WEBVTT - How LIGO Works

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<v Speaker 1>With Technology Stuff. Hey there, and welcome to tex Stuff.

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<v Speaker 1>I'm your host, Jonathan Strickland, and today I wanted to

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<v Speaker 1>talk about something that was in the news recently, at

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<v Speaker 1>least recently when I'm recording this episode. On February eleven, sixteen,

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<v Speaker 1>that was, of course, the day when we got the

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<v Speaker 1>confirmation from a collaboration of scientists that in fact, the

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<v Speaker 1>Ligo Observatory had picked up a gravitational wave. And this

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<v Speaker 1>was huge news around the world. And in case you

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<v Speaker 1>were wondering, what the heck is this news all about?

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<v Speaker 1>How did they pick up that gravitational wave? What what

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<v Speaker 1>exactly is the technology powering our sensors to detect this stuff?

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<v Speaker 1>How does it all work? That's what this episode is

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<v Speaker 1>all about. So this was the very first time anyone

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<v Speaker 1>had been able to measure a gravitational wave directly. So

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<v Speaker 1>today we're gonna talk all about what that means and

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<v Speaker 1>how it happened. Now, to begin with, we need to

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<v Speaker 1>lay some groundwork and to to really get an understanding

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<v Speaker 1>what gravitational waves are. So gravitational waves, ultimately, we're one

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<v Speaker 1>of the predictions made by a certain Albert Einstein with

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<v Speaker 1>his theory of general relativity. So in that theory, Einstein

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<v Speaker 1>presented this idea that our universe is filled with spacetime.

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<v Speaker 1>If you're a fan of science fiction, you have undoubtedly

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<v Speaker 1>come across that term star trek is all about the

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<v Speaker 1>spacetime continuum, and that you've got to be careful. You

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<v Speaker 1>could rip a hole in the fabric of space time.

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<v Speaker 1>As far as we know, that's not really that possible. Um.

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<v Speaker 1>I mean, black holes could sort of be that maybe,

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<v Speaker 1>But at any rate, spacetime itself is this calling it

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<v Speaker 1>stuff is probably the wrong way of putting it, but

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<v Speaker 1>it is like a fabric and mass hangs inside this fabric.

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<v Speaker 1>And by mass, i'm talking about stuff like stars or

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<v Speaker 1>even an entire solar systems or galaxies that hang in

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<v Speaker 1>this fabric, and just like you would see in a

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<v Speaker 1>two dimensional display, Uh, it ends up curving the fabric

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<v Speaker 1>around the mass. Uh. We often talk about this in

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<v Speaker 1>terms of a very simple example that's easy to imagine. Uh.

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<v Speaker 1>You get some sort of stretchy material. Often you'll just

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<v Speaker 1>hear someone say, Okay, get a trampoline. You've got a trampoline,

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<v Speaker 1>and you put a big, heavy bowling ball on the trampoline,

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<v Speaker 1>so that bowling ball is going to deform the trampoline surface.

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<v Speaker 1>It's no longer going to be straight. It's going to

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<v Speaker 1>end up curving around the bowling ball to some extent,

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<v Speaker 1>creating kind of a dimple where the bowling ball has

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<v Speaker 1>has created this impression inside the trampoline, and as long

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<v Speaker 1>as the bowling ball is there, that impression is going

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<v Speaker 1>to stay. This is sort of the like the way

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<v Speaker 1>spacetime curves around giant masses like stars and and black

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<v Speaker 1>holes things like that. Of course, we have to remember

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<v Speaker 1>that spacetime is actually four dimensional, not a two dimensional

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<v Speaker 1>thing like a trampoline. I mean, I know that trampolines

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<v Speaker 1>technically have three dimensions, but we're really looking at a surface,

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<v Speaker 1>so it's more like a two dimensional plane in reality.

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<v Speaker 1>In spacetime it's four dimensional because you've got the three

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<v Speaker 1>spatial dimensions plus time, and that is a little difficult

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<v Speaker 1>to get your head around. But that's why we tend

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<v Speaker 1>to look at this two dimensional example. It's a lot

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<v Speaker 1>easier for us to imagine. So let's go a little

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<v Speaker 1>further with that analogy to kind of talk about gravity. See,

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<v Speaker 1>Einstein proposed that gravity was a manifestation of this curved

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<v Speaker 1>space time. And if we take that trampoline example. Let's

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<v Speaker 1>say that you have a regular trampoline. You haven't put

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<v Speaker 1>the bowling ball on there yet, so it's a nice

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<v Speaker 1>flat surface, and you have a marble, and you roll

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<v Speaker 1>the marble across the surface of the trampoline. So if

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<v Speaker 1>there's nothing else there, and if the trampoline is level,

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<v Speaker 1>if the surfaces level, the marble should just roll in

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<v Speaker 1>the straight line from one side of the trampoline to

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<v Speaker 1>the other. No problem. Now let's say you put that big,

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<v Speaker 1>heavy bowling ball on the trampoline. It creates that dimple,

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<v Speaker 1>and then you try and roll the marble across the

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<v Speaker 1>trampoline surface. Well, now that dimple is going to end

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<v Speaker 1>up affecting the pathway of the marble. It's going to

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<v Speaker 1>start to spiral inward toward the bowling ball. Ultimately it'll

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<v Speaker 1>end up making contact with the bowling ball. And Einstein said,

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<v Speaker 1>that's essentially what gravity is. It's that you've got these

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<v Speaker 1>large masses that curves spacetime to the extent that smaller

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<v Speaker 1>masses are spiraling inward toward the large mass. It's just

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<v Speaker 1>happening on a scale that's much, much, much larger than

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<v Speaker 1>any bowling ball marble example, But that this isn't essentially

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<v Speaker 1>what we see when we see planets orbiting a sun,

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<v Speaker 1>or or we see a moon orbiting a planet, or

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<v Speaker 1>we see star systems orbiting a galaxy, you know, the

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<v Speaker 1>center of a galaxy. And uh, it's all because of

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<v Speaker 1>this curved spacetime. Now, all of that already is pretty

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<v Speaker 1>heavy stuff. And keep in mind, there was not really

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<v Speaker 1>any way to directly observe this. It was mostly the

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<v Speaker 1>the just just Einstein using logic to work all this

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<v Speaker 1>out and math, logic and math, and ultimately it fit

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<v Speaker 1>with what we saw of the universe. But we weren't

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<v Speaker 1>able to test a lot of this. But then it

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<v Speaker 1>gets even more mind blowing because now we have to

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<v Speaker 1>get to gravitational waves. So Einstein said that if a

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<v Speaker 1>mass were large enough and either changed shape rapidly enough,

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<v Speaker 1>or it changed its movement in some way, uh really

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<v Speaker 1>really quickly, it would cause ripples of space time to

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<v Speaker 1>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 or water or some other liquid. Uh.

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<v Speaker 1>That's a gravity wave on a planet's surface. It's not

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<v Speaker 1>the same thing as a gravitational wave, which is really

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<v Speaker 1>a ripple of spacetime, and like I said, it moves

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<v Speaker 1>outward from that event at the speed of light um

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<v Speaker 1>And stuff that could cause significant gravitational waves, things that

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<v Speaker 1>would be big enough for us to potentially pick up

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<v Speaker 1>here on Earth if we had the right equipment, would

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<v Speaker 1>include things like two black holes orbiting or colliding with

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<v Speaker 1>one another, which in fact, that was the event that

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<v Speaker 1>we were able to pick up with the Ligo facilities.

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<v Speaker 1>And I'll talk about those in just a bit. But

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<v Speaker 1>there could be other stuff too, like neutron stars orbiting

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<v Speaker 1>one another fast enough would generate gravitational waves, or a

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<v Speaker 1>supernova explosion would create one as well. And each of

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<v Speaker 1>these events give off a huge amount of energy, and

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<v Speaker 1>some of that energy gets converted into making these gravitational waves.

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<v Speaker 1>So one takeaway from this prediction something that Einstein said

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<v Speaker 1>would happen is that any event that produces gravitational waves

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<v Speaker 1>is an event in which energy is being lost, So

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<v Speaker 1>you would expect to see less energy within that system

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<v Speaker 1>afterward than before. Uh. And it would be a hundred

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<v Speaker 1>years from the time of publication of the theory of

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<v Speaker 1>general relativity to the time when scientists announced that they

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<v Speaker 1>had detected a gravitational wave directly. And that's because gravitational

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<v Speaker 1>waves are devilish lye difficult to detect. And that's some

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<v Speaker 1>alliteration for you right there. So gravitational waves are invisible.

