WEBVTT - Seti Not at Home

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<v Speaker 1>Welcome to Tech Stuff, a production from I 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 as I record this,

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<v Speaker 1>it is early March twenty twenty, just days after I

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<v Speaker 1>received some devastating news. Technically, the whole world received this news.

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<v Speaker 1>I'm just taking it particularly hard. I heard that the

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<v Speaker 1>distributed computing project SETI at Home is shutting down, at

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<v Speaker 1>least for a while. It's going on hiatus by the

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<v Speaker 1>end of March. Now, for two decades, this project has

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<v Speaker 1>been relying on computer processing cycles provided by people like

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<v Speaker 1>all of you guys out there, just using regular computer

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<v Speaker 1>processors rather than some sort of massive super computer. Why

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<v Speaker 1>was it making use of that, Well, it was combing

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<v Speaker 1>through massive amounts of information gathered by radio telescopes in

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<v Speaker 1>search for signals created not through some natural cosmological process,

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<v Speaker 1>but rather as evidence of intelligent communication. SETTI, you see,

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<v Speaker 1>stands for the search for extra terrestrial intelligence. Now, in

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<v Speaker 1>this episode, I'm going to talk about the history of

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<v Speaker 1>SETTI as a science, and then as well, I'm gonna

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<v Speaker 1>I'm gonna kind of pivot around and talk about the

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<v Speaker 1>distributed computer programs and the CETI at Home program in particular.

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<v Speaker 1>We'll find out how distributed computing works. We'll talk about

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<v Speaker 1>a couple of other distributed computing programs that you can

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<v Speaker 1>still participate in if you're so inclined, and we'll also

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<v Speaker 1>look into what's next for SETI at Home and learn

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<v Speaker 1>why it's going on hiatus in the first place. Now,

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<v Speaker 1>we human beings have hypothesized about the possibility of extra

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<v Speaker 1>terrestrial or alien intelligence for a really long time. It's

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<v Speaker 1>a frequent topic in pop culture. But perhaps I shouldn't

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<v Speaker 1>even use the word hypothesize, because for a really long

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<v Speaker 1>time in our history, there really wasn't any way to

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<v Speaker 1>test that hypothesis other than for us to, you know,

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<v Speaker 1>look up at the sky and say, Nope, that ain't it.

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<v Speaker 1>But that would all change with the invention of the

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<v Speaker 1>radio telescope. So it was in the nineteen twenties when

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<v Speaker 1>an engineer named Carl Jansky, working for Bell Telephone Laboratories

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<v Speaker 1>set the stage for radio astronomy. But that wasn't Jansky's

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<v Speaker 1>goal at the time. He had been tasked with figuring

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<v Speaker 1>out where the source was of some signal interference that

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<v Speaker 1>was affecting telephone communications at that time. So in an

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<v Speaker 1>effort to kind of figure this out, he built a

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<v Speaker 1>directional antenna, and I guess that itself deserves its own

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<v Speaker 1>quick explanation. So and enna's can transmitted pickup signals, right,

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<v Speaker 1>I mean, that's what they do, and it actually helps

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<v Speaker 1>to talk about transmitters first to understand how receiving antenna works.

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<v Speaker 1>So a transmitter takes an electrical signal, typically one that's

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<v Speaker 1>been boosted with amplification, and sends that signal to a

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<v Speaker 1>transmitting antenna. Now we know that electricity and magnetism are related, right,

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<v Speaker 1>We've talked about that a ton in previous episodes, and

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<v Speaker 1>we've talked about electro magnetism and the electro magnetic spectrum

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<v Speaker 1>a lot on this show, even recently. So if you

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<v Speaker 1>run a current through a conductor, it generates electromagnetic waves,

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<v Speaker 1>including if the conductor's big enough, radio waves. Now on

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<v Speaker 1>the electromagnetic spectrum, radio waves have the longest wavelengths if

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<v Speaker 1>you look across that spectrum. They are a non ionizing

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<v Speaker 1>form of radiation, meaning they lack the power to strip

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<v Speaker 1>electrons away from atoms, and they aren't harmful. The waste

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<v Speaker 1>stuff like X rays or gamma rays are. So you

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<v Speaker 1>can wander around and you know, I have radio waves

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<v Speaker 1>hitting you. It's not gonna affect you in any way.

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<v Speaker 1>You won't even notice. Okay, So sending a powerful electrical

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<v Speaker 1>current through a big conductor generates radio waves along with

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<v Speaker 1>other electromagnetic radiation. You can encode information on radio waves

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<v Speaker 1>by altering that signal in some way. Otherwise you're just

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<v Speaker 1>sending out a long, steady tone like a sign wave.

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<v Speaker 1>The two main ways to do this are frequency modulation,

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<v Speaker 1>in which you change the frequency of the radio waves

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<v Speaker 1>that you're sending out within a certain band of frequencies,

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<v Speaker 1>or amplitude modulation, in which you change the amplitude. Or

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<v Speaker 1>you can think of it as almost like the strength

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<v Speaker 1>of the radio waves that you're sending out. That would

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<v Speaker 1>end up being FM and a M radio respectively. All right,

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<v Speaker 1>So receivers take that same process, but they reverse it.

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<v Speaker 1>So as long as the signals that the antenna pick

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<v Speaker 1>up are fluctuating in some way, then it's going to

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<v Speaker 1>create an electric current in that antenna. So a properly

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<v Speaker 1>tuned receiver that encounters the respect of radio wave radiation.

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<v Speaker 1>We'll see that whole process go and reverse. The radio

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<v Speaker 1>waves will induce electricity to flow through the antenna to

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<v Speaker 1>whatever device the antenna is hooked up to. It might

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<v Speaker 1>be a meter, in which case you'll see the little

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<v Speaker 1>indicator show that there's a current running through that circuit.

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<v Speaker 1>Or it'll my radio so that you can listen to

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<v Speaker 1>a radio station that way, could be any number of things.

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<v Speaker 1>It usually will require amplification of that signal. Typically the

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<v Speaker 1>signal is too weak to actually power anything significant, so

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<v Speaker 1>you would run it through an amplifier and thus take

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<v Speaker 1>that same signal and just boost its power before sending

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<v Speaker 1>it on to do whatever it was supposed to do.

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<v Speaker 1>Now I've dramatically simplified this whole process. There's other stuff

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<v Speaker 1>we could talk about that really plays an important part,

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<v Speaker 1>like the concept of resonance, but that is really the

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<v Speaker 1>matter for a different episode entirely, and I have covered

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<v Speaker 1>it in previous episodes too. So essentially that's how antenna's work.

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<v Speaker 1>So jen Ski designed a directional antenna as opposed to

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<v Speaker 1>an omnidirectional antenna. So an omnidirectional antenna, as the name implies,

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<v Speaker 1>can pick up signals transmitted from any direction from around

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<v Speaker 1>that antenna. Like, just imagine an antenna poking up straight

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<v Speaker 1>in the air and it can accept radio waves from

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<v Speaker 1>any direction. Uh Now, a directional antenna is designed in

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<v Speaker 1>such a way where it is much more sensitive at

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<v Speaker 1>picking up signals that are coming from specific points. You

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<v Speaker 1>have to point the antenna toward the area where you

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<v Speaker 1>expect there to be a radio wave, and the benefit

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<v Speaker 1>is you can pick up much weaker radio waves typically

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<v Speaker 1>with a directional antenna than with an omnidirect antenna. However,

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<v Speaker 1>if you're a couple of degrees off, if your antenna

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<v Speaker 1>is not pointed directly at the source, you may not

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<v Speaker 1>pick up the signal at all. So if you have

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<v Speaker 1>the directional antenna pointed north, for example, but the source

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<v Speaker 1>of radio waves is to the west, then your antenna

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<v Speaker 1>might not pick it up because it's pointed in a

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<v Speaker 1>different direction. However, this is an incredibly useful tool if

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<v Speaker 1>you're trying to look for a specific you know, source

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<v Speaker 1>of of interference in your telephone communication system. I should

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<v Speaker 1>also add that there's another important thing about directional antennas

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<v Speaker 1>is that even they have a limit to how far

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<v Speaker 1>they can pick up a signal here on Earth. And

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<v Speaker 1>this has to do with the fact that our Earth

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<v Speaker 1>is and brace yourselves round, it's not a flat earth people.

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<v Speaker 1>The way radio waves propagate and it can be transmitted

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<v Speaker 1>and received, that alone would ls that the Earth has

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<v Speaker 1>to be curved. And here's the reason. When you broadcast

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<v Speaker 1>radio waves, they travel outward in a straight line from

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<v Speaker 1>the source of radiation. And if the Earth were flat,

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<v Speaker 1>then no matter how far away you were, if you

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<v Speaker 1>had a sensitive enough antenna, you'd be able to pick

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<v Speaker 1>up radio waves from that source. However, because the Earth curves,

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<v Speaker 1>then you look at two different points on the planet

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<v Speaker 1>that are far enough apart. That curvature means that if

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<v Speaker 1>you're having radio waves travel out at a straight line

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<v Speaker 1>from point A, they won't reach point B because it's

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<v Speaker 1>curved away from the path right, it'll be those radio

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<v Speaker 1>waves will just go out into space instead. There is

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<v Speaker 1>an exception to this, and that's certain radio waves are

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<v Speaker 1>the right length where they can bounce off the Earth's

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<v Speaker 1>ion a sphere. So you can use the ionosphere sort

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<v Speaker 1>of like a mirror. You can point radio waves toward it.

