WEBVTT - The Search for a New Earth

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<v Speaker 1>Welcome to Stuff to Blow your Mind from how Stuff

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<v Speaker 1>Works dot com. Hey, welcome to Stuff to Blow your Mind.

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<v Speaker 1>My name is Robert lamp and my name is Julie

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<v Speaker 1>Tuglas Um Julie. I was over the weekend I caught

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<v Speaker 1>the film John Carter that came out. Are you familiar

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<v Speaker 1>with this one at all? I am? Uh, you know,

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<v Speaker 1>the some dudes of Pixar behind at Disney behind it

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<v Speaker 1>based on Edgar Rice Burrows stories of Mars, in which

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<v Speaker 1>this character, John Carter ends up traveling there and having

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<v Speaker 1>all sorts of squash buckling, princess laden adventures. And uh,

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<v Speaker 1>it's a fun flick. I recommend people see it if

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<v Speaker 1>that's the kind of thing you're into it into McNulty

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<v Speaker 1>from The Wire shows up as the villain, which is fun.

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<v Speaker 1>But but but what really got me thinking and how

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<v Speaker 1>it ties into this podcast is that it really calls

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<v Speaker 1>back to an age when the science fiction of the

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<v Speaker 1>day uh is emerging from this idea that Mars could

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<v Speaker 1>conceivably the habitated world, or a world that had been

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<v Speaker 1>habitated by a a civilization, not just some organism living

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<v Speaker 1>deep in the soil, but it could have had civilization

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<v Speaker 1>on it. In the past or even in the present.

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<v Speaker 1>And it's just amazing to think back to that time.

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<v Speaker 1>It's and and and try to imagine that being possible

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<v Speaker 1>in your mind. Whereas today we have this, Uh, we

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<v Speaker 1>know that Mars is virtually lifeless and if even if

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<v Speaker 1>even if it has life in it, it is Uh,

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<v Speaker 1>it's not cities, it's not things that can think in

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<v Speaker 1>a way that we understand, you know, it's not it's

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<v Speaker 1>not that that vision of swashbuckling adventure that Edgar Rice

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<v Speaker 1>Burrows had. Instead, we're we're looking even farther out. We're

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<v Speaker 1>we're looking, we're having to cast our dreams even farther

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<v Speaker 1>to try and imagine other worlds that could be like Earth,

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<v Speaker 1>because that's it's kind of a simple thing. We kind

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<v Speaker 1>of want on on this very basic level. We want

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<v Speaker 1>to find that other Earth. We want to find our

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<v Speaker 1>twin out there in the galaxy. And no, that we

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<v Speaker 1>are not alone. Right, That's always been the other question, right,

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<v Speaker 1>are are we alone? Um? You know, is there extraterrestrial

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<v Speaker 1>life out there? Um? We've talked about even SETTI, the

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<v Speaker 1>organization that is committed to trying to find a form

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<v Speaker 1>of life out there. And as you said, it's really

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<v Speaker 1>interesting to think that at one point all of this

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<v Speaker 1>just sort of existed in our minds, this idea of

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<v Speaker 1>what is out there in the cosmos, not really knowing,

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<v Speaker 1>not having the sort of data or the technology to

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<v Speaker 1>substantiate um are our theories. And you know, we just

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<v Speaker 1>talked about Prometheus and we talked about how they were

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<v Speaker 1>journeying to an extra planet or an extrasolar planet. The

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<v Speaker 1>idea that it's just it's a planet. It is encircling

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<v Speaker 1>another star, which is not despite what you see in

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<v Speaker 1>Star Trek and and everything, it's not not in every

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<v Speaker 1>and not every star is going to have planets, right right,

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<v Speaker 1>an extra planet too, I mean the planets beyond our

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<v Speaker 1>solar system. This used to be just a theory as well, right,

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<v Speaker 1>So it's it's in context of of thinking about seventeen

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<v Speaker 1>years ago, it's pretty amazing that we know what we

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<v Speaker 1>know now, and it does the question now doesn't isn't

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<v Speaker 1>are their exp planets? The question is where is that

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<v Speaker 1>earth like planet and doesn't contain life. That's that's where

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<v Speaker 1>we're going towards now. Seventeen years ago that we're looking

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<v Speaker 1>back to hubble Right and cast Star gaze out outward

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<v Speaker 1>into the stars and was able to identify what planet

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<v Speaker 1>candidates based on distance stars. Well, first of all, they

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<v Speaker 1>identified two hundred billion star systems, so this was news.

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<v Speaker 1>It wasn't like, hey, here's our solar system and then

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<v Speaker 1>nothing the two hundred billion star systems and um. And

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<v Speaker 1>they did this by gathering light for hundreds of hours

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<v Speaker 1>and staring into deep space and taking all these calculations

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<v Speaker 1>and figuring this out and it was amazing. So then

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<v Speaker 1>they took that information and the Kepler mission, which we'll

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<v Speaker 1>talk about a little bit um, was able, as you say,

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<v Speaker 1>to identify twenty three hundred UM possible planets extra planets.

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<v Speaker 1>We say possible because we don't know enough information about

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<v Speaker 1>and actually call them planet candidates. And they haven't made

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<v Speaker 1>it past the candidates, and they haven't made it passive. Yeah,

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<v Speaker 1>they haven't been vetted yet. But of these we know

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<v Speaker 1>the dimensions and weight of two hundred planets, okay, and um,

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<v Speaker 1>we actually have the composition of atmospheres for twelve planets.

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<v Speaker 1>This is amazing stuff. And we're particularly interested in those

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<v Speaker 1>planets that fall within that habitable zone, that sort of

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<v Speaker 1>goldielike zone, because you look at our planets we have

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<v Speaker 1>and we went into this on the Stuff to Blow

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<v Speaker 1>your Kid's Mind video series. You have you have Venus,

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<v Speaker 1>which is uh to have to have the atmospheres to pressurize,

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<v Speaker 1>and it's too hot. You go over to Mars, you know,

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<v Speaker 1>a little far too far to the right, and you

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<v Speaker 1>find not enough atmosphere and intense cold. But right there

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<v Speaker 1>in the little Earth, it's just right the we live

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<v Speaker 1>in this golden zone. Yeah, we evolved, lack is evolved

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<v Speaker 1>as we know it to exist within these very slim

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<v Speaker 1>parameters that we're specifically talking about the orbital distance from

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<v Speaker 1>a star where liquid water on a planet could exist.

