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Monster Black Hole Merger Is Most Massive Ever Seen
Monster Black Hole Merger Is Most Massive Ever Seen

Scientific American

time14 hours ago

  • Science
  • Scientific American

Monster Black Hole Merger Is Most Massive Ever Seen

Physicists have detected the biggest ever merger of colliding black holes. The discovery has major implications for researchers' understanding of how such bodies grow in the Universe. 'It's super exciting,' says Priyamvada Natarajan, a theoretical astrophysicist at Yale University in New Haven, Connecticut, who was not involved in the research. The merger was between black holes with masses too big for physicists to easily explain. 'We're seeing these forbidden high-mass black holes,' she says. The discovery was made by the Laser Interferometer Gravitational-Wave Observatory (LIGO), a facility involving two detectors in the United States. It comes at a time when US funding for gravitational-wave detection faces devastating cuts. The results, released as a preprint on the arXiv server 1, were presented at the GR-Amaldi gravitational-waves meeting in Glasgow, UK, on 14 July. On supporting science journalism If you're enjoying this article, consider supporting our award-winning journalism by subscribing. By purchasing a subscription you are helping to ensure the future of impactful stories about the discoveries and ideas shaping our world today. Forbidden mass LIGO detects gravitational waves by firing lasers down long, L-shaped arms. Minuscule changes in arm length reveal the passage of gravitational waves through the planet. The waves are ripples in space-time, caused by massive bodies accelerating, such as when two inspiralling black holes or neutron stars merge. Hundreds of these mergers have been observed using gravitational waves since LIGO's first detection in 2015. But this latest detection, made in November 2023, is the biggest yet. By modelling the signal detected by LIGO, scientists have calculated that the event, dubbed GW231123, was caused by two black holes with masses of about 100 and 140 times that of the Sun merging to form a final black hole weighing in at some 225 solar masses. 'It's the most massive [merger] so far,' says Mark Hannam, a physicist at Cardiff University, UK, and part of the LVK Collaboration, a wider network of gravitational-wave detectors that encompasses LIGO, Virgo in Italy and KAGRA in Japan. It's 'about 50% more than the previous record holder', he says. Most of the events captured by LIGO involve stellar mass black holes — those ranging from a few to 100 times the mass of the Sun — which are thought to form when massive stars end their lives as supernovae. However, the two black holes involved in GW231123 fall in or near a predicted range, of 60–130 solar masses, at which this process isn't expected to work, with theories instead predicting that the stars should be blown apart. 'So they probably didn't form by this normal mechanism,' says Hannam. Instead, the two black holes probably formed from earlier merger events — hierarchical mergers of massive bodies that led to the event detected by LIGO, which is estimated to have happened 0.7 to 4.1 billion parsecs away (2.3—13.4 billion light years). It's like 'four grandparents merging into two parents merging into one baby black hole', says Alan Weinstein, a physicist at the California Institute of Technology in Pasadena and also part of the LVK Collaboration. Models of the black holes also suggest that they were spinning exceedingly fast — about 40 times per second, which is near the limit of what Einstein's general theory of relativity predicts black holes can reach while remaining stable. 'They're spinning very close to the maximal spin allowable,' says Weinstein. Both the spin and the mass could provide clues to how black holes grow in the Universe. One of the biggest questions in astronomy is how the largest black holes, the supermassive black holes found at the centres of galaxies such as the Milky Way, grew in the early cosmos. Although there is plenty of evidence for the existence of stellar mass black holes and supermassive black holes — those of more than a million solar masses — intermediate mass black holes in the range of 100 to 100,000 solar masses have been harder to find. 'We don't see them,' says Natarajan. The latest detection might tell us that 'these intermediate-mass black holes of several hundred solar masses play a role in the evolution of galaxies', says Hannam, perhaps through hierarchical mergers, which could increase the spin speed, as well as the mass, of the resulting black holes. 'Little by little, we're building up a list of the kind of black holes that are out there,' he says. Cuts ahead That growth in knowledge could be hampered by the administration of US President Donald Trump and its proposed cuts to the US National Science Foundation, which runs LIGO. Under the proposal, one of LIGO's two gravitational-wave observatories would be shut down. At the time of this detection in November 2023, Virgo and KAGRA were not operational. Without two detectors, scientists would not have been sure that they had made a real detection of two merging black holes, says Hannam. 'Because we had two detectors, we saw the same blip at the same time,' he says. The closure of one of the observatories would be 'catastrophic', says Natarajan. 'This discovery would not be possible if one arm was turned off.' Planned upgrades to LIGO in the coming years, and the addition of new detectors around the world, including one in India, could greatly increase physicists' capabilities in gravitational-wave research, an area of astronomy that is still in its infancy. 'We're going to be seeing thousands of black holes in the next few years,' says Hannam. 'There's this huge investment that's been done, and it's only just beginning to pay off.'

