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| Meta Title | Hereâs the first picture of a black hole |
| Meta Description | The Event Horizon Telescope imaged the supermassive beast lying some 55 million light-years away in a galaxy called M87. |
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| Boilerpipe Text | This is what a black hole looks like.
A black hole isnât really a hole. Itâs an object in space with incredible mass packed into a very small area. All that mass creates such a huge gravitational tug that nothing can escape a black hole, including light.
Explainer: What are black holes?
The newly imaged supermassive monster lies in a galaxy called M87. A world-spanning network of observatories called theÂ
Event Horizon Telescope
, or EHT, zoomed in on M87 to create this first-ever picture of a black hole.
âWe have seen what we thought was unseeable,â Sheperd Doeleman said April 10 in Washington, D.C. âWe have seen and taken a picture of a black hole,â he reported at one of seven concurrent news conferences. Doeleman is EHTâs director. He also is an astrophysicist at the Harvard-Smithsonian Center for Astrophysics in Cambridge, Mass. Results from his teamâs work appear in six papers in the
 Astrophysical Journal Letters
.
The concept of a black hole was first hinted at back in the 1780s. The mathematics behind them came from Albert Einsteinâs 1915 general theory of relativity. And the phenomenon got its name âblack holeâ in the 1960s. But until now, all âpicturesâ of black holes have been illustrations or simulations.
âWeâve been studying black holes so long, sometimes itâs easy to forget that none of us have actually seen one.â
â France CĂłrdova, director of the National Science Foundation     Â
âWeâve been studying black holes so long, sometimes itâs easy to forget that none of us have actually seen one,â France CĂłrdova said in the Washington, D.C., news conference. She is director of the National Science Foundation. Seeing a black hole âis a Herculean task,â she said.
The galaxy M87 sits about 55 million light-years from Earth in the constellation Virgo. Unlike the Milky Wayâs stunning spirals, M87 is a blobby giant elliptical galaxy. The Event Horizon Telescope just took the first image of the black hole at the center of M87.
Thatâs because black holes are famously hard to see. Their gravity is so extreme that nothing, not even light, can escape across the boundary at a black holeâs edge. That edge is known as the event horizon. But some black holes, especially supermassive ones dwelling in galaxiesâ centers, stand out. They gather bright disks of gas and other material that surrounds the black hole. The EHT image reveals the shadow of M87âs black hole on its accretion disk. That disk looks like a fuzzy, asymmetrical ring. It unveils for the first time the dark abyss of one of the universeâs most mysterious objects.
âItâs been such a buildup,â Doeleman said. âIt was just astonishment and wonder⊠to know that youâve uncovered a part of the universe that was off limits to us.â
The much-anticipated big reveal of the image âlives up to the hype, thatâs for sure,â says Priyamvada Natarajan. This astrophysicist at Yale University, in New Haven, Conn., is not on the EHT team. âIt really brings home how fortunate we are as a species at this particular time, with the capacity of the human mind to comprehend the universe, to have built all the science and technology to make it happen.â
Einstein was right
The new image aligns with what physicists expected a black hole to look like based on the theory of general
relativity
by Albert Einstein. That theory predicts how
spacetime
is warped by the extreme mass of a black hole. The picture is âone more strong piece of evidence supporting the existence of black holes. And that, of course, helps verify general relativity,â says Clifford Will. Heâs a physicist at the University of Florida in Gainesville, who is not on the EHT team. âBeing able to actually see this shadow and to detect it is a tremendous first step.â
Studies in the past have tested general relativity by looking at the motions of stars or gas clouds near a black hole, but never at its edge. âItâs as good as it gets,â Will says. Tiptoe any closer and youâd be inside the black hole. And then youâd be unable to report back on the results of any experiments.
âBlack hole environments are a likely place where general relativity would break down,â says EHT team member Feryal Ăzel. She is an astrophysicist who works at the University of Arizona in Tucson. So testing general relativity in such extreme conditions could reveal things that donât seem to support Einsteinâs predictions.
Explainer: Quantum is the world of the super small
However, she adds, just because this first image upholds general relativity âdoesnât mean general relativity is completely fine.â Many physicists think that general relativity wonât be the last word on gravity. Thatâs because itâs incompatible with another essential physics theory,
quantum mechanics
. This theory describes physics on very small scales.
The new image provided a new measurement of the size and heft of M87âs black hole. âOur mass determination by just directly looking at the shadow has helped resolve a longstanding controversy,â Sera Markoff said in the Washington, D.C., news conference. Sheâs a theoretical astrophysicist at the University of Amsterdam in the Netherlands. Estimates made using different techniques have ranged between 3.5 billion and 7.22 billion times the mass of the sun. New EHT measurements show that the mass of this black hole is about 6.5 billion solar masses. Â
The team also has figured out the behemothâs size. Its diameter stretches 38 billion kilometers (24 billion miles). And the black hole spins clockwise. âM87 is a monster even by supermassive black hole standards,â Markoff said. Â
Scientists have been speculating for years about what a black hole would actually look like. Now, they finally know the answer.
Science News/YouTube
Looking ahead
EHT trained its sights on both M87âs black hole and Sagittarius A*. That second supermassive black hole sits at the center of our galaxy, the Milky Way. But, the scientists found it easier to image M87âs monster, even though itâs about 2,000 times as far away as Sgr A*.
