WEBVTT - Is There Anybody Out There?

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<v Speaker 1>Brought to you by Toyota. Let's go places. Welcome to

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<v Speaker 1>Forward Thinking. Hey there, everyone, and welcome to Forward Thinking,

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<v Speaker 1>the podcast that looks at the future and says my

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<v Speaker 1>supersonic ships at your disposal. I'm Jonathan Strickland, I'm Lauren,

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<v Speaker 1>and I'm Joe McCormick. And today we want to talk

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<v Speaker 1>a little bit about who who to thunk its space

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<v Speaker 1>Space space, something that we have touched on once or

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<v Speaker 1>twice on this show, but we specifically wanted to look

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<v Speaker 1>at the potential of extraterrestrial life. We've already decided what

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<v Speaker 1>they look like, right, we had that podcast. Yeah, most

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<v Speaker 1>statistically probable alien life formance according to Joe. So the

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<v Speaker 1>the French aliens called the cone heads are what they're

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<v Speaker 1>gonna look like. But we haven't actually gotten in touch

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<v Speaker 1>with them yet. And we want to talk about some um,

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<v Speaker 1>some some things that that scientists and researchers have proposed

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<v Speaker 1>over the years as a kind of a method to

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<v Speaker 1>figure out how probable is it that we will that

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<v Speaker 1>there are other intelligence species out there and that we're

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<v Speaker 1>going to come in contact with them eventually. Right, everybody

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<v Speaker 1>goes with their gut, don't they? You know, they say

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<v Speaker 1>do you think that there's life out there? And you

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<v Speaker 1>kind of go, well, I don't know. You're like you're

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<v Speaker 1>answering with the part of yourself that decides whether or

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<v Speaker 1>not you want ice cream right now. So the answer

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<v Speaker 1>can change depending upon how hot it is outside and

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<v Speaker 1>whether you and you're not really doing the math in

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<v Speaker 1>your head. I mean, it's it's not the same kind

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<v Speaker 1>of probability with which you would, you know, if you're

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<v Speaker 1>if you're my friends play poker or or a dice

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<v Speaker 1>gambling game or something like that, You're you're more you're

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<v Speaker 1>more going like yeah, totally, or like now we're answering.

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<v Speaker 1>We're answering with our feelings. Um, yeah, But when those

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<v Speaker 1>feelings incorporate things like the more you know about the universe,

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<v Speaker 1>the more you think, well, if considering how enormous it

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<v Speaker 1>is and how much potential there is, and the fact

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<v Speaker 1>that life does exist is where proof, then how likely

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<v Speaker 1>is it to have happened at least one other time?

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<v Speaker 1>And most of us feel like it's pretty likely. Well,

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<v Speaker 1>what if we were to narrow the question down a

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<v Speaker 1>little bit too, something that's a little bit um more

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<v Speaker 1>manageable and more testable than just is their other life?

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<v Speaker 1>You mean, like if we were to come up with

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<v Speaker 1>some sort of crazy equation where we could perhaps determine

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<v Speaker 1>the likelihood that intelligent life out there would exist. Yeah,

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<v Speaker 1>And to limit the product of the equation, say, instead

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<v Speaker 1>of asking is there life out there somewhere? What if

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<v Speaker 1>we were to ask how many civilizations are there in

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<v Speaker 1>our galaxy? That's the milky capable of communicating across solar systems,

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<v Speaker 1>all right, So some sort of interstellar communication, we'd probably

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<v Speaker 1>be talking about radio or maybe lasers. So we'd have

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<v Speaker 1>to be able to detect it, obviously, because if we're

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<v Speaker 1>not able to detect it, there could be all sorts

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<v Speaker 1>of communication going on that we're just unaware of. Right,

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<v Speaker 1>we're ruling out, you know, really intelligent psychic materia that

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<v Speaker 1>that only only communicate via color flash or germ thoughts

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<v Speaker 1>or something. Yeah. Another way of phrasing this is to

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<v Speaker 1>say technological civilizations. How many technological civilizations are there in

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<v Speaker 1>the Milky Way other than us? Obviously we know about one. Well,

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<v Speaker 1>is there a way we could actually start to concert

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<v Speaker 1>this a bit, to think about real numbers that would

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<v Speaker 1>inform our judgment of that probability? Well, according to Frank Drake, yes,

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<v Speaker 1>there is, or at least he proposed a way of

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<v Speaker 1>thinking about the problem that might be able to give

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<v Speaker 1>you at least a likelihood. Although depending on how you

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<v Speaker 1>look at this equation, your mileage berries right, you're talking

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<v Speaker 1>about the Drake equation. Yes, right. What's the Drake equation? Well, essentially,

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<v Speaker 1>it's an equation that predicts the potential number of civilizations

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<v Speaker 1>in the galaxy to have the capability to communicate via

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<v Speaker 1>radio transmission or other interstellar communication that we could actually detect.

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<v Speaker 1>So it actually takes into account lots of different factors.

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<v Speaker 1>This is something that Frank Drake came up with in

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<v Speaker 1>nineteen sixty one when he was trying to get fellow

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<v Speaker 1>astronomers to convene for the first serious um A conference

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<v Speaker 1>on the search for extraterrestrial life, which would become set,

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<v Speaker 1>which is something that we actually haven't talked that much

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<v Speaker 1>about before, I don't think on this podcast. No, crazily

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<v Speaker 1>enough um And And Frank Drake was pretty young at

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<v Speaker 1>the time. I think he was thirty or thirty one.

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<v Speaker 1>He had begun his career as an electronics officer in

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<v Speaker 1>the Navy, partially because he had a he had gotten

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<v Speaker 1>a scholarship to go to Cornell for electronics from his

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<v Speaker 1>RTC and he would go on to get a master's

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<v Speaker 1>in a PhD in astronomy from Harvard and worked there

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<v Speaker 1>by chance his first summer with radio astronomy equipment and

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<v Speaker 1>absolutely fell in love with it. In nineteen fifty nine

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<v Speaker 1>he would help discover Jupiter's radiation belts and observe some pulsars,

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<v Speaker 1>and then in nineteen sixty uh he was working with

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<v Speaker 1>radio telescopes at the National Radio Astronomy Observatory and Green Bank,

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<v Speaker 1>West vir West Virginia, where he form to the very

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<v Speaker 1>first experimental search for radio signals from potential civilizations in

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<v Speaker 1>nearby stars. Yeah. He's also the guy who, along with

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<v Speaker 1>Carl Sagan, helped design the plaque aboard the Pioneer spacecraft

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<v Speaker 1>right right. And the seventies, he was working a lot

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<v Speaker 1>with Carl Sagan. Carl Sagan was a huge proponent of

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<v Speaker 1>the Drake equation. The two of them got along pretty

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<v Speaker 1>famously and they even helped. They even collaborated. They dropped

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<v Speaker 1>a record together, only two copies of which exist and

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<v Speaker 1>both of them are outside well the system now, but

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<v Speaker 1>it totally it did go gold but not platinum. Not

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<v Speaker 1>platinum ones outside the Solar System, and one is on

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<v Speaker 1>its way out. We're talking, of course about the Golden

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<v Speaker 1>records aboard the Voyager spacecraft. Both UH Sagan and UH

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<v Speaker 1>and Drake had a hand in the design of those. Uh.

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<v Speaker 1>Those are sort of our own feeble in a way,

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<v Speaker 1>attempts at communicating with an alien civilization. But of course

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<v Speaker 1>they're not the best ways we could communicate. The best

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<v Speaker 1>ways would be via a radio transmission, or if that

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<v Speaker 1>can travel at the speed of light, and or you know,

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<v Speaker 1>perhaps even better, if we could find a planet that

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<v Speaker 1>we were pretty sure had life capable of receiving a

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<v Speaker 1>signal on it and focus a an optical beam at them.

