WEBVTT - Hitting the Road with GPS

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<v Speaker 1>Welcome to Tech Stuff, a production from iHeartRadio. Hey there,

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<v Speaker 1>and welcome to tech Stuff. I'm your host, Jonathan Strickland.

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<v Speaker 1>I'm an executive producer with iHeart Podcasts and how the

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<v Speaker 1>tech are you so, y'all. I love to travel. I

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<v Speaker 1>love to visit new places or revisit ones after I've

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<v Speaker 1>been away for a long time. I even don't really

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<v Speaker 1>mind the journey part of travel, which can often be

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<v Speaker 1>you know, stressful, in a hassle if things aren't going well.

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<v Speaker 1>One thing that does give me a huge amount of

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<v Speaker 1>anxiety if I'm traveling is just getting lost or even

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<v Speaker 1>the thought of getting lost. I do not do very

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<v Speaker 1>well with that. There's some part of my brain that

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<v Speaker 1>mistakenly believes that as long as I know where I am,

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<v Speaker 1>nothing can go too wrong. And boy I wish that

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<v Speaker 1>were true, but but yeah, whatever, I just need my

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<v Speaker 1>brain to let me function properly when I'm out on holidays.

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<v Speaker 1>So I remember traveling on my honeymoon to London. At

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<v Speaker 1>that point, I had never been outside the United States before.

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<v Speaker 1>This was my first trip outside the country, and I

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<v Speaker 1>was going to a city that I had read about extensively.

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<v Speaker 1>I knew a lot about London. My major in college

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<v Speaker 1>was in English literature, but it was with a focus

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<v Speaker 1>on medieval studies, so things had changed slightly by the

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<v Speaker 1>time I got there, and reading about a city is

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<v Speaker 1>very different from actually walking around one. Also, my honeymoon

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<v Speaker 1>was in the nineteen nineties because I'm old, and that

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<v Speaker 1>meant I was a decade out from the era of smartphones,

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<v Speaker 1>so I didn't have a handy mobile device to tell

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<v Speaker 1>me where I was as I wandered around the city.

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<v Speaker 1>Even if smartphones had been around back then, I wouldn't

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<v Speaker 1>have been able to rely on map apps on the

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<v Speaker 1>smartphone because of something called selective availability. More on that

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<v Speaker 1>in a bit, but at any rate, I had to

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<v Speaker 1>rely on physical maps to get around and hope that

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<v Speaker 1>I didn't mess it up too badly. Yeah, it's like

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<v Speaker 1>the Stone Age right. Well, these days, as long as

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<v Speaker 1>I have my smartphone with me and I'm not buried

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<v Speaker 1>under a mountain or something, I feel fairly confident I'm

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<v Speaker 1>not going to get lost. If I'm going somewhere that

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<v Speaker 1>has limited connectivity, like limited view of the sky, then

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<v Speaker 1>my anxiety starts to creep in again. But usually I'm okay,

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<v Speaker 1>and that's thanks to the Global Positioning System or GPS.

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<v Speaker 1>So today we're going to learn about GPS, what makes

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<v Speaker 1>it work, how the technology has to take into account,

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<v Speaker 1>Einstein's theories of relativity and more. And a huge thank

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<v Speaker 1>to JP Morgan, Chase Bank, and the United Explorer Card

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<v Speaker 1>for sponsoring this episode. We'll hear more about them later too.

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<v Speaker 1>So GPS, well, that story begins back in the nineteen

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<v Speaker 1>teen fifties when the United States and the then Soviet

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<v Speaker 1>Union were locked in a Cold war, and that cold

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<v Speaker 1>war manifested in many different ways, including an effort to

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<v Speaker 1>launch vehicles into space. For one thing, if you could

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<v Speaker 1>launch a rocket into orbit, then you could show your

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<v Speaker 1>technological superiority over your opponent and say, look how much

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<v Speaker 1>further advanced we are compared to you. But you could

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<v Speaker 1>also send the message of hey, if I can send

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<v Speaker 1>a rocket to space, I could send a rocket to

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<v Speaker 1>your front door, all the way from across the world,

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<v Speaker 1>and it could be carrying a heck of a boom boom.

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<v Speaker 1>Now this gram message underpinned what would become the space race.

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<v Speaker 1>But the space race also meant that brilliant engineers and

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<v Speaker 1>scientists would actually get the resources they needed to advance

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<v Speaker 1>technology by incredible leaps and bounds over the following decades.

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<v Speaker 1>So you got to take the good with the bad, right.

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<v Speaker 1>The good part is you suddenly had actual financial support

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<v Speaker 1>for or incredibly important scientific and engineering work. The bad is, well,

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<v Speaker 1>it was all done in service of this perceived rivalry

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<v Speaker 1>with this massive country on the other side of the globe.

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<v Speaker 1>On October fourth, nineteen fifty seven, at approximately seven thirty pm,

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<v Speaker 1>the USSR launched the first man made satellite into orbit, Sputnik.

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<v Speaker 1>Non past episodes, I have referred to the satellite as

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<v Speaker 1>the ball that went beep. That's not exactly inaccurate. The

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<v Speaker 1>satellite was spherical in shape. It did have these long

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<v Speaker 1>antenna extending out the back of it, so it kind

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<v Speaker 1>of looks like a comet, like a silver comet. But

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<v Speaker 1>the antenna transmitted short radio pulses, and these pulses could

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<v Speaker 1>be picked up very easily by ground based audio receivers,

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<v Speaker 1>including radio sets operated by amateurs, just an amateur radio set.

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<v Speaker 1>This meant that Sputnik's existence couldn't be kept a secret

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<v Speaker 1>because if you or someone you knew operated a radio,

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<v Speaker 1>you could learn about the thing. And in the United States,

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<v Speaker 1>it prompted no small amount of anxiety. Americans believed their

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<v Speaker 1>country was well ahead of the Soviet Union, at least

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<v Speaker 1>on a technological basis. But here they could see that

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<v Speaker 1>their adversary had launched stuff into space and did it

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<v Speaker 1>before the US could do it. That really kicked things

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<v Speaker 1>into gear here in the United States. But I would

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<v Speaker 1>argue that Sputnik would ultimately plant a seed that would

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<v Speaker 1>blossom into GPS further down the line, because here you

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<v Speaker 1>had a satellite sending regular radio signals to Earth, and

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<v Speaker 1>those signals were pretty primitive. Essentially, the satellite was signaling

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<v Speaker 1>that it was within range overhead, along with basic information

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<v Speaker 1>about stuff like air pressure and temperature indicated by the

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<v Speaker 1>length of the radio pulses. Like the pulses didn't give

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<v Speaker 1>data the way Wi Fi does. Literally, you would measure

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<v Speaker 1>how long the pulse lasted and that would tell you, oh,

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<v Speaker 1>the temperature is whatever, if you happen to have the chart.

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<v Speaker 1>Two scientists were able to adfer other information, however, from

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<v Speaker 1>this signal, such as how the propagation of radio signals

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<v Speaker 1>interacted in the upper atmosphere like the ionosphere, and it

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<v Speaker 1>hinted that there could be other uses for as satellite

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<v Speaker 1>beaming information down to Earth. Also, those signals were subject

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<v Speaker 1>to what we call the Doppler effect. It's named after

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<v Speaker 1>Christian Doppler effect. No, I'm sorry, it's just Christian Doppler.

