Event Horizon Telescope

EXPERT REACTION: Astronomers capture first ever image of a black hole

Embargoed until: Publicly released:
Researchers have connected a global network of radio dishes to capture the first-ever image of a black hole. The Event Horizon Telescope (EHT) project and the National Science Foundation (NSF) held a press conference on Wednesday, April 10, 2019, 9 a.m. EDT (April 10 at 11pm AEDT) to announce the findings. Here's what the experts had to say.

Journal/conference: The Astrophysical Journal Letters

Link to research (DOI): 10.3847/2041-8213/ab0ec7

Organisation/s: The University of Queensland, The Australian National University, The University of New South Wales, OzGRav, International Centre for Radio Astronomy Research (ICRAR), UNSW Canberra, Swinburne University of Technology, Macquarie University, University of Western Australia, Monash University, Curtin University, University of Technology Sydney (UTS), University of Sydney

Media Release

From: National Science Foundation, USA

Astronomers capture first image of a black hole

National Science Foundation and Event Horizon Telescope contribute to paradigm-shifting observations of the gargantuan black hole at the heart of distant galaxy Messier 87


WASHINGTON - The Event Horizon Telescope (EHT) — a planet-scale array of eight ground-based radio telescopes forged through international collaboration — was designed to capture images of a black hole.

Today, in coordinated press conferences across the globe, EHT researchers reveal that they have succeeded, unveiling the first direct visual evidence of a supermassive black hole and its shadow.

This breakthrough was announced in a series of six papers published in a special issue of The Astrophysical Journal Letters. The image reveals the black hole at the center of Messier 87, a massive galaxy in the nearby Virgo galaxy cluster. This black hole resides 55 million light-years from Earth and has a mass 6.5-billion times that of the Sun.

“This is a huge day in astrophysics,” said NSF Director France Córdova. “We’re seeing the unseeable. Black holes have sparked imaginations for decades. They have exotic properties and are mysterious to us. Yet with more observations like this one they are yielding their secrets. This is why NSF exists. We enable scientists and engineers to illuminate the unknown, to reveal the subtle and complex majesty of our universe.”

The EHT links telescopes around the globe to form an Earth-sized virtual telescope with unprecedented sensitivity and resolution. The EHT is the result of years of international collaboration and offers scientists a new way to study the most extreme objects in the Universe predicted by Einstein’s general relativity during the centennial year of the historic experiment that first confirmed the theory.

"We have taken the first picture of a black hole," said EHT project director Sheperd S. Doeleman of the Center for Astrophysics | Harvard & Smithsonian. "This is an extraordinary scientific feat accomplished by a team of more than 200 researchers."

The National Science Foundation (NSF) played a pivotal role in this discovery by funding individual investigators, interdisciplinary scientific teams and radio astronomy research facilities since the inception of EHT. Over the last two decades, NSF has directly funded more than $28 million in EHT research, the largest commitment of resources for the project.

Black holes are extraordinary cosmic objects with enormous masses but extremely compact sizes. The presence of these objects affects their environment in extreme ways, warping spacetime and super-heating any surrounding material.

"If immersed in a bright region, like a disc of glowing gas, we expect a black hole to create a dark region similar to a shadow — something predicted by Einstein’s general relativity that we’ve never seen before," explained chair of the EHT Science Council Heino Falcke of Radboud University, the Netherlands. "This shadow, caused by the gravitational bending and capture of light by the event horizon, reveals a lot about the nature of these fascinating objects and allowed us to measure the enormous mass of M87’s black hole."

Multiple calibration and imaging methods have revealed a ring-like structure with a dark central region — the black hole’s shadow — that persisted over multiple independent EHT observations.

"Once we were sure we had imaged the shadow, we could compare our observations to extensive computer models that include the physics of warped space, superheated matter and strong magnetic fields. Many of the features of the observed image match our theoretical understanding surprisingly well," remarks Paul T.P. Ho, EHT Board member and Director of the East Asian Observatory. "This makes us confident about the interpretation of our observations, including our estimation of the black hole’s mass."

Creating the EHT was a formidable challenge that required upgrading and connecting a worldwide network of eight pre-existing telescopes deployed at a variety of challenging high-altitude sites. These locations included volcanoes in Hawai`i and Mexico, mountains in Arizona and the Spanish Sierra Nevada, the Chilean Atacama Desert, and Antarctica.

