Black Hole Powerful

Black Hole Powerful

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A black hole eruption marks the most powerful explosion ever spotted

The outburst was five times as energetic as the last record holder

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Radio waves (blue in this composite image) trickle out of a cavity in hot X-ray emitting gas (purple) enveloping a massive galaxy (white, top). The radio waves likely come from high-speed electrons accelerated by an eruption long ago from a gargantuan black hole at the galaxy’s center.
X-ray: S. Giacintucci et al /NRL, CXC/NASA, XMM-Newton/ESA; Radio: GMRT, TIFR, NCRA; Infrared: 2MASS/UMass, IPAC-Caltech/NASA, NSF
Say hello to the Krakatoa of black hole eruptions.
Hundreds of millions of years ago, a supermassive black hole
in a far-off galaxy blew out gas into intergalactic space. The flare-up was
about five
times as powerful as the previous record holder , researchers report in the
March 1 Astrophysical Journal . The energy from this one explosion was
roughly 100 billion times as much as the sun is expected to emit in its entire
lifetime. This makes it not only the most energetic known eruption from a
supermassive black hole — it’s also the most powerful eruption of any kind in
the universe.
Eruptions from enormous black holes aren’t uncommon. The
explosions are powered by the release of pent-up energy in encircling disks of
hot gas. But the team notes that this newfound eruption is thousands of times
more powerful than most.
The source of the eruption was a beast of a galaxy at the
center of the Ophiuchus cluster, a gathering of galaxies nearly 400 million
light-years from Earth. In 2016, researchers noticed the edge of a
cavity in the cluster’s hot, X-ray emitting gas , about 400,000 light-years
from the central galaxy. The excavated region appears to be over a million
light-years across.
To suss out the origin of the cavity, astrophysicist Simona Giacintucci at the U.S. Naval Research Laboratory in Washington, D.C., and colleagues pored through data from several radio telescopes. The scientists found that the cavity glowed with radio waves, likely from electrons accelerated to near the speed of light. The team suggests that the electrons got revved up by a powerful outburst at least 240 million years prior from a supermassive black hole at the heart of the cluster’s central galaxy.
Questions or comments on this article? E-mail us at feedback@sciencenews.org
A version of this article appears in the March 28, 2020 issue of Science News .
S. Giacintucci et al . Discovery of a giant radio fossil in the Ophiuchus galaxy cluster . Astrophysical Journal . Vol. 891, March 1, 2020. doi: 10.3847/1538-4357/ab6a9d.
N. Werner et al . Deep Chandra study of the truncated cool core of the Ophiuchus cluster . Monthly Notices of the Royal Astronomical Society . Vol. 460, August 11, 2016. doi: 10.1093/mnras/stw1171.
Christopher Crockett is an Associate News Editor. He was formerly the astronomy writer from 2014 to 2017, and he has a Ph.D. in astronomy from the University of California, Los Angeles.
Science News was founded in 1921 as an independent, nonprofit source of accurate information on the latest news of science, medicine and technology. Today, our mission remains the same: to empower people to evaluate the news and the world around them. It is published by the Society for Science, a nonprofit 501(c)(3) membership organization dedicated to public engagement in scientific research and education (EIN 53-0196483).

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The quest to understand our solar system begins close to home.
Cassini Significant Events 12/09/09 - 12/15/09
Significant Event Report for Week Ending 1/5/1998

Galaxy NGC 1068 is shown in visible light and X-rays in this composite image. High-energy X-rays (magenta) captured by NASA's Nuclear Spectroscopic Telescope Array, or NuSTAR, are overlaid on visible-light images from both NASA's Hubble Space Telescope and the Sloan Digital Sky Survey. The X-ray light is coming from an active supermassive black hole, also known as a quasar, in the center of the galaxy. This supermassive black hole has been extensively studied due to its relatively close proximity to our galaxy. Image Credit: NASA/JPL-Caltech/Roma Tre Univ.