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<v Speaker 1>They don't omit any sort of a electromagnetic radiation, so

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<v Speaker 1>we can't see them. We can't detect them with radio detectors,

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<v Speaker 1>nothing like that. Uh. And that makes it pretty tricky

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<v Speaker 1>to figure out where they are. But they do just

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<v Speaker 1>pass through the universe. They don't get absorbed or scattered

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<v Speaker 1>the way electromagnetic radiation does. If you hold up a

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<v Speaker 1>mirror and light hits the mirror, light will bounce off

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<v Speaker 1>the mirror. That's not the case with gravitational waves. They

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<v Speaker 1>pass right through. UH. So it's a very different thing

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<v Speaker 1>than electromagnetic radiation. UM. And while they're generated from enormous events.

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<v Speaker 1>The gravitational waves aren't very strong by the time they

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<v Speaker 1>get to Earth. They are pretty weak, so weak that

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<v Speaker 1>you would need an incredibly sensitive tool in order to

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<v Speaker 1>pick them up. And also you have to be searching

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<v Speaker 1>at the right time, because if the event that generated

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<v Speaker 1>the gravitational waves happened a billion years ago, but the

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<v Speaker 1>location is four billion light years from Earth, then we

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<v Speaker 1>would have to wait another three billion years for those

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<v Speaker 1>gravitational waves to get to us, because again, they travel

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<v Speaker 1>at the speed of light, that's their limit. So you

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<v Speaker 1>have to be at the right place at the right

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<v Speaker 1>time to pick these things up. And uh, 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, uh, it looks like the events that

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<v Speaker 1>could generate gravitational waves happened pretty frequently throughout the universe.

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<v Speaker 1>But the universe is huge, so if they're happening far away,

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<v Speaker 1>far enough away, it will take a very long time

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<v Speaker 1>for that information to get to us. So before the

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<v Speaker 1>announcement on February eleven, sixteen, scientists had observed phenomena that

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<v Speaker 1>supported the existence of gravitational waves. But we're 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 relative 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 it's losing energy. It can't keep up at the

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<v Speaker 1>speed it's going. So they decided to keep an eye

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<v Speaker 1>on it. And by keeping an eye on it, I

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<v Speaker 1>mean they continued to observe this pulsar system over the

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<v Speaker 1>course of eight years, and by the end of the

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<v Speaker 1>eight year period, they were comparing the findings they were

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<v Speaker 1>observing to the predictions made by general relativity, and they

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<v Speaker 1>were matching up. It was. It was unfolding exactly the

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<v Speaker 1>way Einstein predicted it should unfold based upon his theory

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<v Speaker 1>of general relativity, which is incredible when you think about

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<v Speaker 1>it that the observations are matching up so neatly against

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<v Speaker 1>the predictions. Uh, you know, it just shows how how

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<v Speaker 1>keenly aware Einstein was of how our universe appears to work.

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<v Speaker 1>Keeping in mind that general relativity, while an amazing idea

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<v Speaker 1>collection of ideas, really it doesn't encompass everything that we know,

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<v Speaker 1>right it doesn't. It doesn't really address quantum mechanics, for example,

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<v Speaker 1>at least not in a way that incorporates it with

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<v Speaker 1>classical physics. But based upon what it did cover, it

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<v Speaker 1>seems like it was an incredibly accurate theory alright. So

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<v Speaker 1>this was really considered strong but indirect support of gravitational

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<v Speaker 1>waves because again the astronomers didn't observe gravitational waves directly.

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<v Speaker 1>They couldn't see them or detect them, but they could

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<v Speaker 1>see the effects, and again it was matching up with

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<v Speaker 1>the predictions made from general relativity, so it was good

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<v Speaker 1>it indirect evidence that gravitational waves existed. Then there was

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<v Speaker 1>an event a couple of years ago that you might

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<v Speaker 1>have heard about, when a team of researchers working on

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<v Speaker 1>the BICEP two telescope, which is an an Antarctica, had

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<v Speaker 1>announced that they thought they might have discovered evidence of

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<v Speaker 1>gravitational waves that supported a hypothesis called cosmic inflation. That's

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<v Speaker 1>a lot of information right there, So let me explain

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<v Speaker 1>what all that means. Cosmic inflation is a hypothesis that

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<v Speaker 1>relates to the Big Bang theory. So, with the Big

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<v Speaker 1>Bang theory, you've got this event in which the universe

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<v Speaker 1>undergoes a period of rapid expansion. Cosmic inflation is kind

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<v Speaker 1>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>the the what we can observe, it appears that are

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<v Speaker 1>observed aitions don't quite match up with what we would

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<v Speaker 1>expect if we had, uh, just steady expansion since the

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<v Speaker 1>Big Bang. In other words, we look at all the

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<v Speaker 1>information we have available to us, and it looks to

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<v Speaker 1>us that it doesn't quite match up. Something's got to

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<v Speaker 1>be wrong. Well, one possible explanation is that shortly after

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<v Speaker 1>the Big Bang, and by shortly I mean tend to

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<v Speaker 1>the negative thirty six power seconds after the Big Bang.

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<v Speaker 1>So you take a ten, you put a decimal point

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<v Speaker 1>behind the tin, then you move the decimal point to

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<v Speaker 1>the left thirties six times did you put seconds behind that.

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<v Speaker 1>We're talking a fraction of a fraction of a fraction

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<v Speaker 1>of a second. The universe underwent massive expansion, and it

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<v Speaker 1>only lasted from from that point to about ten to

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<v Speaker 1>the negative thirty third power or thirty second power seconds.

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<v Speaker 1>So again an instant. It's it's completely unimaginable, at least

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<v Speaker 1>for myself, how short an amount of time this was.

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<v Speaker 1>But that's how how quickly the universe expanded, uh significantly,

0:14:10.640 --> 0:14:14.960
<v Speaker 1>and then it slowed, but it continued to expand. Now,

0:14:15.120 --> 0:14:19.240
<v Speaker 1>if in fact cosmic inflation is correct, it solves a

0:14:19.320 --> 0:14:22.080
<v Speaker 1>lot of the problems we have between the what we

0:14:22.160 --> 0:14:25.280
<v Speaker 1>observe today and what we believe happened with the Big

0:14:25.320 --> 0:14:30.880
<v Speaker 1>Bang um and reconciles those differences. If cosmic inflation is wrong,

0:14:31.280 --> 0:14:34.680
<v Speaker 1>then something else that we believe is wrong. Right. It

0:14:34.760 --> 0:14:38.920
<v Speaker 1>means that what we observe either isn't representative of reality

0:14:39.040 --> 0:14:42.320
<v Speaker 1>somehow we're not getting a big enough picture to understand it,

0:14:42.440 --> 0:14:45.120
<v Speaker 1>or that the Big Bang theory itself is flawed in

0:14:45.160 --> 0:14:49.200
<v Speaker 1>some fundamental way. So the BICEP two team, what they

0:14:49.240 --> 0:14:52.920
<v Speaker 1>were looking for was some evidence of gravitational waves that

0:14:52.960 --> 0:14:56.640
<v Speaker 1>would have been generated during the Big Bang this would

0:14:56.760 --> 0:15:00.160
<v Speaker 1>end up supporting the cosmic inflation hypothesis. And the way

0:15:00.200 --> 0:15:02.120
<v Speaker 1>they did this was they were looking at the cosmic

0:15:02.200 --> 0:15:06.880
<v Speaker 1>microwave background or c MB. Now, the cosmic microwave background

0:15:06.920 --> 0:15:12.640
<v Speaker 1>emerged about three hundred eighty thousand years after the Big Bang. Uh.