The EHT observations use a technique called very-long-baseline interferometry (VLBI). which synchronizes telescope facilities around the world and exploits the rotation of our planet to form one huge, Earth-size telescope observing at a wavelength of 1.3mm. VLBI allows the EHT to achieve an angular resolution of 20 micro-arcseconds — enough to read a newspaper in New York from a sidewalk café in Paris.

The telescopes contributing to this result were ALMA, APEX, the IRAM 30-meter telescope, the James Clerk Maxwell Telescope, the Large Millimeter Telescope Alfonso Serrano, the Submillimeter Array, the Submillimeter Telescope, and the South Pole Telescope. Petabytes of raw data from the telescopes were combined by highly specialized supercomputers hosted by the Max Planck Institute for Radio Astronomy and MIT Haystack Observatory.

The construction of the EHT and the observations announced today represent the culmination of decades of observational, technical, and theoretical work. This example of global teamwork required close collaboration by researchers from around the world. Thirteen partner institutions worked together to create the EHT, using both pre-existing infrastructure and support from a variety of agencies. Key funding was provided by the US National Science Foundation, the EU's European Research Council (ERC), and funding agencies in East Asia.

"We have achieved something presumed to be impossible just a generation ago," concluded Doeleman. "Breakthroughs in technology, connections between the world's best radio observatories, and innovative algorithms all came together to open an entirely new window on black holes and the event horizon."

For additional information and resources, please visit: NSF Exploring Black Holes.


  • Dimitrios Psaltis, University of Arizona in Tucson, EHT project scientist
    "The size and shape of the shadow matches the precise predictions of Einstein’s general theory of relativity, increasing our confidence in this century-old theory. Imaging a black hole is just the beginning of our effort to develop new tools that will enable us to interpret the massively complex data that nature gives us."
  • Colin Lonsdale, Director of MIT Haystack Observatory
    “What really made this realistic as a science goal was technology provided by the computing world, which finally caught up, and overtook, costly custom-built instrumentation.  Haystack adapted newly available high-capacity hard disk drives and fast, flexible processor chips, and designed them into systems that could be used for VLBI. Once that key transition had occurred, successive generations of the systems could readily take advantage of industry-driven performance increases over time, and after more than a decade, the prodigious recording and processing speeds demanded by the EHT and black hole imaging were made a reality.”
  • Tony Beasley, director of NSF's National Radio Astronomy Observatory
    "Through its leadership in ALMA and long-term support for the EHT, NRAO has once again helped to advance our understanding of the cosmos and the fundamental laws physics. This observation clearly illustrates the value of radio astronomy to scientific advancement. The next generation of radio telescopes, including the Next Generation VLA, will yield many more groundbreaking results."


  • Event Horizon Telescope
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  • Event Horizon Telescope
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    Paper I: The Shadow of the Supermassive Black Hole
  • Event Horizon Telescope
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    Paper II: Array and Instrumentation
  • Event Horizon Telescope
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    Paper III: Data processing and Calibration
  • Event Horizon Telescope
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    Paper IV. Imaging the Central Supermassive Black Hole
  • Event Horizon Telescope
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    Paper V. Physical Origin of the Asymmetric Ring
  • Event Horizon Telescope
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    Paper VI. The Shadow and Mass of the Central Black Hole

Expert Reaction

These comments have been collated by the Science Media Centre to provide a variety of expert perspectives on this issue. Feel free to use these quotes in your stories. Views expressed are the personal opinions of the experts named. They do not represent the views of the SMC or any other organisation unless specifically stated.

Samuel Hinton is a PhD student at the University of Queensland, researching cosmology and the dark universe

For decades cosmological models have predicted black holes, and black holes have been validated over and over again with indirect evidence. So it's easy to lose sight of the fact that - until now - we've never actually seen one. But the Event Horizon Telescope has peeled back the curtain and given us our first direct image of an event horizon - the boundary in spacetime that wraps a singularity - the boundary at which, once passed, nothing can ever leave. And we've got it on picture. Lying in the heart of supergiant galaxy Messier 87 is a supermassive black hole dwarfing anything inside the Milky Way, a black hole more than six billion times the mass of our sun. Surrounded by a fiery maelstrom of infalling matter over a hundred billion degrees in temperature, we see the event horizon, a region of deathly calm in the most chaotic region of space ever imaged. This black hole allows us to measure Einstein's General Theory of Relativity in the drastically curving region of spacetime around an event horizon, and Einstein's Theory passes yet one more test with flying colours.

