WEBVTT - TechStuff Classic: How LIGO Works

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<v Speaker 1>Welcome to Tech Stuff, a production from iHeartRadio. Hey there,

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<v Speaker 1>and welcome to tech Stuff. I'm your host Jonathan Strickland.

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<v Speaker 1>I'm an executive producer with iHeartRadio and how the tech

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<v Speaker 1>are here. It is time for a classic episode. This

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<v Speaker 1>one is called How Lego Works. Originally published on February

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<v Speaker 1>twenty fourth, twenty sixteen. This was really cool because this

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<v Speaker 1>came out shortly after we were learning about how Lego

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<v Speaker 1>had detected gravitational waves, which up to that point had

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<v Speaker 1>largely been a hypothetical concept. So this was one of

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<v Speaker 1>those things where we finally figured out a way to

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<v Speaker 1>detect something that had been hypothesized about but previously undetected,

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<v Speaker 1>So really cool use of technology. Then the Ligo Observatory

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<v Speaker 1>had picked up a gravitational wave, and this was huge

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<v Speaker 1>news around the world. And in case you were wondering,

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<v Speaker 1>what the heck is this news all about? How did

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<v Speaker 1>they pick up that gravitational wave? What exactly is the

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<v Speaker 1>technology powering our sensors to detect this stuff? How does

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<v Speaker 1>it all work? That's what this episode's all about. So

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<v Speaker 1>this was the very first time anyone had been able

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<v Speaker 1>to measure a gravitational wave directly So today we're going

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<v Speaker 1>to talk all about what that means and how it happened. Now,

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<v Speaker 1>to begin with, we need to lay some groundwork and

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<v Speaker 1>to really get an understanding of what gravitational waves are.

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<v Speaker 1>So gravitational waves ultimately were one of the predictions made

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<v Speaker 1>by a certain Albert Einstein with this theory of general relativity.

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<v Speaker 1>So in that theory, Einstein presented this idea that our

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<v Speaker 1>universe is filled with spacetime. If you're a fan of

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<v Speaker 1>science fiction, you have undoubtedly come across that term star

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<v Speaker 1>trek is all about the spacetime continuum, and that you've

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<v Speaker 1>got to be careful. You could rip a hole in

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<v Speaker 1>the fabric of spacetime. As far as we know, that's

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<v Speaker 1>not really that possible. I mean, black holes could sort

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<v Speaker 1>of be that maybe, But at any rate, spacetime itself

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<v Speaker 1>is this calling it stuff is probably the wrong way

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<v Speaker 1>of putting it, but it is like a fabric and

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<v Speaker 1>mass hangs inside this fabric, And by mass, i'm talking

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<v Speaker 1>about stuff like stars or even an entire solar systems

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<v Speaker 1>or galaxies that hang in this fabric, and just like

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<v Speaker 1>you would see in a two dimensional display, it ends

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<v Speaker 1>up curving the fabric around the mass. We often talk

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<v Speaker 1>about this in terms of a very simple example that's

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<v Speaker 1>easy to imagine. You get some sort of stretching material.

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<v Speaker 1>Often you'll just hear someone say, okay, get a trampoline.

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<v Speaker 1>You've got a trampoline, and you put a big, heavy

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<v Speaker 1>bowling ball on the trampoline. So that bowling ball is

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<v Speaker 1>going to deform the trampoline surface. It's no longer going

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<v Speaker 1>to be straight. It's going to end up curving around

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<v Speaker 1>the bowling ball to some extent, creating kind of a

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<v Speaker 1>dmple where the bowling ball has has created this impression

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<v Speaker 1>inside the trampoline, and as long as the bowling ball

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<v Speaker 1>is there, that impression is going to stay. This is

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<v Speaker 1>sort of the like the way spacetime curves around giant

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<v Speaker 1>masses like stars and black holes things like that. Of course,

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<v Speaker 1>we have to remember that spacetime is actually four dimensional,

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<v Speaker 1>not a two dimensional thing like a trampoline. I mean,

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<v Speaker 1>I know that trampolines technically have three dimensions, but we're

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<v Speaker 1>really looking at a surface, so it's more like a

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<v Speaker 1>two dimensional plane. In reality. In spacetime it's four dimensional

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<v Speaker 1>because you've got the three spatial dimensions plus time, and

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<v Speaker 1>that is a little difficult to get your head around.

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<v Speaker 1>But that's why we tend to look at this two

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<v Speaker 1>dimensional example. It's a lot easier for us to imagine.

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<v Speaker 1>So let's go a little further with that analogy to

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<v Speaker 1>kind of talk about gravity. See Einstein proposed that gravity

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<v Speaker 1>was a manifestation of this curved space time. And if

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<v Speaker 1>we take that trampoline example, Let's say that you have

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<v Speaker 1>a regular trampoline. You haven't put the bowling ball on

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<v Speaker 1>there yet, so it's a nice flat surface, and you

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<v Speaker 1>have a marble, and you roll the marble across the

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<v Speaker 1>surface of the trampoline. So if there's nothing else there,

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<v Speaker 1>and if the trampoline is level, if the surface is level,

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<v Speaker 1>the marble should just roll in the straight line from

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<v Speaker 1>one side of the trampoline to the other, no problem.

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<v Speaker 1>Now let's say you put that big, heavy bowling ball

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<v Speaker 1>on the trampoline. It creates that dimple, and then you

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<v Speaker 1>try and roll the marble across the trampoline surface. Well,

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<v Speaker 1>now that dimple is going to end up affecting the

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<v Speaker 1>pathway of the marble. It's going to start to spiral

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<v Speaker 1>inward toward the bowling ball. Ultimately it'll end up making

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<v Speaker 1>contact with the bowling ball, and Einstein said, that's essentially

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<v Speaker 1>what gravity is. It's that you've got these large masses

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<v Speaker 1>that curves spacetime to the extent that smaller masses are

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<v Speaker 1>spiraling inward toward the large mass. It's just happening on

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<v Speaker 1>a scale that's much much, much larger than any bowling ball,

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<v Speaker 1>marble example. But that this isn't essentially what we see

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<v Speaker 1>when we see planets orbiting a sun, or we see

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<v Speaker 1>a moon orbiting a planet, or we see star systems

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<v Speaker 1>orbiting a galaxy, you know, the center of a galaxy,

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<v Speaker 1>and it's all because of this curve spacetime. Now, all

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<v Speaker 1>of that already is pretty heavy stuff. And keep in mind,

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<v Speaker 1>there was not really any way to directly observe this.

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<v Speaker 1>It was mostly the the just Einstein using logic to

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<v Speaker 1>work all this out and math, logic and math, and

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<v Speaker 1>ultimately it fit with what we saw of the universe.

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<v Speaker 1>But we weren't able to test a lot of this.

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<v Speaker 1>But then it gets even more mind blowing because now

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<v Speaker 1>we have to get to gravitational waves. So Einstein said

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<v Speaker 1>that if a mass were large enough and either changed

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<v Speaker 1>shape rapidly enough or it changed its movement in some way,

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<v Speaker 1>really really quickly. It would cause ripples of space time

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<v Speaker 1>to move outward from that event at the speed of light.

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<v Speaker 1>And those ripples are what we call gravitational waves, which

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<v Speaker 1>are different from gravity waves. By the way, I have

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<v Speaker 1>been known to accidentally say gravity waves instead of gravitational waves,

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<v Speaker 1>but the two are different things. A gravity wave is

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<v Speaker 1>a wave that exists because of gravity. In other words,

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<v Speaker 1>it's a physical wave of some sort of fluid system,

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<v Speaker 1>whether it's atmosphere or water or some other liquid. That's

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<v Speaker 1>a gravity wave on a planet's surface. It's not the

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<v Speaker 1>same thing as a gravitational wave, which is really a

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<v Speaker 1>ripple of space time, and like I said, it moves

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<v Speaker 1>outward from that event at the speed of light. And

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<v Speaker 1>stuff that could cause significant gravitational waves, things that would

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<v Speaker 1>be big enough for us to potentially pick up here

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<v Speaker 1>on Earth if we had the right equipment, would include

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<v Speaker 1>things like two black holes orbiting or colliding with one another,

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<v Speaker 1>which in fact, that was the event that we were

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<v Speaker 1>able to pick up with the Ligo facilities. And I'll

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<v Speaker 1>talk about those in just a bit. But there could

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<v Speaker 1>be other stuff too, like neutron stars orbiting one another

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<v Speaker 1>fast enough would generate gravitational waves, or a supernova explosion

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<v Speaker 1>would create one as well. And each of these events

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<v Speaker 1>give off a huge amount of energy, and some of

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<v Speaker 1>that energy gets converted into making these gravitational waves. So

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<v Speaker 1>one takeaway from this prediction something that Einstein said would happen,

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<v Speaker 1>is that any event that produces gravitational waves is an

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<v Speaker 1>event in which energy is being lost, So you would

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<v Speaker 1>expect to see less energy within that system afterward than before.