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<v Speaker 1>That's just one of the things that needs to be

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<v Speaker 1>going on UM. So yeah, I mean, we we now

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<v Speaker 1>have seven hundred confirmed exoplanets UM. Just out of that

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<v Speaker 1>all the other data, I just want to mention that

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<v Speaker 1>we do have seven hundred confirmed exoplanets UM and it's

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<v Speaker 1>amazing that we're at this point in the Kepler mission

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<v Speaker 1>is actually looking at a tiny region of the Milky Way,

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<v Speaker 1>in a very small fraction of stars in the galaxy UM.

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<v Speaker 1>And because the stars are being sampled by Kepler, are

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<v Speaker 1>very similar to predominant types of stars in the Milky

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<v Speaker 1>Way galaxy. Uh, we are getting basically, in a sense,

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<v Speaker 1>just narrow little pencil beam of stars that may or

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<v Speaker 1>may not be earth like or that we discover. So

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<v Speaker 1>that perspective is pretty mind blowing in and of itself

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<v Speaker 1>because it's just that tiny little point that they're looking at,

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<v Speaker 1>and what else could the universe contain beyond that? So,

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<v Speaker 1>like I mentioned before, like every solar system is not

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<v Speaker 1>going to be a situation of oh, we have planet one, two, three, four,

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<v Speaker 1>and five around a single star. You have, it's not

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<v Speaker 1>gonna look like ours per se. You have a variety

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<v Speaker 1>of exoplanets in a variety of solar systems. Right. You

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<v Speaker 1>have planets that are orbiting multiple stars where you would

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<v Speaker 1>conceivably have if you had a planet you could stand

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<v Speaker 1>out in that system. You might have to. You would

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<v Speaker 1>have two sons in the sky at the same time

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<v Speaker 1>or at different times, depending on how things are, how

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<v Speaker 1>the celestial mechanics are panning out. Um, you have planets

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<v Speaker 1>that don't orbit stars at all, which sounds kind of

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<v Speaker 1>crazy to just kind of rogue. Yeah, it's just on

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<v Speaker 1>their own. Um. And then you have at least one

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<v Speaker 1>that is is areas styrofoam. Yeah, yeah, And this is

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<v Speaker 1>what they're calling the planetary zoo because they're talking about

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<v Speaker 1>that the variety of planets that they're discovering and their

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<v Speaker 1>atmospheres and their their weights and dimensions. And it turns

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<v Speaker 1>out that there are smaller, more smaller plants and then

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<v Speaker 1>there are large ones at least in the area that

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<v Speaker 1>they're looking in. But it does point to this diversity

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<v Speaker 1>and this idea that things don't always work the way

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<v Speaker 1>we think they do, and so we probably need to

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<v Speaker 1>reframe the way that we're approaching things sometimes, and we

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<v Speaker 1>may even need to reconsider what the habitable habitable zone is.

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<v Speaker 1>A super Earth is basically a planet that is more

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<v Speaker 1>massive than Earth that is still expected to be predominantly rocky.

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<v Speaker 1>And that's something that we want right when we're talking

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<v Speaker 1>about an earthlike planet, we want it to be rocky

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<v Speaker 1>like ours and not gaseous and hot. Um. And this

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<v Speaker 1>is a quote from Sarah Seeger. She is um an

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<v Speaker 1>amazing UM speaker, and she's actually an astrophysicist and and

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<v Speaker 1>um a planet hunter. Her say, and she says, the

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<v Speaker 1>diversity of exto planets has really forced us to reconsider

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<v Speaker 1>what the habitable zone really is. For example, some of

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<v Speaker 1>these super Earth's are massive enough that they could retain

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<v Speaker 1>a different atmosphere than we have on Earth. These super

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<v Speaker 1>earths may hold onto the light gases hydrogen and helium.

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<v Speaker 1>In this case, if they have a massive atmosphere, they

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<v Speaker 1>could have a massive greenhouse effect. So this could actually

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<v Speaker 1>increase the range of habitable zone in a planetary system.

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<v Speaker 1>So it's a little bit different than what we've thought of.

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<v Speaker 1>We thought, Okay, you have to have the exact conditions

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<v Speaker 1>that we have here on Earth. There's this I can't

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<v Speaker 1>help but think, and I imagine some of our listeners

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<v Speaker 1>are probably thinking of this as well. There was a

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<v Speaker 1>there was a PC game back in the day called

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<v Speaker 1>Masters of Orion. They did two of them. Oh they

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<v Speaker 1>did third one that was supposedly not that good, But

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<v Speaker 1>they did two of these things, and it's uh. We

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<v Speaker 1>have different space faring races, and you're exploring new systems.

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<v Speaker 1>In each system you discover will have a range of planets,

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<v Speaker 1>and some of them will be too rocky, someone will

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<v Speaker 1>be gases only some of some of them can be

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<v Speaker 1>colonized with a certain extent and others not so much.

