WEBVTT - Detecting Gravitational Waves

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<v Speaker 1>Brought to you by Toyota. Let's go places. Welcome to

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<v Speaker 1>Forward Thinking. Hey there, and welcome to Forward Thinking, the

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<v Speaker 1>podcast that looks at the future and says white about

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<v Speaker 1>I'm Jonathan Strickland, I'm Lauren voc Obama, and I'm Joe McCormick.

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<v Speaker 1>And today, you guys aren't going to be able to

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<v Speaker 1>depend on me to be my normal plucky self because

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<v Speaker 1>I've got kind of a bad cold. So I'm sorry

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<v Speaker 1>that I'm even talking in your general direction right now,

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<v Speaker 1>but I suppose the show must go on. Well yeah,

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<v Speaker 1>and Joe, it's it's kind of it's kind of fitting

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<v Speaker 1>that that you are a little out of play here,

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<v Speaker 1>right because we're going to revisit a topic that Lauren

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<v Speaker 1>and I talked about, gravitational waves, and you weren't here

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<v Speaker 1>for that episode. God, just act like I'm not here.

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<v Speaker 1>So yeah, so mentally you're you're again not in the room.

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<v Speaker 1>You're on vacation. You're always wonderful and find an excellent Yeah,

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<v Speaker 1>I'm sure that you'll be a joy as always. But hey,

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<v Speaker 1>gravitational waves, this was some big this month. Yeah, huge news.

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<v Speaker 1>And actually it's funny because the discovery happened in two

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<v Speaker 1>thousand and fifteen. But as is the case with any

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<v Speaker 1>really you know, careful, responsible scientific inquiry, it took some

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<v Speaker 1>time for scientists to verify the information the data they

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<v Speaker 1>had gathered before they actually announced what they had found.

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<v Speaker 1>You know, it did, but I don't know if you

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<v Speaker 1>all noticed it, if you follow the the I don't know,

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<v Speaker 1>science writers on Twitter or or the science press in general.

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<v Speaker 1>There were several rounds of rumors flaring up where some

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<v Speaker 1>prominent physicists or cosmologists would sort of like drop a

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<v Speaker 1>hint saying like, I think they found gravity waves. Yeah,

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<v Speaker 1>I know, you're gonna you're gonna get out of your

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<v Speaker 1>red pin about that a little bit. Yeah, And and

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<v Speaker 1>so somebody would print a story about that, and the

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<v Speaker 1>rumor mill would flare up, and then it would all

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<v Speaker 1>end with well, I guess we'll just have to wait

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<v Speaker 1>until they announced their findings and see what happened. But

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<v Speaker 1>it turned out that the rumors were in this case true, right.

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<v Speaker 1>There was a very very strong, very well established piece

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<v Speaker 1>of evidence for gravitational waves in the universe. Yes, a

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<v Speaker 1>a detection that appears to be pretty much air tight.

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<v Speaker 1>So uh, And that was announced on February eleven. We

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<v Speaker 1>were all eagerly waiting for the announcement. In fact, many

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<v Speaker 1>of us were following it live as it was happening. Joe,

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<v Speaker 1>you were tweeting about it live as it was happening.

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<v Speaker 1>As I recall, I think I just I retweeted. Some

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<v Speaker 1>people got you. I wasn't. I wasn't live tweeting, and

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<v Speaker 1>you were tweeting. You weren't undead? Are you undead? Is

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<v Speaker 1>this what this called? Isomie a little bit undead? I

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<v Speaker 1>hope you all both brought across well at any rate.

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<v Speaker 1>The last zombies. Okay, go ahead if you if you're

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<v Speaker 1>really cross with a zombie, they take note. So we

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<v Speaker 1>originally talked about gravitational waves back in September two thousand

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<v Speaker 1>and fourteen, and in that conversation we were talking specifically

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<v Speaker 1>about BICEP two, which is a telescope that's in the Antarctic. Yeah,

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<v Speaker 1>and if you remember some time vaguely in the past,

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<v Speaker 1>either this podcast or just other general news announcements a

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<v Speaker 1>few years ago, and you're saying, like, wait, I thought

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<v Speaker 1>they already discovered gravitational waves. There is a reason you're

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<v Speaker 1>remembering that. Yeah. Yeah, Well they said, hey, guys, I

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<v Speaker 1>think that we we we think that we discovered gravitational waves.

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<v Speaker 1>This is so great. And what they actually discovered was

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<v Speaker 1>spacedest yeah, or at least space dust was enough of

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<v Speaker 1>a factor to throw the results into serious doubt. But

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<v Speaker 1>we'll talk about that a little bit more later in

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<v Speaker 1>the podcast. This time, we're going to really be focusing

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<v Speaker 1>on what Lego found. Uh Ligo is a pair of observatories,

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<v Speaker 1>and we'll talk more about those in a minute. But

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<v Speaker 1>before we get into any of that, perhaps it's best

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<v Speaker 1>to actually take some time to talk about what gravitational

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<v Speaker 1>waves are in the first place, and to understand that

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<v Speaker 1>you've gotta look back in history, all the way back

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<v Speaker 1>to nineteen sixteen, which is when Albert Einstein published his

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<v Speaker 1>his theory of general relativity, had been working on it

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<v Speaker 1>since nineteen o five. Right, So, Alfred B. Iimstein was

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<v Speaker 1>out on a train one day, hurling axes out the

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<v Speaker 1>window at passing herds of buffalo and he never give

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<v Speaker 1>you cold medication before a podcast. And he noticed that

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<v Speaker 1>as he tossed each ax, it arcd towards the ground

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<v Speaker 1>instead of flying off in an infinite direction in which

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<v Speaker 1>he threw it. So why does that happen. Alright, ignoring

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<v Speaker 1>everything that Joe just said, Here's here's what Einstein was

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<v Speaker 1>was considering. He had been really thinking hard about the

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<v Speaker 1>nature of the universe. Uh. This was part mathematics, part philosophy,

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<v Speaker 1>part just uh just using logic to its inevitable conclusion.

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<v Speaker 1>And it was incredible. The theory he came up with,

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<v Speaker 1>it was it was phenomenal, and not just phenomenal. But

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<v Speaker 1>over the years, so much of that theory has proven

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<v Speaker 1>to be accurate to what we see in reality. That

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<v Speaker 1>you know, we we just keep on supporting the various

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<v Speaker 1>predictions that were made, and gravitational waves were one of

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<v Speaker 1>the predictions made in the theory of general relativity. Uh.

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<v Speaker 1>He he had argued that that the universe is made

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<v Speaker 1>up of uh space time continuum. You've probably heard that

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<v Speaker 1>if you've ever watched any Star Trek, you've heard about

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<v Speaker 1>the space time continuum. But the spacetime continuum is is

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<v Speaker 1>sort of this idea of space and time together forming

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<v Speaker 1>kind of a fabric of the universe and matter or

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<v Speaker 1>to be really just just to to talk it in

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<v Speaker 1>the terms he used, mass can change, can can warp spacetime.

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<v Speaker 1>In fact, it does warp spacetime. The presence of matter

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<v Speaker 1>warps spacetime. So the most common analogy that you tend

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<v Speaker 1>to see is that imagine you've got a trampoline and

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<v Speaker 1>you put a bowling ball on the trampoline. It ends

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<v Speaker 1>up making a dimple in the trampoline. It sinks down

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<v Speaker 1>where the bowling ball is resting that here here, the

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<v Speaker 1>trampoline being spacetime and the bowling ball being say a star,

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<v Speaker 1>yeah exactly, let's let's a star, black hole, anything that's

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<v Speaker 1>got a lot of mass, and uh you that would

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<v Speaker 1>show you how the trampoline warps around the bowling ball,

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<v Speaker 1>like spacetime warps around an object of great mass. Keeping

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<v Speaker 1>in mind, of course, that we're using more or less

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<v Speaker 1>a two dimensional representation to talk about three dimensional concept.

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<v Speaker 1>But it's really hard to imagine a three dimensional concept. Really, Yeah,

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<v Speaker 1>that's true, because you're talking about time. It is true.

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<v Speaker 1>But then if you were to take a marble, let's say,

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<v Speaker 1>and roll it across the trampoline. Now, if it were

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<v Speaker 1>if there were no bowling ball on it, the marble

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<v Speaker 1>would just roll from one side to the other, assuming

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<v Speaker 1>that you're on level ground and all that. But with

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<v Speaker 1>the bowling ball. There, it's gonna start spiraling inward towards

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<v Speaker 1>the bowling ball. And Einstein argued that what we see

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<v Speaker 1>with gravity, with with gravitational pull between like a star

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<v Speaker 1>and a planet, or even the center of a galaxy

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<v Speaker 1>and all of the star systems, that's how they behave

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<v Speaker 1>they move in that same spiral. And uh So, now

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<v Speaker 1>one difference you might observe is that you think, hey,

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<v Speaker 1>well if I did that on a trampoline, and probably

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<v Speaker 1>marble would probably only spiral around the bowling ball three

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<v Speaker 1>or four times before it crashed into it. There, I

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<v Speaker 1>would guess the difference is going to be in this

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<v Speaker 1>example friction between the marble and the trampoline. We also

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<v Speaker 1>speak and orbits in space being you know, almost negligible

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<v Speaker 1>amounts of friction. Yeah, that's definitely, that's definitely the case.