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<v Speaker 1>And it would be a hundred years from the time

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<v Speaker 1>of publication of the theory of general relativity to the

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<v Speaker 1>time when scientists announced that they had detected a gravitational

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<v Speaker 1>wave directly. And that's because gravitational waves are devilishly difficult

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<v Speaker 1>to detect. And that's some alliteration for you right there.

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<v Speaker 1>So gravitational waves are invisible. They don't emit any sort

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<v Speaker 1>of electromagnetic radiation, so we can't see them. We can't

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<v Speaker 1>detect them with radio detectors, nothing like that, and that

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<v Speaker 1>makes it pretty tricky to figure out where they are.

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<v Speaker 1>But they do just pass through the universe. They don't

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<v Speaker 1>get absorbed or scattered the way electromagnetic radiation does. If

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<v Speaker 1>you hold up a mirror and light hits the mirror,

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<v Speaker 1>light will bounce off the mirror. That's not the case

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<v Speaker 1>with gravitational waves. They pass right through, so it's a

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<v Speaker 1>very different thing than electromagnetic radiation. And while they're generated

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<v Speaker 1>from enormous events, the gravitational waves aren't very strong. By

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<v Speaker 1>the time they get to Earth. They are pretty weak,

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<v Speaker 1>so weak that you would need an incredibly sensitive tool

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<v Speaker 1>in order to pick them up. And also you have

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<v Speaker 1>to be searching at the right time, because if the

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<v Speaker 1>event that generated the gravitational waves happened a billion years ago,

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<v Speaker 1>but the location is four billion light years from Earth,

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<v Speaker 1>then we would have to wait another three billion years

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<v Speaker 1>for those gravitational waves to get to us, because again,

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<v Speaker 1>they travel at the speed of light. That's their limit.

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<v Speaker 1>So you have to be at the right place at

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<v Speaker 1>the right time to pick these things up, and in

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<v Speaker 1>some cases you might argue that that's incredibly fortuitous. Although

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<v Speaker 1>to be fair, it looks like the events that could

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<v Speaker 1>generate gravitational waves happen pretty frequently throughout the universe. But

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<v Speaker 1>the universe is huge, so if they're happening far away,

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<v Speaker 1>far enough away, will take a very long time for

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<v Speaker 1>that information to get to us. So before the announcement

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<v Speaker 1>on February eleventh, twenty sixteen, scientists had observed phenomena that

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<v Speaker 1>supported the existence of gravitational waves, but were not direct

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<v Speaker 1>observations of a gravitational wave. Here's an example. A pair

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<v Speaker 1>of astronomers in Puerto Rico in the nineteen seventies noticed

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<v Speaker 1>that there was a binary pulsar system and they went

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<v Speaker 1>back to the theory of general relativity because this was

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<v Speaker 1>a sort of system that would be exactly the type

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<v Speaker 1>to generate gravitational waves according to the predictions from general relativity,

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<v Speaker 1>and because general relativity predicted, hey, if it can create

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<v Speaker 1>gravitational waves, it's going to lose energy over time, they

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<v Speaker 1>ended up coming up with the hypothesis that, well, over time,

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<v Speaker 1>this binary pulsar system should start to slow down because

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<v Speaker 1>it's losing energy. It can't keep up at the speed

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<v Speaker 1>it's going. So they decided to keep an eye on it.

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<v Speaker 1>And by keeping an eye on it, I mean they

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<v Speaker 1>continue to observe this pulsar system over the course of

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<v Speaker 1>eight years, and by the end of the eight year period,

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<v Speaker 1>they were comparing the findings they were observing to the

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<v Speaker 1>predictions made by general relativity, and they were matching up.

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<v Speaker 1>It was unfolding exactly the way Einstein predicted it should

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<v Speaker 1>unfold based upon his theory of general relativity, which is

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<v Speaker 1>incredible when you think about it, that the observations are

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<v Speaker 1>matching up so neatly against the predictions. You know, it

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<v Speaker 1>just shows how how keenly aware Einstein was of how

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<v Speaker 1>our universe appears to work. Keeping in mind that general relativity,

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<v Speaker 1>while an amazing idea collection of ideas, really it doesn't

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<v Speaker 1>encompass everything that we know, right. It doesn't really address

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<v Speaker 1>quantum mechanics, for example, at least not in a way

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<v Speaker 1>that incorporates it with classical physics. But based upon what

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<v Speaker 1>it did cover, it seems like it was an incredibly

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<v Speaker 1>accurate theory, all right. So this was really considered strong

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<v Speaker 1>but indirect support of gravitational waves, because again the astronomers

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<v Speaker 1>didn't observe gravitational waves directly. They couldn't see them or

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<v Speaker 1>detect them, but they could see the effects, and again

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<v Speaker 1>it was matching up with the predictions made from general relativity.

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<v Speaker 1>So it was good indirect evidence that gravitational waves existed.

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<v Speaker 1>Then there was an event a couple of years ago

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<v Speaker 1>that you might have heard about when a team of

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<v Speaker 1>researchers working on the BICEP two telescope, which is an

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<v Speaker 1>Antarctica had announced that they thought they might have discovered

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<v Speaker 1>evidence of gravitational waves that supported a hypothesis called cosmic inflation.

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<v Speaker 1>That's a lot of information right there, So let me

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<v Speaker 1>explain what all that means. Cosmic inflation is a hypothesis

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<v Speaker 1>that relates to the Big Bang theory. So, with the

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<v Speaker 1>Big Bang theory, you've got this event in which the

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<v Speaker 1>universe undergoes a period of rapid expansion. Cosmic inflation is

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<v Speaker 1>kind of that rapid expansion on steroids. The idea being that, well,

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<v Speaker 1>when we look at our universe and we look at

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<v Speaker 1>what we can observe, it appears that our observations don't

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<v Speaker 1>quite match up with what we would expect if we

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<v Speaker 1>had just steady expansion since the Big Bang. In other words,

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<v Speaker 1>we look at all the information we have available to us,

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<v Speaker 1>and it looks to us that it doesn't quite match up.

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<v Speaker 1>Something's got to be wrong. Well, one possible explanation is

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<v Speaker 1>that shortly after the Big Bang, and by shortly, I

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<v Speaker 1>mean tend to the negative thirty sixth power seconds after

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<v Speaker 1>the Big Bang, So you take a ten, you put

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<v Speaker 1>a decimal point behind the ten, then you move the

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<v Speaker 1>decimal point to the left thirty six times that you

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<v Speaker 1>put seconds behind that. We're talking a fraction of a

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<v Speaker 1>fraction of a fraction of a second. The universe underwent

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<v Speaker 1>massive expansion, and it only lasted from that point to

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<v Speaker 1>about ten to the negative thirty third power or thirty

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<v Speaker 1>second power seconds. So again an instant. It's completely unimaginable,

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<v Speaker 1>at least for myself, how short an amount of time

0:14:32.000 --> 0:14:37.280
<v Speaker 1>this was. But that's how quickly the universe expanded significantly,

0:14:37.880 --> 0:14:42.200
<v Speaker 1>and then it slowed, but it continued to expand. Now,

0:14:42.360 --> 0:14:46.560
<v Speaker 1>if in fact, cosmic inflation is correct, it solves a

0:14:46.560 --> 0:14:49.360
<v Speaker 1>lot of the problems we have between the what we

0:14:49.440 --> 0:14:52.880
<v Speaker 1>observe today and what we believe happened with the Big Bang,

0:14:53.880 --> 0:14:58.720
<v Speaker 1>and reconciles those differences. If cosmic inflation is wrong, then

0:14:58.800 --> 0:15:02.280
<v Speaker 1>something else that we believe is wrong. Right. It means

0:15:02.320 --> 0:15:06.600
<v Speaker 1>that what we observe either isn't representative of reality somehow

0:15:06.640 --> 0:15:08.920
<v Speaker 1>we're not getting a big enough picture to understand it,

0:15:09.680 --> 0:15:12.400
<v Speaker 1>or that the Big Bang theory itself is flawed in

0:15:12.440 --> 0:15:16.920
<v Speaker 1>some fundamental way. Hey, we'll be back with this heavy

0:15:16.960 --> 0:15:21.120
<v Speaker 1>subject of detecting gravitational waves with LEGO after this short break,

0:15:30.960 --> 0:15:33.800
<v Speaker 1>so the BIS of two team what they were looking

0:15:33.800 --> 0:15:37.360
<v Speaker 1>for was some evidence of gravitational waves that would have

