WEBVTT - How do you navigate in deep space?

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<v Speaker 1>Hey, Daniel, do you remember the days before we had smartphones?

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<v Speaker 1>I try not to think about it too much. Well,

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<v Speaker 1>you can't live with that, Wikipedia do your fingertips? How

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<v Speaker 1>else would I seem like an expert on anything? But no,

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<v Speaker 1>mostly I couldn't live without the direction right. Yeah. Are

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<v Speaker 1>you the kind of driver that needs to check them

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<v Speaker 1>out every ten seconds? Oh? Yeah, that is me. I

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<v Speaker 1>like to know exactly where I am on the surface

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<v Speaker 1>of the air at all times. At all times, I

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<v Speaker 1>need constant updates to make sure I've not gone off. Well,

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<v Speaker 1>what are you gonna do when humans get out into space?

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<v Speaker 1>Are you gonna get around there? I'm just gonna wait

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<v Speaker 1>until there are enough cell towers or at least WiFi. Yeah,

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<v Speaker 1>basic human survival needs in space, air, food, and WiFi. Hi.

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<v Speaker 1>I'm Jorge. I'm a cartoonist and the creator of PhD comments. Hi.

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<v Speaker 1>I'm Daniel. I'm a particle physicist, and I plan to

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<v Speaker 1>be the one million person in space. One million there.

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<v Speaker 1>You know there are seven billion of those, so you

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<v Speaker 1>know you let's put it pretty far ahead in line. Yeah. Well,

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<v Speaker 1>I don't want to be the first person, or the

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<v Speaker 1>second person or the hundredth person, but I also don't

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<v Speaker 1>want to be the last person. You don't want to

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<v Speaker 1>go when it's still kind of new and fresh but

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<v Speaker 1>not dangerous. I'm not a test pilot kind of a person.

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<v Speaker 1>A million sounds about right. A million sounds about right,

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<v Speaker 1>but hey, I'm flexible two million, million and a half.

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<v Speaker 1>You know I'm not going to elbow my way in

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<v Speaker 1>that line. Well, welcome to our podcast where you are

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<v Speaker 1>first in line to hear this. It's called Daniel and

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<v Speaker 1>Jorge Explain the Universe, a production of I Heart Radio

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<v Speaker 1>where normally we take you on a mental trip around

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<v Speaker 1>the cosmos, zooming out from the tiniest little particles that

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<v Speaker 1>define the basic building blocks of the universe all the

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<v Speaker 1>way out to the grandest structures that shape the nature

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<v Speaker 1>of the cosmos itself. Yeah. I just think it was

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<v Speaker 1>as your guide, as your personal GPS to all of

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<v Speaker 1>the amazing and wonderful things that are in the universe

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<v Speaker 1>and also all of the unknown things that are out

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<v Speaker 1>there for us to discover. Do you think we're a

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<v Speaker 1>good mental GPS. Sometimes we get lost, We get on

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<v Speaker 1>a discussion about neutrinos and we end up talking about

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<v Speaker 1>snack foods. Well, you know, I think detours are part

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<v Speaker 1>of the fun of a trip. Right. I wish that

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<v Speaker 1>my navigation like Siri would tell me, like, hey, pull

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<v Speaker 1>over and get some chips. There's a good snack shop

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<v Speaker 1>right here. Why not? Yeah, that should be a setting, right,

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<v Speaker 1>suggests snacks. I like that suggests yeah, AI engineers, get

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<v Speaker 1>on it. Not in a hurry. Should be maybe an

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<v Speaker 1>option open to wonderful discovery. That's right. And on this

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<v Speaker 1>podcast we try to open your mind to all the

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<v Speaker 1>future wonderful discoveries that science will bring us. And we

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<v Speaker 1>do that by talking about the cutting edge of science,

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<v Speaker 1>all the questions that science has not answered, all the

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<v Speaker 1>things scientists are trying to think ground, and all the

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<v Speaker 1>technical problems they're trying to solve on their journey to

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<v Speaker 1>give us the answers. Yeah, because I think sometimes to

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<v Speaker 1>think about a journey of discovery is the journey itself,

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<v Speaker 1>you know, and the friends you make along the way. Yeah,

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<v Speaker 1>you know, not just where you go and what do