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<v Speaker 1>It helps. So what we see here is that spacetime

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<v Speaker 1>curves around objects and then be building upon that. Uh

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<v Speaker 1>Einstein said, if you have a large mass undergo a

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<v Speaker 1>violent change, either it changes shape or it changes its

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<v Speaker 1>motion in some way in a dramatic way, it creates

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<v Speaker 1>these ripples in space time that propagate outward at the

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<v Speaker 1>speed of light. And these are gravitational waves. Um. So

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<v Speaker 1>it's actual ripples in space time itself, and it's kind

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<v Speaker 1>of like an electromagnetic wave, and that it moves at

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<v Speaker 1>that speed of light, but unlike electromagnetic waves, it can't

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<v Speaker 1>be absorbed and it can't be scattered. Yeah, it behaves

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<v Speaker 1>in that way, more like a sound wave. Yeah, exactly.

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<v Speaker 1>So if you think of sound waves, where when you

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<v Speaker 1>hear a sound, what you're actually hearing is the motion

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<v Speaker 1>of air molecules. Those air molecules are being compressed by

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<v Speaker 1>an oncoming wave and then they expand again afterward. It's

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<v Speaker 1>very similar to that, except we're talking about the fabric

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<v Speaker 1>of reality itself. Now, let me play Jonathan for a

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<v Speaker 1>second and be pedantic. It wouldn't necessarily have to be

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<v Speaker 1>air molecules, would it be whatever medium that the sound

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<v Speaker 1>is traveling through. That's true. Yeah, it could be solid

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<v Speaker 1>wood and it's still has um and we should we

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<v Speaker 1>should put in that Einstein himself wasn't entirely sure about

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<v Speaker 1>this gravitational wave stuff. He kind of flip flopped on

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<v Speaker 1>it a few times, but always came back around to

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<v Speaker 1>support it. So I think that he himself would be

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<v Speaker 1>sort of tickled that we a came up with a

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<v Speaker 1>way to detect them and be have actually detected Yeah.

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<v Speaker 1>I think he would be flabber guested because I the

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<v Speaker 1>impression I get is that Einstein was fairly certain because

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<v Speaker 1>the nature of gravitational waves, they would be undetectable. There

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<v Speaker 1>there'll be no way to directly observe them because they

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<v Speaker 1>are invisible, there's nothing. They're not like electromagnetic radiation, where

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<v Speaker 1>you've got an actual visible spectrum. Um. So I think

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<v Speaker 1>that would have really shocked him that we had come

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<v Speaker 1>up with a really clever way of detecting the presence

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<v Speaker 1>of gravitational waves. Now, Jonathan, why is it that you

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<v Speaker 1>have a bone to pick with anybody who calls this

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<v Speaker 1>most recent discovery the discovery of gravity waves? Well, because

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<v Speaker 1>it's wrong. So gravity waves you told me all about

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<v Speaker 1>the wrongness. Gravity and gravitational are two different things. With

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<v Speaker 1>a gravitational wave, you are talking about this ripple through

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<v Speaker 1>space time that travels outward at the speed of light.

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<v Speaker 1>With gravity waves, you're talking about a wave that exists

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<v Speaker 1>due to gravity. It's something that you would find on

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<v Speaker 1>a planet, either in some sort of fluid system, whether

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<v Speaker 1>it's an atmosphere or like a body of water. So, um,

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<v Speaker 1>let's say you've got an ocean and you've got wind

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<v Speaker 1>blowing across the surface of that ocean, it starts to

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<v Speaker 1>disturb the water. Gravity is pulling down on the surface

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<v Speaker 1>of that water, and uh, waters buoyancy is acting in

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<v Speaker 1>opposition to gravity, and that combined with the wind, creates

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<v Speaker 1>a wind driven um wave. That would be a gravity wave.

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<v Speaker 1>It's a wave that exists because gravity is there. If

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<v Speaker 1>there were no gravity through would even be a body

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<v Speaker 1>of water there. Uh. That is a gravity wave totally

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<v Speaker 1>different from a gravitational wave, just a physical wave that

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<v Speaker 1>you can observe through some form of fluidic system. And

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<v Speaker 1>so if you ever hear someone say gravity waves of

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<v Speaker 1>gravitational wave as a matter of shorthand they're technically being incorrect,

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<v Speaker 1>you should probably find a polite way to say, maybe

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<v Speaker 1>you meant gravitational wave, or you could be like me,

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<v Speaker 1>and there's no polite way to say that. Yeah, I

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<v Speaker 1>gave up on being polite years ago, so I just

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<v Speaker 1>tried to caution other people not to make the same

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<v Speaker 1>choices I made. Um. But yeah, there's some some other

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<v Speaker 1>interesting things about gravitational waves. They pass through stuff. So

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<v Speaker 1>like we said, yeah, yeah, they don't act like electromagnetic waves. Yeah,

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<v Speaker 1>they don't get absorbed or reflected, so they just poop

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<v Speaker 1>keep on going. So if you've got, for example, a

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<v Speaker 1>planet between you and electromagnetic radiation such as light from

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<v Speaker 1>the Sun, you will experience in eclipse because the planet

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<v Speaker 1>blocks it. But it will not block these gravity waves exactly, won't.

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<v Speaker 1>It won't eclipse the the movement of waves toward you.

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<v Speaker 1>The waves will get weaker as they propagate out over

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<v Speaker 1>distance though, yes, and uh So if you're talking about

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<v Speaker 1>a gravitational wave that has you know, has happened because

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<v Speaker 1>of some massive event that's a billion light years away,

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<v Speaker 1>they are very very faint by the time they get

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<v Speaker 1>to Earth. Uh And that also leads to why they've

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<v Speaker 1>been so tricky to detect. Not only are they invisible,

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<v Speaker 1>but they're not very strong. So we have to look

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<v Speaker 1>for gravitational waves that have been caused by really really

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<v Speaker 1>big events, like in the case of the one that

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<v Speaker 1>Ligo detected in September two thousand fifteen, it was the

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<v Speaker 1>collision of two black holes. It's a pretty big event.

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<v Speaker 1>Others could be two neutron stars that are orbiting one

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<v Speaker 1>another rapidly, which would create kind of an oscillating and

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<v Speaker 1>continuous a series of gravitational waves. Um or it could

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<v Speaker 1>be like a supernova exploding that to do it. A

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<v Speaker 1>big bang that would do it too. In fact, that

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<v Speaker 1>was what my step two was looking for, was the

0:13:04.520 --> 0:13:07.800
<v Speaker 1>evidence of gravity waves from the era of the Big Bang.

0:13:07.880 --> 0:13:13.880
<v Speaker 1>I just caught you in it. What, oh man, I

0:13:13.360 --> 0:13:18.640
<v Speaker 1>I I stand correct, I sit corrected here in to eat,

0:13:18.840 --> 0:13:21.520
<v Speaker 1>Thank you well, and as soon as I get the

0:13:21.520 --> 0:13:23.400
<v Speaker 1>foot out of my mouth, I will start chewing upon

0:13:23.440 --> 0:13:27.880
<v Speaker 1>the hat. Yes, gravitational wave not gravity wave. No, it's

0:13:27.920 --> 0:13:30.079
<v Speaker 1>true that they have been so difficult to detect and

0:13:30.240 --> 0:13:33.959
<v Speaker 1>that we've had to come up with very interesting methods

0:13:34.000 --> 0:13:39.400
<v Speaker 1>of trying to detect them, involving laser interferometry. Yeah. So

0:13:39.520 --> 0:13:43.680
<v Speaker 1>here's here's something that's really cool about a gravitational wave

0:13:44.240 --> 0:13:47.000
<v Speaker 1>because it's this ripple in space time. It actually is

0:13:47.040 --> 0:13:48.560
<v Speaker 1>a small you can think of it like a small

0:13:48.640 --> 0:13:53.360
<v Speaker 1>fold in spacetime, right, and that means it can actually

0:13:53.559 --> 0:13:57.920
<v Speaker 1>change the distance between two points by compressing that distance

0:13:58.480 --> 0:14:01.880
<v Speaker 1>or expanding it like a rubber band. So you've got

0:14:01.880 --> 0:14:05.000
<v Speaker 1>like a piece of elastic h or if you prefer,

0:14:05.120 --> 0:14:07.800
<v Speaker 1>you know, just just imagine that, Um, Joe, you and

0:14:07.840 --> 0:14:10.800
<v Speaker 1>I are standing across a football field from one another.

0:14:11.160 --> 0:14:13.360
<v Speaker 1>You're on one end zone. I'm in the other end zone.

0:14:14.000 --> 0:14:16.640
<v Speaker 1>Their en zones in football, right, I'm just looking for

0:14:17.280 --> 0:14:21.040
<v Speaker 1>There's no help from the one with the oblong spheroid, right, Yes,

0:14:21.080 --> 0:14:24.240
<v Speaker 1>that's it. Or you know, a soccer field if you prefer,

0:14:24.320 --> 0:14:27.800
<v Speaker 1>But then you know where at either end gravitational wave

0:14:27.840 --> 0:14:30.960
<v Speaker 1>passes through. Let's say it's a massive gravitational wave, something

0:14:31.120 --> 0:14:34.120
<v Speaker 1>way bigger than we would ever actually observe here on Earth.

0:14:34.560 --> 0:14:37.640
<v Speaker 1>What would appear to happen is that Joe and I

0:14:37.680 --> 0:14:40.080
<v Speaker 1>from our perspectives, it would look like we got closer

0:14:40.120 --> 0:14:42.800
<v Speaker 1>and then further apart, and then closer and then further apart,

0:14:43.240 --> 0:14:47.280
<v Speaker 1>without ever taking a step in either direction. That the are,

0:14:47.520 --> 0:14:52.680
<v Speaker 1>the world itself has compressed and expanded around us because

0:14:52.720 --> 0:14:56.680
<v Speaker 1>of this fold in spacetime that's passing through, which sounds

0:14:56.720 --> 0:15:02.080
<v Speaker 1>like some serious like matrix style stuff. But either fortunately

0:15:02.160 --> 0:15:05.600
<v Speaker 1>or unfortunately, depending on how you know, stable you like

0:15:05.680 --> 0:15:10.240
<v Speaker 1>your reality, that's that's that kind of dramatic change is

0:15:10.280 --> 0:15:13.360
<v Speaker 1>not what we observe from gravitational waves, right, Not at all,

0:15:13.480 --> 0:15:16.840
<v Speaker 1>not even remotely in the same football field as it were.