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<v Speaker 1>That would that would be even more In fact, NASA,

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<v Speaker 1>as of the recording this podcast, NASA had just had

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<v Speaker 1>just proven the feasibility of using lasers in space communication

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<v Speaker 1>and showing that it had a much higher capacity for

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<v Speaker 1>carrying data than radio transmission. Right. But but again, that's

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<v Speaker 1>within an extremely narrow location. She really have to be

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<v Speaker 1>pointing it at something. Yeah, it's we're talking line of sight, right,

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<v Speaker 1>so anyway, but either way we would have to we

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<v Speaker 1>would have to be able to get something back from

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<v Speaker 1>whatever intelligent races out there for that to be a

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<v Speaker 1>confirmation that in fact, some other intelligent race has exists

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<v Speaker 1>in the Milky Way. Okay, well, before we talk about

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<v Speaker 1>the search itself, let's talk about the equation and how

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<v Speaker 1>they used it to play this game and see if

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<v Speaker 1>we could predict how many civilizations are out there in

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<v Speaker 1>our galaxy. All right, because what's really fascinating to me

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<v Speaker 1>is that when Drake was designing this equation, we had

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<v Speaker 1>not detected any exit planets at all. That wouldn't be

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<v Speaker 1>until the nineteen nineties. So and now we've detected about

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<v Speaker 1>a thousand of them. But even so, I mean that's

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<v Speaker 1>direct detection, we of course suspect that there are a

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<v Speaker 1>wicked lot of of them out there, that maybe at

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<v Speaker 1>least half of star systems, is what Drake said himself

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<v Speaker 1>in about so uh so. So yeah, So the equation

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<v Speaker 1>is n N being this number of civilizations that could

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<v Speaker 1>that are advanced enough to create technology that we could

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<v Speaker 1>listen to. Um equals are being the rate of star

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<v Speaker 1>formation in the galaxy. Okay, so that's how often the

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<v Speaker 1>galaxy creates new stars that you have planets, right, uh

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<v Speaker 1>f subset P, which is the fraction of stars that

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<v Speaker 1>form planets. So not every star necessarily has a planet

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<v Speaker 1>attached to it, so you have to you have to

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<v Speaker 1>eliminate all the ones that don't planets. As far as

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<v Speaker 1>we know, no life can exist upon a star itself.

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<v Speaker 1>Then you have in subset E, which is the number

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<v Speaker 1>of planets hospitable to life, so earthlike planets, anything that

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<v Speaker 1>could actually sustain life. So now talking about something terrestrial

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<v Speaker 1>and with water being that waters, how we know life exists?

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<v Speaker 1>I mean, you know it's again we're not accounting for

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<v Speaker 1>things that for other forms of life that may or

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<v Speaker 1>may not Right where we are, we're all we are

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<v Speaker 1>having to extrapolate from a sample size of one being

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<v Speaker 1>that there's only one planet we know of that has

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<v Speaker 1>life on it. But within E. Basically, if you think

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<v Speaker 1>that every star has one earthlike planet or one planet

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<v Speaker 1>capable of having life, that that value would be like one, right,

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<v Speaker 1>and then you have wouldn't be like one, it would

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<v Speaker 1>be one. It would be one. Precisely if F sub

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<v Speaker 1>L is the fraction of these planets on which life

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<v Speaker 1>actually emerges. So this is the difference between the potential

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<v Speaker 1>for life and the actual existence of life. And then

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<v Speaker 1>you have of f sub I, which is the fraction

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<v Speaker 1>of these planets on which intelligent life evolves. So we've

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<v Speaker 1>gone beyond just life now to life that's actually intelligent. Right,

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<v Speaker 1>We're not just talking about sebreddit, We're talking about actual

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<v Speaker 1>intelligent life difference between bacteria and dolphins. Then we have

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<v Speaker 1>F sub C, which is the fraction of the planets

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<v Speaker 1>with intelligent beings that are actually capable of interstellar communications.

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<v Speaker 1>So we might have some intelligent life out there, but

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<v Speaker 1>they're still banging rocks together to make fire and haven't

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<v Speaker 1>gotten to the point where they can make you know,

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<v Speaker 1>interstellar communication because they don't have rocks that are big enough.

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<v Speaker 1>Then you finally have L, which is the length of

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<v Speaker 1>time that such a civilization is actually detectable. And this

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<v Speaker 1>is I think one of the cleverer parts of the

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<v Speaker 1>equation that it includes this L. It doesn't assume that

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<v Speaker 1>these ones they exist, will exist forever. They may only

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<v Speaker 1>be transmitting for some range of time. Well, let's let's

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<v Speaker 1>say that this civilization is analogous to Earth and just

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<v Speaker 1>just happens to be that way. There's just some random

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<v Speaker 1>chance where there is an alien civilization. They're intelligent, they

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<v Speaker 1>are capable of communicating through interstellar space. Uh, and they

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<v Speaker 1>are at the same level of sophistication that we are

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<v Speaker 1>at and arrived there at approximately the same time, but

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<v Speaker 1>they're a hundred light years away. Well, we haven't been

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<v Speaker 1>using interstellar means of communication in a way where we

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<v Speaker 1>could necessarily detect that, because it would take a hundred

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<v Speaker 1>years for that those transmissions to travel over here. Now,

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<v Speaker 1>if they had powerful enough radios early on, then theoretically

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<v Speaker 1>we could hear it, but chances are we wouldn't be

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<v Speaker 1>able to pick up on that, even though they would

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<v Speaker 1>be out there right now. Right. I've also seen that

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<v Speaker 1>number expressed as F subset capital L, meaning basically the

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<v Speaker 1>number of civilizations that have not blowed themselves up yet. Yeah,

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<v Speaker 1>so they would not only be sophisticated enough, but they

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<v Speaker 1>still they haven't killed themselves either. Yeah, And you know, right,

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<v Speaker 1>the the idea being that certainly, on our planet, as

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<v Speaker 1>far as we know, dinosaurs were not broadcasting radio signals

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<v Speaker 1>into the sixty five million years ago, but they just

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<v Speaker 1>put someone but someone could have someone could have been

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<v Speaker 1>tuned into our planet at that point, and you know, yeah,

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<v Speaker 1>or really the way that that's expressed, I think was

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<v Speaker 1>a lot of how seventies nine seventies era scientists were

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<v Speaker 1>viewing mankind's um state of affairs at that moment, informed

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<v Speaker 1>a little bit by the Cold War, probably, yeah, saying

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<v Speaker 1>like like, well, you know, humans have this terrible history

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<v Speaker 1>of making war upon each other, and there is the potential,

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<v Speaker 1>particularly with things like nuclear weapons, that we could have

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<v Speaker 1>a catastrophic event. So that you're saying, well, if we

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<v Speaker 1>extrapolate that, then there might be a lot of alien

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<v Speaker 1>aries is out there that have the same problem. Yeah,

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<v Speaker 1>and it's not totally unreasonable to notice that about the

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<v Speaker 1>same time a civilization gets the power to make radio broadcasts,

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<v Speaker 1>they're also starting to get really advanced weaponry. Yeah. So, uh,

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<v Speaker 1>what's interesting is when you start trying to fill these

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<v Speaker 1>variables out. Yeah, so lots of people have tried to

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<v Speaker 1>compute this equation with their own guesses filled in, and

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<v Speaker 1>one thing you start to notice if you read these

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<v Speaker 1>different estimates is they're all over the place. Well, it's

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<v Speaker 1>because we have such a lack of information about some

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<v Speaker 1>of these things, particularly when it comes to the actual

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<v Speaker 1>questions about life. We have not detected life anywhere else.

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<v Speaker 1>We have lots of guesses, but their guesses they're not

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<v Speaker 1>based upon any observable, testable data that we've come that's

0:12:29.040 --> 0:12:31.559
<v Speaker 1>come back to us where we can definitively say, here's

0:12:31.559 --> 0:12:35.240
<v Speaker 1>another example, our our sample size has doubled or whatever.

0:12:35.640 --> 0:12:39.480
<v Speaker 1>So early on in early versions of the Drake equation,

0:12:39.480 --> 0:12:42.120
<v Speaker 1>where people were filling out all these variables. One of

0:12:42.200 --> 0:12:47.520
<v Speaker 1>the earliest is one that was documented in the series Cosmos. Yes,

0:12:48.400 --> 0:12:50.319
<v Speaker 1>highly recommended, by the way, if you have not ever

0:12:50.360 --> 0:12:52.679
<v Speaker 1>watched Cosmos, I mean, you know, you've got to get

0:12:52.679 --> 0:12:57.280
<v Speaker 1>over some dated effects and fashions they are. They're doing

0:12:57.280 --> 0:13:01.160
<v Speaker 1>a remake, but it's my person all favorite thing, getting

0:13:01.160 --> 0:13:02.960
<v Speaker 1>to see all of the super high tech computers in

0:13:02.960 --> 0:13:06.040
<v Speaker 1>the background are way bigger than this podcast, but it's

0:13:06.160 --> 0:13:09.439
<v Speaker 1>it's everything is covered in shag carpets, but it's still

0:13:09.720 --> 0:13:12.400
<v Speaker 1>the science in it is phenomenal. And and of course

0:13:12.400 --> 0:13:15.720
<v Speaker 1>Sagan's enthusiasm for science is one of those things that

0:13:15.760 --> 0:13:19.440
<v Speaker 1>you cannot, you know, easily replicate. You have to actually

0:13:19.600 --> 0:13:22.760
<v Speaker 1>possess that yourself. It's hard. You can't really be insincere

0:13:22.800 --> 0:13:25.280
<v Speaker 1>and try and be like science is great. You can

0:13:25.320 --> 0:13:30.920
<v Speaker 1>just see his sort of like calm tope joy. Right,

0:13:30.960 --> 0:13:33.280
<v Speaker 1>So let's let's talk about his Tope approach to the

0:13:33.360 --> 0:13:37.280
<v Speaker 1>Drake equation. So he said that in his version, he says,

