WEBVTT - TechStuff to Major Tom

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<v Speaker 1>Welcome to Text Stuff, a production from my Heart Radio.

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<v Speaker 1>Hey there, and welcome to tech Stuff. I'm your host,

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<v Speaker 1>Jonathan Strickland. I'm an executive producer with I Heart Radio

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<v Speaker 1>and I love all things tech and today's episode is

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<v Speaker 1>in response to a request Carlos wrote to me and

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<v Speaker 1>asked me this. He said, Hey, Jonathan, great work on

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<v Speaker 1>your podcast. I am looking at satellite communications and I

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<v Speaker 1>find it hard to understand how are they used for

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<v Speaker 1>Internet access, why they use mega hurts instead of megabits

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<v Speaker 1>per second, and in general, how they communicate to Earth

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<v Speaker 1>perhaps a continuation episode. Well that's a great topic, and

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<v Speaker 1>I get how it can be confusing when a technology

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<v Speaker 1>uses different but similar sounding terms. So today we're going

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<v Speaker 1>to break down satellite communications and how they work. Now,

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<v Speaker 1>the simple and there to the question is that satellites

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<v Speaker 1>communicate using radio waves, and in fact that's where the

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<v Speaker 1>mega hurts stuff comes in. But that doesn't really create

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<v Speaker 1>an understanding of what's going on. To do that, we

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<v Speaker 1>need to jump into some history. And you might think

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<v Speaker 1>I would start with nineteen fifty seven with the first

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<v Speaker 1>satellite to achieve orbit, but you're wrong. We're going back

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<v Speaker 1>a bit further I'm going to start all the way

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<v Speaker 1>back in nineteen o three, which sounds crazy, right, but

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<v Speaker 1>that's when a Russian scientist named Konstantine Selkovsky worked out

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<v Speaker 1>the mass that suggested that, yeah, it would be possible

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<v Speaker 1>to build a rocket that we could launch from Earth

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<v Speaker 1>and lift a payload into space, so that that payload,

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<v Speaker 1>that object would be in an orbit around Earth. Now,

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<v Speaker 1>see gravity pulls downward, or if you prefer it, pulls

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<v Speaker 1>towards a center of mass, because you know, once we

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<v Speaker 1>get out into space, concepts like up and down don't

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<v Speaker 1>have so much meaning. Inertia of a moving body tends

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<v Speaker 1>to make it move in a in a straight line.

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<v Speaker 1>So think of it as we have a perfectly leveled table.

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<v Speaker 1>Now we've got a ball on the table, and you

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<v Speaker 1>give a push on the ball, it will tend to

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<v Speaker 1>travel in a straight line in the same direction as

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<v Speaker 1>your push. So if there is a balance between gravity

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<v Speaker 1>and inertia, an object will continue in a straight line

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<v Speaker 1>while being pulled toward a center of mass. So, if

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<v Speaker 1>the object is moving fast enough, the ground of the

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<v Speaker 1>Earth will curve away from its path as it falls

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<v Speaker 1>towards the Earth. So it's kind of in a constant

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<v Speaker 1>state of falling. This, by the way, is one of

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<v Speaker 1>many proofs that the Earth is round, because if it weren't,

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<v Speaker 1>orbits would not work. But we know they work because

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<v Speaker 1>we built stuff, we put it in orbit, We depend

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<v Speaker 1>on that stuff on a day to day basis, So

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<v Speaker 1>that alone is proof that the Earth is round. Now,

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<v Speaker 1>Silkovski proved that an orbiting satellite was possible from a

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<v Speaker 1>mathematical point of view, but there was no real, you know,

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<v Speaker 1>rush to prove him right. For one thing, what the

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<v Speaker 1>heck would the ding dang durn thing do once it

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<v Speaker 1>was up there? I mean, would we just be throwing

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<v Speaker 1>resources at something just to say we did it? I mean,

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<v Speaker 1>this would be the equivalent of answering the question why

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<v Speaker 1>do you want to climb Mount Everest with because it's there?

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<v Speaker 1>That might not be the best answer for all situations. Besides,

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<v Speaker 1>Silkowsky's work wasn't widely known for many years. In fact,

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<v Speaker 1>two decades later, a Romanian scientist named herman O Birth

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<v Speaker 1>essentially worked out the same stuff completely independently of Solkovsky's work.

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<v Speaker 1>He wasn't aware of Silkovsky. But again, even ober It's

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<v Speaker 1>work was confined to a relatively small circle of physicists,

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<v Speaker 1>or as the British would say, Boffin's he. Even well

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<v Speaker 1>read physicists in the United States had never heard of

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<v Speaker 1>either of these two people, and while they were all

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<v Speaker 1>thinking about space, none of them had actually proposed an

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<v Speaker 1>artificial satellite as of yet. Robert Goddard, an American, made

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<v Speaker 1>another important contribution to our space efforts. While pursuing post

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<v Speaker 1>graduate studies at Princeton University. He demonstrated that rocket propulsion

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<v Speaker 1>would work even in the airless environment of space, and

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<v Speaker 1>this was around nineteen sixteen or so, and he built

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<v Speaker 1>a solid fuel rocket in nineteen eighteen. But his funding

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<v Speaker 1>dried up around the time that World War One ended,

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<v Speaker 1>and this is going to be an ongoing theme in

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<v Speaker 1>the space industry. Scientists seem to get way more funds

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<v Speaker 1>when there are possible military applications to the technology they're developing,

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<v Speaker 1>you know, beyond just putting stuff up into space. Goddard

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<v Speaker 1>would continue his work through various colleges up until World

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<v Speaker 1>War Two, when a again he would receive funding to

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<v Speaker 1>work on rocketry with applications for the military, in this

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<v Speaker 1>case largely in the world of jet assisted takeoff or

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<v Speaker 1>j to j A. T O. Germany also famously pursued

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<v Speaker 1>rocketry in World War Two, using it to great effect

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<v Speaker 1>with devastating weapons like the V two rocket. One of

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<v Speaker 1>the scientists chiefly responsible for that V two rocket was

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<v Speaker 1>Werner von Braun, sort of Germany's equivalent of Goddard. Von

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<v Speaker 1>Braun was interested in spaceflight, but like Goddard, he put

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<v Speaker 1>his mind to work for a military in an effort

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<v Speaker 1>to fund his research. Germany used von Braun's rockets to

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<v Speaker 1>fire upon cities like London, killing thousands and devastating entire

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<v Speaker 1>sections of the city. Von Braun wasn't necessarily the most

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<v Speaker 1>ardent supporter of the Nazi regime during World War Two,

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<v Speaker 1>but he joined the Nazi Party and became a member

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<v Speaker 1>of the s S and while he didn't seem to

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<v Speaker 1>share any real political views with the Nazis, he did

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<v Speaker 1>see the allegiance to the party as a necessity for

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<v Speaker 1>him to get the resources he wanted to pursue the

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<v Speaker 1>goal of space flight, so to him, the ends justified

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<v Speaker 1>the means. In nineteen forty three, scientists working for the U. S.

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<v Speaker 1>Navy began to look into the possibility that the Nazis

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<v Speaker 1>were developing rockets capable of putting an artificial satellite into orbit.

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<v Speaker 1>Their worry was that a device like that might be

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<v Speaker 1>used for reconnaissance or spy technology, or maybe even as

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<v Speaker 1>a weapon, whether a weapon capable of actually creating physical

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<v Speaker 1>destruction or a more psychological weapon to terrorize people into

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<v Speaker 1>thinking they'd be subjected to death rays or something. The

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<v Speaker 1>scientists concluded that it could be possible to launch a

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<v Speaker 1>satellite into orbit. Essentially, they were retreading the ground that

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<v Speaker 1>Siolkovsky and o Berth had already walked, and there was

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<v Speaker 1>some early interest in exploring that as an actual option.

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<v Speaker 1>In nineteen four be four, while at a party, Von

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<v Speaker 1>Brown got inebriated and he let it slip that he

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<v Speaker 1>thought the war wouldn't end well for Germany, which was

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<v Speaker 1>pretty much a foregone conclusion, but it was essentially a

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<v Speaker 1>treasonous act. To actually suggest that Germany would lose the

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<v Speaker 1>war was an act of treason. So he was arrested. However,

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<v Speaker 1>he was never incarcerated. It did send a message to him,

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<v Speaker 1>you know, Von Brown said, Wow, my place here is

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<v Speaker 1>not as secure as I would like it to be.

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<v Speaker 1>So he and several other rockets scientists went into hiding.

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<v Speaker 1>Upon hearing that Hitler had committed suicide, these scientists surrendered

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<v Speaker 1>to American soldiers and they were part of a negotiation

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<v Speaker 1>to come to America and essentially pursue the same sort

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<v Speaker 1>of work they had been doing for Germany, but in

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<v Speaker 1>the United States. Now. This was known in classified circles

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<v Speaker 1>as Operation paper Clip, and it involved bringing more than

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<v Speaker 1>fifteen hundred scientists from Germany to the United States. Von

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<v Speaker 1>Braun would continue developing rockets in the US under various

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<v Speaker 1>military projects and research facilities, still with the dream of

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<v Speaker 1>achieving space flight. Now to say that he's a controversial

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<v Speaker 1>historical figure is really putting it mildly, but he's definitely

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<v Speaker 1>an inspiration for science fiction authors who like to create

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<v Speaker 1>sort of those amoral scientists who pursue their obsession with

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<v Speaker 1>no regard for the consequences, you know, following in that

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<v Speaker 1>old Jurassic Park line of you spent so much time

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<v Speaker 1>thinking if you could, you never thought if you should.

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<v Speaker 1>That kind of thing. Anyway, German and American scientists would

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<v Speaker 1>work together in numerous laboratories run by several universities as

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<v Speaker 1>well as the military branches, and they created rockets that

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<v Speaker 1>carried payloads holding scientific equipment designed to measure phenomena in

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<v Speaker 1>the upper atmosphere. So these were rockets that wouldn't escape

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<v Speaker 1>into orbit, but they would go very, very very high up.