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<v Speaker 1>It will bounce off the ionosphere and then angle back

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<v Speaker 1>down toward the surface of the Earth. That way, you

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<v Speaker 1>could actually transmit much further than you could just from

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<v Speaker 1>line of sight. You can think of his line of sight.

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<v Speaker 1>You don't even actually have to be able to see

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<v Speaker 1>the thing. It just has to be, like I said,

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<v Speaker 1>a more or less straight path from point A to

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<v Speaker 1>point B for you to pick it up. Okay, but

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<v Speaker 1>that's beside the point. Jansky's antenna was a directional antenna

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<v Speaker 1>meant to pick up that source of uh of of interference.

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<v Speaker 1>So he's picking up weird signals as he's using this

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<v Speaker 1>directional antenna that don't seem to have any terrestrial source

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<v Speaker 1>to them, Like if he pointed the directional antenna up

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<v Speaker 1>into the air. He was picking up signals, but he

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<v Speaker 1>could not identify where those signals were coming from. And

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<v Speaker 1>in nine after he had been scratching his head over

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<v Speaker 1>where this source could have come from, he concluded that

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<v Speaker 1>at least some of the signals had to be extra

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<v Speaker 1>to rest real and origin. They had to be coming

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<v Speaker 1>from outside the Earth, from space itself. He didn't know

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<v Speaker 1>where they were coming from or what was producing them,

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<v Speaker 1>but he was sure that it wasn't coming from Earth.

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<v Speaker 1>It was seemingly coming from the center of the Milky

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<v Speaker 1>Way galaxy that, by the way, is the galaxy that

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<v Speaker 1>that we're in the Milky Way. Well, Jansky published his

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<v Speaker 1>findings in nineteen thirty two, and then he moved on

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<v Speaker 1>to work with other stuff, with a telephone system. I mean,

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<v Speaker 1>he wasn't an astronomer or an astrophysicist or anything like that,

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<v Speaker 1>so he dedicated his attention elsewhere. But another American engineer

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<v Speaker 1>named Grote Reber would build on Jansky's work, and by

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<v Speaker 1>the way, I am certain I mispronounced his name entirely,

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<v Speaker 1>but we're gonna soldier on. He read Jenski's work and

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<v Speaker 1>then he decided, you know what, I want to find

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<v Speaker 1>out more about these these signals that seemed to be

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<v Speaker 1>coming from space. So he built and actual radio telescope.

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<v Speaker 1>He set out to build a device specifically to detect

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<v Speaker 1>these kind of signals, and so he built a bowl

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<v Speaker 1>shaped antenna, you know, a parabolic kind of antenna in

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<v Speaker 1>nineteen seven, and it was capable of detecting radio signals

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<v Speaker 1>from space. Now, when I say radio signals from space,

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<v Speaker 1>I am not necessarily talking about stuff that was purposefully

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<v Speaker 1>or intelligently transmitted, because a lot of stuff in space

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<v Speaker 1>generates radio waves. The Sun, for example, does it, other

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<v Speaker 1>stars do it. Pulsars and quasars produce radio waves. Radio

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<v Speaker 1>astronomy gave scientists tools to detect and learn more about

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<v Speaker 1>stuff and space. Then we could manage with things like

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<v Speaker 1>optical telescopes, that is, light based telescopes. So in the

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<v Speaker 1>decades following Reaver's work we saw a lot of progress

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<v Speaker 1>in astronomy thanks to radio telescopes. Now we're going to

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<v Speaker 1>skip up to nine teen fifty seven, and that's when

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<v Speaker 1>a telescope designed by Bernard Level and Charles Husband went

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<v Speaker 1>live for the first time at Jodrell Bank at the

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<v Speaker 1>University of Manchester, and it was called the Mark one telescope,

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<v Speaker 1>though these days folks tend to refer to it as

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<v Speaker 1>the Level telescope. And this thing is big. It has

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<v Speaker 1>a parabolic dish to help focus radio waves on the

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<v Speaker 1>antenna and that dish measures seventy six meters or two

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<v Speaker 1>hundred fifty feet across. A complicated analog computer consisting of

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<v Speaker 1>electro mechanical components was designed so that it could position

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<v Speaker 1>this antenna, could point it at different sections of the sky,

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<v Speaker 1>and this antenna could actually track a radio source as

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<v Speaker 1>it moved across the sky, so you could point it

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<v Speaker 1>at something and then use the computer to constantly adjust

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<v Speaker 1>the radio antenna's position so that it moved along with

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<v Speaker 1>this whatever the source was of the R waves, and

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<v Speaker 1>you could get a better read on it. And there's

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<v Speaker 1>a really impressive piece of technology. Uh. And it also

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<v Speaker 1>picked up the third stage of the rocket that was

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<v Speaker 1>used to launch spot Nick. That's the first man made satellite,

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<v Speaker 1>that's the one the Soviet Union put up into space.

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<v Speaker 1>And uh, it was launched just a few months after

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<v Speaker 1>the level telescope came online, so it actually detected that.

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<v Speaker 1>That was one of the things that indicated how useful

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<v Speaker 1>and important radio telescopes could be beyond just their astronomical

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<v Speaker 1>or cosmological uses. Now, the power of the level telescope

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<v Speaker 1>impressed a lot of very smart people, and a couple

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<v Speaker 1>of those people were Giuseppe Coccone and Philip Morrison. They

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<v Speaker 1>proposed that a sufficiently powerful transmitter and a sufficiently powerful

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<v Speaker 1>receiver would be able to send communications across vast reaches

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<v Speaker 1>of space. So if you had parabolic antennas of particularly

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<v Speaker 1>strong power in two different locations, you could transmit and

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<v Speaker 1>receive radio signals even if you were you know, light

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<v Speaker 1>years apart from each other. Now that communication is still

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<v Speaker 1>restricted by the speed of light, because radio weights travel

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<v Speaker 1>at the speed of light and nothing goes faster than

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<v Speaker 1>the speed of light. So if the two points of

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<v Speaker 1>contact are let's say, eight light years apart from each other,

0:14:20.360 --> 0:14:23.320
<v Speaker 1>it would take eight years for an outgoing message to

0:14:23.480 --> 0:14:26.600
<v Speaker 1>reach the recipient and another eight years to wait for

0:14:26.600 --> 0:14:31.120
<v Speaker 1>a response. So um, there will be no instant messaging.

0:14:31.480 --> 0:14:34.120
<v Speaker 1>But beyond that, it meant that you could take a

0:14:34.240 --> 0:14:37.120
<v Speaker 1>radio telescope and you could use it to search for

0:14:37.240 --> 0:14:40.680
<v Speaker 1>signs that maybe someone out there in space has already

0:14:40.720 --> 0:14:44.640
<v Speaker 1>been using radio technology for communications or for other purposes,

0:14:44.920 --> 0:14:47.680
<v Speaker 1>and that perhaps this could help us determine if there

0:14:47.720 --> 0:14:51.760
<v Speaker 1>are other examples of intelligent life out there. I'll explain

0:14:51.840 --> 0:14:55.200
<v Speaker 1>more about how this was used in just a moment,

0:14:55.200 --> 0:15:05.240
<v Speaker 1>but first let's take a quick break. Coach Tony and

0:15:05.280 --> 0:15:09.640
<v Speaker 1>Morrison wrote a paper about their proposal titled searching for

0:15:09.800 --> 0:15:14.760
<v Speaker 1>Interstellar Communications. The journal Nature published this paper, and the

0:15:14.800 --> 0:15:20.640
<v Speaker 1>two scientists address some pretty big questions. See now, as

0:15:20.680 --> 0:15:26.720
<v Speaker 1>the late great Douglas Adams once observed, space is big,

0:15:27.520 --> 0:15:32.200
<v Speaker 1>really big, and these radio telescopes are directional, so you

0:15:32.280 --> 0:15:35.640
<v Speaker 1>have to pick a spot to point the telescope at.

0:15:36.680 --> 0:15:39.920
<v Speaker 1>But how do you determine where you should look? How

0:15:39.960 --> 0:15:42.840
<v Speaker 1>do you decide this is the point in space we're

0:15:42.880 --> 0:15:46.360
<v Speaker 1>going to search right now. You might start off searching

0:15:46.360 --> 0:15:49.200
<v Speaker 1>the equivalent of a ghost town, and it could be

0:15:49.280 --> 0:15:52.840
<v Speaker 1>that a neighboring region of space might be absolutely teeming

0:15:53.120 --> 0:15:56.720
<v Speaker 1>with life. But because of that directional telescope, you wouldn't

0:15:56.960 --> 0:16:01.760
<v Speaker 1>know that. You're just be getting data from total uninhabited

0:16:01.840 --> 0:16:04.840
<v Speaker 1>part of space. So the implication you get as oh,

0:16:04.840 --> 0:16:08.760
<v Speaker 1>there's nobody out there. Meanwhile, like two space doors down,

0:16:08.800 --> 0:16:12.200
<v Speaker 1>there's a raging party going on. It's kind of like

0:16:12.240 --> 0:16:15.920
<v Speaker 1>if you were staring into a warehouse from the keyhole

0:16:16.000 --> 0:16:18.560
<v Speaker 1>of a door. You would only see stuff within the

0:16:18.640 --> 0:16:21.160
<v Speaker 1>view of that keyhole, but there could be a whole

0:16:21.280 --> 0:16:24.440
<v Speaker 1>lot more warehouse just outside your area of view. You

0:16:24.480 --> 0:16:27.640
<v Speaker 1>would have no idea if anything was actually in the

0:16:27.680 --> 0:16:30.320
<v Speaker 1>warehouse or not. You would only be able to see

0:16:30.960 --> 0:16:34.520
<v Speaker 1>from that narrow range of the keyhole. That was the

0:16:34.560 --> 0:16:38.200
<v Speaker 1>same issue they were having with radio telescopes. Moreover, you

0:16:38.240 --> 0:16:40.720
<v Speaker 1>could point the radio telescope at a place where there

0:16:40.880 --> 0:16:45.280
<v Speaker 1>is intelligent life but maybe it's at a region that's

0:16:45.360 --> 0:16:49.400
<v Speaker 1>so far away from the Earth we can't detect that life.

