named after a giant in Greek mythology. Alcyoneus, which was discovered in 2022 by the same team that found Porphyrion, spans the equivalent of around 100 Milky Ways. For comparison, the well-known Centaurus A major jet system, the closest such system to Earth, spans 10 Milky Ways.

The latest finding suggests that these giant jet systems may have had a larger influence on the formation of galaxies in the young universe than previously believed. Porphyrion existed during an early epoch when the wispy filaments that connect and feed galaxies, known as the cosmic web, were closer together than they are now. That means enormous jets like Porphyrion reached across a greater portion of the cosmic web compared to jets in the local universe.

"Astronomers believe that galaxies and their central black holes co-evolve, and one key aspect of this is that jets can spread huge amounts of energy that affect the growth of their host galaxies and other galaxies near them," says co-author George Djorgovski, professor of astronomy and data science at Caltech. "This discovery shows that their effects can extend much farther out than we thought."

Unveiling a Vast Population

The Porphyrion jet system is the biggest found so far during a sky survey that has revealed a shocking number of the faint megastructures: more than 10,000. This massive population of gargantuan jets was found using Europe's LOFAR (LOw Frequency ARray) radio telescope.

While hundreds of large jet systems were known before the LOFAR observations, they were thought to be rare and on average smaller in size than the thousands of systems uncovered by the radio telescope.

"Giant jets were known before we started the campaign, but we had no idea that there would turn out to be so many," says Martin Hardcastle, second author of the study and a professor of astrophysics at the University of Hertfordshire in England. "Usually when we get a new observational capability, such as LOFAR's combination of wide field of view and very high sensitivity to extended structures, we find something new, but it was still very exciting to see so many of these objects emerging."

Back in 2018, Oei and his colleagues began using LOFAR to study not black hole jets but the cosmic web of wispy filaments that crisscrosses the space between galaxies. As the team inspected the radio images for the faint filaments, they began to notice several strikingly long jet systems.

"When we first found the giant jets, we were quite surprised," says Oei, who is also affiliated with Leiden Observatory in the Netherlands. "We had no idea that there were this many."

To systematically search for more hidden jets, the team inspected the radio images by eye, used machine-learning tools to scan the images for signs of the looming jets, and enlisted the help of citizen scientists around the globe to eyeball the images further. A paper describing their most recent batch of giant outflows, containing more than 8,000 jet pairs, has been accepted for publication in the journal Astronomy & Astrophysics.

Lurking in the Past

To find the galaxy from which Porphyrion originated, the team used the Giant Metrewave Radio Telescope (GMRT) in India along with ancillary data from a project called Dark Energy Spectroscopic Instrument (DESI), which operates from Kitt Peak National Observatory in Arizona. The observations pinpointed the home of the jets to a hefty galaxy about 10 times more massive than our Milky Way.

Giant Metrewave Radio Telescope in India

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Giant Metrewave Radio Telescope in India

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The team then used the W. M. Keck Observatory in Hawai‘i to show that Porphyrion is 7.5 billion light-years from Earth. "Up until now, these giant jet systems appeared to be a phenomenon of the recent universe," Oei says. "If distant jets like these can reach the scale of the cosmic web, then every place in the universe may have been affected by black hole activity at some point in cosmic time," Oei says.

The observations from Keck also revealed that Porphyrion emerged from what is called a radiative-mode active black hole, as opposed to one that is in a jet-mode state. When supermassive black holes become active—in other words, when their immense forces of gravity tug on and heat up surrounding material—they are thought to either emit energy in the form of radiation or jets. Radiative-mode black holes were more common in the young, or distant, universe, while jet-mode ones are more common in the present-day universe. 

W.M. Keck Observatory in Hawai‘i

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W.M. Keck Observatory in Hawai‘i

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The fact that Porphyrion came from a radiative-mode black hole came as a surprise because astronomers did not know this mode could produce such huge and powerful jets. What is more, because Porphyrion lies in the distant universe where radiative-mode black holes abound, the finding implies there may be a lot more colossal jets left to be found.

"We may be looking at the tip of the iceberg," Oei says. "Our LOFAR survey only covered 15 percent of the sky. And most of these giant jets are likely difficult to spot, so we believe there are many more of these behemoths out there."

Ongoing Mysteries

How the jets can extend so far beyond their host galaxies without destabilizing is still unclear. "Martijn's work has shown us that there isn't anything particularly special about the environments of these giant sources that causes them to reach those large sizes," says Hardcastle, who is an expert in the physics of black hole jets. "My interpretation is that we need an unusually long-lived and stable accretion event around the central, supermassive black hole to allow it to be active for so long—about a billion years—and to ensure that the jets keep pointing in the same direction over all of that time. What we're learning from the large number of giants is that this must be a relatively common occurrence."

As a next step, Oei wants to better understand how these megastructures influence their surroundings. The jets spread cosmic rays, heat, heavy atoms, and magnetic fields throughout the space between galaxies. Oei is specifically interested in finding out the extent to which giant jets spread magnetism. "The magnetism on our planet allows life to thrive, so we want to understand how it came to be," he says. "We know magnetism pervades the cosmic web, then makes its way into galaxies and stars, and eventually to planets, but the question is: Where does it start? Have these giant jets spread magnetism through the cosmos?"

The Nature study, "Black hole jets on the scale of the cosmic web," was funded by the Dutch Research Council, the European Research Council, the UK Science and Technology Facilities Council, the UK Research and Innovation Future Leaders Fellowship, and the European Union. Other Caltech authors include graduate student Antonio Rodriguez. Additional authors are Roland Timmerman of Durham University; Reinout J. van Weeren, Huub J.A. Röttgering, and Huib T. Intema of Leiden University (Timmerman is also affiliated with Leiden University); Aivin R.D.J.G.I.B. Gast of the University of Oxford; Andrea Botteon and Francesco de Gasperin of the Institute for Radio Astronomy of Italy's National Institute of Astrophysics; Daniel Stern of the Jet Propulsion Laboratory, which is managed by Caltech for NASA; and Gabriela Calistro Rivera of the European Southern Observatory and the German Aerospace Center.