Largest-ever merger of black holes forms one 225 times the mass of the sun, astronomers say
Largest-ever merger of black holes forms one 225 times the mass of the sun, astronomers say

CBS News

time16 hours ago

  • Science
  • CBS News

Largest-ever merger of black holes forms one 225 times the mass of the sun, astronomers say

Scientists say they detected the largest-ever merger of two black holes, forming one that is 225 times the mass of the sun, adding that the new discovery "pushes the limits of" how astronomers understand how black holes are created. Two black holes combined to make the massive one, according to the LIGO-Virgo-KAGRA Collaboration, an international group that uses gravitational waves to detect black hole mergers and who identified the event. Gravitational waves occur when there are minute distortions in spacetime, caused by events like black hole mergers, the group said in a news release. One of the black holes was about 103 times the mass of the sun. The other was about 137 times it. These large black holes may have been formed by even earlier mergers, Professor Mark Hannam, from Cardiff University and a member of the LIGO Scientific Collaboration, said in a news release. Even within the merger, the black holes are rapidly spinning, scientists said. Their rotation speed is about 400,000 Earth's rotation speed, the collaboration said in a graphic. They are moving at about 80% to 90% of the maximum possible speed. "The black holes appear to be spinning very rapidly — near the limit allowed by Einstein's theory of general relativity," said Dr. Charlie Hoy, a gravitational-wave astrophysicist, LIGO member and postdoctoral research fellow at the University of Portsmouth, in the news release. "That makes the signal difficult to model and interpret." The massive black hole has been dubbed GW231123. Its unusual size and behavior is challenging scientists' understanding of black hole formation, Hannam said. Previously, the largest known black hole that came from a merger was about 140 times the mass of the sun. GW231123's discovery is also opening doors for new avenues of research, astronomers said. The behavior and size of the black hole "pushes the limits of" current theoretical models and existing gravitational-wave detection technology, the LIGO-Virgo-KAGRA Collaboration said. "It will take years for the community to fully unravel this intricate signal pattern and all its implications," Dr. Gregorio Carullo, a LIGO member and an assistant professor at the University of Birmingham's Institute for Gravitational Wave Astronomy, said in a statement. "Despite the most likely explanation remaining a black hole merger, more complex scenarios could be the key to deciphering its unexpected features. Exciting times ahead!" The black hole was discovered in November 2023, during an observation period by the LIGO-Virgo-KAGRA Collaboration. The observation period began in May 2023, and the first part of the period ended in January 2024. More information about GW231123 and other black holes discovered by the collaboration will be presented this month at the 24th International Conference on General Relativity and Gravitation (GR24) and the 16th Edoardo Amaldi Conference on Gravitational Waves, two conferences presented jointly in Glasgow, Scotland. Data from the observation window will be published later in the summer. The data used to detect and study the massive black hole will also be made available for other researchers to use, the collaboration said.