0:16:49.480 --> 0:16:52.760
<v Speaker 1>So let me put that another way. Human beings started

0:16:52.800 --> 0:16:57.520
<v Speaker 1>broadcasting radio in the early nineteen hundreds, so it's really

0:16:57.560 --> 0:17:00.800
<v Speaker 1>been less than a hundred fifty years since we started

0:17:00.880 --> 0:17:04.760
<v Speaker 1>using radio for communication. There are stars in the Milky

0:17:04.760 --> 0:17:08.600
<v Speaker 1>Way Galaxy again, the same galaxy that our solar system

0:17:08.680 --> 0:17:12.919
<v Speaker 1>is in, that are around nine hundred thousand light years

0:17:13.000 --> 0:17:16.840
<v Speaker 1>away from us. That means it would take light nine

0:17:17.000 --> 0:17:20.840
<v Speaker 1>hundred thousand earth years to travel from that distant star

0:17:21.440 --> 0:17:25.520
<v Speaker 1>to us, so it takes nearly a million years for

0:17:25.560 --> 0:17:28.680
<v Speaker 1>the information to get to us. A radio communication would

0:17:28.680 --> 0:17:31.040
<v Speaker 1>require the same amount of time to get to us.

0:17:31.520 --> 0:17:35.320
<v Speaker 1>That means that if intelligent alien life exists, or even

0:17:35.359 --> 0:17:39.680
<v Speaker 1>existed on a planet around that distant star, that life

0:17:39.680 --> 0:17:42.359
<v Speaker 1>would have had to have invented and made use of

0:17:42.480 --> 0:17:45.920
<v Speaker 1>radio technology a million years ago for us to pick

0:17:46.000 --> 0:17:49.880
<v Speaker 1>up those signals today. That's assuming that intelligent life would

0:17:49.920 --> 0:17:54.639
<v Speaker 1>have somehow survived that million years. Uh for us to

0:17:54.960 --> 0:17:58.440
<v Speaker 1>say that intelligent life exists today, right we we wouldn't

0:17:58.440 --> 0:18:00.800
<v Speaker 1>know that for sure. All we could say is there

0:18:00.800 --> 0:18:04.399
<v Speaker 1>appears to have been an intelligent civilization that existed a

0:18:04.520 --> 0:18:08.000
<v Speaker 1>million years ago, we aren't really sure what they're up

0:18:08.040 --> 0:18:11.480
<v Speaker 1>to now because we'd have no way of knowing. We

0:18:11.520 --> 0:18:15.040
<v Speaker 1>would only know from the signals that were sent from

0:18:15.080 --> 0:18:18.320
<v Speaker 1>the past. That's the neat thing about space too. The

0:18:18.440 --> 0:18:21.520
<v Speaker 1>further you look, the more you're looking into the past,

0:18:22.119 --> 0:18:26.239
<v Speaker 1>you're not seeing present situations just because the restriction of

0:18:26.280 --> 0:18:30.680
<v Speaker 1>the speed of light. So you'd only really be able

0:18:30.760 --> 0:18:36.919
<v Speaker 1>to see any current alien civilization if they were, you know,

0:18:37.160 --> 0:18:40.879
<v Speaker 1>relatively close to us, because otherwise you can't be certain

0:18:40.920 --> 0:18:44.879
<v Speaker 1>that that civilization still exists if it's thousands of light

0:18:44.920 --> 0:18:49.200
<v Speaker 1>years away. Moreover, alien civilizations would only have been able

0:18:49.240 --> 0:18:52.639
<v Speaker 1>to hear us if they were around a hundred fifty

0:18:52.760 --> 0:18:56.719
<v Speaker 1>light years or closer to Earth. If they're further than

0:18:56.760 --> 0:19:01.119
<v Speaker 1>a hundred fifty light years away, then our podcasts would

0:19:01.119 --> 0:19:05.199
<v Speaker 1>not have gone far enough out to reach them. This,

0:19:05.280 --> 0:19:06.960
<v Speaker 1>by the way, is why a lot of science fiction

0:19:07.000 --> 0:19:10.240
<v Speaker 1>stories are really more like fantasy stories. A lot of

0:19:10.280 --> 0:19:13.920
<v Speaker 1>them involve aliens finding out about Earth because they picked

0:19:14.000 --> 0:19:17.800
<v Speaker 1>up a radio or television broadcast, but those broadcasts have

0:19:17.880 --> 0:19:20.320
<v Speaker 1>only been around for a few decades, so that would

0:19:20.320 --> 0:19:23.159
<v Speaker 1>require the aliens to be relatively close to Earth in

0:19:23.160 --> 0:19:26.199
<v Speaker 1>the first place to pick up those transmissions because of

0:19:26.200 --> 0:19:29.600
<v Speaker 1>those limitations of the speed of light. Anyway, my point

0:19:29.640 --> 0:19:33.080
<v Speaker 1>was we might be quote unquote looking at the right spot,

0:19:33.280 --> 0:19:35.439
<v Speaker 1>but the right spot might be far enough away that

0:19:35.520 --> 0:19:39.240
<v Speaker 1>any radio broadcasts would still be in transit to us

0:19:39.680 --> 0:19:41.800
<v Speaker 1>and wouldn't have arrived yet. It may not arrive for

0:19:41.880 --> 0:19:45.040
<v Speaker 1>thousands of years. And that's just one more tiny part

0:19:45.080 --> 0:19:47.879
<v Speaker 1>of why looking for meaningful signals in the sky is

0:19:47.920 --> 0:19:51.159
<v Speaker 1>a huge challenge. You've heard the phrase looking for a

0:19:51.200 --> 0:19:53.800
<v Speaker 1>needle in a haystack. Well, it's like that, but you know,

0:19:54.800 --> 0:19:59.280
<v Speaker 1>roughly a bazillion times harder than that. Conconi and Morrison

0:19:59.480 --> 0:20:02.360
<v Speaker 1>said out an argument about which areas of the galaxy

0:20:02.400 --> 0:20:05.960
<v Speaker 1>would be most likely to host an intelligent civilization capable

0:20:06.000 --> 0:20:10.119
<v Speaker 1>of radio transmissions. This included targeting stars that are neither

0:20:10.359 --> 0:20:15.760
<v Speaker 1>too hot nor too small or cold. Hot stars burnout quickly,

0:20:16.240 --> 0:20:19.560
<v Speaker 1>and the thought was, if it's a really hot star,

0:20:19.800 --> 0:20:23.440
<v Speaker 1>it might go through its life cycle fast enough that

0:20:23.800 --> 0:20:27.080
<v Speaker 1>life doesn't have a chance to evolve on any planets

0:20:27.119 --> 0:20:30.159
<v Speaker 1>that might be an orbit around that star. So the

0:20:30.240 --> 0:20:33.240
<v Speaker 1>star's life cycle is literally too short for life to

0:20:33.400 --> 0:20:39.159
<v Speaker 1>have formed around that system, smaller, colder stars tend to

0:20:39.200 --> 0:20:41.680
<v Speaker 1>be the really old ones, ones that have been around

0:20:41.720 --> 0:20:45.960
<v Speaker 1>for billions of years, and with that much time, eventually,

0:20:46.040 --> 0:20:50.000
<v Speaker 1>orbiting planets will lock on a star so that one

0:20:50.040 --> 0:20:52.480
<v Speaker 1>side of the planet always faces the star and the

0:20:52.480 --> 0:20:55.399
<v Speaker 1>opposite side of the planet always faces away from the start,

0:20:55.760 --> 0:20:58.480
<v Speaker 1>So one side is always lit and the other side

0:20:58.520 --> 0:21:01.800
<v Speaker 1>is always dark, and that kind of planet would probably

0:21:01.880 --> 0:21:06.720
<v Speaker 1>be incapable of supporting life. So said coach Tony and Morrison,

0:21:07.359 --> 0:21:09.840
<v Speaker 1>we should look for stars that are not that different

0:21:09.920 --> 0:21:12.879
<v Speaker 1>from the Sun. These would be the right age and

0:21:13.040 --> 0:21:17.080
<v Speaker 1>size to potentially support life if an orbiting planet were

0:21:17.119 --> 0:21:19.960
<v Speaker 1>within a certain range, which we tend to refer to

0:21:20.000 --> 0:21:23.240
<v Speaker 1>as the Goldilocks region. It has to be a distance

0:21:23.280 --> 0:21:26.200
<v Speaker 1>that's not too close to the Sun, but not too

0:21:26.240 --> 0:21:30.000
<v Speaker 1>far away either, and that really narrows things down in fact,

0:21:30.040 --> 0:21:33.960
<v Speaker 1>and it means we can cross off potentially thousands or

0:21:34.040 --> 0:21:38.480
<v Speaker 1>millions of stars from our otherwise unmanageably huge list of

0:21:38.520 --> 0:21:41.639
<v Speaker 1>potential targets to look at. And so with this in mind,

0:21:42.119 --> 0:21:46.760
<v Speaker 1>another astronomer and an astrophysicist named Frank Drake decided to

0:21:46.800 --> 0:21:49.920
<v Speaker 1>take this hypothesis and to actually put it in action.