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<v Speaker 1>you find when you get there? For also how do

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<v Speaker 1>you get there and how do you how do you

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<v Speaker 1>even know where to go when you're going? Yeah, I

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<v Speaker 1>think people imagine that it's hard to get to Jupiter

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<v Speaker 1>or Pluto because it's so far out there. It's just

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<v Speaker 1>like you gotta throw a rock really far into space,

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<v Speaker 1>but it's not just really far away. It's like very

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<v Speaker 1>hard to find. You know. Pluto is a small rock

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<v Speaker 1>in the vast, vast reaches of space. If you're gonna

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<v Speaker 1>throw something in that direction, you have to be really precise.

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<v Speaker 1>You have to really know how to aim it and

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<v Speaker 1>have to be able to course correct along the way.

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<v Speaker 1>And that turns out to be not so easy. It's

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<v Speaker 1>much harder than stopping for snacks. Yeah, you know, they

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<v Speaker 1>have good snacks and jubiter. You know, it makes a

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<v Speaker 1>little gassy at the end, but you know it's all

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<v Speaker 1>totally worth it, right right the Red Storm chips. I

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<v Speaker 1>love this. Yeah. So today we're gonna be asking a

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<v Speaker 1>question that I personally have had a lot of curiosity

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<v Speaker 1>about over the years. I've always wondered about this question,

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<v Speaker 1>and even more so now recently I've been rewatching all

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<v Speaker 1>the Star Wars movies and so this is a question

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<v Speaker 1>that's really present in my mind that I've been asking

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<v Speaker 1>myself recently, And why is that? Are you imagining how

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<v Speaker 1>you're going to navigate to your in law's house on

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<v Speaker 1>the Jovian moons from your vacation place in Saturn or

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<v Speaker 1>what inspires you to think about this? Well, my wife

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<v Speaker 1>and I are immigrants, but we're not that that kind

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<v Speaker 1>of alien. But no, I just kind of wondered, you know, Um,

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<v Speaker 1>in Star Wars they always get lost or they pop

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<v Speaker 1>up in all kinds of places, and so how do

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<v Speaker 1>you know where you are? And how do you know

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<v Speaker 1>where to go? Or you know, they talk about like

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<v Speaker 1>a map of the galaxy, what does that even look like?

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<v Speaker 1>Or how would that even be useful? Yeah, it's it's

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<v Speaker 1>very rare that they're like, make a wrong turn. They're like,

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<v Speaker 1>we're we supposed to turn left at that pulsar or right.

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<v Speaker 1>I don't even really remember. It feels like that's all

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<v Speaker 1>just sort of been integrated into the electron next they

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<v Speaker 1>have in front of them. But those are hard problems, right,

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<v Speaker 1>it's not necessarily trivial to figure out. Yeah, and if

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<v Speaker 1>you think about it, in popular culture, there's only been

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<v Speaker 1>like one TV show about getting lost in space. You mean,

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<v Speaker 1>it was called space and you know at least you

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<v Speaker 1>know what it's about. Yeah, So today on the program,

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<v Speaker 1>we'll be asking the question, how do you navigate in

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<v Speaker 1>space space, and this is a problem that's relevant to

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<v Speaker 1>future navigation. Like imagine you are flying a spaceship with

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<v Speaker 1>lots of people on board and trying to get everybody

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<v Speaker 1>safely to Alpha Centauri. And it's also a question today

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<v Speaker 1>as NASA and the E s A launched satellites to

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<v Speaker 1>explore our Solar system. How do they make sure they

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<v Speaker 1>get to the right spot? How do they course correct

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<v Speaker 1>if they are off? Who does those calculations? Is that

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<v Speaker 1>on board the satellite or back here on Earth? Are

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<v Speaker 1>there people with protractors and pencils scribbling things furiously? How

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<v Speaker 1>does that actually work? Yeah, because you know, space is

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<v Speaker 1>pretty big, and it's three dementi all, you know, at

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<v Speaker 1>least three dimensions at least, yeah that we know of

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<v Speaker 1>that we think about right now. But it's a multi

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<v Speaker 1>dimensional and you're out there and you know, there's no

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<v Speaker 1>mountain to reference, no street signs. How do you get around?

