Dark matter: The matter we can't see - James Gillies

3,083,797 views ・ 2013-05-03

TED-Ed


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Translator: Andrea McDonough Reviewer: Jessica Ruby
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The ancient Greeks had a great idea:
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The universe is simple.
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In their minds,
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all you needed to make it were four elements:
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earth,
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air,
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fire,
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and water.
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As theories go, it's a beautiful one.
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It has simplicity and elegance.
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It says that by combining
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the four basic elements in different ways,
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you could produce all the wonderful diversity of the universe.
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Earth and fire, for example,
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give you things that are dry.
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Air and water, things that are wet.
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But as theories go, it had a problem.
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It didn't predict anything that could be measured,
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and measurement is the basis of experimental science.
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Worse still, the theory was wrong.
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But the Greeks were great scientists of the mind
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and in the 5th century B.C.,
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Leucippus of Miletus came up
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with one of the most enduring scientific ideas ever.
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Everything we see is made up
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of tiny, indivisible bits of stuff called atoms.
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This theory is simple and elegant,
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and it has the advantage
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over the earth, air, fire, and water theory
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of being right.
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Centuries of scientific thought and experimentation
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have established that the real elements,
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things like hydrogen,
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carbon,
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and iron,
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can be broken down into atoms.
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In Leucippus's theory, the atom is the smallest,
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indivisible bit of stuff that's still recognizable
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as hydrogen,
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carbon,
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or iron.
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The only thing wrong with Leucippus's idea
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is that atoms are, in fact, divisible.
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Furthermore, his atoms idea turns out
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to explain just a small part
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of what the universe is made of.
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What appears to be the ordinary stuff of the universe
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is, in fact, quite rare.
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Leucippus's atoms, and the things they're made of,
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actually make up only about 5%
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of what we know to be there.
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Physicists know the rest of the universe,
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95% of it,
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as the dark universe,
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made of dark matter and dark energy.
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How do we know this?
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Well, we know because we look at things
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and we see them.
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That might seem rather simplistic,
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but it's actually quite profound.
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All the stuff that's made of atoms is visible.
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Light bounces off it, and we can see it.
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When we look out into space,
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we see stars and galaxies.
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Some of them, like the one we live in,
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are beautiful, spiral shapes, spinning gracefully through space.
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When scientists first measured the motion
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of groups of galaxies in the 1930's
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and weighed the amount of matter they contained,
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they were in for a surprise.
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They found that there's not enough visible stuff
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in those groups to hold them together.
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Later measurements of individual galaxies
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confirmed this puzzling result.
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There's simply not enough visible stuff in galaxies
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to provide enough gravity to hold them together.
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From what we can see,
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they ought to fly apart, but they don't.
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So there must be stuff there
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that we can't see.
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We call that stuff dark matter.
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The best evidence for dark matter today
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comes from measurements of something
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called the cosmic microwave background,
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the afterglow of the Big Bang,
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but that's another story.
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All of the evidence we have
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says that dark matter is there
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and it accounts for much of the stuff
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in those beautiful spiral galaxies
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that fill the heavens.
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So where does that leave us?
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We've long known that the heavens
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do not revolve around us
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and that we're residents of a fairly ordinary planet,
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orbiting a fairly ordinary star,
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in the spiral arm of a fairly ordinary galaxy.
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The discovery of dark matter took us
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one step further away from the center of things.
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It told us that the stuff we're made of
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is only a small fraction of what makes up the universe.
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But there was more to come.
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Early this century,
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scientists studying the outer reaches of the universe
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confirmed that not only is everything moving apart
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from everything else,
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as you would expect in a universe
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that began in hot, dense big bang,
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but that the universe's expansion
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also seems to be accelerating.
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What's that about?
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Either there is some kind of energy
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pushing this acceleration,
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just like you provide energy to accelerate a car,
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or gravity does not behave exactly as we think.
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Most scientists think it's the former,
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that there's some kind of energy driving the acceleration,
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and they called it <i>dark energy</i>.
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Today's best measurements allow us to work out
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just how much of the universe is dark.
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It looks as if dark energy makes up
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about 68% of the universe
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and dark matter about 27%,
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leaving just 5% for us
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and everything else we can actually see.
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So what's the dark stuff made of?
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We don't know,
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but there's one theory, called <i>supersymmetry</i>,
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that could explain some of it.
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Supersymmetry, or SUSY for short,
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predicts a whole range of new particles,
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some of which could make up the dark matter.
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If we found evidence for SUSY,
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we could go from understanding 5% of our universe,
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the things we can actually see,
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to around a third.
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Not bad for a day's work.
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Dark energy would probably be harder to understand,
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but there are some speculative theories out there
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that might point the way.
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Among them are theories that go back
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to that first great idea of the ancient Greeks,
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the idea that we began with several minutes ago,
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the idea that the universe must be simple.
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These theories predict that there is just a single element
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from which all the universe's wonderful diversity stems,
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a vibrating string.
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The idea is that all the particles we know today
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are just different harmonics on the string.
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Unfortunately, string theories today
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are, as yet, untestable.
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But, with so much of the universe waiting to be explored,
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the stakes are high.
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Does all of this make you feel small?
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It shouldn't.
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Instead, you should marvel
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in the fact that, as far as we know,
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you are a member of the only species in the universe
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able even to begin to grasp its wonders,
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and you're living at the right time
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to see our understanding explode.
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