Posted on 07/14/2025 9:19:21 AM PDT by Red Badger
This artist's conception depicts ordinary matter in the warm, thin gas making up the intergalactic medium (IGM)—which has been difficult for scientists to directly observe until now. Different colors of light travel at different speeds through space. Here, the artist has used blue to highlight denser regions of the cosmic web, transitioning to redder light for void areas. Credit: Jack Madden, IllustrisTNG, Ralf Konietzka, Liam Connor/CfA
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Using Caltech's DSA-110 radio telescope, astronomers pinpoint whereabouts of "fog" between galaxies
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The vast majority of matter in the universe is dark—it is entirely invisible and detected only through its gravitational effects. Ordinary matter—everything from protons to planets to people—makes up only 16 percent. Unlike dark matter, ordinary matter emits light of various wavelengths and thus can be seen. But a large chunk of it is diffuse and spread thinly among halos that surround galaxies as well as in the vast spaces between galaxies.
Due to its diffuse nature, roughly half of ordinary matter in the universe went unaccounted for and had been considered "missing"—until now.
A new study has pinpointed the universe's "missing" matter using fast radio bursts (FRBs)—brief, bright radio signals from distant galaxies—as a guide. This artist's conception depicts a bright pulse of radio waves (the FRB) on its journey through the fog between galaxies, known as the intergalactic medium. Long wavelengths, shown in red, are slowed down compared to shorter, bluer wavelengths, allowing astronomers to "weigh" the otherwise invisible ordinary matter. Credit: Melissa Weiss/CfA
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In a new study in Nature Astronomy, a team of astronomers at Caltech and the Center for Astrophysics | Harvard & Smithsonian (CfA) has, for the first time, directly detected and accounted for all the missing matter. To do this, the team used brief, bright radio flashes in the distant cosmos, called fast radio bursts (FRBs), to illuminate the matter lying between the FRBs and us.
"The FRBs shine through the fog of the intergalactic medium, and by precisely measuring how the light slows down, we can weigh that fog, even when it's too faint to see," says Liam Connor, assistant professor at Harvard and lead author of the study, who performed much of the work while a Caltech research assistant professor working with Vikram Ravi, assistant professor of astronomy at Caltech.
This artist's diagram depicts some of the 60 FRBs in the study—FRB 20221219A, FRB 20231220A, and FRB 20240123A—which were used to track the journey of gas through the space between galaxies and map the cosmic web. Credit: Jack Madden/CfA, IllustrisTNG Simulations
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The study looked at a total of 69 FRBs located at distances ranging from about 11.74 million to about 9.1 billion light-years away. The object 9.1 billion light-years away, named FRB 20230521B, now holds the record for the most distant FRB ever recorded. While more than a thousand FRBs have been detected, only about a hundred have been pinpointed to specific host galaxies; in other words, their origins and distances from Earth are known. These localized FRBs were needed for the current study.
Of the 69 localized FRBs in the study, 39 were found using the DSA (Deep Synoptic Array)-110, a National Science Foundation (NSF)-funded network of 110 radio telescopes located at Caltech's Owen Valley Radio Observatory (OVRO), near Bishop, California. The radio array, which was designed specifically to catch and localize FRBs, detected the 39 objects and identified their galaxy of origin, while instruments at Hawaii's W. M. Keck Observatory and at the Palomar Observatory near San Diego ascertained their distance. The 30 other FRBs in the study were discovered by telescopes around the world, primarily the Australian Square Kilometre Array Pathfinder.
These FRBs, though fascinating in their own right, were used in this study to detect the missing ordinary matter; other techniques had only hinted at its existence. As radio-frequency light travels from the FRBs to Earth, the light becomes spread out into different wavelengths like a prism turns sunlight into a rainbow. The degree of this spreading, or dispersion, depends on how much matter is in the path of the light.
"It's like we're seeing the shadow of all the baryons, with FRBs as the backlight," says Ravi. "If you see a person in front of you, you can find out a lot about them. But if you just see their shadow, you still know that they're there and roughly how big they are."
The results revealed that 76 percent of the universe's normal matter lies in the space between galaxies, also known as the intergalactic medium. About 15 percent resides in galaxy halos, and the remainder is concentrated within galaxies—in stars or in cold galactic gas. This distribution lines up with predictions from advanced cosmological simulations but has never been observationally confirmed until now.
The findings will help researchers better understand how galaxies grow, and also demonstrate how FRBs can help with problems in cosmology, including the determination of the typical mass of subatomic particles called neutrinos. (The neutrino mass depends on the degree to which baryons cluster.) The standard model of physics predicts that neutrinos should have no mass, but observations have shown that these particles do have an incredibly tiny amount. Knowing the precise mass of neutrinos may therefore lead to new physics beyond the standard model of particle physics.
According to Ravi, this is just the beginning of the use of FRBs in cosmology. In the future, Caltech's DSA-2000 radio telescope in the Nevada desert, currently in the planning stage, will build upon studies like this one. The radio array will find and localize up to 10,000 FRBs per year, dramatically enhancing their role as probes of normal matter and deepening our overall knowledge of the extreme blasts.
The study titled
"A gas rich cosmic web revealed by partitioning the missing baryons,"
was funded by the NSF. Other Caltech authors include Kritti Sharma (MS '24), Stella Koch Ocker, Jakob Faber (MS '24), Gregg Hallinan, Charlie Harnach, Greg Hellbourg, Rick Hobbs, David Hodge, Mark Hodges, Nikita Kosogorov (MS '24), James Lamb, Casey Law, Paul Rasmussen, Myles Sherman, Jean Somalwar, Sander Weinreb, and David Woody.
in the bank in the middle of Beverly Hills under somebody else’s name.
Here come the fairy tales again.
Help me out here. Are these simply presumed based upon statistical data of the behavior of FRBs? Are these "shifts" so big they are obvious? I don't get it.
Sorry.
It was all under my bed.
I was afraid to admit it.
To another dimension.
Lol Good one.
Measure the time lag of the different ‘colors’ of the same FRB spectrum.........
For something that large, she would need a convex mirror to give enough surface area.
Quantum Superposition means a particle can exist in multiple states simultaneously.
An electron can be here and there.
A photon can spin clockwise and counterclockwise.
An atom can be excited and relaxed at the same time.
We only see one outcome when we measure it. (Heisenberg effect)
I can be excited and relaxed at the same time.
I understood the metric. What I don't understand is how they know what was the spectrum at the source by which to measure the change.
If I have a flashlight, and I shoot it through a lens, if I don't know anything about that lens or the incident source, how do I characterize the lens from the detecting instruments at the receiving side of the lens?
Sounds like a better way to describe what we cannot see.
All that Fog? Does not sound like good explanation.
Who knows? Maybe to Heaven which is beyond the universe.
Yes.
My point, man is not meant to understand everything. Just to keep us in our place.
AI will not be the solution either.
God is laughing at us. Smile.
That’s one big couch.
It’s always in the last place you look.
I can confirm that the universe is missing matter. There is a pile of Gold missing from my back yard.
Good. I’m short a sock.
excited and relaxed at the same time: the Lazmataz effect.
Professor Laz, care to elucidate? I don’t know how it happens. It just does.
We know that certain elements absorb certain wavelengths and not others. So if a certain wavelength is missing, slowed or shifted, then we know that some particular matter must be in between the source and our observation...........
It was hiding in plain sight...
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