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<v Speaker 1>How do you know where to go? Do you think

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<v Speaker 1>that third dimension is going to lead to like a

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<v Speaker 1>lot more marital arguments in the future, Like I told

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<v Speaker 1>you to turn up at that move man, why did

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<v Speaker 1>you turn down? This is just like so many more

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<v Speaker 1>ways to call new dimension to divorces. Probably no, but

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<v Speaker 1>it is really hard and it's also vital because you're

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<v Speaker 1>so much further away from your resources. Like these spaceships

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<v Speaker 1>they leave Earth, they're never getting a refill, like they

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<v Speaker 1>run out of gas because they got lost. They're just lost.

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<v Speaker 1>So you have like a very limited window to make

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<v Speaker 1>the moves you need to make to enter that orbit

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<v Speaker 1>or to fly by the moon. There's no reduce, like

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<v Speaker 1>you have a one tank and that's it. So it's

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<v Speaker 1>absolutely critical that you don't get lost and that you

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<v Speaker 1>figure out how to get where you need to go. Yeah, So,

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<v Speaker 1>as usually, we were wondering how many people out there

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<v Speaker 1>have thought about this question or even have an idea

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<v Speaker 1>about how to navigate in space. So as usual, Daniel

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<v Speaker 1>went out there and ask the internet to try to

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<v Speaker 1>answer this question, how do you navigate in space? That's right,

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<v Speaker 1>and if you'd like to participate in our virtual person

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<v Speaker 1>on the street interviews, just shoot us an email two

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<v Speaker 1>questions at Daniel and Jorge dot com. We would love

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<v Speaker 1>to put your uninformed speculation on the podcast. And so

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<v Speaker 1>think about it for a second. If you were out

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<v Speaker 1>in space in the middle of the galaxy or in

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<v Speaker 1>between galaxies? How would you know which way to make

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<v Speaker 1>your way home? Here's what people had to say. Because

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<v Speaker 1>gravity distill space and time and everything. Maybe you'd have

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<v Speaker 1>to go. Maybe you'd have to shoot a little bit

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<v Speaker 1>off it because as you as you go close to

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<v Speaker 1>and an object, you'd kind of be taken into its

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<v Speaker 1>gravitational swing. Other than that, I don't know how do

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<v Speaker 1>you navigate through deep space to just keep a set

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<v Speaker 1>of stars to your left and hopefully you're going the

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<v Speaker 1>same direct action. I have no idea. Maybe like by

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<v Speaker 1>distracting energy from the Sun, or if we're very patient,

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<v Speaker 1>maybe with solar sales, we could navigate deep space, maybe

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<v Speaker 1>through a pulse of a star, or like I don't know,

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<v Speaker 1>pole stars or something. I think the only way you

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<v Speaker 1>can navigating these spaces the way we do it now

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<v Speaker 1>by using stars and galaxies, things that are consistent, not

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<v Speaker 1>necessarily constellations, because that could you know, in three D

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<v Speaker 1>space they have depth and they have angles that they

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<v Speaker 1>are relative each other. You know, constellations do. But if

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<v Speaker 1>you use stuff like pulsars and quasars and you know

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<v Speaker 1>the Andromeda gag, see those things, we can coordinate ourselves

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<v Speaker 1>using a couple of those angles, we can coordinate ourselves

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<v Speaker 1>in deep space. I think navere taking in a deep

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<v Speaker 1>space or americum woulds to need the bicycles of navigation.

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<v Speaker 1>You're do either use inertial navigation, sitting time, speed, and

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<v Speaker 1>directions from someone In a short stuff you will have

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<v Speaker 1>to pick something like the sun and navigating reference to

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<v Speaker 1>the sun. Let's see, if you're heading to a prime centuri,

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<v Speaker 1>we should at least have an inbuilt special I had

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<v Speaker 1>invisible telescopes, I mean lens and meadows and special lists

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<v Speaker 1>and optimal path correction systems and some kind of special clocks.

