The invisible glue holding our universe together

Evidence Showing Why Dark Matter Almost Certainly Exists · 17:57 · Video: Arvin Ash · Watch at the source

In short: Every second, trillions of dark matter particles flow through your body without leaving a single trace. It doesn't reflect light, emit radiation, or interact with the electromagnetic spectrum. Yet, without this ghostly substance, galaxies would fly apart like spinning merry-go-rounds missing their bolts.

The existence of dark matter was first proposed in 1933 by Swiss astronomer Fritz Zwicky. While observing the Coma Cluster, Zwicky noticed that galaxies were moving far too quickly to be held together by the gravity of their visible mass alone. He realized something else—which he called "dunkle Materie" or dark matter—was acting as an invisible glue. This concept remained on the fringes until the 1970s, when Vera Rubin and Kent Ford observed that stars at the edges of galaxies orbited just as fast as those near the center, defying Newtonian laws.

Today, we know dark matter makes up about 85% of all matter in the universe, while ordinary baryonic matter—everything from planets to people—accounts for only about 5%. We can map its distribution through gravitational lensing, where the mass of invisible dark matter halos bends light from distant objects. One of the most compelling proofs is the Bullet Cluster: a collision between two galaxy clusters where gravitational lensing shows that dark matter passed straight through the collision, pulling ahead of the visible gas and stars.

Beyond individual galaxies, dark matter acted as "gravitational seeds" in the early universe. It created density fluctuations that allowed ordinary matter to clump together into the first structures. Without these invisible anchors, galaxies might never have formed at all. While some suggest Modified Newtonian Dynamics (MOND) could explain these movements by changing gravity equations, there is no theoretical basis for such changes other than to fit the data. Every major measurement—from galaxy rotation and light bending to the Cosmic Microwave Background—consistently points to a universe dominated by this invisible substance.

Despite its dominance, the specific particles making up dark matter remain unidentified. Since the 1990s, scientists have built massive experiments to catch these elusive particles, but they continue to come up empty-handed. We know it is there because of how it behaves, even if we still don't know what it is.

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