0:15:12.680 --> 0:15:14.880
<v Speaker 1>This was still a period where the universe was so

0:15:15.000 --> 0:15:17.440
<v Speaker 1>dense that light could not pass through it. It was

0:15:17.600 --> 0:15:21.720
<v Speaker 1>dark and dense, But the cosmic microwave background formed around

0:15:21.760 --> 0:15:28.840
<v Speaker 1>that time, and the hypothesis stated, well, gravitational waves would

0:15:28.920 --> 0:15:34.360
<v Speaker 1>have affected the cosmic microwave background, polarizing some of those uh,

0:15:34.440 --> 0:15:38.120
<v Speaker 1>some of those particles really not particles, but some of

0:15:38.120 --> 0:15:42.080
<v Speaker 1>the energy polarizing some of the cosmic microwave background in

0:15:42.120 --> 0:15:45.280
<v Speaker 1>such a way that if you were to observe it,

0:15:45.360 --> 0:15:49.000
<v Speaker 1>you could see the effect of a gravitational wave passing

0:15:49.080 --> 0:15:54.160
<v Speaker 1>through the CMB. UH. And then as the universe expand

0:15:55.040 --> 0:15:59.600
<v Speaker 1>expanded rather uh, that that mark would also expand. It's

0:15:59.680 --> 0:16:03.600
<v Speaker 1>kind of like imagine leaving a fingerprint on some sort

0:16:03.600 --> 0:16:07.760
<v Speaker 1>of stretchy material and then stretching that material out. The

0:16:07.800 --> 0:16:10.840
<v Speaker 1>fingerprint is still there. It's deformed, but still there. That's

0:16:10.880 --> 0:16:12.920
<v Speaker 1>what the Bicept two team was looking for. Was this

0:16:13.640 --> 0:16:17.880
<v Speaker 1>pattern in the CMB that would indicate that gravitational waves

0:16:17.920 --> 0:16:20.640
<v Speaker 1>from the Big Bang had passed through, and if they

0:16:20.680 --> 0:16:23.680
<v Speaker 1>found that, that would be a huge support for cosmic inflation.

0:16:24.640 --> 0:16:27.600
<v Speaker 1>And in the spring of they announced that they believed

0:16:27.760 --> 0:16:32.680
<v Speaker 1>they had found such evidence, and they also invited other

0:16:32.760 --> 0:16:35.400
<v Speaker 1>researchers to take a look at their data and see

0:16:35.440 --> 0:16:39.920
<v Speaker 1>if it was verifiable or maybe they overlooked something. And

0:16:40.040 --> 0:16:43.920
<v Speaker 1>in the fall often another team said, we're sorry, but

0:16:44.000 --> 0:16:48.680
<v Speaker 1>it looks to us like space dust might have created

0:16:48.680 --> 0:16:52.760
<v Speaker 1>a false positive that what you thought it was the

0:16:53.000 --> 0:16:56.360
<v Speaker 1>polarized CMB that you had been looking for was actually

0:16:56.440 --> 0:16:59.400
<v Speaker 1>just space dust that's not actually part of the CMB.

0:17:00.520 --> 0:17:03.840
<v Speaker 1>And uh so that ended up kind of putting a

0:17:04.760 --> 0:17:08.200
<v Speaker 1>dampener on the whole celebration of finding gravitational waves to

0:17:08.200 --> 0:17:12.240
<v Speaker 1>support cosmic inflation. But even if it was completely verified,

0:17:12.280 --> 0:17:15.640
<v Speaker 1>even if BICEP two had irrefutable evidence that they had

0:17:15.640 --> 0:17:20.560
<v Speaker 1>found the presence of gravitational waves through a uh you know,

0:17:20.920 --> 0:17:24.639
<v Speaker 1>the way it affected the CNB, even then that's not

0:17:24.840 --> 0:17:28.600
<v Speaker 1>direct detection. It's still indirect. You're looking at the way

0:17:28.680 --> 0:17:34.280
<v Speaker 1>it's affected something else. So uh, you know, again, we're

0:17:34.280 --> 0:17:36.720
<v Speaker 1>still not discovering one and and part of that is

0:17:36.760 --> 0:17:39.640
<v Speaker 1>that BICEP two is a telescope. It's looking at through

0:17:40.040 --> 0:17:44.000
<v Speaker 1>the electromagnetic spectrum, and again, gravitational waves don't show up

0:17:44.040 --> 0:17:46.879
<v Speaker 1>that way, So no telescope would help you find a

0:17:46.880 --> 0:17:50.400
<v Speaker 1>gravitational wave directly. You might be able to find how

0:17:50.400 --> 0:17:54.920
<v Speaker 1>it affected something else, but not the wave itself. Now

0:17:54.960 --> 0:17:58.120
<v Speaker 1>that's not the case with the LIGO observatories. Actually it's

0:17:58.160 --> 0:18:03.880
<v Speaker 1>technically one observatory, but it has four different facilities, two detectors,

0:18:04.440 --> 0:18:07.800
<v Speaker 1>UH and to research facilities that are all part of

0:18:07.800 --> 0:18:12.520
<v Speaker 1>the LIGO observatory. LIGO itself is an acronym and it

0:18:12.600 --> 0:18:18.840
<v Speaker 1>stands for Laser Interferometer Gravitational Wave Observatory. So it's a

0:18:18.960 --> 0:18:21.760
<v Speaker 1>pair of giant detectors built on the surface of the Earth.

0:18:21.800 --> 0:18:27.440
<v Speaker 1>One is located in Hanford, Washington, the other is in Livingston, Louisiana.

0:18:27.640 --> 0:18:31.080
<v Speaker 1>Now they're about just a little under two thousand miles

0:18:31.119 --> 0:18:34.680
<v Speaker 1>apart or just over three thousand kilometers apart from each other.

0:18:35.280 --> 0:18:37.760
<v Speaker 1>And that's really important. I'll explain why in a little bit.

0:18:38.920 --> 0:18:40.639
<v Speaker 1>So to understand how they work, we also have to

0:18:40.640 --> 0:18:44.520
<v Speaker 1>talk about something else that gravitational waves do. As they

0:18:44.560 --> 0:18:51.200
<v Speaker 1>pass through space, they stretch and compress space itself. So again,

0:18:51.240 --> 0:18:52.520
<v Speaker 1>if you were to if you were to take a

0:18:52.520 --> 0:18:56.440
<v Speaker 1>piece of elastic, Let's say you've got a rubber band,

0:18:56.840 --> 0:19:00.639
<v Speaker 1>a nice thick rubber band, and you cut it so

0:19:00.720 --> 0:19:03.520
<v Speaker 1>that it's just one strip. When you pull on that

0:19:03.600 --> 0:19:07.760
<v Speaker 1>rubber band, it stretches along the line where you're applying force.

0:19:08.600 --> 0:19:12.480
<v Speaker 1>So it stretches in that direction, in the perpendicular direction

0:19:13.280 --> 0:19:17.560
<v Speaker 1>ninety degrees from where you're pulling. It compresses, it gets

0:19:17.800 --> 0:19:21.480
<v Speaker 1>more narrow, and then when you let it return to

0:19:21.520 --> 0:19:25.000
<v Speaker 1>its normal shape, it gets you know, the the long

0:19:25.119 --> 0:19:28.199
<v Speaker 1>part ends up getting shorter and the narrow part ends

0:19:28.240 --> 0:19:32.320
<v Speaker 1>up getting wider as a result, gravitational waves do this

0:19:32.359 --> 0:19:36.160
<v Speaker 1>to reality. They do this to actual space. They stretch

0:19:36.240 --> 0:19:39.680
<v Speaker 1>and compress, and it happens several times as the wave

0:19:39.720 --> 0:19:43.240
<v Speaker 1>oscillates through. Really, I should just say as the wave

0:19:43.280 --> 0:19:48.199
<v Speaker 1>passes through rather than oscillates. Uh, the distortion oscillates, but

0:19:48.280 --> 0:19:52.040
<v Speaker 1>the wave passes through. So that means the actual distance

0:19:52.240 --> 0:19:57.200
<v Speaker 1>changes between two points as that gravitational wave passes through

0:19:57.200 --> 0:19:59.600
<v Speaker 1>that area. So if we were to magnify this effect,

0:19:59.680 --> 0:20:05.159
<v Speaker 1>and I mean magnify it to a ludicrous degree, you

0:20:05.200 --> 0:20:07.280
<v Speaker 1>would be able to see it. You would actually be

0:20:07.320 --> 0:20:10.520
<v Speaker 1>able to witness this. You could stand ten feet away

0:20:10.560 --> 0:20:14.359
<v Speaker 1>from someone else, and when the gravitational wave passes through,

0:20:14.880 --> 0:20:16.639
<v Speaker 1>it would make it look like the two of you

0:20:16.680 --> 0:20:19.359
<v Speaker 1>suddenly got further away and then closer to each other,

0:20:19.400 --> 0:20:21.320
<v Speaker 1>and then further away and closer to each other, even

0:20:21.320 --> 0:20:25.719
<v Speaker 1>though you haven't moved anywhere, because the distance itself is

0:20:25.760 --> 0:20:31.720
<v Speaker 1>stretching and compressing. So why don't we see that? I mean,

0:20:31.720 --> 0:20:34.760
<v Speaker 1>if the celestial events that produce gravitational waves happen on

0:20:34.800 --> 0:20:37.959
<v Speaker 1>the order of something like every fifteen minutes, why are

0:20:38.040 --> 0:20:42.639
<v Speaker 1>we all noticing this wibbly wobbly effect. Well, it's because