0:21:50.400 --> 0:21:54.000
<v Speaker 1>He conducted the first search for extraterrestrial intelligence with the

0:21:54.040 --> 0:21:58.119
<v Speaker 1>help of radio astronomy, and it was called Project OSMA,

0:21:58.240 --> 0:22:02.400
<v Speaker 1>named after the care or Ozma from L. Frank Baum's

0:22:02.440 --> 0:22:07.480
<v Speaker 1>oz books. Drake secured time on a radio telescope that

0:22:07.520 --> 0:22:10.960
<v Speaker 1>measured twenty six ms or eighty five ft across to

0:22:11.080 --> 0:22:14.800
<v Speaker 1>scan for radio frequencies that originated out of towels CT

0:22:15.440 --> 0:22:19.000
<v Speaker 1>and epsilon Eri. Donnie. Those are two different stars, and

0:22:19.040 --> 0:22:22.840
<v Speaker 1>both stars are relatively close to our own solar system,

0:22:23.000 --> 0:22:26.639
<v Speaker 1>and both our sun like enough that they could serve

0:22:26.800 --> 0:22:31.880
<v Speaker 1>as potentially good targets based on Cochoni and Morrison's proposed guidelines.

0:22:32.520 --> 0:22:36.439
<v Speaker 1>Apart from one outlier, his team found no evidence of

0:22:36.520 --> 0:22:41.560
<v Speaker 1>radio signals indicating potential intelligent communication. The one outlier they

0:22:41.600 --> 0:22:45.280
<v Speaker 1>did pick up, while initially interesting, proved to be terrestrial

0:22:45.400 --> 0:22:49.320
<v Speaker 1>in nature, meaning that it originated from an aircraft made

0:22:49.320 --> 0:22:52.760
<v Speaker 1>by dull old humans, didn't come from outer space. It

0:22:52.880 --> 0:22:55.800
<v Speaker 1>was something that we had created and this radio telescope

0:22:55.840 --> 0:22:58.240
<v Speaker 1>just happened to pick it up. And uh. That actually

0:22:58.240 --> 0:23:02.600
<v Speaker 1>illustrates another challenge with using radio telescopes, weeding out the

0:23:02.680 --> 0:23:06.639
<v Speaker 1>signals that are actually coming from us as opposed to

0:23:06.760 --> 0:23:10.639
<v Speaker 1>coming from space, and it sure would be embarrassing to

0:23:10.720 --> 0:23:13.840
<v Speaker 1>come forward with a claim that you've discovered alien communication

0:23:14.280 --> 0:23:16.520
<v Speaker 1>only for it to turn out to be a terrestrial signal,

0:23:16.720 --> 0:23:20.200
<v Speaker 1>like an old Mork and Mindy episode or something that's

0:23:20.240 --> 0:23:22.600
<v Speaker 1>only got a character who's supposed to be an alien

0:23:22.640 --> 0:23:26.440
<v Speaker 1>and it it's not actually alien. Now, luckily, this early

0:23:26.480 --> 0:23:30.720
<v Speaker 1>experience taught researchers to include a secondary antenna that would

0:23:30.800 --> 0:23:35.199
<v Speaker 1>only be sensitive enough to detect terrestrial signals. So you

0:23:35.240 --> 0:23:38.920
<v Speaker 1>put this secondary antenna near the first antenna. They're both

0:23:38.920 --> 0:23:42.000
<v Speaker 1>pointed at the same section of sky, and then when

0:23:42.040 --> 0:23:46.120
<v Speaker 1>you get a a beep, you know you register a signal.

0:23:46.600 --> 0:23:50.320
<v Speaker 1>You can compare the primary telescope, the one that you're

0:23:50.400 --> 0:23:55.840
<v Speaker 1>using to search for extra terrestrial intelligence, against this smaller antenna,

0:23:56.040 --> 0:23:58.800
<v Speaker 1>and if the smaller antenna also picked up the signal,

0:23:59.000 --> 0:24:02.840
<v Speaker 1>you know that signal was terrestrial, because the smaller intenna

0:24:03.240 --> 0:24:06.000
<v Speaker 1>isn't powerful enough to pick up stuff from outer space.

0:24:06.480 --> 0:24:08.320
<v Speaker 1>So you say, all right, well, if it appears on both,

0:24:08.760 --> 0:24:11.080
<v Speaker 1>we know that that came from Earth. We know that

0:24:11.080 --> 0:24:14.280
<v Speaker 1>that's not actually a signal scent from somewhere out in space.

0:24:14.640 --> 0:24:17.720
<v Speaker 1>So they learned that lesson very quickly, and that was

0:24:17.840 --> 0:24:21.520
<v Speaker 1>very helpful. Drake further contributed to the discourse about the

0:24:21.520 --> 0:24:24.960
<v Speaker 1>search for extraterrestrial intelligence by proposing a way to sort

0:24:25.000 --> 0:24:30.160
<v Speaker 1>of conceptualize the possibility of detecting intelligent civilizations in the universe.

0:24:30.480 --> 0:24:33.840
<v Speaker 1>These days. We call it the Drake equation, and it's

0:24:33.840 --> 0:24:37.080
<v Speaker 1>a pretty cool concept, and it goes something like this.

0:24:37.440 --> 0:24:39.800
<v Speaker 1>All right, there's a variable that we're going to call in.

0:24:40.560 --> 0:24:44.159
<v Speaker 1>In represents the number of civilizations in our galaxy with

0:24:44.200 --> 0:24:48.399
<v Speaker 1>which we could possibly communicate. So in is that number.

0:24:48.640 --> 0:24:53.800
<v Speaker 1>It's an unknown number. What determines the value of that number, Well,

0:24:53.800 --> 0:24:56.160
<v Speaker 1>it's a bunch of stuff that you have to take

0:24:56.160 --> 0:25:00.000
<v Speaker 1>into account, and that includes the average rate at which

0:25:00.119 --> 0:25:03.000
<v Speaker 1>stars form in the Milky Way, the number of those

0:25:03.040 --> 0:25:06.600
<v Speaker 1>stars that will actually have planets form around them, because

0:25:06.640 --> 0:25:10.320
<v Speaker 1>not every star has planets, the average number of those

0:25:10.359 --> 0:25:14.920
<v Speaker 1>planets that could potentially support life, the number of planets

0:25:15.119 --> 0:25:19.280
<v Speaker 1>that could support life that actually go on to support life.

0:25:19.800 --> 0:25:23.639
<v Speaker 1>So far, we haven't found any that definitively fit that

0:25:23.640 --> 0:25:27.160
<v Speaker 1>that definition. Then the number of those planets in which

0:25:27.200 --> 0:25:29.919
<v Speaker 1>the life that forms can develop to the point of

0:25:29.960 --> 0:25:33.960
<v Speaker 1>gaining intelligence, The number of planets with intelligent life that

0:25:34.040 --> 0:25:37.280
<v Speaker 1>then develop and use communication tools that would be detectable

0:25:37.400 --> 0:25:41.680
<v Speaker 1>from Earth. And then the length of time such civilizations

0:25:41.960 --> 0:25:44.840
<v Speaker 1>have been doing that, because that length of time will

0:25:44.880 --> 0:25:48.080
<v Speaker 1>determine whether or not they would be detectable. Right so,

0:25:48.160 --> 0:25:51.320
<v Speaker 1>even if they exist, again, if they're far far away,

0:25:52.000 --> 0:25:54.920
<v Speaker 1>there's no way we could detect them anyway, because again

0:25:54.960 --> 0:25:57.479
<v Speaker 1>the speed of light is a limiting factor. So this

0:25:57.520 --> 0:25:59.520
<v Speaker 1>equation is not meant to give us a heart and

0:25:59.560 --> 0:26:03.320
<v Speaker 1>fast now where like three or something. Instead, it helps

0:26:03.400 --> 0:26:07.840
<v Speaker 1>us frame the likelihood of detecting intelligent life, uh specifically

0:26:07.840 --> 0:26:12.760
<v Speaker 1>intelligent life that is using radio communication. We don't really

0:26:12.800 --> 0:26:15.440
<v Speaker 1>know anything about the number of plants that can definitively

0:26:15.520 --> 0:26:20.680
<v Speaker 1>support life or anything else beyond that particular variable. Right

0:26:20.720 --> 0:26:23.480
<v Speaker 1>we we've got information about some of the other stuff.