0:13:37.280 --> 0:13:40.600
<v Speaker 1>all right, so in the Milky Way, imagine there are

0:13:40.760 --> 0:13:44.040
<v Speaker 1>four hundred billion stars there, and then about a quarter

0:13:44.080 --> 0:13:46.400
<v Speaker 1>of those have planets exactly. So then you you have

0:13:46.520 --> 0:13:49.079
<v Speaker 1>just gotten down to one billion stars that have the

0:13:49.120 --> 0:13:52.839
<v Speaker 1>potential to have plants that would perhaps support life. So that,

0:13:52.880 --> 0:13:55.520
<v Speaker 1>of course, if you extrapolated this to other galaxies, which

0:13:55.559 --> 0:13:58.360
<v Speaker 1>the Drake equation does not do, it's specifically for the

0:13:58.400 --> 0:14:00.520
<v Speaker 1>Milky Way, but he said, if you were, you'd end

0:14:00.600 --> 0:14:04.680
<v Speaker 1>up with trillions of stars to work with. But sticking

0:14:04.679 --> 0:14:07.000
<v Speaker 1>to the Milky Way hundred billion, he then suggests that

0:14:07.000 --> 0:14:10.960
<v Speaker 1>in every star system there will be approximately two planets

0:14:11.000 --> 0:14:13.840
<v Speaker 1>suitable for life on average, meaning that some would have more,

0:14:14.280 --> 0:14:17.400
<v Speaker 1>some might not have any, uh, and then that perhaps

0:14:17.480 --> 0:14:20.000
<v Speaker 1>a one half of those might be planets on which

0:14:20.000 --> 0:14:23.280
<v Speaker 1>life actually arose. Right, So now we're back to specifically

0:14:23.320 --> 0:14:26.240
<v Speaker 1>a hundred billion planets. Once you look at those those

0:14:26.560 --> 0:14:29.480
<v Speaker 1>numbers into the equation. We're not done yet, though, he says,

0:14:29.520 --> 0:14:32.280
<v Speaker 1>then you have to look at the likelihood that the

0:14:32.400 --> 0:14:35.680
<v Speaker 1>life sustaining planets actually give rise to intelligence, and he

0:14:35.800 --> 0:14:38.680
<v Speaker 1>gave it as a conservative estimate of one out of

0:14:38.680 --> 0:14:42.040
<v Speaker 1>ten uh, saying that you know, some scientists say that

0:14:42.040 --> 0:14:47.680
<v Speaker 1>that intelligence is something that is so advantageous evolution evolutionary,

0:14:47.800 --> 0:14:51.360
<v Speaker 1>Lee speaking that it's almost a given that that life

0:14:51.400 --> 0:14:55.520
<v Speaker 1>will get to an intelligent level. But other scientists disagree

0:14:55.520 --> 0:14:57.680
<v Speaker 1>with this assessment. So he says, let's be conservative. We'll

0:14:57.680 --> 0:14:59.760
<v Speaker 1>say one out of ten. And then he said that

0:15:00.240 --> 0:15:03.000
<v Speaker 1>only one out of ten of those might be able

0:15:03.040 --> 0:15:05.560
<v Speaker 1>to come up with some form of interstellar communications, So

0:15:05.600 --> 0:15:08.200
<v Speaker 1>you have to multiply by one tent twice. And he

0:15:08.480 --> 0:15:10.920
<v Speaker 1>called that middle of the road, meaning that you know,

0:15:11.080 --> 0:15:14.320
<v Speaker 1>again there are different opinions on how likely this is.

0:15:14.520 --> 0:15:18.200
<v Speaker 1>He considered that relatively conservative. And then he said, now

0:15:18.240 --> 0:15:20.000
<v Speaker 1>you have to look at that length of time when

0:15:20.040 --> 0:15:23.200
<v Speaker 1>such a civilization is active that would allow us to

0:15:23.280 --> 0:15:25.760
<v Speaker 1>detect them, so that they would be active at a

0:15:25.760 --> 0:15:28.400
<v Speaker 1>time when we would be able to right now find

0:15:28.400 --> 0:15:30.720
<v Speaker 1>out about them. He says that would be the really

0:15:30.760 --> 0:15:33.600
<v Speaker 1>limiting factor. He said that you know, Earth is an

0:15:33.600 --> 0:15:36.600
<v Speaker 1>example of this. But despite tens of thousands of years

0:15:36.680 --> 0:15:39.680
<v Speaker 1>humans have that humans have been on this planet, we

0:15:39.760 --> 0:15:44.360
<v Speaker 1>have only really relatively recently harnessed radio, so just a

0:15:44.400 --> 0:15:48.520
<v Speaker 1>few decades really, So in the grand uh amount of

0:15:48.520 --> 0:15:51.680
<v Speaker 1>time that humans have been alive, we've only had a

0:15:51.760 --> 0:15:54.360
<v Speaker 1>tiny little sliver of a window when we've actually been

0:15:54.360 --> 0:15:57.480
<v Speaker 1>active with this radio technology. And in the same may

0:15:57.520 --> 0:16:00.960
<v Speaker 1>be true for other civilizations. So he said that you know,

0:16:01.240 --> 0:16:05.040
<v Speaker 1>you might have as little as one in one hundred millions,

0:16:05.120 --> 0:16:08.000
<v Speaker 1>so one millions of a chance for that. So that

0:16:08.080 --> 0:16:10.680
<v Speaker 1>was the last variable he filled in. Once you fill

0:16:10.680 --> 0:16:13.160
<v Speaker 1>in all those numbers and multiple I'm altogether, you are

0:16:13.240 --> 0:16:17.680
<v Speaker 1>left with the number of ten ten civilizations across the

0:16:17.720 --> 0:16:21.840
<v Speaker 1>Milky Way galaxy that we could potentially detect, assuming they

0:16:21.840 --> 0:16:25.680
<v Speaker 1>were close enough for us to be able to communicate

0:16:25.720 --> 0:16:29.119
<v Speaker 1>with them on some meaningful way, which sounds really pessimistic,

0:16:29.200 --> 0:16:32.400
<v Speaker 1>especially for Carl Sagan, for for someone who's generally optimistic,

0:16:32.440 --> 0:16:34.280
<v Speaker 1>as he was, But he went on to say that

0:16:34.480 --> 0:16:36.360
<v Speaker 1>you know, if if you if you play with that

0:16:36.480 --> 0:16:38.280
<v Speaker 1>last number just a little bit, you could wind up

0:16:38.280 --> 0:16:42.720
<v Speaker 1>with millions if possible civilizations. And some people have estimated millions,

0:16:42.760 --> 0:16:44.920
<v Speaker 1>Oh absolutely, I think most of the estimates that I've

0:16:44.960 --> 0:16:48.080
<v Speaker 1>seen are more around the ten thousand range. Issues I

0:16:48.120 --> 0:16:52.080
<v Speaker 1>did see one that gave it to point zero zero

0:16:52.240 --> 0:16:57.480
<v Speaker 1>zero zero zero zero eight civilizations. So that's not even

0:16:57.520 --> 0:17:00.640
<v Speaker 1>accounting for others. Yeah, that seems to account the fact

0:17:00.680 --> 0:17:03.560
<v Speaker 1>that Earth is there. But but yeah, I I don't

0:17:03.560 --> 0:17:07.360
<v Speaker 1>have all the numbers there to tell you exactly how

0:17:07.400 --> 0:17:09.800
<v Speaker 1>that number was arrived at. But that was I think

0:17:09.840 --> 0:17:11.879
<v Speaker 1>I think someone took a right turn in Albuquerque and

0:17:12.040 --> 0:17:15.920
<v Speaker 1>in that in that equation. Well, as we've discussed um,

0:17:16.160 --> 0:17:19.439
<v Speaker 1>part of the problem with this equation is is that

0:17:19.520 --> 0:17:22.560
<v Speaker 1>as you move from the left to the right along

0:17:23.040 --> 0:17:25.840
<v Speaker 1>the different variables that you have to plug in, your

0:17:26.119 --> 0:17:30.840
<v Speaker 1>level of certainty decreases. So we we know pretty well,

0:17:31.000 --> 0:17:34.320
<v Speaker 1>uh say, like the rate of star formation of the galaxy.