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<v Speaker 1>As early as nineteen forty six, these different facilities were

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<v Speaker 1>looking at the possibility of launching a satellite into orbit,

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<v Speaker 1>but they largely concluded that these technologies weren't sophisticated enough

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<v Speaker 1>to make that a reality just yet. It was, however,

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<v Speaker 1>a long term goal. Now this brings us up to

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<v Speaker 1>the nineteen fifties. That's when the United States and the

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<v Speaker 1>then Soviet Union were deep in the Cold War. The

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<v Speaker 1>two nations had become more antagonistic to one another since

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<v Speaker 1>the end of World War Two, and each nation was

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<v Speaker 1>attempting to keep the other in check while expanding its

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<v Speaker 1>own power. They were also both racing to develop technologies

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<v Speaker 1>that can demonstrate superiority over the other. This is part

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<v Speaker 1>of what fueled the space race. Now, I don't want

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<v Speaker 1>to take anything away from the thousands of scientists, engineers, pilots,

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<v Speaker 1>and everyone else who worked on those early days in

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<v Speaker 1>the space industry. Though at this point it wasn't yet

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<v Speaker 1>an industry, there were lots of people who genuinely wanted

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<v Speaker 1>to use technology to explore beyond what humans had previously

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<v Speaker 1>been capable of and to push back our boundaries of ignorance.

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<v Speaker 1>There were a lot of brilliant people who worked on

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<v Speaker 1>projects with the motivation to further our scientific knowledge. But

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<v Speaker 1>the reason they really got the chance to do this

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<v Speaker 1>was because governments were willing to pour a lot of

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<v Speaker 1>resources into the endeavor in an effort to try and

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<v Speaker 1>get ahead of the opposition. So that's the backdrop, but

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<v Speaker 1>let's get to some details. In nineteen fifty two, the

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<v Speaker 1>International Council of Scientific Unions established that the period of

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<v Speaker 1>July one, nineteen fifty seven to December thirty one, nineteen

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<v Speaker 1>fifty eight, would be the international geophysical year to coincide

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<v Speaker 1>with a cycle of increased solar activity. And in case

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<v Speaker 1>you didn't know, the Sun goes through these cycles in

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<v Speaker 1>which there's more solar events like solar flares that happen

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<v Speaker 1>in that cycle. Then that's followed by a period of

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<v Speaker 1>decreased solar act ativity, not no solar activity, but less

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<v Speaker 1>of it. And these are regular and predictable, though the

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<v Speaker 1>individual activities the individual flares are not as predictable. Then

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<v Speaker 1>in nineteen fifty four, this same council said, Hey, you

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<v Speaker 1>know what would be really needo if we figured out

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<v Speaker 1>how to launch a scientific device up so that could

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<v Speaker 1>enter Earth's orbit. Such a thing had never been done before,

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<v Speaker 1>and the proposed goal was a device that would be

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<v Speaker 1>capable of mapping the surface of the Earth, giving us

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<v Speaker 1>the most accurate vision of the Earth's surface to date.

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<v Speaker 1>Several organizations had been looking at the logistics of getting

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<v Speaker 1>a payload up into orbit, though not necessarily as part

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<v Speaker 1>of the Council's proposal. The dream back in nineteen six

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<v Speaker 1>had never really gone away. It just was on the

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<v Speaker 1>back burner because it wasn't really possible. And then something

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<v Speaker 1>happened to spur the American government to put more support

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<v Speaker 1>behind this endeavor. A nineteen fifty four broadcast on Moscow

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<v Speaker 1>our radio revealed that the Soviets were seriously gearing up

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<v Speaker 1>to push for space flight. Now, that bit of information

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<v Speaker 1>didn't reach the general American public, but you can bet

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<v Speaker 1>that the federal government was very much aware of it.

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<v Speaker 1>A year later, in nineteen fifty the US government announced

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<v Speaker 1>a plan to launch a satellite, and that timing is

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<v Speaker 1>definitely not a coincidence. The government began to request proposals

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<v Speaker 1>from various laboratories to assist in getting this done, essentially saying,

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<v Speaker 1>give us your plan so we can figure out where

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<v Speaker 1>we're going to put our money. The Naval Research Laboratory

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<v Speaker 1>responded to this request for proposals with a project called Vanguard,

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<v Speaker 1>while other groups had alternative proposals and lacking a real

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<v Speaker 1>sense of urgency, the White House kind of waffled on this.

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<v Speaker 1>They delayed on selecting an option. They were kind of

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<v Speaker 1>weighing all of the choices, and this was somewhat understandable

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<v Speaker 1>as any path was going to require millions of taxpayer dollars,

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<v Speaker 1>so if the project was a success, it would be

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<v Speaker 1>a high point in science history. But if it failed,

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<v Speaker 1>taxpayers would get mighty miffed at what had been seen

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<v Speaker 1>as a huge waste of money, Like you took millions

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<v Speaker 1>of our dollars and you put it towards something that

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<v Speaker 1>didn't even work. That would be disastrous. Ultimately, the White

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<v Speaker 1>House chose Project Vanguard, and the hope was to be

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<v Speaker 1>the first nation to launch a man made satellite into orbit.

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<v Speaker 1>But that's not how things turned out. While Project Vanguard

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<v Speaker 1>was underway, the Soviets had been busy, and on October fourth,

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<v Speaker 1>nineteen fifty seven, the USSR shocked the world by launching

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<v Speaker 1>a nearly four pound or eighty three point six kilogram

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<v Speaker 1>satellite into orbit. That satellite's name was Sputnik. It was

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<v Speaker 1>about the size of a beach ball, and it would

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<v Speaker 1>orbit the Earth every hour and a half or so,

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<v Speaker 1>and it also essentially went beep. It sent out a

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<v Speaker 1>radio ping signal that could be picked up by radio

0:14:01.120 --> 0:14:06.160
<v Speaker 1>stations as the satellite passed overhead. That included radio sets

0:14:06.160 --> 0:14:10.440
<v Speaker 1>that were operated by amateurs, so ham radio operators could

0:14:10.480 --> 0:14:14.800
<v Speaker 1>hear as the satellite passed over and this launch shocked

0:14:14.960 --> 0:14:18.160
<v Speaker 1>the American public. Americans were under the belief that the

0:14:18.200 --> 0:14:21.600
<v Speaker 1>Soviet Union was far behind the United States from a

0:14:21.640 --> 0:14:26.480
<v Speaker 1>scientific and technological standpoint. Spot Nik flew in the face

0:14:26.560 --> 0:14:29.960
<v Speaker 1>of that, and it also raised a terrifying possibility. If

0:14:30.000 --> 0:14:33.520
<v Speaker 1>the USSR could launch a payload into space, could it

0:14:33.640 --> 0:14:36.280
<v Speaker 1>also create a weapon that could be fired from across

0:14:36.360 --> 0:14:40.240
<v Speaker 1>the world and still hit the United States. Spot Nik

0:14:40.400 --> 0:14:44.520
<v Speaker 1>launch spurred the U s Government into emergency mode. Vanguard

0:14:44.600 --> 0:14:46.880
<v Speaker 1>was still on the books, but the White House would

0:14:46.920 --> 0:14:50.760
<v Speaker 1>turn to the Army Redstone Arsenal Team led by one

0:14:51.160 --> 0:14:54.600
<v Speaker 1>Werner von Braun for an alternative, and it would be

0:14:54.640 --> 0:14:57.960
<v Speaker 1>called the Explorer one, and it would become the first

0:14:58.000 --> 0:15:01.320
<v Speaker 1>satellite launched by the United Dates. We have a bit

0:15:01.320 --> 0:15:03.120
<v Speaker 1>more history to go through when we come back, but

0:15:03.200 --> 0:15:05.960
<v Speaker 1>after that we'll go into how we get these satellites

0:15:05.960 --> 0:15:09.200
<v Speaker 1>into orbit, and then how they communicate with each other

0:15:09.240 --> 0:15:11.680
<v Speaker 1>and with stations here on Earth. But first let's take

0:15:11.920 --> 0:15:22.640
<v Speaker 1>a quick break. The first Spotnik satellite orbited the Earth

0:15:22.800 --> 0:15:26.200
<v Speaker 1>in October nineteen fifty seven, and it was never intended

0:15:26.240 --> 0:15:30.400
<v Speaker 1>to be a permanent fixture. It's orbit gradually decayed until

0:15:30.520 --> 0:15:33.840
<v Speaker 1>in January nineteen fifty eight, it burned up while re

0:15:34.000 --> 0:15:37.240
<v Speaker 1>entering the Earth's atmosphere. The Soviets launched spot Nick two

0:15:37.360 --> 0:15:40.720
<v Speaker 1>in November of nineteen fifty seven, and that's all I'm

0:15:40.760 --> 0:15:43.520
<v Speaker 1>going to say about that story. I've covered it before,

0:15:43.680 --> 0:15:46.680
<v Speaker 1>and that story makes me super sad and I hate

0:15:46.720 --> 0:15:50.200
<v Speaker 1>to talk about it. So the United States would launch

0:15:50.320 --> 0:15:54.480
<v Speaker 1>Explorer one on January thirty one, nineteen fifty eight, So

0:15:54.600 --> 0:15:57.760
<v Speaker 1>several months after both spot Nik and spot Nick two,

0:15:58.280 --> 0:16:02.280
<v Speaker 1>it did more than beep. Explore one did not just beep.

0:16:02.360 --> 0:16:05.360
<v Speaker 1>It also didn't kill a dog, So that's two things

0:16:05.400 --> 0:16:08.160
<v Speaker 1>that made it more advanced than either of the Sputnik satellites.