Biggest black hole merger EVER detected has created terrifying ‘monster' that's 225 times as massive as our Sun
Biggest black hole merger EVER detected has created terrifying ‘monster' that's 225 times as massive as our Sun

The Irish Sun

time17 hours ago

  • Science
  • The Irish Sun

Biggest black hole merger EVER detected has created terrifying ‘monster' that's 225 times as massive as our Sun

SCIENTISTS have discovered the biggest black hole merger e ver recorded, as two massive spacetime ripples spiral into each other. The monstrous collision occurred on the outskirts of our Milky Way galaxy, and produced a black hole roughly 225 times more massive than the sun. Advertisement 3 Aerial shot of the advanced LIGO gravitational detector in Livingston, Louisiana - one of the four LVK Collaboration detectors Credit: Alamy Before now, the most massive black hole merger had a total mass of 140 suns. The new collision event, dubbed GW231123, was found by the LIGO-Virgo-KAGRA (LVK) Collaboration - a group of four detectors that identify cataclysmic cosmic events. Each black hole was roughly 100 to 140 times the mass of our Sun before they combined. "This is the most massive black hole binary we've observed through gravitational waves, and it presents a real challenge to our understanding of black hole formation," Mark Hannam, of Cardiff University and a member of the LVK Collaboration, said in a Advertisement READ MORE ON SPACE "Black holes this massive are forbidden through standard stellar evolution models. "One possibility is that the two black holes in this binary formed through earlier mergers of smaller black holes." Evidence of the GW231123 event was discovered in late 2023, when two slight distortions in spacetime were spotted by laser detectors in Louisiana and Washington. 3 The black holes are moving so fast they are too difficult to properly analyse Credit: Alamy Advertisement The signal that arrived at the detectors was coming from two high-mass black holes that were spinning rapidly - meaning they were hard to analyse. Most read in Science Charlie Hoy, of the University of Portsmouth and also a member of the LVK, explained: "The black holes appear to be spinning very rapidly - near the limit allowed by Einstein's theory of general relativity. "That makes the signal difficult to model and interpret. "It's an excellent case study for pushing forward the development of our theoretical tools." Advertisement Horrifying black hole simulation shows what 'spaghettification' looks like when objects fall into 'extreme slurp' Researchers say they need to observe more similar, high-spin mergers to better calculate just how massive this most recent black hole merger is. Gregorio Carullo, of the University of Birmingham and a member of the LVK, noted: "It will take years for the community to fully unravel this intricate signal pattern and all its implications. "Despite the most likely explanation remaining a black hole merger, more complex scenarios could be the key to deciphering its unexpected features." The researchers are set to present their findings at the Advertisement Black holes are formed through the collapse of massive stars or through the merging of smaller black holes. Known black holes currently fall into just two categories: stellar-mass black holes, which range from a few to a few dozen times the Sun's mass; and supermassive black holes, which can be anywhere from about 100,000 to 50 billion times as massive as the Sun. Intermediate-mass black holes fall into the gap of these two mass ranges and are physically unable to form from direct star collapse and are incredibly rare. Astrophysicists reckon these rare types of black holes grow from merging with others that are similar in size - like our most recent collision event. Advertisement 3 Researchers say they need to observe more similar, high-spin mergers to better calculate just how massive this most recent black hole merger is Credit: Alamy What is a black hole? The key facts Here's what you need to know... A black hole is a region of space where absolutely nothing can escape That's because they have extremely strong gravitational effects, which means once something goes into a black hole, it can't come back out They get their name because even light can't escape once it's been sucked in – which is why a black hole is completely dark What is an event horizon? There has to be a point at which you're so close to a black hole you can't escape Otherwise, literally everything in the universe would have been sucked into one The point at which you can no longer escape from a black hole's gravitational pull is called the event horizon The event horizon varies between different black holes, depending on their mass and size What is a singularity? The gravitational singularity is the very centre of a black hole It's a one-dimensional point that contains an incredibly large mass in an infinitely small space At the singularity, space-time curves infinitely, and the gravitational pull is infinitely strong Conventional laws of physics stop applying at this point How are black holes created? Most black holes are made when a supergiant star dies This happens when stars run out of fuel – like hydrogen – to burn, causing the star to collapse When this happens, gravity pulls the centre of the star inwards quickly and collapses into a tiny ball It expands and contracts until one final collapse, causing part of the star to collapse inwards thanks to gravity, and the rest of the star to explode outwards The remaining central ball is extremely dense, and if it's especially dense, you get a black hole