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<v Speaker 1>And a lot of thought. Wind of the game is

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<v Speaker 1>a very smart early um computer game, but but even

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<v Speaker 1>even it managed to feel like it misses the mark

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<v Speaker 1>and just the vast variety. Because if this game of

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<v Speaker 1>Masters a Ryan lined up with what we know now

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<v Speaker 1>about the layout of of other solar systems and the

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<v Speaker 1>existence of extraplanets, you would encounter a lot of these

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<v Speaker 1>systems that we just have nothing in them, right, yeah, yeah, again,

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<v Speaker 1>you know, we have this idea that you know, other

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<v Speaker 1>solar systems were supposed to be like ours, but yeah,

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<v Speaker 1>they're vastly different. Some of them are spinning in what

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<v Speaker 1>we think of is the wrong direction, um, like Australian

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<v Speaker 1>one that don't really a line up to the science

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<v Speaker 1>all that well, but but still backwards rotating solar systems. Yeah, yeah,

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<v Speaker 1>So actually I was just thinking, like, how cool would

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<v Speaker 1>it be if they had a planetary Zoo Tycoon game

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<v Speaker 1>similar to sort of what you're saying. If you've ever

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<v Speaker 1>played Zoo Tycoon, you know this is again another way

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<v Speaker 1>to to think about well at least start understanding of

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<v Speaker 1>what's out there. It would be very interesting. Yeah, if

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<v Speaker 1>they if they took that sort of that basic expansion

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<v Speaker 1>and colonization computer game model and really made it match

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<v Speaker 1>up with with what we know now and what the

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<v Speaker 1>conceivable uh near to long term future of of exploration is.

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<v Speaker 1>I'm just thinking, you put some really cool graphics of

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<v Speaker 1>like pandas and giraffe planets and get kids to sort

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<v Speaker 1>through the data for you. You can have like a

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<v Speaker 1>million kids playing these games and inadvertently like punching some

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<v Speaker 1>data for you. It could it could be a win

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<v Speaker 1>win um. Alright, So here's the question, how are these

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<v Speaker 1>far flung planets actually inferred? How do we know that

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<v Speaker 1>they're out there? We suspect they're out there. They don't

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<v Speaker 1>actually say definitively out there, they say inferred. Well, you

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<v Speaker 1>have two types of detection. Basically, you have you have

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<v Speaker 1>direct detection and indirect detection, all right, Um, With direct

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<v Speaker 1>detection detection, and it's one thing to detect a star,

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<v Speaker 1>but it's another thing to detect the planet. The visible

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<v Speaker 1>light output by a planet like Jupiter is one billion

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<v Speaker 1>that of its star, but if you shift into the

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<v Speaker 1>infrared spectrum, the contrast is merely a few thousands, all right,

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<v Speaker 1>So it helps to to shift the shift out of

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<v Speaker 1>that visible light spectrum. You can also block out starlight

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<v Speaker 1>and just focus on the corona, that outer plasma region

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<v Speaker 1>of the star's atmosphere, and then you can catch the

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<v Speaker 1>shine of the planets. Um. Direct imaging is the only

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<v Speaker 1>way to access some of the really important qualities of

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<v Speaker 1>an exoplanet, like how much water it has on its surface.

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<v Speaker 1>But then there are these indirect detection methods, and some

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<v Speaker 1>of these are are are pretty pretty crazy, like uh

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<v Speaker 1>another crazy that they're they're really they're really fascinating because

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<v Speaker 1>it's not a direct method of detection. You kind of

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<v Speaker 1>have to find have to find a work around to

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<v Speaker 1>detect the presence of this planet. Yeah, are you talking

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<v Speaker 1>about the biosignature gasses. Yes, that's one of the methods

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<v Speaker 1>that pops up. UM. I love this because it's like

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<v Speaker 1>a game of clue, you know. Um. This is where

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<v Speaker 1>different chemicals absorb or they take a bite out of

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<v Speaker 1>the photons and light at different parts of the spectrum

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<v Speaker 1>and can be used as a fingerprint um of the

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<v Speaker 1>atmosphere of this planet. So if we imagine the planet,

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<v Speaker 1>we can run the light given off from it through

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<v Speaker 1>a machine called a spectrograph, which analyzes the data determine

0:12:27.440 --> 0:12:31.360
<v Speaker 1>the chemicals and the planet's atmosphere um some chemicals which

0:12:31.360 --> 0:12:36.000
<v Speaker 1>science is called biomarkers. Biomarkers may hint at life on

0:12:36.040 --> 0:12:38.160
<v Speaker 1>a planet. At least, that doesn't mean that there's life.

0:12:38.200 --> 0:12:40.160
<v Speaker 1>It just means that if you have certain chemicals that

0:12:40.200 --> 0:12:42.720
<v Speaker 1>are taking a bite out of that light spectrum and

0:12:42.760 --> 0:12:44.800
<v Speaker 1>you can see it missing, then you can start to

0:12:44.880 --> 0:12:48.480
<v Speaker 1>ascertain the percentages of chemicals in the atmosphere. And I

0:12:48.480 --> 0:12:52.400
<v Speaker 1>think that is amazing. Yeah, there's also the wheat gravity

0:12:52.440 --> 0:12:55.679
<v Speaker 1>of a planet pulls the star into the small circular

0:12:55.760 --> 0:12:59.400
<v Speaker 1>orbit and induces a minute wobble that can be detected

0:12:59.480 --> 0:13:03.559
<v Speaker 1>using radial velocity tracking, which is which is pretty cool.

0:13:03.600 --> 0:13:06.160
<v Speaker 1>And then there's a there's also this scenaria where the

0:13:06.679 --> 0:13:09.559
<v Speaker 1>planet moves between a star and the observer and the

0:13:09.840 --> 0:13:14.080
<v Speaker 1>luminosity shifts. There's a that's that's the transit method, and

0:13:14.080 --> 0:13:17.400
<v Speaker 1>that's actually what the Kepler telescope is using. And just

0:13:17.480 --> 0:13:19.480
<v Speaker 1>to go back to the Kepler mission, we're talking about

0:13:20.280 --> 0:13:23.959
<v Speaker 1>basically a giant ninety eight megapixel digital camera that is

0:13:24.000 --> 0:13:28.360
<v Speaker 1>taking these photos. Like you were saying, when it crosses

0:13:28.400 --> 0:13:32.040
<v Speaker 1>the star, you're basically going to see um that a

0:13:32.040 --> 0:13:33.959
<v Speaker 1>little bit of the light is blocked out and then

0:13:33.960 --> 0:13:36.319
<v Speaker 1>the camera will measure a dip in the star's brightness,

0:13:36.400 --> 0:13:38.679
<v Speaker 1>and if a planet is really what's causing that dip,

0:13:38.720 --> 0:13:40.520
<v Speaker 1>it'll come around and cause the same kind of dip

0:13:40.559 --> 0:13:42.600
<v Speaker 1>again and again and again. So a lot of this

0:13:42.640 --> 0:13:45.000
<v Speaker 1>is pointing toward this idea that you have to have

0:13:45.080 --> 0:13:49.240
<v Speaker 1>a ton of patients if you are a planet hunter. Yeah, because,

0:13:49.520 --> 0:13:51.719
<v Speaker 1>like I said, it's one thing to find a start. Um.