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<v Speaker 1>He first observed this effect back in eighteen forty two.

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<v Speaker 1>And this is how the frequency of a wave changes

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<v Speaker 1>relative to an independent observer if the thing that's emitting

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<v Speaker 1>the wave is moving toward or away from that observer.

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<v Speaker 1>Which was a clumsy explanation, Let's just take an example

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<v Speaker 1>because that makes it way more clear. So let's say

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<v Speaker 1>you're just walking down the street. You're on a sidewalk,

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<v Speaker 1>and say one hundred feet or so in front of you,

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<v Speaker 1>there's an emergency vehicle and it's parked. It's not currently

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<v Speaker 1>driving anywhere, but it is running its siren. The sound

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<v Speaker 1>of that siren is going to remain consistent relative to you, right,

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<v Speaker 1>it may increase and decrease in pitch because the nature

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<v Speaker 1>of the siren, but it's going to keep doing that

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<v Speaker 1>pattern over and over again. But now let's say that

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<v Speaker 1>it's an emergency vehicle that's rushing off away from you.

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<v Speaker 1>It's driving off. You'll notice the pitch of the siren

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<v Speaker 1>will start to go lower. The frequency of the sound

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<v Speaker 1>wave decreases as the vehicle accelerates away from you, or

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<v Speaker 1>let's say the vehicle is driving towards you, the pitch

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<v Speaker 1>of the siren will go up as the frequency increases.

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<v Speaker 1>You can kind of think of it like this. An

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<v Speaker 1>approaching object emitting a wave is effectively pushing or compressing

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<v Speaker 1>that wave as it moves closer to you. An object

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<v Speaker 1>moving away from you is stretching out the wave it's

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<v Speaker 1>emitting as it moves away from you. That is the

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<v Speaker 1>Doppler effect. Scientists at the Applied Physics Laboratory or APL,

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<v Speaker 1>at Johns Hopkins University noticed that the Doppler effect was

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<v Speaker 1>also applicable to Sputnik's radio waves. The satellite's radio pulses

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<v Speaker 1>were compressed as Sputnik would approach, and then they would

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<v Speaker 1>stretch out as the satellite would move away from their

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<v Speaker 1>point of observation, and this meant that just by listening

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<v Speaker 1>to the pulses, the scientists could track Sputnik's movements. They

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<v Speaker 1>didn't need to have eyes on the satellite to track it.

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<v Speaker 1>They could just follow the pulses and observe the Doppler

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<v Speaker 1>effect in order to know generally where it was and

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<v Speaker 1>when it was heading away, but very generally, like they

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<v Speaker 1>couldn't give you a pinpointed location. However, this was another

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<v Speaker 1>important seed for what would become GPS, because it would

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<v Speaker 1>lead to the hypothesis that a satellite could send signals

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<v Speaker 1>to a receiver on Earth, and if that receiver quote

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<v Speaker 1>unquote knew how far away the satellite was from the receiver,

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<v Speaker 1>you could determine the location of that receiver on Earth.

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<v Speaker 1>You would need to be able to get signals from

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<v Speaker 1>more than one satellite, however, to do that, otherwise, you

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<v Speaker 1>would really just know how far away you were from

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<v Speaker 1>one satellite. But that's not really useful information because it

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<v Speaker 1>doesn't narrow stuff down enough, or to put it in

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<v Speaker 1>another way, let's say, let's take this to two dimensions.

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<v Speaker 1>So let's talk about a map. Let's say you've got

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<v Speaker 1>a map of North Georgia, Okay, because that's where I live.

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<v Speaker 1>And I could say, hey, I live twenty miles away

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<v Speaker 1>from my parents. And let's say you happen to know

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<v Speaker 1>where I live. Not that I'm gonna dox myself, but

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<v Speaker 1>let's say you know where I live, so you can

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<v Speaker 1>take that point on the map you could draw out

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<v Speaker 1>a line that's twenty miles out and then create a

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<v Speaker 1>circle with a radius of twenty miles but without more information,

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<v Speaker 1>that could mean they could be anywhere along that circumference

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<v Speaker 1>of the circle right in a radius of twenty miles

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<v Speaker 1>from me. They could be east or west, or north

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<v Speaker 1>or south, or any point in between, as long as

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<v Speaker 1>it was twenty miles out from my location. We'll come

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<v Speaker 1>back to this analogy in a little bit. Let's get

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<v Speaker 1>back to the Doppler effect. It could all be used

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<v Speaker 1>to get a more accurate location. If you know where

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<v Speaker 1>the satellite is as you receive signals, you can use

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<v Speaker 1>a series of pulses from that satellite to determine your

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<v Speaker 1>location on Earth. This actually takes a bit, right. So

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<v Speaker 1>if you know where a satellite is as it's beaming

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<v Speaker 1>down these radio pulses to you, and you are able

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<v Speaker 1>to get a sequence of measurements, and you're taking the

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<v Speaker 1>Doppler effect into account, and you have all this information

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<v Speaker 1>available to you, you can then use that info to

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<v Speaker 1>reckon where you are on Earth. You have to keep

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<v Speaker 1>receiving signals as the satellite is moving through its orbit

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<v Speaker 1>and then use the series of data pulses to track

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<v Speaker 1>where you are on Earth. If a satellite isn't within range,

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<v Speaker 1>then you have to wait until one is close enough

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<v Speaker 1>to you for you to start picking up the signals.

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<v Speaker 1>That could be up to an hour, depending upon when

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<v Speaker 1>the last one passed overhead, but it would work. So

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<v Speaker 1>this would become a very early satellite based navigation system

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<v Speaker 1>for the US Navy. So back to our history lesson.

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<v Speaker 1>Following Sputnik's incredible impact both figuratively and then semi literally,

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<v Speaker 1>because it would burn up upon descending through the Earth's

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<v Speaker 1>atmosphere about three months and more than fourteen hundred orbits

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<v Speaker 1>after initial launch, the US Advanced Research Projects Agency, or

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<v Speaker 1>ARPA got to work on funding research for a satellite

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<v Speaker 1>navigation system that would be called TRANSIT. Today we call

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<v Speaker 1>ARPA DARPA, and it's a branch of the US Department

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<v Speaker 1>of Defense that offers contracts to various organizations and companies

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<v Speaker 1>to advance technologies that would be potentially useful in national defense.

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<v Speaker 1>It's the agency that's responsible for bringing together the folks

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<v Speaker 1>who actually built the infrastructure for the Internet. It's also

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<v Speaker 1>largely responsible for the initial boom in autonomous vehicle research. Anyway,

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<v Speaker 1>Transit would be handy for the United States Navy. The

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<v Speaker 1>boffins over at Johns Hopkins University APL designed the satellites,

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<v Speaker 1>which were intend to provide location information on Earth and

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<v Speaker 1>in the Earth's socians, to an accuracy of within tens

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<v Speaker 1>of meters, which thay sounds pretty loosey goosey, right, Like,

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<v Speaker 1>if you were tens of meters away from your location

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<v Speaker 1>based upon the app you would think, wow, this is

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<v Speaker 1>not very useful. But at the time it was significantly

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<v Speaker 1>more accurate than what we had been used to, So

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<v Speaker 1>we were able to use this for mapping purposes and

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<v Speaker 1>it was really handy. It would allow for far more precision,

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<v Speaker 1>and it proved beyond a shadow of a doubt that

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<v Speaker 1>England is not a conspiracy among cartographers and shout out

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<v Speaker 1>to me if you actually recognize that reference. The first

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<v Speaker 1>attempt to get a Transit satellite into orbit was a failure.

