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Scientists have captured images of magnetic fields around a black hole using polarized light
25.03.2021 [12:18],
Konstantin Khodakovsky

Following the impressive publication of the first image of a black hole in 2021, astronomers have taken another step towards understanding these massive space objects by shedding light on how magnetic fields behave near black holes.

In 2021, the European Southern Observatory (ESO) announced an achievement whose importance for astronomy was difficult to overestimate: researchers managed to obtain the first direct visual image of a supermassive black hole and its «shadow». The studies were carried out using the virtual Event Horizon Telescope (EHT) — a planetary-scale antenna array of eight ground-based radio telescopes.

This was the first ever direct image of a black hole — an object with a mass of 6.5 billion solar masses was captured, lying in the center of the galaxy Messier 87 in the constellation Virgo, 55 million light years from Earth. The image showed a bright ring with a dark center, which was the shadow of a black hole. While taking this image, astronomers noticed a significant amount of polarized light around the black hole, and hard work in this direction made it possible to see magnetic fields.

Polarized light waves have a different orientation and brightness compared to unpolarized light. And just as light is polarized when it passes through some sunglasses, it polarizes when radiation occurs in magnetized and hot environments. Since polarization is a sign of magnetic fields, this image clearly shows that the black hole’s ring is highly magnetized. «This polarized image suggests that the radiation in the ring is probably created by magnetic fields located very close to the event horizon,» — said in an interview with Monika Moscibrodzka, EHT Polarimetry Working Group Coordinator and Associate Professor at Radbud University in the Netherlands.

This is the first time astronomers have managed to measure polarization so close to the edge of a black hole. The new image of the black hole is not only impressive, but also provides information about the powerful jets emitted from the M87. Bright jets are jets of energy and matter emanating from the core of galaxy M87 and extending 5,000 light-years from the center of the galaxy. This is one of the most mysterious and striking in terms of energy release features of this galaxy. Most of the matter around the black hole gets inside it, but some particles escape absorption and are ejected far into the universe in the form of jets.

Pictured is a jet in the galaxy M87 in polarized light

“In the first images we showed only the intensity,” said Ms Moskibrodzkaya of the first released image of the object. «We’ve now added polarization information on top of the original image.».

“The new polarized images mark an important step towards learning more about gas near a black hole and, in turn, how black holes grow and emit jets,” said an assistant professor at the University of Colorado at Boulder and coordinator of the EHT theoretical working group. Jason Dexter in Space

“EHT radio telescopes have receivers capable of detecting signals from space in polarized light,” said Ivan Marti-Vidal, coordinator of the EHT Polarimetry Working Group and distinguished researcher of Ghent at the University of Valencia in Spain. «These polarized receivers work just like the polarized sunglasses that some people use.».

By showing the black hole in galaxy M87 through polarized light, the team gained a better understanding of the black hole’s event horizon, also known as the «point of no return». This is a space-time region, whose gravitational attraction is so great that not a single object, including light quanta, can leave it. They were also able to better study the interaction with the object’s accretion disk — a cloud of hot gas and other diffuse material that falls towards the black hole and swirls around it.

The team’s observations and this new look at an object in galaxy M87 deepens scientists’ understanding of the structure of magnetic fields directly outside the black hole — it remains a mystery how jets larger than the galaxy itself radiate from the black hole.

“Astronomers have long believed that the magnetic fields carried by hot gas near black holes play an important role in the entry of gas into the interior and launch of relativistic jets of energy particles into the surrounding galaxy. The polarized image that we see speaks of the structure and strength of these magnetic fields very close to the black hole in M87, from where the jets are launched, «said Mr. Dexter.

These observations not only revealed magnetic fields at the edge of the black hole in M87, but also showed that the gas there is very highly magnetized.

“The main discovery is that not only do we see magnetic fields near the black hole, as expected, but they also appear to be strong. Our results show that magnetic fields can move gas around a black hole and interfere with its propagation. The result is an interesting clue to how black holes grow by absorbing gas, «added the scientist.

“We still don’t know all the details about how jets are created, but we do know that magnetic fields can play a crucial role in this process,” said Mr Marty-Vidal. In the future, the team hopes to continue observing M87 not only in the polarized spectrum, but also at different wavelengths of light, in order to build a more complete picture of the space around the black hole and study the magnetic fields in more detail.

The work was published in two articles in the Astrophysical Journal Letters by the EHT team, which brings together more than 300 researchers from organizations around the world.

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