0:26:23.520 --> 0:26:26.400
<v Speaker 1>We have a general idea of how frequently stars form

0:26:26.400 --> 0:26:30.719
<v Speaker 1>in the milky Way. We are refining our understanding of

0:26:30.760 --> 0:26:33.760
<v Speaker 1>how many stars have planets. Turns out that way more

0:26:33.800 --> 0:26:37.480
<v Speaker 1>stars have planets than we initially thought. Then we have

0:26:37.560 --> 0:26:39.159
<v Speaker 1>to think, all right, well, how many of those plants

0:26:39.160 --> 0:26:42.359
<v Speaker 1>could potentially support life based upon their distance from the star,

0:26:42.560 --> 0:26:44.240
<v Speaker 1>the age of the star, the heat of the star

0:26:44.359 --> 0:26:47.880
<v Speaker 1>all of those other variables. So we're slowly learning more

0:26:47.920 --> 0:26:50.520
<v Speaker 1>about the front half of that equation, and the back

0:26:50.600 --> 0:26:55.320
<v Speaker 1>half is still largely a mystery to us. Now, Uh,

0:26:55.520 --> 0:26:58.439
<v Speaker 1>it's important so that we can use that kind of

0:26:58.480 --> 0:27:01.280
<v Speaker 1>information to help refine our search. Right. We want to

0:27:01.280 --> 0:27:05.240
<v Speaker 1>make sure that we are looking at the places most

0:27:05.560 --> 0:27:10.200
<v Speaker 1>likely to produce good results, because again, space is really big.

0:27:10.240 --> 0:27:13.720
<v Speaker 1>If we just randomly point the telescope in any given direction,

0:27:14.119 --> 0:27:18.639
<v Speaker 1>the odds of success are miniscule. We want to improve

0:27:18.760 --> 0:27:21.920
<v Speaker 1>those odds as best we can by making some intelligent

0:27:22.080 --> 0:27:28.800
<v Speaker 1>decisions based on educated guesses. Really now, Uh, The SETI Institute,

0:27:29.280 --> 0:27:33.920
<v Speaker 1>a not for profit scientific research organization, wouldn't come into

0:27:33.920 --> 0:27:39.159
<v Speaker 1>being until ninety four. However, between Drake's project OZMA in

0:27:39.200 --> 0:27:44.280
<v Speaker 1>the early nineteen sixties and the set Institute's formation in four,

0:27:44.359 --> 0:27:47.160
<v Speaker 1>there were lots of astronomers who were looking for signals

0:27:47.200 --> 0:27:51.159
<v Speaker 1>that might have originated from an intelligent civilization out in space.

0:27:51.720 --> 0:27:55.160
<v Speaker 1>I find a lot of people confuse SET the science

0:27:55.440 --> 0:27:59.159
<v Speaker 1>that's the general science of searching for extraterrestrial intelligence, and

0:27:59.280 --> 0:28:03.720
<v Speaker 1>SET the Institute. Uh. Those are the SETI Institute is

0:28:03.760 --> 0:28:07.320
<v Speaker 1>dedicated toward a deeper understanding of life in general and

0:28:07.359 --> 0:28:10.520
<v Speaker 1>its place in the universe, and the potential existence of

0:28:10.560 --> 0:28:15.359
<v Speaker 1>extraterrestrial intelligence. But the two are not synonymous. It's not

0:28:15.600 --> 0:28:20.400
<v Speaker 1>Set and the SETI Institute are related but distinct. Now,

0:28:20.440 --> 0:28:23.720
<v Speaker 1>back in nineteen seven, there was an astronomer named Jocelyn

0:28:23.840 --> 0:28:28.640
<v Speaker 1>Bell who noticed something that initially seemed really promising from

0:28:28.640 --> 0:28:33.680
<v Speaker 1>a set perspective. Turned out it was incredible information, period,

0:28:33.880 --> 0:28:36.480
<v Speaker 1>but we just didn't understand its significance at the time.

0:28:37.119 --> 0:28:40.560
<v Speaker 1>She noticed what appeared to be a pulsing radio signal.

0:28:41.000 --> 0:28:45.480
<v Speaker 1>She and her supervisor charted the pulses that they were detecting,

0:28:45.880 --> 0:28:49.600
<v Speaker 1>and they were detecting them at regular intervals, like each day,

0:28:50.240 --> 0:28:55.360
<v Speaker 1>slightly off by hours or whatever. But it was it

0:28:55.440 --> 0:28:58.160
<v Speaker 1>was unusual. They weren't expecting it, and at the time

0:28:58.200 --> 0:29:00.360
<v Speaker 1>they didn't have an explanation for the origin of those

0:29:00.480 --> 0:29:03.479
<v Speaker 1>radio pulses, so they had to label it as something,

0:29:03.840 --> 0:29:06.600
<v Speaker 1>and at the time they labeled it l g M.

0:29:07.000 --> 0:29:12.560
<v Speaker 1>One l g M stood for Little Green Men. It

0:29:12.680 --> 0:29:15.000
<v Speaker 1>was a somewhat tongue in cheap way to indicate that,

0:29:15.480 --> 0:29:18.640
<v Speaker 1>I don't know, maybe this is purposeful radio broadcasting. We

0:29:18.720 --> 0:29:21.800
<v Speaker 1>don't know. They kept looking into it. They kept trying

0:29:21.800 --> 0:29:24.360
<v Speaker 1>to figure out exactly what it was and where the

0:29:24.400 --> 0:29:28.080
<v Speaker 1>signal was originating from, and over time they concluded that

0:29:28.120 --> 0:29:31.880
<v Speaker 1>it was actually a naturally occurring pulse. It was not

0:29:32.840 --> 0:29:37.320
<v Speaker 1>like an outgoing phone message from beyond the stars or something. Ultimately,

0:29:37.840 --> 0:29:39.959
<v Speaker 1>this hunch that they had that it was a naturally

0:29:40.040 --> 0:29:44.640
<v Speaker 1>occurring phenomenon proved correct, and scientists were able to figure

0:29:44.680 --> 0:29:48.040
<v Speaker 1>out that the pulse was coming from rotating neutron stars

0:29:48.120 --> 0:29:51.160
<v Speaker 1>called pulsars. So while it didn't turn out to be aliens,

0:29:51.200 --> 0:29:54.600
<v Speaker 1>astronomers were able to expand our understanding of space. So

0:29:54.640 --> 0:29:58.040
<v Speaker 1>it's still super cool. It just you know, it wasn't aliens.

0:29:58.720 --> 0:30:02.920
<v Speaker 1>Ohio State University launched the first long term set study

0:30:03.040 --> 0:30:06.720
<v Speaker 1>in nineteen seventy three, and unlike other attempts, this one

0:30:06.800 --> 0:30:11.240
<v Speaker 1>surveyed the entire night sky as the Earth rotated. Instead

0:30:11.320 --> 0:30:14.200
<v Speaker 1>of honing in on a specific region of space and

0:30:14.200 --> 0:30:17.040
<v Speaker 1>then just staying locked onto that region, it would do

0:30:17.120 --> 0:30:20.840
<v Speaker 1>a full scan every night, slightly different arc each night,

0:30:21.040 --> 0:30:24.240
<v Speaker 1>but a full scan of the night sky. In ninety seven,

0:30:24.560 --> 0:30:28.240
<v Speaker 1>that system registered a signal that was many times stronger

0:30:28.240 --> 0:30:31.840
<v Speaker 1>than the background signals that the telescope was recording. There

0:30:31.880 --> 0:30:35.120
<v Speaker 1>was an analyst named Jerry Emmon who wrote down the

0:30:35.120 --> 0:30:38.360
<v Speaker 1>word wow in the margin of the computer print out

0:30:38.440 --> 0:30:41.400
<v Speaker 1>for that detection, and to this day we call it

0:30:41.480 --> 0:30:45.040
<v Speaker 1>the Wow signal. And the signal had a profile that

0:30:45.080 --> 0:30:48.200
<v Speaker 1>suggested it wasn't your typical, naturally occurring radio wave, it

0:30:48.240 --> 0:30:52.840
<v Speaker 1>was this weird spike. But despite numerous efforts, the telescope

0:30:52.840 --> 0:30:55.840
<v Speaker 1>did not pick up any subsequent signals from that part

0:30:55.960 --> 0:30:59.640
<v Speaker 1>of space. Em and himself later guessed that perhaps the

0:30:59.680 --> 0:31:03.000
<v Speaker 1>signal originated from Earth. Maybe it was something that got

0:31:03.280 --> 0:31:06.320
<v Speaker 1>beamed up and then reflected off of something in space,

0:31:06.360 --> 0:31:09.480
<v Speaker 1>like a piece of space debris, and thus it didn't

0:31:09.560 --> 0:31:13.760
<v Speaker 1>originate from, you know, extraterrestrial sources at all, but we

0:31:13.840 --> 0:31:18.360
<v Speaker 1>don't know for sure. Astronomers oversaw similar efforts with different

0:31:18.440 --> 0:31:21.040
<v Speaker 1>radio telescopes around the world over the years, and it's

0:31:21.080 --> 0:31:25.240
<v Speaker 1>a bit tricky because it requires securing time on radio

0:31:25.280 --> 0:31:29.080
<v Speaker 1>telescopes for the purposes of searching for extra terrestrial intelligence,

0:31:29.400 --> 0:31:34.040
<v Speaker 1>and the owners of those telescopes, frequently scientific research institutions

0:31:34.120 --> 0:31:37.440
<v Speaker 1>universities that kind of thing. They often have their own priorities,

0:31:37.560 --> 0:31:40.240
<v Speaker 1>which may or may not involve seeking out evidence of

0:31:40.280 --> 0:31:44.040
<v Speaker 1>intelligent life in the galaxy, so finding time when you

0:31:44.120 --> 0:31:47.640
<v Speaker 1>can use those radio telescopes is pretty tricky stuff. In

0:31:49.160 --> 0:31:52.880
<v Speaker 1>Thomas Pearson and Jill Tarter found the not for profit

0:31:53.000 --> 0:31:56.440
<v Speaker 1>organization called the City Institute with the mission to understand

0:31:56.480 --> 0:32:00.200
<v Speaker 1>life and a sort of universal context. So again, while

0:32:00.200 --> 0:32:03.000
<v Speaker 1>there is a set organization, SET as a whole really

0:32:03.040 --> 0:32:07.720
<v Speaker 1>refers to the science the effort, the specific application of

0:32:08.320 --> 0:32:12.160
<v Speaker 1>techniques and processes, and an effort to attain a particular outcome,

0:32:12.240 --> 0:32:17.200
<v Speaker 1>namely to find evidence of extraterrestrial intelligence. Astronomers interested in

0:32:17.240 --> 0:32:20.520
<v Speaker 1>pursuing goals related to SET often have to wait for

0:32:20.600 --> 0:32:23.600
<v Speaker 1>times when radio telescopes aren't in active use for some

0:32:23.760 --> 0:32:26.800
<v Speaker 1>other purpose, and that really limits what they can accomplish.