0:15:37.400 --> 0:15:41.200
<v Speaker 1>been generated during the Big Bang. This would end up

0:15:41.240 --> 0:15:44.520
<v Speaker 1>supporting the cosmic inflation hypothesis. And the way they did

0:15:44.600 --> 0:15:47.480
<v Speaker 1>this was they were looking at the cosmic microwave background

0:15:47.640 --> 0:15:52.320
<v Speaker 1>or CMBAM. Now, the cosmic microwave background emerged about three

0:15:52.400 --> 0:15:57.040
<v Speaker 1>hundred eighty thousand years after the Big Bang. This was

0:15:57.080 --> 0:15:59.720
<v Speaker 1>still a period where the universe was so dense that

0:16:00.000 --> 0:16:02.800
<v Speaker 1>I could not pass through it. It was dark and dense,

0:16:03.440 --> 0:16:07.800
<v Speaker 1>but the cosmic microwave background formed around that time, and

0:16:07.880 --> 0:16:14.040
<v Speaker 1>the hypothesis stated, well, gravitational waves would have affected the

0:16:14.160 --> 0:16:19.160
<v Speaker 1>cosmic microwave background, polarizing some of those some of those

0:16:20.000 --> 0:16:24.080
<v Speaker 1>particles really not particles, but some of that energy polarizing

0:16:24.120 --> 0:16:26.760
<v Speaker 1>some of the cosmic microwave background in such a way

0:16:26.800 --> 0:16:30.240
<v Speaker 1>that if you were to observe it, you could see

0:16:30.280 --> 0:16:34.960
<v Speaker 1>the effect of a gravitational wave passing through the cmb

0:16:36.800 --> 0:16:42.400
<v Speaker 1>And then as the universe expand expanded, rather that mark

0:16:42.600 --> 0:16:45.760
<v Speaker 1>would also expand. It's kind of like imagine leaving a

0:16:45.800 --> 0:16:50.200
<v Speaker 1>fingerprint on some sort of stretchy material and then stretching

0:16:50.240 --> 0:16:53.680
<v Speaker 1>that material out, the fingerprint is still there. It's deformed,

0:16:53.720 --> 0:16:56.200
<v Speaker 1>but still there. That's what the BICEP two team was

0:16:56.240 --> 0:16:59.880
<v Speaker 1>looking for, was this pattern in the CMB that would

0:17:00.040 --> 0:17:03.680
<v Speaker 1>indicate that gravitational waves from the Big Bang had passed through,

0:17:04.320 --> 0:17:06.400
<v Speaker 1>and if they found that, that would be a huge

0:17:06.400 --> 0:17:10.359
<v Speaker 1>support for cosmic inflation. And in the spring of twenty fourteen,

0:17:10.359 --> 0:17:13.800
<v Speaker 1>they announced that they believed they had found such evidence,

0:17:14.800 --> 0:17:18.040
<v Speaker 1>and they also invited other researchers to take a look

0:17:18.040 --> 0:17:21.320
<v Speaker 1>at their data and see if it was verifiable or

0:17:21.480 --> 0:17:25.680
<v Speaker 1>maybe they overlooked something. And in the fall of twenty fourteen,

0:17:25.840 --> 0:17:29.040
<v Speaker 1>another team said, we're sorry, but it looks to us

0:17:29.960 --> 0:17:34.159
<v Speaker 1>like space dust might have created a false positive that

0:17:35.080 --> 0:17:38.479
<v Speaker 1>what you thought it was the polarized CMB that you

0:17:38.520 --> 0:17:41.920
<v Speaker 1>had been looking for was actually just space dust that's

0:17:41.960 --> 0:17:47.160
<v Speaker 1>not actually part of the CMB. And so that ended

0:17:47.200 --> 0:17:50.840
<v Speaker 1>up kind of putting a dampener on the whole celebration

0:17:50.920 --> 0:17:54.480
<v Speaker 1>of finding gravitational waves to support cosmic inflation. But even

0:17:54.480 --> 0:17:57.840
<v Speaker 1>if it was completely verified, even if BICEP two had

0:17:58.200 --> 0:18:01.399
<v Speaker 1>irrefutable evidence that they had found the presence of gravitational

0:18:01.400 --> 0:18:07.040
<v Speaker 1>waves through a you know, the way it affected the CMB.

0:18:07.800 --> 0:18:11.560
<v Speaker 1>Even then that's not direct detection. It's still indirect. You're

0:18:11.560 --> 0:18:17.520
<v Speaker 1>looking at the way it's affected something else. So you know,

0:18:17.760 --> 0:18:20.720
<v Speaker 1>again we're still not discovering one. And part of that

0:18:20.800 --> 0:18:23.520
<v Speaker 1>is that BICEP two is a telescope. It's looking at

0:18:23.520 --> 0:18:27.920
<v Speaker 1>through the electromagnetic spectrum, and again, gravitational waves don't show

0:18:28.000 --> 0:18:30.840
<v Speaker 1>up that way. So no telescope would help you find

0:18:30.920 --> 0:18:33.879
<v Speaker 1>a gravitational wave directly. You might be able to find

0:18:34.320 --> 0:18:37.720
<v Speaker 1>how it affected something else, but not the wave itself.

0:18:38.840 --> 0:18:42.040
<v Speaker 1>Now that's not the case with the LIGO observatories. Actually

0:18:42.080 --> 0:18:46.640
<v Speaker 1>it's technically one observatory, but it has four different facilities,

0:18:47.000 --> 0:18:51.800
<v Speaker 1>two detectors and two research facilities that are all part

0:18:51.840 --> 0:18:56.439
<v Speaker 1>of the LIGO observatory. LIGO itself is an acronym and

0:18:56.560 --> 0:19:02.760
<v Speaker 1>it stands for Laser Interferometer Gravitational Wave Observatory. So it's

0:19:02.840 --> 0:19:05.560
<v Speaker 1>a pair of giant detectors built on the surface of

0:19:05.560 --> 0:19:09.320
<v Speaker 1>the Earth. One is located in Hanford, Washington, the other

0:19:09.400 --> 0:19:14.000
<v Speaker 1>is in Livingstone, Louisiana. Now they're about just a little

0:19:14.080 --> 0:19:17.159
<v Speaker 1>under two thousand miles apart, or just over three thousand

0:19:17.240 --> 0:19:20.600
<v Speaker 1>kilometers apart from each other, and that's really important. I'll

0:19:20.600 --> 0:19:23.919
<v Speaker 1>explain why in a little bit. So to understand how

0:19:23.960 --> 0:19:25.680
<v Speaker 1>they work, we also have to talk about something else

0:19:25.720 --> 0:19:30.280
<v Speaker 1>that gravitational waves do as they pass through space. They

0:19:30.359 --> 0:19:35.719
<v Speaker 1>stretch and compress space itself. So again, if you were

0:19:35.920 --> 0:19:38.960
<v Speaker 1>if you were to take a piece of elastic, I'd say,

0:19:38.960 --> 0:19:42.240
<v Speaker 1>you've got a rubber band, a nice thick rubber band,

0:19:43.200 --> 0:19:45.959
<v Speaker 1>and you cut it so that it's just one strip.

0:19:46.800 --> 0:19:49.720
<v Speaker 1>When you pull on that rubber band, it stretches along

0:19:49.960 --> 0:19:53.720
<v Speaker 1>the line where you're applying force, So it stretches in

0:19:53.800 --> 0:19:58.920
<v Speaker 1>that direction, in the perpendicular direction ninety degrees from where

0:19:58.920 --> 0:20:04.040
<v Speaker 1>you're pulling. It compresses, it gets more narrow, and then

0:20:04.080 --> 0:20:07.200
<v Speaker 1>when you let it return to its normal shape, it

0:20:07.320 --> 0:20:10.560
<v Speaker 1>gets you know, the long part ends up getting shorter

0:20:10.720 --> 0:20:13.920
<v Speaker 1>and the narrow part ends up getting wider as a result,

0:20:15.200 --> 0:20:18.560
<v Speaker 1>gravitational waves do this to reality. They do this to

0:20:18.640 --> 0:20:22.760
<v Speaker 1>actual space. They stretch and compress, and it happens several

0:20:22.800 --> 0:20:26.639
<v Speaker 1>times as the wave oscillates through. Really I should just

0:20:26.680 --> 0:20:30.680
<v Speaker 1>say as the wave passes through, rather than oscillates. The

0:20:30.760 --> 0:20:35.200
<v Speaker 1>distortion oscillates, but the wave passes through, so That means

0:20:35.200 --> 0:20:40.359
<v Speaker 1>the actual distance changes between two points as that gravitational

0:20:40.359 --> 0:20:42.679
<v Speaker 1>wave passes through that area. So if we were to