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<v Speaker 1>As Monty Python might put it, it sank into the swamp,

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<v Speaker 1>but it did not take four tries to get it right.

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<v Speaker 1>Transit one B successfully achieved orbit on April thirteenth, nineteen sixty.

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<v Speaker 1>It passed test with orbiting colors, but it would take

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<v Speaker 1>more satellites. To create a system that would be useful

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<v Speaker 1>and reliable, you needed a group of them, or a

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<v Speaker 1>constellation of satellites in other words, and that's what we

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<v Speaker 1>call a collection of satellites that collectively provide some specific

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<v Speaker 1>information or service. It's a constellation anyway. By the mid

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<v Speaker 1>nineteen sixties, the US launched several satellites into orbit, and

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<v Speaker 1>this orbital path took the satellites past the Earth's poles,

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<v Speaker 1>and once there were six satellites making up a very

0:13:27.760 --> 0:13:30.959
<v Speaker 1>small constellation. The Navy would use those satellites and the

0:13:31.000 --> 0:13:34.040
<v Speaker 1>Doppler effect to keep track of US subs that happen

0:13:34.080 --> 0:13:37.160
<v Speaker 1>to be carrying big old boom booms on them, like

0:13:37.520 --> 0:13:40.360
<v Speaker 1>the nuclear kind of boom booms. When you're on a

0:13:40.400 --> 0:13:43.600
<v Speaker 1>submersible that happens to be outfitted with nuclear weaponry, you

0:13:43.679 --> 0:13:46.120
<v Speaker 1>want to keep an accurate account of where you are

0:13:46.280 --> 0:13:50.120
<v Speaker 1>and where you're going, and more importantly, the country that's

0:13:50.120 --> 0:13:52.400
<v Speaker 1>in charge of you wants to know where you are,

0:13:52.640 --> 0:13:56.880
<v Speaker 1>because if you suddenly disappear, that's a huge problem. Using transit,

0:13:56.920 --> 0:14:00.240
<v Speaker 1>the subs could gain accurate location reading from satellite in

0:14:00.400 --> 0:14:03.079
<v Speaker 1>just a few minutes, which again was a huge improvement

0:14:03.240 --> 0:14:08.360
<v Speaker 1>over simply using map making and plotting. I mean, there

0:14:08.400 --> 0:14:11.640
<v Speaker 1>are people who are phenomenal at figuring out where a

0:14:11.679 --> 0:14:16.040
<v Speaker 1>submarine is based upon knowing the heading and how long

0:14:16.280 --> 0:14:19.960
<v Speaker 1>a sub was traveling in that direction. I marvel at

0:14:20.000 --> 0:14:24.680
<v Speaker 1>it when I see films of navigators doing those kind

0:14:24.720 --> 0:14:28.480
<v Speaker 1>of calculations. But the nice thing is this would allow

0:14:28.600 --> 0:14:33.200
<v Speaker 1>for relatively quick and accurate results, assuming that you were

0:14:33.280 --> 0:14:37.800
<v Speaker 1>within range of receiving a satellite signal. The US Navy

0:14:37.800 --> 0:14:41.040
<v Speaker 1>took over the operation of these satellites from ARPA by

0:14:41.160 --> 0:14:44.240
<v Speaker 1>the mid nineteen sixties, and by nineteen sixty eight the

0:14:44.280 --> 0:14:47.720
<v Speaker 1>system had a total of thirty six satellites in orbit.

0:14:48.280 --> 0:14:50.480
<v Speaker 1>While the primary function of the system was to keep

0:14:50.560 --> 0:14:53.920
<v Speaker 1>tabs on nuclear armed submarines, researchers also used it to

0:14:53.920 --> 0:14:56.360
<v Speaker 1>map out locations, including using it to get a more

0:14:56.480 --> 0:14:59.720
<v Speaker 1>accurate measurement of Mount Everest's elevation, which I thought was

0:14:59.760 --> 0:15:02.920
<v Speaker 1>pretty neat. Now. That was in the nineteen sixties and

0:15:03.040 --> 0:15:06.360
<v Speaker 1>nineteen seventies, and transit would remain in operation until nineteen

0:15:06.440 --> 0:15:09.640
<v Speaker 1>ninety six, at which point it was retired for navigational

0:15:09.680 --> 0:15:14.480
<v Speaker 1>purposes anyway, in favor of GPS, which had come online

0:15:14.520 --> 0:15:18.680
<v Speaker 1>not long before that, actually, but we've still got some

0:15:18.720 --> 0:15:21.960
<v Speaker 1>steps in between that we're going to need to talk about.

0:15:22.000 --> 0:15:25.160
<v Speaker 1>So while Transit was taking shape with occasional launches to

0:15:25.160 --> 0:15:28.560
<v Speaker 1>build out its constellation, another team over at the Aerospace

0:15:28.600 --> 0:15:33.240
<v Speaker 1>Corporation was developing a more advanced navigational satellite system. Among

0:15:33.280 --> 0:15:40.200
<v Speaker 1>the scientists and engineers was Ivan getting Hideyoshi Nakamura, James Woodford,

0:15:40.320 --> 0:15:42.760
<v Speaker 1>and Philip Diamond, and they figured out that with a

0:15:42.840 --> 0:15:46.120
<v Speaker 1>large enough constellation of satellites, with each satellite carrying an

0:15:46.200 --> 0:15:50.000
<v Speaker 1>incredibly accurate clock on board, you could provide even more

0:15:50.040 --> 0:15:53.720
<v Speaker 1>accurate positional information to a receiver on Earth. What's more,

0:15:53.960 --> 0:15:57.280
<v Speaker 1>the receiver itself wouldn't need to be a super accurate clock.

0:15:57.720 --> 0:15:59.880
<v Speaker 1>The clocks would just be on the satellites, and this

0:16:00.040 --> 0:16:04.720
<v Speaker 1>would dramatically reduce the cost of building out receivers on land.

0:16:04.960 --> 0:16:08.200
<v Speaker 1>Like before, if the receiver on land needed to have

0:16:08.640 --> 0:16:12.920
<v Speaker 1>an incredibly accurate clock as well as the satellite, then

0:16:13.080 --> 0:16:16.320
<v Speaker 1>the cost would have been prohibitive for the average person.