0:16:08.800 --> 0:16:13.160
<v Speaker 1>It carried scientific equipment designed to detect cosmic rays, and

0:16:13.200 --> 0:16:16.320
<v Speaker 1>the fact that it sent data with lower cosmic raid

0:16:16.400 --> 0:16:20.520
<v Speaker 1>counts than was anticipated. Let a scientist named James Van

0:16:20.600 --> 0:16:23.920
<v Speaker 1>Allen to hypothesize about the existence of a belt of

0:16:24.080 --> 0:16:28.040
<v Speaker 1>charged particles that were trapped by Earth's magnetic field. A

0:16:28.120 --> 0:16:32.040
<v Speaker 1>second satellite confirmed this hypothesis a couple of months later,

0:16:32.120 --> 0:16:35.840
<v Speaker 1>and the scientific community would name the charged particles the

0:16:35.960 --> 0:16:40.320
<v Speaker 1>Van Allen Belts. It took Explore one just under one

0:16:40.800 --> 0:16:44.160
<v Speaker 1>fifteen minutes to complete an orbit around the Earth, so

0:16:44.320 --> 0:16:46.880
<v Speaker 1>it would go around the planet about twelve and a

0:16:46.960 --> 0:16:50.200
<v Speaker 1>half times per day. It stayed in orbit a little

0:16:50.200 --> 0:16:53.320
<v Speaker 1>longer than Sputnik did. While the Soviet satellite burned up

0:16:53.320 --> 0:16:56.000
<v Speaker 1>on reentry just a few months after being launched, the

0:16:56.080 --> 0:17:01.480
<v Speaker 1>Explorer one remained in orbit from ninety eight until eighteen seventy.

0:17:01.520 --> 0:17:06.879
<v Speaker 1>It completed fifty eight thousand trips around Earth. The era

0:17:07.040 --> 0:17:10.000
<v Speaker 1>of the satellite was just beginning. While a lot of

0:17:10.040 --> 0:17:15.000
<v Speaker 1>media attention would shift towards space flights with humans and spacecraft,

0:17:15.000 --> 0:17:18.280
<v Speaker 1>the scientific community around the world continued to develop new

0:17:18.359 --> 0:17:22.480
<v Speaker 1>satellites for all sorts of purposes, from scientific research to

0:17:22.720 --> 0:17:27.840
<v Speaker 1>military reconnaissance to eventually global communications. One other thing I

0:17:27.880 --> 0:17:30.840
<v Speaker 1>want to mention before getting into the communications tech is

0:17:30.880 --> 0:17:34.200
<v Speaker 1>how a science fiction author proposed a type of satellite

0:17:34.200 --> 0:17:38.000
<v Speaker 1>that would be capable of communicating with a ground station

0:17:38.680 --> 0:17:41.119
<v Speaker 1>every hour of the day. See, if you have a

0:17:41.119 --> 0:17:44.240
<v Speaker 1>satellite in orbit like Explorer one, there's going to be

0:17:44.320 --> 0:17:47.639
<v Speaker 1>times when that satellite cannot send communications back to a

0:17:47.720 --> 0:17:51.560
<v Speaker 1>specific ground station because it's going to be out of sight.

0:17:52.080 --> 0:17:56.320
<v Speaker 1>Once the satellite passes a certain point overhead, communications will

0:17:56.359 --> 0:17:59.719
<v Speaker 1>start to drop. Placing ground stations around the world can

0:17:59.760 --> 0:18:02.159
<v Speaker 1>saw of that problem, but that gets into the issue

0:18:02.160 --> 0:18:06.720
<v Speaker 1>of establishing listening stations in places that you know aren't yours,

0:18:07.000 --> 0:18:11.040
<v Speaker 1>and that gets tricky from a political and real estate standpoint.

0:18:11.200 --> 0:18:13.640
<v Speaker 1>But obviously, if a satellite is on the opposite side

0:18:13.640 --> 0:18:16.880
<v Speaker 1>of the Earth from a listening station, the radio signals

0:18:16.960 --> 0:18:19.920
<v Speaker 1>can't get to the listening station, so you really only

0:18:19.960 --> 0:18:24.119
<v Speaker 1>have a window where you can have useful communications with

0:18:24.200 --> 0:18:28.800
<v Speaker 1>that particular type of satellite. For an effective communication satellite,

0:18:28.840 --> 0:18:31.679
<v Speaker 1>you need something in orbit that will remain over the

0:18:31.760 --> 0:18:36.040
<v Speaker 1>same fixed point here on Earth or in a pattern

0:18:36.119 --> 0:18:39.119
<v Speaker 1>that keeps it over the same general area of the Earth.

0:18:39.480 --> 0:18:42.240
<v Speaker 1>The satellite would need to travel around an orbital path

0:18:42.480 --> 0:18:45.240
<v Speaker 1>that keeps pace with the rotation of the Earth itself,

0:18:45.560 --> 0:18:49.880
<v Speaker 1>and this is called a geosynchronous orbit. The satellite will

0:18:49.880 --> 0:18:52.320
<v Speaker 1>travel over the same general region of the Earth because

0:18:52.359 --> 0:18:55.040
<v Speaker 1>it will orbit at the rate of once per day,

0:18:55.640 --> 0:18:59.520
<v Speaker 1>the same as the Earth's rotation. Now, science fiction author

0:18:59.640 --> 0:19:02.919
<v Speaker 1>Arthur See Clark, known for writing stuff like two thousand

0:19:03.000 --> 0:19:06.439
<v Speaker 1>one a Space Odyssey, made a sort of observation and

0:19:06.480 --> 0:19:10.720
<v Speaker 1>prediction back in nine It was published in a magazine

0:19:10.760 --> 0:19:14.080
<v Speaker 1>called Wireless World, and it proposed the idea of a

0:19:14.160 --> 0:19:19.040
<v Speaker 1>geo stationary satellite. Clark stated that a satellite at sufficient altitude,

0:19:19.400 --> 0:19:22.879
<v Speaker 1>and he was talking about a an altitude of forty

0:19:22.880 --> 0:19:26.480
<v Speaker 1>two thousand, one sixty four kilometers or around thirty five thousand,

0:19:26.560 --> 0:19:31.320
<v Speaker 1>seven eighty seven miles above the Earth's surface and placed

0:19:31.359 --> 0:19:34.879
<v Speaker 1>over the equator would have an orbital period equal to

0:19:34.920 --> 0:19:38.359
<v Speaker 1>the Earth's rotation, and so would remain above the same

0:19:38.440 --> 0:19:43.359
<v Speaker 1>fixed point on the equator. Now, forty two thousand, sixty

0:19:43.400 --> 0:19:48.720
<v Speaker 1>four kilometers altitude is obviously a lot, but without any context,

0:19:48.840 --> 0:19:52.160
<v Speaker 1>it's hard to say that's not so bad or wow,

0:19:52.400 --> 0:19:55.440
<v Speaker 1>that's way the heck out there. So just for comparison's sake,

0:19:55.720 --> 0:19:58.760
<v Speaker 1>it's good to remember that the International Space Station, which

0:19:58.960 --> 0:20:01.960
<v Speaker 1>isn't in geo sin grannous orbit, is a mirror four

0:20:02.080 --> 0:20:07.719
<v Speaker 1>hundred kilometers in altitude typically four hundred versus forty two thousand,

0:20:07.880 --> 0:20:12.720
<v Speaker 1>one d sixty four. Wow. Still as far out as

0:20:12.840 --> 0:20:17.880
<v Speaker 1>geosynchronous orbital areas are. That's not even halfway to the Moon.

0:20:18.000 --> 0:20:21.920
<v Speaker 1>The Moon is three four thousand, four hundred kilometers from Earth,

0:20:22.600 --> 0:20:27.399
<v Speaker 1>So a geostationary orbit is a specific subset of orbits

0:20:27.480 --> 0:20:31.440
<v Speaker 1>that fall into the geosynchronous orbit category. A satellite in

0:20:31.520 --> 0:20:35.280
<v Speaker 1>geosynchronous orbit will remain over a general region of Earth,

0:20:35.440 --> 0:20:39.399
<v Speaker 1>but if the satellite isn't directly above the equator, that

0:20:39.600 --> 0:20:42.720
<v Speaker 1>region varies a bit due to the Earth's tilt. In fact,

0:20:43.400 --> 0:20:45.920
<v Speaker 1>from the Earth's standpoint, it looks like the satellite is

0:20:45.960 --> 0:20:50.160
<v Speaker 1>moving in a figure eight pattern across the Earth's surface.

0:20:50.560 --> 0:20:53.680
<v Speaker 1>That's because the path of the satellite crosses above and

0:20:53.800 --> 0:20:57.240
<v Speaker 1>below the equator during the orbit and the Earth's rotation

0:20:57.359 --> 0:21:00.159
<v Speaker 1>throughout the day. A geo stationary orbit has to be

0:21:00.359 --> 0:21:03.360
<v Speaker 1>above the equator, and a satellite along that orbital path

0:21:03.640 --> 0:21:07.960
<v Speaker 1>will remain over its fixed point on Earth. Uh with

0:21:08.200 --> 0:21:11.360
<v Speaker 1>some caveats that I'll get to. Such a satellite could

0:21:11.400 --> 0:21:15.360
<v Speaker 1>remain in constant contact with the exact same ground stations,

0:21:15.680 --> 0:21:18.360
<v Speaker 1>and those ground stations would never need to move their

0:21:18.400 --> 0:21:21.800
<v Speaker 1>antenna to maintain contact, right they would just point their

0:21:21.840 --> 0:21:24.480
<v Speaker 1>antenna where the satellite is, and that's where the satellite

0:21:24.520 --> 0:21:27.880
<v Speaker 1>is going to stay. So it really makes it simplified

0:21:28.000 --> 0:21:31.800
<v Speaker 1>to communicate with that particular satellite. A network of those

0:21:31.840 --> 0:21:34.840
<v Speaker 1>types of satellites could communicate with one another as well

0:21:34.920 --> 0:21:37.320
<v Speaker 1>as their respective ground stations, and boom, you've got your

0:21:37.359 --> 0:21:41.840
<v Speaker 1>framework for a global communications infrastructure using radio signals beamed

0:21:41.880 --> 0:21:45.119
<v Speaker 1>out into space and then beamed back down to the Earth. Now,

0:21:45.240 --> 0:21:48.440
<v Speaker 1>Clark's idea was sound, but there wasn't really any practical

0:21:48.520 --> 0:21:52.520
<v Speaker 1>way to achieve it. Back in it would take twenty

0:21:52.640 --> 0:21:55.359
<v Speaker 1>years before the world would see the first commercial geo

0:21:55.480 --> 0:21:59.800
<v Speaker 1>stationary communications satellite, and that was called the Intel SAT one.