M87âs black hole sits about 55 million light-years from Earth in the constellation Virgo. But itâs also about 1,000 times as massive as the Milky Wayâs giant. Sgr A* only weighs the equivalent of roughly 4 million suns. M87âs extra heft nearly compensates for its greater distance. The size it covers in our sky âis pretty darn similar,â says EHT team member Ăzel. Â
Because M87âs black hole is bigger and has more gravity, gases swirling around it move and vary in brightness more slowly than they do around Sgr A*. And hereâs why thatâs important. âDuring a single observation, Sgr A* doesnât sit still, whereas M87 does,â says Ăzel. âJust based on this âDoes the black hole sit still and pose for me?â point of view, we knew M87 would cooperate more.â
With more data analysis, the team hopes to solve some long-standing mysteries about black holes. These include how M87âs black hole spews such a bright jet of charged particles many thousands of light-years into space. Â
Some black holes launch jets of charged particles thousands of light-years into space, such as the one shown in this image from a simulation. Data collected to create the first image of a black hole, the one in galaxy M87, may help reveal how these jets are produced.
This first image is like the âshot heard round the worldâ that kicked off the American Revolutionary War, says Avi Loeb. He is an astrophysicist at Harvard University in Cambridge, Mass. âItâs very significant. It gives a glimpse of what the future might hold. But it doesnât give us all the information that we want.â
The team does not yet have a picture of Sgr A*. But the researchers were able to collect some data on it. They are continuing to analyze those data in the hopes of adding to a new gallery of black hole portraits. Since the appearance of that black hole changes so quickly, the team is having to develop new techniques to analyze the data from it.
âThe Milky Way is a very different galaxy from M87,â Loeb notes. Studying such different environments could reveal more details of how black holes behave, he says.
The next look at the M87 and Milky Way behemoths will have to wait, though. Scientists got a lucky stretch of good weather at all eight sites that made up the Event Horizon Telescope in 2017. Then there was bad weather in 2018. (Water vapor in the atmosphere can interfere with the telescopeâs measurements.) Technical difficulties cancelled this yearâs observing run.
The good news is that by 2020, EHT will include 11 observatories. The Greenland Telescope joined the consortium in 2018. The Kitt Peak National Observatory outside Tucson, Ariz., and the NOrthern Extended Millimeter Array (NOEMA) in the French Alps will join EHT in 2020.
Adding more telescopes should allow the team to extend the image. That would let EHT better capture the jets that spew from the black hole. The researchers also plan to make observations using light having a slightly higher frequency. That can further sharpen the image. And even bigger plans are on the horizon â adding telescopes that orbit Earth. âWorld domination is not enough for us. We also want to go to space,â Doeleman quipped.Â
These extra eyes may be just whatâs needed to bring black holes into even greater focus.
Staff writer Maria Temming contributed to this story.
Power Words
More About Power Words
align
     (noun: alignment) To place or organize things in a patterned order, following an apparent line.
astrophysics
     An area of astronomy that deals with understanding the physical nature of stars and other objects in space. People who work in this field are known as
astrophysicists
.
behemoth
     A term for anything that is amazingly big. The term comes from a monstrous animal described in the Bibleâs book of Job.
black hole
     A region of space having a gravitational field so intense that no matter or radiation (including light) can escape.
consortium
     A group or association of independent organizations.
constellation
     Patterns formed by prominent stars that lie close to each other in the night sky. Modern astronomers divide the sky into 88 constellations, 12 of which (known as the zodiac) lie along the sunâs path through the sky over the course of a year. Cancri, the original Greek name for the constellation Cancer, is one of those 12 zodiac constellations.
diameter
     The length of a straight line that runs through the center of a circle or spherical object, starting at the edge on one side and ending at the edge on the far side.
event horizon
     An imaginary sphere that surrounds a black hole. The more massive the black hole, the bigger the sphere. Anything that happens inside the event horizon is invisible, because gravity is so strong that under normal circumstances even light canât escape. But according to some theories of physics, in certain situations small amounts of radiation can escape.
galaxy
     A massive group of stars bound together by gravity. Galaxies, which each typically include between 10 million and 100 trillion stars, also include clouds of gas, dust and the remnants of exploded stars.
gravity
     The force that attracts anything with mass, or bulk, toward any other thing with mass. The more mass that something has, the greater its gravity.
light-year
     The distance light travels in one year, about 9.48 trillion kilometers (almost 6 trillion miles). To get some idea of this length, imagine a rope long enough to wrap around the Earth. It would be a little over 40,000 kilometers (24,900 miles) long. Lay it out straight. Now lay another 236 million more that are the same length, end-to-end, right after the first. The total distance they now span would equal one light-year.
mass
     A number that shows how much an object resists speeding up and slowing down â basically a measure of how much matter that object is made from.
mechanics
     The study of how things move.
Milky Way
     The galaxy in which Earthâs solar system resides.
National Science Foundation
     The U.S. Congress created this independent federal agency in 1950 to promote the advancement of science; national health, prosperity and welfare; and the nationâs defense. This agency funds nearly one-fourth of all federally supported basic research in U.S. colleges and universities. In many fields such as mathematics, computer science and the social sciences, NSF is the major source of federal funding.
network
     A group of interconnected people or things. (v.) The act of connecting with other people who work in a given area or do similar thing (such as artists, business leaders or medical-support groups), often by going to gatherings where such people would be expected, and then chatting them up. (n. networking)
observatory
     (in astronomy) The building or structure (such as a satellite) that houses one or more telescopes.
particle
     A minute amount of something.
physics
     The scientific study of the nature and properties of matter and energy. Classical physics is an explanation of the nature and properties of matter and energy that relies on descriptions such as Newtonâs laws of motion. Quantum physics, a field of study that emerged later, is a more accurate way of explaining the motions and behavior of matter. A scientist who works in such areas is known as a
physicist
.
quantum
     (pl. quanta) A term that refers to the smallest amount of anything, especially of energy or subatomic mass.
quantum mechanics
     A branch of physics dealing with the behavior of matter on the scale of atoms or subatomic particles.