0:20:42.640 --> 0:20:47.520
<v Speaker 1>the actual distortion that happens here on Earth is much

0:20:47.920 --> 0:20:52.880
<v Speaker 1>much much smaller in magnitude, so much more, so much

0:20:52.920 --> 0:20:56.919
<v Speaker 1>smaller that it's difficult to even explain. But if you

0:20:56.960 --> 0:21:00.879
<v Speaker 1>were to have a supernova explode in the Milky Way galaxy,

0:21:01.000 --> 0:21:05.760
<v Speaker 1>in our galaxy, the gravitational waves generated by that explosion

0:21:06.760 --> 0:21:10.080
<v Speaker 1>would maybe be powerful enough to distort the distance between

0:21:10.160 --> 0:21:13.439
<v Speaker 1>the Earth and the Sun by about the diameter of

0:21:13.480 --> 0:21:19.480
<v Speaker 1>a hydrogen atom, so not noticeable to any degree, and

0:21:19.720 --> 0:21:22.879
<v Speaker 1>not at least to human senses. So if you were

0:21:22.920 --> 0:21:24.719
<v Speaker 1>to even go on a smaller scale, Let's say that

0:21:24.760 --> 0:21:28.199
<v Speaker 1>you you pick two points that are a kilometer apart

0:21:28.280 --> 0:21:31.760
<v Speaker 1>here on the surface of the Earth, the amount of

0:21:31.760 --> 0:21:35.080
<v Speaker 1>distortion would be equivalent to a few thousands of the

0:21:35.200 --> 0:21:38.720
<v Speaker 1>diameter of a proton. So you're talking about a sub

0:21:38.760 --> 0:21:42.880
<v Speaker 1>atomic particle, and just a tiny, tiny, tiny fraction of

0:21:42.920 --> 0:21:46.600
<v Speaker 1>that subatomic particles diameter would be the amount of distortion

0:21:46.840 --> 0:21:50.080
<v Speaker 1>that would happen across a kilometer worth of distance here

0:21:50.119 --> 0:21:54.800
<v Speaker 1>on Earth. Again, that means it's so small that it's

0:21:55.280 --> 0:21:59.200
<v Speaker 1>incredibly difficult to detect, so much so that Einstein himself

0:22:00.200 --> 0:22:02.920
<v Speaker 1>was pretty sure we would never be able to directly

0:22:03.000 --> 0:22:06.480
<v Speaker 1>detect gravitational waves because he could not imagine a system

0:22:06.520 --> 0:22:09.560
<v Speaker 1>that would be sensitive enough to pick up such a

0:22:09.640 --> 0:22:14.679
<v Speaker 1>minute change, a distortion that's happening so quickly because it's

0:22:14.720 --> 0:22:18.200
<v Speaker 1>a fraction of a second, and it's so small as

0:22:18.240 --> 0:22:23.280
<v Speaker 1>to be unnoticeable. So the other problem here is not

0:22:23.359 --> 0:22:26.520
<v Speaker 1>just that it's such a very tiny effect that lasts

0:22:26.520 --> 0:22:28.960
<v Speaker 1>a short amount of time. It's also that a lot

0:22:29.000 --> 0:22:32.399
<v Speaker 1>of other stuff could create false positives. You can have

0:22:32.440 --> 0:22:38.760
<v Speaker 1>incredibly sensitive instrumentation, but if that instrument is really really sensitive.

0:22:39.280 --> 0:22:42.760
<v Speaker 1>Any sort of interference could set off and you could

0:22:42.840 --> 0:22:46.560
<v Speaker 1>end up getting false readings. So a change in air

0:22:46.600 --> 0:22:52.600
<v Speaker 1>pressure or temperature, or seismic activity, even a heavy truck

0:22:52.680 --> 0:22:56.879
<v Speaker 1>driving nearby could set off false results. So you'd have

0:22:56.920 --> 0:22:59.600
<v Speaker 1>to come up with a really clever way to measure distortion,

0:22:59.680 --> 0:23:03.600
<v Speaker 1>to limit vibration, and to eliminate the chance that it

0:23:03.680 --> 0:23:06.560
<v Speaker 1>was a false positive. And LEGO is the answer to

0:23:06.640 --> 0:23:10.439
<v Speaker 1>all of that. So the Lego Observatory is actually the

0:23:10.440 --> 0:23:14.959
<v Speaker 1>result of decades of collaborative work among different scientific research

0:23:15.000 --> 0:23:19.280
<v Speaker 1>centers and international bodies and universities, and all started back

0:23:19.320 --> 0:23:23.040
<v Speaker 1>in nineteen seventy nine. That's when the National Science Foundation

0:23:23.080 --> 0:23:25.600
<v Speaker 1>approved funds for cal Tech and m i T to

0:23:25.680 --> 0:23:30.160
<v Speaker 1>develop laser interferometer research and development. And a few years later,

0:23:30.200 --> 0:23:32.760
<v Speaker 1>in nineteen eighty three, Caltech and m i T submitted

0:23:32.760 --> 0:23:38.240
<v Speaker 1>a proposal for a kilometer scale detector. Uh. But keep

0:23:38.240 --> 0:23:40.520
<v Speaker 1>in mind, all right, so nineteen seventy nine you get

0:23:40.520 --> 0:23:44.680
<v Speaker 1>the funding for R and D three, there's the submission

0:23:44.680 --> 0:23:49.640
<v Speaker 1>of a proposal for a kilometer scale detector. There wouldn't

0:23:49.680 --> 0:23:54.240
<v Speaker 1>be approval for a detector until nineteen nine, so almost

0:23:54.320 --> 0:23:59.920
<v Speaker 1>a decade later, and which turns out was probably a

0:24:00.119 --> 0:24:05.280
<v Speaker 1>k because we really didn't have the technological ability to

0:24:05.440 --> 0:24:08.679
<v Speaker 1>detect things on a scale small enough to register a

0:24:08.720 --> 0:24:12.639
<v Speaker 1>gravitational wave in the first place. But but still, you know,

0:24:12.800 --> 0:24:15.280
<v Speaker 1>a decade's delay before you even get approval is still

0:24:15.320 --> 0:24:21.800
<v Speaker 1>pretty rough. Construction didn't begin until nine The inauguration of

0:24:21.840 --> 0:24:26.280
<v Speaker 1>the Ligo Observatory took place in nineteen nine, but even

0:24:26.359 --> 0:24:30.160
<v Speaker 1>then that didn't mean that the the observatory was online

0:24:30.200 --> 0:24:33.560
<v Speaker 1>collecting data. It didn't do that until two thousand two.

0:24:34.720 --> 0:24:39.200
<v Speaker 1>And here's the kicker. Eventually scientists came to the conclusion

0:24:39.320 --> 0:24:43.520
<v Speaker 1>that this Ligo Observatory was not sensitive enough to detect

0:24:43.560 --> 0:24:46.480
<v Speaker 1>gravitational waves. That despite the fact that it was this

0:24:47.320 --> 0:24:52.000
<v Speaker 1>large UH detector or pair of large detectors, actually because

0:24:52.040 --> 0:24:56.280
<v Speaker 1>again one in Louisiana one in Washington, it wasn't sensitive

0:24:56.440 --> 0:25:00.680
<v Speaker 1>enough to be effective. So it was not quite back

0:25:00.720 --> 0:25:03.239
<v Speaker 1>to the drawing board. But it didn't mean that they

0:25:03.280 --> 0:25:07.520
<v Speaker 1>had to think about how they would upgrade these facilities

0:25:07.960 --> 0:25:10.199
<v Speaker 1>so that they could be sensitive enough to pick up

0:25:10.240 --> 0:25:13.879
<v Speaker 1>a gravitational wave. So in twos ten Ligo went offline

0:25:14.080 --> 0:25:19.159
<v Speaker 1>to undergo a big overhaul, and it took four years

0:25:19.200 --> 0:25:22.840
<v Speaker 1>of construction and testing to get it into shape, and

0:25:22.920 --> 0:25:26.359
<v Speaker 1>another year to set it up for new observations, which

0:25:26.400 --> 0:25:28.720
<v Speaker 1>means that it wasn't until twenty fifteen that it was

0:25:28.760 --> 0:25:32.280
<v Speaker 1>ready to come back online. By now it's called the

0:25:32.320 --> 0:25:36.760
<v Speaker 1>Advanced Ligo Observatory, and it began collecting data in September.