0:20:42.720 --> 0:20:47.520
<v Speaker 1>magnify this effect, and I mean magnify it to a

0:20:47.680 --> 0:20:50.760
<v Speaker 1>ludicrous degree, you would be able to see it. You

0:20:50.760 --> 0:20:53.719
<v Speaker 1>would actually be able to witness this. You could stand

0:20:53.800 --> 0:20:57.040
<v Speaker 1>ten feet away from someone else and when the gravitational

0:20:57.040 --> 0:21:00.280
<v Speaker 1>wave passes through, it would make it look like the

0:21:00.320 --> 0:21:03.040
<v Speaker 1>two of you suddenly got further away and then closer

0:21:03.040 --> 0:21:04.879
<v Speaker 1>to each other, and then further away and closer to

0:21:04.880 --> 0:21:08.280
<v Speaker 1>each other, even though you haven't moved anywhere, because the

0:21:08.320 --> 0:21:14.840
<v Speaker 1>distance itself is stretching and compressing. So why don't we

0:21:14.960 --> 0:21:17.679
<v Speaker 1>see that? I mean, if these celestial events that produce

0:21:17.720 --> 0:21:20.080
<v Speaker 1>gravitational waves happen on the order of something like every

0:21:20.119 --> 0:21:25.520
<v Speaker 1>fifteen minutes, why are we all noticing this whibbly wobbly effect. Well,

0:21:26.200 --> 0:21:30.160
<v Speaker 1>it's because the actual distortion that happens here on Earth

0:21:31.080 --> 0:21:35.920
<v Speaker 1>is much much much smaller in magnitude, so much more

0:21:36.600 --> 0:21:40.359
<v Speaker 1>so much smaller that it's difficult to even explain. But

0:21:40.760 --> 0:21:43.800
<v Speaker 1>if you were to have a supernova explode in the

0:21:43.840 --> 0:21:48.840
<v Speaker 1>Milky Way galaxy, in our galaxy, the gravitational waves generated

0:21:48.880 --> 0:21:53.200
<v Speaker 1>by that explosion would maybe be powerful enough to distort

0:21:53.240 --> 0:21:56.679
<v Speaker 1>the distance between the Earth and the Sun by about

0:21:56.720 --> 0:22:02.480
<v Speaker 1>the diameter of a hydrogen atom, so not noticeable to

0:22:02.560 --> 0:22:06.600
<v Speaker 1>any degree, and not at least to human senses. So

0:22:06.640 --> 0:22:08.320
<v Speaker 1>if you were to even go on a smaller scale,

0:22:08.359 --> 0:22:11.280
<v Speaker 1>let's say that you pick two points that are a

0:22:11.320 --> 0:22:15.360
<v Speaker 1>kilometer apart here on the surface of the Earth, the

0:22:15.400 --> 0:22:18.680
<v Speaker 1>amount of distortion would be equivalent to a few thousandth

0:22:18.880 --> 0:22:22.600
<v Speaker 1>of the diameter of a proton, So you're talking about

0:22:22.600 --> 0:22:26.680
<v Speaker 1>a subatomic particle, and just a tiny, tiny, tiny fraction

0:22:26.840 --> 0:22:30.159
<v Speaker 1>of that subatomic particles diameter would be the amount of

0:22:30.200 --> 0:22:34.040
<v Speaker 1>distortion that would happen across a kilometer worth of distance

0:22:34.080 --> 0:22:38.520
<v Speaker 1>here on Earth. Again, that means it's so small that

0:22:38.720 --> 0:22:42.760
<v Speaker 1>it's incredibly difficult to detect, so much so that Einstein

0:22:42.880 --> 0:22:46.560
<v Speaker 1>himself was pretty sure we would never be able to

0:22:46.640 --> 0:22:50.159
<v Speaker 1>directly detect gravitational waves because he could not imagine a

0:22:50.200 --> 0:22:53.040
<v Speaker 1>system that would be sensitive enough to pick up such

0:22:53.119 --> 0:22:58.640
<v Speaker 1>a minute change, a distortion that's happening so quickly because

0:22:58.680 --> 0:23:01.920
<v Speaker 1>it's a fraction of a second, and it's so small

0:23:02.119 --> 0:23:07.240
<v Speaker 1>as to be unnoticeable. So the other problem here is

0:23:07.280 --> 0:23:10.280
<v Speaker 1>not just that it's such a very tiny effect that

0:23:10.359 --> 0:23:12.919
<v Speaker 1>lasts a short amount of time. It's also that a

0:23:12.920 --> 0:23:16.359
<v Speaker 1>lot of other stuff could create false positives. You can

0:23:16.440 --> 0:23:22.880
<v Speaker 1>have incredibly instrumentation, but if that instrument is really really sensitive,

0:23:23.400 --> 0:23:26.880
<v Speaker 1>any sort of interference could set off and you could

0:23:26.960 --> 0:23:30.680
<v Speaker 1>end up getting false readings. So a change in air

0:23:30.720 --> 0:23:36.720
<v Speaker 1>pressure or temperature, or seismic activity, even a heavy truck

0:23:36.800 --> 0:23:41.000
<v Speaker 1>driving nearby could set off false results. So you'd have

0:23:41.040 --> 0:23:43.720
<v Speaker 1>to come up with a really clever way to measure distortion,

0:23:43.840 --> 0:23:47.760
<v Speaker 1>to limit vibration, and to eliminate the chance that it

0:23:47.800 --> 0:23:50.679
<v Speaker 1>was a false positive. And Lego is the answer to

0:23:50.760 --> 0:23:54.560
<v Speaker 1>all of that. So the Lego Observatory is actually the

0:23:54.600 --> 0:23:59.120
<v Speaker 1>result of decades of collaborative work among different scientific research

0:23:59.160 --> 0:24:03.240
<v Speaker 1>centers and internet national bodies and universities, and all started

0:24:03.280 --> 0:24:06.639
<v Speaker 1>back in nineteen seventy nine. That's when the National Science

0:24:06.680 --> 0:24:10.560
<v Speaker 1>Foundation approved funds for Caltech and MIT to develop laser

0:24:10.560 --> 0:24:14.399
<v Speaker 1>interferometer research and development. And a few years later, in

0:24:14.480 --> 0:24:17.600
<v Speaker 1>nineteen eighty three, Caltech and MIT submitted a proposal for

0:24:17.680 --> 0:24:22.879
<v Speaker 1>a kilometer scale detector. But keep in mind, all right,

0:24:22.920 --> 0:24:25.159
<v Speaker 1>so in nineteen seventy nine you get the funding for

0:24:25.400 --> 0:24:28.879
<v Speaker 1>R and d nineteen eighty three, there's the submission of

0:24:28.880 --> 0:24:33.840
<v Speaker 1>a proposal for a kilometer scale detector. There wouldn't be

0:24:33.880 --> 0:24:38.520
<v Speaker 1>approval for a detector until nineteen ninety, so almost a

0:24:38.680 --> 0:24:44.720
<v Speaker 1>decade later, and which turns out was probably okay, because

0:24:44.720 --> 0:24:50.240
<v Speaker 1>we really didn't have the technological ability to detect things

0:24:50.280 --> 0:24:53.640
<v Speaker 1>on a scale small enough to register a gravitational wave

0:24:53.640 --> 0:24:57.560
<v Speaker 1>in the first place. But still, you know, a decade's

0:24:57.560 --> 0:24:59.920
<v Speaker 1>delay before you even get approval is still pretty rough.

0:25:00.880 --> 0:25:05.920
<v Speaker 1>Construction didn't begin until nineteen ninety four. The inauguration of

0:25:05.960 --> 0:25:10.119
<v Speaker 1>the Ligo Observatory took place in nineteen ninety nine, but

0:25:10.200 --> 0:25:14.320
<v Speaker 1>even then that didn't mean that the observatory was online

0:25:14.359 --> 0:25:17.640
<v Speaker 1>collecting data. It didn't do that until two thousand and two.

