Half of ordinary matter in universe has long been 'missing.' Astronomers just found it.
Astronomers have long estimated that ordinary matter – basically, anything other than dark matter – makes up only a fraction of the known universe.
The conclusion stemmed from a complex calculation involving observed light left over from the Big Bang roughly 13.8 billion years ago. But there was one major problem: they had no clue where about half of it was.
Now, it seems as if a team of astronomers has finally tracked down that missing "ordinary" matter, which they discovered hiding as gas spread out in the vast expanses between galaxies. Revelations made possible by studying radio waves hurtling through space suggest that violent cosmic forces have played a role in the remote locations of almost all of the "missing" matter.
"The question we've been grappling with was: Where is it hiding? The answer appears to be: in a diffuse wispy cosmic web, well away from galaxies," Harvard University astronomy Liam Connor, lead author of the study, told Reuters.
Ordinary matter makes up everything from the cosmic (planets and stars) to the earthly (people and trees.) But it only accounts for about 15% of matter in all of the known universe.
The vast majority of matter is dark – invisible until it is detected only through its gravitational effects.
Unlike dark matter, ordinary matter emits light in various wavelengths, which allow it to easily be seen. Still, scientists have long struggled to account for where all of it is located since a large chunk of ordinary matter is spread so thin among galaxies and the vast spaces between them.
For that reason, about half of ordinary matter has long been considered missing.
Until now.
Powerful bursts of radio waves emanating from 69 locations in the cosmos have helped researchers at long last find the missing matter.
The discovery came from a team of astronomers at the California Institute of Technology and the Center for Astrophysics, a research institute jointly operated by the Harvard College Observatory and Smithsonian Astrophysical Observatory.
The team studied brief, bright radio flashes in the distant cosmos, called fast radio bursts (FRBs), to illuminate the matter lying between the radio waves and Earth.
Astronomers have been studying fast radio bursts from across the universe since 2007 when the first millisecond-long burst was discovered.
The bright burst of electromagnetic radiation may be brief, but fast radio bursts are so powerful that they produce more energy than what our sun emits in an entire year, astronomers say.
The 69 radio frequencies the team studied were located at distances ranging up to about 9.1 billion light-years from Earth – making the furthest one the most distant fast radio burst ever recorded. The previous record was a fast radio burst documented about 8 billion light-years away in 2023.
By measuring how the light from the radio bursts spread and dispersed – not unlike how a prism turns sunlight into a rainbow – while traveling toward Earth, the astronomers were able to determine how much matter was in their path.
"If you see a person in front of you, you can find out a lot about them," Vikram Ravi, a Caltech astronomer who coauthored the study, said in a statement. "But if you just see their shadow, you still know that they're there and roughly how big they are."
The results revealed that about 75% of the universe's ordinary matter resides in the space between galaxies, also known as the intergalactic medium.
How did it all end up in the middle of nowhere? Astronomers theorize it happens as gas is ejected from galaxies when massive stars explode in supernovas, or when supermassive black holes inside galaxies expel material after consuming stars or gas.
The remaining 15% of the "missing" matter exists within either galaxies in the form of stars and cold galactic gas, or in the halos of diffuse material around them, according to the researchers.
While this distribution is in line with predictions from advanced cosmological simulations, this is the first time it has been observed and confirmed, the researchers claim. The findings will help researchers better understand how galaxies grow.
Caltech is also planning for its future deep-space radio telescope in the Nevada desert, the DSA-2000, to build upon the findings when it becomes operational. The radio array is being planned to detect up to 10,000 fast radio bursts per year.
The findings were published June 16 in the journal Nature.
Contributing: Reuters
Eric Lagatta is the Space Connect reporter for the USA TODAY Network. Reach him at elagatta@gannett.com
This article originally appeared on USA TODAY: Astronomers just found the universe's 'missing' matter: Here's how

Try Our AI Features
Explore what Daily8 AI can do for you:
Comments
No comments yet...
