Eerste foto van Sagittarius A*, het zwarte gat in de Melkweg

Astronomers reveal first image of the black hole at the heart of our galaxy

Astronomers have unveiled the first image of the supermassive black hole at the centre of our own Milky Way galaxy. This result provides overwhelming evidence that the object is indeed a black hole and yields valuable clues about the workings of such giants, which are thought to reside at the centre of most galaxies.

The image was produced by a global research team called the Event Horizon Telescope (EHT) Collaboration. The image is presented today by EHT Director Huib Jan van Langevelde (JIVE/Leiden University) on a press conference in the European Southern Observatory (ESO) headquarters in Germany.

The team has made use of observations from a worldwide network of radio telescopes. In the Netherlands, astronomers and technicians from University of Amsterdam, Radboud University, Leiden University, University of Groningen, JIVE and ASTRON are part of the EHT collaboration. The EHT team's results are being published today in a special issue of The Astrophysical Journal Letters.

First evidence of Sagittarius A*

The image is a long-anticipated look at the massive object that sits at the very centre of our galaxy. Scientists had previously seen stars orbiting around something invisible, compact, and very massive at the centre of the Milky Way. This strongly suggested that this object — known as Sagittarius A* (Sgr A*, pronounced "sadge-ay-star") — is a black hole, and today’s image provides the first direct visual evidence of it.

Although we cannot see the black hole itself, because it is completely dark, glowing gas around it reveals a telltale signature: a dark central region (called a “shadow”) surrounded by a bright ring-like structure. The new view captures light bent by the powerful gravity of the black hole, which is four million times more massive than our Sun.

“We were stunned by how well the size of the ring agreed with predictions from Einstein’s Theory of General Relativity," said EHT Project Scientist Geoffrey Bower from the Institute of Astronomy and Astrophysics, Academia Sinica, Taipei. "These unprecedented observations have greatly improved our understanding of what happens at the very centre of our galaxy, and offer new insights on how these giant black holes interact with their surroundings.”

Donut on the moon

Because the black hole is about 27,000 light-years away from Earth, it appears to us to have about the same size in the sky as a donut on the Moon. To image it, the team created the powerful EHT, which linked together eight existing radio observatories across the planet to form a single “Earth-sized” virtual telescope. The EHT observed Sgr A* on multiple nights, collecting data for many hours in a row, similar to using a long exposure time on a camera.

Remarkably similar

The breakthrough follows the EHT collaboration’s 2019 release of the first image of a black hole, called M87*, at the centre of the more distant Messier 87 galaxy. The two black holes look remarkably similar, even though our galaxy’s black hole is more than a thousand times smaller and less massive than M87*. "We have two completely different types of galaxies and two very different black hole masses, but close to the edge of these black holes they look amazingly similar,” says Sera Markoff, Co-Chair of the EHT Science Council and a professor of theoretical astrophysics at the University of Amsterdam, the Netherlands. "This tells us that General Relativity governs these objects up close, and any differences we see further away must be due to differences in the material that surrounds the black holes.”

This achievement was considerably more difficult than for M87*, even though Sgr A* is much closer to us. EHT scientist Chi-kwan (‘CK’) Chan, from Steward Observatory and Department of Astronomy and the Data Science Institute of the University of Arizona, US, explains: “The gas in the vicinity of the black holes moves at the same speed — nearly as fast as light — around both Sgr A* and M87*. But where gas takes days to weeks to orbit the larger M87*, in the much smaller Sgr A* it completes an orbit in mere minutes. This means the brightness and pattern of the gas around Sgr A* was changing rapidly as the EHT Collaboration was observing it — a bit like trying to take a clear picture of a puppy quickly chasing its tail.”

The researchers had to develop sophisticated new tools that accounted for the gas movement around Sgr A*. While M87* was an easier, steadier target, with nearly all images looking the same, that was not the case for Sgr A*. The image of the Sgr A* black hole is an average of the different images the team extracted, finally revealing the giant lurking at the centre of our galaxy for the first time.

Already predicted 20 years ago

The effort was made possible through the ingenuity of more than 300 researchers from 80 institutes around the world that together make up the EHT Collaboration. In addition to developing complex tools to overcome the challenges of imaging Sgr A*, the team worked rigorously for five years, using supercomputers to combine and analyse their data, all while compiling an unprecedented library of simulated black holes to compare with the observations.

In 2000, Heino Falcke, EHT board member and professor of astroparticle physics and radio astronomy at Radboud University, the Netherlands, came up with the term ‘black hole shadow’, describing how the black hole diverges the light of the surrounding glowing gas cloud. He predicted that it should be possible to image a black hole using radio telescopes. Together with Sera Markoff, he made the first calculations of the radiation of this black hole. “Now, it seems that the predictions that we made 20 years ago are now confirmed”, says Markoff.

Read more below infographic

Radboud Researchers hunting for black holes

Two black holes imaged

Scientists are particularly excited to finally have images of two black holes of very different sizes, which offers the opportunity to understand how they compare and contrast. They have also begun to use the new data to test theories and models of how gas behaves around supermassive black holes. This process is not yet fully understood but is thought to play a key role in shaping the formation and evolution of galaxies.

“Now we can study the differences between these two supermassive black holes to gain valuable new clues about how this important process works,” said EHT scientist Keiichi Asada from the Institute of Astronomy and Astrophysics, Academia Sinica, Taipei. “We have images for two black holes — one at the large end and one at the small end of supermassive black holes in the Universe — so we can go a lot further in testing how gravity behaves in these extreme environments than ever before.”

Africa Millimetre Telescope

Progress on the EHT continues: a major observation campaign in March 2022 included more telescopes than ever before. The ongoing expansion of the EHT network and significant technological upgrades will allow scientists to share even more impressive images as well as movies of black holes in the near future. Radboud University, together with the University of Namibia, develops the Africa Millimetre Telescope (AMT) on the Gamsberg mountain in Namibia. The AMT telescope, which is expected in 2026, is a crucial addition to the EHT network for making dynamic images of black holes.

More information:

Contact information

  • Geoffrey Bower, EHT-projectwetenschapper, Institute of Astronomy and Astrophysics, Academic Sinica, Taipei, +1-808-961-2945, gbower [at] asiaa.sinica.edu.tw
  • Huib Jan van Langevelde, EHT-projectdirecteur, JIVE en Universiteit Leiden, 06 21201419, langevelde [at] jive.eu
  • Sera Markoff, Vice-voorzitter EHT Wetenschapsraad, Universiteit van Amsterdam, 06-28547250, S.B.Markoff [at] uva.nl
  • Heino Falcke, EHT-bestuur, Radboud Universiteit, +49 1512 3040365, h.falcke [at] astro.ru.nl
  • Communication NOVA/Marieke Baan, h.m.baan [at] uva.nl, 0614322627
  • Science Communication Radboud University, +31 24 361 6000, media [at] ru.nl
Theme
Universe
Institute
Astrophysics

This website is still under construction. More information: 'a new website'.