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At the heart of the Milky Way, where stars orbit dangerously close to a supermassive black hole, some of them may be living on borrowed time—or not aging at all. New research explores an extraordinary idea: certain stars near the galactic center might be powered not by fusion alone, but by the energy released from collisions between dark matter particles and their antimatter counterparts. This concept doesn’t just challenge conventional models—it reshapes what we understand about stellar evolution. What Shapes a Star's Life? The foundation of a star’s life lies in its mass. Mass determines how quickly a star burns hydrogen, when it moves on to heavier elements, and how it ultimately fades. The "main sequence"...
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Why Most of the Universe’s Matter Isn’t in Stars or Galaxies
The universe often appears to us as a glittering sea of stars, planets, and galaxies. Because these luminous objects fill the images we see, it’s natural to think they house most of the matter in the cosmos. But in truth, only a small slice of ordinary, atom-based matter exists inside them. The majority is distributed across vast, nearly empty regions.
Thanks to recent studies, astronomers are beginning to map where this hidden matter actually resides.
The Small Share Held by Stars and Galaxies
The Big Bang theory predicts that roughly 5% of the universe consists of atoms. Stars might seem the obvious repositories. Galaxies host hundreds of billions of stars, and the observable universe contains around 10²³ stars—far outnumbering every grain of sand on Earth. Despite this, the total atoms in stars is modest.
Instagram | sciencewithjahir | The vast majority of atomic matter lies beyond stars and galaxies.
Highlights include:
- Stars contain only 0.5% of matter.
- About 0.03% of matter consists of heavier elements, like carbon and oxygen.
- The universe has roughly 10⁸² atoms, most of which aren’t in visible structures.
This leaves a vast amount of ordinary matter unaccounted for—scattered far beyond the glowing cores of galaxies.
The Vast Reservoir Between Galaxies
The intergalactic medium—the space between galaxies—is the most likely hiding place. Often called a vacuum, it is far from empty. This region hosts faint, wispy filaments known as the cosmic web. Though its average density is only about one atom per cubic meter—a fraction of anything on Earth—the immense scale of the universe gives this matter significant mass.
This medium also reaches temperatures of millions of degrees, making it glow primarily in X-rays. Most X-ray telescopes lack the sensitivity needed to map this thin, hot gas with precision, which is why so much ordinary matter remained undetected for decades.
Radio Bursts as a New Measuring Stick
A breakthrough came from studying mysterious cosmic signals known as fast radio bursts (FRBs). These bursts release as much energy in a single millisecond as the Sun emits in three days. Since their first discovery in 2007, researchers have traced them to the surroundings of ultra-dense neutron stars.
A specific type, called a magnetar, is believed to generate many of these bursts. Magnetars possess magnetic fields a thousand trillion times stronger than Earth’s, making them some of the most extreme objects known.
As FRBs travel across the universe, electrons in intergalactic gas slow the longer wavelengths of their radio waves. This stretching of the signal acts like a measurement tool. By analyzing how much the wavelengths spread, astronomers can estimate how much gas each burst passed through on its journey to Earth.
Completing the Inventory of Ordinary Matter
edition.cnn.com | Fast radio bursts confirm the Big Bang model’s predicted 5% distribution of normal matter.
A major study released in June 2025 by scientists from Caltech and the Harvard Center for Astrophysics used 69 fast radio bursts collected with an array of 110 radio telescopes in California. Their findings clarified where the universe’s matter is distributed:
1. 76% lies in the intergalactic medium.
2. 15% resides in halos around galaxies.
3. 9% sits inside galaxies as stars and cold gas.
This distribution matches the Big Bang model’s predictions almost exactly. Recovering the expected 5% of normal matter serves as a powerful confirmation of the theory’s accuracy.
As new radio telescope arrays come online, the number of detected bursts is expected to rise to 10,000 per year. With such large samples, FRBs may soon help map the three-dimensional structure of the cosmic web itself.
What About the Rest of the Universe?
Although the distribution of ordinary matter is now fully mapped, most of the universe consists of mysterious components. Dark matter, which makes up about 27% of the cosmos, functions like an invisible skeleton that shapes galaxies. Its effects are visible through gravitational lensing, where light bends more strongly than visible matter alone could explain, indicating that dark matter outweighs ordinary matter by over five times.
Meanwhile, dark energy is the enigmatic force accelerating the universe’s expansion. Together, these unseen elements dominate the universe, yet their true nature remains elusive. Ordinary matter—everything made of atoms—forms just a tiny portion, much of it floating in the vast spaces between galaxies. Thanks to fast radio bursts and new observational techniques, astronomers can now trace this hidden matter with unprecedented clarity.
While dark matter and dark energy remain mysteries, the case of the universe’s missing atoms has finally been closed.