Related Articles
Yahoo
7 hours ago
- Yahoo
Scientists Working to Decode Signal From Earliest Years of Universe
As mysterious as the Big Bang that gave birth to the universe is the brief but tumultuous period that immediately followed it. How did the cosmos transform from a uniform sea of darkness into a chaotic swirl brimming with radiant stars? What were these first stars like, and how were they born? So far, we have very strong suspicions, but no hard answers. One reason is that the light from this period, called the cosmic dawn, is extremely faint, making it nearly impossible to infer the traits of these first cosmic objects, let alone directly observe them. But that's about to change, according to a team of international astronomers. In a new study published in the journal Nature Astronomy, the astronomers argue that we're on the verge of finally decoding a radio signal that was emitted just one hundred millions years after the Big Bang. Known as the 21 centimeter signal, which refers to its distinct wavelength, this burst of radiation was unleashed as the inchoate cosmos spawned the earliest stars and black holes. "This is a unique opportunity to learn how the universe's first light emerged from the darkness," said study co-author Anastasia Fialkov, an astronomer from the University of Cambridge in a statement about the work. "The transition from a cold, dark universe to one filled with stars is a story we're only beginning to understand." After several hundred thousand years of cooling following the Big Bang, the first atoms to form in the universe were overwhelmingly neutral hydrogen atoms made of one positively charged proton and one negatively charged electron. But the formation of the first stars unbalanced that. As these cosmic reactors came online, they radiated light energetic enough to reionize this preponderance of neutral hydrogen atoms. In the process, they emitted photons that produced light in the telltale 21 centimeter wavelength, making it an unmistakeable marker of when the first cosmic structures formed. Deciphering these emissions would be tantamount to obtaining a skeleton key to the dawn of the universe. And drum roll, please: employing the Radio Experiment for the Analysis of Cosmic Hydrogen telescope, which is currently undergoing calibration, and the enormous Square Kilometer Array, which is under construction Australia, the researchers say they've developed a model that can tease out the masses of the first stars, sometimes dubbed Population III stars, that are locked inside the 21 centimeter signal. While developing the model, their key revelation was that, until now, astronomers weren't properly accounting for the impact of star systems called x-ray binaries among these first stars. These are systems where a black hole or neutron star is stripping material off a more ordinary star that's orbiting it, producing light in the x-ray spectrum. In short, it appears that x-ray binaries are both brighter and more numerous than what was previously thought. "We are the first group to consistently model the dependence of the 21-centimeter signal of the masses of the first stars, including the impact of ultraviolet starlight and X-ray emissions from X-ray binaries produced when the first stars die," said Fialkov. "These insights are derived from simulations that integrate the primordial conditions of the universe, such as the hydrogen-helium composition produced by the Big Bang." All told, it's another promising leap forward in the field of radio astronomy, where recent advances have begun to reveal an entire "low surface brightness" universe — and a potentially profound one as well, with the promise to illuminate our understanding of the cosmic dawn as never never before. "The predictions we are reporting have huge implications for our understanding of the nature of the very first stars in the universe," said co-author Eloy de Lera Acedo, a Cambridge astronomer and a principal investigator of the REACH telescope. "We show evidence that our radio telescopes can tell us details about the mass of those first stars and how these early lights may have been very different from today's stars." More on astronomy: Scientists Investigating Small Orange Objects Coating Surface of the Moon


Washington Post
10 hours ago
- Washington Post
Blasts seen near Iran's Isfahan nuclear research facility
World Blasts seen near Iran's Isfahan nuclear research facility June 22, 2025 | 8:46 AM GMT Social media video verified by Mitchell Ulrich on X and Reuters shows strikes seen in the direction of the nuclear research facility in Isfahan, Iran.
Yahoo
a day ago
- Yahoo
How could an explosive Big Bang be the birth of our universe?