In 2015, researchers discovered a black hole named CID-947 that grew much more quickly than its host galaxy. The black hole at the galaxy’s center is nearly 7 billion times the mass of our Sun, placing it among the most massive black holes discovered. The galaxy’s mass, however, is considered normal. Because its light had to travel a very long distance, scientists were observing it at a period when the universe was less than 2 billion years old, just 14% of its current age (almost 14 billion years have passed since the Big Bang). Image credit: M. Helfenbein, Yale University / OPAC

Scientists obtained the first image of a black hole, seen here, using Event Horizon Telescope observations of the center of the galaxy M87. The image shows a bright ring formed as light bends due to the intense gravity around a black hole that is 6.5 billion times more massive than our Sun. Image credit: Event Horizon Telescope Collaboration

This animation illustrates the activity surrounding a black hole. While the matter that has passed the black hole's event horizon can't be seen, material swirling outside this threshold is accelerated to millions of degrees and radiates in X-rays. Image credit: CXC/A.Hobart

This illustration shows a glowing stream of material from a star disrupted as it was being devoured by a supermassive black hole. The black hole is surrounded by a ring of dust. When a star passes close enough to be swallowed by a black hole, the stellar material is stretched and compressed as it is pulled in, releasing an enormous amount of energy. Image credit: NASA/JPL-Caltech

NASA’s Chandra X-ray observatory detected record-breaking wind speeds coming from a disk around a black hole. This artist's impression shows how the strong gravity of the black hole, on the left, is pulling gas away from a companion star on the right. This gas forms a disk of hot gas around the black hole, and the wind is driven off this disk at 20 million mph, or about 3% the speed of light. Image credit: NASA/CXC/M.Weiss | More info ›

The central region of our galaxy, the Milky Way, contains an exotic collection of objects, including a supermassive black hole, called Sagittarius A*, weighing about 4 million times the mass of the Sun, clouds of gas at temperatures of millions of degrees, neutron stars and white dwarf stars tearing material from companion stars and beautiful tendrils of radio emission. The region around Sagittarius A* is shown in this composite image with Chandra data (green and blue) combined with radio data (red) from the MeerKAT telescope in South Africa, which will eventually become part of the Square Kilometer Array (SKA). Image credit: X-Ray: NASA/CXC/UMass/D. Wang et al.; Radio: SARAO/MeerKAT

This artist's concept shows the most distant supermassive black hole ever discovered. It is part of a quasar from just 690 million years after the Big Bang. Image credit: Robin Dienel/Carnegie Institution for Science

The central region of this image contains the highest concentration of supermassive black holes ever seen and about a billion over the entire sky. Made with over 7 million seconds of Chandra observing time, this 2017 image is part of the Chandra Deep Field-South. With its unprecedented look at the early universe in X-rays, it offers astronomers a look at the growth of black holes over billions of years starting soon after the Big Bang. In this image, low, medium and high-energy X-rays that Chandra detects are shown as red, green, and blue respectively. Image credit: NASA/CXC/Penn State/B.Luo et al. | More info ›

In this illustration of a black hole and its surrounding disk, gas spiraling toward the black hole piles up just outside it, creating a traffic jam. The traffic jam is closer in for smaller black holes, so X-rays are emitted on a shorter timescale. Image credit: NASA

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This artist concept illustrates a supermassive black hole with millions to billions times the mass of our Sun. Supermassive black holes are enormously dense objects buried at the hearts of galaxies. Image credit: NASA/JPL-Caltech
A black hole is an extremely dense object in space from which no light can escape. While black holes are mysterious and exotic, they are also a key consequence of how gravity works: When a lot of mass gets compressed into a small enough space, the resulting object rips the very fabric of space and time, becoming what is called a singularity. A black hole's gravity is so powerful that it will be able to pull in nearby material and "eat" it.
Want to visit a black hole? We don't recommend it. Find out why these gravitational mysteries are better studied from afar. › More
Here are 10 things you might want to know about black holes:
No light of any kind, including X-rays, can escape from inside the event horizon of a black hole, the region beyond which there is no return. NASA's telescopes that study black holes are looking at the surrounding environments of the black holes, where there is material very close to the event horizon. Matter is heated to millions of degrees as it is pulled toward the black hole, so it glows in X-rays. The immense gravity of black holes also distorts space itself, so it is possible to see the influence of an invisible gravitational pull on stars and other objects.
A stellar-mass black hole, with a mass of tens of times the mass of the Sun, can likely form in seconds, after the collapse of a massive star. These relatively small black holes can also be made through the merger of two dense stellar remnants called neutron stars. A neutron star can also merge with a black hole to make a bigger black hole, or two black holes can collide. Mergers like these also make black holes quickly, and produce ripples in space-time called gravitational waves.
More mysterious are the giant black holes found at the centers of galaxies — the "supermassive" black holes, which can weigh millions or billions of times the mass of the Sun. It can take less than a billion years for one to reach a very large size, but it is unknown how long it takes them to form, generally.
The research involves looking at the motions of stars in the centers of galaxies. These motions imply a dark, massive body whose mass can be computed from the speeds of the stars. The matter that falls into a black hole adds to the mass of the black hole. Its gravity doesn't disappear from the universe.
No. There is no way a black hole would eat an entire galaxy. The gravitational reach of supermassive black holes contained in the middle of galaxies is large, but not nearly large enough for eating the whole galaxy.
It certainly wouldn't be good! But what we know about the interior of black holes comes from Albert Einstein's General Theory of Relativity.
For black holes, distant observers will only see regions outside the event horizon, but individual observers falling into the black hole would experience quite another "reality." If you got into the event horizon, your perception of space and time would entirely change. At the same time, the immense gravity of the black hole would compress you horizontally and stretch you vertically like a noodle, which is why scientists call this phenomenon (no joke) "spaghettification."
Fortunately, this has never happened to anyone — black holes are too far away to pull in any matter from our solar system. But scientists have observed black holes ripping stars apart , a process that releases a tremendous amount of energy.
The Sun will never turn into a black hole because it is not massive enough to explode. Instead, the Sun will become a dense stellar remnant called a white dwarf.
But if, hypothetically, the Sun suddenly became a black hole with the same mass as it has today, this would not affect the orbits of the planets, because its gravitational influence on the solar system would be the same. So, Earth would continue to revolve around the Sun without getting pulled in — although the lack of sunlight would be disastrous for life on Earth.
Stellar-mass black holes are left behind when a massive star explodes. These explosions distribute elements such as carbon, nitrogen and oxygen that are necessary for life into space. Mergers between two neutron stars, two black holes, or a neutron star and black hole, similarly spread heavy elements around that may someday become part of new planets. The shock waves from stellar explosions may also trigger the formation of new stars and new solar systems. So, in some sense, we owe our existence on Earth to long-ago explosions and collision events that formed black holes.