Last updated: 14 Oct 2019 3:00pm
Declared conflicts of interest:
None declared.
Dr David Gozzard is a Forrest Postdoctoral Fellow in the International Centre for Radio Astronomy Research at the The University of Western Australia and has contributed to the design and development of the Square Kilometre Array radio telescope.

This is really exciting because it is the first time we have got a clear look at a black hole. The black hole’s event horizon is where the laws of physics as we know them break down. Studying this region is crucial to understanding what goes on inside a black hole, what happened at the moment of the Big Bang, and the deeper underlying laws of nature. But this is just the start. The image is still pretty blurry. It’s like looking through frosted glass. As we work to make our telescopes get bigger and more powerful, we can expect many more exciting images and discoveries to come.

Last updated: 16 Apr 2019 5:47pm
Declared conflicts of interest:
None declared.

Ms Fiona Panther is an Associate Lecturer at UNSW Canberra at ADFA

The image that you see of the supermassive black hole comes from material that has teetered on the brink of a supermassive black hole. This material emits millimetre radio waves, that reach telescopes on Earth after a journey that took 55 million years. Collecting and analysing these radio waves is a challenging task and these remarkable images are a testament to how human curiosity about our universe, and our ability to collaborate, can be harnessed to do incredible things. The new challenge will be to interpret what has been observed, and to investigate how the new knowledge we have gained fits into our current understanding of how black holes work.

Last updated: 11 Apr 2019 3:39pm
Declared conflicts of interest:
None declared.
Daniel Terno is an Associate Professor in the Department of Physics and Astronomy at Macquarie University

The images synthesized from the data obtained by the Event Horizon Telescope collaboration for the first time show the black hole shadow surrounded by the bright light ring, the key signature of black holes predicted by general relativity and a variety of other ultra-compact objects that are produced in more or less exotic models.

That means that now we know that the black hole candidates are true ultra-compact objects. Now the race begins: there are many reasons to suspect (and Hawking’s works were one of the primary motivations) that what is inside is not a black hole, and many arguments why it can or should be. Now the game to find out what is in the shadow truly begins.

Last updated: 11 Apr 2019 2:17pm
Declared conflicts of interest:
None declared.
Martin Bell is an astrophysicist and lecturer at University of Technology Sydney

The result is an outstanding achievement and certainly provides the strongest direct evidence for the existence of (Kerr) black holes. The result makes use of a technique called Very Long Baseline Interferometry (VLBI) which connects radio telescopes over long distances to increase resolution.

This is not a new idea, in fact, it is one of the oldest tricks in the book. Nature and evolution long ago worked out that it was better for humans (and other animals) to have two eyes (separated by some distance) rather than one central eye, to help us see further and catch prey.

In the cases of imaging a black hole, we must separate our radio telescopes by Earth-size distances to help us hunt black holes. This work will allow theorists and astrophysics alike to really probe some of the fundamental physics of black holes and in future observations, I hope we will see imaging of our own black hole at the centre of the Milky Way, Sag A*

Last updated: 11 Apr 2019 2:14pm
Declared conflicts of interest:
None declared.
Professor Karl Glazebrook is Director and Distinguished Professor at the Centre for Astrophysics and Supercomputing, Swinburne University of Technology

This is an extremely significant result. Astronomers have been talking about observing black holes for years, but this is the first image with enough resolution to actually resolve the Schwartzchild radius - the radius of the event horizon. General relativity (GR) of course predicts black holes and there are a variety of observations in astronomy that are explained by black holes, for example, the high-energy activity seen in the centre of galaxies. Motions of stars in the centre of our galaxy show the presence of a compact massive object, and the orbits show general relativistic effects. In fact, astronomers take the existence of black holes pretty much for granted. 

However, we have never had an actual image of the event horizon of a black hole, the existence of which is a key GR prediction. Maybe gravity is different from GR in these extreme strong field regime and we get something different to a black hole but which still is massive and dark and looks the same at large scales? These observations demonstrate that the event horizon exists in the monster black hole at the centre of the galaxy M87. What is actually seen is a ring of light, caused by the gravity of the hole bending light around it at the scale of the horizon, and this ring can be compared with detailed predictions from GR - which one of the papers does! I expect future work will compare this data with non-GR models now we have the capability.