0:15:17.720 --> 0:15:20.200
<v Speaker 1>Uh No, Instead, if you were to have something like

0:15:20.280 --> 0:15:24.880
<v Speaker 1>a supernova explosion, and I should say an asymmetric supernova

0:15:24.960 --> 0:15:28.720
<v Speaker 1>explosion for reasons I don't understand, a symmetrical supernova does

0:15:28.760 --> 0:15:33.280
<v Speaker 1>not a supernova explosion does not generate gravitational waves. I

0:15:33.360 --> 0:15:36.160
<v Speaker 1>don't know why I was reading it trying to find

0:15:36.160 --> 0:15:37.840
<v Speaker 1>more information, but it got to a point where the

0:15:37.880 --> 0:15:42.440
<v Speaker 1>astrophysics got way too complicated for me to understand. However,

0:15:42.480 --> 0:15:44.240
<v Speaker 1>what I do understand is that if there were a

0:15:44.240 --> 0:15:47.840
<v Speaker 1>supernova explosion in our galaxy in the Milky Way, the

0:15:47.880 --> 0:15:52.200
<v Speaker 1>gravitational waves generated from that would only be powerful enough

0:15:52.320 --> 0:15:55.880
<v Speaker 1>to change the distance between Earth and the Sun by

0:15:55.880 --> 0:15:58.640
<v Speaker 1>the diameter of one hydrogen atom. That's how much it

0:15:58.640 --> 0:16:04.640
<v Speaker 1>would oscillate. Oh yeah, okay, you probably would notice. So

0:16:04.800 --> 0:16:06.520
<v Speaker 1>this is like a princess and the p kind of thing,

0:16:06.560 --> 0:16:12.000
<v Speaker 1>isn't it. Yeah, definitely, definitely on that level. Obviously, we

0:16:12.040 --> 0:16:16.520
<v Speaker 1>need to build a more sensitive princess. That's that's the

0:16:16.840 --> 0:16:20.400
<v Speaker 1>you know, that's entirely the plot. Yeah, yeah, we're about

0:16:20.400 --> 0:16:24.120
<v Speaker 1>a mattress. You know, it's all musical about that. Oh

0:16:24.280 --> 0:16:30.800
<v Speaker 1>I didn't build a robot princess, any number of mattress.

0:16:30.920 --> 0:16:35.560
<v Speaker 1>They just they just uh collued to make her uncomfortable

0:16:35.600 --> 0:16:39.760
<v Speaker 1>so that she she complains about the the lumpiness of

0:16:39.760 --> 0:16:41.360
<v Speaker 1>the mattress, and it turns out that there's not just

0:16:41.400 --> 0:16:43.400
<v Speaker 1>a p under there. There's also a suit of armor

0:16:43.400 --> 0:16:46.640
<v Speaker 1>and a shield. Spoiler alert for any of you who

0:16:46.680 --> 0:16:49.040
<v Speaker 1>are really looking forward to what's upon a mattress. Yeah.

0:16:49.080 --> 0:16:50.640
<v Speaker 1>But but but I suppose they did kind of create

0:16:50.720 --> 0:16:53.000
<v Speaker 1>like a laser princess. So yeah, but we'll get into that.

0:16:53.040 --> 0:16:56.480
<v Speaker 1>So anyway, So so I just mentioned that if you're

0:16:56.520 --> 0:16:59.640
<v Speaker 1>looking at the Earth and the Sun, you're talking about

0:16:59.640 --> 0:17:02.600
<v Speaker 1>the differ prints of the diameter of an hydrogen atom

0:17:02.880 --> 0:17:06.600
<v Speaker 1>in the distance, which is incredible to think about. But

0:17:07.040 --> 0:17:11.120
<v Speaker 1>that that change, that difference in distance gets smaller as

0:17:11.160 --> 0:17:14.600
<v Speaker 1>you get two smaller scales. So let's talk about if

0:17:14.640 --> 0:17:16.960
<v Speaker 1>you were on Earth and trying to measure this, because

0:17:16.960 --> 0:17:20.439
<v Speaker 1>this gets to why it has been so challenging to

0:17:20.520 --> 0:17:23.520
<v Speaker 1>detect gravitational waves here on Earth. Okay, don't use a

0:17:23.520 --> 0:17:27.080
<v Speaker 1>football field analogy. What about the need to how about

0:17:27.080 --> 0:17:29.560
<v Speaker 1>the beginning and end of the line for space Mountain.

0:17:31.280 --> 0:17:33.879
<v Speaker 1>That's a queue that goes like, yeah, that one already

0:17:33.920 --> 0:17:36.400
<v Speaker 1>loops around back on itself in weird ways. Yeah, it's

0:17:36.440 --> 0:17:38.800
<v Speaker 1>not really gonna work. No, I don't need to make

0:17:38.800 --> 0:17:42.240
<v Speaker 1>that comparison. I was just to to establish the weirdness

0:17:42.400 --> 0:17:45.160
<v Speaker 1>of what happens. But no, I wanted to just talk

0:17:45.200 --> 0:17:47.920
<v Speaker 1>about the scale. So if you were talking about here

0:17:47.960 --> 0:17:51.760
<v Speaker 1>on Earth and you're trying to measure that that change

0:17:51.840 --> 0:17:56.040
<v Speaker 1>in reality, that change in distance because the spacetime continuum

0:17:56.119 --> 0:17:58.720
<v Speaker 1>is being folded in this ripple. Uh. If you had

0:17:58.720 --> 0:18:00.600
<v Speaker 1>two objects that are about a column butt are apart,

0:18:01.080 --> 0:18:04.199
<v Speaker 1>the change in distance they would experience due to that

0:18:04.280 --> 0:18:09.040
<v Speaker 1>gravitational wave would be thousands of the diameter of a proton.

0:18:09.840 --> 0:18:13.159
<v Speaker 1>So take a sub atomic particle and go a teeny

0:18:13.200 --> 0:18:16.240
<v Speaker 1>tiny fraction of the diameter of that subotomic particle, and

0:18:16.280 --> 0:18:20.480
<v Speaker 1>that's how much difference in distance it would experience. Get

0:18:20.680 --> 0:18:23.800
<v Speaker 1>out your your proton knife and your proton measuring set,

0:18:24.000 --> 0:18:26.720
<v Speaker 1>and it turns out your ruler is not going to

0:18:26.800 --> 0:18:30.360
<v Speaker 1>be terribly helpful in that case. So that is one

0:18:30.359 --> 0:18:33.720
<v Speaker 1>of the reasons why it's been so incredibly challenging to

0:18:33.880 --> 0:18:37.640
<v Speaker 1>detect the presence of a gravitational wave. And and we

0:18:37.640 --> 0:18:40.399
<v Speaker 1>we've had a few leads, or if you prefer, a

0:18:40.400 --> 0:18:43.840
<v Speaker 1>few false starts in detecting them throughout history. Back in

0:18:44.000 --> 0:18:48.200
<v Speaker 1>nineteen sixty nine, University of Maryland physicist Joseph Weber created

0:18:48.240 --> 0:18:51.840
<v Speaker 1>this this six foot aluminum cylinder that he claimed would

0:18:51.880 --> 0:18:55.320
<v Speaker 1>act like an antenna for gravitational waves. He said that

0:18:55.400 --> 0:18:57.640
<v Speaker 1>when such a wave hit the cylinder, it would ring

0:18:57.760 --> 0:19:01.280
<v Speaker 1>like a tuning fork, but nobody else could replicate his results.

0:19:01.359 --> 0:19:03.680
<v Speaker 1>It was a kind of neat looking device, though. There's

0:19:03.720 --> 0:19:05.679
<v Speaker 1>actual video of this, and it look kind of like

0:19:05.720 --> 0:19:09.399
<v Speaker 1>a mirrored two inside another tube, like there was like

0:19:09.440 --> 0:19:13.840
<v Speaker 1>some sort of crazy physics disco going on inside there. Uh,

0:19:14.520 --> 0:19:16.720
<v Speaker 1>or at least that's what I like to think. Back

0:19:16.720 --> 0:19:19.280
<v Speaker 1>in nineteen seventy four, there are a pair of scientists

0:19:19.680 --> 0:19:25.879
<v Speaker 1>in Puerto Rico who saw a binary pulsar system and

0:19:26.359 --> 0:19:29.520
<v Speaker 1>they looked at the theory of general relativity, which predicted

0:19:29.560 --> 0:19:33.119
<v Speaker 1>that such a system would gradually lose energy due to

0:19:33.280 --> 0:19:36.720
<v Speaker 1>the too emitting gravitational waves. Some of its energy would

0:19:36.800 --> 0:19:40.720
<v Speaker 1>go into creating these gravitational waves, and because you have

0:19:40.760 --> 0:19:43.400
<v Speaker 1>a system losing energy, it would start to lose speed.