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<v Speaker 1>Navigating in deep space, I would have to assume is

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<v Speaker 1>much like seiling the ocean. You look at the stars

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<v Speaker 1>and see whe're at relative to the stars. After your

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<v Speaker 1>statement that space is expanding faster than um the speed

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<v Speaker 1>of light, or faster than light can travel through it,

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<v Speaker 1>I really have no idea. Now I think you could

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<v Speaker 1>go anywhere you you go. Yeah, well, hopefully you can

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<v Speaker 1>do that, but how you do it? My idea would

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<v Speaker 1>be to mount a big giant telescope on the top

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<v Speaker 1>of your spacecraft, on the front and the back, so

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<v Speaker 1>you can see where you're going and where you're where

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<v Speaker 1>you came from. Maybe a telescope as big as hubble,

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<v Speaker 1>because your spacecraft is going to have to be that big.

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<v Speaker 1>After we leave the planet and learn about the like

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<v Speaker 1>further stars that we don't see on Earth, we can

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<v Speaker 1>pick three stars, and by keeping track of the distance

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<v Speaker 1>between us and the stars, we can know our position.

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<v Speaker 1>And when the stars are too far away, we can

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<v Speaker 1>always peak three new stars that we found out about

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<v Speaker 1>along the way in our journey. So there are a

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<v Speaker 1>lot of ideas there. What do you think of that?

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<v Speaker 1>Pretty good? Pretty good? I feel like people were sort

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<v Speaker 1>of thinking about triangulation and using the stars somehow to

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<v Speaker 1>tell where you are. I feel like that's a pretty

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<v Speaker 1>common idea in science fiction movies and boots. It's like, oh,

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<v Speaker 1>you just look at the stars around you, and do

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<v Speaker 1>you know where you are and you know where to go?

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<v Speaker 1>Or like if you look at the stars and you

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<v Speaker 1>don't recognize things, then you're kind of in trouble. I

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<v Speaker 1>like the I said, let's put a huge telescope on

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<v Speaker 1>the front and on the back of your spaceship, because

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<v Speaker 1>I want that anyway, Like, if I'm flying through space,

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<v Speaker 1>I want a big telescope because I want to see

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<v Speaker 1>with what stuffed around me. You know, I want to

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<v Speaker 1>do some sight seeing when I'm out there. But what

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<v Speaker 1>do you need one in the bag though, just to

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<v Speaker 1>see the fit is of people that you leave behind. Well,

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<v Speaker 1>because I mean, I guess you could turn your telescope.

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<v Speaker 1>Maybe you're saying you'll need one telescope plus like a

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<v Speaker 1>mount or something, but hey, more telescopes are better. Well,

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<v Speaker 1>I feel like that is a sort of a common thing,

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<v Speaker 1>is to look at the stars around you, and somehow

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<v Speaker 1>you use that to orient yourself, you know, kind of

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<v Speaker 1>like we use the North Star for a long time

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<v Speaker 1>to kind of tell which way was north when you're

0:11:37.440 --> 0:11:39.559
<v Speaker 1>out in the middle of the ocean. Is that kind

0:11:39.600 --> 0:11:41.600
<v Speaker 1>of an idea that we can use at all? It

0:11:41.720 --> 0:11:43.280
<v Speaker 1>is an idea that we can use. And the rest

0:11:43.320 --> 0:11:45.480
<v Speaker 1>on this notion that if you have an accurate map

0:11:45.600 --> 0:11:48.040
<v Speaker 1>of the stars, you can compare that to what you're

0:11:48.080 --> 0:11:51.880
<v Speaker 1>seeing and look for landmarks and try to measure angles

0:11:51.920 --> 0:11:54.040
<v Speaker 1>between the stars to give you a sense for where

0:11:54.080 --> 0:11:57.600
<v Speaker 1>you are. For example, if two stars are almost lined

0:11:57.679 --> 0:11:59.920
<v Speaker 1>up in your vision, then that tells you that you're

0:12:00.040 --> 0:12:03.200
<v Speaker 1>along a line drawn between those two stars. And if

0:12:03.240 --> 0:12:07.240
<v Speaker 1>you can find other examples measuring angles between stars, you

0:12:07.240 --> 0:12:09.240
<v Speaker 1>can give you sort of a point in three D

0:12:09.400 --> 0:12:11.880
<v Speaker 1>space for where you are at that moment. Well, I

0:12:12.080 --> 0:12:14.080
<v Speaker 1>guess the problem that I have always should have thought

0:12:14.120 --> 0:12:15.920
<v Speaker 1>about is like, what if you find yourself on the