On a larger scale, most galaxies seem to have supermassive black holes at their centers. The connection between the formation of these supermassive black holes and the formation of galaxies is still not understood. It is possible that a black hole could have played a role in the formation of our Milky Way galaxy. But this chicken-and-egg problem — that is, which came first, the galaxy or the black hole? — is one of the great puzzles of our universe.
The most distant black hole ever detected is located in a galaxy about 13.1 billion light-years from Earth. (The age of the universe is currently estimated to be about 13.8 billion years, so this means this black hole existed about 690 million years after the Big Bang.)
This supermassive black hole is what astronomers call a “quasar,” where large quantities of gas are pouring into the black hole so rapidly that the energy output is a thousand times greater than that of the galaxy itself. Its extreme brightness is how astronomers can detect it at such great distances.
The universe is a big place. In particular, the size of a region where a particular black hole has significant gravitational influence is quite limited compared to the size of a galaxy. This applies even to supermassive black holes like the one found in the middle of the Milky Way. This black hole has probably already "eaten" most or all of the stars that formed nearby, and stars further out are mostly safe from being pulled in. Since this black hole already weighs a few million times the mass of the Sun, there will only be small increases in its mass if it swallows a few more Sun-like stars. There is no danger of the Earth (located 26,000 light years away from the Milky Way's black hole) being pulled in.

Future galaxy collisions will cause black holes to grow in size, for example by merging of two black holes. But collisions won't happen indefinitely because the universe is big and because it's expanding, and so it's very unlikely that any sort of black hole runaway effect will occur.
Yes. The late physicist Stephen Hawking proposed that while black holes get bigger by eating material, they also slowly shrink because they are losing tiny amounts of energy called "Hawking radiation."
Hawking radiation occurs because empty space, or the vacuum, is not really empty. It is actually a sea of particles continually popping into and out of existence. Hawking showed that if a pair of such particles is created near a black hole, there is a chance that one of them will be pulled into the black hole before it is destroyed. In this event, its partner will escape into space. The energy for this comes from the black hole, so the black hole slowly loses energy, and mass, by this process.
Eventually, in theory, black holes will evaporate through Hawking radiation. But it would take much longer than the entire age of the universe for most black holes we know about to significantly evaporate. Black holes, even the ones around a few times the mass of the Sun, will be around for a really, really long time!

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By European Space Agency (ESA)
March 15, 2020
Astronomers using ESA’s XMM-Newton and NASA ’s Chandra X-ray space observatories, along with radio telescopes on ground, have spotted the aftermath of the most powerful explosion ever seen in the Universe.
The huge outburst occurred in the Ophiuchus galaxy cluster, a large cosmic conglomerate with thousands of galaxies , hot gas, and dark matter held together by gravity. It is located approximately 39
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