Curious Kids is a series for children of all ages. If you have a question you'd like an expert to answer, send it to curiouskidsus@ How can a Big Bang have been the start of the universe, since intense explosions destroy everything? – Tristan S., age 8, Newark, Delaware Pretend you're a perfectly flat chess piece in a game of chess on a perfectly flat and humongous chessboard. One day you look around and ask: How did I get here? How did the chessboard get here? How did it all start? You pull out your telescope and begin to explore your universe, the chessboard…. What do you find? Your universe, the chessboard, is getting bigger. And over more time, even bigger! The board is expanding in all directions that you can see. There's nothing that seems to be causing this expansion as far as you can tell – it just seems to be the nature of the chessboard. But wait a minute. If it's getting bigger, and has been getting bigger and bigger, then that means in the past, it must have been smaller and smaller and smaller. At some time, long, long ago, at the very beginning, it must have been so small that it was infinitely small. Let's work forward from what happened then. At the beginning of your universe, the chessboard was infinitely tiny and then expanded, growing bigger and bigger until the day that you decided to make some observations about the nature of your chess universe. All the stuff in the universe – the little particles that make up you and everything else – started very close together and then spread farther apart as time went on. Our universe works exactly the same way. When astronomers like me make observations of distant galaxies, we see that they are all moving apart. It seems our universe started very small and has been expanding ever since. In fact, scientists now know that not only is the universe expanding, but the speed at which it's expanding is increasing. This mysterious effect is caused by something physicists call dark energy, though we know very little else about it. Astronomers also observe something called the Cosmic Microwave Background Radiation. It's a very low level of energy that exists all throughout space. We know from those measurements that our universe is 13.8 billion years old – way, way older than people, and about three times older than the Earth. If astronomers look back all the way to the event that started our universe, we call that the Big Bang. Many people hear the name 'Big Bang' and think about a giant explosion of stuff, like a bomb going off. But the Big Bang wasn't an explosion that destroyed things. It was the beginning of our universe, the start of both space and time. Rather than an explosion, it was a very rapid expansion, the event that started the universe growing bigger and bigger. This expansion is different than an explosion, which can be caused by things like chemical reactions or large impacts. Explosions result in energy going from one place to another, and usually a lot of it. Instead, during the Big Bang, energy moved along with space as it expanded, moving around wildly but becoming more spread out over time since space was growing over time. Back in the chessboard universe, the 'Big Bang' would be like the beginning of everything. It's the start of the board getting bigger. It's important to realize that 'before' the Big Bang, there was no space and there was no time. Coming back to the chessboard analogy, you can count the amount of time on the game clock after the start but there is no game time before the start – the clock wasn't running. And, before the game had started, the chessboard universe hadn't existed and there was no chessboard space either. You have to be careful when you say 'before' in this context because time didn't even exist until the Big Bang. You also have wrap your mind around the idea that the universe isn't expanding 'into' anything, since as far as we know the Big Bang was the start of both space and time. Confusing, I know! Astronomers aren't sure what caused the Big Bang. We just look at observations and see that's how the universe did start. We know it was extremely small and got bigger, and we know that kicked off 13.8 billion years ago. What started our own game of chess? That's one of the deepest questions anyone can ask. Hello, curious kids! Do you have a question you'd like an expert to answer? Ask an adult to send your question to CuriousKidsUS@ Please tell us your name, age and the city where you live. And since curiosity has no age limit – adults, let us know what you're wondering, too. We won't be able to answer every question, but we will do our best. This article is republished from The Conversation, a nonprofit, independent news organization bringing you facts and trustworthy analysis to help you make sense of our complex world. It was written by: Michael Lam, Rochester Institute of Technology Read more: After our universe's cosmic dawn, what happened to all its original hydrogen? Hubble in pictures: astronomers' top picks Curious Kids: Can people colonize Mars? Michael Lam does not work for, consult, own shares in or receive funding from any company or organization that would benefit from this article, and has disclosed no relevant affiliations beyond their academic appointment.