0:16:16.760 --> 0:16:21.000
<v Speaker 1>But this brought all the onus of time keeping onto

0:16:21.040 --> 0:16:23.400
<v Speaker 1>the satellite site, not the receiver side, and it made

0:16:23.400 --> 0:16:27.040
<v Speaker 1>it much much more affordable. So you still need those

0:16:27.080 --> 0:16:29.600
<v Speaker 1>clocks in the satellites themselves, but the receivers on Earth

0:16:29.640 --> 0:16:33.200
<v Speaker 1>could be drastically simplified and manageurized and again accurate reading

0:16:33.240 --> 0:16:36.320
<v Speaker 1>on position. A receiver would need to connect with four satellites,

0:16:36.360 --> 0:16:39.040
<v Speaker 1>so the constellation of navigational spacecraft would need to be

0:16:39.120 --> 0:16:42.000
<v Speaker 1>fairly large in order to be able to receive signals

0:16:42.000 --> 0:16:45.520
<v Speaker 1>from four satellites simultaneously. But those four satellites would give

0:16:45.600 --> 0:16:49.280
<v Speaker 1>enough information to really hone in on the receiver's location

0:16:49.760 --> 0:16:52.200
<v Speaker 1>here on Earth. So what we're going to do now

0:16:52.280 --> 0:16:54.000
<v Speaker 1>is we're going to take a quick break to thank

0:16:54.080 --> 0:16:56.480
<v Speaker 1>our sponsor, and then when we come back, I'll talk

0:16:56.560 --> 0:17:00.960
<v Speaker 1>more about how this works, like how state lights are

0:17:01.320 --> 0:17:04.040
<v Speaker 1>able to send information that a receiver on Earth can

0:17:04.080 --> 0:17:08.320
<v Speaker 1>take and interpret as positional information on the surface of

0:17:08.320 --> 0:17:21.240
<v Speaker 1>the planet. But first let's take this quick break, all right.

0:17:21.320 --> 0:17:23.640
<v Speaker 1>I think it's best we now take time to talk

0:17:23.640 --> 0:17:27.040
<v Speaker 1>about how all this works, and that's what we've been

0:17:27.040 --> 0:17:29.960
<v Speaker 1>building towards. So remember when I said my parents live

0:17:30.400 --> 0:17:34.040
<v Speaker 1>like twenty miles away from me, and that just tells

0:17:34.080 --> 0:17:36.800
<v Speaker 1>you that they're somewhere within a twenty mile radius of

0:17:36.880 --> 0:17:40.239
<v Speaker 1>my location. That's that's all it tells you. But if

0:17:40.280 --> 0:17:42.800
<v Speaker 1>I gave you another data point. Let's say that I said, oh,

0:17:42.840 --> 0:17:46.400
<v Speaker 1>they happen to live seventy miles from Athens, Georgia. Well,

0:17:46.440 --> 0:17:48.679
<v Speaker 1>now you can take a map and draw two circles,

0:17:48.760 --> 0:17:51.640
<v Speaker 1>assuming you know where I live. So one circle would

0:17:51.640 --> 0:17:54.919
<v Speaker 1>be centered on my location with a twenty mile radius

0:17:54.960 --> 0:17:59.280
<v Speaker 1>around it. The second circle would be around Athens, Georgia

0:17:59.359 --> 0:18:02.080
<v Speaker 1>at the center. It would extend out seventy miles. So

0:18:02.119 --> 0:18:05.399
<v Speaker 1>these two circles would overlap slightly. They kind of cross

0:18:05.520 --> 0:18:08.080
<v Speaker 1>one another at two points, kind of like a ven diagram.

0:18:08.200 --> 0:18:10.600
<v Speaker 1>And now you've narrowed down my parents' house to one

0:18:10.720 --> 0:18:14.199
<v Speaker 1>of two possible points. Because where they live needs to

0:18:14.200 --> 0:18:16.880
<v Speaker 1>be within twenty miles of me and seventy miles of Athens.

0:18:16.920 --> 0:18:19.880
<v Speaker 1>That only leaves two locations on the map. Now, unless

0:18:19.880 --> 0:18:21.840
<v Speaker 1>one of those points happens to be somewhere where a

0:18:21.880 --> 0:18:24.840
<v Speaker 1>house could not possibly be located, like in the middle

0:18:24.880 --> 0:18:28.120
<v Speaker 1>of a lake or something, they're still ambiguity. You don't

0:18:28.160 --> 0:18:31.320
<v Speaker 1>know if they're in location one or location two. Ah.

0:18:31.560 --> 0:18:34.240
<v Speaker 1>But what if I also said my parents live within

0:18:34.760 --> 0:18:38.080
<v Speaker 1>or ten miles away from the amusement park six lags

0:18:38.080 --> 0:18:40.800
<v Speaker 1>over Georgia. Well, you could draw a third circle with

0:18:40.880 --> 0:18:43.720
<v Speaker 1>a radius of ten miles around that park, and you

0:18:43.760 --> 0:18:46.440
<v Speaker 1>should see that this circle intersects with the other two

0:18:46.600 --> 0:18:50.480
<v Speaker 1>already drawn at a single point. They three circles meet

0:18:50.600 --> 0:18:53.639
<v Speaker 1>only in one location, and that is where my parents

0:18:53.680 --> 0:18:56.359
<v Speaker 1>would live, or it would be if I weren't giving

0:18:56.840 --> 0:19:00.800
<v Speaker 1>total made up answers to these different distances. For one thing,

0:19:00.880 --> 0:19:03.760
<v Speaker 1>I don't think you could have circles that overlap seventy

0:19:03.840 --> 0:19:06.280
<v Speaker 1>miles out from Athens and ten miles out from six Legs.

0:19:06.280 --> 0:19:09.720
<v Speaker 1>They're too far apart. But you get the idea. GPS

0:19:09.760 --> 0:19:12.199
<v Speaker 1>satellites work in a similar way, except we need to

0:19:12.200 --> 0:19:15.720
<v Speaker 1>think about spheres rather than circles. We have to go

0:19:15.760 --> 0:19:19.280
<v Speaker 1>into three dimensions, right, So a GPS satellite essentially sends

0:19:19.280 --> 0:19:22.200
<v Speaker 1>out a pulse of data and it indicates a time

0:19:22.320 --> 0:19:26.400
<v Speaker 1>stamp and the satellite's location. A receiver on Earth receives

0:19:26.480 --> 0:19:28.840
<v Speaker 1>this message and by doing a little math, figures out

0:19:29.040 --> 0:19:33.280
<v Speaker 1>how far away it is from the satellite by knowing

0:19:33.320 --> 0:19:35.879
<v Speaker 1>how long it took the message to travel from the

0:19:35.920 --> 0:19:38.800
<v Speaker 1>satellite to the receiver. These pulses are traveling at the

0:19:38.800 --> 0:19:41.560
<v Speaker 1>speed of light, so we actually do know the velocity

0:19:41.720 --> 0:19:44.680
<v Speaker 1>or the speed rather of those signals. So we've got

0:19:44.800 --> 0:19:48.360
<v Speaker 1>time and we've got speed. We need to figure out

0:19:48.480 --> 0:19:52.680
<v Speaker 1>the distance to know how far the receiver is from

0:19:52.720 --> 0:19:56.919
<v Speaker 1>the specific satellite, and we can eliminate all the positions

0:19:57.240 --> 0:20:00.880
<v Speaker 1>that aren't on Earth. Right once we figure out, oh,

0:20:00.880 --> 0:20:03.320
<v Speaker 1>it took x amount of time to get here, that

0:20:03.359 --> 0:20:06.800
<v Speaker 1>means where why number of miles away from the satellite

0:20:06.880 --> 0:20:09.600
<v Speaker 1>we happen to know where the satellite is located, you

0:20:09.640 --> 0:20:14.480
<v Speaker 1>could create a sphere representing all the points around the

0:20:14.480 --> 0:20:17.480
<v Speaker 1>satellite that are the proper distance away. A lot of

0:20:17.520 --> 0:20:19.600
<v Speaker 1>those points are going to be out in space. We

0:20:19.680 --> 0:20:23.359
<v Speaker 1>can disregard those because obviously we're not in outer space.