0:19:44.160 --> 0:19:47.960
<v Speaker 1>And so they said, well, based upon this prediction, we

0:19:48.000 --> 0:19:51.159
<v Speaker 1>should observe this change in speed as long as we

0:19:51.280 --> 0:19:55.040
<v Speaker 1>keep an eye on this binary pulsar system. So they

0:19:55.119 --> 0:19:58.200
<v Speaker 1>tracked it for eight years. At the end of the

0:19:58.280 --> 0:20:02.040
<v Speaker 1>eight year period, they said the behavior of the binary

0:20:02.080 --> 0:20:06.440
<v Speaker 1>pulsar system was completely in line with the predictions from

0:20:06.440 --> 0:20:11.159
<v Speaker 1>general relativity. He said, it is behaving precisely the way

0:20:11.280 --> 0:20:15.160
<v Speaker 1>it would if, in fact, gravitational waves are reality. Therefore,

0:20:15.680 --> 0:20:19.000
<v Speaker 1>this is in support of gravitational waves. And even since then,

0:20:19.640 --> 0:20:23.199
<v Speaker 1>over the forty years of observations that have happened with

0:20:23.280 --> 0:20:27.639
<v Speaker 1>this binary pulsar system, those predictions continued to be supported.

0:20:28.040 --> 0:20:33.760
<v Speaker 1>So that was great, you know, indirect evidence of gravitational waves, saying, well,

0:20:33.800 --> 0:20:37.320
<v Speaker 1>if they don't exist, something else must be happening for

0:20:37.480 --> 0:20:39.600
<v Speaker 1>this system to slow down the way it is. But

0:20:39.680 --> 0:20:42.160
<v Speaker 1>the thing that makes most sense is that Einstein was right.

0:20:42.920 --> 0:20:45.560
<v Speaker 1>Then we move ahead quite a bit. Let's talk about

0:20:45.600 --> 0:20:48.639
<v Speaker 1>BICEP two. Now, BICEP two was going a different way

0:20:49.240 --> 0:20:52.520
<v Speaker 1>about looking for gravitational waves. They were specifically looking for

0:20:52.600 --> 0:20:58.080
<v Speaker 1>evidence of UH that would support a hypothesis called cosmic inflation,

0:20:58.840 --> 0:21:02.359
<v Speaker 1>and inflation is a big deal in physical cosmology today.

0:21:02.400 --> 0:21:07.399
<v Speaker 1>This is I think most physical cosmologists look at inflation

0:21:07.520 --> 0:21:11.000
<v Speaker 1>is very promising theory. Yeah, And the whole reason why

0:21:11.119 --> 0:21:13.800
<v Speaker 1>we have this this idea in the first place is

0:21:13.840 --> 0:21:17.600
<v Speaker 1>to explain why the universe appears the way it does,

0:21:18.280 --> 0:21:22.320
<v Speaker 1>while also trying to reconcile that with the Big Bang theory.

0:21:22.400 --> 0:21:25.359
<v Speaker 1>Because I'm not going to get too far into the

0:21:25.359 --> 0:21:32.399
<v Speaker 1>weeds here, but the basically the hypothesis says that about

0:21:32.520 --> 0:21:37.639
<v Speaker 1>ten to the negative thirty six seconds. So take a

0:21:37.720 --> 0:21:40.840
<v Speaker 1>ten and then take a decimal point and move that

0:21:41.119 --> 0:21:43.919
<v Speaker 1>thirty six places to the left. Get get that proton

0:21:44.000 --> 0:21:47.000
<v Speaker 1>knife out again, did up a second, right, That's that's

0:21:47.040 --> 0:21:49.480
<v Speaker 1>where you get down to the teeny tiny, tiny tiny

0:21:49.480 --> 0:21:52.040
<v Speaker 1>fraction of a second to about ten to the negative

0:21:52.080 --> 0:21:57.119
<v Speaker 1>thirty three or thirty second power seconds. So so in

0:21:57.200 --> 0:22:01.760
<v Speaker 1>an instant, as far as we're concerned, into an instant, Yeah,

0:22:02.000 --> 0:22:06.240
<v Speaker 1>that at that moment, that's when the universe underwent rapid expansion,

0:22:07.320 --> 0:22:12.159
<v Speaker 1>far greater than the rate of expansion it currently is

0:22:12.200 --> 0:22:15.960
<v Speaker 1>going through. And it's expanding fast today. Yeah. Actually, then

0:22:15.960 --> 0:22:18.159
<v Speaker 1>it's picking up speed, which is a little uh, at

0:22:18.240 --> 0:22:20.600
<v Speaker 1>least according to our measurements, it is picking up speed.

0:22:20.640 --> 0:22:23.719
<v Speaker 1>But that's that's something that we hope gravitational waves will

0:22:23.760 --> 0:22:26.440
<v Speaker 1>help us learn more about in the future at any rate.

0:22:26.560 --> 0:22:30.080
<v Speaker 1>A scientist named Alan Gooth proposed a hypothesis to explain

0:22:31.200 --> 0:22:34.560
<v Speaker 1>why the universe looks the way it does and stay

0:22:34.640 --> 0:22:36.800
<v Speaker 1>in line with the Big Bang theory. It was kind

0:22:36.840 --> 0:22:39.800
<v Speaker 1>of like, well, in order for us to be where

0:22:39.840 --> 0:22:43.520
<v Speaker 1>we are now based upon the observations of the universe

0:22:43.560 --> 0:22:45.760
<v Speaker 1>we have made so far, and in order for the

0:22:45.760 --> 0:22:48.760
<v Speaker 1>Big Bang theory to make any sense whatsoever, there had

0:22:48.800 --> 0:22:51.480
<v Speaker 1>to be this period of cosmic inflation or else. It

0:22:51.560 --> 0:22:54.560
<v Speaker 1>just doesn't work out. The math doesn't work out. And

0:22:55.119 --> 0:22:57.119
<v Speaker 1>in a way you could argue, all this is almost

0:22:57.160 --> 0:22:59.800
<v Speaker 1>like a placeholder, except again, it's kind of like Einstein.

0:23:00.119 --> 0:23:02.960
<v Speaker 1>It's using logic saying, well, we we know about this,

0:23:03.359 --> 0:23:06.080
<v Speaker 1>we're pretty sure about this other thing. But in order

0:23:06.119 --> 0:23:08.720
<v Speaker 1>for those two things to reconcile, this other, this third

0:23:08.720 --> 0:23:11.840
<v Speaker 1>thing must have happened at some point. Yeah. Yeah, it's

0:23:11.840 --> 0:23:15.880
<v Speaker 1>theoretically solving for X in this equation. Yeah, and if

0:23:15.880 --> 0:23:19.960
<v Speaker 1>you fast forward three thousand years after the Big Bang,

0:23:20.800 --> 0:23:23.960
<v Speaker 1>you then have the emergence of the cosmic microwave background

0:23:24.119 --> 0:23:27.720
<v Speaker 1>or c MB. Now, this is a radiation that's sort

0:23:27.760 --> 0:23:31.119
<v Speaker 1>of a fingerprint left over from the from the era

0:23:31.240 --> 0:23:33.840
<v Speaker 1>after the Big Bang. It's from it's when the universe

0:23:33.920 --> 0:23:37.080
<v Speaker 1>was still seeing birdies. Like in the cartoon, universe really

0:23:37.119 --> 0:23:39.720
<v Speaker 1>wasn't seeing anything. It was so dense that even light

0:23:39.800 --> 0:23:43.679
<v Speaker 1>couldn't pass through it at this point. Um, but it is.

0:23:43.760 --> 0:23:46.000
<v Speaker 1>It's sort of the remnant of that era, and we

0:23:46.040 --> 0:23:49.960
<v Speaker 1>can we can detect the cosmic microwave background. So BICEP

0:23:50.000 --> 0:23:52.680
<v Speaker 1>two I didn't mention to se either. BICEP actually stands

0:23:52.720 --> 0:23:57.280
<v Speaker 1>for background imaging of cosmic extra galactic polarization. Was looking

0:23:57.359 --> 0:24:02.239
<v Speaker 1>for polarized cosmic microwave background radiation. The idea being that

0:24:02.840 --> 0:24:08.040
<v Speaker 1>gravitational waves should have aligned certain segments of the CMB,

0:24:08.640 --> 0:24:11.199
<v Speaker 1>so if you could detect that, then that would be

0:24:11.240 --> 0:24:15.520
<v Speaker 1>indirect evidence of gravitational waves and therefore also indirect evidence

0:24:15.640 --> 0:24:19.320
<v Speaker 1>of this cosmic inflation idea, because something as dramatic as

0:24:19.320 --> 0:24:23.320
<v Speaker 1>cosmic inflation would have generated gravitational waves and they would

0:24:23.320 --> 0:24:27.120
<v Speaker 1>have left their mark on something like the CNB, and

0:24:27.160 --> 0:24:29.680
<v Speaker 1>they the team thought they found it. They actually thought

0:24:29.720 --> 0:24:32.560
<v Speaker 1>they found it a couple of years before the news broke.

0:24:32.640 --> 0:24:37.160
<v Speaker 1>They spent years trying to verify the information they found

0:24:37.160 --> 0:24:41.160
<v Speaker 1>to make sure that they eliminated other possibilities. They went

0:24:41.520 --> 0:24:45.480
<v Speaker 1>public with the UH the announcement I think March of

0:24:45.480 --> 0:24:48.680
<v Speaker 1>two thousand fourteen, and it was September two thousand fourteen

0:24:48.680 --> 0:24:51.879
<v Speaker 1>when other teams came out and said, we think it

0:24:51.960 --> 0:24:55.880
<v Speaker 1>might be the presence of space dust that has at

0:24:56.000 --> 0:25:01.080
<v Speaker 1>least complicated your findings, if not discredit it. Did them, Yeah,

0:25:01.119 --> 0:25:03.680
<v Speaker 1>well yeah, and that's you know, they had opened up

0:25:03.720 --> 0:25:06.199
<v Speaker 1>their research to that kind of scientific scrutiny. They were

0:25:06.200 --> 0:25:08.760
<v Speaker 1>basically saying, hey, y'all, would you please check this for us?