0:22:00.440 --> 0:22:02.640
<v Speaker 1>I think it would be handy for us to look

0:22:02.680 --> 0:22:06.560
<v Speaker 1>at what makes putting satellites into geo stationary orbits so tricky,

0:22:06.880 --> 0:22:09.280
<v Speaker 1>because it gives us an appreciation for the amount of

0:22:09.400 --> 0:22:13.320
<v Speaker 1>science and technology required to make stuff like communication networks

0:22:13.680 --> 0:22:19.200
<v Speaker 1>actually work. So let's start with just putting something into orbit. First,

0:22:19.400 --> 0:22:22.199
<v Speaker 1>you gotta put your satellite on a launch vehicle. Now,

0:22:22.359 --> 0:22:24.960
<v Speaker 1>essentially what we're talking about is a rocket. Now, back

0:22:25.000 --> 0:22:27.560
<v Speaker 1>in the old days, it was the Space Shuttle. We

0:22:27.680 --> 0:22:30.160
<v Speaker 1>often use the Space Shuttle to put satellites up into orbit,

0:22:30.280 --> 0:22:32.960
<v Speaker 1>and the Space Shuttle had rocket boosters attached to it

0:22:33.040 --> 0:22:36.200
<v Speaker 1>as well as its own rocket engine. But these days

0:22:36.240 --> 0:22:38.520
<v Speaker 1>we don't have a space Shuttle. We're talking about a

0:22:38.600 --> 0:22:42.359
<v Speaker 1>rocket here. Usually from our perspective, we launch those rockets

0:22:42.640 --> 0:22:45.680
<v Speaker 1>straight up from the Earth's surface. And there's a good

0:22:45.760 --> 0:22:48.720
<v Speaker 1>reason for this when you think about it. If you're

0:22:48.760 --> 0:22:52.840
<v Speaker 1>looking anywhere from above the horizon in one direction across

0:22:52.920 --> 0:22:55.760
<v Speaker 1>the entire arc of the sky to the horizon, and

0:22:55.840 --> 0:22:58.520
<v Speaker 1>the other direction. So let's say you're doing it from

0:22:58.560 --> 0:23:00.720
<v Speaker 1>east to west. Well, the whole time you do that,

0:23:00.880 --> 0:23:04.000
<v Speaker 1>you're technically looking out towards space. So why would you

0:23:04.080 --> 0:23:08.320
<v Speaker 1>launch straight up if every direction in that arc is

0:23:08.560 --> 0:23:11.760
<v Speaker 1>out towards space. What's because the shortest distance between two

0:23:11.800 --> 0:23:15.400
<v Speaker 1>points is a straight line, and launching straight up means

0:23:15.440 --> 0:23:18.960
<v Speaker 1>you're taking the shortest path to push through the thickest

0:23:19.000 --> 0:23:21.800
<v Speaker 1>part of the atmosphere. You're doing it in the most

0:23:21.880 --> 0:23:25.480
<v Speaker 1>efficient way, and that's really important because that means you're

0:23:25.480 --> 0:23:29.560
<v Speaker 1>consuming less fuel. Since fuel is one of the expensive

0:23:29.640 --> 0:23:33.800
<v Speaker 1>factors in space launches, and since adding more fuel adds

0:23:33.920 --> 0:23:36.520
<v Speaker 1>more weight to your launch vehicle, which means you then

0:23:36.600 --> 0:23:40.560
<v Speaker 1>have to factor that weight into your calculations, being frugal

0:23:41.040 --> 0:23:44.879
<v Speaker 1>with stuff is generally a really good idea. Once the

0:23:45.000 --> 0:23:48.960
<v Speaker 1>rocket reaches a certain altitude, the flight plan will call

0:23:49.280 --> 0:23:52.000
<v Speaker 1>for the rocket to adjust its direction so that the

0:23:52.040 --> 0:23:55.520
<v Speaker 1>payload our satellite in other words, gets to where it's

0:23:55.520 --> 0:23:58.639
<v Speaker 1>supposed to be, and a system called the inertial guidance

0:23:58.800 --> 0:24:01.840
<v Speaker 1>system will calculate the specific adjustments needed to put the

0:24:01.920 --> 0:24:06.600
<v Speaker 1>rocket on the correct path. That system uses accelerometers to

0:24:06.920 --> 0:24:10.400
<v Speaker 1>measure the various stresses it's experiencing in order to interpret

0:24:10.520 --> 0:24:14.359
<v Speaker 1>that as how the rocket is oriented with respect to

0:24:14.400 --> 0:24:17.719
<v Speaker 1>the Earth and what altitude it's at. Those accelerometers are

0:24:17.800 --> 0:24:20.439
<v Speaker 1>in gimbals so that they remain in the same orientation

0:24:20.520 --> 0:24:23.600
<v Speaker 1>with respect to the Earth. Typically, the rocket will head

0:24:23.880 --> 0:24:27.959
<v Speaker 1>toward the east once it reaches that altitude. So why

0:24:28.040 --> 0:24:30.320
<v Speaker 1>does it go toward the east was because the Earth

0:24:30.440 --> 0:24:33.159
<v Speaker 1>rotates to the east, and by going in that direction,

0:24:33.240 --> 0:24:37.120
<v Speaker 1>the rocket gets a bit of a boost, and you'd

0:24:37.160 --> 0:24:39.639
<v Speaker 1>get the best boost in speed if you happen to

0:24:39.720 --> 0:24:43.280
<v Speaker 1>be traveling along the path of the equator and going east.

0:24:43.800 --> 0:24:47.920
<v Speaker 1>The circumference of the Earth is approximately forty thousand kilometers,

0:24:48.160 --> 0:24:51.639
<v Speaker 1>and we know the Earth rotates once every twenty four hours,

0:24:52.800 --> 0:24:55.600
<v Speaker 1>not exactly twenty four hours, but close enough, so that

0:24:55.760 --> 0:24:58.280
<v Speaker 1>means a point on the equator must travel at a

0:24:58.359 --> 0:25:02.800
<v Speaker 1>speed of one thousand, six hundred sixty nine kilometers per hour.

0:25:03.240 --> 0:25:06.200
<v Speaker 1>If you are further north or south of the equator

0:25:06.640 --> 0:25:09.480
<v Speaker 1>and you are traveling east, you don't get quite that

0:25:09.760 --> 0:25:13.440
<v Speaker 1>same speed boost. For example, at Cape Canaveral, which is

0:25:13.480 --> 0:25:16.480
<v Speaker 1>in Florida in the United States, you start off at

0:25:16.520 --> 0:25:19.720
<v Speaker 1>a latitude that is twenty eight degrees thirty six minutes

0:25:19.800 --> 0:25:23.440
<v Speaker 1>twenty nine point seven seconds north of the equator, and

0:25:23.680 --> 0:25:27.000
<v Speaker 1>at this latitude the rotational speed of the Earth is

0:25:27.119 --> 0:25:31.119
<v Speaker 1>one thousand, four hundred forty kilometers per hour, so a

0:25:31.240 --> 0:25:34.880
<v Speaker 1>little bit less than the equatorial speed of one thousand,

0:25:34.960 --> 0:25:38.760
<v Speaker 1>six hundred sixty nine kilometers per hour. It might not

0:25:39.080 --> 0:25:42.359
<v Speaker 1>seem like a huge difference, but again that speed boost

0:25:42.440 --> 0:25:46.000
<v Speaker 1>means that you consume less fuel, So a flight path

0:25:46.119 --> 0:25:48.840
<v Speaker 1>that moves closer to the equator also means you need

0:25:49.000 --> 0:25:51.800
<v Speaker 1>less juice to get to your final orbit, as long

0:25:51.880 --> 0:25:55.040
<v Speaker 1>as that orbit is also near the equator. To escape

0:25:55.080 --> 0:25:58.040
<v Speaker 1>Earth's gravity, a rocket would have to accelerate to at

0:25:58.119 --> 0:26:03.159
<v Speaker 1>least forty thousand, three hundred twenty kilometers per hour. That

0:26:03.440 --> 0:26:06.960
<v Speaker 1>is Earth's escape velocity. If you move slower than that,

0:26:07.800 --> 0:26:10.359
<v Speaker 1>gravity claims the rocket, it will go into an orbit,

0:26:10.480 --> 0:26:15.040
<v Speaker 1>it won't escape Earth's gravitational pull, and eventually it'll fall

0:26:15.160 --> 0:26:18.560
<v Speaker 1>back to Earth if it's uh. If it's inertia, isn't

0:26:19.000 --> 0:26:22.520
<v Speaker 1>enough to keep it in space. But to put a

0:26:22.560 --> 0:26:26.400
<v Speaker 1>satellite into orbit, you don't need escape velocity, right, You're

0:26:26.440 --> 0:26:30.159
<v Speaker 1>not trying to escape Earth's gravity because an orbit is

0:26:30.320 --> 0:26:34.040
<v Speaker 1>a kind of controlled fall. It depends upon a gravitational pull.