0:20:23.720 --> 0:20:26.439
<v Speaker 1>But for the ones that are on Earth, there's going

0:20:26.480 --> 0:20:28.320
<v Speaker 1>to be a lot, right, Some are going to actually

0:20:28.320 --> 0:20:32.359
<v Speaker 1>extend into the Earth. We can probably dismiss those as well.

0:20:32.640 --> 0:20:34.640
<v Speaker 1>So we're just looking at the ones that actually intersect

0:20:34.680 --> 0:20:37.439
<v Speaker 1>with the surface of the Earth. But there's still a lot,

0:20:37.600 --> 0:20:39.840
<v Speaker 1>so we have to narrow it down. We do that

0:20:40.240 --> 0:20:46.480
<v Speaker 1>by receiving multiple signals from multiple satellites, preferably for satellites

0:20:46.560 --> 0:20:49.679
<v Speaker 1>to really get rid of any ambiguity. If the receiver

0:20:49.760 --> 0:20:52.920
<v Speaker 1>does this with at least three but typically four satellites.

0:20:52.920 --> 0:20:55.080
<v Speaker 1>Then it can pinpoint where on the surface of the

0:20:55.119 --> 0:20:58.200
<v Speaker 1>Earth the receiver happens to be. It's a clever way

0:20:58.200 --> 0:21:01.040
<v Speaker 1>to figure out locations because once we do figure out all, right,

0:21:01.080 --> 0:21:05.159
<v Speaker 1>where why number of miles from satellite A, where Z

0:21:05.359 --> 0:21:08.439
<v Speaker 1>number of miles from satellite B, where AA number of

0:21:08.480 --> 0:21:13.840
<v Speaker 1>miles or satellite three and BB from satellite four, you

0:21:14.080 --> 0:21:16.600
<v Speaker 1>create the spheres around all four of those satellites. You

0:21:16.640 --> 0:21:18.440
<v Speaker 1>know where they are, they've told you where they are.

0:21:18.480 --> 0:21:21.080
<v Speaker 1>You know what time stamps you're looking at. The time

0:21:21.119 --> 0:21:24.720
<v Speaker 1>stamps also need to be in sync with the receiver's clock,

0:21:24.800 --> 0:21:27.040
<v Speaker 1>but the receiver's clock can be modified here on Earth.

0:21:27.040 --> 0:21:29.080
<v Speaker 1>We don't have to worry about the satellites doing that,

0:21:29.480 --> 0:21:33.520
<v Speaker 1>and collectively that will end up giving you a single

0:21:33.520 --> 0:21:37.040
<v Speaker 1>location where it's the only place on the surface of

0:21:37.040 --> 0:21:40.399
<v Speaker 1>the Earth where all of those points of data converge.

0:21:40.640 --> 0:21:43.960
<v Speaker 1>And that's how GPS works. So the scientists work fed

0:21:44.080 --> 0:21:46.720
<v Speaker 1>nicely into work that was already being done at the

0:21:46.800 --> 0:21:50.320
<v Speaker 1>US Naval Center for Space Technology, where other brilliant people

0:21:50.320 --> 0:21:53.480
<v Speaker 1>were hard at work developing atomic clocks. So let's talk

0:21:53.480 --> 0:21:57.120
<v Speaker 1>about that for a second too, because this timekeeping element

0:21:57.359 --> 0:22:02.199
<v Speaker 1>is absolutely vital for navigation purposes. Remember, all of our

0:22:02.280 --> 0:22:06.480
<v Speaker 1>navigation calculations are based upon how far we are from

0:22:06.520 --> 0:22:10.280
<v Speaker 1>these satellites. But if the timekeeping is off, then our

0:22:10.320 --> 0:22:13.080
<v Speaker 1>distance is going to be off, which means we're going

0:22:13.119 --> 0:22:15.600
<v Speaker 1>to think we're somewhere else on the surface of the

0:22:15.600 --> 0:22:18.199
<v Speaker 1>Earth and where we actually are. So let's take quartz

0:22:18.280 --> 0:22:21.480
<v Speaker 1>based risk watches as sort of a starting point. Quarts

0:22:21.600 --> 0:22:25.920
<v Speaker 1>will vibrate physically when subjected to a voltage. This relates

0:22:25.960 --> 0:22:29.200
<v Speaker 1>to piezo electricity, which is the ability for certain materials

0:22:29.200 --> 0:22:32.040
<v Speaker 1>like quartz to store an electric charge in response to

0:22:32.080 --> 0:22:35.720
<v Speaker 1>mechanical force that's been applied to that substance. In other words,

0:22:35.720 --> 0:22:39.680
<v Speaker 1>like if you'll whack quartz, it'll build up an electric charge.

0:22:39.840 --> 0:22:43.679
<v Speaker 1>But the other effect can also be true. Certain materials,

0:22:43.720 --> 0:22:47.280
<v Speaker 1>when exposed to an electric field, will produce physical vibrations,

0:22:47.320 --> 0:22:50.720
<v Speaker 1>and quartz is one of those materials. What's more, it

0:22:50.760 --> 0:22:54.360
<v Speaker 1>will always produce the same frequency of vibrations in response

0:22:54.400 --> 0:22:58.159
<v Speaker 1>to specific applied voltage. So if you apply the same

0:22:58.280 --> 0:23:01.600
<v Speaker 1>voltage over and over, is going to vibrate at the

0:23:01.640 --> 0:23:05.400
<v Speaker 1>same frequency over and over. It does not vary, at

0:23:05.480 --> 0:23:09.320
<v Speaker 1>least not for the purposes of wristwatches. As it turns out,

0:23:09.359 --> 0:23:13.760
<v Speaker 1>for the purposes of space navigation, it's not nearly precise enough.

0:23:13.920 --> 0:23:16.479
<v Speaker 1>But if you apply specific voltage to a quartz crystal,

0:23:16.480 --> 0:23:19.200
<v Speaker 1>the crystal will produce a vibration of a specific frequency,

0:23:19.240 --> 0:23:21.240
<v Speaker 1>which you can then use as if it were the

0:23:21.280 --> 0:23:24.760
<v Speaker 1>swinging pendulum of an old timey grandfather clock, and you

0:23:24.800 --> 0:23:28.560
<v Speaker 1>can calculate the passage of time by the frequency of vibrations.

0:23:28.840 --> 0:23:33.760
<v Speaker 1>If you know that it takes twenty thousand vibrations per second,

0:23:34.240 --> 0:23:36.600
<v Speaker 1>then once you hit twenty thousand, you know a second

0:23:36.640 --> 0:23:40.480
<v Speaker 1>has passed. That's essentially how it works. Now, atomic clocks

0:23:40.520 --> 0:23:44.679
<v Speaker 1>are not that different, but there are many orders of

0:23:44.720 --> 0:23:48.920
<v Speaker 1>magnitude far more precise. So quartz crystals are consistent enough

0:23:48.960 --> 0:23:52.159
<v Speaker 1>for our earthly needs, but when it comes to space operations,

0:23:52.160 --> 0:23:55.879
<v Speaker 1>we need much more stability and much more accuracy. A

0:23:55.960 --> 0:23:59.359
<v Speaker 1>quartz space clock will gradually start to drift and start

0:23:59.400 --> 0:24:02.520
<v Speaker 1>to lose accuracy over time. Now, it typically takes a while.