0:25:18.800 --> 0:25:23.320
<v Speaker 1>And here's the kicker. Eventually scientists came to the conclusion

0:25:23.440 --> 0:25:27.719
<v Speaker 1>that this Ligo observatory was not sensitive enough to detect

0:25:27.720 --> 0:25:30.600
<v Speaker 1>gravitational waves. That despite the fact that it was this

0:25:31.440 --> 0:25:36.400
<v Speaker 1>large detector or pair of large detectors, actually because again

0:25:36.440 --> 0:25:40.840
<v Speaker 1>one in Louisiana one in Washington, it wasn't sensitive enough

0:25:41.040 --> 0:25:44.919
<v Speaker 1>to be effective. So it was not quite back to

0:25:44.960 --> 0:25:47.600
<v Speaker 1>the drawing board, but it did mean that they had

0:25:47.640 --> 0:25:52.240
<v Speaker 1>to think about how they would upgrade these facilities so

0:25:52.280 --> 0:25:54.439
<v Speaker 1>that they could be sensitive enough to pick up a

0:25:54.440 --> 0:25:58.320
<v Speaker 1>gravitational wave. So in twenty ten, Ligo went offline to

0:25:58.440 --> 0:26:03.399
<v Speaker 1>undergo a big overhaul, and it took four years of

0:26:03.440 --> 0:26:07.480
<v Speaker 1>construction and testing to get it into shape and another

0:26:07.560 --> 0:26:10.760
<v Speaker 1>year to set it up for new observations, which means

0:26:10.760 --> 0:26:13.080
<v Speaker 1>that it wasn't until twenty fifteen that it was ready

0:26:13.119 --> 0:26:16.399
<v Speaker 1>to come back online. By now it was called the

0:26:16.440 --> 0:26:20.880
<v Speaker 1>Advanced Ligo Observatory and it began collecting data in September

0:26:21.040 --> 0:26:27.600
<v Speaker 1>twenty fifteen. Literally days after it had come online, it

0:26:27.640 --> 0:26:31.600
<v Speaker 1>picked up a gravitational wave. So that's pretty phenomenal that

0:26:31.960 --> 0:26:34.639
<v Speaker 1>just a couple of days, just a few days really

0:26:34.680 --> 0:26:37.919
<v Speaker 1>after it had been turned on again in twenty fifteen,

0:26:38.400 --> 0:26:41.800
<v Speaker 1>we got a hit. So that was incredibly exciting. So

0:26:41.840 --> 0:26:45.520
<v Speaker 1>how did this happen? How does it actually work? Well,

0:26:45.520 --> 0:26:48.080
<v Speaker 1>we have to take a look at what interferometers are

0:26:48.119 --> 0:26:53.399
<v Speaker 1>all about. An interferometer uses a technique in which electromagnetic

0:26:53.440 --> 0:26:58.160
<v Speaker 1>waves are superimposed on one another in order to get information. Now,

0:26:58.240 --> 0:27:00.680
<v Speaker 1>Ligo does this with a laser beam because it's a

0:27:00.760 --> 0:27:05.120
<v Speaker 1>laser interferometer, and the laser beam gets shot through a

0:27:05.160 --> 0:27:09.159
<v Speaker 1>beam splitter, and the beams, the two beams that result

0:27:09.240 --> 0:27:13.600
<v Speaker 1>go down two long vacuum tubes. So both of the

0:27:13.720 --> 0:27:17.520
<v Speaker 1>Lego detectors are in an L shape. So you've got

0:27:17.520 --> 0:27:20.560
<v Speaker 1>these long, long vacuum tubes that extend two and a

0:27:20.600 --> 0:27:24.200
<v Speaker 1>half miles or about four kilometers out from the crux

0:27:24.920 --> 0:27:31.160
<v Speaker 1>from the angle where they meet up, and each one

0:27:31.359 --> 0:27:33.479
<v Speaker 1>is you know, they're both the same length. They have

0:27:33.560 --> 0:27:36.840
<v Speaker 1>to be exactly the same length. And the way this

0:27:36.880 --> 0:27:39.760
<v Speaker 1>works is that kind of behind the crux, you've got

0:27:39.800 --> 0:27:42.199
<v Speaker 1>a laser that shoots out a beam of light to

0:27:42.280 --> 0:27:46.080
<v Speaker 1>a beam splitter. The splitter does exactly what it sounds like.

0:27:46.119 --> 0:27:49.520
<v Speaker 1>It does. It splits the beam into two separate beams

0:27:50.320 --> 0:27:56.880
<v Speaker 1>with alternating canceling wavelengths. I guess I should say, so

0:27:56.920 --> 0:28:01.600
<v Speaker 1>the troughs and peaks on one match up with the

0:28:01.800 --> 0:28:05.080
<v Speaker 1>peaks and troughs of the other. That's really important when

0:28:05.640 --> 0:28:08.400
<v Speaker 1>we get a little further down the line here. So

0:28:10.240 --> 0:28:14.320
<v Speaker 1>one of those two beams goes down one branch of

0:28:14.359 --> 0:28:17.960
<v Speaker 1>this L shaped detector. The other beam goes down the

0:28:18.000 --> 0:28:20.680
<v Speaker 1>other branch. And keep in mind, like I said, both

0:28:20.680 --> 0:28:23.159
<v Speaker 1>of these branches are exactly the same length. Two and

0:28:23.200 --> 0:28:26.600
<v Speaker 1>a half miles or four kilometers. When the laser gets

0:28:26.600 --> 0:28:29.760
<v Speaker 1>to the end, they hit a mirror. Each beam hits

0:28:29.760 --> 0:28:33.560
<v Speaker 1>a mirror, they come back to the point of origin,

0:28:34.160 --> 0:28:41.920
<v Speaker 1>and because the two laser beams have these counteracting wavelengths,

0:28:42.360 --> 0:28:46.320
<v Speaker 1>they cancel each other out, so the peaks on one

0:28:46.400 --> 0:28:49.480
<v Speaker 1>cancel out the troughs of the other, and vice versa.

0:28:49.680 --> 0:28:53.200
<v Speaker 1>That means that no light gets emitted through this system.

0:28:53.440 --> 0:28:56.520
<v Speaker 1>And that's important because there's actually a light detector that's

0:28:56.560 --> 0:28:58.800
<v Speaker 1>part of this system as well. It's looking for any

0:28:58.880 --> 0:29:02.320
<v Speaker 1>sign of laser light, because a sign of laser light

0:29:02.360 --> 0:29:06.840
<v Speaker 1>would say that something has changed somehow the distances between

0:29:06.880 --> 0:29:10.240
<v Speaker 1>these or the distances represented by these two vacuum tubes

0:29:10.280 --> 0:29:13.000
<v Speaker 1>has changed, and that would be indicative of an event

0:29:13.040 --> 0:29:17.800
<v Speaker 1>like a gravitational wave moving through. So if any light

0:29:17.840 --> 0:29:23.200
<v Speaker 1>shines through, you know something has happened. Essentially, it says

0:29:23.240 --> 0:29:25.680
<v Speaker 1>that there's a mismatch in the lengths of the vacuum

0:29:25.680 --> 0:29:30.280
<v Speaker 1>tubes themselves. So when a gravitational wave passes through, one

0:29:30.360 --> 0:29:33.960
<v Speaker 1>vacuum tube will get shorter while the other gets longer.

0:29:34.440 --> 0:29:38.680
<v Speaker 1>And that's because the two tubes are offset by ninety degrees,

0:29:39.720 --> 0:29:42.600
<v Speaker 1>so one is going to be along one side of

0:29:42.600 --> 0:29:45.600
<v Speaker 1>the wave and that will lengthen the other will be

0:29:45.640 --> 0:29:49.600
<v Speaker 1>along will be perpendicular to that, and will shorten as

0:29:49.640 --> 0:29:52.800
<v Speaker 1>a result. And this means that the lasers will have

0:29:52.920 --> 0:29:57.400
<v Speaker 1>different distances to travel down, So the laser traveling the

0:29:57.440 --> 0:30:00.680
<v Speaker 1>shorter distance takes less time to get back to the crux.

0:30:01.240 --> 0:30:03.680
<v Speaker 1>The laser going down the longer distance takes more time.

0:30:04.120 --> 0:30:06.360
<v Speaker 1>And even though this is only happening within a fraction

0:30:06.360 --> 0:30:08.640
<v Speaker 1>of a second, it's long enough for us to be

0:30:08.680 --> 0:30:11.400
<v Speaker 1>able to detect the difference. And it also means that

0:30:11.440 --> 0:30:15.040
<v Speaker 1>those wavelengths don't match up anymore, they don't cancel each

0:30:15.040 --> 0:30:17.880
<v Speaker 1>other out anymore. So some of that laser light gets

0:30:17.880 --> 0:30:22.960
<v Speaker 1>emitted to the light detector, which then indicates what's going on.

0:30:23.880 --> 0:30:28.280
<v Speaker 1>It knows which one of the branches was short versus long,

0:30:28.720 --> 0:30:30.760
<v Speaker 1>and knows how long it happened. It knows how much

0:30:30.760 --> 0:30:34.360
<v Speaker 1>it oscillated back and forth, because obviously this is continuing

0:30:34.560 --> 0:30:38.840
<v Speaker 1>as these as the gravitational wave moves through, So you

0:30:38.880 --> 0:30:41.160
<v Speaker 1>collect a lot of data in a short amount of time.

0:30:41.160 --> 0:30:44.160
<v Speaker 1>And we're talking like teeny tiny slices of a second.