0:26:34.400 --> 0:26:37.600
<v Speaker 1>So instead you have to reach orbital velocity. That's that

0:26:37.760 --> 0:26:41.480
<v Speaker 1>balance between a satellite's inertia and moving in a generally

0:26:41.600 --> 0:26:45.520
<v Speaker 1>straight line and the force of gravity that's pulling it downward.

0:26:46.040 --> 0:26:50.400
<v Speaker 1>That speed is dependent upon altitude. The closer the satellite

0:26:50.520 --> 0:26:53.880
<v Speaker 1>is to Earth, the greater the orbital velocity is required

0:26:53.920 --> 0:26:57.080
<v Speaker 1>in order to balance out the force of gravity. If

0:26:57.119 --> 0:27:00.440
<v Speaker 1>the satellite we're at two kilometers over the Earth, it

0:27:00.480 --> 0:27:03.760
<v Speaker 1>would have to travel at twenty seven thousand, four hundred

0:27:03.840 --> 0:27:07.919
<v Speaker 1>kilometers per hour to maintain orbit and not come falling

0:27:08.000 --> 0:27:12.120
<v Speaker 1>back down. But in a geo stationary orbit much much

0:27:12.240 --> 0:27:15.320
<v Speaker 1>much further out from Earth, it can travel at a

0:27:15.359 --> 0:27:20.440
<v Speaker 1>comparatively sluggish eleven thousand, three hundred kilometers per hour to

0:27:20.560 --> 0:27:23.679
<v Speaker 1>keep pace. Now remember that's to stay in a fixed

0:27:23.760 --> 0:27:26.359
<v Speaker 1>position above a point on the Earth that's traveling at

0:27:26.760 --> 0:27:29.760
<v Speaker 1>one thousand, six hundred sixty nine kilometers per hour. So

0:27:29.840 --> 0:27:33.320
<v Speaker 1>the satellite has to cover more distance because it's further

0:27:33.440 --> 0:27:35.680
<v Speaker 1>out in the same amount of time as the fixed

0:27:35.680 --> 0:27:37.560
<v Speaker 1>point on Earth, which is why it has to travel

0:27:37.720 --> 0:27:42.240
<v Speaker 1>faster than that relative position. And this is also why

0:27:42.359 --> 0:27:44.680
<v Speaker 1>we need to remember that those satellites that are closer

0:27:44.800 --> 0:27:48.280
<v Speaker 1>to us, they're actually going around the Earth more than

0:27:48.440 --> 0:27:50.760
<v Speaker 1>once per day. They might not be a whole lot

0:27:50.840 --> 0:27:52.800
<v Speaker 1>more than once per day, depending on how far out

0:27:52.840 --> 0:27:56.360
<v Speaker 1>it is, but they are not maintaining a fixed position

0:27:56.640 --> 0:27:59.320
<v Speaker 1>above a point on the Earth, so they actually do

0:27:59.440 --> 0:28:05.520
<v Speaker 1>have to travel faster. Not around in altitude, the rocket

0:28:05.600 --> 0:28:10.680
<v Speaker 1>will fire smaller thrusters to change that rocket's altitude and orientation,

0:28:10.840 --> 0:28:14.080
<v Speaker 1>so it enters into a more horizontal position relative to

0:28:14.160 --> 0:28:18.200
<v Speaker 1>the Earth, and at that orientation, the rocket releases its payload.

0:28:18.320 --> 0:28:21.240
<v Speaker 1>The satellite will part ways with the rocket and the

0:28:21.359 --> 0:28:23.840
<v Speaker 1>rocket will then fire some other thrusters that will help

0:28:23.920 --> 0:28:27.879
<v Speaker 1>create separation between the rocket and the satellite. Okay, so

0:28:28.440 --> 0:28:31.040
<v Speaker 1>we've boosted a satellite with a rocket so that it

0:28:31.119 --> 0:28:34.960
<v Speaker 1>can move into its orbital path. Upon separation, the satellite

0:28:35.080 --> 0:28:38.160
<v Speaker 1>is at the parage. Now, this is the lowest point

0:28:38.480 --> 0:28:41.719
<v Speaker 1>of its orbit, the closest it will be to the Earth. Now,

0:28:41.800 --> 0:28:44.520
<v Speaker 1>the satellite may cross the equator a couple of times

0:28:44.600 --> 0:28:47.480
<v Speaker 1>and it will reach its apogee, or its highest point

0:28:48.400 --> 0:28:51.360
<v Speaker 1>at at this section. And you can think of this

0:28:51.680 --> 0:28:55.160
<v Speaker 1>orbit is looking like it's spiraling out from the Earth,

0:28:55.240 --> 0:28:58.520
<v Speaker 1>like it starts off close and then as the satellite

0:28:58.560 --> 0:29:01.600
<v Speaker 1>goes around the planet, it starts to get further away

0:29:01.760 --> 0:29:04.920
<v Speaker 1>before it starts to come back in. So when we

0:29:04.960 --> 0:29:07.680
<v Speaker 1>talk about lowest and highest points, there's really quite a range.

0:29:07.960 --> 0:29:12.040
<v Speaker 1>So for example, the g Sat fourteen communications satellite, which

0:29:12.080 --> 0:29:16.840
<v Speaker 1>had a geostationary orbit, had a parody of KOs that's

0:29:16.840 --> 0:29:20.040
<v Speaker 1>where it's separated from its launch vehicle and its APOGE

0:29:20.560 --> 0:29:24.720
<v Speaker 1>was thirty six thousand kilometers now an appo G. The

0:29:24.800 --> 0:29:28.360
<v Speaker 1>satellite will conduct a series of controlled burns with onboard

0:29:28.440 --> 0:29:32.240
<v Speaker 1>thrusters on the satellite itself. This helps reshape the orbit

0:29:32.400 --> 0:29:36.040
<v Speaker 1>from being an elliptical path where it's further out from

0:29:36.080 --> 0:29:38.080
<v Speaker 1>the Earth on one side and closer to the Earth

0:29:38.160 --> 0:29:41.000
<v Speaker 1>on the other side, into a more circular path where

0:29:41.080 --> 0:29:44.840
<v Speaker 1>the Earth is at the center. This typically takes a

0:29:45.000 --> 0:29:48.440
<v Speaker 1>few different controlled burns. You could technically do it in one,

0:29:49.120 --> 0:29:51.520
<v Speaker 1>but it would probably require a lot more fuel, so

0:29:51.960 --> 0:29:57.800
<v Speaker 1>it's more frequently done in short bursts to gently reshape

0:29:57.840 --> 0:30:01.480
<v Speaker 1>that orbit. Ultimately re each in orbit where the satellite

0:30:01.520 --> 0:30:05.760
<v Speaker 1>remains in a fixed position above a specific point somewhere

0:30:05.800 --> 0:30:09.960
<v Speaker 1>along the equator. However, the satellite won't stay there forever

0:30:10.080 --> 0:30:12.360
<v Speaker 1>if you just leave things the way they are, because

0:30:12.440 --> 0:30:15.320
<v Speaker 1>stuff like the Moon and even the Earth itself will

0:30:15.440 --> 0:30:20.200
<v Speaker 1>affect the satellite's path through gravitational pull. Earth's gravitational field

0:30:20.360 --> 0:30:23.920
<v Speaker 1>is not uniform and these forces will slowly but surely

0:30:24.040 --> 0:30:26.400
<v Speaker 1>pull the satellite out of position, so once in a

0:30:26.440 --> 0:30:29.040
<v Speaker 1>while the satellite has to use those thrusters to correct

0:30:29.120 --> 0:30:31.480
<v Speaker 1>for that. It's another reason why it's really important to

0:30:31.520 --> 0:30:35.960
<v Speaker 1>conserve fuel. It conserves the lifespan of that satellite. The

0:30:36.040 --> 0:30:39.920
<v Speaker 1>more fuel you use, the less time that satellite is

0:30:39.920 --> 0:30:42.240
<v Speaker 1>going to be able to maintain that position, and it

0:30:42.280 --> 0:30:46.320
<v Speaker 1>will ultimately have an orbital decay and eventually it will

0:30:46.400 --> 0:30:50.320
<v Speaker 1>fall back to the Earth and break apart upon re entry. Now,

0:30:50.360 --> 0:30:52.960
<v Speaker 1>when we come back, we'll talk about how these satellites

0:30:53.080 --> 0:31:04.040
<v Speaker 1>actually communicate. But first let's take another quick break. Okay,

0:31:04.120 --> 0:31:07.920
<v Speaker 1>we've covered the early history of satellites and the challenges

0:31:08.040 --> 0:31:11.320
<v Speaker 1>of getting one into geo stationary orbit. Let's tackle how

0:31:11.440 --> 0:31:15.480
<v Speaker 1>they communicate. Now. I mentioned that a geostationary satellite is

0:31:15.560 --> 0:31:19.040
<v Speaker 1>ideal for communications because it will always maintain its relative

0:31:19.080 --> 0:31:21.520
<v Speaker 1>position above the Earth. So once you know where the

0:31:21.560 --> 0:31:24.200
<v Speaker 1>satellite is, you point your antenna in that direction and

0:31:24.280 --> 0:31:27.320
<v Speaker 1>you can pick up signals from that satellite. So let's

0:31:27.320 --> 0:31:30.120
<v Speaker 1>say you are a satellite TV subscriber and the company

0:31:30.160 --> 0:31:33.800
<v Speaker 1>providing your signal beams information up to a communication satellite

0:31:33.840 --> 0:31:36.760
<v Speaker 1>that's up in orbit, which then can broadcast that same

0:31:36.840 --> 0:31:40.520
<v Speaker 1>signal back down toward a region on Earth. If your

0:31:40.520 --> 0:31:43.600
<v Speaker 1>satellite dish is pointed toward that satellite, you should be

0:31:43.680 --> 0:31:45.960
<v Speaker 1>able to pick up on that signal. But what do

0:31:46.080 --> 0:31:49.440
<v Speaker 1>I mean when I say signals. So we're talking about

0:31:49.480 --> 0:31:53.880
<v Speaker 1>the electro magnetic spectrum, and specifically we're talking about radio waves.