0:24:02.920 --> 0:24:04.800
<v Speaker 1>It might be more than a month before the clock

0:24:04.880 --> 0:24:07.280
<v Speaker 1>is off by so much as a millisecond, but that

0:24:07.320 --> 0:24:11.520
<v Speaker 1>would still be enough to provide extremely wrong navigational information.

0:24:11.960 --> 0:24:15.560
<v Speaker 1>So imagine you're looking at your GPS app and you

0:24:15.800 --> 0:24:18.960
<v Speaker 1>are flabbric acid because according to the app, you are

0:24:18.960 --> 0:24:22.080
<v Speaker 1>like two hundred miles away from you where you actually are.

0:24:22.400 --> 0:24:24.520
<v Speaker 1>And it's all because the receiver would be depending upon

0:24:24.640 --> 0:24:27.399
<v Speaker 1>the wrong information, that time code would be wrong, and

0:24:27.440 --> 0:24:30.240
<v Speaker 1>that would mean that it would be calculating the wrong distance.

0:24:30.560 --> 0:24:35.560
<v Speaker 1>So yeah, a small error in space translates into an

0:24:35.760 --> 0:24:38.760
<v Speaker 1>enormous error when you get to navigation systems on Earth.

0:24:38.920 --> 0:24:43.479
<v Speaker 1>So atomic clocks rely upon oscillations of atomic energy states.

0:24:43.560 --> 0:24:47.680
<v Speaker 1>Like think of electron energy states. You probably know atoms

0:24:47.680 --> 0:24:51.800
<v Speaker 1>are made up of a nucleus around which are orbiting electrons.

0:24:51.800 --> 0:24:54.960
<v Speaker 1>These electrons in habit various energy states. If you pour

0:24:55.119 --> 0:24:58.920
<v Speaker 1>energy into an atom, you can make an electron go

0:24:59.440 --> 0:25:02.960
<v Speaker 1>move out to a higher energy state, and then once

0:25:03.040 --> 0:25:06.560
<v Speaker 1>you stop pouring energy in, the electron will naturally move

0:25:06.640 --> 0:25:10.800
<v Speaker 1>back down to its normal energy state. So this can

0:25:10.840 --> 0:25:13.879
<v Speaker 1>be an oscillation. Now to go into this further, to

0:25:14.000 --> 0:25:16.800
<v Speaker 1>really dive into it, would get far too complicated for

0:25:16.840 --> 0:25:19.199
<v Speaker 1>this episode. But the important thing to remember is that

0:25:19.280 --> 0:25:22.639
<v Speaker 1>atomic clocks are both more stable and more accurate than

0:25:22.720 --> 0:25:25.760
<v Speaker 1>quartz crystal based time pieces. Depending on the type of

0:25:25.840 --> 0:25:30.400
<v Speaker 1>atom being used, the clock might count billions of oscillations

0:25:30.440 --> 0:25:34.640
<v Speaker 1>per second, like more than nine billion, So you're really

0:25:34.680 --> 0:25:40.960
<v Speaker 1>dividing a second down into unfathomably small units of time

0:25:41.280 --> 0:25:44.240
<v Speaker 1>by looking at the frequency of these oscillations. This is

0:25:44.280 --> 0:25:47.600
<v Speaker 1>an incredible level of accuracy, which is a necessary component

0:25:47.600 --> 0:25:50.520
<v Speaker 1>when we're talking about navigation. But I also promise y'

0:25:50.520 --> 0:25:53.199
<v Speaker 1>all some relativity up here in this podcast. So what

0:25:53.359 --> 0:25:57.600
<v Speaker 1>does that have to do with anything, Well, Einstein's theories

0:25:57.600 --> 0:26:01.240
<v Speaker 1>of relativity. Both of these special relativity and general relativity

0:26:01.320 --> 0:26:04.600
<v Speaker 1>varieties have something to say about the passage of time.

0:26:04.880 --> 0:26:08.240
<v Speaker 1>It's all relative, you see. And some factors that determine

0:26:08.240 --> 0:26:11.240
<v Speaker 1>the speed at which time passes for a subject relative

0:26:11.280 --> 0:26:15.480
<v Speaker 1>to an outside observer includes stuff like gravity and speed. Now,

0:26:16.560 --> 0:26:19.040
<v Speaker 1>let's get one thing out of the way first, because

0:26:19.040 --> 0:26:22.439
<v Speaker 1>this gets whibbly wobbly timey. Whymy, Like, you wouldn't believe

0:26:22.920 --> 0:26:26.879
<v Speaker 1>the passage of time to an observer like their own sense,

0:26:26.920 --> 0:26:29.879
<v Speaker 1>their own sensation of the passage of time, that doesn't change.

0:26:29.960 --> 0:26:33.600
<v Speaker 1>To them. Time continues on as it would in any

0:26:33.640 --> 0:26:38.240
<v Speaker 1>other condition. It's only as they observe outside points of

0:26:38.280 --> 0:26:42.440
<v Speaker 1>reference that the sense of time changes. So like, for example,

0:26:42.800 --> 0:26:45.040
<v Speaker 1>one thing is that the faster you go, the slower

0:26:45.080 --> 0:26:48.359
<v Speaker 1>time moves for you relative to an outside observer. So

0:26:49.000 --> 0:26:50.960
<v Speaker 1>if you're in a ship and you're going super super

0:26:51.000 --> 0:26:54.119
<v Speaker 1>super fast, it would feel like time is passing as normal.

0:26:54.200 --> 0:26:57.480
<v Speaker 1>To someone outside of the spaceship here on Earth, it

0:26:57.480 --> 0:27:00.520
<v Speaker 1>would look like you were moving in slow motion. If

0:27:00.520 --> 0:27:03.680
<v Speaker 1>they could magically see you inside this ship, even though

0:27:03.680 --> 0:27:05.679
<v Speaker 1>the ship is moving super fast, you would appear to

0:27:05.680 --> 0:27:08.320
<v Speaker 1>be moving at a crawl. And that's why at the

0:27:08.440 --> 0:27:11.600
<v Speaker 1>end of your journey, when you would get off your spaceship,

0:27:12.080 --> 0:27:14.920
<v Speaker 1>your friends and family who had stayed behind on Earth

0:27:14.960 --> 0:27:18.040
<v Speaker 1>would have all aged much more than you did, because

0:27:18.320 --> 0:27:22.199
<v Speaker 1>relative to them, time passed more slowly. For you. Your experience, however,

0:27:22.400 --> 0:27:25.639
<v Speaker 1>was that time just continued on as it always has,

0:27:26.200 --> 0:27:29.399
<v Speaker 1>very very mind binding kind of stuff. Right, But what

0:27:29.440 --> 0:27:32.000
<v Speaker 1>does this have to do with satellites. Well, let's talk

0:27:32.000 --> 0:27:36.000
<v Speaker 1>about general relativity first. It explains that gravity can alter

0:27:36.200 --> 0:27:39.639
<v Speaker 1>time such that a satellite that's in orbit around Earth

0:27:40.119 --> 0:27:42.560
<v Speaker 1>will have clocks that are running a little bit faster

0:27:43.000 --> 0:27:45.160
<v Speaker 1>than they would if they were just on Earth. And

0:27:45.240 --> 0:27:47.199
<v Speaker 1>by a little bit faster, I'm talking about like forty