0:17:34.400 --> 0:17:37.440
<v Speaker 1>We're learning a lot more right now about the number

0:17:37.480 --> 0:17:39.919
<v Speaker 1>of those stars that have planets and the number of

0:17:39.960 --> 0:17:43.200
<v Speaker 1>those planets detecting some and then we're extrapolating a lot

0:17:43.240 --> 0:17:45.960
<v Speaker 1>from what we're detecting. But it seems to be bearing out. Yeah,

0:17:46.240 --> 0:17:48.200
<v Speaker 1>so we're learning a lot more. But once you get

0:17:48.200 --> 0:17:51.439
<v Speaker 1>into stuff about the fraction of these planets on which

0:17:51.560 --> 0:17:55.760
<v Speaker 1>life emerges, well, how do we know? So you have

0:17:55.920 --> 0:17:58.600
<v Speaker 1>you have to just guess. In these cases, you have

0:17:58.680 --> 0:18:01.760
<v Speaker 1>to use your intuitions and all that, But we get

0:18:01.760 --> 0:18:03.800
<v Speaker 1>back to those ice cream feelings that we were talking

0:18:03.840 --> 0:18:07.600
<v Speaker 1>about earlier. Yeah. Um, one of the things that might

0:18:07.840 --> 0:18:12.240
<v Speaker 1>encourage us to be more conservative or some might use

0:18:12.280 --> 0:18:16.200
<v Speaker 1>the word pessimistic in estimating those later numbers is something

0:18:16.240 --> 0:18:20.720
<v Speaker 1>called the Fermi paradox. Yes, Fermis paradox. Yeah, this is uh,

0:18:20.800 --> 0:18:23.320
<v Speaker 1>this is pretty simple, right, It's that if if this

0:18:23.400 --> 0:18:26.840
<v Speaker 1>equation in fact suggests that there are potentially thousands of

0:18:26.880 --> 0:18:30.119
<v Speaker 1>civilizations of intelligent creatures out there, you can sum it

0:18:30.200 --> 0:18:33.520
<v Speaker 1>up in three words, where are they? Where is everybody?

0:18:34.200 --> 0:18:37.400
<v Speaker 1>If they're supposed to be out there? But we haven't

0:18:37.480 --> 0:18:39.200
<v Speaker 1>heard him, and he was talking about this before the

0:18:39.280 --> 0:18:42.280
<v Speaker 1>Drake equation actually existed back in nineteen fifty. But right,

0:18:42.359 --> 0:18:46.159
<v Speaker 1>it asks if extraterrestrials are so common, why haven't they visited,

0:18:46.160 --> 0:18:49.440
<v Speaker 1>why haven't they communicated with us? Or why haven't they

0:18:49.520 --> 0:18:52.440
<v Speaker 1>left behind some residue of their existence? And we would

0:18:52.440 --> 0:18:54.960
<v Speaker 1>be able to pick up He actually went on to suggest, like,

0:18:55.040 --> 0:18:57.720
<v Speaker 1>imagine this, and it's not difficult to imagine if you

0:18:57.800 --> 0:19:01.080
<v Speaker 1>just look back at human history. So human history, we

0:19:01.160 --> 0:19:05.160
<v Speaker 1>have this history of exploration and colonization, whether you want

0:19:05.160 --> 0:19:08.200
<v Speaker 1>to talk about the ancient peoples and spreading out across

0:19:08.200 --> 0:19:14.440
<v Speaker 1>the Earth, or the more relatively recent European expansions and colonization.

0:19:14.840 --> 0:19:16.880
<v Speaker 1>We've got this history where we want to go and

0:19:16.960 --> 0:19:19.720
<v Speaker 1>explore the world that we that is unfamiliar to us.

0:19:19.720 --> 0:19:23.160
<v Speaker 1>And then uh claimant, so he says, well, it's it's

0:19:23.200 --> 0:19:26.159
<v Speaker 1>not always so nice. Let's assume that there's at least

0:19:26.240 --> 0:19:31.080
<v Speaker 1>one intelligent alien civilization that has the same sort of

0:19:31.080 --> 0:19:35.680
<v Speaker 1>of of propensity for colonization, someone out there who does

0:19:35.760 --> 0:19:37.439
<v Speaker 1>essentially the same sort of thing, but they can do

0:19:37.480 --> 0:19:40.919
<v Speaker 1>it on an interstellar level, and it may take thousands

0:19:40.920 --> 0:19:44.119
<v Speaker 1>of years for their civilization to spread, but as they spread,

0:19:44.160 --> 0:19:48.160
<v Speaker 1>they spread into more vectors, so they'll colonize one world

0:19:48.440 --> 0:19:51.359
<v Speaker 1>and then over time will branch out and start colonizing

0:19:51.359 --> 0:19:53.480
<v Speaker 1>other worlds. And every world they colonize means that that's

0:19:53.520 --> 0:19:56.959
<v Speaker 1>another base of operations from which they launch. And if

0:19:57.040 --> 0:20:00.479
<v Speaker 1>you expand this out over the course of millions of years,

0:20:00.920 --> 0:20:04.040
<v Speaker 1>then surely they would have reached a point of saturation

0:20:04.080 --> 0:20:06.480
<v Speaker 1>where we would be able to detect them. And that

0:20:06.600 --> 0:20:09.160
<v Speaker 1>sounds kind of crazy, but then you remember the universe

0:20:09.320 --> 0:20:12.600
<v Speaker 1>is billions of years old, so a few tens of

0:20:12.680 --> 0:20:16.359
<v Speaker 1>millions of years is nothing in the grand cosmological scheme

0:20:16.400 --> 0:20:18.520
<v Speaker 1>of things. So if you were to think of it

0:20:18.560 --> 0:20:23.600
<v Speaker 1>that way, then where are they? Yeah, So there are

0:20:23.640 --> 0:20:28.480
<v Speaker 1>a lot of hypotheses to explain this question of, uh,

0:20:28.520 --> 0:20:31.320
<v Speaker 1>you know, why aren't we detecting them? The most obvious

0:20:31.400 --> 0:20:34.399
<v Speaker 1>one I think you should start with is they just

0:20:34.960 --> 0:20:39.480
<v Speaker 1>detecting them because they're not out there. Nobody's home psychic bacteria.

0:20:39.840 --> 0:20:43.280
<v Speaker 1>And so how would you explain this? Well, you could

0:20:43.359 --> 0:20:46.320
<v Speaker 1>look at this equation and say, okay, so we know

0:20:46.440 --> 0:20:52.040
<v Speaker 1>the problem is not in say like h R or FP,

0:20:52.840 --> 0:20:55.359
<v Speaker 1>as in the stars that are forming or the number

0:20:55.400 --> 0:20:57.360
<v Speaker 1>of planets that are out there. Right, We've got some

0:20:57.440 --> 0:21:00.119
<v Speaker 1>data coming in on that, and we know pretty well

0:21:00.119 --> 0:21:02.560
<v Speaker 1>that well, there's going to be enough of that. But

0:21:02.640 --> 0:21:06.080
<v Speaker 1>once you get into those later variables, you say, it

0:21:06.160 --> 0:21:11.000
<v Speaker 1>could be that one or more of those variables is zero. Right,

0:21:11.040 --> 0:21:13.399
<v Speaker 1>It could be it could be that the number of

0:21:13.400 --> 0:21:16.880
<v Speaker 1>plants that actually support life is very very very low,

0:21:17.080 --> 0:21:19.720
<v Speaker 1>and then that on top of that, the plants that

0:21:19.920 --> 0:21:23.119
<v Speaker 1>actually support life zero. Yeah. The so that would be

0:21:23.160 --> 0:21:28.080
<v Speaker 1>known as the rare Earth hypothesis. It's the idea that

0:21:28.720 --> 0:21:31.840
<v Speaker 1>Earth is actually even more special than we thought that.

0:21:31.960 --> 0:21:37.040
<v Speaker 1>It's just this really really super lucky situation with just

0:21:37.160 --> 0:21:39.840
<v Speaker 1>the right chemicals. If all plants are special, then no

0:21:39.960 --> 0:21:45.359
<v Speaker 1>planets are I get you. Okay, well, okay, no, we

0:21:45.440 --> 0:21:48.080
<v Speaker 1>know Earth is at least somewhat special. It's at least

0:21:48.160 --> 0:21:50.680
<v Speaker 1>very special in our solar systeah, sure than one out

0:21:50.680 --> 0:21:54.919
<v Speaker 1>of eight planets. I'm still calling Pluto a planet. I'm

0:21:54.960 --> 0:21:57.840
<v Speaker 1>going one nine, Okay, but I mean we just know that, like,

0:21:57.960 --> 0:22:01.280
<v Speaker 1>mercury ain't that special. It's just not very good. No,

0:22:01.520 --> 0:22:04.479
<v Speaker 1>it's no offense to mercury, but it's kind of crappy

0:22:05.760 --> 0:22:07.960
<v Speaker 1>down on mercury. So and and to be fair, a

0:22:07.960 --> 0:22:09.960
<v Speaker 1>lot of the terrestrial planets that we have found out

0:22:09.960 --> 0:22:13.679
<v Speaker 1>there so far have been um too too hot and

0:22:13.760 --> 0:22:20.720
<v Speaker 1>too um black, lacking in atmosphere. I think things they

0:22:20.800 --> 0:22:23.720
<v Speaker 1>do not appear to be capable of sustaining life as

0:22:23.760 --> 0:22:26.760
<v Speaker 1>we are familiar with it. Okay, So that's that's like

0:22:26.800 --> 0:22:30.840
<v Speaker 1>the rare Earth hypothesis. But maybe there are other things

0:22:30.840 --> 0:22:34.760
<v Speaker 1>that could explain it. So maybe earthlike planets are pretty common,

0:22:34.960 --> 0:22:38.760
<v Speaker 1>but for some reason, A biogenesis is just super rare.