0:31:54.160 --> 0:31:58.240
<v Speaker 1>So remember that the electro magnetic spectrum is huge. On

0:31:58.400 --> 0:32:01.520
<v Speaker 1>one end, you have the long are electromagnetic waves that

0:32:01.600 --> 0:32:05.120
<v Speaker 1>carry less energy. We have radio waves in that section.

0:32:05.640 --> 0:32:08.560
<v Speaker 1>On the opposite side, you have very short waves that

0:32:08.680 --> 0:32:12.360
<v Speaker 1>carry more energy. Gamma rays are on that side. So

0:32:12.520 --> 0:32:16.000
<v Speaker 1>within this spectrum, if we go longest to shortest in

0:32:16.120 --> 0:32:20.200
<v Speaker 1>wavelength of the types of electromagnetic radiation we have discovered,

0:32:20.640 --> 0:32:23.520
<v Speaker 1>keeping in mind, there can be others out there on

0:32:23.720 --> 0:32:26.239
<v Speaker 1>either end of the spectrum, we just have no way

0:32:26.280 --> 0:32:30.160
<v Speaker 1>of really detecting them. We have radio waves on alongside,

0:32:30.400 --> 0:32:35.480
<v Speaker 1>than microwaves, then infrared radiation, than visible light, than ultra

0:32:35.600 --> 0:32:40.320
<v Speaker 1>violet radiation, then X rays, and finally gamma raise. All

0:32:40.400 --> 0:32:43.280
<v Speaker 1>of these forms of energy travel at the speed of light,

0:32:43.640 --> 0:32:46.520
<v Speaker 1>which makes sense right. I mean, light is one of

0:32:46.680 --> 0:32:51.560
<v Speaker 1>the forms of electromagnetic energy. But they all have different

0:32:51.800 --> 0:32:55.000
<v Speaker 1>frequencies and that can get a little confusing. And this

0:32:55.240 --> 0:32:58.080
<v Speaker 1>is where an audio podcast really hits the challenge. So

0:32:58.960 --> 0:33:01.280
<v Speaker 1>let's imagine first second, that you've got a sheet of

0:33:01.400 --> 0:33:03.760
<v Speaker 1>graph paper in front of you, and you draw a

0:33:03.920 --> 0:33:06.680
<v Speaker 1>center line in the middle of that sheet, so there's

0:33:06.720 --> 0:33:09.760
<v Speaker 1>a solid center line, and you start on the left

0:33:09.840 --> 0:33:12.000
<v Speaker 1>side of the sheet at that center line, and you

0:33:12.080 --> 0:33:15.440
<v Speaker 1>start drawing a curve that moves upward from the center

0:33:15.560 --> 0:33:19.080
<v Speaker 1>line and has a peak that's at five squares above

0:33:19.240 --> 0:33:22.200
<v Speaker 1>the center line. Then you curve it back down so

0:33:22.360 --> 0:33:25.880
<v Speaker 1>it crosses that center line. You keep going past it,

0:33:26.320 --> 0:33:29.800
<v Speaker 1>and you draw essentially the mirror image of that curve,

0:33:29.920 --> 0:33:32.760
<v Speaker 1>but you're going down now to you hit five squares

0:33:32.880 --> 0:33:36.480
<v Speaker 1>below center. Then you slowly go back up to the

0:33:36.600 --> 0:33:40.560
<v Speaker 1>center again. That's sort of a representation of a sign wave.

0:33:40.800 --> 0:33:46.160
<v Speaker 1>You've drawn one full wavelength. So electromagnetic energy travels in

0:33:46.280 --> 0:33:50.560
<v Speaker 1>waves like this, but radio waves have much longer wavelengths

0:33:50.640 --> 0:33:53.840
<v Speaker 1>than gamma waves. That's, by the way, a heck of

0:33:53.920 --> 0:33:57.680
<v Speaker 1>an understatement. Radio waves carry less energy than gamma rays

0:33:57.720 --> 0:33:59.520
<v Speaker 1>as well, But there are a couple of reasons that

0:33:59.600 --> 0:34:03.880
<v Speaker 1>we you radio waves for communication. One is that they

0:34:04.000 --> 0:34:07.200
<v Speaker 1>require way less energy to generate than stuff like light.

0:34:08.000 --> 0:34:11.800
<v Speaker 1>But another very practical reason is that light waves and

0:34:11.920 --> 0:34:16.359
<v Speaker 1>shorter wavelengths of electromagnetic radiation get absorbed and scattered by

0:34:16.400 --> 0:34:20.560
<v Speaker 1>the Earth's atmosphere. In fact, gamma rays can even penetrate

0:34:20.640 --> 0:34:23.600
<v Speaker 1>the air, which is really good news for us, because

0:34:23.640 --> 0:34:26.080
<v Speaker 1>otherwise life as we know it would not have formed

0:34:26.160 --> 0:34:29.520
<v Speaker 1>on this planet. Gamma radiation would have wiped out anything

0:34:29.680 --> 0:34:34.120
<v Speaker 1>remotely resembling life as we know it. Radio waves, though

0:34:34.360 --> 0:34:38.000
<v Speaker 1>lower energy, can pass through the atmosphere without distortion, so

0:34:38.160 --> 0:34:42.160
<v Speaker 1>they are ideal for communication. And because the radio waves

0:34:42.200 --> 0:34:45.640
<v Speaker 1>are longer, fewer full wave lengths will pass a given

0:34:45.880 --> 0:34:49.680
<v Speaker 1>fixed point within a second than with gamma waves. Now,

0:34:49.760 --> 0:34:52.800
<v Speaker 1>I always use the analogy of a road to understand

0:34:52.880 --> 0:34:56.200
<v Speaker 1>this concept. So let's say you're standing by a road

0:34:56.680 --> 0:34:59.319
<v Speaker 1>and there's going to be a line of smart cars

0:34:59.400 --> 0:35:02.120
<v Speaker 1>that are travel bumper to bumper, and they're all going

0:35:02.200 --> 0:35:05.320
<v Speaker 1>to pass by you. The cars are all going fifty

0:35:05.400 --> 0:35:08.440
<v Speaker 1>kilometers per hour, and your job is to count the

0:35:08.560 --> 0:35:12.120
<v Speaker 1>number of smart cars that go past you in thirty seconds.

0:35:12.880 --> 0:35:15.080
<v Speaker 1>Then you've got to do the exact same thing, except

0:35:15.200 --> 0:35:18.880
<v Speaker 1>this time, instead of using smart cars, we're using double

0:35:19.000 --> 0:35:22.239
<v Speaker 1>length buses. Those double length busses are also going by

0:35:22.360 --> 0:35:26.560
<v Speaker 1>bumper to bumper. They're also traveling at fifty kilometers per hour. Now,

0:35:26.719 --> 0:35:29.480
<v Speaker 1>the smart cars and the buses are all traveling at

0:35:29.600 --> 0:35:32.360
<v Speaker 1>the same speed. Right, they're all traveling at fifty kilometers

0:35:32.400 --> 0:35:35.040
<v Speaker 1>per hour, but you're going to count way more smart

0:35:35.120 --> 0:35:38.040
<v Speaker 1>cars in those thirty seconds because they're shorter, more can

0:35:38.120 --> 0:35:41.359
<v Speaker 1>fit in that space within that time. Well, the same

0:35:41.440 --> 0:35:45.040
<v Speaker 1>thing is true with electromagnetic radiation. The speed limit is

0:35:45.160 --> 0:35:48.120
<v Speaker 1>set right the speed of light. It's the length of

0:35:48.200 --> 0:35:52.279
<v Speaker 1>the vehicles that changes. Now we measure of frequencies in

0:35:52.480 --> 0:35:56.040
<v Speaker 1>hurts h E R t Z. This refers to the

0:35:56.200 --> 0:35:59.919
<v Speaker 1>number of cycles or wavelengths that pass a fixed point

0:36:00.560 --> 0:36:04.320
<v Speaker 1>within a second. So one hurts would mean one wavelength

0:36:04.400 --> 0:36:08.279
<v Speaker 1>would pass in one second. The U. S. Navy initiated

0:36:08.320 --> 0:36:11.759
<v Speaker 1>a project that would transmit radio signals at frequencies as

0:36:11.840 --> 0:36:15.880
<v Speaker 1>low as thirty hurts, so that's thirty wavelengths in a second. Now,

0:36:16.000 --> 0:36:18.719
<v Speaker 1>keep in mind this is energy that's traveling at the

0:36:18.840 --> 0:36:23.000
<v Speaker 1>speed of light. The speed of light is two hundred thousand,

0:36:23.120 --> 0:36:27.959
<v Speaker 1>seven kilometers per second, so if we divide that number

0:36:28.000 --> 0:36:30.719
<v Speaker 1>by thirty cycles per second, we would see that the

0:36:30.840 --> 0:36:34.680
<v Speaker 1>wave length for thirty hurts is somewhere around nine thousand,

0:36:35.120 --> 0:36:40.520
<v Speaker 1>nine hundred nine three kilometers per cycle. So that means

0:36:40.760 --> 0:36:43.880
<v Speaker 1>a thirty hurts radio signal has a wavelength that is

0:36:44.040 --> 0:36:49.160
<v Speaker 1>nearly ten thousand kilometers long. Using that to communicate is

0:36:49.480 --> 0:36:53.840
<v Speaker 1>tricky because typically we need antenna to be some regular

0:36:54.000 --> 0:36:58.239
<v Speaker 1>fraction of the length of the wavelength that we're transmitting

0:36:58.280 --> 0:37:02.560
<v Speaker 1>and receiving, and a very common one is to have

0:37:02.800 --> 0:37:05.640
<v Speaker 1>an antenna that is one half or one quarter the

0:37:05.840 --> 0:37:09.279
<v Speaker 1>length of the wavelength of radio wave. But at ten

0:37:09.320 --> 0:37:13.399
<v Speaker 1>thousand kilometers, even half or one quarter is still way

0:37:13.480 --> 0:37:18.120
<v Speaker 1>too long, right, So practically we use much shorter wavelength

0:37:18.840 --> 0:37:22.680
<v Speaker 1>radio communications. Uh, it just doesn't make sense to build

0:37:22.719 --> 0:37:26.319
<v Speaker 1>antenna for the longer ones, and different countries chop up

0:37:26.360 --> 0:37:31.120
<v Speaker 1>the radio spectrum and designate bands of frequencies for specific uses.