0:32:27.360 --> 0:32:31.800
<v Speaker 1>Other groups have to developed a way to piggyback onto

0:32:32.320 --> 0:32:37.440
<v Speaker 1>existing radio telescopes. So piggyback systems tend to be systems

0:32:37.480 --> 0:32:41.640
<v Speaker 1>that monitor data picked up by a radio telescope, so

0:32:41.680 --> 0:32:46.280
<v Speaker 1>it's like it's like an additional computer readout of what's

0:32:46.320 --> 0:32:49.760
<v Speaker 1>going on. So the team that's using the radio telescope

0:32:49.800 --> 0:32:53.040
<v Speaker 1>is doing it to do some specific purpose. Meanwhile, SET

0:32:53.280 --> 0:32:58.400
<v Speaker 1>researchers are using a a parallel readoubt just looking for

0:32:58.440 --> 0:33:02.040
<v Speaker 1>anything that might stand out as a potential example of

0:33:02.200 --> 0:33:06.760
<v Speaker 1>evidence for extraterrestrial intelligence. Uh, this is tricky because again

0:33:06.880 --> 0:33:12.400
<v Speaker 1>the set researchers have no say on where a telescope

0:33:12.400 --> 0:33:14.760
<v Speaker 1>is going to be pointed. They're just looking at the

0:33:14.800 --> 0:33:19.480
<v Speaker 1>same data but for a different reason, So it's not ideal.

0:33:19.800 --> 0:33:23.120
<v Speaker 1>But again, radio telescopes are kind of hard to come by.

0:33:23.240 --> 0:33:27.880
<v Speaker 1>Even with all these limitations, scientists were generating a lot

0:33:27.920 --> 0:33:31.400
<v Speaker 1>of information that they needed to sift through. Radio telescopes

0:33:31.440 --> 0:33:34.360
<v Speaker 1>pick up a lot of noise, and there may be

0:33:34.560 --> 0:33:36.520
<v Speaker 1>signal in that noise. I mean, that signal might be

0:33:36.560 --> 0:33:40.760
<v Speaker 1>incredibly weak. But you have to really examine the data

0:33:40.800 --> 0:33:43.880
<v Speaker 1>closely in order to figure out what is truly a

0:33:43.920 --> 0:33:47.480
<v Speaker 1>signal versus just random noise in the background. And then

0:33:47.520 --> 0:33:49.680
<v Speaker 1>you have to weed out all the other stuff like

0:33:50.040 --> 0:33:53.560
<v Speaker 1>did that signal come from a natural phenomenon? Did it

0:33:53.760 --> 0:33:58.239
<v Speaker 1>come from a terrestrial source? This is not easy to do.

0:33:58.760 --> 0:34:01.520
<v Speaker 1>Scientists were already have to work pretty hard to secure

0:34:01.560 --> 0:34:04.160
<v Speaker 1>time with radio telescopes. It would be even harder to

0:34:04.280 --> 0:34:08.480
<v Speaker 1>secure time with something like a supercomputer because supercomputers also

0:34:08.960 --> 0:34:13.000
<v Speaker 1>are owned by just a few different universities and research

0:34:13.080 --> 0:34:16.560
<v Speaker 1>organizations and labs, and they typically are being used for

0:34:16.640 --> 0:34:20.040
<v Speaker 1>other stuff that takes a higher priority than searching for

0:34:20.239 --> 0:34:24.200
<v Speaker 1>extraterrestrial intelligence. And then there was a breakthrough, and that

0:34:24.280 --> 0:34:27.560
<v Speaker 1>breakthrough came in the form of network connectivity. In the

0:34:27.560 --> 0:34:31.440
<v Speaker 1>early nineteen nineties, the mainstream public first began learning about

0:34:31.560 --> 0:34:37.319
<v Speaker 1>this weird thing called the Internet, and by the Internet was,

0:34:37.800 --> 0:34:41.000
<v Speaker 1>if not a household term, at least something most folks

0:34:41.040 --> 0:34:45.160
<v Speaker 1>had some experience or knowledge of, and that's what opened

0:34:45.239 --> 0:34:48.759
<v Speaker 1>up the opportunity for study at home. I'll explain more

0:34:48.800 --> 0:34:51.360
<v Speaker 1>in just a minute, but first let's take another quick break.

0:34:58.760 --> 0:35:04.120
<v Speaker 1>So they there are many different models for computing. When

0:35:04.160 --> 0:35:06.680
<v Speaker 1>I was growing up, I was familiar with a more

0:35:06.880 --> 0:35:10.080
<v Speaker 1>centralized model. So in my case, I was growing up

0:35:10.080 --> 0:35:13.400
<v Speaker 1>in the era of personal computers, and the computers I

0:35:13.440 --> 0:35:17.319
<v Speaker 1>first used were completely self contained. They didn't connect to

0:35:17.560 --> 0:35:22.080
<v Speaker 1>a larger network. All the processing capability, all the programs,

0:35:22.120 --> 0:35:25.560
<v Speaker 1>all the capacity for storage. We're connected to the physical

0:35:25.640 --> 0:35:28.680
<v Speaker 1>computer itself. They might be peripherals, but it was all

0:35:28.760 --> 0:35:32.880
<v Speaker 1>part of the personal computer. A few years ago, the

0:35:32.880 --> 0:35:36.200
<v Speaker 1>big trend was cloud computing. So with cloud computing, you've

0:35:36.239 --> 0:35:38.799
<v Speaker 1>got networked servers that are doing a lot of the

0:35:38.840 --> 0:35:43.400
<v Speaker 1>processing power for big applications. The devices we're using, whether

0:35:43.480 --> 0:35:47.160
<v Speaker 1>they're computers or mobile devices or sensors or whatever, are

0:35:47.239 --> 0:35:51.480
<v Speaker 1>mostly acting as transmitters and receivers. For many tasks. We

0:35:51.600 --> 0:35:56.120
<v Speaker 1>provide input to these devices, and the device than transmits

0:35:56.560 --> 0:35:59.480
<v Speaker 1>commands to some distant group of servers that takes that

0:35:59.520 --> 0:36:03.880
<v Speaker 1>information and does some sort of operation on it, produces

0:36:03.920 --> 0:36:06.560
<v Speaker 1>some sort of result, and sends that back to us.

0:36:07.080 --> 0:36:09.640
<v Speaker 1>So no longer do we have to have really powerful

0:36:09.680 --> 0:36:13.840
<v Speaker 1>computers directly at our disposal. We can rely on cloud

0:36:13.880 --> 0:36:16.160
<v Speaker 1>services to do that computing for us, at least for

0:36:16.200 --> 0:36:19.000
<v Speaker 1>some things. For other things, like if you want to

0:36:19.040 --> 0:36:26.200
<v Speaker 1>do low latency, high graphics fidelity gaming, for example, you

0:36:26.239 --> 0:36:29.440
<v Speaker 1>want to have a really good, strong computer processor at

0:36:29.440 --> 0:36:34.200
<v Speaker 1>your disposal because latency with transmission can completely ruin that experience.

0:36:34.239 --> 0:36:36.520
<v Speaker 1>But for the most part, you get what I'm saying well.

0:36:37.120 --> 0:36:39.560
<v Speaker 1>Setting at Home was an example of sort of a

0:36:39.640 --> 0:36:44.319
<v Speaker 1>third model called distributed computing. The idea was that you

0:36:44.360 --> 0:36:47.360
<v Speaker 1>could take a group of regular, old personal computers, the

0:36:47.440 --> 0:36:51.359
<v Speaker 1>kind that any average person could have in their home.

0:36:51.920 --> 0:36:55.160
<v Speaker 1>You would install some software on those computers, and that

0:36:55.280 --> 0:36:58.680
<v Speaker 1>software would allow the computers to process chunks of data

0:36:58.920 --> 0:37:02.719
<v Speaker 1>in some particular a before sending the results back to

0:37:02.800 --> 0:37:05.160
<v Speaker 1>wherever that data was coming from in the first place.