Biggest black hole merger EVER detected has created terrifying ‘monster' that's 225 times as massive as our Sun
Biggest black hole merger EVER detected has created terrifying ‘monster' that's 225 times as massive as our Sun

Scottish Sun

time17 hours ago

  • Science
  • Scottish Sun

Biggest black hole merger EVER detected has created terrifying ‘monster' that's 225 times as massive as our Sun

Each black hole was roughly 100 to 140 times the mass of our Sun before they combined HOLE-Y SMOKES Biggest black hole merger EVER detected has created terrifying 'monster' that's 225 times as massive as our Sun Click to share on X/Twitter (Opens in new window) Click to share on Facebook (Opens in new window) SCIENTISTS have discovered the biggest black hole merger ever recorded, as two massive spacetime ripples spiral into each other. The monstrous collision occurred on the outskirts of our Milky Way galaxy, and produced a black hole roughly 225 times more massive than the sun. Sign up for Scottish Sun newsletter Sign up 3 Aerial shot of the advanced LIGO gravitational detector in Livingston, Louisiana - one of the four LVK Collaboration detectors Credit: Alamy Before now, the most massive black hole merger had a total mass of 140 suns. The new collision event, dubbed GW231123, was found by the LIGO-Virgo-KAGRA (LVK) Collaboration - a group of four detectors that identify cataclysmic cosmic events. Each black hole was roughly 100 to 140 times the mass of our Sun before they combined. "This is the most massive black hole binary we've observed through gravitational waves, and it presents a real challenge to our understanding of black hole formation," Mark Hannam, of Cardiff University and a member of the LVK Collaboration, said in a statement. "Black holes this massive are forbidden through standard stellar evolution models. "One possibility is that the two black holes in this binary formed through earlier mergers of smaller black holes." Evidence of the GW231123 event was discovered in late 2023, when two slight distortions in spacetime were spotted by laser detectors in Louisiana and Washington. 3 The black holes are moving so fast they are too difficult to properly analyse Credit: Alamy The signal that arrived at the detectors was coming from two high-mass black holes that were spinning rapidly - meaning they were hard to analyse. Charlie Hoy, of the University of Portsmouth and also a member of the LVK, explained: "The black holes appear to be spinning very rapidly - near the limit allowed by Einstein's theory of general relativity. "That makes the signal difficult to model and interpret. "It's an excellent case study for pushing forward the development of our theoretical tools." Horrifying black hole simulation shows what 'spaghettification' looks like when objects fall into 'extreme slurp' Researchers say they need to observe more similar, high-spin mergers to better calculate just how massive this most recent black hole merger is. Gregorio Carullo, of the University of Birmingham and a member of the LVK, noted: "It will take years for the community to fully unravel this intricate signal pattern and all its implications. "Despite the most likely explanation remaining a black hole merger, more complex scenarios could be the key to deciphering its unexpected features." The researchers are set to present their findings at the 24th International Conference on General Relativity and Gravitation (GR24) and the 16th Edoardo Amaldi Conference on Gravitational Waves in Glasgow, Scotland this week. Black holes are formed through the collapse of massive stars or through the merging of smaller black holes. Known black holes currently fall into just two categories: stellar-mass black holes, which range from a few to a few dozen times the Sun's mass; and supermassive black holes, which can be anywhere from about 100,000 to 50 billion times as massive as the Sun. Intermediate-mass black holes fall into the gap of these two mass ranges and are physically unable to form from direct star collapse and are incredibly rare. Astrophysicists reckon these rare types of black holes grow from merging with others that are similar in size - like our most recent collision event. 3 Researchers say they need to observe more similar, high-spin mergers to better calculate just how massive this most recent black hole merger is Credit: Alamy

Biggest black hole merger EVER detected has created terrifying ‘monster' that's 225 times as massive as our Sun
Biggest black hole merger EVER detected has created terrifying ‘monster' that's 225 times as massive as our Sun