0:25:08.800 --> 0:25:11.240
<v Speaker 1>And so that's and that's the process of science. And

0:25:11.240 --> 0:25:13.040
<v Speaker 1>that's really what Jonathan and I talked about in our

0:25:13.040 --> 0:25:17.639
<v Speaker 1>previous episode about BICEP. Let's be responsible scientists, folks, And

0:25:17.680 --> 0:25:20.440
<v Speaker 1>that's exactly what was going on here, which sometimes leads

0:25:20.480 --> 0:25:25.400
<v Speaker 1>to disappointing outcomes, but it's better than UH being wrong

0:25:25.760 --> 0:25:28.800
<v Speaker 1>and just sticking to being wrong, and and even even

0:25:28.840 --> 0:25:32.520
<v Speaker 1>disproving an outcome can be fascinating and in terms of

0:25:32.680 --> 0:25:35.760
<v Speaker 1>research progress moving forward. Right, So, in the case of

0:25:35.760 --> 0:25:38.159
<v Speaker 1>BICEP two, we're talking about using telescopes to try and

0:25:38.200 --> 0:25:42.240
<v Speaker 1>detect UH the presence of gravitational waves through its effects

0:25:42.240 --> 0:25:45.000
<v Speaker 1>on other stuff. But what about just trying to detect

0:25:45.119 --> 0:25:48.240
<v Speaker 1>the presence of gravitational waves themselves, not look at how

0:25:48.280 --> 0:25:51.880
<v Speaker 1>it's affecting something else, but somehow detecting their presence here

0:25:51.960 --> 0:25:56.680
<v Speaker 1>on earth. So let me guess you get two things,

0:25:57.160 --> 0:25:59.399
<v Speaker 1>and you put them a kilometer apart, and you watch

0:25:59.440 --> 0:26:01.639
<v Speaker 1>them real close to see if they vary by the

0:26:01.680 --> 0:26:05.840
<v Speaker 1>width of a thousandth of a proton very close. You

0:26:05.880 --> 0:26:09.800
<v Speaker 1>actually have to get at least three things. Uh, and

0:26:09.840 --> 0:26:13.080
<v Speaker 1>then you have to watch them very close with lasers.

0:26:13.680 --> 0:26:16.280
<v Speaker 1>So this was an idea that was proposed by Ray

0:26:16.359 --> 0:26:21.399
<v Speaker 1>weiss Um. He suggested creating a laser interferometer system to

0:26:21.520 --> 0:26:26.960
<v Speaker 1>detect any sort of distortion in spacetime. And uh, it's

0:26:27.000 --> 0:26:30.960
<v Speaker 1>a really brilliant and elegant solution to a difficult problem. Yeah,

0:26:31.040 --> 0:26:34.000
<v Speaker 1>and and he started working on this along with one

0:26:34.040 --> 0:26:35.800
<v Speaker 1>of the other people who would become a lead on

0:26:35.840 --> 0:26:39.520
<v Speaker 1>the project, Kip Thorne. Kip Thorne, by the way, good name,

0:26:40.040 --> 0:26:44.199
<v Speaker 1>good good job. Kip Thorne's parents. Anyway, So they got

0:26:44.240 --> 0:26:46.720
<v Speaker 1>their start way back in five when the two of

0:26:46.760 --> 0:26:49.120
<v Speaker 1>them happened to share a hotel room at a conference

0:26:49.160 --> 0:26:51.840
<v Speaker 1>and wound up just staying up all night chattering about

0:26:51.920 --> 0:26:55.720
<v Speaker 1>gravitational waves and feel that's not what's going to happen

0:26:55.760 --> 0:26:59.440
<v Speaker 1>to me at south By Southwest, I know anyway, So

0:26:59.600 --> 0:27:03.399
<v Speaker 1>so Thorn wound up pulling in Ronald Drever, who's whose

0:27:03.520 --> 0:27:06.720
<v Speaker 1>original idea I think it was to use lasers for this,

0:27:07.080 --> 0:27:10.439
<v Speaker 1>And the work was originally out of cal Tech because Weiss,

0:27:10.440 --> 0:27:12.359
<v Speaker 1>who was at m I T at the time, couldn't

0:27:12.359 --> 0:27:14.520
<v Speaker 1>convince M I T the black holes were cool enough

0:27:14.560 --> 0:27:19.200
<v Speaker 1>to study sat draw bone. Yeah, he says, by the way,

0:27:19.200 --> 0:27:23.879
<v Speaker 1>that M I T has since gotten better. So LEGO

0:27:24.119 --> 0:27:28.080
<v Speaker 1>is the pair of observatories that was responsible for detecting

0:27:28.160 --> 0:27:31.040
<v Speaker 1>this particular gravitational wave. Have you seen a picture of

0:27:31.040 --> 0:27:33.840
<v Speaker 1>one of the LEGO facilities. Yes, they're really cool. Yeah,

0:27:33.960 --> 0:27:38.720
<v Speaker 1>they look like giant V or an L. Yeah, depends

0:27:38.720 --> 0:27:41.800
<v Speaker 1>on your perspective. I suppose, I guess. I guess so.

0:27:41.840 --> 0:27:43.760
<v Speaker 1>I always thought it L not V shaped, But I

0:27:43.840 --> 0:27:49.440
<v Speaker 1>understand entirely. Um. The so LEGO, the Laser Interferometer Gravitational

0:27:49.480 --> 0:27:55.879
<v Speaker 1>Wave Observatory. Its purpose wasn't to look for gravitational waves

0:27:55.920 --> 0:28:00.800
<v Speaker 1>that were responsible during or were a result oather of

0:28:00.840 --> 0:28:04.800
<v Speaker 1>cosmic inflation. Uh, they're looking for things that happened after

0:28:04.840 --> 0:28:07.920
<v Speaker 1>the Big Bang, things like black holes colliding or these

0:28:07.960 --> 0:28:11.240
<v Speaker 1>neutron stars that are in orbit around one another. That's

0:28:11.240 --> 0:28:14.159
<v Speaker 1>sort of stuff. Those those sort of gravitational waves. The

0:28:14.160 --> 0:28:17.840
<v Speaker 1>presence of gravitational waves that are actively passing through Earth,

0:28:18.480 --> 0:28:21.800
<v Speaker 1>that's what these are looking for. And so they're not telescopes.

0:28:21.920 --> 0:28:26.520
<v Speaker 1>So the discovery that was announced in February is though

0:28:26.520 --> 0:28:29.560
<v Speaker 1>they're both involving gravitational waves, they were sort of fundamentally

0:28:29.560 --> 0:28:35.000
<v Speaker 1>different discoveries between that and the one from Yes. So, uh,

0:28:35.520 --> 0:28:38.920
<v Speaker 1>some interesting stuff about LEGO. It originally went online in

0:28:39.040 --> 0:28:42.560
<v Speaker 1>two thousand two UM and it was the largest project

0:28:42.640 --> 0:28:45.400
<v Speaker 1>to ever be funded by the National Science Foundation at

0:28:45.440 --> 0:28:48.640
<v Speaker 1>that time. They've spent over the past forty years about

0:28:48.760 --> 0:28:52.320
<v Speaker 1>one point one billion dollars in pursuit of this. YEP.

0:28:52.520 --> 0:28:55.040
<v Speaker 1>And like I mentioned before, there are two observing stations.

0:28:55.080 --> 0:28:57.600
<v Speaker 1>One is in Louisiana and the other is in Washington.

0:28:57.680 --> 0:29:01.320
<v Speaker 1>There almost two thousand miles apart. Part I'll talk more

0:29:01.360 --> 0:29:03.720
<v Speaker 1>about exactly how far they are a little bit later,

0:29:03.760 --> 0:29:07.400
<v Speaker 1>but uh uh, the two stations are necessary to confirm

0:29:07.440 --> 0:29:11.200
<v Speaker 1>the presence of gravitational waves. You want that same observation

0:29:11.240 --> 0:29:14.840
<v Speaker 1>to be picked up by both facilities within like ten

0:29:14.880 --> 0:29:17.800
<v Speaker 1>milliseconds of one another for it to be considered a

0:29:17.800 --> 0:29:21.560
<v Speaker 1>potential gravitational wave. Hit right, because otherwise, you know, like

0:29:21.600 --> 0:29:24.760
<v Speaker 1>a really big truck passing by could possibly set off

0:29:24.800 --> 0:29:27.560
<v Speaker 1>one of the monitors. It could be a seismic activity,

0:29:27.600 --> 0:29:32.400
<v Speaker 1>could be anything that would uh jitter the system, if

0:29:32.440 --> 0:29:34.800
<v Speaker 1>you will. And if one of them picks it up

0:29:34.800 --> 0:29:37.040
<v Speaker 1>and the other one doesn't, then that tells you it

0:29:37.080 --> 0:29:40.240
<v Speaker 1>was probably a localized event that gave a false positive

0:29:40.320 --> 0:29:42.880
<v Speaker 1>at one observatory. If both of them pick it up

0:29:42.920 --> 0:29:45.360
<v Speaker 1>again within ten milliseconds of each other and it's clearly

0:29:45.360 --> 0:29:47.920
<v Speaker 1>the same frequency wave, we know it's not a giant

0:29:47.920 --> 0:29:51.400
<v Speaker 1>crayfish attack in the Louisiana location. That's right. It's probably

0:29:51.400 --> 0:29:55.800
<v Speaker 1>we're probably not John Balaya related at that point unless

0:29:55.840 --> 0:30:04.440
<v Speaker 1>they've unless they've colluded, colluding crawfish Washington, right, crawfish collusion.