0:25:39.119 --> 0:25:44.080
<v Speaker 1>Literally days after it had come online, it picked up

0:25:44.119 --> 0:25:48.159
<v Speaker 1>a gravitational wave. So that's pretty phenomenal that just a

0:25:48.200 --> 0:25:51.199
<v Speaker 1>couple of days, just a few days really after it

0:25:51.240 --> 0:25:54.960
<v Speaker 1>had been turned on again in we got a hit.

0:25:56.080 --> 0:25:58.480
<v Speaker 1>So that was incredibly exciting. So how did this happen?

0:25:58.800 --> 0:26:01.880
<v Speaker 1>How does it actually were? Well we have to take

0:26:01.920 --> 0:26:06.320
<v Speaker 1>a look at what interferometers are all about. An interferometer

0:26:06.520 --> 0:26:11.040
<v Speaker 1>uses a technique in which electromagnetic waves are superimposed on

0:26:11.040 --> 0:26:14.720
<v Speaker 1>one another in order to get information. Now, Ligo does

0:26:14.760 --> 0:26:17.720
<v Speaker 1>this with a laser beam because it's a laser interferometer,

0:26:18.440 --> 0:26:21.880
<v Speaker 1>and the laser beam gets shot through a beam splitter

0:26:22.280 --> 0:26:25.480
<v Speaker 1>and the beams, the two beams that result go down

0:26:25.480 --> 0:26:30.760
<v Speaker 1>too long vacuum tubes, so both of the Lego detectors

0:26:30.800 --> 0:26:34.080
<v Speaker 1>are in an L shape. So you've got these long,

0:26:34.240 --> 0:26:37.240
<v Speaker 1>long vacuum tubes that extend two and a half miles

0:26:37.320 --> 0:26:41.119
<v Speaker 1>or about four kilometers out from the crux from the

0:26:41.400 --> 0:26:47.320
<v Speaker 1>the angle where they meet up, and each one is

0:26:47.600 --> 0:26:49.480
<v Speaker 1>you know, they're both the same length. They have to

0:26:49.520 --> 0:26:53.040
<v Speaker 1>be exactly the same length. And the way this works

0:26:53.080 --> 0:26:55.680
<v Speaker 1>is that, uh, kind of behind the crux, you've got

0:26:55.680 --> 0:26:58.040
<v Speaker 1>a laser that shoots out a beam of light to

0:26:58.160 --> 0:27:01.840
<v Speaker 1>a beam splitter. This letter does exactly what it sounds

0:27:01.880 --> 0:27:04.640
<v Speaker 1>like it does. It splits the beam into two separate

0:27:04.920 --> 0:27:12.560
<v Speaker 1>beams with with alternating canceling wavelengths. I guess I should say,

0:27:12.600 --> 0:27:16.720
<v Speaker 1>so the the troughs and peaks on one match up

0:27:16.960 --> 0:27:20.160
<v Speaker 1>with the peaks and troughs of the other. That's really

0:27:20.200 --> 0:27:24.000
<v Speaker 1>important when we get a little further down the line here.

0:27:24.080 --> 0:27:29.440
<v Speaker 1>So one of those two beams goes down one branch

0:27:29.920 --> 0:27:33.720
<v Speaker 1>of this l shaped detector. The other beam goes down

0:27:33.760 --> 0:27:36.040
<v Speaker 1>the other branch. And keep in mind, like I said,

0:27:36.280 --> 0:27:38.960
<v Speaker 1>both of these branches are exactly the same length two

0:27:39.000 --> 0:27:42.200
<v Speaker 1>and a half miles or four kilometers. When the laser

0:27:42.240 --> 0:27:45.359
<v Speaker 1>gets to the end, they hit a mirror. Each beam

0:27:45.440 --> 0:27:49.440
<v Speaker 1>hits a mirror. They come back to the point of origin.

0:27:50.080 --> 0:27:55.560
<v Speaker 1>And because the two laser beams have these uh, these

0:27:55.600 --> 0:28:01.800
<v Speaker 1>counteracting wavelengths, they cancel each other out, so the peaks

0:28:01.840 --> 0:28:04.239
<v Speaker 1>on one cancel out the troughs of the other, and

0:28:04.359 --> 0:28:08.040
<v Speaker 1>vice versa. That means that no light gets emitted through

0:28:08.400 --> 0:28:11.000
<v Speaker 1>this system. And that's important because there's actually a light

0:28:11.040 --> 0:28:14.159
<v Speaker 1>detector that's part of this system as well. It's looking

0:28:14.200 --> 0:28:17.520
<v Speaker 1>for any sign of laser light, because a sign of

0:28:17.640 --> 0:28:21.280
<v Speaker 1>laser light would say that something has changed somehow the

0:28:21.440 --> 0:28:25.399
<v Speaker 1>distances between these or the distances represented by these two

0:28:25.480 --> 0:28:28.320
<v Speaker 1>vacuum tubes has changed, and that would be indicative of

0:28:28.359 --> 0:28:32.840
<v Speaker 1>an event like a gravitational wave moving through. So if

0:28:32.880 --> 0:28:38.600
<v Speaker 1>any light shines through, you know something has happened. Essentially,

0:28:38.640 --> 0:28:41.000
<v Speaker 1>it says that there's a mismatch in the lengths of

0:28:41.000 --> 0:28:44.920
<v Speaker 1>the vacuum tubes themselves. So when a gravitational wave passes through,

0:28:45.960 --> 0:28:49.760
<v Speaker 1>one vacuum tube will get shorter while the other gets longer.

0:28:50.360 --> 0:28:54.520
<v Speaker 1>And that's because the two tubes are offset by ninety degrees,

0:28:55.640 --> 0:28:58.440
<v Speaker 1>so one is going to be along one side of

0:28:58.480 --> 0:29:01.880
<v Speaker 1>the wave and that lengthen the other will be along

0:29:02.320 --> 0:29:05.480
<v Speaker 1>uh will be perpendicular to that and will shorten as

0:29:05.480 --> 0:29:08.680
<v Speaker 1>a result. And this means that the lasers will have

0:29:08.760 --> 0:29:13.280
<v Speaker 1>different distances to travel down. So the laser traveling the

0:29:13.280 --> 0:29:16.560
<v Speaker 1>shorter distance takes less time to get back to the crux.

0:29:17.120 --> 0:29:19.600
<v Speaker 1>The laser going down the longer distance takes more time.

0:29:20.040 --> 0:29:22.200
<v Speaker 1>And even though this is only happening within a fraction

0:29:22.240 --> 0:29:24.520
<v Speaker 1>of a second, it's long enough for us to be

0:29:24.560 --> 0:29:27.280
<v Speaker 1>able to detect the difference. And it also means that

0:29:27.320 --> 0:29:30.640
<v Speaker 1>those wave lengths don't match up anymore, they don't cancel

0:29:30.720 --> 0:29:33.480
<v Speaker 1>each other out anymore. So some of that laser light

0:29:33.560 --> 0:29:38.360
<v Speaker 1>gets admitted to the light detector, which then indicates what's

0:29:38.400 --> 0:29:42.680
<v Speaker 1>going on. It knows which which one of the branches

0:29:42.880 --> 0:29:46.000
<v Speaker 1>was short versus long, It knows how long it happened,

0:29:46.040 --> 0:29:48.680
<v Speaker 1>It knows how much it oscillated back and forth, because

0:29:48.720 --> 0:29:52.800
<v Speaker 1>obviously this is continuing as these as the gravitational wave

0:29:52.840 --> 0:29:56.080
<v Speaker 1>moves through. So you collect a lot of data in

0:29:56.080 --> 0:29:58.560
<v Speaker 1>a short amount of time. And we're talking like teeny

0:29:58.600 --> 0:30:01.480
<v Speaker 1>tiny slices of a second as we're getting all this information,

0:30:01.720 --> 0:30:06.680
<v Speaker 1>which is pretty incredible. So once you get all that data,

0:30:06.720 --> 0:30:10.080
<v Speaker 1>you can then analyze it. Actually, more importantly, before you

0:30:10.120 --> 0:30:13.360
<v Speaker 1>analyze it, you have to verify it. Now. This is

0:30:13.400 --> 0:30:16.640
<v Speaker 1>why it's important that there are two detectors, and it's

0:30:16.640 --> 0:30:19.120
<v Speaker 1>also important that they are so far apart, like three

0:30:19.120 --> 0:30:22.560
<v Speaker 1>thousand kilometers apart from each other. That's because if you

0:30:22.560 --> 0:30:25.560
<v Speaker 1>get a blip on one of them, if it's a

0:30:25.560 --> 0:30:28.360
<v Speaker 1>true gravitational wave, you should also get a blip on

0:30:28.440 --> 0:30:31.640
<v Speaker 1>the other one. And because gravitational waves move at the

0:30:31.640 --> 0:30:34.520
<v Speaker 1>speed of light, there should be a slight difference in

0:30:34.640 --> 0:30:38.880
<v Speaker 1>time when both detectors pick up on this gravitational wave,

0:30:39.640 --> 0:30:43.840
<v Speaker 1>somewhere right around ten milliseconds or less. In the case

0:30:43.920 --> 0:30:47.240
<v Speaker 1>of the one that was detected back in the fall

0:30:47.360 --> 0:30:50.720
<v Speaker 1>of two thousand fifteen but not announced until two thousand sixteen,

0:30:51.480 --> 0:30:56.480
<v Speaker 1>it hit the Louisiana detector first, and seven milliseconds later

0:30:56.640 --> 0:31:01.400
<v Speaker 1>it hit the Washington detector, So that was indicative of

0:31:01.440 --> 0:31:04.080
<v Speaker 1>something like a gravitational wave, as opposed to some local

0:31:04.200 --> 0:31:07.360
<v Speaker 1>event that would have caused interference and created a false positive.