0:13:51.840 --> 0:13:54.760
<v Speaker 1>We can sometimes detect things like black holes, for instance,

0:13:54.920 --> 0:13:57.920
<v Speaker 1>or potential black holes with gravitational lensing, where we see

0:13:57.960 --> 0:14:00.960
<v Speaker 1>the way that the mass of an object causes light

0:14:01.000 --> 0:14:04.320
<v Speaker 1>to bend around it. Well, then there's gravitational micro lensing

0:14:04.640 --> 0:14:07.840
<v Speaker 1>where you're kind of you're you're you're observing the way

0:14:07.840 --> 0:14:10.280
<v Speaker 1>that the star is causing light to bend. But then

0:14:10.320 --> 0:14:12.400
<v Speaker 1>you're also on top of that observing the way that

0:14:12.400 --> 0:14:16.120
<v Speaker 1>that stars planets are adding, uh, in a smaller sense

0:14:16.200 --> 0:14:19.400
<v Speaker 1>to the bending of that light. Yeah. What I like

0:14:19.480 --> 0:14:21.880
<v Speaker 1>about this too, this planet hunting, is that it kind

0:14:21.880 --> 0:14:25.600
<v Speaker 1>of pulls in so many different disciplines. And you have astrophysicists, physicists,

0:14:25.880 --> 0:14:29.440
<v Speaker 1>you have astrobiologists who are really interested in trying to

0:14:29.480 --> 0:14:32.280
<v Speaker 1>figure out what the atmosphere looked like in the early days,

0:14:32.320 --> 0:14:34.800
<v Speaker 1>because having that sort of data can help us then

0:14:34.840 --> 0:14:37.080
<v Speaker 1>look at another planet and say, well, this could be

0:14:37.800 --> 0:14:41.160
<v Speaker 1>an earth light planet perhaps in four billion years, because

0:14:41.200 --> 0:14:43.280
<v Speaker 1>it really matches what we think the Earth look like

0:14:43.400 --> 0:14:47.000
<v Speaker 1>back in the day um or maybe it's halfway to

0:14:47.080 --> 0:14:50.440
<v Speaker 1>that point or so. It's really interesting that everybody is

0:14:51.000 --> 0:14:54.600
<v Speaker 1>sharing all of this data and trying to to get

0:14:54.600 --> 0:14:58.200
<v Speaker 1>to the to the answer to the question, which is

0:14:58.200 --> 0:15:00.360
<v Speaker 1>is there another Us out there? Yeah? And you mentioned

0:15:00.400 --> 0:15:03.040
<v Speaker 1>clue earlier, and I keep coming back to that because

0:15:03.080 --> 0:15:05.760
<v Speaker 1>because it's kind of like this, it reminds me a

0:15:05.800 --> 0:15:11.040
<v Speaker 1>lot of high tech movie TV show crime scene where

0:15:11.080 --> 0:15:13.200
<v Speaker 1>you have like people are coming in. You have your

0:15:13.240 --> 0:15:15.840
<v Speaker 1>botanists that are looking at what what what plants are doing?

0:15:15.880 --> 0:15:19.160
<v Speaker 1>You have you know, biologists, you have entomologists coming in,

0:15:19.320 --> 0:15:22.160
<v Speaker 1>think of for an experts, people are shining lasers. All

0:15:22.200 --> 0:15:24.480
<v Speaker 1>of these different disciplines are coming together, all of these

0:15:24.480 --> 0:15:28.800
<v Speaker 1>different technologies coming together to put a face on this

0:15:28.920 --> 0:15:32.680
<v Speaker 1>question mark you know, where who is the killer? And uh?

0:15:32.800 --> 0:15:34.320
<v Speaker 1>And we see a similar thing here with it with

0:15:34.360 --> 0:15:37.600
<v Speaker 1>the question mark being is there another Earth? Is there

0:15:37.640 --> 0:15:41.240
<v Speaker 1>is there another planet out there that that resembles us? Yeah,

0:15:41.280 --> 0:15:43.080
<v Speaker 1>and I like that that you pointed out that way

0:15:43.080 --> 0:15:45.880
<v Speaker 1>that is sort of backing up into the equation and

0:15:45.960 --> 0:15:49.160
<v Speaker 1>taking all that data and trying to reconstruct the crime

0:15:49.200 --> 0:15:52.040
<v Speaker 1>scene or the scene of the life, I guess, the

0:15:52.320 --> 0:15:55.560
<v Speaker 1>scene of possible life. Um, let's take a quick break

0:15:55.640 --> 0:15:57.760
<v Speaker 1>and then when we get back, we'll talk about trying

0:15:57.800 --> 0:16:07.200
<v Speaker 1>to find a true Earth twin. So we're back, and uh, yeah,

0:16:07.240 --> 0:16:10.400
<v Speaker 1>the idea of finding a true Earth twin. It reminds

0:16:10.400 --> 0:16:13.520
<v Speaker 1>me a lot of house hunting because you're looking at

0:16:13.560 --> 0:16:17.800
<v Speaker 1>potential houses, and some houses are not on the market

0:16:17.800 --> 0:16:20.560
<v Speaker 1>at all, so there's not even you know, like much

0:16:20.600 --> 0:16:23.680
<v Speaker 1>like these solar systems or even non solar systems, where

0:16:23.680 --> 0:16:27.600
<v Speaker 1>there's just nothing resembling a planet, uh that we're interested in. Uh.

