logo
Astronomers Discover Most Energetic Cosmic Explosions Ever Observed

Astronomers Discover Most Energetic Cosmic Explosions Ever Observed

Gizmodo05-06-2025
Astronomers in Hawaii have discovered a new kind of explosion, and they're the most energetic stellar explosions ever recorded.
Meet 'extreme nuclear transients' (ENTs): when supermassive black holes tear apart stars at least three times heavier than the Sun, triggering an immense release of energy. An international team of researchers describes the discovery of this newly observed phenomenon in a study published Wednesday in the journal Science Advances, shedding light on events that will help astronomers study the distant universe.
'We've observed stars getting ripped apart as tidal disruption events for over a decade, but these ENTs are different beasts, reaching brightnesses nearly ten times more than what we typically see,' Jason Hinkle, lead author of the study and PhD student at the Institute for Astronomy at the University of Hawaii, said in a W. M. Keck Observatory statement. Tidal disruptions consist of supermassive black holes tearing apart any star that wanders too close, so ENTs are a kind of tidal disruption.
'Not only are ENTs far brighter than normal tidal disruption events, but they remain luminous for years, far surpassing the energy output of even the brightest known supernova explosions,' he added.
Their discovery took place almost by accident. While searching for enduring flares projecting from the center of galaxies in data from the European Space Agency's Gaia mission, Hinkle came across two strange signals from 2016 and 2018, which started a multi-year investigation. At the same time, two separate teams found a comparable flare from 2020 in an astronomical survey called the Zwicky Transient Facility (ZTF). More data from the W. M. Keck Observatory in Hawaii confirmed the 2020 event's similarity to the two Gaia events.
Given that these events unleashed more energy than any supernova known to science, Hinkle and his colleagues concluded that they weren't your average stellar explosions. The enormous energy release and the shape of the event's light curves indicated the presence of a supermassive black hole actively absorbing material, a process called accretion. Unlike regular black hole accretion, however—which sees nearby matter heat up and project irregular light—the astronomers discovered that these astrophysical events clearly involve a supermassive black hole systematically shredding and eating a giant star.
ENTs represent the most energetic known explosions in the universe. Gaia18cdj, the team's strongest documented ENT, released 25 times more energy than the most energetic supernovae known to science. More broadly, each ENT releases as much energy as 100 Suns would emit over their entire 10-billion-year lifespans. For comparison, a regular supernova usually unleashes similar amounts of energy to a single Sun.
'These ENTs don't just mark the dramatic end of a massive star's life,' Hinkle explained. 'They illuminate the processes responsible for growing the largest black holes in the universe.' ENTs are also at least 10 million times rarer than supernovae. Nevertheless, their massive energy outputs will prove to be extremely useful for astronomers studying far-away massive black holes.
'Because they're so bright, we can see them across vast cosmic distances—and in astronomy, looking far away means looking back in time,' said Benjamin Shappee, study co-author and Associate Professor at the University of Hawaii's Institute for Astronomy. 'By observing these prolonged flares, we gain insights into black hole growth during a key era known as cosmic noon, when the universe was half its current age when galaxies were happening places—forming stars and feeding their supermassive black holes 10 times more vigorously than they do today.'
From theories of black holes leading to white holes to the suggestion that the universe might exist in a black hole and that supermassive black holes could replace particle colliders, the recent study joins a host of research shedding light on one of the most mysterious components of our universe.
Orange background

Try Our AI Features

Explore what Daily8 AI can do for you:

Comments

No comments yet...