0:22:38.880 --> 0:22:43.640
<v Speaker 1>A biogenesis is the word that means life arising, So

0:22:43.800 --> 0:22:47.480
<v Speaker 1>we know what's happened once it's here on Earth. Um,

0:22:47.560 --> 0:22:51.160
<v Speaker 1>but we don't know how it happened, and we don't

0:22:51.200 --> 0:22:53.200
<v Speaker 1>know how special it is. We don't know how rare

0:22:53.280 --> 0:22:56.439
<v Speaker 1>that is. Right. It could be something that's fairly common

0:22:56.560 --> 0:23:00.360
<v Speaker 1>given the kind of conditions our planet underwent, what four

0:23:00.400 --> 0:23:02.840
<v Speaker 1>point five billion years ago or so, Or it could

0:23:02.880 --> 0:23:06.479
<v Speaker 1>be something that's super super special and almost never happened.

0:23:07.200 --> 0:23:10.240
<v Speaker 1>Or it could be that life happens all over the place,

0:23:10.280 --> 0:23:15.080
<v Speaker 1>but intelligent life hardly ever evolves from it. So our

0:23:15.119 --> 0:23:18.800
<v Speaker 1>galaxy could be full of planets that have bacteria but

0:23:19.160 --> 0:23:22.440
<v Speaker 1>nothing with a brain. Right. Uh. And then beyond that,

0:23:22.560 --> 0:23:25.960
<v Speaker 1>you could say, well, maybe intelligent life does exist out there,

0:23:25.960 --> 0:23:28.480
<v Speaker 1>and that's fine and everything. Everything in that part of

0:23:28.480 --> 0:23:30.640
<v Speaker 1>the equation up to that point is supportive. But then

0:23:30.880 --> 0:23:33.440
<v Speaker 1>they like the radio. Well, it could be that humans.

0:23:33.560 --> 0:23:36.119
<v Speaker 1>I mean, it's it's really weird to think about this,

0:23:36.160 --> 0:23:40.640
<v Speaker 1>and it makes us kind of, uh, a little more grandiose,

0:23:40.680 --> 0:23:43.440
<v Speaker 1>I would say, But it could be that humans are

0:23:43.480 --> 0:23:46.800
<v Speaker 1>the first intelligent race to hit that threshold. I think

0:23:46.800 --> 0:23:51.800
<v Speaker 1>that highly unlikely, considering the relative youth of Earth and humans.

0:23:52.240 --> 0:23:55.720
<v Speaker 1>But let's say that that's a possibility. Our sense of

0:23:55.760 --> 0:23:59.800
<v Speaker 1>avoiding hubris kind of makes us not want to choose

0:23:59.800 --> 0:24:03.840
<v Speaker 1>that position but can't. Or or perhaps that those those

0:24:03.840 --> 0:24:06.439
<v Speaker 1>civilizations that also have it are too far away for us,

0:24:06.480 --> 0:24:08.800
<v Speaker 1>like you were saying earlier, Joe, Yeah, it could be

0:24:08.840 --> 0:24:11.160
<v Speaker 1>that they're just too young for us to have detected.

0:24:11.160 --> 0:24:13.200
<v Speaker 1>All right, I mean it's important to think. Maybe the

0:24:13.680 --> 0:24:17.440
<v Speaker 1>number out there is not zero, but if it's sufficiently small. Uh,

0:24:17.520 --> 0:24:20.800
<v Speaker 1>the Milky Way galaxy is a hundred thousand light years wide.

0:24:21.119 --> 0:24:24.000
<v Speaker 1>I mean, what if they're watching skies for a hundred

0:24:24.000 --> 0:24:27.120
<v Speaker 1>thousand years? Right, So what if there are ten other

0:24:27.280 --> 0:24:30.240
<v Speaker 1>civilizations is pretty low number. They are there, but they're

0:24:30.240 --> 0:24:32.439
<v Speaker 1>on the other side of the galaxy. I mean that

0:24:32.480 --> 0:24:34.840
<v Speaker 1>would mean they would have had to have been transmitting

0:24:34.880 --> 0:24:38.040
<v Speaker 1>for a hundred thousand years. They might be chatting with

0:24:38.080 --> 0:24:39.880
<v Speaker 1>each other quite a bit and just leaving us out

0:24:39.880 --> 0:24:42.160
<v Speaker 1>of it. And we're just the unpopular kid in high

0:24:42.160 --> 0:24:44.119
<v Speaker 1>school has to stand in the corner all the popular

0:24:44.200 --> 0:24:46.800
<v Speaker 1>kids dance over there. Not that I'm bitter or anything.

0:24:48.160 --> 0:24:52.560
<v Speaker 1>Some memories don't die anyway. Sorry. Well, and then the

0:24:52.600 --> 0:24:56.840
<v Speaker 1>final variable is l Well, that flits into that fits

0:24:56.840 --> 0:24:58.600
<v Speaker 1>into it at length of time. So let's say that,

0:24:58.920 --> 0:25:00.720
<v Speaker 1>let's say that the length of time, like you were saying,

0:25:00.720 --> 0:25:03.680
<v Speaker 1>the length of time just hasn't been sufficient enough for

0:25:03.760 --> 0:25:05.600
<v Speaker 1>us to be able to detect them because they're too

0:25:05.640 --> 0:25:07.439
<v Speaker 1>far away, and the speed of light, as far as

0:25:07.520 --> 0:25:10.280
<v Speaker 1>we know, is the limiting factor. Now, some of the

0:25:10.440 --> 0:25:13.040
<v Speaker 1>people who have estimated that the length of time a

0:25:13.119 --> 0:25:17.720
<v Speaker 1>civilization transmits um is low. They've estimated this because they

0:25:17.720 --> 0:25:23.000
<v Speaker 1>have feelings about civilizations destroying themselves, really negative feelings. It

0:25:23.080 --> 0:25:25.360
<v Speaker 1>could be that, but it could also be that they

0:25:25.400 --> 0:25:28.840
<v Speaker 1>don't want to transmit all that long, or they don't

0:25:28.880 --> 0:25:33.080
<v Speaker 1>have the resources to do it, or perhaps even natural disasters.

0:25:33.119 --> 0:25:35.280
<v Speaker 1>I mean, I could easily envision a planet that was

0:25:35.320 --> 0:25:38.920
<v Speaker 1>even more bombarded by meteoroids than Earth is. Well, there

0:25:38.960 --> 0:25:41.800
<v Speaker 1>was that one planet that was being pulled into its son,

0:25:41.840 --> 0:25:45.120
<v Speaker 1>and so that one family sent their only son off

0:25:45.160 --> 0:25:47.600
<v Speaker 1>to Earth in order to act as guardian. I'm talking

0:25:47.600 --> 0:25:51.160
<v Speaker 1>about supermanager. That is a really bizarre way of communicating. Yeah,

0:25:51.400 --> 0:25:54.399
<v Speaker 1>pretty you think it would say? You think it's in

0:25:54.440 --> 0:25:57.679
<v Speaker 1>a note first, and rather than just just eject them

0:25:57.680 --> 0:26:00.560
<v Speaker 1>to Earth, consider this radio message the light to show

0:26:00.560 --> 0:26:02.720
<v Speaker 1>you the way. See. Yeah, maybe maybe people are way

0:26:02.720 --> 0:26:06.040
<v Speaker 1>into sending babies as communicators and not radio signals. Oh,

0:26:06.080 --> 0:26:08.560
<v Speaker 1>that's right, because they travel at a slower than light speed,

0:26:08.600 --> 0:26:11.600
<v Speaker 1>so we're still waiting on the babies. But it also

0:26:11.920 --> 0:26:13.520
<v Speaker 1>to get back to what you were saying, there could

0:26:13.560 --> 0:26:16.760
<v Speaker 1>be that sort of Star trek Uh concept of the

0:26:16.760 --> 0:26:21.280
<v Speaker 1>prime directive, where so we assume that they want to

0:26:21.320 --> 0:26:24.960
<v Speaker 1>contact us, they might not want to for for positive

0:26:25.080 --> 0:26:27.920
<v Speaker 1>or negative reasons. We assume first of all that they're

0:26:27.920 --> 0:26:30.760
<v Speaker 1>not paranoid. What if they are paranoid, I mean, it

0:26:30.760 --> 0:26:34.160
<v Speaker 1>would be entirely reasonable for them to just kind of

0:26:34.200 --> 0:26:36.679
<v Speaker 1>hold up and say we don't want to go messing

0:26:36.720 --> 0:26:39.520
<v Speaker 1>around where we you know, don't know if we're gonna win,