0:12:15.960 --> 0:12:18.439
<v Speaker 1>other side of the galaxy, how would you even recognize

0:12:18.520 --> 0:12:20.640
<v Speaker 1>any of the stars because the stars are gonna look

0:12:20.679 --> 0:12:23.480
<v Speaker 1>totally different from the other side of the galaxy. Yeah,

0:12:23.480 --> 0:12:25.880
<v Speaker 1>if you just look at like teleported to a random

0:12:25.920 --> 0:12:28.760
<v Speaker 1>place in the universe where you have no reference points,

0:12:28.960 --> 0:12:31.840
<v Speaker 1>there's literally no way to know where you are because

0:12:31.960 --> 0:12:35.200
<v Speaker 1>there's no absolute reference there's no like point in space

0:12:35.240 --> 0:12:38.560
<v Speaker 1>that's defined in zero and you can measure your location

0:12:38.640 --> 0:12:41.560
<v Speaker 1>relative to that. If you get teleported to an arbitrary

0:12:41.600 --> 0:12:44.880
<v Speaker 1>point in space, special relativity says it's impossible to know

0:12:44.920 --> 0:12:48.080
<v Speaker 1>where you are. You can only measure your distance relative

0:12:48.120 --> 0:12:50.280
<v Speaker 1>to other stuff. So if you have no familiar references,

0:12:50.520 --> 0:12:53.760
<v Speaker 1>you're totally screwed. Wow, and things are like changing in time. Also,

0:12:53.920 --> 0:12:56.720
<v Speaker 1>everything's moving, so you're sort of totally lost in You're

0:12:56.760 --> 0:12:59.280
<v Speaker 1>totally lost. You have. The only way to orient yourself

0:12:59.320 --> 0:13:02.440
<v Speaker 1>in space is relative to known things. So if you

0:13:02.480 --> 0:13:05.640
<v Speaker 1>get teleported to some part of space that's totally unfamiliar.

0:13:06.040 --> 0:13:08.800
<v Speaker 1>Then you literally have no way to find your way

0:13:08.800 --> 0:13:12.400
<v Speaker 1>back except for randomly exploring until you do find a landmark.

0:13:12.760 --> 0:13:14.079
<v Speaker 1>And when I try that the next time I get

0:13:14.120 --> 0:13:17.960
<v Speaker 1>lost and my spouse is complaining, I'm like, it's special relativity.

0:13:18.160 --> 0:13:20.680
<v Speaker 1>It's it's law of the universe. It's not my fault.

0:13:20.840 --> 0:13:24.079
<v Speaker 1>Daniel said, this should work. Don't you feel like smartphones

0:13:24.160 --> 0:13:27.720
<v Speaker 1>must have solved this marital complaint? Right, houses don't have

0:13:27.720 --> 0:13:29.720
<v Speaker 1>to argue about how to navigating anymore, and they just

0:13:29.840 --> 0:13:32.600
<v Speaker 1>listened to the phone. That's right. The phone has saved

0:13:32.600 --> 0:13:35.680
<v Speaker 1>a lot of marriages. Probably maybe, or maybe people are like, no,

0:13:35.800 --> 0:13:38.439
<v Speaker 1>listen to my phone. Well, my phone says it's faster

0:13:38.520 --> 0:13:43.400
<v Speaker 1>take the expressway using Google Maps. No way, we aren't

0:13:43.480 --> 0:13:46.760
<v Speaker 1>using ways. People who argue are going to argue anyway.

0:13:46.880 --> 0:13:50.080
<v Speaker 1>I guess, So I guess the phones can't fix that. Yeah,

0:13:50.120 --> 0:13:53.920
<v Speaker 1>And you know, navigators in throughout history have used the stars.

0:13:53.960 --> 0:13:56.360
<v Speaker 1>Like if you have sailed the oceans, then to figure

0:13:56.360 --> 0:13:59.120
<v Speaker 1>out where you are in this vast sea where you

0:13:59.160 --> 0:14:01.480
<v Speaker 1>can see no land marks is just to look up

0:14:01.600 --> 0:14:04.440
<v Speaker 1>and look for star marks. Right, to look for the

0:14:04.440 --> 0:14:06.520
<v Speaker 1>positions of stars in the sky that gives you a

0:14:06.520 --> 0:14:08.640
<v Speaker 1>sense for where you might be. All right, well, let's

0:14:08.640 --> 0:14:11.120
<v Speaker 1>get into the sort of the nitty gritty of this problem.

