New images from the Event Horizon Telescope (EHT) collaboration have revealed a dynamic environment with changing polarization patterns in the magnetic fields of the supermassive black hole M87*. As shown in the images above, while M87*’s magnetic fields appeared to spiral in one direction in 2017, they settled in 2018 and reversed direction in 2021. The cumulative effects of this polarization change over time suggests that M87* and its surrounding environment are constantly evolving.
Credit: EHT Collaboration
Cambridge, MA— The Event Horizon Telescope (EHT) collaboration has unveiled new, detailed images of the supermassive black hole at the center of the galaxy M87— known as M87*— revealing a dynamic environment with changing polarization patterns near the black hole.
Additionally, the scientists found the first signatures of the extended jet emission near the jet base, which connects to the ring around M87*, in EHT data. These new observations, published today Astronomy & Astrophysics are providing new insight into how matter and energy behave in the extreme environments surrounding black holes. Scientists from the Center for Astrophysics | Harvard & Smithsonian (CfA) are helping lead the international effort to unlock the secrets of M87* and its flipping polarization.
“Using a range of synthetic data tests, we ensured our algorithms could reliably track changes in both the polarization and the black hole shadow of M87*,” said Erandi Chavez, a CfA astronomy graduate student at Harvard University and project collaborator. “These careful checks give us confidence that the shifts we see in M87*’s polarization over the years are genuine, not artifacts of our methods.”
The Center for Astrophysics | Harvard & Smithsonian is a collaboration between Harvard and the Smithsonian designed to ask, and ultimately answer, humanity’s greatest unresolved questions about the nature of the universe. The CfA is headquartered in Cambridge, MA, with research facilities across the U.S. and around the world.
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