Astronomers have found the universe’s missing matter at last, thanks to exotic ‘fast radio bursts’
https://www.space.com/astronomy/scientists-find-universes-missing-matter-while-watching-fast-radio-bursts-shine-through-cosmic-fog
Astronomers have found the universe’s missing matter at last, thanks to exotic ‘fast radio bursts’
https://www.space.com/astronomy/scientists-find-universes-missing-matter-while-watching-fast-radio-bursts-shine-through-cosmic-fog
4 Comments
>This previously missing stuff isn’t dark matter, the mysterious substance that accounts for around 85% of the material universe but remains invisible because it doesn’t interact with light. Instead, it is ordinary matter made out of atoms (composed of baryons) that does interact with light but has until now just been too dark to see.
For anyone else assuming dark matter from the headline like I did.
The article is misleading. They are talking as if they have solved dark matter as being a very disperse fog of atoms. Yet dark matter is like 5x the amount of matter vs visible matter. What am I missing?
I wonder if this will change how old we think the universe is. If light is interacting with this 85%, its slowing it down (how it was measured in the first place) so does that affect the redshift?
Astronomer here! **This is not dark matter.** But it’s still an important result, and I know the guys involved in this (lead author came to my Halloween party in grad school!), so let’s get to it!
This result is about [this paper](https://www.nature.com/articles/s41550-025-02566-y), and uses [fast radio bursts (FRBs)](https://en.wikipedia.org/wiki/Fast_radio_burst) in an exciting way to map out material in the universe. Specifically, FRBs are as the name implies brief radio bursts that last a millisecond and originate from well beyond the galaxy- millions or even billions of light years away! We can tell because when a FRB is seen, it is over a frequency band, and that radio signal interacts slightly with all the material that it encounters between its origin and us- called the [dispersion measure (DM)](https://astronomy.swin.edu.au/cosmos/*/Pulsar+Dispersion+Measure). The DM is bigger the further you are from Earth and is thus a rough proxy for both distance and how much material is in a given direction.
Now the problem with FRBs to date has been how we have a rough time knowing precisely where one comes from. radio telescopes until recently for FRBs didn’t provide this level of needed detail (if your field of view is say half the size of the moon, it’s still a big sky with a LOT of distant galaxies in it), and we’re only finally getting the hardware in place to rectify this. But the dream was once we figure that out, FRBs could be used to map the very diffuse “normal” matter in our universe spread between galaxies, which right now we don’t know a lot about (such as how much of it there was).
Enter this paper! Liam and his colleagues looked at 69 FRBs that had galaxies identified with them, coming over a range of distances 11 million to 9.1 *billion* light years from us. Once they had the distances pinned down, any extra DM has to do with material on the line of sight between us and those FRBs… and it turns out it adds up to the full amount of “normal” matter we expect to see in the universe! Big deal! It’s just really tough to measure diffuse gas on a line of sight with nothing around it, and looks like FRBs can indeed allow us to do that.
Anyway, big result, but the next work is gonna be more exciting- we will start to be able to map all this diffuse stuff across most of the visible universe! It’ll be cool to see what we find!