relativity
     (in physics) A theory developed by physicist Albert Einstein showing that neither space nor time are constant, but instead affected by oneâs velocity and the mass of things in your vicinity.
spacetime
     A term made essential by Einsteinâs theory of relativity, it describes a designation for some spot given in terms of its three-dimensional coordinates in space, along with a fourth coordinate corresponding to time.
standards
     (in research) The values or materials used as benchmarks against which other things can be compared.
star
     The basic building block from which galaxies are made. Stars develop when gravity compacts clouds of gas. When they become dense enough to sustain nuclear-fusion reactions, stars will emit light and sometimes other forms of electromagnetic radiation. The sun is our closest star.
sun
     The star at the center of Earthâs solar system. Itâs an average size star about 26,000 light-years from the center of the Milky Way galaxy. Also a term for any sunlike star.
telescope
     Usually a light-collecting instrument that makes distant objects appear nearer through the use of lenses or a combination of curved mirrors and lenses. Some, however, collect radio emissions (energy from a different portion of the electromagnetic spectrum) through a network of antennas.
theoretical
     An adjective for an analysis or assessment of something that based on pre-existing knowledge of how things behave. It is not based on experimental trials. Theoretical research tends to use math â usually performed by computers â to predict how or what will occur for some specified series of conditions. Experimental testing or observations of natural systems will then be needed to confirm what had been predicted.
theory
     (in science) A description of some aspect of the natural world based on extensive observations, tests and reason. A theory can also be a way of organizing a broad body of knowledge that applies in a broad range of circumstances to explain what will happen. Unlike the common definition of theory, a theory in science is not just a hunch. Ideas or conclusions that are based on a theory â and not yet on firm data or observations â are referred to as theoretical. Scientists who use mathematics and/or existing data to project what might happen in new situations are known as theorists.
universe
     The entire cosmos: All things that exist throughout space and time. It has been expanding since its formation during an event known as the Big Bang, some 13.8 billion years ago (give or take a few hundred million years).
verify
     (n. verification) To demonstrate or confirm in some way that a particular claim or suspicion is true.
weather
     Conditions in the atmosphere at a localized place and a particular time. It is usually described in terms of particular features, such as air pressure, humidity, moisture, any precipitation (rain, snow or ice), temperature and wind speed. Weather constitutes the actual conditions that occur at any time and place. Itâs different from climate, which is a description of the conditions that tend to occur in some general region during a particular month or season.
Lisa Grossman is the astronomy writer at
Science News
. She has a degree in astronomy from Cornell University and a graduate certificate in science writing from University of California, Santa Cruz. She lives near Boston.
Science News
physics writer Emily Conover studied physics at the University of Chicago. She loves physics for its ability to reveal the secret rules about how stuff works, from tiny atoms to the vast cosmos. |
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# Hereâs the first picture of a black hole
The supermassive beast lies some 55 million light-years away in a galaxy called M87

The first image of a black hole shows a bright ring with a dark, central spot. That ring is a bright disk of gas orbiting the supermassive behemoth in the galaxy M87. The spot is the black holeâs shadow.
Event Horizon Telescope Collaboration
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April 10, 2019 at 3:15 pm
This is what a black hole looks like.
A black hole isnât really a hole. Itâs an object in space with incredible mass packed into a very small area. All that mass creates such a huge gravitational tug that nothing can escape a black hole, including light.
#### [Explainer: What are black holes?](https://www.sciencenewsforstudents.org/article/explainer-what-are-black-holes)
The newly imaged supermassive monster lies in a galaxy called M87. A world-spanning network of observatories called the [Event Horizon Telescope](https://eventhorizontelescope.org/), or EHT, zoomed in on M87 to create this first-ever picture of a black hole.
âWe have seen what we thought was unseeable,â Sheperd Doeleman said April 10 in Washington, D.C. âWe have seen and taken a picture of a black hole,â he reported at one of seven concurrent news conferences. Doeleman is EHTâs director. He also is an astrophysicist at the Harvard-Smithsonian Center for Astrophysics in Cambridge, Mass. Results from his teamâs work appear in six papers in the *Astrophysical Journal Letters*.
The concept of a black hole was first hinted at back in the 1780s. The mathematics behind them came from Albert Einsteinâs 1915 general theory of relativity. And the phenomenon got its name âblack holeâ in the 1960s. But until now, all âpicturesâ of black holes have been illustrations or simulations.
#### âWeâve been studying black holes so long, sometimes itâs easy to forget that none of us have actually seen one.â
###### â France CĂłrdova, director of the National Science Foundation
âWeâve been studying black holes so long, sometimes itâs easy to forget that none of us have actually seen one,â France CĂłrdova said in the Washington, D.C., news conference. She is director of the National Science Foundation. Seeing a black hole âis a Herculean task,â she said.

The galaxy M87 sits about 55 million light-years from Earth in the constellation Virgo. Unlike the Milky Wayâs stunning spirals, M87 is a blobby giant elliptical galaxy. The Event Horizon Telescope just took the first image of the black hole at the center of M87.
Thatâs because black holes are famously hard to see. Their gravity is so extreme that nothing, not even light, can escape across the boundary at a black holeâs edge. That edge is known as the event horizon. But some black holes, especially supermassive ones dwelling in galaxiesâ centers, stand out. They gather bright disks of gas and other material that surrounds the black hole. The EHT image reveals the shadow of M87âs black hole on its accretion disk. That disk looks like a fuzzy, asymmetrical ring. It unveils for the first time the dark abyss of one of the universeâs most mysterious objects.