0:30:44.200 --> 0:30:47.040
<v Speaker 1>As we're getting all this information, which is pretty incredible.

0:30:48.240 --> 0:30:51.680
<v Speaker 1>We're almost done with our discussion about LEGO, but before

0:30:51.680 --> 0:30:53.320
<v Speaker 1>we can do that, we need to take one more

0:30:53.400 --> 0:31:06.120
<v Speaker 1>quick break. So once you get all that data, you

0:31:06.160 --> 0:31:09.960
<v Speaker 1>can then analyze it. Actually, more importantly, before you analyze it,

0:31:10.000 --> 0:31:13.200
<v Speaker 1>you have to verify it. Now. This is why it's

0:31:13.240 --> 0:31:16.640
<v Speaker 1>important that there are two detectors, and it's also important

0:31:16.640 --> 0:31:19.280
<v Speaker 1>that they are so far apart, like three thousand kilometers

0:31:19.320 --> 0:31:22.120
<v Speaker 1>apart from each other. That's because if you get a

0:31:22.120 --> 0:31:26.160
<v Speaker 1>blip on one of them, if it's a true gravitational wave,

0:31:26.240 --> 0:31:28.440
<v Speaker 1>you should also get a blip on the other one.

0:31:28.840 --> 0:31:31.600
<v Speaker 1>And because gravitational waves move at the speed of light,

0:31:32.160 --> 0:31:35.400
<v Speaker 1>there should be a slight difference in time when both

0:31:35.440 --> 0:31:40.280
<v Speaker 1>detectors pick up on this gravitational wave, somewhere right around

0:31:40.400 --> 0:31:43.680
<v Speaker 1>ten milliseconds or less. In the case of the one

0:31:43.760 --> 0:31:47.840
<v Speaker 1>that was detected back in the fall of twenty fifteen

0:31:47.880 --> 0:31:52.800
<v Speaker 1>but not announced until twenty sixteen, it hit the Louisiana

0:31:52.960 --> 0:31:58.080
<v Speaker 1>detector first, and seven milliseconds later it hit the Washington detector,

0:31:59.000 --> 0:32:02.120
<v Speaker 1>So that is indicative of something like a gravitational wave

0:32:02.160 --> 0:32:04.920
<v Speaker 1>as opposed to some local event that would have caused

0:32:04.960 --> 0:32:07.960
<v Speaker 1>interference and created a false positive. If an earthquake had

0:32:08.000 --> 0:32:13.360
<v Speaker 1>happened in Washington, then the facility may may have picked

0:32:13.400 --> 0:32:16.160
<v Speaker 1>something up, but you wouldn't expect to see it in

0:32:16.200 --> 0:32:20.240
<v Speaker 1>Louisiana because it was a localized event. Same thing is

0:32:20.240 --> 0:32:23.880
<v Speaker 1>true if something had happened in Louisiana. So by seeing

0:32:23.960 --> 0:32:28.040
<v Speaker 1>it happen at both within this ten millisecond timeframe meant

0:32:28.120 --> 0:32:31.720
<v Speaker 1>that it was a very good candidate for a gravitational

0:32:31.760 --> 0:32:36.720
<v Speaker 1>wave passing through. And that's exactly what happened. It was

0:32:36.840 --> 0:32:39.440
<v Speaker 1>a home run in the first ending of the game,

0:32:39.760 --> 0:32:42.360
<v Speaker 1>or even really the first at bat of the game.

0:32:42.400 --> 0:32:45.040
<v Speaker 1>It's like your first player steps up on the first

0:32:45.120 --> 0:32:48.280
<v Speaker 1>day of baseball and knocks a home run and that

0:32:48.440 --> 0:32:52.880
<v Speaker 1>defines the moment the season. Really, that's that's the equivalent

0:32:52.880 --> 0:32:56.920
<v Speaker 1>of what we saw here on a scientific basis. So

0:32:58.800 --> 0:33:01.960
<v Speaker 1>the other thing I want to talk about was how

0:33:02.040 --> 0:33:06.800
<v Speaker 1>LEGO tries to minimize the possibility of detecting a false

0:33:06.840 --> 0:33:09.440
<v Speaker 1>positive in the first place. So, yeah, false positives are

0:33:09.480 --> 0:33:11.720
<v Speaker 1>something that they worry about, and the fact that there

0:33:11.720 --> 0:33:14.760
<v Speaker 1>are two detectors helps minimize that. But even so, you

0:33:14.800 --> 0:33:18.200
<v Speaker 1>want to eliminate the possibility of a false positive so

0:33:18.240 --> 0:33:21.880
<v Speaker 1>that you're not constantly sifting through noise looking for a signal.

0:33:22.720 --> 0:33:24.920
<v Speaker 1>Do you want to minimize noise as much as possible.

0:33:25.800 --> 0:33:30.520
<v Speaker 1>So Lego does this through using combinations of active and

0:33:30.680 --> 0:33:36.920
<v Speaker 1>passive vibration reduction systems. One thing that they do is

0:33:36.920 --> 0:33:40.360
<v Speaker 1>they remove the air from the tubes. That is why

0:33:40.360 --> 0:33:43.960
<v Speaker 1>they're vacuum tubes. They remove the air for two reasons. One,

0:33:44.040 --> 0:33:47.560
<v Speaker 1>they don't want any sound passing through the chambers. Sound

0:33:47.640 --> 0:33:52.760
<v Speaker 1>could possibly interfere with the measurements. Sound would impact the mirrors,

0:33:53.400 --> 0:33:58.040
<v Speaker 1>and even a small impact would be enough to cause

0:33:58.120 --> 0:34:01.360
<v Speaker 1>a problem when you're measuring this laser. For one thing,

0:34:01.520 --> 0:34:04.960
<v Speaker 1>they're looking at distances when they're measuring the changes between

0:34:05.000 --> 0:34:08.560
<v Speaker 1>the two branches. You know, I mentioned that one's getting longer,

0:34:08.600 --> 0:34:12.600
<v Speaker 1>one's getting smaller. The distances they're looking at are very

0:34:12.719 --> 0:34:17.400
<v Speaker 1>very tiny. We're talking ten to the negative nineteenth power meters.

0:34:17.920 --> 0:34:20.080
<v Speaker 1>So again, you take the number ten, you move a

0:34:20.120 --> 0:34:24.280
<v Speaker 1>decimal place nineteen times to the left of that, and

0:34:24.400 --> 0:34:27.400
<v Speaker 1>you put meters at the end. That's the distance that

0:34:27.560 --> 0:34:32.520
<v Speaker 1>these lasers are are measuring the distortion and distance. So

0:34:32.560 --> 0:34:35.080
<v Speaker 1>it's very very very tiny, and something as simple as

0:34:35.120 --> 0:34:38.800
<v Speaker 1>sound could change that. So you can't have any sound

0:34:38.800 --> 0:34:42.000
<v Speaker 1>in these vacuum tubes, you've got to get the air out. Also,

0:34:42.040 --> 0:34:47.960
<v Speaker 1>air can absorb and scatter laser light, which would interfere

0:34:48.000 --> 0:34:50.000
<v Speaker 1>with the experiment as well, so you've got to get

0:34:50.000 --> 0:34:54.440
<v Speaker 1>air out. Now down to the vibration reduction systems. So

0:34:54.480 --> 0:34:57.719
<v Speaker 1>the active isolation system is meant to weed out the

0:34:57.760 --> 0:35:03.040
<v Speaker 1>majority of vibration, and it's active because it is actively

0:35:03.120 --> 0:35:07.719
<v Speaker 1>working against any vibration it encounters. You've got sensors that

0:35:07.880 --> 0:35:14.160
<v Speaker 1>detect vibration, they send commands to force actuators that move

0:35:14.520 --> 0:35:17.480
<v Speaker 1>in opposition to the vibration. So it's kind of like

0:35:17.640 --> 0:35:20.520
<v Speaker 1>noise canceling headphones. If you put on a pair of

0:35:20.560 --> 0:35:23.480
<v Speaker 1>noise canceling headphones, what they're supposed to do is pick

0:35:23.560 --> 0:35:27.080
<v Speaker 1>up any incoming sound and then generate sound waves that

0:35:27.120 --> 0:35:31.120
<v Speaker 1>are in direct opposition of the incoming sound, so that

0:35:31.160 --> 0:35:34.279
<v Speaker 1>you get a cancelation effect. That's the same thing that

0:35:34.360 --> 0:35:36.920
<v Speaker 1>these active systems are trying to do at LIGO, except

0:35:36.960 --> 0:35:39.600
<v Speaker 1>instead of it just being sound, it's really any vibration.