0:30:05.720 --> 0:30:10.680
<v Speaker 1>I gotta find your stash of though medication, because I

0:30:10.760 --> 0:30:14.240
<v Speaker 1>want whatever you're on, So you don't let's talk about

0:30:14.480 --> 0:30:16.880
<v Speaker 1>so I don't want the cold, that's true. Let's talk

0:30:16.920 --> 0:30:19.880
<v Speaker 1>about the the actual facility. So I think of them

0:30:19.920 --> 0:30:23.360
<v Speaker 1>as being L shaped because there they are the two

0:30:23.680 --> 0:30:26.920
<v Speaker 1>branches or two arms of this facility are at a

0:30:27.000 --> 0:30:30.120
<v Speaker 1>ninety degree angle from one another. And maybe because Lego

0:30:30.240 --> 0:30:33.120
<v Speaker 1>starts with a nail, that also a bit of priming there. Yeah,

0:30:33.240 --> 0:30:35.800
<v Speaker 1>that probably probably helps. You're right, they are at ninety

0:30:35.840 --> 0:30:39.280
<v Speaker 1>degree angle, but it's this giant nine degree angle with

0:30:39.480 --> 0:30:42.720
<v Speaker 1>arms stretching way out into the into the fields. Yeah.

0:30:42.920 --> 0:30:46.280
<v Speaker 1>So there's one that goes under a little road. Did

0:30:46.320 --> 0:30:48.719
<v Speaker 1>you see that one? Because like there's like a they

0:30:48.760 --> 0:30:51.280
<v Speaker 1>built a little tunnel that the arm goes through and

0:30:51.400 --> 0:30:53.680
<v Speaker 1>a road passes over it. And by road, I mean

0:30:53.680 --> 0:30:55.800
<v Speaker 1>like a dirt road. I'm not talking like a highway

0:30:55.880 --> 0:30:59.520
<v Speaker 1>or something. So each branch of the l each arm

0:30:59.640 --> 0:31:01.640
<v Speaker 1>of the is two and a half miles or four

0:31:01.720 --> 0:31:05.560
<v Speaker 1>kilometers long, and it's actually a vacuum tube. They pump

0:31:05.560 --> 0:31:08.600
<v Speaker 1>out all the air uh in the facility in order

0:31:08.640 --> 0:31:12.600
<v Speaker 1>to avoid any kind of absorption, refraction or anything like that,

0:31:12.640 --> 0:31:16.800
<v Speaker 1>any any interference that atmosphere could create while you're firing

0:31:16.800 --> 0:31:19.640
<v Speaker 1>a laser down this tube. And they actually have a

0:31:19.680 --> 0:31:22.720
<v Speaker 1>beam splitter, So they have a single laser that generates

0:31:22.720 --> 0:31:25.640
<v Speaker 1>a laser beam hits a beam splitter. The beam splitter

0:31:25.760 --> 0:31:29.200
<v Speaker 1>splits the beam as the name would indicate into two.

0:31:29.520 --> 0:31:31.440
<v Speaker 1>One goes down one branch, the other one goes down

0:31:31.480 --> 0:31:34.720
<v Speaker 1>the other branch. Remember they're perpendicular to each other. H

0:31:34.720 --> 0:31:37.280
<v Speaker 1>branch has a series of mirrors in it, so the

0:31:37.360 --> 0:31:40.479
<v Speaker 1>lasers bounce off the mirrors and return back to the

0:31:40.520 --> 0:31:45.400
<v Speaker 1>crux of the l and there, because they're both from

0:31:45.440 --> 0:31:48.880
<v Speaker 1>the same laser, they have the same wavelength, they cancel

0:31:49.000 --> 0:31:52.160
<v Speaker 1>one another out. That's where the interferometry comes in. Yes,

0:31:52.360 --> 0:31:57.560
<v Speaker 1>so they interfere with one another. They end up creating uh. Well,

0:31:57.600 --> 0:31:59.959
<v Speaker 1>because they cancel out, there's no more light that's admitted

0:32:00.160 --> 0:32:05.120
<v Speaker 1>through the the that area. And they have a light detector,

0:32:05.560 --> 0:32:08.240
<v Speaker 1>so the light detector would detect if any laser light

0:32:08.280 --> 0:32:13.360
<v Speaker 1>came through. But as long as everything is going perfectly well,

0:32:14.000 --> 0:32:16.360
<v Speaker 1>they cancel each other out. But what if somebody were

0:32:16.360 --> 0:32:18.800
<v Speaker 1>to come along and shorten one of those long arms

0:32:18.800 --> 0:32:21.920
<v Speaker 1>a little bit, Well, then one laser would travel a

0:32:21.960 --> 0:32:26.080
<v Speaker 1>shorter distance than the other laser, and those wavelengths would

0:32:26.120 --> 0:32:28.840
<v Speaker 1>be out of alignment, and then you would get some

0:32:28.960 --> 0:32:32.200
<v Speaker 1>laser light coming out from that, and the light detector

0:32:32.280 --> 0:32:36.560
<v Speaker 1>would pick it up and say, hey, uh, things are hinky.

0:32:36.640 --> 0:32:40.000
<v Speaker 1>So when a gravitational wave moves through. What happens is

0:32:40.120 --> 0:32:43.479
<v Speaker 1>one arm will start to get longer while another arm

0:32:43.520 --> 0:32:46.680
<v Speaker 1>will start to get shorter, and then they alternate because

0:32:46.720 --> 0:32:48.680
<v Speaker 1>they're perpendicular to one another, and that's the way the

0:32:48.680 --> 0:32:52.480
<v Speaker 1>wave propagates across the facility. That's why you have an

0:32:52.600 --> 0:32:55.200
<v Speaker 1>l shape in the first place, because of that ninety

0:32:55.280 --> 0:32:58.840
<v Speaker 1>degree perpendicular alignment means one side is going to always

0:32:58.920 --> 0:33:00.840
<v Speaker 1>be getting shorter while the the one is getting longer

0:33:00.880 --> 0:33:04.360
<v Speaker 1>as a gravitational wave passes through. So that means that

0:33:04.560 --> 0:33:07.600
<v Speaker 1>while the wave is passing through, the laser on one

0:33:07.640 --> 0:33:10.520
<v Speaker 1>side is traveling a shorter distance than the laser on

0:33:10.560 --> 0:33:14.080
<v Speaker 1>the other side, and that ends up creating this mismatch

0:33:14.320 --> 0:33:18.040
<v Speaker 1>of wavelengths, and you get the light leaking through. The

0:33:18.120 --> 0:33:20.920
<v Speaker 1>light detector picks it up and and and then you've

0:33:20.920 --> 0:33:23.080
<v Speaker 1>got data to analyze and you can say, all right,

0:33:23.320 --> 0:33:27.080
<v Speaker 1>we've got a hit. Let's find out if our counterparts

0:33:27.120 --> 0:33:30.560
<v Speaker 1>at the other observatory also picked this up. And if

0:33:30.560 --> 0:33:34.040
<v Speaker 1>they did, then that's a potential gravitational wave. And it's

0:33:34.600 --> 0:33:38.760
<v Speaker 1>really elegant approach to detecting something like this, and it's

0:33:38.800 --> 0:33:43.240
<v Speaker 1>incredibly precise. So I was watching a video where one

0:33:43.240 --> 0:33:47.360
<v Speaker 1>of the engineers was talking about the measurements that are

0:33:47.440 --> 0:33:50.440
<v Speaker 1>made by this, and they said, when we talk about

0:33:50.440 --> 0:33:54.360
<v Speaker 1>differences in distance, we're talking about the distance of ten

0:33:54.520 --> 0:33:59.200
<v Speaker 1>to the minus nineteen power meters small. So again, you

0:33:59.240 --> 0:34:01.800
<v Speaker 1>take a take the number ten, take a decimal place,

0:34:02.200 --> 0:34:05.560
<v Speaker 1>moveing to the left nineteen times put meter behind it.

0:34:05.920 --> 0:34:08.680
<v Speaker 1>That's the distance we're talking about for uh. You know

0:34:08.800 --> 0:34:11.840
<v Speaker 1>that has to be measured when one of these gravitational

0:34:11.840 --> 0:34:15.640
<v Speaker 1>waves passes through, and they're passing through at a fraction

0:34:15.680 --> 0:34:21.680
<v Speaker 1>of a second, so it's incredibly precise, very fast measurement

0:34:21.760 --> 0:34:24.600
<v Speaker 1>that has to take place in order for even one

0:34:24.680 --> 0:34:27.680
<v Speaker 1>of the observatories to say we got a hit. But

0:34:27.840 --> 0:34:30.799
<v Speaker 1>as we mentioned earlier, if only one of them has

0:34:30.840 --> 0:34:33.480
<v Speaker 1>a hit, we know that that's probably a false positive.

0:34:33.680 --> 0:34:39.280
<v Speaker 1>It's probably a localized event in Louisiana or possibly Washington,

0:34:39.320 --> 0:34:42.360
<v Speaker 1>in which case it will make the news. In Louisiana

0:34:42.360 --> 0:34:45.320
<v Speaker 1>it's old hat, but in Washington that would be unusual.