0:31:07.720 --> 0:31:12.520
<v Speaker 1>If an earthquake had happened in Washington, then the facility

0:31:12.560 --> 0:31:16.040
<v Speaker 1>may have may have picked something up, but you wouldn't

0:31:16.080 --> 0:31:18.920
<v Speaker 1>expect to see it in Louisiana because it was a

0:31:18.960 --> 0:31:21.960
<v Speaker 1>localized event. Same thing is true if something had happened

0:31:22.000 --> 0:31:25.840
<v Speaker 1>in Louisiana. So by seeing it happen at both within

0:31:25.960 --> 0:31:30.080
<v Speaker 1>this ten millisecond time frame meant that it was a

0:31:30.200 --> 0:31:35.000
<v Speaker 1>very good candidate for a gravitational wave passing through. And

0:31:35.040 --> 0:31:38.240
<v Speaker 1>that's exactly what happened. Um it was a home run

0:31:38.600 --> 0:31:41.200
<v Speaker 1>in the first ending of the game, or even really

0:31:41.240 --> 0:31:44.160
<v Speaker 1>the first at bat of the game. It's like your

0:31:44.160 --> 0:31:46.720
<v Speaker 1>first player steps up on the first day of baseball

0:31:46.800 --> 0:31:50.600
<v Speaker 1>and knocks a home run and that defines the moment

0:31:50.720 --> 0:31:53.920
<v Speaker 1>the season. Really, that's that's the equivalent of what we

0:31:53.920 --> 0:32:00.240
<v Speaker 1>saw here on a scientific basis. Uh So the eat.

0:32:01.000 --> 0:32:02.640
<v Speaker 1>The other thing I want to talk about was how

0:32:02.760 --> 0:32:07.520
<v Speaker 1>LEGO tries to minimize the possibility of detecting a false

0:32:07.520 --> 0:32:10.120
<v Speaker 1>positive in the first place. So, yeah, false positives are

0:32:10.160 --> 0:32:12.280
<v Speaker 1>something that that they worry about, and the fact that

0:32:12.320 --> 0:32:15.239
<v Speaker 1>there are two detectors helps minimize that. But even so,

0:32:15.360 --> 0:32:18.160
<v Speaker 1>you want to eliminate the possibility of a false positive

0:32:18.760 --> 0:32:22.040
<v Speaker 1>so that you're not constantly sifting through noise looking for

0:32:22.080 --> 0:32:25.000
<v Speaker 1>a signal. Do you want to minimize noise as much

0:32:25.040 --> 0:32:30.360
<v Speaker 1>as possible. So Lego does this through using combinations of

0:32:30.600 --> 0:32:36.960
<v Speaker 1>active and passive UH vibration reduction systems. One thing that

0:32:37.000 --> 0:32:40.600
<v Speaker 1>they do is they remove the air from the tubes.

0:32:40.640 --> 0:32:42.760
<v Speaker 1>That's why their vacuum tubes they remove the air for

0:32:42.840 --> 0:32:46.880
<v Speaker 1>two reasons. One, they don't want any sound passing through

0:32:46.920 --> 0:32:51.680
<v Speaker 1>the chambers. Sound could possibly interfere with the measurements. Sound

0:32:51.680 --> 0:32:56.080
<v Speaker 1>would impact the mirrors, and even a small impact would

0:32:56.080 --> 0:33:01.000
<v Speaker 1>be enough to cause a problem. When you're measuring this laser.

0:33:01.520 --> 0:33:04.360
<v Speaker 1>For one thing, they're looking at distances when they're measuring

0:33:04.400 --> 0:33:08.240
<v Speaker 1>the changes between the two branches. You know, I mentioned

0:33:08.240 --> 0:33:12.400
<v Speaker 1>that one's getting longer, one's getting smaller. The distances they're

0:33:12.440 --> 0:33:15.160
<v Speaker 1>looking at are very very tiny. We're talking ten to

0:33:15.280 --> 0:33:19.360
<v Speaker 1>the negative nineteenth power meters. So again, you take the

0:33:19.440 --> 0:33:22.880
<v Speaker 1>number ten, you move a decimal place nineteen times to

0:33:22.960 --> 0:33:26.280
<v Speaker 1>the left of that, and you put meters at the end.

0:33:26.600 --> 0:33:30.880
<v Speaker 1>That's the distance that these lasers are are measuring the

0:33:30.920 --> 0:33:34.800
<v Speaker 1>distortion and distance. So it's very very very tiny, and

0:33:34.880 --> 0:33:38.400
<v Speaker 1>something as simple as sound could change that. So you

0:33:38.480 --> 0:33:40.840
<v Speaker 1>can't have any sound in these vacuum tubes. You've got

0:33:40.840 --> 0:33:44.080
<v Speaker 1>to get the air out. Also, air can absorb and

0:33:44.240 --> 0:33:48.800
<v Speaker 1>uh and and scatter laser light, which would interfere with

0:33:48.880 --> 0:33:51.080
<v Speaker 1>the experiment as well. So you've got to get air out.

0:33:52.520 --> 0:33:55.720
<v Speaker 1>Now dawn to the vibration reduction systems. So the active

0:33:55.760 --> 0:33:59.800
<v Speaker 1>isolation system is meant to weed out the majority of vibration.

0:34:00.640 --> 0:34:04.920
<v Speaker 1>And it's active because it is actively working against any

0:34:05.000 --> 0:34:10.879
<v Speaker 1>vibration it encounters. You've got sensors that detect vibration, they

0:34:10.920 --> 0:34:16.279
<v Speaker 1>send commands to force actuators that move in opposition to

0:34:16.360 --> 0:34:19.680
<v Speaker 1>the vibration. So it's kind of like noise canceling headphones.

0:34:19.960 --> 0:34:21.520
<v Speaker 1>If you if you put on a pair of noise

0:34:21.520 --> 0:34:24.359
<v Speaker 1>canceling headphones, what they're supposed to do is pick up

0:34:24.360 --> 0:34:27.960
<v Speaker 1>any incoming sound and then generate sound waves that are

0:34:28.000 --> 0:34:31.920
<v Speaker 1>in direct opposition of the incoming sound, so that you

0:34:31.960 --> 0:34:35.200
<v Speaker 1>get a cancelation effect. That's the same thing that these

0:34:35.239 --> 0:34:38.000
<v Speaker 1>active systems are trying to do at LIGO, except instead

0:34:38.000 --> 0:34:41.240
<v Speaker 1>of it just being sound, it's really any vibration. Although

0:34:41.280 --> 0:34:43.680
<v Speaker 1>I guess you could argue that any vibration really is sound,

0:34:44.080 --> 0:34:47.240
<v Speaker 1>so it's kind of a moot point. But anyway, they're

0:34:47.280 --> 0:34:52.960
<v Speaker 1>actively trying to counteract that vibration. But then you've got

0:34:52.960 --> 0:34:56.320
<v Speaker 1>the passive system. This is the suspension system for the mirrors,

0:34:57.280 --> 0:34:59.680
<v Speaker 1>and this is you know, the next step. So you

0:35:00.000 --> 0:35:04.160
<v Speaker 1>you've eliminated a huge percentage of the vibration at this point,

0:35:04.200 --> 0:35:06.600
<v Speaker 1>but that's not good enough. You need to eliminate as

0:35:06.680 --> 0:35:09.919
<v Speaker 1>much as close to the vibration as you possibly can.

0:35:11.080 --> 0:35:15.640
<v Speaker 1>So next we look at the suspension system of ligos mirrors,

0:35:15.760 --> 0:35:19.760
<v Speaker 1>and they are at the base of a four pendulum system.