0:14:11.280 --> 0:14:13.000
<v Speaker 1>And because I know you, you've told me that there

0:14:13.040 --> 0:14:16.200
<v Speaker 1>are sort of several ways in which we can right

0:14:16.200 --> 0:14:18.480
<v Speaker 1>now sort of calculate where we are in space, you know,

0:14:18.559 --> 0:14:22.440
<v Speaker 1>barring kind of like a complete map of the entire galaxy. Um,

0:14:22.440 --> 0:14:24.320
<v Speaker 1>so step us through. What's the what's the sort of

0:14:24.360 --> 0:14:26.760
<v Speaker 1>the basic way that we get around in space. So

0:14:26.800 --> 0:14:29.200
<v Speaker 1>the simplest way, in the dumbest way, and the worst

0:14:29.280 --> 0:14:33.080
<v Speaker 1>way is basically dead reckoning. And that says you know

0:14:33.160 --> 0:14:36.000
<v Speaker 1>where you started, and you started on Earth, and if

0:14:36.000 --> 0:14:38.320
<v Speaker 1>you have a record of all the moves you took,

0:14:38.520 --> 0:14:41.080
<v Speaker 1>you went in this direction at this velocity, you should

0:14:41.080 --> 0:14:43.680
<v Speaker 1>be able to calculate where you went. Because you know,

0:14:43.800 --> 0:14:46.840
<v Speaker 1>spacecraft follow the laws of physics, and we know what

0:14:46.920 --> 0:14:49.400
<v Speaker 1>those laws are. We have a whole model of the

0:14:49.440 --> 0:14:52.360
<v Speaker 1>Solar System, so we should be able to predict if

0:14:52.400 --> 0:14:55.120
<v Speaker 1>you leave in this direction at this time, and you

0:14:55.200 --> 0:14:57.640
<v Speaker 1>fire your rockets here and there, we should be able

0:14:57.640 --> 0:14:59.880
<v Speaker 1>to predict where you end up. That's kind of like

0:15:00.040 --> 0:15:03.320
<v Speaker 1>closing your eyes and like knowing where you are right now,

0:15:03.360 --> 0:15:05.880
<v Speaker 1>closing your eyes and just by like counting your steps

0:15:06.280 --> 0:15:08.680
<v Speaker 1>and how you think you turn, sort of like making

0:15:08.720 --> 0:15:10.360
<v Speaker 1>it to your fridge or something like that. It's like

0:15:10.360 --> 0:15:13.200
<v Speaker 1>following one of those treasure maps, like fifteen paces forward

0:15:13.440 --> 0:15:17.080
<v Speaker 1>then turn left step four paces, then dig right right.

0:15:17.360 --> 0:15:19.640
<v Speaker 1>And that's a little terrifying. Like if you remember the

0:15:19.720 --> 0:15:22.960
<v Speaker 1>days before smartphones where people had to like actually write

0:15:22.960 --> 0:15:26.080
<v Speaker 1>down directions and there were things like drive for fifteen

0:15:26.080 --> 0:15:28.600
<v Speaker 1>miles then take a left right, and you had no

0:15:28.680 --> 0:15:32.360
<v Speaker 1>idea is this the correct left or not? You know, yeah, yeah,

0:15:32.400 --> 0:15:33.640
<v Speaker 1>and we all know how well that works. In the

0:15:33.680 --> 0:15:34.760
<v Speaker 1>middle of the night when you have to go to

0:15:34.800 --> 0:15:39.320
<v Speaker 1>the bathroom in total darkness, you know, you better put

0:15:39.320 --> 0:15:41.080
<v Speaker 1>your hands in front of you, just in cakes. Yeah,

0:15:41.120 --> 0:15:44.120
<v Speaker 1>and so sailors used to call this dead reckoning, and

0:15:44.200 --> 0:15:47.040
<v Speaker 1>you know it's not terrible, like it works. Okay, we

0:15:47.120 --> 0:15:49.640
<v Speaker 1>have a pretty good model of the solar system, and

