After taking the first images of black holes, the ground-breaking Event Horizon Telescope (EHT) is poised to reveal how black holes launch powerful jets into space. Now, a research team led by Anne-Kathrin Baczko from Chalmers University of Technology in Sweden has shown that the EHT will be able to make exciting images of a supermassive black hole and its jets in the galaxy NGC 1052. The measurements, made with interconnected radio telescopes, also confirm strong magnetic fields close to the black hole’s edge.
The main research question for the project’s scientists was how do supermassive black holes launch galaxy-size streams of high-energy particles – known as jets – into space at almost light-speed? Now, scientists have taken an important step towards being able to answer this question, with intricate measurements of the centre of the galaxy NGC 1052, at a distance of 60 million light years from Earth.
The scientists made coordinated measurements using several radio telescopes, providing new insights into the workings of a galaxy and its supermassive black hole. The results are reported in a paper published in the scientific journal Astronomy & Astrophysics on 17 December 2024.
A promising yet challenging target
The work has been led by Anne-Kathrin Baczko, astronomer at Onsala Space Observatory, Chalmers University of Technology.
“The centre of this galaxy, NGC 1052, is a promising target for imaging with the Event Horizon Telescope, but it’s faint, complex and more challenging than all other sources we’ve attempted so far”, says Anne-Kathrin Baczko.
The galaxy has a supermassive black hole that is the source of two powerful jets which stretch thousands of light years outwards through space.
“We want to investigate not just the black hole itself, but also the origins of the jets which stream out from the east and west sides of the black hole as seen from Earth”, says Eduardo Ros, team member and astronomer at the Max Planck Institute for Radio Astronomy in Bonn, Germany.
The team made measurements using just five of the telescopes in the EHT’s global network – including ALMA (the Atacama Large Millimeter/submillimeter Array) in Chile, in a configuration that would allow the best possible estimate of its potential for future observations, and supplemented with measurements from other telescopes.
“For such a faint and unknown target, we were not sure if we would get any data at all. But the strategy worked, thanks in particular to the sensitivity of ALMA and complementary data from many other telescopes,” says Anne-Kathrin Baczko.
Measurements show successful imaging possible in the future
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The scientists are now convinced that successful imaging will be possible in the future, thanks to two new key pieces of information: The black hole’s surroundings shine brightly at just the right frequency of radio waves to be sure that they can be measured by the EHT.
From their measurements, the scientists have also estimated the strength of the magnetic field close to the black hole’s event horizon. The field strength, 2.6 tesla, is about 400 times stronger than the Earth’s magnetic field. That’s consistent with previous estimates for this galaxy.
“This is such a powerful magnetic field that we think it can probably stop material from falling into the black hole. That in turn can help to launch the galaxy’s two jets”, says Matthias Kadler.
Even though the source is as challenging as this, the future looks bright as radio astronomers prepare for new generations of telescope networks, like the NRAO’s ngVLA (next generation Very Large Array) and the ngEHT (The next generation Event Horizon Telescope).
“Our measurements give us a clearer idea of how the innermost centre of the galaxy shines at different wavelengths. Its spectrum is bright at wavelengths around one millimetre, where we can make the very sharpest images today. It’s even brighter at slightly longer wavelengths, which makes it a prime target for the next generation of radio telescopes”, says team member Matthias Kadler, astronomer at the University of Würzburg in Germany.
More about the research
The research paper, The putative center in NGC 1052, by Anne-Kathrin Baczko (Chalmers University of Technolgy, Sweden) and 286 co-authors, is published in the journal Astronomy & Astrophysics. The research team also includes Chalmers scientists John Conway and Michael Lindqvist (both Onsala Space Observatory) and Chiara Ceccobello (now at AI Sweden).
The measurements were made by five telescopes in the EHT network: ALMA (the Atacama Large Millimeter/submillimeter Array) in Chile, the IRAM 30-metre telescope in Spain; the James Clerk Maxwell Telescope (JCMT) and the Submillimeter Array (SMA) in Hawaii; and the South Pole Telescope (SPT) in Antarctica. These were supplemented with measurements from 14 other radio telescopes in the GMVA network (Global Millimetre VLBI Array), in Spain, Finland and Germany, including the 20-metre telescope at Onsala Space Observatory, Sweden, and the telescopes of the VLBA (Very Long Baseline Array) in the US.
The EHT Collaboration involves more than 400 researchers from Africa, Asia, Europe, North and South America. The international collaboration aims to capture the most detailed black hole images ever obtained by creating a virtual Earth-sized telescope.
Read more about EHT here.
All visual materials related to this press release can be downloaded via this link.
For more information, please contact:
Robert Cumming, Communicator, Onsala Space Observatory, Chalmers University of Technology, Sweden. robert.cumming@chalmers.se, +46 70 493 31 14
Anne-Kathrin Baczko, Astronomer, Onsala Space Observatory and Department of Space, Earth and Environment, Chalmers University of Technology, Sweden, anne-kathrin.baczko@chalmers.se
Robert Cumming speaks English and Swedish, Anne-Kathrin Baczko speaks English and German.
At Chalmers, we have podcast studios and broadcast filming equipment on site and would be able to assist a request for a television, radio or podcast interview.
Image captions and credits:
A. (animation) Zooming in on the black hole in the centre of NGC 1052 (artist’s impression).
How do black holes launch their powerful jets? In this visualisation of the centre of galaxy NGC 1052, we zoom in through layers of gas and dust to almost reveal the supermassive black hole. New measurements now show that the final close-up of the black hole – and the origin of its jets – are within the reach of the Event Horizon Telescope.(download the animation here)
Credit: Chalmers University of Technolgy | 3dVision | Johan Bournonville | Anne-Kathrin Baczko
B. The jets and hidden centre of galaxy NGC 1052 (artist’s impression).
In this artist’s impression we are approaching the centre of galaxy NGC 1052. Behind clouds of gas and dust (shown in orange) lies the galaxy’s central supermassive black hole. The two jets of high-energy particles (shown in blue) are launched by the black hole, but no one knows how. Radio telescopes can see through the clouds to reveal the centre of the galaxy.
Credit: Chalmers University of Technolgy | 3dVision | Johan Bournonville | Anne-Kathrin Baczko
C. The hidden centre of galaxy NGC 1052 (artist’s impression).
In this artist’s impression we are nearing the supermassive black hole at the centre of galaxy NGC 1052. Here, material collects in a spinning disk before falling into the black hole, and magnetic fields build up which may help launch the galaxy’s powerful jets.
Credit: Chalmers University of Technolgy | 3dVision | Johan Bournonville | Anne-Kathrin Baczko
D. Galaxy NGC 1052 and its neighbour NGC 1042 in visible light.
NGC 1052 (lower right) is an elliptical galaxy located about 60 million light years from Earth in the constellation Cetus the Whale, seen here in visible light together with its neighbour, the spiral galaxy NGC 1042 (bottom right), and many faint stars in our own galaxy. The image was created from images forming part of the Digitized Sky Survey 2.
Credit: ESA/Hubble, NASA, Digitized Sky Survey 2; Acknowledgement: Davide de Martin.
Mia Halleröd Palmgren
Press Officer
+46 31 772 32 52
mia.hallerodpalmgren@chalmers.se
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