0:35:40.239 --> 0:35:42.479
<v Speaker 1>Although I guess you could argue that any vibration really

0:35:42.560 --> 0:35:46.120
<v Speaker 1>is sound, so it's kind of a moot point. But anyway,

0:35:46.160 --> 0:35:52.080
<v Speaker 1>they're actively trying to counteract that vibration. But then you've

0:35:52.080 --> 0:35:55.000
<v Speaker 1>got the passive system. This is the suspension system for

0:35:55.040 --> 0:35:59.400
<v Speaker 1>the mirrors, and this is the next step. So you've

0:35:59.560 --> 0:36:03.479
<v Speaker 1>eliminated a huge percentage of the vibration at this point,

0:36:03.520 --> 0:36:05.879
<v Speaker 1>but that's not good enough. You need to eliminate as

0:36:06.000 --> 0:36:08.240
<v Speaker 1>much as close to one hundred percent of the vibration

0:36:08.280 --> 0:36:11.880
<v Speaker 1>as you possibly can. So next we look at the

0:36:11.920 --> 0:36:16.160
<v Speaker 1>suspension system of Ligo's mirrors, and they are at the

0:36:16.200 --> 0:36:20.359
<v Speaker 1>base of a four pendulum system. Meaning imagine you've got

0:36:20.360 --> 0:36:24.800
<v Speaker 1>a string and it ends in a pendulum. A weight

0:36:25.000 --> 0:36:27.799
<v Speaker 1>a mass of some sort, and it has to be

0:36:27.840 --> 0:36:32.920
<v Speaker 1>a mass of significant size so that it will it'll

0:36:35.000 --> 0:36:39.359
<v Speaker 1>resist moving. It's the law of inertia. You know, an

0:36:39.360 --> 0:36:43.799
<v Speaker 1>object at rest tends to stay at rest, so it

0:36:43.840 --> 0:36:48.200
<v Speaker 1>will end up absorbing a lot of vibration and minimizing

0:36:48.239 --> 0:36:51.840
<v Speaker 1>it on the other end. So you've got that first pendulum,

0:36:51.920 --> 0:36:55.840
<v Speaker 1>that's pendulum number one. From that you suspend pendulum number two.

0:36:56.400 --> 0:37:00.440
<v Speaker 1>So already you're getting fewer vibrations because pendulum number one

0:37:00.560 --> 0:37:03.520
<v Speaker 1>is picking them up. What vibrations do manage to pass

0:37:03.560 --> 0:37:05.919
<v Speaker 1>through start to get picked up by pendulum number two,

0:37:06.880 --> 0:37:10.279
<v Speaker 1>and again the law of inertia means that it will

0:37:10.360 --> 0:37:12.880
<v Speaker 1>dampen a lot of that vibration. Then you've got pendulum

0:37:13.000 --> 0:37:16.320
<v Speaker 1>number three, and then beneath that you finally have the mirror,

0:37:16.360 --> 0:37:19.719
<v Speaker 1>which is forty kilograms or about eighty eight pounds worth

0:37:19.719 --> 0:37:25.000
<v Speaker 1>of mirror. And hopefully, after the active impassive systems have

0:37:25.120 --> 0:37:27.720
<v Speaker 1>all taken care of the vibration, nothing else is getting

0:37:27.760 --> 0:37:30.399
<v Speaker 1>to that mirror. By the way, you can actually test

0:37:30.440 --> 0:37:35.120
<v Speaker 1>this out yourself, if you like, by getting four strings

0:37:35.160 --> 0:37:38.520
<v Speaker 1>that are all equal length, and some washers, some nice

0:37:38.560 --> 0:37:42.000
<v Speaker 1>heavy washers. Tie a washer at the end of the

0:37:42.080 --> 0:37:47.719
<v Speaker 1>string of the first string. Then tie a washer so

0:37:47.760 --> 0:37:50.839
<v Speaker 1>that one end of the string connects to washer number one,

0:37:51.160 --> 0:37:53.160
<v Speaker 1>one end of the string connects to washer number two,

0:37:53.840 --> 0:37:55.640
<v Speaker 1>and so on and so forth. And if you hold

0:37:55.680 --> 0:37:59.440
<v Speaker 1>it up and you start shaking your hand holding the string,

0:38:00.200 --> 0:38:03.239
<v Speaker 1>notice that the washer at the top moves more than

0:38:03.280 --> 0:38:06.359
<v Speaker 1>the second washer, which moves more than the third, And

0:38:06.400 --> 0:38:08.000
<v Speaker 1>by the time you get down to the fourth one,

0:38:08.200 --> 0:38:10.840
<v Speaker 1>it's not moving much at all because it's been the

0:38:10.960 --> 0:38:14.719
<v Speaker 1>vibrations have been dampened by the previous pendulums. That's the

0:38:14.760 --> 0:38:19.440
<v Speaker 1>principle of this passive system. So that helps eliminate a

0:38:19.440 --> 0:38:23.680
<v Speaker 1>lot of that vibration. Without those dampening systems in place,

0:38:23.719 --> 0:38:26.399
<v Speaker 1>the two LIGO detectors would be picking up a lot

0:38:26.400 --> 0:38:30.239
<v Speaker 1>of noise, and since we're still not really sure how

0:38:30.239 --> 0:38:34.000
<v Speaker 1>often gravitational waves pass through the Earth, that would be

0:38:34.000 --> 0:38:37.360
<v Speaker 1>a problem now. Between two thousand and two and twenty

0:38:37.520 --> 0:38:39.800
<v Speaker 1>and ten, with the early version of LEGO, they didn't

0:38:39.800 --> 0:38:43.880
<v Speaker 1>pick up any gravitational waves at all, which we think

0:38:44.680 --> 0:38:48.960
<v Speaker 1>is because the detectors weren't sensitive enough. We think that's

0:38:48.960 --> 0:38:54.160
<v Speaker 1>the reason, but an alternative reason could be that gravitational

0:38:54.200 --> 0:38:56.799
<v Speaker 1>waves aren't as frequent as we think they are, that

0:38:56.880 --> 0:38:59.719
<v Speaker 1>they don't pass through the Earth as frequently as we

0:39:00.160 --> 0:39:04.400
<v Speaker 1>otherwise believe. However, the opposite could be true. We could

0:39:04.600 --> 0:39:08.960
<v Speaker 1>have way more gravitational waves passing through Earth than we

0:39:09.320 --> 0:39:12.600
<v Speaker 1>had anticipated. Some of them may be so faint that

0:39:12.680 --> 0:39:15.839
<v Speaker 1>even this advanced LIGO system cannot pick it up. There

0:39:15.840 --> 0:39:19.359
<v Speaker 1>are already plans to upgrade LIGO again, and there are

0:39:19.400 --> 0:39:24.560
<v Speaker 1>other LIGO observatory systems that will that are in development

0:39:24.600 --> 0:39:30.440
<v Speaker 1>now that will also listen in for gravitational waves. And

0:39:30.600 --> 0:39:33.000
<v Speaker 1>listen tends to be the way most people refer to it,

0:39:33.080 --> 0:39:39.080
<v Speaker 1>like you're listening for this universal vibration moving through the Earth.

0:39:40.480 --> 0:39:44.360
<v Speaker 1>So because it was only a few days after they

0:39:44.560 --> 0:39:47.520
<v Speaker 1>came online, a lot of people are thinking that gravitational

0:39:47.560 --> 0:39:51.879
<v Speaker 1>waves are probably fairly common. Otherwise, it was just extraordinarily

0:39:51.960 --> 0:39:55.040
<v Speaker 1>lucky that we picked it up just days after the

0:39:55.480 --> 0:39:59.680
<v Speaker 1>observatory was online. Again, the one that we did pick

0:39:59.719 --> 0:40:03.360
<v Speaker 1>up one point three billion light years away, which means

0:40:03.400 --> 0:40:06.000
<v Speaker 1>that the event happened one point three billion years ago.

0:40:06.080 --> 0:40:09.560
<v Speaker 1>That event being two black holes colliding with one another

0:40:09.640 --> 0:40:16.440
<v Speaker 1>to form a solitary black hole mass. In the process,

0:40:16.520 --> 0:40:21.880
<v Speaker 1>it vaporized about three solar masses worth of mass I guess,

0:40:22.800 --> 0:40:26.719
<v Speaker 1>which is a huge amount to think about being converted

0:40:26.760 --> 0:40:30.880
<v Speaker 1>into energy, and the gravitational waves emanated from there at

0:40:30.880 --> 0:40:34.720
<v Speaker 1>the speed of light. So one point three billion years later, Earth,

0:40:34.800 --> 0:40:37.799
<v Speaker 1>which was one point three billion light years away, picked

0:40:37.880 --> 0:40:42.040
<v Speaker 1>them up. So in a way, it was incredibly lucky.