0:16:27.640 --> 0:16:30.120
<v Speaker 1>And then you have then you have planets. I mean,

0:16:30.160 --> 0:16:32.680
<v Speaker 1>then you have houses that are either they're either too

0:16:32.720 --> 0:16:35.360
<v Speaker 1>expensive or you get to look at them and they're

0:16:35.360 --> 0:16:38.240
<v Speaker 1>just to run down, or or they look good at first,

0:16:38.280 --> 0:16:39.640
<v Speaker 1>but then you find out that they have some sort

0:16:39.680 --> 0:16:42.280
<v Speaker 1>of major problem like uh, you know, it's a part

0:16:42.280 --> 0:16:46.480
<v Speaker 1>of the house is collapsing, or it's uh, it's atmosphere

0:16:46.520 --> 0:16:49.240
<v Speaker 1>is too heavy and won't allow life to exist. In

0:16:49.240 --> 0:16:51.920
<v Speaker 1>it that you see what I'm saying here, it becomes this.

0:16:52.080 --> 0:16:55.000
<v Speaker 1>It's like the Goldilocks scenario, except with a far pickier

0:16:55.040 --> 0:17:00.560
<v Speaker 1>Goldilocks and so many more um unacceptable containers of poor it. Well,

0:17:00.600 --> 0:17:03.800
<v Speaker 1>if you are Sarah Seg, you're the planetary scientists, um

0:17:03.840 --> 0:17:06.800
<v Speaker 1>an astrophysicists, you do kind of want a mystery house,

0:17:07.359 --> 0:17:09.520
<v Speaker 1>at least for her. She she says, she that we

0:17:09.560 --> 0:17:12.280
<v Speaker 1>want to look at an atmosphere in search for things

0:17:12.280 --> 0:17:16.760
<v Speaker 1>that are unusual. So our own atmosphere is oxygen by volume.

0:17:16.920 --> 0:17:20.000
<v Speaker 1>If she says, an alien civilization is looking at us

0:17:20.000 --> 0:17:23.320
<v Speaker 1>from four light years away, presumably with an awesome telescope,

0:17:23.720 --> 0:17:26.399
<v Speaker 1>and it knows something about chemistry, then it will know

0:17:26.480 --> 0:17:29.119
<v Speaker 1>that we have millions to billions of times more oxygen

0:17:29.119 --> 0:17:31.280
<v Speaker 1>than we should if there were no life on Earth.

0:17:31.560 --> 0:17:34.080
<v Speaker 1>So that should be a clue to them. There's something

0:17:34.080 --> 0:17:38.960
<v Speaker 1>going on here through further synthesis, through the interaction of

0:17:39.040 --> 0:17:43.720
<v Speaker 1>oxygen and carbon dioxide, that that is not fitting uh

0:17:43.720 --> 0:17:46.720
<v Speaker 1>in line with what its composition should be, and so

0:17:46.760 --> 0:17:48.560
<v Speaker 1>we're looking for something that's not right. We're looking in

0:17:48.760 --> 0:17:52.560
<v Speaker 1>the same way to the murder investigation is ends up

0:17:52.760 --> 0:17:56.080
<v Speaker 1>chasing after individuals that are suspicious in some way, shape

0:17:56.160 --> 0:17:58.840
<v Speaker 1>or form, whose story doesn't quite add up. We're doing

0:17:58.920 --> 0:18:01.600
<v Speaker 1>looking for that planet with a story that doesn't quite

0:18:01.600 --> 0:18:04.320
<v Speaker 1>add up. Why does it have this much oxygen? Why

0:18:04.359 --> 0:18:06.919
<v Speaker 1>was it spotted leaving it's a it's apartment at the

0:18:07.000 --> 0:18:10.120
<v Speaker 1>three in the morning garbage bag. That's right to fear

0:18:10.160 --> 0:18:13.399
<v Speaker 1>the planetary dick detective. Then these are the questions that

0:18:13.440 --> 0:18:17.120
<v Speaker 1>they're asking and UM, And what I think is interesting

0:18:17.200 --> 0:18:20.560
<v Speaker 1>is that these these seventeen years, so much of this

0:18:20.640 --> 0:18:23.560
<v Speaker 1>has just been an exercise. And let's let's comb through

0:18:23.560 --> 0:18:25.760
<v Speaker 1>the data and let's try to take measurements. First. That

0:18:25.800 --> 0:18:27.119
<v Speaker 1>was the first thing that they wanted to do. Can

0:18:27.160 --> 0:18:31.520
<v Speaker 1>we take measurements of these planets? Um? The second thing

0:18:31.560 --> 0:18:34.560
<v Speaker 1>is can we figure out what's in them the habitable zone?

0:18:34.640 --> 0:18:38.040
<v Speaker 1>Can we start to really figure out whether native? Are

0:18:38.040 --> 0:18:40.639
<v Speaker 1>they hot and gassie or they rocky? And then it

0:18:40.720 --> 0:18:43.920
<v Speaker 1>became well, let's really see what's taking a bite out

0:18:43.920 --> 0:18:47.040
<v Speaker 1>of the atmosphere here. Let's see if if the composition

0:18:47.119 --> 0:18:50.560
<v Speaker 1>can give us um a clue as to an earth

0:18:50.640 --> 0:18:56.760
<v Speaker 1>like twin for us And now Seeger and obviously others

0:18:56.800 --> 0:19:00.639
<v Speaker 1>in her labs are looking much more specifically at that

0:19:00.760 --> 0:19:03.320
<v Speaker 1>data set that Kepler has given them, those twenty three

0:19:03.400 --> 0:19:07.600
<v Speaker 1>hundred planetary candidates, And she is actually helping to build

0:19:07.600 --> 0:19:12.359
<v Speaker 1>a prototype nano satellite that will be launched in and

0:19:12.440 --> 0:19:13.960
<v Speaker 1>she says that instead of looking at a hundred and

0:19:14.000 --> 0:19:16.560
<v Speaker 1>fifties six thousand distant stars, we hope to survey the

0:19:16.640 --> 0:19:20.080
<v Speaker 1>very nearest sunlight star for transitting Earth sized planets. So

0:19:20.480 --> 0:19:24.000
<v Speaker 1>the return to studying individual extra planets will be for

0:19:24.040 --> 0:19:27.040
<v Speaker 1>those orbiting stars that are close enough for detailed follow up.