I believe it is the highest resolution image ever made, it uses the technique of 'Very Long Baseline Interferometry' where radio telescopes all across the earth have their signals electronically combined to make a virtual telescope with a resolution equivalent to one the size of the Earth. However, it does this at super high radio frequencies (230 Ghz) which gives even higher resolution. This is technically challenging, and you have to combine a lot of telescopes to get a decent image, and this is the first time that has been done. M87 is 50 million light years away and the event horizon is only the size of our solar system. (The radius is about 3x Pluto’s orbit).

This has been an exciting few years for black hole science! First, we discovered the first gravitational wave signals from monster black holes merging, and how this exciting image! It is a fantastic time to live through.

We have been expecting these results from the Event Horizon Telescope project for a year or two now, next we will see the more technically challenging observation of the black hole at the centre of our galaxy. This is more challenging because the gravitational timescale here (time for matter to swirl around the hole in a final orbit) would be less than a minute, compared to a day for M87. This complicates the analysis but on the flip side if this can be done we may look forward to seeing a cool movie emerging especially if the telescope is able to capture the black hole consuming a large chunk of matter being consumed in real time!

Last updated: 11 Apr 2019 2:13pm
Declared conflicts of interest:
None declared.
Ms Teresa Slaven-Blair is a PhD candidate at the University of Western Australia where she is researching gravitational wave astrophysics, and is a science member of OzGrav and the LIGO/Virgo Collaboration

We have had good evidence that black holes exist for a long time. We have been observing their effects on the motion of the stars around them, and the way they warp spacetime as they collide. This is the first time we can see the light swirling around the event horizon of a black hole right before falling into it, never to be seen again. It’s this evidence of light being removed from the Universe that is so amazing.

Last updated: 11 Apr 2019 2:12pm
Declared conflicts of interest:
None declared.
Dr Christian Wolf is from the Research School of Astronomy and Astrophysics at the ANU College of Science

[Pre-press conference comment:] The only black holes anyone has seen so far have been works of fiction. We have watched movie heroes battle with the immense gravitational attraction of giant black holes, but what do these black holes really look like?

With my team, I am hunting for black holes that grow and these are ablaze with light. But most black holes in the Universe are dormant, such as the one at the centre of our own Milky Way galaxy. All we can hope to see is their shadow in the darkness of space – that strikes me as one of the hardest pictures to take, ever.

The Event Horizon Telescope team have worked for years to construct a picture of these two black holes, which are the two easiest ones to image. I very much hope this is only the beginning, because there are billions of giant black holes out there, one in the centre of every galaxy.

Last updated: 11 Apr 2019 2:09pm
Declared conflicts of interest:
None declared.
Professor Matthew Colless is Director of the Research School of Astronomy and Astrophysics at ANU

[Pre-press conference comment:] This image is going to be the most visually direct image of a black hole so far. There’s been a long-standing challenge to capture an image of a black hole’s immediate surroundings – the region around its event horizon, from inside which no light or other electromagnetic radiation can escape.

What we will see is the absence of background radiation where the supermassive black hole is and a ring of light around it caused by stars and gas falling into the black hole and creating huge amounts of friction and heat. Depending on how sharp this image will be, the detail of the black hole’s shape and the distortions of gravity it produces could offer a test of Albert Einstein’s theory of General Relativity.

This theory, one of the most extraordinary scientific achievements of the 20th century, explains that the force of gravity arises from the curvature of space and time. This new black hole image could confirm whether Einstein was right or whether we need to revisit this theory.

The Event Horizon Telescope is working at a radio wavelength of 1.3mm, a very short wavelength in the context of radio astronomy. The shorter the wavelength, the sharper the image, so we can hope to see very fine detail in this first-ever image of a black hole.

Last updated: 11 Apr 2019 2:08pm
Declared conflicts of interest:
None declared.
Dr Brad Tucker is a Research Fellow and Outreach Manager at Mt. Stromlo Observatory at the Australian National University

[Pre-press conference comment:] Black holes are some of the most fascinating objects in the Universe. In the past few years, we’ve made great progress in understanding these objects. And today we make another big leap – being able to see the effects of a black hole.

