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Credit: NASA’s Chandra X-Ray Observatory
Using an array of telescopes that spans the globe, astronomers detected evidence of magnetic fields near Sagittarius A*, the 4.5-million-solar-mass black hole at the centre of the Milky Way.
Time-Lapse of Supermassive Black Hole Sagittarius A*
Credit; NASA
Decades of theoretical work, including enormous computer simulations, have painted a picture of how strong horizon-scale magnetic fields near the black hole contribute to its growth. Now that this international collaboration has discovered high levels of polarization in the radio emissions from Sagittarius A*, physicists have proof that these magnetic fields indeed exist.
Were these magnetic fields not there, “a lot theoretical astrophysics would have to go back to the drawing board,” says Avery Broderick, an Associate Faculty member at Perimeter Institute for Theoretical Physics, jointly appointed at the University of Waterloo.
Researchers achieved this new finding using the Event Horizon Telescope – an interconnected array of millimeter-wavelength telescopes located around the world. Together, they form an Earth-sized telescope capable of extremely high resolution, which, in the near future, will enable astronomers to image the event horizon of a black hole for the first time in human history.
Those images will enable astrophysicists to transform our understanding of how black holes grow, how they interact with their surroundings, and even the nature of gravity.
“We are on the cusp of a true first in astronomical exploration,” says Avery Broderick. “We fully expect to have imaged a black hole’s event horizon in a matter of years. This would be an incredible accomplishment, not just for science, but humankind.”
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