0:19:27.160 --> 0:19:29.600
<v Speaker 1>So they just keep honing in more and more on

0:19:29.680 --> 0:19:32.440
<v Speaker 1>this idea that we can answer this question in this generation,

0:19:32.680 --> 0:19:34.760
<v Speaker 1>and then coming in ten, we have a James Webb

0:19:34.800 --> 0:19:37.720
<v Speaker 1>telescope which is going to just even look more laser

0:19:37.720 --> 0:19:41.480
<v Speaker 1>focused at those habitable zones. Yeah, and Singer was on

0:19:41.520 --> 0:19:44.400
<v Speaker 1>a panel at the World Science Festival about exp planets

0:19:44.480 --> 0:19:47.480
<v Speaker 1>along with Natalie to Halla. She's a physicist and team

0:19:47.560 --> 0:19:50.720
<v Speaker 1>leader the Kepler YEP, and that Mountain, the director of

0:19:50.720 --> 0:19:53.760
<v Speaker 1>the Space Telescope Science Institute. Now, they all it was

0:19:53.800 --> 0:19:56.479
<v Speaker 1>a very spirited conversation and they all had different ideas

0:19:56.480 --> 0:19:59.520
<v Speaker 1>about how to go about planet hunting, but I think

0:19:59.560 --> 0:20:03.639
<v Speaker 1>they all degree agree that UM this is something that

0:20:03.760 --> 0:20:06.960
<v Speaker 1>is going to happen in our generation, and they're pretty

0:20:07.040 --> 0:20:09.480
<v Speaker 1>much hamstrung by the technology. Now they could do it.

0:20:09.640 --> 0:20:12.720
<v Speaker 1>They could find an earthlike planet if they had every

0:20:12.720 --> 0:20:15.880
<v Speaker 1>dollar at their disposal, because they could build the right

0:20:15.920 --> 0:20:19.199
<v Speaker 1>sort of UM instruments to do this with it. But

0:20:19.359 --> 0:20:22.159
<v Speaker 1>they are saying that it's very hopeful that you have

0:20:22.280 --> 0:20:25.960
<v Speaker 1>space X, that you have asteroid mining and basically some

0:20:26.040 --> 0:20:29.080
<v Speaker 1>private companies coming in and creating the technology which will

0:20:29.119 --> 0:20:32.600
<v Speaker 1>allow them, just like the nano satellite that seekers working on,

0:20:32.920 --> 0:20:35.960
<v Speaker 1>to really get in and study it much further. And

0:20:36.000 --> 0:20:40.160
<v Speaker 1>it's I think it's just really exciting time to know that, um,

0:20:41.720 --> 0:20:45.480
<v Speaker 1>you know, again, this earthlike planet might be identified, Would

0:20:45.520 --> 0:20:47.760
<v Speaker 1>we travel to it? Would there being aliens that consume us?

0:20:47.880 --> 0:20:51.800
<v Speaker 1>I don't know. Yeah, it's I think I've missed this before,

0:20:51.840 --> 0:20:54.879
<v Speaker 1>but things like this kind of remind me of of

0:20:55.000 --> 0:20:58.320
<v Speaker 1>that day when I first started out stuff works and

0:20:58.359 --> 0:21:01.399
<v Speaker 1>the news head hit that some guys in World, Georgia

0:21:01.440 --> 0:21:03.840
<v Speaker 1>had a cooler with a big foot in it, an

0:21:03.880 --> 0:21:07.399
<v Speaker 1>actual dead sasquatch, And for a split second there I

0:21:07.440 --> 0:21:09.639
<v Speaker 1>was kind of like, is this really going to happen?

0:21:09.800 --> 0:21:12.920
<v Speaker 1>Is this really gonna turn out to be Bigfoot, and

0:21:12.920 --> 0:21:15.760
<v Speaker 1>of course it didn't. But but there was a moment

0:21:15.760 --> 0:21:20.159
<v Speaker 1>there of possibility, and with our search for exoplanets, that

0:21:20.280 --> 0:21:25.119
<v Speaker 1>moment of possibility continues to to draw out. Um, you

0:21:25.119 --> 0:21:26.920
<v Speaker 1>can draw out to the point where some people perhaps

0:21:27.000 --> 0:21:29.240
<v Speaker 1>lose interest in it and they just tend to think, oh, well,

0:21:29.280 --> 0:21:31.080
<v Speaker 1>I guess the rest of the universe is empty because

0:21:31.080 --> 0:21:35.399
<v Speaker 1>we haven't found uh, that magic planet yet. But you know,

0:21:35.720 --> 0:21:37.159
<v Speaker 1>some people would say that there are a lot of

0:21:37.200 --> 0:21:39.040
<v Speaker 1>fish in the sea, there are a lot of planets

0:21:39.520 --> 0:21:41.680
<v Speaker 1>uh out there in the universe, and if we look

0:21:41.720 --> 0:21:44.760
<v Speaker 1>long enough, uh, we will find it. Well. And what

0:21:44.800 --> 0:21:47.280
<v Speaker 1>they said on the panel is if, if, if anything,

0:21:47.480 --> 0:21:50.560
<v Speaker 1>scientists are patient and they will come for the data

0:21:50.640 --> 0:21:52.840
<v Speaker 1>and they will find that needle in the haystack. It's

0:21:52.920 --> 0:21:56.040
<v Speaker 1>just a matter of time, um Seeker said. And I

0:21:56.040 --> 0:21:58.120
<v Speaker 1>thought this was interesting. If you want to look back

0:21:58.119 --> 0:22:00.760
<v Speaker 1>to what we remember hundreds of years ago, inevitably it

0:22:00.880 --> 0:22:03.919
<v Speaker 1>is the great explorers, Christopher Columbus didn't know what he

0:22:04.000 --> 0:22:06.000
<v Speaker 1>was going to find, and he came across North America.