The direct image of the event horizon is amazing. It allows us to directly measure how black holes affect gravity and time. I never thought we would be able to see something that has been so mysterious.

Last updated: 11 Apr 2019 2:07pm
Declared conflicts of interest:
None declared.
Professor Geoff Bicknell is from the Research School of Astronomy and Astrophysics at the ANU College of Science

[Pre-press conference comment:] The observations with the Event Horizon Telescope may provide crucial information on the way in which the interactions of black holes with surrounding matter produce energy. This is relevant to all black holes in the Universe.

The observations may also tell us the way in which jets moving close to the speed of light are accelerated away from the black hole, as well as improving our understanding of the composition of plasma which is ejected from the black hole environs.

Last updated: 11 Apr 2019 2:07pm
Declared conflicts of interest:
None declared.
Professor Alister Graham is from the ARC Centre for Gravitational Wave Discovery, Swinburne University of Technology

Astronomers have successfully observed the invisible.

An enigmatic monster of the Universe has just been imaged.

The self-created cloak of invisibility around the black hole has betrayed its presence. 

A 55 million-year-old photo of a spinning black hole 6.5 billion times the mass of our Sun.  

Having spent years studying the influence of these previously unobservable objects, it feels like a validation. 

Observationally confirmed a quarter of a century ago, this shadow of a black hole removes any shadow of a doubt as to their existence.

Outflows from these massive black holes shape the galaxies upon which they feed.

This has driven global research into black holes for over 20 years. 

At Swinburne University, we have studied these connections and interplays in over 100 galaxies with directly measured black hole masses. Their existence has now been further confirmed by this beautiful fuzzy ring showing the silhouette of a black hole.  We have studied and dissected images of these galaxies, using infrared images from the Spitzer Space Telescope.  

This photon ring illuminating a black hole's event horizon also provides the world with an undeniable ring of truth to Einstein's theory which told us over 100 years ago how our Universe operates."


"Observing the hole in this supermassive doughnut is a testament to humanity's scientific capacity.

To have dreamt up the existence of black holes in the 1700s, confirmed their reality a quarter of a century ago, and now imaged the ghostly silhouette of one, is truly remarkable.

Furthermore, from an engineering standpoint, what has been accomplished is akin to seeing a pinhead from ten thousand kilometres."


In an extraordinary feat of science and engineering, astronomers have attained an image resolution equivalent to observing a pinhead at a distance of ten thousand kilometres. They have achieved this by effectively linking many of the world's radio telescopes with the intent of seeing the first-ever silhouette of a black hole.

The upcoming announcement from the international Event Horizon Telescope (EHT) team is expected to show the dark face, the so-called "event horizon", of our Milky Way galaxy's central black hole, with a mass four million times that of the Sun. While this black hole is located 240 million billion km away, when feeding, such supermassive black holes can influence their entire galaxy.

The results are expected to provide further confirmation of Einstein's theory of relativity, famously known for distorting space and time, no doubt also happily along with the minds of many science enthusiasts and science fiction fans.

Although black holes were confirmed to exist from observations a quarter of a century ago, the anticipated radio image should be able to see detail just three times the size of the black hole's event horizon - the infamous boundary marking the point of no return. This close to the gravitational prison, from which not even light is fast enough to escape, Einstein's astonishing general relativistic effects should be apparent, revealing the shadow of the black hole.
The power of the human spirit to predict, discover, and then directly observe the invisible face of a black hole is a remarkable achievement.

Last updated: 11 Apr 2019 2:05pm
Declared conflicts of interest:
None declared.
Dr Adam Deller is an Associate Professor of Astrophysics at Swinburne University of Technology and an Australian Research Council Future Fellow

This was an amazing technical feat – to make it work, the EHT team used radio telescopes that are thousands of kilometres apart and lined up the signals they receive to around a millionth of a millionth of a second! When they do, they’re able to make phenomenally sharp images – if your digital camera was this good, you could take a photo of a person hundreds of kilometres away and make out individual strands of hair on their head. 

They used this capability to capture the shadow that a supermassive black hole casts – it’s the first time astronomers have ever really “seen” a black hole.  When you think about it, the photons that travelled almost 60 million years to hit the EHT telescopes in 2017 and make this image were extremely lucky – they were born right next door to a monstrous black hole and nearly, nearly fell in. The shadow we see in the image is the absence of photons right next to them that weren’t so lucky, they fell over the black hole’s event horizon and no-one will ever see them again.