0:37:31.360 --> 0:37:34.440
<v Speaker 1>For example, in the United States, AM radio uses a

0:37:34.520 --> 0:37:38.080
<v Speaker 1>frequency range between five dred twenty five killer hurts that

0:37:38.200 --> 0:37:42.200
<v Speaker 1>means five twenty five thousand cycles per second, so five

0:37:42.880 --> 0:37:45.520
<v Speaker 1>five thousand wavelengths will pass a fixed point in a

0:37:45.640 --> 0:37:48.840
<v Speaker 1>second at that frequency all the way up to one thousand,

0:37:48.920 --> 0:37:52.400
<v Speaker 1>seven hundred five killer hurts, which would be one million,

0:37:52.520 --> 0:37:56.719
<v Speaker 1>seven hundred five thousand cycles per second or one point

0:37:56.800 --> 0:37:58.680
<v Speaker 1>seven oh five mega hurts if you want to think

0:37:58.680 --> 0:38:01.719
<v Speaker 1>of it that way. And here we get too part

0:38:01.760 --> 0:38:05.040
<v Speaker 1>of that original question. The hurts here refers to the

0:38:05.239 --> 0:38:09.000
<v Speaker 1>radio frequency we're using as a carrier signal. It's all

0:38:09.040 --> 0:38:13.040
<v Speaker 1>about the frequency used to transmit and to receive information.

0:38:13.120 --> 0:38:16.400
<v Speaker 1>It has nothing to do with the amount of information

0:38:16.560 --> 0:38:20.640
<v Speaker 1>in that signal. It's specifically the frequency we're using to

0:38:20.920 --> 0:38:24.000
<v Speaker 1>transmit that signal. It's not directly related to the amount

0:38:24.040 --> 0:38:27.680
<v Speaker 1>of information being sent or processed. This is the medium

0:38:28.000 --> 0:38:30.080
<v Speaker 1>through which we're sending data. So you can think of

0:38:30.120 --> 0:38:33.120
<v Speaker 1>it as serving the exact same purpose as a physical

0:38:33.280 --> 0:38:36.879
<v Speaker 1>wire or cable, except instead of sending a signal down

0:38:36.960 --> 0:38:40.279
<v Speaker 1>a physical piece of hardware, we're sending it through the

0:38:40.440 --> 0:38:44.040
<v Speaker 1>air and through space as radio waves. Now, you could

0:38:44.120 --> 0:38:48.480
<v Speaker 1>try and communicate with a basic unaltered radio wave, but

0:38:48.760 --> 0:38:51.560
<v Speaker 1>you would really be limited by just doing pulses. Right,

0:38:51.680 --> 0:38:54.960
<v Speaker 1>the wave is either on or it's off, and this

0:38:55.040 --> 0:38:58.480
<v Speaker 1>would be kind of like sending Morse code. And maybe

0:38:58.760 --> 0:39:01.160
<v Speaker 1>do you leave it on for a short amount, like

0:39:01.239 --> 0:39:03.800
<v Speaker 1>a very short pulse as a dot, and maybe you

0:39:03.880 --> 0:39:05.680
<v Speaker 1>leave it on a little bit longer as a dash.

0:39:06.400 --> 0:39:09.239
<v Speaker 1>And when you don't have it on, there's a gap, right,

0:39:09.280 --> 0:39:12.920
<v Speaker 1>You know that that's a gap between individual pulses, But

0:39:13.080 --> 0:39:16.640
<v Speaker 1>that's not terribly useful. It's also really easy to have

0:39:16.920 --> 0:39:20.359
<v Speaker 1>errors introduced in that kind of signal, so we don't

0:39:20.440 --> 0:39:25.279
<v Speaker 1>typically use it that way. Instead, radio communications take a

0:39:25.480 --> 0:39:30.160
<v Speaker 1>basic frequency as a carrier signal, like I mentioned a

0:39:30.280 --> 0:39:33.359
<v Speaker 1>minute ago, and this is sort of the baseline. You've

0:39:33.360 --> 0:39:37.840
<v Speaker 1>got a basic signal at a specific frequency. By altering

0:39:37.920 --> 0:39:42.320
<v Speaker 1>that signal or modulating it, we can encode information with it,

0:39:42.800 --> 0:39:46.440
<v Speaker 1>and the deviations from the carrier signal all have meaning.

0:39:47.080 --> 0:39:50.440
<v Speaker 1>As long as we define what those deviations from the

0:39:50.520 --> 0:39:54.839
<v Speaker 1>carrier signal represent, we can encode and decode information sent

0:39:54.960 --> 0:39:58.719
<v Speaker 1>along that carrier wave. I mentioned a M radio a

0:39:58.760 --> 0:40:02.719
<v Speaker 1>couple of moments ago, and that stands for amplitude modulation.

0:40:03.200 --> 0:40:07.040
<v Speaker 1>Amplitude describes the measure of change in a single period

0:40:07.280 --> 0:40:11.359
<v Speaker 1>or cycle. But what does that actually mean in practical terms. Well,

0:40:11.440 --> 0:40:14.239
<v Speaker 1>in our drawing of a sign wave, when we drew

0:40:14.360 --> 0:40:18.160
<v Speaker 1>that that curve that went up and down, that amplitude

0:40:18.160 --> 0:40:21.160
<v Speaker 1>would describe how tall the peak and how deep the

0:40:21.280 --> 0:40:24.520
<v Speaker 1>trough is. And in our example we said it was

0:40:24.640 --> 0:40:28.640
<v Speaker 1>five squares, So that would be the amplitude of that

0:40:28.800 --> 0:40:31.880
<v Speaker 1>sign wave. If we were describing amplitude in terms of

0:40:32.000 --> 0:40:37.640
<v Speaker 1>squares with sound waves, amplitude corresponds with volume. The greater

0:40:37.800 --> 0:40:40.600
<v Speaker 1>the amplitude of a sound wave, the louder it is.

0:40:40.920 --> 0:40:44.360
<v Speaker 1>This does not affect the frequency, which with sound waves

0:40:44.440 --> 0:40:48.239
<v Speaker 1>we would experience as pitch. Right, a higher frequency would

0:40:48.239 --> 0:40:52.439
<v Speaker 1>be a higher pitch sound, So amplitude and pitch are

0:40:52.760 --> 0:40:56.840
<v Speaker 1>not connected. There are two different things. By making precise

0:40:57.120 --> 0:41:00.640
<v Speaker 1>changes in the amplitude of a radio wave as a

0:41:00.719 --> 0:41:04.080
<v Speaker 1>carrier wave, you can encode information on that radio wave.

0:41:04.360 --> 0:41:07.440
<v Speaker 1>A receiver tuned to the proper frequency will pick up

0:41:07.520 --> 0:41:11.520
<v Speaker 1>this incoming signal. It will detect those changes in amplitude

0:41:11.880 --> 0:41:15.480
<v Speaker 1>and it will decode that into useful information. So all

0:41:15.560 --> 0:41:17.800
<v Speaker 1>you really need to do to make this work is

0:41:17.880 --> 0:41:20.520
<v Speaker 1>to come up with a set of rules that corresponds

0:41:20.560 --> 0:41:22.640
<v Speaker 1>to the changes you're going to make in that signal.

0:41:23.040 --> 0:41:25.799
<v Speaker 1>If you say, if I change the amplitude in this way,

0:41:26.280 --> 0:41:29.359
<v Speaker 1>it means X, and if I change it in that way,

0:41:29.800 --> 0:41:32.480
<v Speaker 1>it means why. And then you have a decoder that

0:41:32.560 --> 0:41:35.719
<v Speaker 1>follows those same rules, but just reverses the process. You

0:41:35.800 --> 0:41:40.080
<v Speaker 1>can encode and decode information. It's a really elegant way

0:41:40.320 --> 0:41:43.919
<v Speaker 1>of being able to send data. But what about FM

0:41:44.040 --> 0:41:47.440
<v Speaker 1>radio Then, well, that that still involves modulation. But now

0:41:47.480 --> 0:41:51.480
<v Speaker 1>we're talking about frequency modulation. So you take that carrier

0:41:51.600 --> 0:41:55.200
<v Speaker 1>signal of a very specific radio frequency, and then you

0:41:55.280 --> 0:41:58.879
<v Speaker 1>make small changes to that frequency, not not big ones,

0:41:59.000 --> 0:42:02.920
<v Speaker 1>just small one. You're actually changing the wavelength of the

0:42:03.080 --> 0:42:06.880
<v Speaker 1>wave that you're sending out, making it slightly shorter or

0:42:06.960 --> 0:42:11.320
<v Speaker 1>slightly longer, and you can encode information onto the carrier

0:42:11.400 --> 0:42:14.920
<v Speaker 1>signal in a way similar to you could with amplitude modulation.