0:34:45.960 --> 0:34:50.839
<v Speaker 1>Uh So, yeah, because they are so far apart by

0:34:51.360 --> 0:34:54.880
<v Speaker 1>specifically it's one thousand between the two or three thousand

0:34:54.920 --> 0:34:59.759
<v Speaker 1>two kilometers, that light does take a little longer to

0:35:00.000 --> 0:35:02.000
<v Speaker 1>it to one versus the other. It all depends on

0:35:02.000 --> 0:35:05.040
<v Speaker 1>what what direction the gravitational wave is coming from. But

0:35:05.239 --> 0:35:08.600
<v Speaker 1>there will be a delay. It's a tiny delay again,

0:35:08.760 --> 0:35:11.720
<v Speaker 1>less than ten milliseconds, but it's enough of a delay

0:35:11.760 --> 0:35:14.680
<v Speaker 1>that if there is that amount of time between the

0:35:14.680 --> 0:35:18.640
<v Speaker 1>two and they're picking up the same frequency wave or

0:35:18.680 --> 0:35:23.560
<v Speaker 1>same frequency in in this interference, then that suggests that

0:35:23.719 --> 0:35:27.359
<v Speaker 1>they found a gravitational wave. And now this kind of

0:35:27.400 --> 0:35:30.359
<v Speaker 1>precision means that they had to go through a little

0:35:30.360 --> 0:35:34.000
<v Speaker 1>bit of a growth period before they could really get

0:35:34.040 --> 0:35:37.600
<v Speaker 1>these things working. Yeah, so here's here's the bad news

0:35:37.680 --> 0:35:40.759
<v Speaker 1>they had to give. The facility came online in two

0:35:40.800 --> 0:35:45.759
<v Speaker 1>thousand two, by it was clear that the instrumentation they

0:35:45.760 --> 0:35:47.880
<v Speaker 1>were using was not going to be precise enough to

0:35:47.880 --> 0:35:50.440
<v Speaker 1>pick up gravitational waves. It didn't matter how long they

0:35:50.520 --> 0:35:55.200
<v Speaker 1>left it on, it was just not precise enough. And

0:35:55.280 --> 0:35:57.600
<v Speaker 1>they had to go back to the drawing board and say,

0:35:57.640 --> 0:36:00.040
<v Speaker 1>we're gonna need to upgrade these facilities in order for

0:36:00.239 --> 0:36:02.680
<v Speaker 1>them to be capable of detecting this. If in fact,

0:36:02.719 --> 0:36:06.720
<v Speaker 1>gravitational waves are a thing, then we're going and we

0:36:06.880 --> 0:36:08.640
<v Speaker 1>know that they are, but in order for us to

0:36:08.640 --> 0:36:11.480
<v Speaker 1>detect them, we're gonna have to get more precise. So

0:36:11.880 --> 0:36:16.000
<v Speaker 1>in twousen LIGO goes offline and there was an international

0:36:16.040 --> 0:36:21.160
<v Speaker 1>collaboration that took five years of work to overhaul and

0:36:21.360 --> 0:36:29.280
<v Speaker 1>upgrade LIGO until they got advanced LEGO or a. Yeah.

0:36:29.480 --> 0:36:33.200
<v Speaker 1>The observatories came back online in September two thou fifteen,

0:36:33.239 --> 0:36:38.480
<v Speaker 1>and literally days after turning on, they detected a gravitational wave.

0:36:39.239 --> 0:36:41.640
<v Speaker 1>So think about this for a second. The gravitational wave

0:36:41.680 --> 0:36:45.120
<v Speaker 1>they detected was from a pair of black holes colliding.

0:36:45.400 --> 0:36:49.200
<v Speaker 1>That pair of black holes collided one point three billion

0:36:49.600 --> 0:36:53.359
<v Speaker 1>years ago, and that means that the black holes were

0:36:53.480 --> 0:36:57.320
<v Speaker 1>by definition one point three billion light years away from Earth,

0:36:57.560 --> 0:37:01.799
<v Speaker 1>because again, gravitational waves travel at speed of light. So

0:37:02.600 --> 0:37:05.520
<v Speaker 1>one point three billion years ago, one point three billion

0:37:05.600 --> 0:37:09.960
<v Speaker 1>light years away, two black holes collided, and the facility

0:37:10.000 --> 0:37:15.000
<v Speaker 1>came online just days earlier at you know, on Earth

0:37:15.760 --> 0:37:20.200
<v Speaker 1>one point three billion years later. To catch it. That's

0:37:20.239 --> 0:37:25.120
<v Speaker 1>like the biggest dartboard you can imagine with the tiniest

0:37:25.120 --> 0:37:27.680
<v Speaker 1>bull's eye, and you are miles away and you just

0:37:27.760 --> 0:37:30.880
<v Speaker 1>happened to throw it perfectly well, so that catches the

0:37:30.920 --> 0:37:33.920
<v Speaker 1>air and flies over and hits that bull's eye. Now granted,

0:37:34.080 --> 0:37:36.800
<v Speaker 1>that is pretty amazing, but it's also it's a big universe.

0:37:36.960 --> 0:37:39.560
<v Speaker 1>Is a big universe, and people have said that things

0:37:39.600 --> 0:37:43.040
<v Speaker 1>like the black holes colliding events of that nature happened

0:37:43.040 --> 0:37:45.600
<v Speaker 1>in the universe on the order of about every fifteen minutes,

0:37:45.680 --> 0:37:48.080
<v Speaker 1>but it all depends on when and where they happened,

0:37:48.200 --> 0:37:51.160
<v Speaker 1>right like if it happened a billion years ago, but

0:37:51.239 --> 0:37:54.279
<v Speaker 1>it's four billion light years away, it will be three

0:37:54.320 --> 0:37:57.280
<v Speaker 1>billion more years before those gravitational waves make it to Earth.

0:37:57.920 --> 0:38:02.279
<v Speaker 1>So because the universe is big, yes, these things happen

0:38:02.320 --> 0:38:06.680
<v Speaker 1>all the time, but they don't hit Earth all the time. Yeah,

0:38:06.719 --> 0:38:08.799
<v Speaker 1>it was still pretty cool. Yeah, it's really really cool,

0:38:08.880 --> 0:38:11.560
<v Speaker 1>so cool that I remember on the day it was

0:38:11.600 --> 0:38:15.080
<v Speaker 1>announced one of the people working at Lego said, Yeah,

0:38:15.120 --> 0:38:17.360
<v Speaker 1>at first we thought that they might have been testing

0:38:17.400 --> 0:38:20.799
<v Speaker 1>the system again, and then we checked and no one

0:38:20.960 --> 0:38:25.160
<v Speaker 1>was testing the system and we were like, whoa, it works.

0:38:25.600 --> 0:38:28.800
<v Speaker 1>And so that was just one of those like great

0:38:29.280 --> 0:38:35.720
<v Speaker 1>fortuitous moments um and yeah, it was very exciting. Of course,

0:38:35.760 --> 0:38:38.080
<v Speaker 1>they wanted to take time to confirm it, to validate

0:38:38.080 --> 0:38:40.719
<v Speaker 1>the information, which is why we did not hear about

0:38:40.719 --> 0:38:45.200
<v Speaker 1>it till February eleven, twenty sixteen, so it was some

0:38:45.400 --> 0:38:48.520
<v Speaker 1>time later before we got a chance to find out

0:38:48.560 --> 0:38:50.680
<v Speaker 1>what the big discovery was. You know. One of the

0:38:50.680 --> 0:38:54.040
<v Speaker 1>cool things to me about this, uh, this observation, they

0:38:54.040 --> 0:38:57.160
<v Speaker 1>called it a chirp. Yeah, the thing that they detected

0:38:57.239 --> 0:39:00.640
<v Speaker 1>of the gravitational waves. And because it's a wave with

0:39:00.840 --> 0:39:04.120
<v Speaker 1>a certain number of number of oscillations per second represented

0:39:04.160 --> 0:39:08.120
<v Speaker 1>as hurts, you can actually represent this chirp as sound,

0:39:08.239 --> 0:39:12.200
<v Speaker 1>which people have done there. I watched one YouTube video

0:39:12.239 --> 0:39:16.000
<v Speaker 1>that was a compilation of different scientists and people who

0:39:16.000 --> 0:39:19.240
<v Speaker 1>were involved with the project doing doing little chirps, doing

0:39:19.239 --> 0:39:22.160
<v Speaker 1>their little gravitational wave of chirps with their mouths and

0:39:22.440 --> 0:39:24.799
<v Speaker 1>devices and stuff. I'm so glad I didn't make one

0:39:24.800 --> 0:39:26.520
<v Speaker 1>of those videos, would be so tempted just to do

0:39:26.560 --> 0:39:31.080
<v Speaker 1>the whole stupid Rick Roll thing. So the Louisiana Observatory

0:39:31.120 --> 0:39:35.319
<v Speaker 1>detected that gravitational wave first, and seven milliseconds later the

0:39:35.400 --> 0:39:39.319
<v Speaker 1>Washington Observatory detected it. So that's what when they were

0:39:39.360 --> 0:39:41.400
<v Speaker 1>able to say, yes, this does appear to be a

0:39:41.400 --> 0:39:45.359
<v Speaker 1>gravitational wave. And they used triangulation to determine where did

0:39:45.400 --> 0:39:47.759
<v Speaker 1>this come from, and they determined that it was coming

0:39:47.800 --> 0:39:51.480
<v Speaker 1>from the Southern hemisphere skies um and that's what led

0:39:51.520 --> 0:39:55.560
<v Speaker 1>them to the conclusion of hey, you know, we this

0:39:55.560 --> 0:39:58.680
<v Speaker 1>this is working. We understand where this is coming from

0:39:58.760 --> 0:40:01.480
<v Speaker 1>and even what's causing it, which was really cool, But

0:40:01.680 --> 0:40:03.680
<v Speaker 1>that wasn't all they were able to tell about it

0:40:03.719 --> 0:40:06.040
<v Speaker 1>from the data collected. In fact, they were able to

0:40:06.480 --> 0:40:09.080
<v Speaker 1>look at the data they had and say what they

0:40:09.160 --> 0:40:14.239
<v Speaker 1>think happened to cause these gravitational waves? Yeah, yeah, Like so,

0:40:14.360 --> 0:40:20.000
<v Speaker 1>let's it's hard to explain how huge a moment this is.

