Black Hole Image Revealed for First Time Ever

Astronomers announced on Wednesday that at last they had observed the unobserveable: a black hole, a cosmic abyss so deep and dense that not even light can escape it.

“We have seen what we thought was unseeable,” said Shep Doeleman, an astronomer at the Harvard-Smithsonian Center for Astrophysics, and director of the effort to capture the image, during a Wednesday news conference in Washington, D.C.

The image, of a lopsided ring of light surrounding a dark circle deep in the heart of the galaxy known as Messier 87, some 55 million light-years away from Earth, resembled the Eye of Sauron, a reminder yet again of the power and malevolence of nature. It is a smoke ring framing a one-way portal to eternity.

To capture the image, astronomers reached across intergalactic space to Messier 87, a giant galaxy in the constellation Virgo. There, a black hole several billion times more massive than the sun is unleashing a violent jet of energy some 5,000 light-years into space.

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The image offered a final, ringing affirmation of an idea so disturbing that even Einstein, from whose equations black holes emerged, was loath to accept it. If too much matter is crammed into one place, the cumulative force of gravity becomes overwhelming, and the place becomes an eternal trap, a black hole. Here, according to Einstein’s theory, matter, space and time come to an end and vanish like a dream.

On Wednesday morning that dark vision became a visceral reality. As far as the Event Horizon team could ascertain, the shape of the shadow is circular, as Einstein’s theory predicts.

It would have been easy for the theory to come out wrong, said Avery Broderick of the Perimeter Institute for Theoretical Physics in Waterloo, Ontario: “In April 2017 this was the dog that did not bark.”

The results were announced simultaneously at news conferences in Washington, D.C., and five other places around the world, befitting a collaboration involving 200 members and nine telescopes around the world. When the image was put up on the screen in Washington, cheers and gasps, followed by applause, broke out in the room and throughout a universe of astrofans who were following the live-streamed event.

“Einstein must be totally chuffed,” said Priyamvada Natarajan, an astrophysicist at Yale. “His theory has just been stress-tested under conditions of extreme gravity and looks to have held up.”

“What a time to be alive,” said Janna Levin, a cosmologist and professor at Barnard College in New York.

The image emerged from two years of computer analysis of observations from a network of radio antennas called the Event Horizon Telescope. In all, eight radio observatories on six mountains and four continents observed the galaxy in Virgo on and off for 10 days in April 2017.

The telescope array also monitored a dim source of radio noise called Sagittarius A* (pronounced Sagittarius A-star), at the heart of our Milky Way galaxy. There, 26,000 light-years from Earth, and buried in the depths of interstellar dust and gas, lurks another black hole, with a mass of 4.1 million suns.

The network is named after the edge of a black hole, the point of no return; beyond the event horizon, not even light can escape the black hole’s gravitational pull.

The image provided astrophysicists with the first look at the innards of a black hole and a mystery that has tantalized astronomers for more than half a century.

In the 1950s, astronomers with radio telescopes discovered that pearly, seemingly peaceful galaxies were spewing radio energy from their cores — far more energy than would be produced by the ordinary thermonuclear engines that make stars shine. Quasars are the most extreme examples: distant, pointlike fountains of energy that outshine their source galaxies.

Perhaps, astrophysicists thought, the energy was being liberated by matter falling onto supermassive, dense objects — later called black holes. The process would generate energy the way water pouring over Niagara Falls generates sound and spray.

Since then, scientists have devised detailed models of how this would work. As hot, dense gas swirls around the black hole, like water headed down a drain, the intense pressures and magnetic fields cause energy to squirt from either side. As a paradoxical result, supermassive black holes, which lurk in the centers of galaxies, can be the most luminous objects in the universe.

Einstein disliked that idea, but the consensus today is that the universe is speckled with black holes furiously consuming their surroundings.

Now the reality has a face.

The proof that these objects are really black holes would be to find that the darkness at the heart of Virgo was smaller than the mathematical predictions for a black hole. But the more astronomers narrowed it down, the harder they had to work.

Interstellar space is filled with charged particles such as electrons and protons; these scatter the radio waves emanating from a black hole into a blur that obscures details of the source. “It’s like looking through frosted glass,” said Dr. Doeleman, director of the Event Horizon Telescope.

To penetrate the haze and see deeper into the shadows of Virgo, astronomers needed to be able to tune their radio telescope to shorter wavelengths. And they needed a bigger telescope. The bigger the antenna, the higher the resolution, or magnification, it can achieve.

Enter the Event Horizon Telescope, named for a black hole’s point of no return; whatever crosses the event horizon falls into blackness everlasting. The telescope was the dream-child of Dr. Doeleman, who was inspired to study black holes by examining the mysterious activity in the centers of violent radio galaxies such as M87.

By combining data from radio telescopes as far apart as the South Pole, France, Chile and Hawaii, using a technique called very long baseline interferometry, Dr. Doeleman and his colleagues created a telescope as big as Earth itself, with the power to resolve details as small as an orange on the lunar surface.

The data from the South Pole could not arrive before December 2017, Dr. Doeleman said, “because it was Antarctic winter, when nothing could go in or out.”

Last year the team divided into four groups to assemble images from the data dump. To stay objective and guard against bias, the teams had no contact with each other, Dr. Doeleman said.

In the meantime, the telescope kept growing. In April 2018, a telescope in Greenland was added to the collaboration. Another observation run was made of the Milky Way and M87, and captured twice the amount of data gathered in 2017.

“We’ve hitched our wagon to a bandwidth rocket,” Dr. Doeleman said last week. The new observations weren’t included in Wednesday’s reveal, but they will allow the astronomers to check the 2017 results and to track changes in the black holes as the years go by.

“The plan is to carry out these observations indefinitely,” said Dr. Doeleman, embarking on his new career as a tamer of extragalactic beasts, “and see how things change.

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