0:37:05.400 --> 0:37:09.320
<v Speaker 1>So if someone needed to tackle a really big data

0:37:09.400 --> 0:37:13.880
<v Speaker 1>processing job, one that could be divided up into smaller chunks,

0:37:14.360 --> 0:37:17.239
<v Speaker 1>that person could use a centralized computer or maybe a

0:37:17.280 --> 0:37:20.520
<v Speaker 1>network of computers to send out these smaller chunks of

0:37:20.600 --> 0:37:25.960
<v Speaker 1>data to this distribution of personal computers for processing and

0:37:26.000 --> 0:37:28.120
<v Speaker 1>then wait for the results to come back and then

0:37:28.360 --> 0:37:30.799
<v Speaker 1>group them all together and see what you got. It

0:37:30.880 --> 0:37:34.880
<v Speaker 1>speeds things up considerably. It increases the processing assets of

0:37:34.880 --> 0:37:38.560
<v Speaker 1>the project as more computers joined that project, and it

0:37:38.600 --> 0:37:42.839
<v Speaker 1>reduces the need to turn to stuff like supercomputers. And

0:37:42.840 --> 0:37:46.600
<v Speaker 1>it also achieved another goal which the founders of the

0:37:46.600 --> 0:37:50.000
<v Speaker 1>project had in mind, which was to encourage enthusiasm and

0:37:50.120 --> 0:37:57.000
<v Speaker 1>excitement around the subject of science. Computer scientist David Gedgay,

0:37:57.040 --> 0:38:01.879
<v Speaker 1>astronomers Woody Sullivan and Dan Wertheimer, and David Anderson, who

0:38:01.960 --> 0:38:06.000
<v Speaker 1>was David's graduate school advisor collectively came up with this

0:38:06.080 --> 0:38:11.919
<v Speaker 1>idea all the way back in specifically with set at Home.

0:38:12.000 --> 0:38:15.520
<v Speaker 1>They were trying to come up with a scientific application

0:38:16.040 --> 0:38:20.239
<v Speaker 1>people would be excited to participate in, and while they

0:38:20.239 --> 0:38:26.840
<v Speaker 1>weren't necessarily super optimistic, that set at home would produce,

0:38:27.080 --> 0:38:31.160
<v Speaker 1>you know, incredible results from a scientific perspective. They thought

0:38:31.160 --> 0:38:34.360
<v Speaker 1>from a motivating perspective, it was just the ticket, and

0:38:34.400 --> 0:38:38.080
<v Speaker 1>it was pretty genius. Upon launch, anyone with a computer

0:38:38.200 --> 0:38:41.400
<v Speaker 1>and an Internet connection could conceivably help in the search

0:38:41.480 --> 0:38:46.880
<v Speaker 1>for extraterrestrial intelligence. The researchers created a screen saver program,

0:38:46.960 --> 0:38:49.880
<v Speaker 1>so if you wanted to participate, you could download the

0:38:49.920 --> 0:38:53.759
<v Speaker 1>screen saver and install it on your personal computer. When

0:38:53.800 --> 0:38:56.960
<v Speaker 1>your computer would go idle and activate the screen saver,

0:38:57.719 --> 0:39:00.879
<v Speaker 1>the processor of your computer, which wise would be doing

0:39:01.160 --> 0:39:04.600
<v Speaker 1>very little, would get to work on some data sent

0:39:04.760 --> 0:39:08.480
<v Speaker 1>over from the set research project. So the research project

0:39:08.520 --> 0:39:13.200
<v Speaker 1>would pull information from a radio telescope divided into chunks

0:39:13.280 --> 0:39:16.440
<v Speaker 1>and then parcel it out to people participating in this

0:39:16.480 --> 0:39:20.160
<v Speaker 1>project when complete. When your processor was done working on

0:39:20.160 --> 0:39:22.720
<v Speaker 1>a chunk of data, it would send the results back

0:39:23.040 --> 0:39:25.920
<v Speaker 1>to the central point for the project and wait for

0:39:25.960 --> 0:39:28.040
<v Speaker 1>the next chunk of data. And if you were to

0:39:28.120 --> 0:39:30.520
<v Speaker 1>come back to do some work on your computer, Let's

0:39:30.520 --> 0:39:32.960
<v Speaker 1>say you come back after taking a break for half

0:39:33.000 --> 0:39:36.359
<v Speaker 1>an hour, the screensaver goes inactive and the program would

0:39:36.400 --> 0:39:39.799
<v Speaker 1>surrender your processing cycles back to you, so you didn't

0:39:39.800 --> 0:39:42.279
<v Speaker 1>have to worry about cet at Home suddenly taking up

0:39:42.320 --> 0:39:45.319
<v Speaker 1>all of your computers processing power. It would only jump

0:39:45.400 --> 0:39:48.040
<v Speaker 1>back onto the job when your computer went idle again

0:39:48.480 --> 0:39:53.200
<v Speaker 1>and your your CPU had availability. Now, as I said,

0:39:53.239 --> 0:39:56.239
<v Speaker 1>this idea was genius, but the original implementation of the

0:39:56.280 --> 0:40:00.080
<v Speaker 1>idea was less. So now that's not a slight on

0:40:00.120 --> 0:40:05.600
<v Speaker 1>the researchers, because when they launched the project in May,

0:40:05.880 --> 0:40:08.759
<v Speaker 1>they were expecting that they might get as many as

0:40:08.760 --> 0:40:13.000
<v Speaker 1>a thousand people signing up. They figured that, well, this

0:40:13.040 --> 0:40:15.800
<v Speaker 1>is an interesting idea, and we'll probably see some folks

0:40:15.920 --> 0:40:18.440
<v Speaker 1>really you know, who are really into science joined, but

0:40:18.560 --> 0:40:23.920
<v Speaker 1>I'm not sure about anything beyond that. Now, with that expectation,

0:40:24.480 --> 0:40:29.040
<v Speaker 1>they only dedicated a single desktop PC for the purposes

0:40:29.120 --> 0:40:32.799
<v Speaker 1>of assigning processing tasks and receiving the results from the

0:40:32.840 --> 0:40:37.440
<v Speaker 1>distributed computers. They did not anticipate how enthusiastic the reception

0:40:37.480 --> 0:40:41.880
<v Speaker 1>to the project would be. They didn't see a thousand

0:40:41.920 --> 0:40:45.440
<v Speaker 1>people sign up when they launched Setting at Home. They

0:40:45.440 --> 0:40:48.600
<v Speaker 1>saw a million people sign up. So let's put that

0:40:48.640 --> 0:40:51.840
<v Speaker 1>into perspective. Let's say you've set up a lemonade stand

0:40:51.920 --> 0:40:55.360
<v Speaker 1>and you did some brief scouting work, and you anticipated

0:40:55.480 --> 0:40:58.319
<v Speaker 1>that the location you're setting up in. You're gonna see

0:40:58.360 --> 0:41:02.160
<v Speaker 1>maybe ten customers and third minutes, and you think that's manageable. Well,

0:41:02.200 --> 0:41:05.000
<v Speaker 1>what you didn't realize is that you've actually set up

0:41:05.040 --> 0:41:08.879
<v Speaker 1>your stand in sour puss scurvy town. It's a town

0:41:08.920 --> 0:41:13.200
<v Speaker 1>populated entirely by people with an unquenchable thirst for lemonade.

0:41:13.560 --> 0:41:15.919
<v Speaker 1>So instead of ten people showing up in that first

0:41:15.920 --> 0:41:20.359
<v Speaker 1>half hour, ten thousand people mob your lemonade stand. You

0:41:20.400 --> 0:41:23.560
<v Speaker 1>are overwhelmed. Well, the same thing happened to the ct

0:41:23.760 --> 0:41:26.640
<v Speaker 1>at Home PC that was in charge of sending out

0:41:26.640 --> 0:41:29.240
<v Speaker 1>and receiving all that data. It was a good problem

0:41:29.239 --> 0:41:33.520
<v Speaker 1>to have, but it was still a problem. Sun Microsystems

0:41:33.600 --> 0:41:36.359
<v Speaker 1>jumped in and donated a bunch of computers to help

0:41:36.400 --> 0:41:40.440
<v Speaker 1>the City at Home administrators make the system work, and

0:41:40.480 --> 0:41:43.360
<v Speaker 1>from that moment on the program went into high gear.

0:41:43.840 --> 0:41:47.799
<v Speaker 1>People in the program were contributing to scientific exploration just

0:41:47.960 --> 0:41:52.319
<v Speaker 1>by allowing their IDOL computers to focus on complicated mathematical

0:41:52.320 --> 0:41:55.239
<v Speaker 1>problems when the computer was otherwise not in use. It

0:41:55.280 --> 0:41:57.960
<v Speaker 1>was a beautiful thing. The response also meant that the

0:41:58.000 --> 0:42:02.799
<v Speaker 1>project could go through information orders of magnitude faster than

0:42:02.840 --> 0:42:05.839
<v Speaker 1>if it had all been handled in house. The they

0:42:05.840 --> 0:42:09.239
<v Speaker 1>had the advantage of a million processors. That's something that

0:42:09.320 --> 0:42:12.120
<v Speaker 1>no SETI project could have afforded on its own at

0:42:12.160 --> 0:42:16.400
<v Speaker 1>that time. It also inspired other scientific projects to launch

0:42:16.480 --> 0:42:21.080
<v Speaker 1>distributed computing efforts. Folding at Home, for example, taps into

0:42:21.120 --> 0:42:24.680
<v Speaker 1>idle computers to solve protein folding problems that could lead

0:42:24.680 --> 0:42:28.799
<v Speaker 1>to incredible advances in medicine and biology. On top of that,

0:42:29.320 --> 0:42:33.759
<v Speaker 1>online communities formed around Seat at Home. People connected over

0:42:33.880 --> 0:42:37.440
<v Speaker 1>forums and formed friendships. There were even stories about people

0:42:37.600 --> 0:42:41.560
<v Speaker 1>meeting online, falling in love, and getting married out in

0:42:41.600 --> 0:42:44.640
<v Speaker 1>the real world, all while using their computers to seek

0:42:44.640 --> 0:42:49.440
<v Speaker 1>out evidence of intelligent life. It was all really remarkable

0:42:49.520 --> 0:42:53.160
<v Speaker 1>and beautiful. But hey, if it was so super cool,

0:42:53.640 --> 0:42:56.200
<v Speaker 1>why the heck is the project shutting down now? Twenty

0:42:56.280 --> 0:42:59.440
<v Speaker 1>one years after it launched? Is the book closed on

0:42:59.640 --> 0:43:04.279
<v Speaker 1>extra terrestrial intelligent life? Are we done? Have we given up? Well?