0:26:39.880 --> 0:26:42.760
<v Speaker 1>say in a conflict or something like that. Or it

0:26:42.760 --> 0:26:45.640
<v Speaker 1>could be benevolent like the vulcans well, and it could

0:26:45.760 --> 0:26:49.119
<v Speaker 1>very possibly be that again, that they have shifted to

0:26:49.359 --> 0:26:52.760
<v Speaker 1>a different type of interstellar communication that we don't use

0:26:52.880 --> 0:26:57.000
<v Speaker 1>and cannot detect. So radio waves is pretty is a

0:26:57.000 --> 0:27:00.040
<v Speaker 1>pretty safe bet simply because it was it appears to

0:27:00.160 --> 0:27:03.720
<v Speaker 1>have been kind of a building block along the way

0:27:03.760 --> 0:27:08.359
<v Speaker 1>of learning how to communicate in an interstellar environment. But

0:27:08.480 --> 0:27:10.920
<v Speaker 1>like we were saying, with lasers, that's a much more

0:27:10.960 --> 0:27:14.359
<v Speaker 1>precise way of communicating. You have to have it lined

0:27:14.440 --> 0:27:16.439
<v Speaker 1>up between laser and censor in order for you to

0:27:16.440 --> 0:27:18.800
<v Speaker 1>be able to communicate. You know, you can't just fire

0:27:18.800 --> 0:27:22.040
<v Speaker 1>a laser off into the sky and it it's meaningful

0:27:22.080 --> 0:27:26.280
<v Speaker 1>in any way. So what if these uh, these intelligent

0:27:26.359 --> 0:27:30.160
<v Speaker 1>civilizations have gone beyond where radio waves are and they're

0:27:30.280 --> 0:27:34.560
<v Speaker 1>using something like lasers to communicate because it as allows

0:27:34.560 --> 0:27:38.480
<v Speaker 1>them to have far more bandwidth than they would with radio. Well,

0:27:38.480 --> 0:27:41.080
<v Speaker 1>we wouldn't necessarily pick up on that because they're communicating

0:27:41.080 --> 0:27:45.240
<v Speaker 1>a very specific points among themselves, not necessarily shooting off

0:27:45.440 --> 0:27:48.120
<v Speaker 1>rays at random directions hoping to hit something that could

0:27:48.359 --> 0:27:51.399
<v Speaker 1>figure out what's going on. Yeah, it's entirely possible. And

0:27:51.960 --> 0:27:56.399
<v Speaker 1>we also aren't even imagining all of the weird little

0:27:56.440 --> 0:28:00.320
<v Speaker 1>technological trip ups that might be involved in this, uh

0:28:00.680 --> 0:28:05.200
<v Speaker 1>in this filter. You know that that's creating this paradox. Uh.

0:28:05.320 --> 0:28:08.280
<v Speaker 1>What if it's just that they are sending signals but

0:28:08.560 --> 0:28:13.640
<v Speaker 1>we're not listening close enough to the right place. Sure, right,

0:28:13.800 --> 0:28:16.240
<v Speaker 1>things that that people like Karl Saken and Drake were

0:28:16.280 --> 0:28:18.719
<v Speaker 1>talking about, where that we are really only listening to

0:28:18.840 --> 0:28:21.119
<v Speaker 1>any given section of the sky for a very short

0:28:21.200 --> 0:28:23.439
<v Speaker 1>period of time, and so you know, and if we

0:28:23.520 --> 0:28:25.320
<v Speaker 1>you know, what if they're broadcasting and then they turn

0:28:25.359 --> 0:28:27.640
<v Speaker 1>it off and we tune in a second after that,

0:28:27.760 --> 0:28:30.040
<v Speaker 1>and you know, it's when when you're working with these

0:28:30.200 --> 0:28:34.520
<v Speaker 1>telescopes that, yes, are are tremendously powerful compared to what

0:28:34.560 --> 0:28:37.840
<v Speaker 1>they were forty years ago. But but right you know,

0:28:37.920 --> 0:28:41.600
<v Speaker 1>only a very small segment of the entire sky, yeah,

0:28:41.760 --> 0:28:43.800
<v Speaker 1>much less the universe. Yeah. And and not only that,

0:28:43.840 --> 0:28:47.360
<v Speaker 1>but think about if you've ever studied things like, you know,

0:28:47.400 --> 0:28:52.200
<v Speaker 1>the Voyager spacecraft and how NASA has continued to retrieve

0:28:52.320 --> 0:28:55.400
<v Speaker 1>data or receive really I should say received data from

0:28:55.400 --> 0:28:58.240
<v Speaker 1>the Voyager spacecraft. Uh, they had they had to keep

0:28:58.280 --> 0:29:02.160
<v Speaker 1>building bigger and bigger radar antenna arrays in order to

0:29:02.200 --> 0:29:06.320
<v Speaker 1>detect that increasingly faint signal. So again, if the signals

0:29:06.320 --> 0:29:08.720
<v Speaker 1>that are being sent out by these civilizations are faint,

0:29:09.040 --> 0:29:13.680
<v Speaker 1>it may fade and so well with just background noise

0:29:13.800 --> 0:29:16.360
<v Speaker 1>that we can't quite filter it out yet. Or what

0:29:16.400 --> 0:29:18.720
<v Speaker 1>if they're broadcasting it is slightly different bandwidth then we're

0:29:18.720 --> 0:29:21.720
<v Speaker 1>listening to. Yeah, I think we usually listen to a

0:29:21.760 --> 0:29:26.840
<v Speaker 1>microwave frequency that we we judged would be a good

0:29:26.840 --> 0:29:30.560
<v Speaker 1>one for them to transmit it on but um, you know,

0:29:30.640 --> 0:29:32.959
<v Speaker 1>maybe they don't like that one. Yeah. Yeah, that's according

0:29:33.000 --> 0:29:37.200
<v Speaker 1>to human people. And you know, are our sensory apparatus

0:29:37.240 --> 0:29:40.640
<v Speaker 1>for listening to the universes is limited? Yeah, and again,

0:29:40.840 --> 0:29:43.280
<v Speaker 1>like I said, we're having to extrapolate a lot just

0:29:43.280 --> 0:29:45.560
<v Speaker 1>based upon our own experience because we can't we don't

0:29:45.600 --> 0:29:48.560
<v Speaker 1>have anything else to compare it to. So if if

0:29:48.600 --> 0:29:52.600
<v Speaker 1>some other civilization is significantly different enough from ours, that

0:29:52.720 --> 0:29:58.840
<v Speaker 1>alone makes this incredibly complicated. Yeah. So since we talk

0:29:58.920 --> 0:30:02.560
<v Speaker 1>about the future here, we thinking one thing I want

0:30:02.560 --> 0:30:06.040
<v Speaker 1>to focus on is sort of how future discoveries, those

0:30:06.080 --> 0:30:07.880
<v Speaker 1>that are going on right now and in the near

0:30:07.920 --> 0:30:10.680
<v Speaker 1>future and maybe even in the far future, could affect

0:30:10.760 --> 0:30:14.640
<v Speaker 1>the way we calculate the Drake equation? Are there ways

0:30:14.760 --> 0:30:17.600
<v Speaker 1>that variables in the equation that are fuzzy to us

0:30:17.680 --> 0:30:20.680
<v Speaker 1>right now could become much more clear The more we

0:30:20.720 --> 0:30:24.920
<v Speaker 1>know about Earth, sure, I mean some of the more

0:30:24.960 --> 0:30:26.720
<v Speaker 1>we know about Earth and the more we know about

0:30:26.800 --> 0:30:31.440
<v Speaker 1>just our immediate surroundings. Yeah, As our methods of detecting

0:30:31.680 --> 0:30:35.640
<v Speaker 1>other planets, other terrestrial planets, get better, um, we'll be

0:30:35.680 --> 0:30:38.760
<v Speaker 1>able to see how many might be able to hold

0:30:39.480 --> 0:30:43.680
<v Speaker 1>microbial life and then be able to perhaps maybe someday.

0:30:43.760 --> 0:30:45.320
<v Speaker 1>I mean, you know, how do we how do we

0:30:45.360 --> 0:30:49.120
<v Speaker 1>test for life that isn't building pyramids or something like that,

0:30:49.120 --> 0:30:52.520
<v Speaker 1>that's that's hundreds of light years away? Yeah, well, if

0:30:52.680 --> 0:30:56.000
<v Speaker 1>if we just start with those planets, like say, um,

0:30:56.120 --> 0:30:58.840
<v Speaker 1>when Frank Drake came up with this equation, they didn't

0:30:59.000 --> 0:31:02.360
<v Speaker 1>know how how many of the stars out there had planets.