âItâs been such a buildup,â Doeleman said. âIt was just astonishment and wonder⊠to know that youâve uncovered a part of the universe that was off limits to us.â
The much-anticipated big reveal of the image âlives up to the hype, thatâs for sure,â says Priyamvada Natarajan. This astrophysicist at Yale University, in New Haven, Conn., is not on the EHT team. âIt really brings home how fortunate we are as a species at this particular time, with the capacity of the human mind to comprehend the universe, to have built all the science and technology to make it happen.â
#### **Einstein was right**
The new image aligns with what physicists expected a black hole to look like based on the theory of general [*relativity*](https://www.sciencenewsforstudents.org/article/einstein-taught-us-its-all-relative) by Albert Einstein. That theory predicts how *spacetime* is warped by the extreme mass of a black hole. The picture is âone more strong piece of evidence supporting the existence of black holes. And that, of course, helps verify general relativity,â says Clifford Will. Heâs a physicist at the University of Florida in Gainesville, who is not on the EHT team. âBeing able to actually see this shadow and to detect it is a tremendous first step.â
Studies in the past have tested general relativity by looking at the motions of stars or gas clouds near a black hole, but never at its edge. âItâs as good as it gets,â Will says. Tiptoe any closer and youâd be inside the black hole. And then youâd be unable to report back on the results of any experiments.
âBlack hole environments are a likely place where general relativity would break down,â says EHT team member Feryal Ăzel. She is an astrophysicist who works at the University of Arizona in Tucson. So testing general relativity in such extreme conditions could reveal things that donât seem to support Einsteinâs predictions.
#### [Explainer: Quantum is the world of the super small](https://www.sciencenewsforstudents.org/article/explainer-quantum-world-super-small)
However, she adds, just because this first image upholds general relativity âdoesnât mean general relativity is completely fine.â Many physicists think that general relativity wonât be the last word on gravity. Thatâs because itâs incompatible with another essential physics theory, *quantum mechanics*. This theory describes physics on very small scales.
The new image provided a new measurement of the size and heft of M87âs black hole. âOur mass determination by just directly looking at the shadow has helped resolve a longstanding controversy,â Sera Markoff said in the Washington, D.C., news conference. Sheâs a theoretical astrophysicist at the University of Amsterdam in the Netherlands. Estimates made using different techniques have ranged between 3.5 billion and 7.22 billion times the mass of the sun. New EHT measurements show that the mass of this black hole is about 6.5 billion solar masses.
The team also has figured out the behemothâs size. Its diameter stretches 38 billion kilometers (24 billion miles). And the black hole spins clockwise. âM87 is a monster even by supermassive black hole standards,â Markoff said.
Scientists have been speculating for years about what a black hole would actually look like. Now, they finally know the answer.
Science News/YouTube
#### **Looking ahead**
EHT trained its sights on both M87âs black hole and Sagittarius A\*. That second supermassive black hole sits at the center of our galaxy, the Milky Way. But, the scientists found it easier to image M87âs monster, even though itâs about 2,000 times as far away as Sgr A\*.
M87âs black hole sits about 55 million light-years from Earth in the constellation Virgo. But itâs also about 1,000 times as massive as the Milky Wayâs giant. Sgr A\* only weighs the equivalent of roughly 4 million suns. M87âs extra heft nearly compensates for its greater distance. The size it covers in our sky âis pretty darn similar,â says EHT team member Ăzel.
Because M87âs black hole is bigger and has more gravity, gases swirling around it move and vary in brightness more slowly than they do around Sgr A\*. And hereâs why thatâs important. âDuring a single observation, Sgr A\* doesnât sit still, whereas M87 does,â says Ăzel. âJust based on this âDoes the black hole sit still and pose for me?â point of view, we knew M87 would cooperate more.â
With more data analysis, the team hopes to solve some long-standing mysteries about black holes. These include how M87âs black hole spews such a bright jet of charged particles many thousands of light-years into space.

Some black holes launch jets of charged particles thousands of light-years into space, such as the one shown in this image from a simulation. Data collected to create the first image of a black hole, the one in galaxy M87, may help reveal how these jets are produced.
This first image is like the âshot heard round the worldâ that kicked off the American Revolutionary War, says Avi Loeb. He is an astrophysicist at Harvard University in Cambridge, Mass. âItâs very significant. It gives a glimpse of what the future might hold. But it doesnât give us all the information that we want.â
The team does not yet have a picture of Sgr A\*. But the researchers were able to collect some data on it. They are continuing to analyze those data in the hopes of adding to a new gallery of black hole portraits. Since the appearance of that black hole changes so quickly, the team is having to develop new techniques to analyze the data from it.
âThe Milky Way is a very different galaxy from M87,â Loeb notes. Studying such different environments could reveal more details of how black holes behave, he says.
The next look at the M87 and Milky Way behemoths will have to wait, though. Scientists got a lucky stretch of good weather at all eight sites that made up the Event Horizon Telescope in 2017. Then there was bad weather in 2018. (Water vapor in the atmosphere can interfere with the telescopeâs measurements.) Technical difficulties cancelled this yearâs observing run.
The good news is that by 2020, EHT will include 11 observatories. The Greenland Telescope joined the consortium in 2018. The Kitt Peak National Observatory outside Tucson, Ariz., and the NOrthern Extended Millimeter Array (NOEMA) in the French Alps will join EHT in 2020.
Adding more telescopes should allow the team to extend the image. That would let EHT better capture the jets that spew from the black hole. The researchers also plan to make observations using light having a slightly higher frequency. That can further sharpen the image. And even bigger plans are on the horizon â adding telescopes that orbit Earth. âWorld domination is not enough for us. We also want to go to space,â Doeleman quipped.
These extra eyes may be just whatâs needed to bring black holes into even greater focus.