Related Articles

A cosmic murder mystery: Scientists spot supernova of star violently stripped to the bone
A cosmic murder mystery: Scientists spot supernova of star violently stripped to the bone

Yahoo

time43 minutes ago

  • Yahoo

A cosmic murder mystery: Scientists spot supernova of star violently stripped to the bone

Israeli and American scientists have uncovered a never-before-seen type of supernova, shedding light on how stars produce and expel heavy elements like silicon and sulfur during their violent deaths. Israeli and American scientists discovered a never-before-seen type of supernova, one that blasts out heavy elements like silicon and sulfur from the body of a dying star, a new study reveals. The findings of this study were published in the peer-reviewed academic journal Nature, and provide evidence for a long theorized part of stellar anatomy. All of this was made possible by witnessing an extremely violent and unusual death of a star, the result of which allowed scientists to look deeper than ever before. Of violence and onions: The death of a star and supernovae To understand what exactly happened, it's important to understand what a supernova is and, before that, to understand what a star is. Stars are, at their core, massive and extremely hot balls of gas, specifically hydrogen and helium. These two elements are very common - in fact, they are so common that they make up almost all matter in the universe. So where does everything else come from? To oversimplify complex astrophysics and chemistry, when these hydrogen and helium come together, they can heat up and new elements can be formed - if the circumstances are right. Stars are where this happens. These giant balls of gas possess cores that are a lot more solid, specifically made of iron. The cores are active and are fueled by a process of energy production, which sees the lighter elements to form heavier ones. This is known by nuclear fusion, and it is this process that keeps the star hot, allowing gases to expand while simultaneously drawing its mass toward the core in a delicate gravitational balance. So that's how some of the heavier elements are made, but others still need more heat - hotter than what a star's core can usually handle. What's more, all those heavier elements are still stuck in the stars. How do they get out and expand into the universe, forming planets and asteroids and more? The answer is that the star has to die. When the star can no longer produce energy, it collapses in on itself. When this happens, it results in a massive explosion, one of the most powerful forces of energy in the universe - a supernova. This fuses some of those heavy elements together to make even heavier ones, and all of them get blasted out into the cosmos. This process is essential to the function of the universe, allowing everything to keep expanding and ultimately sending forth the building blocks of the universe's continued expansion. In other words, everything in the universe is made of stardust, and supernovas are what send that stardust out there to accumulate and make new things. The remnants of that progenitor star are still there, condensing together to form a neutron star or a black hole, or maybe even a diffuse nebula of sorts. So that's what scientists have already known. But there is more to this story. See, stars are a lot like onions and - they have layers. The heavier elements occupy the inner layers, getting heavier and heavier as they get closer to the iron core. The massive outer layers are where those lighter elements, like hydrogen and helium, are. But this was only a theory. Studying a supernova can be hard, as while the stars that go supernova are always 10-100 times heavier than the Sun, the explosion happens in a fraction of a second. Even still, it's possible to observe the bright light from the supernova for some time - even weeks can go by without the light fading. But until now, scientists have only ever seen the traces of light elements like hydrogen and helium, rather than anything heavier. But all of that changed with this study The now deceased star in question is SN2021yfj, a massive star far heavier than our Sun. In September 2021, the flare from its supernova was spotted by Dr. Steve Schulze, a former member of Weizmann Institute of Science's astrophysics team and now a researcher at Northwestern University. Using the