Scientists have finally located the missing ordinary matter in the universe, which makes up stars, planets, and people.
Through a study by the Center for Astrophysics | Harvard & Smithsonian and Caltech, it was found that over three-quarters of the universe's ordinary matter is in the intergalactic medium (IGM), the thin hot gas between galaxies.
Fast radio bursts (FRBs) were key to this discovery as they slowed down based on the amount of gas they passed through, helping track the missing matter.
The team analyzed 60 FRBs, some from extremely distant galaxies, to map the distribution of matter in the universe.
Lead author Liam Connor noted that the missing matter was always present but its location was unknown until now.
76% of the universe's baryonic matter was found in the IGM, while 15% resides in halos around galaxies and a small fraction is inside galaxies.
This confirmation aligns with computer models and offers insights into galaxy formation and evolution.
The movement of matter in and out of galaxies influences the universe's structure, akin to a cosmic thermostat.
Upcoming powerful radio telescopes like Caltech's DSA-2000 and Canada's CHORD will enable the discovery of more FRBs, enhancing our understanding of the cosmos.