Last updated: 11 Apr 2019 2:04pm
Declared conflicts of interest:
"I have previously been a co-author on a couple of papers with some of the authors of these papers, on some semi-related work (millimetre images of the black hole in the middle of our galaxy). Also, I developed some of the instrumentation that was used in part of the data analysis in this work (the DiFX software correlator) so I got an acknowledgement at the end of their papers for that. I don't personally consider either of these to be a conflict, as I'm not involved with these sub-millimetre observations at all, but thought I should mention it."
Ilya Mandel is a Professor of Theoretical Astrophysics at Monash University

It was hugely exciting to see the fantastic results from the Event Horizon Telescope.

Using a network of radio telescope around the Earth and incredibly precise interferometry, the EHT team imaged the central black hole in the galaxy M87, more than 50 million light years away.  Their image matched the predictions of Einstein's general theory of relativity: in the image of radiation from a disk of matter spiralling into the black hole, this supermassive black hole itself casts a gargantuan shadow.  

The size of the shadow has been used to get the most precise measurement of the black hole's mass: a whopping 6 billion times the mass of the Sun. It's a monster, but a very law-abiding one, precisely following the rules laid out by general relativity.

Last updated: 11 Apr 2019 2:02pm
Declared conflicts of interest:
None declared.
Professor Steven Tingay is the Executive Director of the Curtin Institute of Radio Astronomy (CIRA)

The Event Horizon Telescope (EHT) project has just released the first direct image of material disappearing across the event horizon of a supermassive black hole in a galaxy approximately 55 million light years away (one of our closest neighbour galaxies).

For decades, we have been studying black holes but could only indirectly see the effects of their extreme masses and gravitational fields. In the last few years, we have famously seen black holes merging, via the LIGO and VIRGO gravitational wave observatories, confirming the predictions of Einstein from one hundred years ago from his theory of General Relativity.

The EHT images show, for the first time, the point close to the black hole from which nothing can escape, even light, the so-called event horizon. The simple but astonishing images show a ring of radio emission that hugs the black hole event horizon, again confirming the predictions of General Relativity.

The EHT is composed of a collection of radio telescopes operating at very high frequencies, scattered around the world, generally in remote and high elevation locations, posing very challenging problems in engineering and data processing to effectively build a telescope with a diameter equal to the Earth's diameter.  This is an astonishing result, obtained in record time, built on international collaboration and multi-disciplinary efforts. There is clearly lots of room for improvement and I expect we will see in the near future even better images from the EHT, uncovering more of the mystery of black holes.

Last updated: 11 Apr 2019 2:01pm
Declared conflicts of interest:
None declared.
Dr Daniel Reardon is a postdoctoral researcher for the ARC Centre of Excellence for Gravitational Wave Discovery (OzGrav) at Swinburne University of Technology

The Event Horizon Telescope (EHT) is a network of radio telescopes around the globe, whose data are synchronised precisely so as to function as one “virtual” telescope the size of our planet. The imaging resolution possible with the virtual telescope is absolutely mind-bending. Capturing an image of the black hole shadow is like standing in Sydney and imaging a flea in Perth. The image of the supermassive black hole in the centre of M87 is stunning and looks just like simulations predicted, meaning that Einstein’s theory passes yet another test. The dark shadow we see is actually almost three times larger than the black hole, because light rays along our line of sight get funnelled in by the extreme curvature of spacetime near this giant. We can beautifully see that the hot gas falling onto the black hole is brighter on one side of the shadow than the other – this is because it is travelling near lightspeed and confirms predictions of Einstein’s general relativity. This hefty black hole weighs in at 6.5 billion times the mass of our Sun, and is the size of our Solar system.

Last updated: 11 Apr 2019 1:59pm
Declared conflicts of interest:
None declared.
Richard de Grijs is Professor of Astrophysics at Macquarie University and Associate Dean responsible for the global engagement of its Faculty of Science and Engineering.

The technical challenges were formidable, but that didn’t stop an international team of more than 200 scientists to link together essentially all existing submillimetre telescopes – as far south as the South Pole – to create a virtual telescope the size of the Earth.