*Staff writer Maria Temming contributed to this story.*
### Power Words
[More About Power Words](https://www.snexplores.org/power-words-aid-stem-literacy/)
**align** (noun: alignment) To place or organize things in a patterned order, following an apparent line.
**astrophysics** An area of astronomy that deals with understanding the physical nature of stars and other objects in space. People who work in this field are known as **astrophysicists**.
**behemoth** A term for anything that is amazingly big. The term comes from a monstrous animal described in the Bibleâs book of Job.
**black hole** A region of space having a gravitational field so intense that no matter or radiation (including light) can escape.
**consortium** A group or association of independent organizations.
**constellation** Patterns formed by prominent stars that lie close to each other in the night sky. Modern astronomers divide the sky into 88 constellations, 12 of which (known as the zodiac) lie along the sunâs path through the sky over the course of a year. Cancri, the original Greek name for the constellation Cancer, is one of those 12 zodiac constellations.
**diameter** The length of a straight line that runs through the center of a circle or spherical object, starting at the edge on one side and ending at the edge on the far side.
**event horizon** An imaginary sphere that surrounds a black hole. The more massive the black hole, the bigger the sphere. Anything that happens inside the event horizon is invisible, because gravity is so strong that under normal circumstances even light canât escape. But according to some theories of physics, in certain situations small amounts of radiation can escape.
**galaxy** A massive group of stars bound together by gravity. Galaxies, which each typically include between 10 million and 100 trillion stars, also include clouds of gas, dust and the remnants of exploded stars.
**gravity** The force that attracts anything with mass, or bulk, toward any other thing with mass. The more mass that something has, the greater its gravity.
**light-year** The distance light travels in one year, about 9.48 trillion kilometers (almost 6 trillion miles). To get some idea of this length, imagine a rope long enough to wrap around the Earth. It would be a little over 40,000 kilometers (24,900 miles) long. Lay it out straight. Now lay another 236 million more that are the same length, end-to-end, right after the first. The total distance they now span would equal one light-year.
**mass** A number that shows how much an object resists speeding up and slowing down â basically a measure of how much matter that object is made from.
**mechanics** The study of how things move.
**Milky Way** The galaxy in which Earthâs solar system resides.
**National Science Foundation** The U.S. Congress created this independent federal agency in 1950 to promote the advancement of science; national health, prosperity and welfare; and the nationâs defense. This agency funds nearly one-fourth of all federally supported basic research in U.S. colleges and universities. In many fields such as mathematics, computer science and the social sciences, NSF is the major source of federal funding.
**network** A group of interconnected people or things. (v.) The act of connecting with other people who work in a given area or do similar thing (such as artists, business leaders or medical-support groups), often by going to gatherings where such people would be expected, and then chatting them up. (n. networking)
**observatory** (in astronomy) The building or structure (such as a satellite) that houses one or more telescopes.
**particle** A minute amount of something.
**physics** The scientific study of the nature and properties of matter and energy. Classical physics is an explanation of the nature and properties of matter and energy that relies on descriptions such as Newtonâs laws of motion. Quantum physics, a field of study that emerged later, is a more accurate way of explaining the motions and behavior of matter. A scientist who works in such areas is known as a **physicist**.
**quantum** (pl. quanta) A term that refers to the smallest amount of anything, especially of energy or subatomic mass.
**quantum mechanics** A branch of physics dealing with the behavior of matter on the scale of atoms or subatomic particles.
**relativity** (in physics) A theory developed by physicist Albert Einstein showing that neither space nor time are constant, but instead affected by oneâs velocity and the mass of things in your vicinity.
**spacetime** A term made essential by Einsteinâs theory of relativity, it describes a designation for some spot given in terms of its three-dimensional coordinates in space, along with a fourth coordinate corresponding to time.
**standards** (in research) The values or materials used as benchmarks against which other things can be compared.
**star** The basic building block from which galaxies are made. Stars develop when gravity compacts clouds of gas. When they become dense enough to sustain nuclear-fusion reactions, stars will emit light and sometimes other forms of electromagnetic radiation. The sun is our closest star.
**sun** The star at the center of Earthâs solar system. Itâs an average size star about 26,000 light-years from the center of the Milky Way galaxy. Also a term for any sunlike star.
**telescope** Usually a light-collecting instrument that makes distant objects appear nearer through the use of lenses or a combination of curved mirrors and lenses. Some, however, collect radio emissions (energy from a different portion of the electromagnetic spectrum) through a network of antennas.
**theoretical** An adjective for an analysis or assessment of something that based on pre-existing knowledge of how things behave. It is not based on experimental trials. Theoretical research tends to use math â usually performed by computers â to predict how or what will occur for some specified series of conditions. Experimental testing or observations of natural systems will then be needed to confirm what had been predicted.
**theory** (in science) A description of some aspect of the natural world based on extensive observations, tests and reason. A theory can also be a way of organizing a broad body of knowledge that applies in a broad range of circumstances to explain what will happen. Unlike the common definition of theory, a theory in science is not just a hunch. Ideas or conclusions that are based on a theory â and not yet on firm data or observations â are referred to as theoretical. Scientists who use mathematics and/or existing data to project what might happen in new situations are known as theorists.
**universe** The entire cosmos: All things that exist throughout space and time. It has been expanding since its formation during an event known as the Big Bang, some 13.8 billion years ago (give or take a few hundred million years).
**verify** (n. verification) To demonstrate or confirm in some way that a particular claim or suspicion is true.
**weather** Conditions in the atmosphere at a localized place and a particular time. It is usually described in terms of particular features, such as air pressure, humidity, moisture, any precipitation (rain, snow or ice), temperature and wind speed. Weather constitutes the actual conditions that occur at any time and place. Itâs different from climate, which is a description of the conditions that tend to occur in some general region during a particular month or season.