0:40:42.120 --> 0:40:46.480
<v Speaker 1>But if this happens more frequently than we originally believed,

0:40:47.040 --> 0:40:50.080
<v Speaker 1>we might see that this is not an uncommon event.

0:40:50.600 --> 0:40:54.080
<v Speaker 1>It's very possible that there are things we cannot see

0:40:54.160 --> 0:40:59.640
<v Speaker 1>in the universe that create gravitational waves. So in other words,

0:40:59.640 --> 0:41:03.120
<v Speaker 1>it's off that does not give off electromagnetic radiation at all,

0:41:03.719 --> 0:41:06.399
<v Speaker 1>but it does create gravitational waves, meaning that we now

0:41:06.480 --> 0:41:09.520
<v Speaker 1>have the capacity to detect things that otherwise would have

0:41:09.560 --> 0:41:13.120
<v Speaker 1>remained completely undetectable by us. So one of the many

0:41:13.200 --> 0:41:17.480
<v Speaker 1>reasons why this discovery is so exciting, it opens up

0:41:17.719 --> 0:41:21.400
<v Speaker 1>brand new science. It creates a new discipline of science,

0:41:21.400 --> 0:41:25.960
<v Speaker 1>gravitational astronomy, which can really get going now because it's

0:41:26.080 --> 0:41:30.920
<v Speaker 1>not that different from when the telescope was invented. Before

0:41:30.960 --> 0:41:34.359
<v Speaker 1>the telescope, astronomy was pretty limited. You could map out

0:41:34.440 --> 0:41:38.239
<v Speaker 1>astrological bodies when you were way back in the day

0:41:38.280 --> 0:41:41.920
<v Speaker 1>before the science of astronomy had really gotten going. Once

0:41:41.960 --> 0:41:45.360
<v Speaker 1>you started figuring out the difference between mythology and science,

0:41:45.440 --> 0:41:49.600
<v Speaker 1>then astronomy really takes over. You could map out where

0:41:49.600 --> 0:41:52.759
<v Speaker 1>these different bodies go. You could figure out which ones

0:41:52.800 --> 0:41:56.959
<v Speaker 1>are must be planets versus stars, but you couldn't really

0:41:58.040 --> 0:42:01.040
<v Speaker 1>gather a lot more information than that. You could still

0:42:01.080 --> 0:42:04.840
<v Speaker 1>get an impressive amount of data just from observing with

0:42:04.840 --> 0:42:08.600
<v Speaker 1>the naked eye, but the telescope opened up a whole

0:42:08.640 --> 0:42:13.840
<v Speaker 1>new world of study, and this gravitational wave detector system

0:42:13.920 --> 0:42:17.480
<v Speaker 1>has opened up a similar, all new world that was

0:42:17.719 --> 0:42:23.399
<v Speaker 1>not accessible by us until this year really late last year,

0:42:23.480 --> 0:42:27.959
<v Speaker 1>late twenty fifteen, So we might end up discovering things

0:42:28.000 --> 0:42:31.240
<v Speaker 1>that we've never been able to observe before. Will also

0:42:31.560 --> 0:42:34.800
<v Speaker 1>likely be able to study all sorts of cool stuff,

0:42:34.840 --> 0:42:38.040
<v Speaker 1>like how fast is the universe expanding, how much dark

0:42:38.160 --> 0:42:41.680
<v Speaker 1>energy is in our universe. We might learn more about

0:42:41.680 --> 0:42:47.640
<v Speaker 1>black holes already. The gravitational wave detected by LIGO has

0:42:47.719 --> 0:42:52.400
<v Speaker 1>given us the strongest direct evidence of black holes. I

0:42:52.440 --> 0:42:55.360
<v Speaker 1>guess I should say indirect evidence because it's the gravity

0:42:55.400 --> 0:43:00.040
<v Speaker 1>waves generated by the black holes. But not that we

0:43:00.320 --> 0:43:03.360
<v Speaker 1>ever doubted the existence of black holes, but this is

0:43:03.440 --> 0:43:07.920
<v Speaker 1>yet more evidence in support of them. So it's really

0:43:08.280 --> 0:43:11.680
<v Speaker 1>an exciting time. We could end up learning all sorts

0:43:11.680 --> 0:43:14.359
<v Speaker 1>of stuff, stuff that we can't even anticipate right now,

0:43:14.880 --> 0:43:17.880
<v Speaker 1>and that's why it's such a big deal. I also

0:43:17.880 --> 0:43:21.200
<v Speaker 1>think that LEGO is just an incredibly elegant way of

0:43:21.440 --> 0:43:25.080
<v Speaker 1>detecting something that otherwise is impossible for us to see

0:43:25.200 --> 0:43:30.240
<v Speaker 1>or feel or experience, and it's incredibly simple, at least

0:43:30.360 --> 0:43:33.640
<v Speaker 1>on the principle of it. The technology itself is very

0:43:33.640 --> 0:43:36.120
<v Speaker 1>complicated because it has to be so sensitive to detect

0:43:36.160 --> 0:43:41.000
<v Speaker 1>these very tiny changes in distance and time. But the

0:43:41.040 --> 0:43:45.640
<v Speaker 1>principle behind it is elegant, and I mean, you don't

0:43:45.640 --> 0:43:48.120
<v Speaker 1>get much more simple than a ninety degree angle. That's

0:43:48.280 --> 0:43:52.680
<v Speaker 1>pretty bare bones there, but a very clever way of

0:43:52.719 --> 0:43:56.880
<v Speaker 1>detecting something that Einstein believed was going to be beyond

0:43:56.960 --> 0:44:02.600
<v Speaker 1>our ability to ever experience. So now we have a

0:44:02.640 --> 0:44:06.680
<v Speaker 1>revolutionary new way to examine the universe. We have no

0:44:06.719 --> 0:44:09.239
<v Speaker 1>way of knowing what sort of stuff we might learn

0:44:09.400 --> 0:44:13.520
<v Speaker 1>as a result, which is incredibly exciting. And it's all

0:44:13.600 --> 0:44:17.560
<v Speaker 1>due to some lasers, some beam splitters, and some mirrors.

0:44:17.600 --> 0:44:20.800
<v Speaker 1>And since we're already looking at lots of different organizations

0:44:21.239 --> 0:44:27.360
<v Speaker 1>building their own LIGO observatories and also increasing the capacity

0:44:27.480 --> 0:44:32.800
<v Speaker 1>or at least the sensitivity of the current LEGO system,

0:44:33.040 --> 0:44:37.279
<v Speaker 1>who knows what we're going to see next. I hope

0:44:37.320 --> 0:44:41.600
<v Speaker 1>you enjoyed that classic episode on HOWLEGO works way back

0:44:41.640 --> 0:44:44.400
<v Speaker 1>in twenty sixteen. I should definitely do an update on

0:44:44.480 --> 0:44:47.000
<v Speaker 1>that and talk more about the sort of things we've

0:44:47.080 --> 0:44:51.000
<v Speaker 1>learned since the detection of gravitational waves and how that

0:44:51.120 --> 0:44:57.040
<v Speaker 1>has affected science. But if you have suggestions for things

0:44:57.080 --> 0:44:59.439
<v Speaker 1>I should cover in future episodes of tech Stuff, I'd

0:44:59.440 --> 0:45:01.399
<v Speaker 1>love to hear. There are a couple of different ways

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<v Speaker 1>you can do that. You can download the iHeartRadio app.

0:45:04.000 --> 0:45:06.239
<v Speaker 1>It's free to downloads free to us. You can just

0:45:06.360 --> 0:45:08.480
<v Speaker 1>navigate over to tech Stuff. Put tech Stuff in that

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<v Speaker 1>little search field. It'll take it to the podcast page.

0:45:11.280 --> 0:45:13.640
<v Speaker 1>You'll see a little microphone icon. If you click on that,

0:45:13.680 --> 0:45:16.720
<v Speaker 1>you can leave a voice message up thirty seconds in length,

0:45:17.120 --> 0:45:19.680
<v Speaker 1>and I love hearing from y'all, so feel free to

0:45:19.680 --> 0:45:22.680
<v Speaker 1>do that. If you would prefer to send me something

0:45:22.800 --> 0:45:25.959
<v Speaker 1>via text, well, you can go over to Twitter and

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<v Speaker 1>use send a message to the handled text Stuff HSW

0:45:29.920 --> 0:45:32.239
<v Speaker 1>that's our handle, and let me know what it is

0:45:32.280 --> 0:45:34.160
<v Speaker 1>you would like me to do. Cover in future episodes

0:45:34.200 --> 0:45:37.760
<v Speaker 1>of tech Stuff and I'll talk to you again really soon.

0:45:43.760 --> 0:45:48.440
<v Speaker 1>Text Stuff is an iHeartRadio production. For more podcasts from iHeartRadio,

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