The monstrous black hole is 6.5 billion times bigger than the sun, and it lies in the centre of an enormous elliptical galaxy, Messier 87, about 55 million light-years away in the constellation Virgo. Two years ago, the team photographed it, producing the first image of a black hole. The previously invisible entity — a porthole to eternity — looked like a fuzzy smoke ring, much as Albert Einstein’s equations had predicted a century ago.
The group has spent the past two years extracting more data from their observations about the polarisation of the radio waves, which can reveal the shape of the magnetic fields in the hot gas swirling around the hole.
Now, seen through the radio equivalent of polarised sunglasses, the M87 black hole appears as a finely whiskered vortex, like the spinning fan blades of a jet engine, pumping matter into the black hole and energy outward into space.
“It’s like putting on a pair of polarised sunglasses on a bright sunny day — all of a sudden you can see what’s going on,” said Sheperd Doeleman, an astronomer at the Harvard-Smithsonian Center for Astrophysics and founding director of the collaboration.
“Now we can actually see the patterns of these fields in M87 and begin to study how the black hole is funnelling material to its centre,” he said.
Daniel Holz, an astrophysicist at the University of Chicago who was not part of the research, said: “These relativistic jets are some of the most extreme phenomena in nature, combining gravity and hot gas and magnetic fields to produce a beam which crosses an entire galaxy. It is exciting that EHT is helping us learn more about what is going on at the heart of these relativistic jets which originate very near the ‘surface’ of a black hole.”
Janna Levin, an astrophysicist at Barnard College of Columbia University who studies black holes but was not part of the EHT team, called the results “thrilling,” as they revealed details about how a black hole can create “a lethal, powerful, astronomical ray gun that extends thousands of light-years.”
The level of detail in the new image, she said, could renew theorists’ interests in features they had given up on ever being able to observe. “A lot of people will be racing back to their pretty calculations, just daydreams in pen on paper, to ask, all excited and nervous, ‘Could the EHT actually see this?’” Levin said. “I’m going to be one of them.”
The results were announced Wednesday in two papers published in the Astrophysical Journal Letters by the Event Horizon Telescope Collaboration, and in a third paper — by Ciriaco Goddi of Radboud University in the Netherlands and a large international cast — that has been accepted by the same journal.
Dark Demons of the Cosmos
Black holes are bottomless pits in space-time, where gravity is so powerful that not even light can escape; whatever enters essentially disappears from the universe. The cosmos is littered with black holes. Many are dead stars that have collapsed in catastrophically on themselves. One sits at the centre of almost every galaxy and is millions or billions of times larger than any star.
Paradoxically, despite their light-swallowing capability, black holes are the most luminous objects in the universe. Material — gas, dust, shredded stars — that falls into a black hole is heated to millions of degrees as it swirls around the drain of doom in a dense maelstrom of electromagnetic fields. Most of that matter falls into the black hole, but some is pushed out, like toothpaste, by enormous pressures and magnetic fields. How all of this energy arises and is marshalled remains unknown to astronomers.
Such fireworks, which can outshine galaxies a thousandfold, can be seen across the universe; when first observed in the early 1960s, they were called quasars. That discovery led physicists and astronomers to first take seriously the notion that black holes exist.
In 2009, eager to explore the underlying mechanisms and to verify Einstein’s predictions about black holes, Doeleman and his colleagues formed the Event Horizon Telescope, an international collaboration composed of about 300 astronomers from 13 institutions.
The telescope is named after the point of no return around a black hole; beyond the event horizon, all light and matter is consumed. In April 2017, when the telescope spent 10 days observing M87, it consisted of a network of eight radio observatories around the globe — “a telescope as big as the world,” as Doeleman likes to say, able to spot details as small as an orange on the moon. The team then took two years to process the data. The results came together in April 2019, when Doeleman and his colleagues presented the first images — radio maps, really — of a black hole, the monster in M87.
Black holes were first “heard” colliding in 2015, by the Laser Interferometer Gravitational-Wave Observatory. Now they could be seen, as an inky portal of nothingness framed by a swirling doughnut of radiant gas in the centre of the galaxy Messier 87.
“We have seen what we thought was unseeable,” Doeleman said at the time. The picture appeared on the front page of newspapers around the world, and a copy is now in the permanent collection of the Museum of Modern Art in New York.
But that was only the beginning of the journey inward.
Inside the Dynamo
It took another two years for researchers to produce the polarised images released Wednesday.
Jets and lobes of radio, X-ray and other forms of energy extend more than 100,000 light-years from the black hole in M87. Much of this radiation comes from energetic electrical particles spiralling around in magnetic fields.
The newly processed image allows the astronomers to trace these fields back to their origins, in a hot, chaotic ring of electrified gas, or plasma, about 30 billion miles across — four times as wide as the orbit of Pluto. That achievement is made possible because the light from the disk is partly polarised, vibrating more in one direction than in others.
“The direction and intensity of the polarisation in the image tells us about the magnetic fields near the event horizon of the black hole,” said Andrew Chael, an astrophysicist at Princeton University who is part of the EHT team.
Astronomers have debated for years whether the magnetic fields surrounding so-called low-luminosity black holes like M87 were weak and turbulent or “strong” and coherent. In this case, Chael said, the magnetic fields are strong enough to disrupt the fall of the gas and transfer energy from the spinning black hole to the jet.
“The EHT images also provide hints that the bright jet in M87 is actually powered from the rotational energy of the black hole, which twists the magnetic fields as it rotates,” said Michael Johnson, another EHT member from the Harvard-Smithsonian Center for Astrophysics.
As a result, Doeleman said, “This gives the emitted radio waves the azimuthal twist” observed in the curving pattern of the new, polarised images. He noted that azimuthal twist would be a “fine name for a cocktail.”
A byproduct of the work, Doeleman said, was that the astronomers were able to estimate the rate at which the black hole is feeding on its environment. Apparently it isn’t terribly hungry; the black hole is eating “a paltry” one-thousandth of the mass of the sun per year.
“Yet it’s enough to launch powerful jets that stretch for thousands of light years, and it’s radiant enough for us to capture it with the EHT,” he said.
Doeleman is already laying the groundwork for what he calls the “next generation” EHT, which will produce movies of this magnetic propulsion structure in action.
“This is really the next big question,” Doeleman said. “How do magnetic fields extract energy from a spinning black hole? We know it happens, but we don’t know how it works. To solve that, we will need to create the first black hole cinema.”
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