What is dark matter? Searching with gravity, lensing, WIMPs, and antiparticles.

I’m Looking for Evidence That Dark Matter Messed With Stars and Galaxies

I’m Looking for Evidence That Dark Matter Messed With Stars and Galaxies

What are astronomy's most intriguing puzzles?
Feb. 25 2014 8:00 AM

The Dark Matter Poltergeist

It’s real, but what is it?

The pink is the hot gas (by far most of the mass of the luminous matter) and the blue is a visualization of the dark matter based on gravitational lensing measurements.
The pink represents the hot gas (by far most of the mass of the luminous matter), and the blue is a visualization of the dark matter based on gravitational lensing measurements.

Photo courtesy NASA/CXC/CfA/M.Markevitch

Touch something. Anything. What do you feel? Does it push back? That’s electromagnetism. Any time you touch something solid, the sensation of not being able to put your hand right through it is caused by the electromagnetic force of the atoms in your hand pushing against the atoms of the object in question. Electromagnetism governs every interaction we have with the world—touch, sight, even smell and taste when you consider that the chemical reactions we perceive through these senses are changes in (electromagnetic) molecular bonds.

How strange, then, that the evolution of the universe, the motions of galaxies, the formation of massive objects on the largest scales, are all governed by something that appears to have no interaction with electromagnetism at all. Dark matter, the mysterious substance that makes up more than 80 percent of the matter in the universe, is literally untouchable. It passes right through you, through the planet, through stars and gas and everything in the universe that we can see. It is invisible, at the most fundamental level. But it does have gravity, which is the defining property of things we call matter. And it is so abundant that “luminous” matter—the stuff we can see and touch—is little more than an afterthought in the large-scale structure of the cosmos.

Astronomers have known about dark matter since the 1930s, and they’ve been seeking an explanation ever since. The first clues came from the mysterious motions of galaxies. Like a poltergeist, dark matter makes things fly around in ways they really aren’t supposed to. Stars orbiting the centers of their galaxies travel so fast that they should be flung out into the cosmos, but they aren’t. Galaxies in clusters dance around one another, held in formation by something unseen. We study astronomical images, carefully accounting for the gravitational pull of everything we can see—stars, gas, dust, even black holes lit up by the matter they’re consuming—and it simply isn’t enough. There must be something else there, a ghostly cloud of invisible matter surrounding and enveloping each galaxy and cluster. At a loss as to what this invisible substance could be, we call it dark matter.


The mystery of dark matter’s true identity lies at the intersection of cosmology and fundamental physics. If we can understand what it is, how it behaves, and where it came from, we can explain how the cosmos was built into the web of clusters and filaments we observe today. If we can identify dark matter as a new fundamental particle, we will have the first major departure from the standard model of particle physics—a paradigm that has held up to nearly every experimental test to an astounding degree of accuracy. Dark matter has the potential to open up the world of supersymmetry, a theoretical extension of the standard model that posits the existence of a whole new set of fundamental particles normally hidden from us. If the dark matter particle turns out not to be consistent with supersymmetry’s predictions, a huge branch of theoretical physics gets sent back to the drawing board.

So what do we know? We know dark matter is real—the evidence is overwhelming. Something must be responsible for the extra gravity messing with the motions of stars and galaxies. If that doesn’t convince you, you can look to gravitational lensing—the bending of light around massive objects. The presence of dark matter accounts for the way the light from distant stars and galaxies is distorted as it travels through the universe, following the gravitationally induced curving of space-time itself. If motion and lensing don’t convince you, look at the evidence that galaxies existed within a billion years of the Big Bang. Without dark matter as a kind of cosmic glue, galaxies would have taken much longer to form, as the gravity of gas and dust and stars had to fight against the pressure of all that matter colliding and heating up. Or just take a look at the Bullet Cluster. It’s the aftermath of a cosmic collision in which clusters of galaxies collided but the bulk of the matter passed right through the collision, in the way only ghostly dark matter could.

Even if somehow the clues have misled us completely, and some physical process were presented that mimicked dark matter without a new fundamental particle, it would require a rethinking of the basic laws of gravity and lead to a major revolution in our understanding of the universe.

What else do we know about dark matter? We know it doesn’t interact with electromagnetism in any significant way. It doesn’t absorb or emit light, and it doesn’t seem to experience friction or collisions with itself or other matter. It is probably passing through you right now, but without electromagnetic interactions, you won’t feel a thing. We know that it’s “cold,” in the sense that whatever makes it up is not moving at anything close to the speed of light. (Exactly how cold is still a matter of some debate—it could still be a little bit warm, or, perhaps, tepid.) We’re pretty sure dark matter is some kind of particle, but as far as we’ve seen, the only way dark matter particles interact with anything at all is through their gravity. Our theories (and our hopes!) depend on the possibility that dark matter can interact, if only rarely, via another kind of force: the weak force.