0:40:20.400 --> 0:40:23.120
<v Speaker 1>It's it's very difficult to kind of put that into words.

0:40:23.200 --> 0:40:27.279
<v Speaker 1>But keep in mind that black holes, while we understand

0:40:27.440 --> 0:40:31.560
<v Speaker 1>they are a thing, it's not something that we directly observe, right,

0:40:31.600 --> 0:40:35.120
<v Speaker 1>But you can't see a black hole, because that's rather

0:40:35.200 --> 0:40:37.279
<v Speaker 1>the point. Yeah, they really, you really can't. You can

0:40:37.320 --> 0:40:40.560
<v Speaker 1>see the effects off of them and nothing escapes from them.

0:40:40.640 --> 0:40:43.440
<v Speaker 1>So yeah, you can. You can see how gas clouds

0:40:43.480 --> 0:40:46.799
<v Speaker 1>behave in vicinity of you know, like in the Kessel run,

0:40:46.880 --> 0:40:50.120
<v Speaker 1>you see gravitational lensing. Yes, you can see gravitational lensing.

0:40:50.960 --> 0:40:55.120
<v Speaker 1>But you know, this is about as strong evidence for

0:40:55.200 --> 0:40:57.479
<v Speaker 1>the existence of black holes as you can get without

0:40:57.520 --> 0:41:02.920
<v Speaker 1>sending Matthew McConaughey through one um, and certainly the strongest

0:41:02.960 --> 0:41:06.480
<v Speaker 1>evidence for binary black holes where you have to colliding

0:41:06.520 --> 0:41:09.920
<v Speaker 1>with one another, and the data picked up matched the

0:41:10.040 --> 0:41:15.400
<v Speaker 1>calculations that that people had made based upon the knowledge

0:41:15.400 --> 0:41:18.279
<v Speaker 1>of general relativity in physics about what would happen with

0:41:18.320 --> 0:41:20.839
<v Speaker 1>these two black holes so well that it was phenomenal.

0:41:21.719 --> 0:41:24.040
<v Speaker 1>So reality and math were actually agreeing with one another,

0:41:24.080 --> 0:41:27.560
<v Speaker 1>which is fantastic. They determined the black holes in question

0:41:27.920 --> 0:41:31.560
<v Speaker 1>were pretty pretty big, not like super massive black holes.

0:41:31.600 --> 0:41:33.359
<v Speaker 1>We're not talking about the kind that would be at

0:41:33.360 --> 0:41:35.520
<v Speaker 1>the center of a galaxy or anything. But one had

0:41:35.560 --> 0:41:37.960
<v Speaker 1>twenty nine times the mass of our Sun and the

0:41:38.000 --> 0:41:41.080
<v Speaker 1>other thirty six times the Sun's mass, and right before

0:41:41.120 --> 0:41:44.160
<v Speaker 1>they collided, they were circling each other two and fifty

0:41:44.200 --> 0:41:48.080
<v Speaker 1>times a second UM. During the actual collision, which took

0:41:48.080 --> 0:41:51.240
<v Speaker 1>place over about a fifth of a second, they blogged

0:41:51.280 --> 0:41:54.960
<v Speaker 1>together and then coalesced into like a smooth sphere in

0:41:55.000 --> 0:42:00.120
<v Speaker 1>a process that's called ring down and ring down and

0:42:00.120 --> 0:42:04.080
<v Speaker 1>it's and it's this process in which three solar masses

0:42:04.280 --> 0:42:09.960
<v Speaker 1>worth of energy was vaporized that that caused the gravitational

0:42:10.000 --> 0:42:13.120
<v Speaker 1>waves that we observed um. The resulting black hole, by

0:42:13.120 --> 0:42:16.000
<v Speaker 1>the way, is therefore only sixty two times the mass

0:42:16.000 --> 0:42:19.840
<v Speaker 1>of the Sun, being that three masses just went. Yeah,

0:42:19.880 --> 0:42:22.840
<v Speaker 1>and when you think about energy equals mass times the

0:42:22.880 --> 0:42:27.520
<v Speaker 1>speed of light squared, and you think three solar masses vaporized,

0:42:29.200 --> 0:42:33.239
<v Speaker 1>that's that's an unimaginably huge amount of energy, right, Like

0:42:33.480 --> 0:42:36.120
<v Speaker 1>it's so enormous that I can't even begin to think

0:42:36.120 --> 0:42:38.520
<v Speaker 1>about it, so I won't. Yeah, yeah that but but yeah,

0:42:38.600 --> 0:42:41.800
<v Speaker 1>if you're wondering how something that was that far away

0:42:41.840 --> 0:42:46.280
<v Speaker 1>propagated all the way to Earth, that's why. So again

0:42:46.520 --> 0:42:50.360
<v Speaker 1>remarkable that this facility even picked up the signal in

0:42:50.400 --> 0:42:52.520
<v Speaker 1>the first place, considering that, you know, it all has

0:42:52.560 --> 0:42:55.560
<v Speaker 1>to be timed out where this thing that happened one

0:42:55.560 --> 0:42:58.319
<v Speaker 1>point three billion years ago, one point three billion light

0:42:58.400 --> 0:43:03.480
<v Speaker 1>years away. Uh, just the observatory coming online when it did,

0:43:03.640 --> 0:43:06.680
<v Speaker 1>like all of that is pretty phenomenal stuff. Yeah, and

0:43:06.719 --> 0:43:09.880
<v Speaker 1>they almost didn't do the engineering run during which the

0:43:09.880 --> 0:43:14.160
<v Speaker 1>signal was found. Uh, just three days prior, the Livingstone

0:43:14.200 --> 0:43:18.239
<v Speaker 1>antenna was getting some radio interference and White actually recommended

0:43:18.280 --> 0:43:20.480
<v Speaker 1>that they put off the run. But his colleagues they're

0:43:20.480 --> 0:43:23.520
<v Speaker 1>were like, Nah, let's let's go ahead. We think it's ready,

0:43:23.640 --> 0:43:26.520
<v Speaker 1>so don't worry about it. The nice thing is that

0:43:26.600 --> 0:43:30.319
<v Speaker 1>we know eventually this would have worked anyway, but it

0:43:30.360 --> 0:43:33.120
<v Speaker 1>was still just just one of those cool stories about

0:43:33.160 --> 0:43:36.360
<v Speaker 1>how much came into alignment to allow it to happen

0:43:36.480 --> 0:43:40.080
<v Speaker 1>so early. When it came back online, it's a great

0:43:40.120 --> 0:43:42.560
<v Speaker 1>story for science. Well. One of the things that I

0:43:42.640 --> 0:43:45.800
<v Speaker 1>have definitely heard reported from some of the people involved

0:43:45.840 --> 0:43:48.440
<v Speaker 1>in the project is that the signal was much stronger

0:43:48.480 --> 0:43:51.600
<v Speaker 1>than they expected it to be. Like they they were

0:43:51.640 --> 0:43:55.440
<v Speaker 1>able to see the signal clearly in the data with

0:43:55.520 --> 0:43:58.160
<v Speaker 1>the naked eye just looking at the data. They're like, oh,

0:43:58.200 --> 0:44:00.520
<v Speaker 1>there it is. When what they thought they we're gonna

0:44:00.560 --> 0:44:03.760
<v Speaker 1>have to do was like run a you know, computational

0:44:03.840 --> 0:44:07.520
<v Speaker 1>analysis across all the data and compare it to uh

0:44:07.520 --> 0:44:10.920
<v Speaker 1>to random noise generated as a sort of cross reference,

0:44:11.000 --> 0:44:14.239
<v Speaker 1>and see if it maybe was a gravitational wave. But no,

0:44:14.360 --> 0:44:18.920
<v Speaker 1>it was just obvious, which is amazing. And so this

0:44:19.000 --> 0:44:22.920
<v Speaker 1>is kind of wrapping up our initial discussion about gravitational waves.

0:44:23.239 --> 0:44:25.200
<v Speaker 1>In our next episode, we're gonna talk a little bit

0:44:25.200 --> 0:44:27.799
<v Speaker 1>more about the specifics of what Lego found. I'm gonna

0:44:27.840 --> 0:44:31.160
<v Speaker 1>talk a little bit about some angular momentum. In that episode,

0:44:31.200 --> 0:44:34.360
<v Speaker 1>we'll also talk about what does this mean and the

0:44:34.480 --> 0:44:38.680
<v Speaker 1>rise of a new type of astronomy, gravitational astronomy, which

0:44:38.719 --> 0:44:43.160
<v Speaker 1>is literally in its infancy right now. Uh and what

0:44:43.239 --> 0:44:47.640
<v Speaker 1>could this possibly mean for the future? That will be

0:44:47.640 --> 0:44:50.000
<v Speaker 1>in our next episode. Guys, if you have suggestions for

0:44:50.080 --> 0:44:53.680
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0:44:58.760 --> 0:45:02.279
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0:45:02.280 --> 0:45:07.480
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0:45:07.480 --> 0:45:10.200
<v Speaker 1>sushi in Atlanta. That's all I'm saying. Now, send us

0:45:10.239 --> 0:45:15.360
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0:45:34.760 --> 0:45:37.200
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