The first-ever photographed black hole has changed “radically” in just four years, according to a new study.

Changes in the magnetic field of the black hole M87* are visible in three images taken in 2017, 2018, and 2021. (Image credit: EHT Collaboration)

New images of its dramatically changing environment show that one of the first images ever taken of a black hole is even stranger than we thought.

The object, known as M87*, experienced unexpected changes in its magnetic fields, which show up in polarized light, meaning light waves oriented in the same way (such as vertically or horizontally).

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“With just three images of M87*, we're only just beginning to unravel the galaxy's deep mysteries, but we're confident we can,” Sebastiano von Fellenberg, then a research fellow at Germany's Max Planck Institute for Radio Astronomy (MPIfR), told Live Science in an email.

A black hole comes to light

Images of M87* were taken in 2017, 2018, and 2021 by the Event Horizon Telescope (EHT) collaboration—a global network of radio telescopes that recently added two new observatories in Arizona and France. As its name suggests, the black hole resides at the center of the galaxy Messier 87 (M87), 55 million light-years from Earth.

Now, the EHT, in collaboration with MpiFR, is tracking the “dynamic environment” surrounding the black hole by analyzing these three images, the consortium said in a press release.

M87* is quite massive, more than six billion times the mass of the Sun. New polarization data provides scientists with insight into the structure and strength of the magnetic fields around it.

According to theory, the magnetic fields of supermassive black holes are contained in a disk of plasma (superheated gas) surrounding the black hole. These rotating fields form “magnetic towers” filled with incredible energy.

This energy, in turn, pushes matter along jets stabilized by magnetic fields and moving at speeds close to the speed of light. These jets originate from a small region around the black hole, but still have a significant impact on star formation and energy distribution within the galaxy, which in turn plays a crucial role in its evolution.

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Von Fellenberg, now a research fellow at the Canadian Institute for Theoretical Astrophysics at the University of Toronto, said there are two main takeaways from the work: the polarization is highly variable, but the overall intensity images (topographic images) of M87* remain consistent.

“Both of these results are expected to varying degrees,” he explained. The overall intensity is related to the black hole's gravitational potential, which shouldn't have changed much over the few years the images were taken.

But polarization, he added, “traces the state of the matter and magnetic field in the accretion flow—and, to some extent, along the base of the jet.” Therefore, von Fellenberg said, “the changes we observe imply that each image captures a different state of these properties, which is consistent with theoretical predictions.”

A sharp shift

A major surprise was the polarization measurement obtained in 2021, called the β₂ angle. Compared to previous measurements in 2017 and 2018, this measurement “had changed so dramatically that it no longer corresponded to the electromagnetic energy flux of previous years,” von Fellenberg said.

Or, as officials put it in a press release, the polarization pattern “switched direction” between the three images: the magnetic fields twisted in one direction in 2017, stabilized in 2018, and then reversed in 2021.

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Scientists are trying to explain why this happened. They know from physics that this discrepancy can only be explained if there are no additional polarization changes caused by electrons or matter along the line of sight, known as external Faraday rotation.

This leaves the team with four possible explanations: a change in the underlying structure of the magnetic field, a change in the degree of Faraday rotation, an evolving contribution from different emitting regions (such as a disk or jet), or a combination of the first three factors.

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Elizabeth Howell, Live Science contributor

Elizabeth Howell served as a staff writer for Space.com from 2022 to 2024 and was a regular contributor to Live Science and Space.com from 2012 to 2022. Elizabeth's reporting includes numerous exclusive interviews with the White House, several appearances on the International Space Station, observing five human spaceflight launches on two continents, parabolic flights, working in a spacesuit, and participating in a simulated Mars mission. Her latest book, “Why Am I Taller?” (ECW Press, 2022), was co-authored with astronaut Dave Williams.

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