The universe is mostly empty space, but even the parts that aren’t empty hold secrets. We once thought that dark matter was a single, monolithic ghost floating around galaxies. Now scientists have divided it into two different varieties. This difference is important because it changes our understanding of the history of the cosmos and what makes up most of its mass.

The first variety is surprisingly familiar. It makes up about 4.5 percent of the entire universe. This is not the scary, invisible thing that bends light. It consists of baryons – protons, neutrons and atomic nuclei. These are the same building blocks that make up the stars, the planets, and you. But here’s the catch: most of this baryonic matter doesn’t glow. It’s dark. It does not emit light and is therefore difficult to detect, but it is physically made of the same substances as everything else we know.

Then there is the remaining 26.1 percent. This is real dark matter. It is non-baryonic. We don’t know what it’s made of. It is not atoms. They are not protons or neutrons. It’s something completely different. And it is relatively “cold”. In physics terms, this means that it is not relativistic. It moves slowly compared to the speed of light. This slowness is the key. Cold dark matter clumps together under the influence of gravity to form the framework that holds galaxies together. If it were hot and moving fast, it would fly apart and the galaxies we know wouldn’t exist.

So why separate them? Because one is made of stuff we could touch if only we could find it. The other is a mystery. 4.5 percent is ordinary matter in disguise. 26.1 percent is something new. We’ve detected the first type through its gravitational pull, even though we can’t see it. The second type is identified even more indirectly by the way galaxies rotate and the way light bends around them.

This division is not only semantic. It shows us that “dark matter” is a misnomer for half of it. Half is just normal matter that is hard to detect. The second half is really strange. We don’t have a particle for it yet. We have the equations. We have some clues. But no direct detection.

The cold, non-baryonic variant dominates the mass budget. It’s the glue. The baryonic dark matter is the debris. Both are invisible. Both are dark. But only one is strange. The other just hides.