0:42:15.400 --> 0:42:18.480
<v Speaker 1>Now you can't change the wavelength too much or else

0:42:18.520 --> 0:42:21.200
<v Speaker 1>you'll push the signal outside of the effectiveness of your

0:42:21.239 --> 0:42:24.239
<v Speaker 1>transmitting and receiving antenna. But you actually have a good

0:42:24.320 --> 0:42:29.000
<v Speaker 1>deal of leeway there. With communication satellites, the modulation is

0:42:29.080 --> 0:42:33.799
<v Speaker 1>a little more complicated than changing amplitude or frequency. Satellites

0:42:33.920 --> 0:42:37.560
<v Speaker 1>use what is called phase modulation. So for this, let's

0:42:37.600 --> 0:42:40.920
<v Speaker 1>imagine you've got two radio waves, and let's say that

0:42:41.040 --> 0:42:44.759
<v Speaker 1>they are absolutely identical radio waves. They both have the

0:42:44.840 --> 0:42:48.160
<v Speaker 1>same frequency, and they have it where the crest of

0:42:48.280 --> 0:42:50.839
<v Speaker 1>one wave is lined up with the crest of another wave.

0:42:50.920 --> 0:42:54.360
<v Speaker 1>So wave one's crest and wave two's crest are perfectly

0:42:54.520 --> 0:42:57.600
<v Speaker 1>in alignment, and because they're the same frequency, they match

0:42:57.680 --> 0:42:59.759
<v Speaker 1>up all the way down the line. So they're in

0:43:00.000 --> 0:43:02.440
<v Speaker 1>box step with each other, or they're in phase with

0:43:02.600 --> 0:43:06.399
<v Speaker 1>one another. However, if you offset those two waves even

0:43:06.520 --> 0:43:09.120
<v Speaker 1>just a little bit, they are out of phase with

0:43:09.239 --> 0:43:12.840
<v Speaker 1>each other, and we can measure that bit by degrees,

0:43:13.680 --> 0:43:15.520
<v Speaker 1>if it's a lot or a little. If you have

0:43:15.640 --> 0:43:18.440
<v Speaker 1>two waves that are one degrees out of phase with

0:43:18.520 --> 0:43:21.400
<v Speaker 1>each other, it would mean that the crest of wave

0:43:21.480 --> 0:43:24.000
<v Speaker 1>one would match up with the lowest point of the

0:43:24.160 --> 0:43:27.239
<v Speaker 1>trough of wave two. They would be as out of

0:43:27.360 --> 0:43:31.839
<v Speaker 1>phase as they possibly could be. So phase modulation first

0:43:32.000 --> 0:43:37.000
<v Speaker 1>establishes a baseline wavelength of the signal. Then you begin

0:43:37.080 --> 0:43:39.920
<v Speaker 1>to alter the phase of that signal by moving that

0:43:40.040 --> 0:43:42.960
<v Speaker 1>wave out of phase in predetermined ways to represent a

0:43:43.120 --> 0:43:46.239
<v Speaker 1>zero or a one communicating in binary data. And you

0:43:46.320 --> 0:43:50.239
<v Speaker 1>can do this at incredibly fast speeds. And this is

0:43:50.280 --> 0:43:53.279
<v Speaker 1>where we get to data throughput, which we measure in

0:43:53.440 --> 0:43:57.040
<v Speaker 1>bits per second. Remember a bit is a basic unit

0:43:57.320 --> 0:44:00.400
<v Speaker 1>of digital information. It's a zero or a one. A

0:44:00.560 --> 0:44:05.480
<v Speaker 1>high throughput satellite can communicate at really high data throughput rates.

0:44:05.520 --> 0:44:08.200
<v Speaker 1>We're talking about on the order of a hundred gigabits

0:44:08.280 --> 0:44:13.080
<v Speaker 1>per second or more, and a gigabit is one billion bits,

0:44:13.400 --> 0:44:18.160
<v Speaker 1>so one billion basic units of digital information every second.

0:44:18.520 --> 0:44:22.239
<v Speaker 1>One billion bits per second. That's a lot of information.

0:44:22.719 --> 0:44:26.560
<v Speaker 1>So now we see what the mega hurts versus megabits

0:44:26.719 --> 0:44:29.360
<v Speaker 1>thing really comes down to. Mega hurts refers to the

0:44:29.520 --> 0:44:32.640
<v Speaker 1>frequency of the radio wave signal that we're using as

0:44:32.719 --> 0:44:35.640
<v Speaker 1>a medium. It's really just telling us the type of

0:44:35.719 --> 0:44:38.480
<v Speaker 1>connection being used, the signal that's being sent out by

0:44:38.520 --> 0:44:41.239
<v Speaker 1>a transmitter and the signal that's being picked up by

0:44:41.280 --> 0:44:45.480
<v Speaker 1>a receiver. The receiver is ignoring all other signals except

0:44:45.520 --> 0:44:48.399
<v Speaker 1>for the one that it's tuned into. Otherwise you would

0:44:48.440 --> 0:44:50.880
<v Speaker 1>just be getting tons of noise and you wouldn't be

0:44:50.920 --> 0:44:53.239
<v Speaker 1>able to tell what was the signal you were looking

0:44:53.280 --> 0:44:56.600
<v Speaker 1>for versus everything else. There are a few other factors

0:44:56.719 --> 0:44:59.400
<v Speaker 1>that allow a receiver to lock into a specific transmission,

0:44:59.440 --> 0:45:02.800
<v Speaker 1>but that gets a lot more technical and uh, mega

0:45:02.880 --> 0:45:06.920
<v Speaker 1>hurts does not directly correlate to data throughput. Uh. The

0:45:07.040 --> 0:45:09.200
<v Speaker 1>frequency does have an effect, but I'll have to go

0:45:09.320 --> 0:45:12.040
<v Speaker 1>into more detail in the future episode because it requires

0:45:12.080 --> 0:45:18.040
<v Speaker 1>a more involved discussion about the nature of frequencies versus

0:45:18.160 --> 0:45:22.360
<v Speaker 1>data throughput. Megabits or gigabits or kill a bits or

0:45:22.400 --> 0:45:26.040
<v Speaker 1>whatever just tells us how much information can be transmitted

0:45:26.200 --> 0:45:30.040
<v Speaker 1>per unit of time per second, for example. Now, I

0:45:30.160 --> 0:45:33.000
<v Speaker 1>hope all of this gives you, guys a deeper understanding

0:45:33.040 --> 0:45:36.200
<v Speaker 1>of what's going on with satellites, including how amazing it

0:45:36.360 --> 0:45:38.640
<v Speaker 1>is the humans figured out how to get stuff out

0:45:38.719 --> 0:45:41.719
<v Speaker 1>into space in the first place, let alone use it

0:45:41.800 --> 0:45:46.680
<v Speaker 1>to communicate information back to Earth. It's a phenomenal achievement

0:45:46.960 --> 0:45:50.800
<v Speaker 1>and really a remarkable display of how a deep understanding

0:45:50.840 --> 0:45:53.520
<v Speaker 1>of science leads to us being able to leverage that

0:45:53.680 --> 0:45:57.399
<v Speaker 1>understanding through technology. It's also why I argue that exploratory

0:45:57.520 --> 0:46:00.879
<v Speaker 1>science is a great thing in gen a role where

0:46:01.000 --> 0:46:05.160
<v Speaker 1>you set out to understand more about the universe, not

0:46:05.440 --> 0:46:09.200
<v Speaker 1>for a specific application, but more just to get that understanding,

0:46:09.480 --> 0:46:13.839
<v Speaker 1>because you never know what kind of applications could come

0:46:13.960 --> 0:46:16.839
<v Speaker 1>from that as we learn more about how the universe works.

0:46:16.880 --> 0:46:20.080
<v Speaker 1>That's why I think funding for sciences is so important.

0:46:20.280 --> 0:46:22.520
<v Speaker 1>You never know what we'll learn and then how we'll

0:46:22.560 --> 0:46:25.800
<v Speaker 1>put that learning to use to benefit people in the future.

0:46:26.120 --> 0:46:29.239
<v Speaker 1>So um fund science, I guess, is what I'm saying.

0:46:29.719 --> 0:46:33.839
<v Speaker 1>All right, guys, that wraps up this discussion about communications satellites,

0:46:34.080 --> 0:46:38.040
<v Speaker 1>very very high overview pun intended of communication satellites. We

0:46:38.080 --> 0:46:39.759
<v Speaker 1>can get into a lot more detail if you guys

0:46:39.840 --> 0:46:43.000
<v Speaker 1>want to um, but it does get pretty tricky. Also,

0:46:43.040 --> 0:46:45.120
<v Speaker 1>it gets tricky for me because I have to get

0:46:45.160 --> 0:46:47.040
<v Speaker 1>a deeper understanding myself in order to be able to

0:46:47.080 --> 0:46:50.160
<v Speaker 1>communicate it properly. And also just figuring out how to

0:46:50.280 --> 0:46:53.319
<v Speaker 1>explain stuff without visual aids is always a challenge. If

0:46:53.360 --> 0:46:56.000
<v Speaker 1>you have any other suggestions, maybe there's some other topic

0:46:56.160 --> 0:46:58.960
<v Speaker 1>totally unrelated to satellite communications that you would like me

0:46:59.040 --> 0:47:01.360
<v Speaker 1>to talk about. Reach out to me on Twitter. The

0:47:01.440 --> 0:47:04.520
<v Speaker 1>handle is text stuff h s W and I'll talk

0:47:04.560 --> 0:47:12.440
<v Speaker 1>to you again really soon y. Text Stuff is an

0:47:12.480 --> 0:47:16.120
<v Speaker 1>I Heart Radio production. For more podcasts from my Heart Radio,

0:47:16.520 --> 0:47:19.640
<v Speaker 1>visit the i Heart Radio app, Apple Podcasts, or wherever

0:47:19.760 --> 0:47:21.280
<v Speaker 1>you listen to your favorite shows.