### Citations
**Journal:** The Event Horizon Telescope Collaboration et al. [First M87 Event Horizon Telescope Results. I. The Shadow of the Supermassive Black Hole](https://iopscience.iop.org/article/10.3847/2041-8213/ab0ec7). *The Astrophysical Journal Letters*. Published online April 10, 2019. doi:10.3847/2041-8213/ab0cc7.
**Journal:** The Event Horizon Telescope Collaboration et al. [First M87 Event Horizon Telescope Results. II. Array and Instrumentation](https://iopscience.iop.org/article/10.3847/2041-8213/ab0c96). *The Astrophysical Journal Letters*. Published online April 10, 2019. doi:10.3847/2041-8213/ab0c96.
**Journal:** The Event Horizon Telescope Collaboration et al. [First M87 Event Horizon Telescope Results. III. Data Processing and Calibration](https://iopscience.iop.org/article/10.3847/2041-8213/ab0c57). *The Astrophysical Journal Letters*. Published online April 10, 2019. doi:10.3847/2041-8213/ab0c57.
**Journal:** The Event Horizon Telescope Collaboration et al. [First M87 Event Horizon Telescope Results. IV. Imaging the Central Supermassive Black Hole](https://iopscience.iop.org/article/10.3847/2041-8213/ab0e85). *The Astrophysical Journal Letters*. Published online April 10, 2019. doi:10.3847/2041-8213/ab0e85.
**Journal:** The Event Horizon Telescope Collaboration et al*.* [First M87 Event Horizon Telescope Results. V. Physical Origin of the Asymmetric Ring](https://iopscience.iop.org/article/10.3847/2041-8213/ab0f43). *The Astrophysical Journal Letters*. Published online April 10, 2019. doi:10.3847/2041-8213/ab0f43.
**Journal:** The Event Horizon Telescope Collaboration et al*.* [First M87 Event Horizon Telescope Results. VI. The Shadow and Mass of the Central Black Hole](https://iopscience.iop.org/article/10.3847/2041-8213/ab1141). *The Astrophysical Journal Letters*. Published online April 10, 2019. doi:10.3847/2041-8213/ab1141.
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*Science News* physics writer Emily Conover studied physics at the University of Chicago. She loves physics for its ability to reveal the secret rules about how stuff works, from tiny atoms to the vast cosmos.
### Classroom Resources for This Article
- [Power Words](https://www.snexplores.org/article/black-hole-first-photo-event-horizon-telescope#power-words)
Readability Score: 7.8
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| Readable Markdown | This is what a black hole looks like.
A black hole isnât really a hole. Itâs an object in space with incredible mass packed into a very small area. All that mass creates such a huge gravitational tug that nothing can escape a black hole, including light.
[Explainer: What are black holes?](https://www.sciencenewsforstudents.org/article/explainer-what-are-black-holes)
The newly imaged supermassive monster lies in a galaxy called M87. A world-spanning network of observatories called the [Event Horizon Telescope](https://eventhorizontelescope.org/), or EHT, zoomed in on M87 to create this first-ever picture of a black hole.
âWe have seen what we thought was unseeable,â Sheperd Doeleman said April 10 in Washington, D.C. âWe have seen and taken a picture of a black hole,â he reported at one of seven concurrent news conferences. Doeleman is EHTâs director. He also is an astrophysicist at the Harvard-Smithsonian Center for Astrophysics in Cambridge, Mass. Results from his teamâs work appear in six papers in the *Astrophysical Journal Letters*.
The concept of a black hole was first hinted at back in the 1780s. The mathematics behind them came from Albert Einsteinâs 1915 general theory of relativity. And the phenomenon got its name âblack holeâ in the 1960s. But until now, all âpicturesâ of black holes have been illustrations or simulations.
#### âWeâve been studying black holes so long, sometimes itâs easy to forget that none of us have actually seen one.â
â France CĂłrdova, director of the National Science Foundation
âWeâve been studying black holes so long, sometimes itâs easy to forget that none of us have actually seen one,â France CĂłrdova said in the Washington, D.C., news conference. She is director of the National Science Foundation. Seeing a black hole âis a Herculean task,â she said.

The galaxy M87 sits about 55 million light-years from Earth in the constellation Virgo. Unlike the Milky Wayâs stunning spirals, M87 is a blobby giant elliptical galaxy. The Event Horizon Telescope just took the first image of the black hole at the center of M87.
Thatâs because black holes are famously hard to see. Their gravity is so extreme that nothing, not even light, can escape across the boundary at a black holeâs edge. That edge is known as the event horizon. But some black holes, especially supermassive ones dwelling in galaxiesâ centers, stand out. They gather bright disks of gas and other material that surrounds the black hole. The EHT image reveals the shadow of M87âs black hole on its accretion disk. That disk looks like a fuzzy, asymmetrical ring. It unveils for the first time the dark abyss of one of the universeâs most mysterious objects.
âItâs been such a buildup,â Doeleman said. âIt was just astonishment and wonder⊠to know that youâve uncovered a part of the universe that was off limits to us.â
The much-anticipated big reveal of the image âlives up to the hype, thatâs for sure,â says Priyamvada Natarajan. This astrophysicist at Yale University, in New Haven, Conn., is not on the EHT team. âIt really brings home how fortunate we are as a species at this particular time, with the capacity of the human mind to comprehend the universe, to have built all the science and technology to make it happen.â
#### **Einstein was right**
The new image aligns with what physicists expected a black hole to look like based on the theory of general [*relativity*](https://www.sciencenewsforstudents.org/article/einstein-taught-us-its-all-relative) by Albert Einstein. That theory predicts how *spacetime* is warped by the extreme mass of a black hole. The picture is âone more strong piece of evidence supporting the existence of black holes. And that, of course, helps verify general relativity,â says Clifford Will. Heâs a physicist at the University of Florida in Gainesville, who is not on the EHT team. âBeing able to actually see this shadow and to detect it is a tremendous first step.â
Studies in the past have tested general relativity by looking at the motions of stars or gas clouds near a black hole, but never at its edge. âItâs as good as it gets,â Will says. Tiptoe any closer and youâd be inside the black hole. And then youâd be unable to report back on the results of any experiments.