Zwicky Transient Facility telescope in California, Schulze and his team did a spectral analysis. What this means is that they looked at the different colors of the flare's light. Each color represents a different element, and by observing which colors are present in its spectrum, scientists can figure out what elements are present. In other words, this is how you can use light and colors to figure out what things are made of. This isn't exactly easy, though, as intrusive obstacles can get in the way of a spectral analysis. In Schulze's case, those obstacles came in the form of clouds, stopping researchers from getting a clear enough image. But someone at the University of California, Berkeley, managed to get it. And the results were shocking. Normally, when studying a supernova, one expects to see the usual suspects of light and abundant elements, like helium, carbon, oxygen, and so on. But that's not what they found. Instead, the light fired out by SN2021yfj with its dying breaths consisted largely of sulfur, silicon, and argon. That's not supposed to happen. So how could the supernova just not have the lighter elements, and instead have the far heavier ones? A cosmic murder mystery: How a star was stripped to its core before death by explosion The conclusion Schulze came to was that something went wrong. Massive stars like SN2021yfj are, as mentioned previously, like onions - they have layers. And some of those layers have been peeled off. This itself isn't unheard of. Stripped stars, as they are known, have been seen before. But those usually have layers made of helium, carbon, or oxygen - exposed when the outermost hydrogen layers were lost somehow. But SN2021yfj must have had even those layers stripped away. That's not like just peeling a few layers off an onion. Rather, it's more like stripping it to the bone - and that's the part that's unheard of. 'This star lost most of the material that it produced throughout its lifetime,' Schulze said in a statement. 'So we could only see the material formed during the months right before its explosion. Something very violent must have happened to cause that.' This is not a thing that should happen. As noted by Weizmann's Dr. Ofer Yaron, a leading expert on supernovae, this level of deep exposure is a major challenge to prevailing theories on how these layers fall away. Something happened that caused this star to die like this. But what? Several theories were put forward. A companion star could have theoretically exerted force that caused the layers to be stripped away. Another explosion or strong stellar winds could have been the culprit. But the main suspect is actually SN2021yfj itself. The star's core likely produced so much heat that the nuclear fusion caused an incredibly powerful burst of energy. This then may have caused the star's layers to be blown apart, sending the outer layers away. This, essentially, means that SN2021yfj ripped itself apart. But this may have happened before. In fact, the shed layers may have collided into one another, or into another layer that had been blown out a previous time, and that resulted in another explosion. But how much does this factor into the death of SN2021yfj? That, currently, is still a mystery. But what is sure is that no one has ever had the chance to look at stellar anatomy this closely, going deeper than anyone has gone before. 'It's always surprising – and deeply satisfying – to discover a completely new kind of physical phenomenon,' said Prof. Avishay Gal-Yam, whose research group in Weizmann's Particle Physics and Astrophysics Department focuses on understanding how the elements are formed in the universe. 'As soon as I saw the data Dr. Schulze sent me, it was obvious we were witnessing something no one had ever seen before. 'Once we identified the spectral signatures of silicon, sulfur, and argon, it was clear this was a major step forward: Peering into the depths of a giant star helps us understand where the heavy elements come from. Every atom in our bodies and in the world around us was created somewhere in the universe and went through countless transformations over billions of years before arriving at its current place, so tracing its origin and the process that created it is incredibly difficult. Now it appears that the inner layers of giant stars are production sites for some of these important, relatively heavy elements.'

