![]() Studying supermassive black holes such as Sagittarius A* will help scientists learn more about how galaxies evolve over time and how they congregate in vast clusters across the universe. The image also constitutes “one of the most important visual proofs of general relativity,” our current best theory of gravity, says Sera Markoff, an astrophysicist at the University of Amsterdam and member of the EHT collaboration. The latest image tells the tale of the epic journey of radio waves from the center of the Milky Way, providing unprecedented detail about Sagittarius A*. The blurry orange ring seen in the images are an elaborate reconstruction of these radio waves captured by eight telescopes scattered around the Earth, collectively known as the Event Horizon Telescope (EHT). As plasma spirals around the black hole, its accelerating particles emit radio waves. The plasma is composed of high-energy charged particles. They actually record portions of the flat pancake of hot plasma swirling around the black hole at high speeds in what’s known as the accretion disk. These “photos” do not, of course, directly show a black hole, defined as the region of space inside a point-of-no-return barrier known as an event horizon. The black hole shadow and emission ring shown here are gravitationally-lensed projections of the far-side of the black hole’s event horizon and accretion disk, respectively. Those radio waves are bent and warped by gravity (through the effect of “gravitational lensing”) to produce the image of the orange outer circles. Hot plasma speeds around the massive object in the accretion disk, emitting radio waves. ![]() The point at which no light can escape from the black hole, called the event horizon, is determined by this mass and by the spin of the black hole. The mass of the black hole determines its size, or what scientists call its gravitational diameter. The new image of the black hole Sagittarius A*, confirms and refines previous predictions of its size and orientation. Doing so required an international collaboration of hundreds of astronomers, engineers and computer scientists, and the development of sophisticated computer algorithms to piece together the image from the raw data. So even though the observations of our own black hole were conducted at the same time as M87’s, it took three additional years to create the picture. But the Milky Way’s black hole, Sagittarius A*, is actually much smaller than the first and was more difficult to see, since it required peering through the hazy disk of our galaxy. The image shows an orange, donut-shaped blob that looks remarkably similar to the earlier picture of the black hole in the center of galaxy Messier 87. Then, in spring 2022, astronomers unveiled another black hole photo - this time of the one at the center of our own Milky Way. So great fanfare accompanied the release in 2019 of the first image of a black hole. It would seem, then, that a black hole should be invisible - and taking its picture impossible. Light itself can’t escape a black hole’s hungry pull. They imprison forever anything that enters.
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