0:22:06.400 --> 0:22:08.879
<v Speaker 1>Many of us working in the field of exoplanets believe

0:22:08.920 --> 0:22:11.080
<v Speaker 1>that thousands of years from now, when people look back

0:22:11.080 --> 0:22:13.679
<v Speaker 1>at our generation in the early twenty first century, they

0:22:13.720 --> 0:22:16.280
<v Speaker 1>will remember the discovery of other earths as one of

0:22:16.320 --> 0:22:20.080
<v Speaker 1>our most significant accomplishments. That is the beginning of what's

0:22:20.119 --> 0:22:22.680
<v Speaker 1>out there? What are the what are the planets? Known?

0:22:23.200 --> 0:22:25.760
<v Speaker 1>And in the future, we hope that our descendants will

0:22:25.800 --> 0:22:31.480
<v Speaker 1>find signs of life. I don't know, Yeah, there you go. Um.

0:22:31.720 --> 0:22:34.080
<v Speaker 1>I certainly hope to see it, and I think that

0:22:34.119 --> 0:22:36.720
<v Speaker 1>would just be a super exciting thing. Yeah, I think

0:22:36.720 --> 0:22:39.760
<v Speaker 1>it would be tremendous. And again, it's what I love

0:22:39.760 --> 0:22:41.720
<v Speaker 1>about stuff like this is that it forces us to

0:22:41.760 --> 0:22:45.000
<v Speaker 1>recast our understanding of the universe, universe in our place

0:22:45.040 --> 0:22:47.680
<v Speaker 1>in it, and we've talked a lot about that. So

0:22:47.960 --> 0:22:51.359
<v Speaker 1>if it comes to fruition, that's pretty awesome. Coo, Well,

0:22:51.680 --> 0:22:56.199
<v Speaker 1>let's call the robot over. We well, we didn't call

0:22:56.280 --> 0:22:59.000
<v Speaker 1>him over in the Prometheus episode because it was super

0:22:59.080 --> 0:23:03.080
<v Speaker 1>long and all, so we had some some rather complex

0:23:03.119 --> 0:23:06.880
<v Speaker 1>thoughts to convey about the nature of AI and yeah,

0:23:06.920 --> 0:23:08.600
<v Speaker 1>basically you boot him on the room because we didn't

0:23:08.600 --> 0:23:11.159
<v Speaker 1>want to give him any funny ideas about how he

0:23:11.200 --> 0:23:14.520
<v Speaker 1>could emulate David. So all right, let's see what we

0:23:14.560 --> 0:23:17.280
<v Speaker 1>have here from listeners. Well, this one was exciting because

0:23:17.480 --> 0:23:20.560
<v Speaker 1>we got hats. We did. Some of the podcasters also

0:23:20.800 --> 0:23:23.159
<v Speaker 1>received these and like them. We will will have to

0:23:23.280 --> 0:23:25.680
<v Speaker 1>get a snapshot here of us wearing them. But we

0:23:25.800 --> 0:23:29.080
<v Speaker 1>heard from Adam. Adam wrote in to say, first I

0:23:29.119 --> 0:23:31.560
<v Speaker 1>have to say I've been a lawyer a lawyer. I've

0:23:31.560 --> 0:23:34.520
<v Speaker 1>been a loyal listener since the stuff you missed in

0:23:34.560 --> 0:23:39.040
<v Speaker 1>science class days um, and you actually read a listener

0:23:39.080 --> 0:23:41.320
<v Speaker 1>of feedback. I wrote about the oil industry on the

0:23:41.359 --> 0:23:44.160
<v Speaker 1>Old Show, how it's not as luxurious as the rig

0:23:44.240 --> 0:23:47.199
<v Speaker 1>on the rigs as people think, though the platforms are nicer.

0:23:47.600 --> 0:23:50.840
<v Speaker 1>As an engineer out of practice, your episodes captivate the

0:23:50.840 --> 0:23:53.399
<v Speaker 1>inner scientist and geek within me. Thank you for that.

0:23:53.520 --> 0:23:56.000
<v Speaker 1>Switching gears. For the past ten months, I've been traveling

0:23:56.040 --> 0:23:59.119
<v Speaker 1>through Latin America on what I call the Happy Nomad Tour.

0:23:59.440 --> 0:24:02.840
<v Speaker 1>After being miserable quote unquote living the dream of living

0:24:02.960 --> 0:24:06.159
<v Speaker 1>working in worry free Denmark for a wind power company,

0:24:06.200 --> 0:24:09.199
<v Speaker 1>I finally started asking myself what my passions are, what

0:24:09.320 --> 0:24:11.840
<v Speaker 1>my dreams are, and what I want out of life.

0:24:11.920 --> 0:24:16.359
<v Speaker 1>I call this process the happiness plunge um, which also

0:24:16.400 --> 0:24:20.679
<v Speaker 1>sounds like maybe like a novelty dessert that you would get.