Basic physics tells us that the larger a telescope is, the smaller the details are that one can observe. With a truly Earth-sized telescope, the Event Horizon Telescope (EHT) team took the ultimate picture and, in the process, proved Einstein right once again.

Training their facilities on the centre of the massive elliptical galaxy Messier 87, in one of the most densely populated regions of the Virgo Cluster of galaxies some 55 million light-years from Earth, the EHT recorded the first-ever image of the ‘event horizon’, the point of no return on an imaginary journey towards the galaxy’s central black hole.

Nothing, not even light, can escape from inside the event horizon. Yet, when matter falls into the event horizon, it becomes superheated and outshines pretty much everything else nearby. The image shown today shows a slightly blurred ring, but one should keep in mind that given the small size of the event horizon at the distance of Messier 87, this is a truly remarkable measurement.

Today represents indeed an historic moment: it marks the confirmation that black holes exist and that support for Einstein’s theory of general relativity is as strong as ever. This could only have been achieved by collaborating internationally, by putting science on a pedestal irrespective of political, religious or other controversies. Once again, this team has proven that science diplomacy is a viable means of bringing people together to work on common goals while overcoming numerous challenges against almost insurmountable odds.

Last updated: 11 Apr 2019 1:57pm
Declared conflicts of interest:
None declared.
Associate Professor James Miller-Jones is from the Curtin University node of the International Centre for Radio Astronomy Research (ICRAR)

An international team of astronomers have, for the first time, peered into the heart of a black hole, imaging the dark region corresponding to its event horizon—the point from which light can no longer escape.

Creating a telescope by combining the data from multiple antennas spanning the entire globe, the Event Horizon Telescope collaboration made an image of the supermassive black hole at the centre of the nearby galaxy Messier 87.

With a mass 6.5 billion times that of the Sun, this black hole has an event horizon roughly the size of our entire solar system. Located at a distance of 55 million light years, the magnifying power of the telescope required to see the black hole's shadow was the equivalent of being in Perth and reading the writing on a coin located in Sydney.

The image confirms that black holes do have event horizons as opposed to dim but solid surfaces, and was in full agreement with predictions from Einstein's theory of general relativity, allowing this century-old theory to pass yet another rigorous test with flying colours.

The centre of the galaxy Messier 87 is known to launch extremely powerful jets that travel at close to the speed of light, carrying energy away to distances of thousands of light years.

Emanating from a region no larger than our solar system, these jets affect the entire galaxy, as well as its surrounding environment.

This new measurement is proof that a black hole is indeed responsible for launching such energetic jets, which in other, more distant galaxies, are known to shape some of the most massive structures in our Universe.

Last updated: 11 Apr 2019 1:54pm
Declared conflicts of interest:
None declared.
Professor Fred Watson AM, is the Astronomer-at-Large at the Department of Industry, Innovation and Science

Revealing the Eye of M87’s storm

Today, the Event Horizon Telescope has shown us the invisible. On a truly historic day in the annals of astronomy, the world’s media were treated to a remarkable image. It shows the shadow of the event horizon of a 6 billion solar mass black hole at the centre of the active galaxy M87, clearly defined by a telescope the size of the Earth.

While M87 is active in the sense that its black hole is consuming gas and stars around it, it is currently relatively quiescent, allowing the event horizon shadow to be well resolved. The observed ring of light – really high-frequency radio waves – is consistent with the prediction of a photon ring that has only just escaped the clutches of the black hole.

The successful observations were made using an array of eight radio telescopes equipped with special data recorders, atomic clocks and sensitive detectors. As well as the equipment working properly, the weather had to be good at all the sites for the experiment to work. In fact, out of a 10-day allocation of telescope time, only seven days of observation were required. The result was five petabytes of data – the equivalent of 5,000 years-worth of MP3 plays – which have now been reduced to an image of a few kilobytes. 

The feat involved a decade of work by a major international collaboration. Project Director Shep Doeleman paid tribute to the many scientists involved, with special praise for the early-career researcher who carried out much of the drudgery of routine data reduction. Asked whether there was a party once the final image had emerged, Doeleman admitted that the overwhelming emotion was surprise that the image was as expected. National Science Foundation Director, France A. Córdova, who had not seen the image prior to the media conference, confessed that it brought tears to her eyes. 