0:31:02.480 --> 0:31:05.680
<v Speaker 1>I mean, they didn't have a Kepler survey. Yet we

0:31:05.720 --> 0:31:08.000
<v Speaker 1>still we still don't really know. We have we have

0:31:08.080 --> 0:31:11.360
<v Speaker 1>some good data that gives us some some educated guesses,

0:31:11.760 --> 0:31:16.200
<v Speaker 1>very strong educated guesses. But for as for direct direct

0:31:16.240 --> 0:31:21.520
<v Speaker 1>evidence of uh, it's a relatively small number, but it's encouraging. Yeah,

0:31:21.520 --> 0:31:25.040
<v Speaker 1>we're well, I think we're getting pretty good evidence that

0:31:25.320 --> 0:31:30.080
<v Speaker 1>lots of stars have planets, but it certainly appears that way. Yes, yeah, um,

0:31:30.120 --> 0:31:32.400
<v Speaker 1>but then you know, how do we again, how do

0:31:32.480 --> 0:31:34.360
<v Speaker 1>how do we detect life on this planets because we

0:31:34.400 --> 0:31:36.880
<v Speaker 1>haven't even detected life elsewhere in our own solar system,

0:31:36.880 --> 0:31:40.480
<v Speaker 1>which is a lot more accessible. Well, we can possibly

0:31:40.480 --> 0:31:44.040
<v Speaker 1>do that through lots of spectral analysis and looking at

0:31:44.760 --> 0:31:47.800
<v Speaker 1>the different atmospheres of plants based upon the color that

0:31:47.840 --> 0:31:50.240
<v Speaker 1>we get back that can give us some indications. But

0:31:50.280 --> 0:31:53.200
<v Speaker 1>also yeah, so if if a planet reflects back in

0:31:53.200 --> 0:31:56.120
<v Speaker 1>a way that shows that it's atmosphere is composed primarily

0:31:56.120 --> 0:31:59.160
<v Speaker 1>of oxygen, we seem to think that's something that happens

0:31:59.200 --> 0:32:01.760
<v Speaker 1>when there's life, right, or perhaps even if we can

0:32:01.800 --> 0:32:04.320
<v Speaker 1>watch something over the next couple of thousand years and

0:32:04.360 --> 0:32:08.320
<v Speaker 1>see how you see how the atmosphere of these planets developed. Uh,

0:32:08.680 --> 0:32:11.320
<v Speaker 1>there was also the chance that we might still find

0:32:11.400 --> 0:32:14.200
<v Speaker 1>some evidence of life within our own solar system. Right, say,

0:32:14.240 --> 0:32:17.320
<v Speaker 1>if we were to go to Jupiter's moon Europa and

0:32:17.400 --> 0:32:19.960
<v Speaker 1>discover microbial life there. I mean that I think that

0:32:20.000 --> 0:32:23.400
<v Speaker 1>would blow one of these variables out of the water.

0:32:23.840 --> 0:32:26.200
<v Speaker 1>The idea that that life had arisen twice in our

0:32:26.240 --> 0:32:30.040
<v Speaker 1>own solar system would be Well, if we knew that

0:32:30.120 --> 0:32:32.600
<v Speaker 1>there was life on another planet in our own solar system,

0:32:32.680 --> 0:32:34.880
<v Speaker 1>we would know that it is just it is just

0:32:35.000 --> 0:32:37.960
<v Speaker 1>not that hard for life to arrive. Right. We would

0:32:38.000 --> 0:32:40.600
<v Speaker 1>have to say, oh, okay, all right, all right, that's

0:32:40.600 --> 0:32:43.760
<v Speaker 1>going to that makes that number larger in our estimation

0:32:43.800 --> 0:32:47.080
<v Speaker 1>than it was before when we plug it into this equation. Right,

0:32:47.080 --> 0:32:48.720
<v Speaker 1>So then we would have to think, well that that

0:32:48.920 --> 0:32:52.440
<v Speaker 1>filtering variable probably needs to be one of the other ones. Then,

0:32:52.520 --> 0:32:55.040
<v Speaker 1>So maybe it's that life is less likely to become

0:32:55.080 --> 0:32:58.600
<v Speaker 1>intelligent or to develop radio technology, right, or to be

0:32:58.720 --> 0:33:01.840
<v Speaker 1>around at the same time we're around. I think that's

0:33:01.880 --> 0:33:05.200
<v Speaker 1>the big one. Um, there are here's another one to

0:33:05.240 --> 0:33:09.600
<v Speaker 1>think about. Um, maybe more we discover about the evolution

0:33:09.640 --> 0:33:14.360
<v Speaker 1>of the brain would help us understand better, Um, how

0:33:14.520 --> 0:33:17.960
<v Speaker 1>likely it is that, say, microbial life, given enough time,

0:33:18.040 --> 0:33:21.360
<v Speaker 1>will evolve into intelligent life. Right. Right, Because as much

0:33:21.360 --> 0:33:23.440
<v Speaker 1>as we don't understand about the far reaches of space,

0:33:23.520 --> 0:33:25.960
<v Speaker 1>we also don't understand a whole lot about our own

0:33:25.960 --> 0:33:29.680
<v Speaker 1>bodies and especially those very delicate, very integral nervous systems

0:33:29.720 --> 0:33:31.960
<v Speaker 1>that are that are making up what we consider to

0:33:31.960 --> 0:33:34.640
<v Speaker 1>be intelligence. Right, And when you look at you know,

0:33:34.680 --> 0:33:37.680
<v Speaker 1>even the sample size we do have, which again is Earth,

0:33:37.880 --> 0:33:41.200
<v Speaker 1>that's all we've got. Uh, we only have one species

0:33:41.280 --> 0:33:45.880
<v Speaker 1>that evolved into the type of intelligence capable of interstellar communication. No,

0:33:46.000 --> 0:33:48.800
<v Speaker 1>but you have lots of species that evolved to have

0:33:48.920 --> 0:33:52.360
<v Speaker 1>pretty complex brains. Sure, Sure, ones that you know, like

0:33:52.360 --> 0:33:56.400
<v Speaker 1>like chimpanzees that that do have communication or um or

0:33:56.520 --> 0:33:59.040
<v Speaker 1>or octopi or cuttle fish that in a very different

0:33:59.040 --> 0:34:02.080
<v Speaker 1>way than we communicate, but do absolutely have a form

0:34:02.200 --> 0:34:05.800
<v Speaker 1>of almost language proto language. I mean, you know, the

0:34:05.920 --> 0:34:08.360
<v Speaker 1>exact definitions are a little bit shaky, but you know,

0:34:08.400 --> 0:34:12.200
<v Speaker 1>these are these are creatures that recognize their reflection and

0:34:12.200 --> 0:34:14.520
<v Speaker 1>and can respond to it. But if it if it

0:34:14.560 --> 0:34:18.000
<v Speaker 1>doesn't ever reach the sophistication, Uh, well, first of all,

0:34:18.040 --> 0:34:19.680
<v Speaker 1>for the Drake equation to work, we have to have

0:34:19.760 --> 0:34:21.880
<v Speaker 1>it to the point where they can do interstellar communication,

0:34:21.880 --> 0:34:24.080
<v Speaker 1>because it's just part of the equation. And unless you're

0:34:24.120 --> 0:34:28.080
<v Speaker 1>going by Douglas Adams response to it, dolphins, dolphins cannot

0:34:28.080 --> 0:34:32.240
<v Speaker 1>do that. Yeah, but that's there's no telling that given

0:34:32.280 --> 0:34:34.800
<v Speaker 1>them another you know, millions and millions of years, but

0:34:34.880 --> 0:34:36.640
<v Speaker 1>they would not. Yeah, but there's no telling that they

0:34:36.680 --> 0:34:39.160
<v Speaker 1>would either. So no, no, but but but also but also,

0:34:39.200 --> 0:34:41.359
<v Speaker 1>I mean we're talking about this this handful. I mean,

0:34:41.400 --> 0:34:44.439
<v Speaker 1>maybe less than ten species that we would consider even

0:34:44.520 --> 0:34:47.520
<v Speaker 1>moderately intelligent on the planet. Out of how many billions,

0:34:48.120 --> 0:34:50.759
<v Speaker 1>there's a lot there's still a lot of humans that

0:34:50.800 --> 0:34:54.600
<v Speaker 1>I don't necessarily lump in with intelligent groups. So fair enough,

0:34:54.840 --> 0:34:59.160
<v Speaker 1>that's that's a joke. Mostly you're not that anti social.

0:34:59.239 --> 0:35:01.960
<v Speaker 1>But I got I got a family reunion, a human

0:35:02.000 --> 0:35:05.839
<v Speaker 1>beings can build radios. It's really it's actually pretty simple.

