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New Images Revealed Structures Near the first Ever Supermassive Black Hole to be pictured



Scientists have released another, revealing new image of the first ever black hole to be pictured.

 

The latest image is a new look at the massive object, showing how it looks in polarized light.

 

That in turn allows scientists to measure the polarization, and understand how magnetic fields operate so close to a black hole.

 

(This composite image shows three radio-telescope views of the central region of the galaxy Messier 87 (M87), where a jet of fast-moving particles is ejected from the galaxy's core. In these images, the lines indicate polarization -- the alignment of the electric fields in the radio waves coming from the object. The polarization is a signature of the magnetic fields. The ALMA image shows the inner 6000 light-years of the jet. The image from the National Science Foundation's Very Long Baseline Array (VLBA) zooms down to show the inner one light-year of the jet, and the EHT image shows the region closest to the supermassive black hole at the galaxy's core. Labels indicate the observing frequency in GigaHertz (GHz) and the distance indicated by the scale bar below the frequency. Combined, these images allow astronomers to study the structure of magnetic fields from very close to the black hole to thousands of light-years outward from it.)


That could help researchers understand the powerful, energetic jets that are launched out from the core of the black hole’s galaxy, Messier 87 or M87.

 

The new image shows how the area around the black hole looks in polarized light, of the kind that can be seen by people when they wear special sunglasses. A similar effect happens in hot parts of space, where magnetic fields are present.

 

Just as with sunglasses that are polarized, researchers can use the effect to sharpen the image and reduce the glare caused by bright regions. It means that scientists can identify the magnetic field lines that are found at the inner part of the black hole.

 

As well as being a new look at a now-famous region of space, the study marks the first time scientists have been able to measure the polarization so close to the edge of a black hole.

 


(The new image of the region around the supermassive black hole at the core of the galaxy M87, from the Event Horizon Telescope. Lines show polarization of the radio emission from the area closest to the black hole.)


The black hole at the heart of M87 became famous when it was the subject of the first ever image of such an object, released in 2019.


That first picture looked similar, showing a bright shining ring with a dark circle at its center.

 

Since that image was released, scientists have continued to look into the data taken about the object. And they discovered that much of the light around the black hole is polarized, allowing them to get to know the object much more closely.

 

“This unique observation means that for the first time we can map the magnetic fields around a black hole right into the region of the event horizon” said Derek Ward-Thompson, from the University of Central Lancashire and a member of the Event Horizon Telescope team that also produced the first image.

 

“This is exciting because astronomers believe that the magnetic fields are responsible for launching

ionized
 material millions of light years into space in what we call ‘jets’, which can be ten times larger than the entire galaxy.

 

“This was extremely difficult to do, because not only do we have to record the intensity of the light in the manner of a camera, we also have to record its popularization

 in the manner of a pair of polaroid sunglasses. So, in the same way as sunglasses dim the amount of light we see from the sun, the polariser on our telescope dims the amount of light we can see from the black hole, making it much more difficult to detect.”

 

Co-author and EHT collaboration member Dr Ziri Younsi, of UCL’s Mullard Space Science Laboratory, said: “These ground-breaking measurements of the polarization of light produced at the edge of the black hole‘s event horizon provide us with exciting new insights into the physical processes by which black holes feed on matter, and how they are able to power such prodigious relativistic outflows as astrophysical jets.

 

“In particular, they hint at the role played by magnetic fields in these processes.”

 

Dr Jason Dexter, of the University of Colorado, Boulder, US, said: “The observations suggest that the magnetic fields at the black hole‘s edge are strong enough to push back on the hot gas and help it resist gravity’s pull.

“Only the gas that slips through the field can spiral inwards to the event horizon.”

 

The EHT is an international collaboration set up to image a black hole by linking eight ground-based radio telescopes globally to make an Earth-sized virtual telescope with unprecedented sensitivity and resolution.

 

The resolution is sharp enough to measure an orange on the Moon from Earth.

 

The black hole in the image is located in a galaxy called Messier 87, or M87, and is 55 million light years away. It has a mass 6.5 billion times that of the Sun.

 

The bright jets of energy and matter produced by a black hole are one of the galaxy’s most mysterious features.

 

Most matter close to the edge of a black hole falls in, but some of the surrounding particles escape moments before capture and are blown far out into space in the form of jets.

 

Astronomers have relied on different models of how matter behaves near the black hole to better understand this process.

 

But they still do not know exactly how jets larger than the galaxy are launched from its central region, which is as small in size as the Solar System, nor how exactly matter falls into the black hole.

 

Researchers say the observations provide new information about the structure of the magnetic fields just outside the black hole.

 

They found that only theoretical models featuring strongly magnetized gas can explain what they are seeing at the event horizon.

 

The new observations are described in two papers published in The Astrophysical Journal Letters.

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