0:24:19.720 --> 0:24:25.760
<v Speaker 1>I can't throw yourself back into a refreshing pool of tea,

0:24:25.920 --> 0:24:31.320
<v Speaker 1>but as anyway, he continues, MY goal as a traveler

0:24:31.400 --> 0:24:34.119
<v Speaker 1>is to leave each place better than how I found it,

0:24:34.440 --> 0:24:36.919
<v Speaker 1>which I do by volunteering everywhere I go. I've had

0:24:37.000 --> 0:24:40.359
<v Speaker 1>volunteering experiences such as feeding the elderly at nursing homes

0:24:40.359 --> 0:24:44.440
<v Speaker 1>in Mexico, installing solar panels and rural hunduras, attracting book

0:24:44.720 --> 0:24:47.920
<v Speaker 1>donations for a rural library project in Peru, playing with

0:24:48.000 --> 0:24:51.359
<v Speaker 1>kids at orphanages in Costa Rica and Ecuador, designing a

0:24:51.440 --> 0:24:55.399
<v Speaker 1>financial strategy for a new NGO in El Salvador, and

0:24:55.480 --> 0:24:58.359
<v Speaker 1>marketing an organization that turns donated to use bikes into

0:24:58.359 --> 0:25:02.840
<v Speaker 1>bike machines, washing machines, blenders, water well pumps, etcetera. In Guatemala.

0:25:03.240 --> 0:25:06.160
<v Speaker 1>There's a lot I can offer as an engineer NBA.

0:25:06.480 --> 0:25:08.520
<v Speaker 1>I listened to quite a few hs W podcast on

0:25:08.600 --> 0:25:10.639
<v Speaker 1>my ten to twenty our bus rides and wanted to,

0:25:10.760 --> 0:25:12.320
<v Speaker 1>in a very small way, thank you for what you've

0:25:12.359 --> 0:25:14.640
<v Speaker 1>given me. Peru is my last stop in Latin America,

0:25:14.880 --> 0:25:19.120
<v Speaker 1>and I thought these all pack out wool Julio's Julio's

0:25:22.200 --> 0:25:26.600
<v Speaker 1>feel there's one pronunciation different pronunciation to me, then we'll

0:25:26.600 --> 0:25:29.680
<v Speaker 1>call him Julia. We're a great way to say things.

0:25:30.240 --> 0:25:32.720
<v Speaker 1>And no, it doesn't get too cold. I know it

0:25:32.760 --> 0:25:34.920
<v Speaker 1>doesn't get too cold in Atlanta, but still I wanted

0:25:34.920 --> 0:25:37.679
<v Speaker 1>to protect those knowledge filled noggats. I'm at home now,

0:25:37.760 --> 0:25:39.919
<v Speaker 1>visiting my family and preparing for the Asian leg of

0:25:39.920 --> 0:25:41.919
<v Speaker 1>the Happy Nomad Tour. I look forward to listening to

0:25:41.960 --> 0:25:44.560
<v Speaker 1>you guys on the other side of the planet very soon.

0:25:44.960 --> 0:25:46.679
<v Speaker 1>Once again, thank you for all you've taught me. I

0:25:46.720 --> 0:25:50.639
<v Speaker 1>hope you know how appreciated you are. You're super fan Adam,

0:25:50.680 --> 0:25:53.360
<v Speaker 1>and he also shares a couple of links here, um

0:25:53.400 --> 0:25:56.840
<v Speaker 1>Happiness Plunge one word dot com that's the website for

0:25:56.880 --> 0:26:00.520
<v Speaker 1>this and crazy Hair Fundraiser dot com Crazy z Hair

0:26:01.040 --> 0:26:05.720
<v Speaker 1>fund Raiser h A I R not h R e Um. Yeah,

0:26:05.720 --> 0:26:08.080
<v Speaker 1>thank you, Adams. Really cool. Actually, even though it's eighty

0:26:08.160 --> 0:26:10.120
<v Speaker 1>six degrees in Atlanta today, I was wearing my hat

0:26:10.160 --> 0:26:13.160
<v Speaker 1>this morning, so I appreciate that, and I appreciate your thoughts. Yeah,

0:26:13.240 --> 0:26:15.159
<v Speaker 1>and it really it sounds like, I mean, it's an

0:26:15.160 --> 0:26:17.960
<v Speaker 1>awesome thing that you're doing, so yeah, keep it up. Yeah,

0:26:18.040 --> 0:26:21.000
<v Speaker 1>I mean, gosh, some people take off little time rest,

0:26:21.040 --> 0:26:25.760
<v Speaker 1>do you your you're no? Uh low fer there, I'll

0:26:25.760 --> 0:26:28.360
<v Speaker 1>say that and uh and thanks for the hat. Thanks

0:26:28.359 --> 0:26:30.920
<v Speaker 1>for writing in. If you guys would like to share

0:26:30.960 --> 0:26:34.119
<v Speaker 1>something with us, UM, especially if it's the kind of

0:26:34.119 --> 0:26:36.920
<v Speaker 1>thing you can post on Facebook, you can find us

0:26:37.000 --> 0:26:40.080
<v Speaker 1>on Facebook, where we are Stuff to Blow Your Mind.

0:26:40.160 --> 0:26:41.840
<v Speaker 1>You can find us on Twitter, where our handle is

0:26:41.880 --> 0:26:44.320
<v Speaker 1>blow the Mind. Let us know what you think about

0:26:44.320 --> 0:26:46.320
<v Speaker 1>the search for exoplanets. What do you think it's gonna

0:26:46.359 --> 0:26:49.520
<v Speaker 1>be like the day that that breaks on the local

0:26:49.520 --> 0:26:51.760
<v Speaker 1>news channel. How is it going to be interpreted by

0:26:51.920 --> 0:26:56.000
<v Speaker 1>pundits on various cable news channels. I don't know. We'll

0:26:56.000 --> 0:27:00.800
<v Speaker 1>see what happened shut some thoughts on that will be interesting. UM.

0:27:00.880 --> 0:27:03.360
<v Speaker 1>You can also send us your thoughts via email at

0:27:03.440 --> 0:27:10.600
<v Speaker 1>Blow the Mind at Discovery dot com. Be sure to

0:27:10.680 --> 0:27:13.439
<v Speaker 1>check out our new video podcast, Stuff from the Future.

0:27:13.800 --> 0:27:16.120
<v Speaker 1>Join How Stuff Work staff as we explore the most

0:27:16.119 --> 0:27:18.920
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