0:27:47.200 --> 0:27:52.240
<v Speaker 1>five microseconds per day drifting right, like they're getting ahead

0:27:52.600 --> 0:27:56.680
<v Speaker 1>by about forty five microseconds per day. However, we also

0:27:56.760 --> 0:28:00.120
<v Speaker 1>have special relativity. This says that because the satellites are

0:28:00.119 --> 0:28:02.720
<v Speaker 1>whizzing through space pretty darn fast, the clocks run a

0:28:02.720 --> 0:28:06.040
<v Speaker 1>little more slowly relative to the ones on Earth, and

0:28:06.080 --> 0:28:09.399
<v Speaker 1>they end up losing about seven microseconds per day. So

0:28:09.920 --> 0:28:11.880
<v Speaker 1>you've got to factor both of these in. Right, you're

0:28:11.960 --> 0:28:15.000
<v Speaker 1>gaining forty five microseconds on one side and losing seven

0:28:15.080 --> 0:28:17.640
<v Speaker 1>microseconds on the other side. But this means that we

0:28:17.800 --> 0:28:23.560
<v Speaker 1>have to send up clock modifications corrections to the satellite's

0:28:23.800 --> 0:28:26.359
<v Speaker 1>clocks in order to adjust them and make sure they

0:28:26.359 --> 0:28:30.600
<v Speaker 1>don't drift too much over time, because the longer they

0:28:30.640 --> 0:28:33.600
<v Speaker 1>do so without a correction, the more inaccurate the results

0:28:33.600 --> 0:28:35.479
<v Speaker 1>are going to be here on Earth when we're depending

0:28:35.560 --> 0:28:37.879
<v Speaker 1>upon them for navigation. All right, let's get back to

0:28:37.920 --> 0:28:41.040
<v Speaker 1>our history. So in the late nineteen seventies, a US

0:28:41.080 --> 0:28:45.000
<v Speaker 1>military GPS constellation was slowly taking shape, and initially it

0:28:45.040 --> 0:28:48.080
<v Speaker 1>was called Navstar. And this project took the work that

0:28:48.160 --> 0:28:51.680
<v Speaker 1>was being done independently in the Army, the Navy, and

0:28:51.720 --> 0:28:55.240
<v Speaker 1>the Air Force and kind of brought all that learning

0:28:55.320 --> 0:29:01.160
<v Speaker 1>together and became a really massive nationwide effort and eventually

0:29:01.200 --> 0:29:03.240
<v Speaker 1>it would evolve into what we just referred to as

0:29:03.280 --> 0:29:07.240
<v Speaker 1>GPS these days. The first fully operational satellite in the

0:29:07.320 --> 0:29:11.520
<v Speaker 1>GPS constellation would finally launch in nineteen eighty nine. So yeah,

0:29:11.680 --> 0:29:14.120
<v Speaker 1>this was a system that was in development for like

0:29:14.240 --> 0:29:18.200
<v Speaker 1>two decades pretty much, and then finally in nineteen eighty nine,

0:29:18.240 --> 0:29:20.960
<v Speaker 1>the first satellite goes up. And that's just one. You

0:29:21.040 --> 0:29:24.280
<v Speaker 1>can't navigate just on one satellite, at least not using

0:29:24.320 --> 0:29:29.280
<v Speaker 1>this trilateration approach. But meanwhile, manufacturers here on Terra Firma

0:29:29.440 --> 0:29:33.280
<v Speaker 1>were busy building the navigation devices that would be reliant

0:29:33.360 --> 0:29:36.040
<v Speaker 1>upon these satellites once there were more up in orbit,

0:29:36.560 --> 0:29:41.200
<v Speaker 1>and this would include handheld navigation units. The constellation of

0:29:41.240 --> 0:29:44.960
<v Speaker 1>GPS satellites wouldn't reach what old Emperor Palpatine would consider

0:29:45.280 --> 0:29:50.600
<v Speaker 1>fully operational until nineteen ninety five. The military would end

0:29:50.680 --> 0:29:53.960
<v Speaker 1>up receiving clear signals for the purposes of navigation. So

0:29:54.000 --> 0:29:56.880
<v Speaker 1>if you were using GPS and you were in the

0:29:56.920 --> 0:29:59.520
<v Speaker 1>military and you were using it officially, you would get

0:29:59.640 --> 0:30:03.280
<v Speaker 1>really accurate results. However, the same was not true for

0:30:03.440 --> 0:30:06.360
<v Speaker 1>everybody else. The rest of us got something that was

0:30:06.400 --> 0:30:10.040
<v Speaker 1>called selective availability. I mentioned that at the top of

0:30:10.080 --> 0:30:14.360
<v Speaker 1>this episode. So essentially for civilian use, the satellites were

0:30:14.440 --> 0:30:19.120
<v Speaker 1>fudging the timecode just a tiny, tiny amount in those

0:30:19.200 --> 0:30:22.760
<v Speaker 1>data pulses. Now, it wasn't fudging the timecode enough to

0:30:22.920 --> 0:30:25.880
<v Speaker 1>put you well outside where you actually were and make

0:30:25.920 --> 0:30:29.840
<v Speaker 1>it totally useless, but it was enough to muddle the

0:30:29.920 --> 0:30:34.920
<v Speaker 1>accuracy to within maybe one hundred meters of your actual location.

0:30:35.360 --> 0:30:38.320
<v Speaker 1>So you could still use GPS for general navigation, but

0:30:38.360 --> 0:30:40.560
<v Speaker 1>it wouldn't be suitable for stuff like turn by turn

0:30:40.680 --> 0:30:43.880
<v Speaker 1>directions because the muddled data would not be accurate to

0:30:43.920 --> 0:30:47.400
<v Speaker 1>your real location. So why was this Well, it was

0:30:47.440 --> 0:30:50.520
<v Speaker 1>to protect stuff like military bases and that sort of thing.

0:30:50.680 --> 0:30:53.600
<v Speaker 1>The thought was that the information was potentially too dangerous

0:30:53.640 --> 0:30:57.040
<v Speaker 1>to be made public. This would hold true until two thousand,

0:30:57.200 --> 0:31:02.080
<v Speaker 1>when former President Bill Clinton rescinded select availability. At that point,

0:31:02.120 --> 0:31:06.560
<v Speaker 1>GPS receivers could display accurate information to within a couple

0:31:06.560 --> 0:31:09.600
<v Speaker 1>of meters of a person's actual location on the Earth,

0:31:09.640 --> 0:31:12.440
<v Speaker 1>and this would improve over time, and this is when

0:31:12.480 --> 0:31:15.920
<v Speaker 1>turn by turn directions will become a possibility for civilian use.

0:31:16.200 --> 0:31:19.040
<v Speaker 1>Now today there are more than thirty satellites that are

0:31:19.040 --> 0:31:24.200
<v Speaker 1>part of the GPS constellation. They are frequently updated where

0:31:24.360 --> 0:31:28.640
<v Speaker 1>you know, a newer generation of tech satellite will go

0:31:28.720 --> 0:31:31.560
<v Speaker 1>up and replace ones that are no longer in service

0:31:31.640 --> 0:31:37.120
<v Speaker 1>or have stopped working, and our capabilities improve with each generation.