The Sun

time17 hours ago

  • Science
  • The Sun

Biggest black hole merger EVER detected has created terrifying ‘monster' that's 225 times as massive as our Sun

SCIENTISTS have discovered the biggest black hole merger ever recorded, as two massive spacetime ripples spiral into each other. The monstrous collision occurred on the outskirts of our Milky Way galaxy, and produced a black hole roughly 225 times more massive than the sun. 3 Before now, the most massive black hole merger had a total mass of 140 suns. The new collision event, dubbed GW231123, was found by the LIGO-Virgo-KAGRA (LVK) Collaboration - a group of four detectors that identify cataclysmic cosmic events. Each black hole was roughly 100 to 140 times the mass of our Sun before they combined. "This is the most massive black hole binary we've observed through gravitational waves, and it presents a real challenge to our understanding of black hole formation," Mark Hannam, of Cardiff University and a member of the LVK Collaboration, said in a statement. "Black holes this massive are forbidden through standard stellar evolution models. "One possibility is that the two black holes in this binary formed through earlier mergers of smaller black holes." Evidence of the GW231123 event was discovered in late 2023, when two slight distortions in spacetime were spotted by laser detectors in Louisiana and Washington. 3 The signal that arrived at the detectors was coming from two high-mass black holes that were spinning rapidly - meaning they were hard to analyse. Charlie Hoy, of the University of Portsmouth and also a member of the LVK, explained: "The black holes appear to be spinning very rapidly - near the limit allowed by Einstein's theory of general relativity. "That makes the signal difficult to model and interpret. "It's an excellent case study for pushing forward the development of our theoretical tools." Horrifying black hole simulation shows what 'spaghettification' looks like when objects fall into 'extreme slurp' Researchers say they need to observe more similar, high-spin mergers to better calculate just how massive this most recent black hole merger is. Gregorio Carullo, of the University of Birmingham and a member of the LVK, noted: "It will take years for the community to fully unravel this intricate signal pattern and all its implications. "Despite the most likely explanation remaining a black hole merger, more complex scenarios could be the key to deciphering its unexpected features." The researchers are set to present their findings at the 24th International Conference on General Relativity and Gravitation (GR24) and the 16th Edoardo Amaldi Conference on Gravitational Waves in Glasgow, Scotland this week. Black holes are formed through the collapse of massive stars or through the merging of smaller black holes. Known black holes currently fall into just two categories: stellar-mass black holes, which range from a few to a few dozen times the Sun's mass; and supermassive black holes, which can be anywhere from about 100,000 to 50 billion times as massive as the Sun. Intermediate-mass black holes fall into the gap of these two mass ranges and are physically unable to form from direct star collapse and are incredibly rare. Astrophysicists reckon these rare types of black holes grow from merging with others that are similar in size - like our most recent collision event. 3 What is a black hole? The key facts Here's what you need to know... A black hole is a region of space where absolutely nothing can escape That's because they have extremely strong gravitational effects, which means once something goes into a black hole, it can't come back out They get their name because even light can't escape once it's been sucked in – which is why a black hole is completely dark What is an event horizon? There has to be a point at which you're so close to a black hole you can't escape Otherwise, literally everything in the universe would have been sucked into one The point at which you can no longer escape from a black hole's gravitational pull is called the event horizon The event horizon varies between different black holes, depending on their mass and size What is a singularity? The gravitational singularity is the very centre of a black hole It's a one-dimensional point that contains an incredibly large mass in an infinitely small space At the singularity, space-time curves infinitely, and the gravitational pull is infinitely strong Conventional laws of physics stop applying at this point How are black holes created? Most black holes are made when a supergiant star dies This happens when stars run out of fuel – like hydrogen – to burn, causing the star to collapse When this happens, gravity pulls the centre of the star inwards quickly and collapses into a tiny ball It expands and contracts until one final collapse, causing part of the star to collapse inwards thanks to gravity, and the rest of the star to explode outwards The remaining central ball is extremely dense, and if it's especially dense, you get a black hole

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