The collaboration has also observed the much nearer, but smaller, black hole at the centre of the Milky Way Galaxy known as Sagittarius A*, and data reduction work is continuing on that. There is also the promise of more telescopes being added to the collaboration, together with a move to higher frequencies to improve the resolution.

Watch this space!

Last updated: 11 Apr 2019 1:52pm
Declared conflicts of interest:
None declared.
Associate Professor Michael Brown is an astronomer at Monash University's School of Physics and Astronomy.

Astronomers have been accumulating evidence for black holes for almost half a century. The simplest explanation for quasars and certain X-ray binary stars is that they are powered by black holes. We can see stars zipping around an unseen mass at the centre of our own galaxy, and we similar evidence of stars and gas orbiting vast unseen masses in other galaxies too (including Messier 87). The creation of black holes produces gravitational waves, which were observed for the first time just a few years ago.

But we haven’t had an image of a black hole and its surrounds until now. 

This intriguing image of Messier 87’s black hole may not be as impressive as its CGI cousin from the movie "Interstellar.’’ However, it is consistent with what theoreticians have been expecting. We can see a ring of light around a circular shadow, the result of luminous plasma near the black hole moving at close to light speed and light being deflected by the black hole’s vast gravitational pull.

Last updated: 11 Apr 2019 1:50pm
Declared conflicts of interest:
None declared.
Professor Lisa Harvey-Smith is an astronomer at the University of New South Wales and Australia’s Women in STEM Ambassador.

As someone who has studied the environments of supermassive black holes, this long-awaited result from the Event Horizon Telescope is extremely exciting. Although we have been able to measure the properties of supermassive black holes before, this is the first time that we have seen a picture of the light from their very edges. 
By using a telescope the size of the Earth, the team has been able to make an exquisite picture, in unprecedented detail, of the light bent around the edge of the black hole in the middle of a nearby galaxy.

This research is particularly important because it has the potential to test Einstein’s theory of gravity to the limits.

Last updated: 11 Apr 2019 1:49pm
Declared conflicts of interest:
None declared.
Professor Richard Hunstead is a member and former head of the Sydney Institute for Astronomy (SIfA) and the Director of the Molonglo Observatory Synthesis Telescope (MOST) at the University of Sydney

What is the event horizon? This is the boundary around a black hole inside of which nothing can escape, not even light. This was predicted by Einstein but has never been observed. The nearest black hole, 4 million times the mass of the Sun, is at the centre of our Milky Way galaxy, and the orbits of stars close to the black hole have been mapped at infrared wavelengths for more than a decade.

At this time of year, the centre of the Milky Way is high in the sky in Australia in the early hours of the morning. This is the target of the Event Horizon Telescope (EHT) and its observations will be reported in simultaneous world-wide press conferences on 10 April. An image of the region of sky around the black hole, known as Sagittarius A*, has been made at a frequency of 86 GHz (or a wavelength of 3.5 mm) using the combined power of radio telescopes in Chile, Mexico, Arizona, Hawaii, Spain, and the South Pole. The image will have the resolving power of a telescope more than half the diameter of the Earth, but has it seen the shadow of the event horizon?

Last updated: 11 Apr 2019 1:48pm
Declared conflicts of interest:
None declared.
Swinburne University’s Professor Alan Duffy, Lead Scientist of The Royal Institution of Australia

The worldwide near-decade long experiment is nearly as epic as the prize itself - an impossible picture of a black hole.
Blackholes are black as no light can escape them to reach us so the picture is in fact of the glowing bright material swirling around it. 
While we know black holes exist thanks to hearing their collision through gravitational waves we still want this picture and that’s because seeing is believing.
The shape of the shadow of the black hole against the bright material around it can test Einstein’s Theory of General Relativity. 
Just imagine if the picture isn’t what we expect, a new era of astrophysics could be revealed! If the picture is as predicted then Einstein was vindicated in a way he couldn’t conceive of being possible a century ago.

Last updated: 11 Apr 2019 1:47pm
Declared conflicts of interest:
None declared.

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  • First image ever taken of a black hole
    First image ever taken of a black hole

    The first image ever taken of a supermassive black hole - M87, at the centre of the Virgo A galaxy.

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  • Black Hole M87

    The Australian Academy of Science on Black Hole M87

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    Last Modified: 26 Nov 2019 1:56pm

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