0:31:37.920 --> 0:31:40.240
<v Speaker 1>The United States is also not the only nation to

0:31:40.280 --> 0:31:44.120
<v Speaker 1>operate a global satellite based navigation system. Russia has an

0:31:44.120 --> 0:31:50.480
<v Speaker 1>alternative to GPS. It's called Glonas GLO NASS. Receivers that

0:31:50.520 --> 0:31:54.680
<v Speaker 1>can work with both GPS and clonos are typically more

0:31:54.720 --> 0:31:58.160
<v Speaker 1>reliable because they can more easily receive signals from, at

0:31:58.240 --> 0:32:00.840
<v Speaker 1>least for satellites, like even if you're a place that

0:32:01.160 --> 0:32:05.240
<v Speaker 1>has lots of tall buildings that might block signals, you

0:32:05.320 --> 0:32:07.680
<v Speaker 1>have a lot more satellites up there that you could

0:32:07.680 --> 0:32:11.400
<v Speaker 1>potentially pull from and thus get a better reading on

0:32:11.440 --> 0:32:15.360
<v Speaker 1>where you are, so you can get devices that are

0:32:15.960 --> 0:32:20.200
<v Speaker 1>compliant with both GPS and GLONAS. Glonas initially completed its

0:32:20.200 --> 0:32:22.960
<v Speaker 1>constellation in nineteen ninety five, the same year that the

0:32:23.040 --> 0:32:28.200
<v Speaker 1>GPS constellation went fully operational, but budget cuts in Russia

0:32:28.360 --> 0:32:31.760
<v Speaker 1>led to degradation of the constellation. It lost some of

0:32:31.760 --> 0:32:36.160
<v Speaker 1>its capability, and eventually Russia was able to reinvest and

0:32:36.480 --> 0:32:38.880
<v Speaker 1>in twenty eleven they were able to bring a full

0:32:38.960 --> 0:32:42.520
<v Speaker 1>constellation back online. It's been pretty much that way ever since. Again,

0:32:42.840 --> 0:32:46.880
<v Speaker 1>like the United States, Russia has also upgraded individual satellites

0:32:46.960 --> 0:32:50.000
<v Speaker 1>in the constellation in order to provide better service. So

0:32:50.080 --> 0:32:53.479
<v Speaker 1>that's it. That's kind of how GPS works. It's really

0:32:53.560 --> 0:32:56.800
<v Speaker 1>all about figuring out where you are based on how

0:32:56.840 --> 0:33:00.000
<v Speaker 1>long it took satellites to send you a little data message.

0:33:00.680 --> 0:33:03.760
<v Speaker 1>You know, it's pretty cool, I think. I think it's

0:33:03.800 --> 0:33:08.360
<v Speaker 1>a really intriguing way to figure out your location. It's

0:33:08.360 --> 0:33:11.400
<v Speaker 1>so clever because it's not relying on things like landmarks

0:33:11.480 --> 0:33:13.560
<v Speaker 1>or anything like that. Not the way that people like

0:33:14.160 --> 0:33:18.680
<v Speaker 1>myself typically navigate, right. I navigate through landmarks and street

0:33:18.880 --> 0:33:22.880
<v Speaker 1>names and that kind of stuff. Occasionally I will reorient

0:33:22.960 --> 0:33:26.760
<v Speaker 1>myself based upon which where the sun is, because I

0:33:26.800 --> 0:33:29.720
<v Speaker 1>know enough to know if it's before noon, the sun's

0:33:29.720 --> 0:33:32.720
<v Speaker 1>in the eastern part of the sky, and if it's afternoon,

0:33:32.760 --> 0:33:34.680
<v Speaker 1>it's in the western part of the sky. Once you

0:33:34.720 --> 0:33:37.520
<v Speaker 1>get past that, all bets are off. I was never

0:33:37.560 --> 0:33:40.600
<v Speaker 1>that good of a boy scout, but yeah, GPS is

0:33:40.680 --> 0:33:45.880
<v Speaker 1>really truly revolutionized travel beyond what I can even express. Like,

0:33:46.160 --> 0:33:49.520
<v Speaker 1>it's hard to communicate to people who have never lived

0:33:49.520 --> 0:33:52.719
<v Speaker 1>without GPS what it was like to try and get around,

0:33:52.800 --> 0:33:55.440
<v Speaker 1>like to have an atlass in your car and you know,

0:33:55.560 --> 0:33:58.520
<v Speaker 1>rely on on paper maps or like in the old,

0:33:59.560 --> 0:34:02.600
<v Speaker 1>the old days of things like map quest, you would

0:34:02.720 --> 0:34:05.640
<v Speaker 1>find turn by turn directions on your computer and then

0:34:05.840 --> 0:34:10.479
<v Speaker 1>print them out or write them down because smartphones weren't

0:34:10.480 --> 0:34:12.160
<v Speaker 1>really a thing yet, so you need to have a

0:34:12.200 --> 0:34:15.360
<v Speaker 1>way to actually carry the directions with you. It's a

0:34:15.360 --> 0:34:19.160
<v Speaker 1>different world these days, but still pretty cool. Like I think,

0:34:19.160 --> 0:34:23.240
<v Speaker 1>it's a neat thing to know that this system works

0:34:23.239 --> 0:34:25.360
<v Speaker 1>in this way. It's also important, by the way, to

0:34:25.520 --> 0:34:28.359
<v Speaker 1>learn how to read maps, because you never know. If

0:34:28.400 --> 0:34:31.000
<v Speaker 1>stuff goes down for whatever reason, you want to be

0:34:31.000 --> 0:34:35.160
<v Speaker 1>able to still get around, like things like solar flares

0:34:35.239 --> 0:34:40.000
<v Speaker 1>coronal mass ejections. These big solar events can sometimes wipe

0:34:40.040 --> 0:34:43.120
<v Speaker 1>out stuff or at least shut things down temporarily, and

0:34:43.480 --> 0:34:45.680
<v Speaker 1>if in the process of that you still need to

0:34:45.719 --> 0:34:47.640
<v Speaker 1>get around, knowing how to read a map can be

0:34:47.680 --> 0:34:51.760
<v Speaker 1>really useful, so it's a skill I recommend developing. That's

0:34:51.800 --> 0:34:55.360
<v Speaker 1>it for this episode. I hope you are all well.

0:34:55.440 --> 0:34:58.280
<v Speaker 1>I hope those of you who have fun trips planned

0:34:58.320 --> 0:35:01.560
<v Speaker 1>in the future can take a moment to appreciate the

0:35:01.600 --> 0:35:06.479
<v Speaker 1>beauty and utility of GPS, and how amazing it is

0:35:06.520 --> 0:35:10.280
<v Speaker 1>that we're using things like theory of relativity and space

0:35:10.360 --> 0:35:13.080
<v Speaker 1>technology just so that you know where you need to

0:35:13.120 --> 0:35:15.280
<v Speaker 1>turn to go to the next in and out burger.

0:35:15.400 --> 0:35:18.520
<v Speaker 1>I think that's pretty cool and I will talk to

0:35:18.560 --> 0:35:29.200
<v Speaker 1>you again really soon. Tech Stuff is an iHeartRadio production.

0:35:29.520 --> 0:35:34.520
<v Speaker 1>For more podcasts from iHeartRadio, visit the iHeartRadio app, Apple Podcasts,

0:35:34.680 --> 0:35:36.680
<v Speaker 1>or wherever you listen to your favorite shows.