The Invisible Threads of the Cosmos ✎ express

Original: "Mati\`ere noire et (ou) gravitation modifi\'ee : une approche historique et \'epist\'emologique"
arXiv:2601.06592 · 2026-01-10 · CC BY-NC-ND 4.0 · independent analysis · 1 min
Most of the matter in the universe doesn't shine, but it holds galaxies together like an invisible scaffold.

📄 Showing the "Simple" version — "Advanced" is not ready yet. Add it to favorites to help prioritize it.

The night sky is full of stars, but they are only a small part of everything that exists in the universe. Astronomers have long noticed a strange thing: galaxies rotate so fast that they should fly apart, yet they don't. Something invisible holds them together, like invisible threads linking beads on a spinning wheel.

This "something" was named dark matter. It doesn't shine, doesn't reflect light, but it attracts ordinary matter. Without it, galaxies couldn't have gathered into the clusters we see. Dark matter also explains how light from distant galaxies is bent, as if you were looking through warped glass.

There is about five times more dark matter in the universe than ordinary matter, the stuff that makes up stars, planets, and us.

But there is another path: maybe we don't need new matter, but a change to the law of gravity. Some scientists propose tweaking Newton's formula to do away with invisible matter. So far, no alternative explains everything, so the search continues.

If you took a sugar cube of dark matter, it would weigh as much as a mountain, yet be completely invisible.

In the TV series "Dark Matter," the characters wake up on a ship with no memory — much like scientists who still don't know what this invisible substance is made of.

Scientists
Fritz ZwickyIsaac NewtonJohn MichellRobert HookeVera RubinAdam Riess
Concepts
dark matter dark matter curvature galaxy formation cosmology structure growth cosmic structure formation cosmic microwave background obscuration universe galaxy distribution early universe galaxies background radiation standard cosmological model first stars weak lensing radiation dominated era gravitational theory fritz zwicky gravitational lensing analysis mass distribution galactic evolution