0:43:04.280 --> 0:43:08.239
<v Speaker 1>Not quite. The problem now is that we've got a

0:43:08.320 --> 0:43:13.200
<v Speaker 1>ton a mountain of processed data from this project that

0:43:13.360 --> 0:43:16.800
<v Speaker 1>has to be further analyzed, and that taps into something

0:43:16.840 --> 0:43:19.400
<v Speaker 1>else that I plan to talk about more later on

0:43:19.480 --> 0:43:23.400
<v Speaker 1>this year, the challenges of big data. We're able to

0:43:23.400 --> 0:43:29.359
<v Speaker 1>collect mind staggeringly huge amounts of information, but understanding and

0:43:29.480 --> 0:43:33.240
<v Speaker 1>using that information is another matter. It presents a really

0:43:33.360 --> 0:43:38.680
<v Speaker 1>big challenge. Even with all of these analyzed chunks of info,

0:43:39.200 --> 0:43:41.880
<v Speaker 1>that data still has to be processed to see what's

0:43:41.880 --> 0:43:45.399
<v Speaker 1>actually been found over the two decades of Seating at Home.

0:43:46.320 --> 0:43:49.560
<v Speaker 1>The researchers overseeing Ceting at Home hope to publish a

0:43:49.680 --> 0:43:53.239
<v Speaker 1>paper on the subject, and to do that, they need

0:43:53.280 --> 0:43:55.719
<v Speaker 1>to look at all the results of the stuff that

0:43:55.840 --> 0:43:59.360
<v Speaker 1>the program actually found, and so they need to stop

0:43:59.520 --> 0:44:03.120
<v Speaker 1>gathering data while that happens. They have to actually stop

0:44:03.160 --> 0:44:05.280
<v Speaker 1>so that they can see what they have, as opposed

0:44:05.320 --> 0:44:09.399
<v Speaker 1>to continuously adding to that pile. This hiatus will allow

0:44:09.440 --> 0:44:12.600
<v Speaker 1>the team to look at the results, form conclusions, and

0:44:12.640 --> 0:44:15.560
<v Speaker 1>write a paper based on the whole project. And while

0:44:15.560 --> 0:44:19.640
<v Speaker 1>we don't anticipate any reports of intelligent communications popping up

0:44:19.680 --> 0:44:22.360
<v Speaker 1>as a result of this analysis, the endeavor as a

0:44:22.440 --> 0:44:27.080
<v Speaker 1>whole has been really successful, particularly in the context of

0:44:27.120 --> 0:44:31.359
<v Speaker 1>getting people excited about participating in science. On the back

0:44:31.480 --> 0:44:35.120
<v Speaker 1>end of Seating at Home is an infrastructure that grew

0:44:35.320 --> 0:44:39.359
<v Speaker 1>over time. It is called the Berkeley Open Infrastructure for

0:44:39.440 --> 0:44:45.440
<v Speaker 1>Network Computing. This support system hosts numerous distributed computing projects

0:44:45.520 --> 0:44:48.919
<v Speaker 1>that work on the same basic principles as setting at home.

0:44:49.239 --> 0:44:52.240
<v Speaker 1>It's just that each of these projects have a different

0:44:52.480 --> 0:44:56.280
<v Speaker 1>goal or purpose. Some are dedicated to detecting and measuring

0:44:56.320 --> 0:45:01.000
<v Speaker 1>asteroids uh. Some provide cern process us in capabilities to

0:45:01.000 --> 0:45:04.239
<v Speaker 1>help analyze data produced by the Large Hadron Collider in

0:45:04.280 --> 0:45:06.600
<v Speaker 1>an effort to gain, you know, a deeper understanding of

0:45:06.640 --> 0:45:10.360
<v Speaker 1>particle physics and quantum mechanics. There are projects that focus

0:45:10.400 --> 0:45:15.080
<v Speaker 1>on climate science, physics, cognitive science, and more, and you

0:45:15.120 --> 0:45:19.280
<v Speaker 1>can check them all out at blink dot Berkeley, dot

0:45:19.280 --> 0:45:23.800
<v Speaker 1>e d U, slash projects dot PHP. That's b O

0:45:24.320 --> 0:45:28.920
<v Speaker 1>I n C dot Berkeley, dot E d U, slash

0:45:29.239 --> 0:45:32.880
<v Speaker 1>projects dot p HP. If you want to dedicate some

0:45:32.960 --> 0:45:38.160
<v Speaker 1>of your computer's idle processing power to solving really interesting

0:45:38.280 --> 0:45:41.799
<v Speaker 1>problems and science, it's a great way to contribute. You're

0:45:41.840 --> 0:45:45.160
<v Speaker 1>not even doing anything active, but you are helping, you know,

0:45:45.920 --> 0:45:51.000
<v Speaker 1>peel back the border of our understanding. We're pushing that

0:45:51.080 --> 0:45:53.840
<v Speaker 1>boundary further and further out, and you can do it

0:45:53.920 --> 0:45:57.319
<v Speaker 1>just with your computer's idle time. It's pretty incredible. So

0:45:57.400 --> 0:45:59.840
<v Speaker 1>while study at home is writing off into the sunset,

0:46:00.120 --> 0:46:03.840
<v Speaker 1>at least for a while. Anyway, there are still efforts

0:46:03.880 --> 0:46:07.080
<v Speaker 1>around the world dedicated in full or in part to

0:46:07.200 --> 0:46:11.359
<v Speaker 1>the search for extraterrestrial life. The search hasn't ended yet,

0:46:11.440 --> 0:46:15.200
<v Speaker 1>even if Set at Home is at least for now over,

0:46:15.719 --> 0:46:18.680
<v Speaker 1>And while we don't have anything jumping out to us

0:46:18.719 --> 0:46:22.439
<v Speaker 1>as a positive, absolutely yes, we need to check this out.

0:46:22.520 --> 0:46:25.719
<v Speaker 1>We're pretty sure someone's talking to us kind of uh incident.

0:46:27.000 --> 0:46:32.160
<v Speaker 1>It's good to remember that space is really big. Who knows,

0:46:32.440 --> 0:46:35.560
<v Speaker 1>maybe the next star we point a telescope at will

0:46:35.600 --> 0:46:38.600
<v Speaker 1>be beaming. Whatever the alien version of the Great British

0:46:38.760 --> 0:46:43.080
<v Speaker 1>Bake Off is, one can only hope. And that wraps

0:46:43.160 --> 0:46:46.680
<v Speaker 1>up this episode of tech stuff. My hat is off

0:46:46.920 --> 0:46:49.840
<v Speaker 1>to the CET at Home crew. I think it was

0:46:49.920 --> 0:46:53.480
<v Speaker 1>an admirable use of technology to inspire people to get

0:46:53.520 --> 0:46:58.440
<v Speaker 1>into science. I think it was a worthy endeavor to

0:46:58.520 --> 0:47:01.520
<v Speaker 1>search for extraterrestrial and telligence. It was great to see

0:47:01.920 --> 0:47:05.120
<v Speaker 1>other projects take that same model and apply it to

0:47:05.200 --> 0:47:10.200
<v Speaker 1>their own uh scientific endeavors. So it's to me one

0:47:10.200 --> 0:47:13.760
<v Speaker 1>of those great stories in technology. Even if we didn't

0:47:13.840 --> 0:47:16.879
<v Speaker 1>find any direct evidence of little green men out there,

0:47:17.400 --> 0:47:19.680
<v Speaker 1>who knows what the future will bring. If you guys

0:47:19.680 --> 0:47:23.120
<v Speaker 1>have any suggestions for future topics, for tech Stuff reach

0:47:23.160 --> 0:47:26.320
<v Speaker 1>out to me. You can find me on Facebook or Twitter.

0:47:26.520 --> 0:47:30.120
<v Speaker 1>The handle for both is tech Stuff HSW and I'll

0:47:30.120 --> 0:47:38.000
<v Speaker 1>talk to you again really soon. Text Stuff is an

0:47:38.000 --> 0:47:41.720
<v Speaker 1>I Heart Radio production. For more podcasts from My Heart Radio,

0:47:42.040 --> 0:47:45.200
<v Speaker 1>visit the i Heart Radio app, Apple Podcasts, or wherever

0:47:45.320 --> 0:47:46.840
<v Speaker 1>you listen to your favorite shows.