âBlack hole environments are a likely place where general relativity would break down,â says EHT team member Feryal Ăzel. She is an astrophysicist who works at the University of Arizona in Tucson. So testing general relativity in such extreme conditions could reveal things that donât seem to support Einsteinâs predictions.
[Explainer: Quantum is the world of the super small](https://www.sciencenewsforstudents.org/article/explainer-quantum-world-super-small)
However, she adds, just because this first image upholds general relativity âdoesnât mean general relativity is completely fine.â Many physicists think that general relativity wonât be the last word on gravity. Thatâs because itâs incompatible with another essential physics theory, *quantum mechanics*. This theory describes physics on very small scales.
The new image provided a new measurement of the size and heft of M87âs black hole. âOur mass determination by just directly looking at the shadow has helped resolve a longstanding controversy,â Sera Markoff said in the Washington, D.C., news conference. Sheâs a theoretical astrophysicist at the University of Amsterdam in the Netherlands. Estimates made using different techniques have ranged between 3.5 billion and 7.22 billion times the mass of the sun. New EHT measurements show that the mass of this black hole is about 6.5 billion solar masses.
The team also has figured out the behemothâs size. Its diameter stretches 38 billion kilometers (24 billion miles). And the black hole spins clockwise. âM87 is a monster even by supermassive black hole standards,â Markoff said.
Scientists have been speculating for years about what a black hole would actually look like. Now, they finally know the answer.
Science News/YouTube
#### **Looking ahead**
EHT trained its sights on both M87âs black hole and Sagittarius A\*. That second supermassive black hole sits at the center of our galaxy, the Milky Way. But, the scientists found it easier to image M87âs monster, even though itâs about 2,000 times as far away as Sgr A\*.
M87âs black hole sits about 55 million light-years from Earth in the constellation Virgo. But itâs also about 1,000 times as massive as the Milky Wayâs giant. Sgr A\* only weighs the equivalent of roughly 4 million suns. M87âs extra heft nearly compensates for its greater distance. The size it covers in our sky âis pretty darn similar,â says EHT team member Ăzel.
Because M87âs black hole is bigger and has more gravity, gases swirling around it move and vary in brightness more slowly than they do around Sgr A\*. And hereâs why thatâs important. âDuring a single observation, Sgr A\* doesnât sit still, whereas M87 does,â says Ăzel. âJust based on this âDoes the black hole sit still and pose for me?â point of view, we knew M87 would cooperate more.â
With more data analysis, the team hopes to solve some long-standing mysteries about black holes. These include how M87âs black hole spews such a bright jet of charged particles many thousands of light-years into space.

Some black holes launch jets of charged particles thousands of light-years into space, such as the one shown in this image from a simulation. Data collected to create the first image of a black hole, the one in galaxy M87, may help reveal how these jets are produced.
This first image is like the âshot heard round the worldâ that kicked off the American Revolutionary War, says Avi Loeb. He is an astrophysicist at Harvard University in Cambridge, Mass. âItâs very significant. It gives a glimpse of what the future might hold. But it doesnât give us all the information that we want.â
The team does not yet have a picture of Sgr A\*. But the researchers were able to collect some data on it. They are continuing to analyze those data in the hopes of adding to a new gallery of black hole portraits. Since the appearance of that black hole changes so quickly, the team is having to develop new techniques to analyze the data from it.
âThe Milky Way is a very different galaxy from M87,â Loeb notes. Studying such different environments could reveal more details of how black holes behave, he says.
The next look at the M87 and Milky Way behemoths will have to wait, though. Scientists got a lucky stretch of good weather at all eight sites that made up the Event Horizon Telescope in 2017. Then there was bad weather in 2018. (Water vapor in the atmosphere can interfere with the telescopeâs measurements.) Technical difficulties cancelled this yearâs observing run.
The good news is that by 2020, EHT will include 11 observatories. The Greenland Telescope joined the consortium in 2018. The Kitt Peak National Observatory outside Tucson, Ariz., and the NOrthern Extended Millimeter Array (NOEMA) in the French Alps will join EHT in 2020.
Adding more telescopes should allow the team to extend the image. That would let EHT better capture the jets that spew from the black hole. The researchers also plan to make observations using light having a slightly higher frequency. That can further sharpen the image. And even bigger plans are on the horizon â adding telescopes that orbit Earth. âWorld domination is not enough for us. We also want to go to space,â Doeleman quipped.
These extra eyes may be just whatâs needed to bring black holes into even greater focus.
*Staff writer Maria Temming contributed to this story.*
### Power Words
[More About Power Words](https://www.snexplores.org/power-words-aid-stem-literacy/)
**align** (noun: alignment) To place or organize things in a patterned order, following an apparent line.
**astrophysics** An area of astronomy that deals with understanding the physical nature of stars and other objects in space. People who work in this field are known as **astrophysicists**.
**behemoth** A term for anything that is amazingly big. The term comes from a monstrous animal described in the Bibleâs book of Job.
**black hole** A region of space having a gravitational field so intense that no matter or radiation (including light) can escape.