0:35:19.880 --> 0:35:23.920
<v Speaker 1>Meaning imagine you've got a string and it ends in

0:35:24.000 --> 0:35:27.200
<v Speaker 1>a in a pendulum, a weight a mass of some sort,

0:35:27.840 --> 0:35:30.600
<v Speaker 1>and it has to be a mass of significant size

0:35:31.320 --> 0:35:37.040
<v Speaker 1>so that it will it'll um resist moving. It's the

0:35:37.120 --> 0:35:40.960
<v Speaker 1>law of inertia, you know. Uh. An object at rest

0:35:41.160 --> 0:35:45.440
<v Speaker 1>tends to stay at rest, so it will end up

0:35:45.480 --> 0:35:49.520
<v Speaker 1>absorbing a lot of vibration and minimizing it on the

0:35:49.560 --> 0:35:53.240
<v Speaker 1>other end. So you've got that first pendulum, that's pendulum

0:35:53.320 --> 0:35:57.200
<v Speaker 1>number one. From that you suspend pendulum number two. So

0:35:57.320 --> 0:36:01.239
<v Speaker 1>already you're getting fewer vibrations because pendulum number one is

0:36:01.280 --> 0:36:04.439
<v Speaker 1>picking them up. What vibrations do manage to pass through

0:36:04.560 --> 0:36:07.680
<v Speaker 1>start to get picked up by pendulum number two, and

0:36:07.719 --> 0:36:11.400
<v Speaker 1>again the law of inertia means that it will dampen

0:36:11.440 --> 0:36:14.520
<v Speaker 1>a lot of that vibration. Then you've got pendulum number three,

0:36:14.960 --> 0:36:17.279
<v Speaker 1>and then beneath that you finally have the mirror, which

0:36:17.360 --> 0:36:22.080
<v Speaker 1>is forts or about eighty eight pounds worth of mirror. Uh.

0:36:22.120 --> 0:36:26.320
<v Speaker 1>And hopefully after the active impassive systems have all taken

0:36:26.320 --> 0:36:29.160
<v Speaker 1>care of the vibration, nothing else is getting to that mirror.

0:36:29.719 --> 0:36:32.080
<v Speaker 1>By the way, you can actually test this out yourself,

0:36:32.120 --> 0:36:36.160
<v Speaker 1>if you like, by UH, getting four strings that are

0:36:36.440 --> 0:36:40.080
<v Speaker 1>all equal length and some washers, some nice heavy washers.

0:36:40.680 --> 0:36:43.440
<v Speaker 1>Tie a washer at the end of the string of

0:36:43.520 --> 0:36:48.560
<v Speaker 1>the first string. Then tie a washer um so that

0:36:49.040 --> 0:36:51.480
<v Speaker 1>one end of the string connects to washer number one,

0:36:51.840 --> 0:36:53.919
<v Speaker 1>one end of the string connects to washer number two,

0:36:54.600 --> 0:36:56.359
<v Speaker 1>and so on and so forth. And if you hold

0:36:56.360 --> 0:37:00.120
<v Speaker 1>it up and you start shaking your hand holding the stringing,

0:37:00.520 --> 0:37:03.719
<v Speaker 1>you'll notice that the washer at the top moves more

0:37:03.800 --> 0:37:06.600
<v Speaker 1>than the second washer, which moves more than the third,

0:37:06.960 --> 0:37:08.680
<v Speaker 1>And by the time you get down to the fourth one,

0:37:08.920 --> 0:37:11.560
<v Speaker 1>it's not moving much at all because it's been the

0:37:11.640 --> 0:37:15.400
<v Speaker 1>vibrations have been dampened by the previous pendulums. That's the

0:37:15.440 --> 0:37:20.120
<v Speaker 1>principle of this passive system. So that helps eliminate a

0:37:20.120 --> 0:37:24.360
<v Speaker 1>lot of that vibration. UH. Without those dampening systems in place,

0:37:24.440 --> 0:37:27.080
<v Speaker 1>the two ligo detectors would be picking up a lot

0:37:27.080 --> 0:37:30.920
<v Speaker 1>of noise. And since we're still not really sure how

0:37:30.960 --> 0:37:34.640
<v Speaker 1>often gravitational waves passed through the Earth, that would be

0:37:34.719 --> 0:37:38.240
<v Speaker 1>a problem. Now. Between two thousand two and two thousand

0:37:38.200 --> 0:37:40.439
<v Speaker 1>and ten, with the early version of LEGO, they didn't

0:37:40.480 --> 0:37:44.560
<v Speaker 1>pick up any gravitational waves at all, which we think

0:37:45.360 --> 0:37:49.640
<v Speaker 1>is because the detectors weren't sensitive enough. We think that's

0:37:49.680 --> 0:37:54.879
<v Speaker 1>the reason, but an alternative reason could be that gravitational

0:37:54.880 --> 0:37:57.480
<v Speaker 1>waves aren't as frequent as we think they are, that

0:37:57.560 --> 0:38:00.520
<v Speaker 1>they don't pass through the Earth as frequently as we

0:38:00.600 --> 0:38:04.759
<v Speaker 1>might otherwise believe. However, the opposite could be true. We

0:38:04.800 --> 0:38:09.000
<v Speaker 1>could have way more gravitational waves passing through Earth than

0:38:09.360 --> 0:38:13.040
<v Speaker 1>we had anticipated. Some of them may be so faint

0:38:13.120 --> 0:38:16.120
<v Speaker 1>that even this advanced LIGO system cannot pick it up.

0:38:16.360 --> 0:38:19.920
<v Speaker 1>There are already plans to upgrade LIGO again, and there

0:38:19.920 --> 0:38:24.640
<v Speaker 1>are other LIGO observatory systems that will that are in

0:38:24.719 --> 0:38:31.200
<v Speaker 1>development now that will also listening for gravitational waves. And

0:38:31.280 --> 0:38:33.680
<v Speaker 1>listen tends to be the way most people refer to it,

0:38:33.760 --> 0:38:41.439
<v Speaker 1>like you're listening for this universal vibration moving through the Earth. So,

0:38:41.960 --> 0:38:45.880
<v Speaker 1>because it was only a few days after they came online,

0:38:45.920 --> 0:38:48.680
<v Speaker 1>a lot of people are thinking that gravitational waves are

0:38:48.680 --> 0:38:53.120
<v Speaker 1>probably fairly common. Otherwise, it was just extraordinarily lucky that

0:38:53.160 --> 0:38:57.160
<v Speaker 1>we picked it up just days after the observatory was

0:38:57.520 --> 0:39:00.759
<v Speaker 1>online again. The one that we did pick up was

0:39:00.800 --> 0:39:04.200
<v Speaker 1>one point three billion light years away, which means that

0:39:04.239 --> 0:39:06.840
<v Speaker 1>the event happened one point three billion years ago. That

0:39:06.920 --> 0:39:10.400
<v Speaker 1>event being two black holes colliding with one another to

0:39:10.520 --> 0:39:16.400
<v Speaker 1>form a solitary black hole mass in the UH. In

0:39:16.480 --> 0:39:21.400
<v Speaker 1>the process, it vaporized about three solar masses worth of

0:39:21.400 --> 0:39:25.680
<v Speaker 1>of mass I guess, which is a huge amount to

0:39:25.719 --> 0:39:30.200
<v Speaker 1>think about being converted into energy, and the gravitational waves

0:39:30.560 --> 0:39:32.560
<v Speaker 1>emanated from there at the speed of light. So one

0:39:32.560 --> 0:39:36.319
<v Speaker 1>point three billion years later, Earth, which was one point

0:39:36.320 --> 0:39:40.239
<v Speaker 1>three billion light years away, picked him up. So in

0:39:40.239 --> 0:39:44.240
<v Speaker 1>a way, it was incredibly lucky. But if this happens

0:39:44.280 --> 0:39:48.640
<v Speaker 1>more frequently than we we originally believed, we might see

0:39:48.800 --> 0:39:52.360
<v Speaker 1>that this is not an uncommon event. It's very possible

0:39:52.400 --> 0:39:55.680
<v Speaker 1>that there are things we cannot see in the universe

0:39:56.440 --> 0:40:00.960
<v Speaker 1>that create gravitational waves. So the words, it's stuff that

0:40:01.040 --> 0:40:04.680
<v Speaker 1>does not give off electromagnetic radiation at all, but it

0:40:04.760 --> 0:40:07.520
<v Speaker 1>does create gravitational waves, meaning that we now have the

0:40:07.560 --> 0:40:11.279
<v Speaker 1>capacity to detect things that otherwise would have remained completely

0:40:11.320 --> 0:40:14.800
<v Speaker 1>undetectable by us. So one of the many reasons why

0:40:14.920 --> 0:40:19.640
<v Speaker 1>this discovery is so exciting. It opens up brand new science.