How We Mapped Nightmare Commutes on NJ Transit
How We Mapped Nightmare Commutes on NJ Transit

Bloomberg

timean hour ago

  • Bloomberg

How We Mapped Nightmare Commutes on NJ Transit

Today we're bringing you a special edition of MapLab from Aaron Gordon, our colleague on the data team. Last summer I wrote about a stalled New Jersey Transit commuter train that trapped passengers inside a tunnel for three hours during a heat wave with no air conditioning. The overwhelming reader reaction in my inbox was that I had failed to capture the full extent to which service disruptions on the aging system infuriate riders.

Human emissions driving Colorado River ‘megadrought,' CU Boulder research finds
Human emissions driving Colorado River ‘megadrought,' CU Boulder research finds

Yahoo

timean hour ago

  • Yahoo

Human emissions driving Colorado River ‘megadrought,' CU Boulder research finds

Colorado's drought-stricken Blue Mesa Reservoir near Gunnison is pictured on May 30, 2021. (Chase Woodruff/Colorado Newsline) As historic drought conditions on the Western Slope fuel another dangerous wildfire season, a new paper from researchers at the University of Colorado Boulder warns that human-caused climate change is playing a major role in making those conditions worse. Previously published climatological research has found that the Colorado River Basin's current 'megadrought' is the worst dry spell the region has experienced in at least 1,200 years. But a new study, published last week in the journal Nature, concludes that those persistently dry conditions are being driven by human activity 'more intensely — and more directly — than previously understood,' its authors say. Jeremy Klavans and Pedro DiNezio of CU Boulder's Department of Atmospheric and Oceanic Sciences worked with other scientists from around the country to model how global climate patterns affect rainfall across the U.S. southwest. Their findings concern a climate pattern known as the Pacific decadal oscillation. Related to the better-known El Niño-La Niña cycle to the south, the PDO is a natural fluctuation that brings warm water to the northeastern Pacific Ocean near the U.S. West Coast during its 'positive' phase, leading to more storms and higher-than-average rainfall. During its 'negative' phase, however, cooler water and air temperatures result in less precipitation in Western states. Despite typically reversing itself every one or two decades, the PDO has been 'stuck' in the negative, dry phase since the 1990s. By analyzing more than 500 climate model simulations developed by climatologists around the world, the study's authors were able to paint the clearest picture yet of the influence of human activity on the PDO, and the resulting Southwestern megadrought. 'All of them had this common signal when we averaged them together,' DiNezio said in an interview. 'By having so many simulations, we could be absolutely sure that this was not an artifact of a single model, or of a subset of simulations.' Severe drought conditions have persisted in the Colorado River Basin since 2000, putting increased stress on the water supplies relied on by about 40 million people in Colorado and six other Western states. Water levels in two key reservoirs, Lake Mead and Lake Powell, have fallen to record lows in recent years. What's important here is that we're showing that rainfall has also been influenced by humans, in addition to just evaporation ... Both contribute to drought. – Pedro DiNezio, researcher with CU Boulder's Department of Atmospheric and Oceanic Sciences Rising levels of greenhouse gases, mostly the result of fossil-fuel combustion, have caused much of western Colorado and neighboring states in the Colorado River's Upper Basin to warm by an average of more than 4 degrees Fahrenheit above pre-industrial levels, according to National Oceanic and Atmospheric Administration data. Prior research has attributed about 40% of the post-2000 megadrought to higher temperatures alone, as hotter weather leads to greater evaporation of moisture from water surfaces and soils. Modeling global warming's precise impacts on rainfall patterns has proved more elusive, but DiNezio said the new research 'add(s) more human influence to that previous number.' 'What's important here is that we're showing that rainfall has also been influenced by humans, in addition to just evaporation,' he said. 'Both contribute to drought.' Colorado and other states that are parties to the 103-year-old Colorado River Compact have negotiated for years over how to distribute the cuts to water use made necessary by the basin's ongoing drought. The federal Bureau of Reclamation on Friday announced another year of reduced water allocations for the Lower Basin states of Arizona and Nevada. Not long ago, the possibility that the Pacific decadal oscillation would eventually reverse itself offered hope that the long-term drought outlook for the U.S. Southwest wasn't as bad as it seemed. Instead, evidence now suggests the last two decades are the region's 'new normal.' 'I was a Ph.D. student in 2012, and there was a consensus that eventually (the PDO) was going to flip,' DiNezio. 'We had a big El Niño in 2015, and there was this idea that El Niño will flip the PDO back to the opposite, rainfall-producing phase. And we had that big El Niño event, and the PDO remained stuck. We just had an El Niño event in 2023 … and (it) also didn't flip the PDO.' 'That's the most important implication of our findings,' he added. 'That this drought is here to stay, unless we we do something about rising temperatures and global warming.' Colorado Newsline is part of States Newsroom, a nonprofit news network supported by grants and a coalition of donors as a 501c(3) public charity. Colorado Newsline maintains editorial independence. Contact Editor Quentin Young for questions: info@ SUBSCRIBE: GET THE MORNING HEADLINES DELIVERED TO YOUR INBOX Solve the daily Crossword

DOWNLOAD THE APP

Get Started Now: Download the App

Ready to dive into a world of global content with local flavor? Download Daily8 app today from your preferred app store and start exploring.
app-storeplay-store