**consortium** A group or association of independent organizations.
**constellation** Patterns formed by prominent stars that lie close to each other in the night sky. Modern astronomers divide the sky into 88 constellations, 12 of which (known as the zodiac) lie along the sunâs path through the sky over the course of a year. Cancri, the original Greek name for the constellation Cancer, is one of those 12 zodiac constellations.
**diameter** The length of a straight line that runs through the center of a circle or spherical object, starting at the edge on one side and ending at the edge on the far side.
**event horizon** An imaginary sphere that surrounds a black hole. The more massive the black hole, the bigger the sphere. Anything that happens inside the event horizon is invisible, because gravity is so strong that under normal circumstances even light canât escape. But according to some theories of physics, in certain situations small amounts of radiation can escape.
**galaxy** A massive group of stars bound together by gravity. Galaxies, which each typically include between 10 million and 100 trillion stars, also include clouds of gas, dust and the remnants of exploded stars.
**gravity** The force that attracts anything with mass, or bulk, toward any other thing with mass. The more mass that something has, the greater its gravity.
**light-year** The distance light travels in one year, about 9.48 trillion kilometers (almost 6 trillion miles). To get some idea of this length, imagine a rope long enough to wrap around the Earth. It would be a little over 40,000 kilometers (24,900 miles) long. Lay it out straight. Now lay another 236 million more that are the same length, end-to-end, right after the first. The total distance they now span would equal one light-year.
**mass** A number that shows how much an object resists speeding up and slowing down â basically a measure of how much matter that object is made from.
**mechanics** The study of how things move.
**Milky Way** The galaxy in which Earthâs solar system resides.
**National Science Foundation** The U.S. Congress created this independent federal agency in 1950 to promote the advancement of science; national health, prosperity and welfare; and the nationâs defense. This agency funds nearly one-fourth of all federally supported basic research in U.S. colleges and universities. In many fields such as mathematics, computer science and the social sciences, NSF is the major source of federal funding.
**network** A group of interconnected people or things. (v.) The act of connecting with other people who work in a given area or do similar thing (such as artists, business leaders or medical-support groups), often by going to gatherings where such people would be expected, and then chatting them up. (n. networking)
**observatory** (in astronomy) The building or structure (such as a satellite) that houses one or more telescopes.
**particle** A minute amount of something.
**physics** The scientific study of the nature and properties of matter and energy. Classical physics is an explanation of the nature and properties of matter and energy that relies on descriptions such as Newtonâs laws of motion. Quantum physics, a field of study that emerged later, is a more accurate way of explaining the motions and behavior of matter. A scientist who works in such areas is known as a **physicist**.
**quantum** (pl. quanta) A term that refers to the smallest amount of anything, especially of energy or subatomic mass.
**quantum mechanics** A branch of physics dealing with the behavior of matter on the scale of atoms or subatomic particles.
**relativity** (in physics) A theory developed by physicist Albert Einstein showing that neither space nor time are constant, but instead affected by oneâs velocity and the mass of things in your vicinity.
**spacetime** A term made essential by Einsteinâs theory of relativity, it describes a designation for some spot given in terms of its three-dimensional coordinates in space, along with a fourth coordinate corresponding to time.
**standards** (in research) The values or materials used as benchmarks against which other things can be compared.
**star** The basic building block from which galaxies are made. Stars develop when gravity compacts clouds of gas. When they become dense enough to sustain nuclear-fusion reactions, stars will emit light and sometimes other forms of electromagnetic radiation. The sun is our closest star.
**sun** The star at the center of Earthâs solar system. Itâs an average size star about 26,000 light-years from the center of the Milky Way galaxy. Also a term for any sunlike star.
**telescope** Usually a light-collecting instrument that makes distant objects appear nearer through the use of lenses or a combination of curved mirrors and lenses. Some, however, collect radio emissions (energy from a different portion of the electromagnetic spectrum) through a network of antennas.
**theoretical** An adjective for an analysis or assessment of something that based on pre-existing knowledge of how things behave. It is not based on experimental trials. Theoretical research tends to use math â usually performed by computers â to predict how or what will occur for some specified series of conditions. Experimental testing or observations of natural systems will then be needed to confirm what had been predicted.
**theory** (in science) A description of some aspect of the natural world based on extensive observations, tests and reason. A theory can also be a way of organizing a broad body of knowledge that applies in a broad range of circumstances to explain what will happen. Unlike the common definition of theory, a theory in science is not just a hunch. Ideas or conclusions that are based on a theory â and not yet on firm data or observations â are referred to as theoretical. Scientists who use mathematics and/or existing data to project what might happen in new situations are known as theorists.
**universe** The entire cosmos: All things that exist throughout space and time. It has been expanding since its formation during an event known as the Big Bang, some 13.8 billion years ago (give or take a few hundred million years).
**verify** (n. verification) To demonstrate or confirm in some way that a particular claim or suspicion is true.
**weather** Conditions in the atmosphere at a localized place and a particular time. It is usually described in terms of particular features, such as air pressure, humidity, moisture, any precipitation (rain, snow or ice), temperature and wind speed. Weather constitutes the actual conditions that occur at any time and place. Itâs different from climate, which is a description of the conditions that tend to occur in some general region during a particular month or season.
Lisa Grossman is the astronomy writer at *Science News*. She has a degree in astronomy from Cornell University and a graduate certificate in science writing from University of California, Santa Cruz. She lives near Boston.
*Science News* physics writer Emily Conover studied physics at the University of Chicago. She loves physics for its ability to reveal the secret rules about how stuff works, from tiny atoms to the vast cosmos. |
| Shard | 138 (laksa) |
| Root Hash | 10963673681106489938 |
| Unparsed URL | org,snexplores!www,/article/black-hole-first-photo-event-horizon-telescope s443 |