0:35:06.400 --> 0:35:10.279
<v Speaker 1>Um yeah. Anyway, but yes, I agree that the the

0:35:10.400 --> 0:35:13.560
<v Speaker 1>life variable I think could be tweaked down just and

0:35:13.680 --> 0:35:16.360
<v Speaker 1>probably within our lifetimes. I would expect that to happen,

0:35:16.920 --> 0:35:19.799
<v Speaker 1>or at least I'm optimistic that it will happen. The

0:35:19.920 --> 0:35:23.879
<v Speaker 1>intelligent life. I'm hopeful that, you know, we could as

0:35:23.920 --> 0:35:26.239
<v Speaker 1>we learn more about our brains and the brains of

0:35:26.280 --> 0:35:29.279
<v Speaker 1>other species here on Earth, we might be able to

0:35:29.400 --> 0:35:32.840
<v Speaker 1>draw more conclusions there. The last two variables, though, the

0:35:32.880 --> 0:35:35.640
<v Speaker 1>one about being smart enough for interstellar communication and the

0:35:35.680 --> 0:35:37.880
<v Speaker 1>amount of time, those are the two I think are

0:35:37.880 --> 0:35:40.640
<v Speaker 1>going to be the longest holdouts. Um yeah. There have

0:35:40.800 --> 0:35:43.520
<v Speaker 1>been people who have tried to mess with them to

0:35:43.520 --> 0:35:46.799
<v Speaker 1>to try to inform those variables better. Uh. For one thing,

0:35:47.160 --> 0:35:50.919
<v Speaker 1>Michael Shermer, the skeptic writer and magazine publisher. In two

0:35:50.920 --> 0:35:55.120
<v Speaker 1>thousand two he published an article in Um Scientific American

0:35:55.600 --> 0:35:59.400
<v Speaker 1>where he tried to say, look, we can get a

0:35:59.440 --> 0:36:03.319
<v Speaker 1>pretty good average of the length of time UM that

0:36:03.360 --> 0:36:05.960
<v Speaker 1>we should factor into l by looking at all of

0:36:06.000 --> 0:36:10.000
<v Speaker 1>the civilizations through Earth's history and sort of averaging out

0:36:10.040 --> 0:36:14.960
<v Speaker 1>how long each civilization survived before it's collapse. Um. But

0:36:15.040 --> 0:36:18.600
<v Speaker 1>then I read some criticisms of his piece, and Um,

0:36:18.600 --> 0:36:21.000
<v Speaker 1>while Michael Michael Sherman has written a lot of good stuff,

0:36:21.120 --> 0:36:23.279
<v Speaker 1>I think some of the criticisms of this piece were

0:36:23.360 --> 0:36:25.960
<v Speaker 1>valid because he was looking at, you know, the length

0:36:25.960 --> 0:36:29.960
<v Speaker 1>of time of Chinese civilizations and South American civilizations and

0:36:30.160 --> 0:36:33.360
<v Speaker 1>Rome and African empires and all that, And what you

0:36:33.400 --> 0:36:35.359
<v Speaker 1>think all of these had in common is they didn't

0:36:35.360 --> 0:36:39.040
<v Speaker 1>have radio, so yeah, and they were and they were

0:36:39.080 --> 0:36:42.280
<v Speaker 1>localized civilizations. They weren't a global civilizations. I would argue,

0:36:42.280 --> 0:36:44.920
<v Speaker 1>we have these days, right, So it may be that

0:36:44.960 --> 0:36:48.920
<v Speaker 1>there's something fundamentally different about the length of time ah

0:36:49.160 --> 0:36:54.239
<v Speaker 1>an interstellar communicating civilization lasts as opposed to all these

0:36:54.280 --> 0:36:58.120
<v Speaker 1>empires throughout history. Well. Yeah, and it also again assumes

0:36:58.160 --> 0:37:01.160
<v Speaker 1>that that's some form of you know, almost like a

0:37:01.280 --> 0:37:05.160
<v Speaker 1>universal law that civilization can expect to last X number

0:37:05.200 --> 0:37:08.480
<v Speaker 1>of years. But that's completely based on on just the

0:37:08.560 --> 0:37:13.520
<v Speaker 1>human history, and we simply don't know anything about any

0:37:13.560 --> 0:37:17.400
<v Speaker 1>any extraterrestrial civilizations. If there are any, we don't know

0:37:17.520 --> 0:37:20.440
<v Speaker 1>enough to be able to say the human experience at

0:37:20.440 --> 0:37:24.320
<v Speaker 1>all relates to their experience. Yeah, And again it's assuming

0:37:24.400 --> 0:37:28.160
<v Speaker 1>that as long as a civilization is capable of transmitting it,

0:37:28.200 --> 0:37:31.439
<v Speaker 1>will you know that's not necessarily the case either. Now

0:37:31.719 --> 0:37:34.400
<v Speaker 1>I think you know, it sounds like we're being fairly

0:37:34.440 --> 0:37:37.120
<v Speaker 1>critical here. Uh we didn't make a joke of the

0:37:37.200 --> 0:37:40.800
<v Speaker 1>Drake equation, although some people have a right Yeah. X

0:37:40.880 --> 0:37:43.960
<v Speaker 1>K C. D Um published a comic that said that

0:37:44.000 --> 0:37:49.040
<v Speaker 1>the the unspoken variable here is how how much? What?

0:37:49.040 --> 0:37:51.799
<v Speaker 1>What was your word? What was your word? Bullpucky? Bullpucky?

0:37:51.920 --> 0:37:55.560
<v Speaker 1>You're willing to accept from from Mr Frank Drake. Dr

0:37:56.239 --> 0:37:59.279
<v Speaker 1>I'm afraid that word is offensive. I don't remember where

0:37:59.280 --> 0:38:01.440
<v Speaker 1>I heard. No, No, it's I mean, it doesn't offend me.

0:38:01.520 --> 0:38:03.799
<v Speaker 1>I'm fine with it, all right. So anyway, that being

0:38:03.800 --> 0:38:06.160
<v Speaker 1>the big joke that the unspoken variable is how much

0:38:06.160 --> 0:38:08.560
<v Speaker 1>bullpucky can you take from Frank Drake before you just

0:38:08.600 --> 0:38:11.560
<v Speaker 1>give up on that equation? Uh? Well, you know, it's

0:38:11.600 --> 0:38:14.719
<v Speaker 1>an interesting thought experiment at the very least, and hopefully

0:38:14.760 --> 0:38:17.800
<v Speaker 1>before too long it will go beyond thought experiment to

0:38:17.920 --> 0:38:20.840
<v Speaker 1>something where it's actually applicable as we get more information

0:38:20.880 --> 0:38:23.960
<v Speaker 1>about the universe around us. As I always say, learning

0:38:24.080 --> 0:38:28.040
<v Speaker 1>is just it's just something I can continuously get excited about.

0:38:28.160 --> 0:38:30.920
<v Speaker 1>So I think uh, you know, the future is a

0:38:31.120 --> 0:38:33.520
<v Speaker 1>is a bright one, really, and I expect that there

0:38:33.560 --> 0:38:36.280
<v Speaker 1>will come a time where humans will be in contact

0:38:36.320 --> 0:38:39.239
<v Speaker 1>with some other form of intelligent life out there. I

0:38:39.320 --> 0:38:41.080
<v Speaker 1>doubt that I'll be around to see it, unless I'm

0:38:41.080 --> 0:38:42.920
<v Speaker 1>a head in a jar at that point, but I

0:38:42.960 --> 0:38:45.200
<v Speaker 1>do hope it happens, which we all aspire to be. Yeah.

0:38:45.360 --> 0:38:47.400
<v Speaker 1>By the way, if anyone is putting heads in jars

0:38:47.400 --> 0:38:51.120
<v Speaker 1>and keeping them alive a very important part of that.

0:38:52.080 --> 0:38:54.960
<v Speaker 1>I want to stress that part of the bad equation,

0:38:55.160 --> 0:38:58.520
<v Speaker 1>I can help you to your all. Right, I'm gonna

0:38:58.560 --> 0:39:00.880
<v Speaker 1>wrap this up, guys, this has been a fun conversation.

0:39:00.920 --> 0:39:03.880
<v Speaker 1>I've really enjoyed it. If you've been enjoying the podcast,

0:39:03.920 --> 0:39:07.000
<v Speaker 1>make sure you go to f W Thinking dot com.

0:39:07.000 --> 0:39:11.640
<v Speaker 1>That's our home for all the blog posts, podcasts, video posts, articles,

0:39:11.920 --> 0:39:14.360
<v Speaker 1>all the cool information we talked about about the future

0:39:14.440 --> 0:39:17.000
<v Speaker 1>and other topics. Go check that out and remember to

0:39:17.040 --> 0:39:19.360
<v Speaker 1>follow us on Facebook and Twitter. You can find us

0:39:19.360 --> 0:39:22.080
<v Speaker 1>there are handle its f W Thinking and we will

0:39:22.120 --> 0:39:28.520
<v Speaker 1>taught to you again really soon. For more on this

0:39:28.600 --> 0:39:42.760
<v Speaker 1>topic and the future of technology, visit forward thinking dot com.

0:39:42.880 --> 0:39:45.719
<v Speaker 1>Brought to you by Toyota. Let's go places