0:40:19.800 --> 0:40:24.359
<v Speaker 1>It creates a new discipline of science, gravitational astronomy, which

0:40:24.400 --> 0:40:27.920
<v Speaker 1>can really get going now because it's not that different

0:40:28.040 --> 0:40:33.040
<v Speaker 1>from when the telescope was invented. Before the telescope, astronomy

0:40:33.160 --> 0:40:37.399
<v Speaker 1>was pretty limited. You could map out astrological bodies when

0:40:37.440 --> 0:40:39.800
<v Speaker 1>you were way back in the day, before the science

0:40:39.800 --> 0:40:43.520
<v Speaker 1>of astronomy had really gotten going. Once you started figuring

0:40:43.520 --> 0:40:47.520
<v Speaker 1>out the difference between mythology and science, then astronomy really

0:40:47.520 --> 0:40:51.480
<v Speaker 1>takes over. You could map out where these different bodies go.

0:40:51.920 --> 0:40:54.520
<v Speaker 1>You could figure out which ones are must be planets

0:40:54.600 --> 0:40:59.759
<v Speaker 1>versus stars, but you couldn't really gather a lot more

0:40:59.760 --> 0:41:02.360
<v Speaker 1>in a nation than that. You can still get an

0:41:02.400 --> 0:41:06.239
<v Speaker 1>impressive amount of data just from observing with the naked eye,

0:41:07.000 --> 0:41:11.160
<v Speaker 1>but the telescope opened up a whole new world of study,

0:41:11.440 --> 0:41:15.960
<v Speaker 1>and this gravitational wave detector system has opened up a similar,

0:41:16.200 --> 0:41:21.240
<v Speaker 1>all new world that was not accessible by us until

0:41:21.719 --> 0:41:27.120
<v Speaker 1>this year real really late, last year late. So we

0:41:27.200 --> 0:41:29.640
<v Speaker 1>might end up discovering things that we've never been able

0:41:29.680 --> 0:41:33.960
<v Speaker 1>to observe before. Will also likely be able to study

0:41:34.080 --> 0:41:36.880
<v Speaker 1>all sorts of cool stuff like how fast is the universe,

0:41:36.920 --> 0:41:41.319
<v Speaker 1>expanding how much dark energy is in our universe, we

0:41:41.400 --> 0:41:45.600
<v Speaker 1>might learn more about black holes already. The gravitational wave

0:41:45.680 --> 0:41:49.640
<v Speaker 1>detected by the by ligo has given us the strongest

0:41:49.760 --> 0:41:53.680
<v Speaker 1>direct evidence of black holes. Um, I guess I should

0:41:53.719 --> 0:41:56.960
<v Speaker 1>say indirect evidence, because it's the gravity waves generated by

0:41:56.960 --> 0:42:02.239
<v Speaker 1>the black holes. But not that we ever doubted the

0:42:02.280 --> 0:42:04.880
<v Speaker 1>existence of black holes, but this is yet more evidence

0:42:04.920 --> 0:42:09.960
<v Speaker 1>in support of them. So it's really an exciting time.

0:42:10.440 --> 0:42:13.280
<v Speaker 1>We could end up learning all sorts of stuff, stuff

0:42:13.280 --> 0:42:16.160
<v Speaker 1>that we can't even anticipate right now, and that's why

0:42:16.239 --> 0:42:19.240
<v Speaker 1>it's such a big deal. I also think that Lego

0:42:19.360 --> 0:42:23.080
<v Speaker 1>is just an incredibly elegant way of detecting something that

0:42:23.120 --> 0:42:27.160
<v Speaker 1>otherwise is impossible for us to see or feel or experience.

0:42:28.280 --> 0:42:32.640
<v Speaker 1>And it's incredibly simple, at least on the principle of it.

0:42:32.960 --> 0:42:35.400
<v Speaker 1>The technology itself is very complicated because it has to

0:42:35.400 --> 0:42:38.680
<v Speaker 1>be so sensitive to detect these very tiny changes in

0:42:38.760 --> 0:42:44.960
<v Speaker 1>distance and time, but the principle behind it is elegant,

0:42:45.320 --> 0:42:47.359
<v Speaker 1>and I mean, you don't get much more simple than

0:42:47.400 --> 0:42:51.719
<v Speaker 1>a ninety degree angle. That's pretty bare bones there, but

0:42:51.880 --> 0:42:56.400
<v Speaker 1>a very clever way of detecting something that Einstein believed

0:42:56.520 --> 0:43:00.440
<v Speaker 1>was going to be beyond our ability to ever experience.

0:43:01.360 --> 0:43:05.640
<v Speaker 1>So now we have a revolutionary new way to examine

0:43:05.640 --> 0:43:08.600
<v Speaker 1>the universe. We have no way of knowing what sort

0:43:08.600 --> 0:43:11.040
<v Speaker 1>of stuff we might learn as a result, which is

0:43:11.040 --> 0:43:15.960
<v Speaker 1>incredibly exciting. And it's all due to some lasers, some

0:43:16.040 --> 0:43:19.680
<v Speaker 1>beam splitters, and some mirrors. And since we're already looking

0:43:19.719 --> 0:43:24.360
<v Speaker 1>at lots of different organizations building their own ligo observatories

0:43:24.440 --> 0:43:29.440
<v Speaker 1>and also increasing the capacity or at least the sensitivity

0:43:29.560 --> 0:43:35.279
<v Speaker 1>of the current ligo system, who knows what we're going

0:43:35.320 --> 0:43:39.560
<v Speaker 1>to see next. I'm so excited about this stuff. But guys,

0:43:39.760 --> 0:43:42.440
<v Speaker 1>I want to hear from you what you want to

0:43:42.960 --> 0:43:45.319
<v Speaker 1>you know, hear more about on future episodes of tech Stuff.

0:43:45.320 --> 0:43:48.359
<v Speaker 1>I've got a couple of things in the hopper. I've

0:43:48.400 --> 0:43:51.200
<v Speaker 1>got a couple of special guests that lined up for

0:43:51.280 --> 0:43:53.440
<v Speaker 1>the near future, so you should be getting some pretty

0:43:53.440 --> 0:43:57.640
<v Speaker 1>cool episodes pretty soon. And I also want to examine

0:43:57.800 --> 0:44:00.400
<v Speaker 1>UH one topic. I'm probably gonna try and get one

0:44:00.400 --> 0:44:01.960
<v Speaker 1>of the stuff they don't want you to know. Guys

0:44:01.960 --> 0:44:05.640
<v Speaker 1>to come in here with me to talk about back

0:44:05.719 --> 0:44:11.399
<v Speaker 1>door UH access to things like encryption systems and why

0:44:11.480 --> 0:44:13.720
<v Speaker 1>was that such a big deal and why did Apple

0:44:13.840 --> 0:44:16.239
<v Speaker 1>respond the way it did and why should we be

0:44:16.280 --> 0:44:20.440
<v Speaker 1>happy about it? Because I think that's a really important

0:44:20.480 --> 0:44:23.120
<v Speaker 1>topic and uh, I would love to get them on

0:44:23.239 --> 0:44:24.520
<v Speaker 1>the show, or at least one of them on the

0:44:24.520 --> 0:44:26.960
<v Speaker 1>show to kind of talk about it, So keep an

0:44:26.960 --> 0:44:29.359
<v Speaker 1>ear out for that as well. If you have any

0:44:29.360 --> 0:44:32.560
<v Speaker 1>suggestions for future topics, please get in touch with me

0:44:32.680 --> 0:44:35.040
<v Speaker 1>let me know what you would like to hear. The

0:44:35.200 --> 0:44:38.080
<v Speaker 1>email address for this show is tech stuff at how

0:44:38.160 --> 0:44:40.680
<v Speaker 1>stuff works dot com, or you can drop me along

0:44:40.800 --> 0:44:43.200
<v Speaker 1>on Twitter or Facebook. The handle it both of those

0:44:43.280 --> 0:44:46.520
<v Speaker 1>is text stuff H s W and I will talk

0:44:46.520 --> 0:44:56.360
<v Speaker 1>to you again really soon for more on this and

0:44:56.400 --> 0:45:02.880
<v Speaker 1>bothands of other topics how stuff works dot com, wh

0:45:03.760 --> 0:45:05.040
<v Speaker 1>wh whon