0:15:49.920 --> 0:15:52.000
<v Speaker 1>we have rockets, and we can even measure we don't

0:15:52.040 --> 0:15:54.440
<v Speaker 1>even have to just guess. And like the effect of thrust,

0:15:54.480 --> 0:15:59.080
<v Speaker 1>you can measure how much you've accelerated using accelerometers, you

0:15:59.120 --> 0:16:01.440
<v Speaker 1>can measure your the direction that you ended up in

0:16:01.560 --> 0:16:05.280
<v Speaker 1>using gyroscopes, So we've tried to be really careful about this,

0:16:05.320 --> 0:16:08.280
<v Speaker 1>and some spacecraft in the history of you know, American

0:16:08.360 --> 0:16:11.920
<v Speaker 1>exploration have used dead reckoning. But I guess it's tricky too,

0:16:11.960 --> 0:16:15.240
<v Speaker 1>because you know, in space you can't count your steps,

0:16:15.280 --> 0:16:17.280
<v Speaker 1>like there's nothing to hold onto to tell you how

0:16:17.320 --> 0:16:20.000
<v Speaker 1>far you move. You have to you have to measure

0:16:20.040 --> 0:16:24.240
<v Speaker 1>your exploration and then integrate DAD to convert to velocity,

0:16:24.280 --> 0:16:26.880
<v Speaker 1>and then integrate DAT to convert it to distance. So

0:16:26.960 --> 0:16:29.680
<v Speaker 1>it's like a lot of room there to get error. Yes,

0:16:29.680 --> 0:16:33.000
<v Speaker 1>and you mentioned a very critical step there, which is integration,

0:16:33.080 --> 0:16:36.280
<v Speaker 1>and that requires knowing the time. You can't count your steps.

0:16:36.440 --> 0:16:39.360
<v Speaker 1>What you need is a very accurate clock. And the

0:16:39.400 --> 0:16:42.080
<v Speaker 1>more accurate your clock, the more you accurately you can

0:16:42.080 --> 0:16:45.240
<v Speaker 1>calculate how far you've gone. Right, you said I shot

0:16:45.240 --> 0:16:47.280
<v Speaker 1>off in this direction of the speed, Well did you

0:16:47.280 --> 0:16:50.240
<v Speaker 1>go for two point seven seconds or two point eight seconds?

0:16:50.400 --> 0:16:53.600
<v Speaker 1>When you're traveling at ten thousand kilometers per second, that

0:16:53.680 --> 0:16:57.640
<v Speaker 1>makes a big difference. Yeah, And when distances are so huge, right,

0:16:57.920 --> 0:17:00.480
<v Speaker 1>and the stakes are so high, like you can't if

0:17:00.480 --> 0:17:02.600
<v Speaker 1>you miss Jupiter by a few miles, it could be

0:17:02.640 --> 0:17:05.520
<v Speaker 1>bad us. Yeah, as you're gonna do a Jupiter drive by, right,

0:17:05.840 --> 0:17:08.480
<v Speaker 1>then you only get one shot at it, literally, and

0:17:08.560 --> 0:17:11.000
<v Speaker 1>so it's pretty tricky. And the problem here is that

0:17:11.200 --> 0:17:13.840
<v Speaker 1>errors build up, Like you make a little mistake because

0:17:13.880 --> 0:17:16.520
<v Speaker 1>you turned a little too far, then you're off, and

0:17:16.520 --> 0:17:18.560
<v Speaker 1>the next time you can't correct it, and so the

0:17:18.680 --> 0:17:21.199
<v Speaker 1>errors just build up in the integrate and eventually you

0:17:21.200 --> 0:17:23.520
<v Speaker 1>can be pretty far from where you thought you right.

0:17:23.600 --> 0:17:27.119
<v Speaker 1>It literally is like walking around with your eyes closed. Yeah, exactly.

0:17:27.280 --> 0:17:30.640
<v Speaker 1>So that's the most basic strategy, and you can make

0:17:30.680 --> 0:17:33.640
<v Speaker 1>that more sophisticated by doing corrections. You can say, well,

0:17:33.840 --> 0:17:37.040
<v Speaker 1>I'm gonna use dead reckoning. Plus I'm going to look

0:17:37.040 --> 0:17:39.000
<v Speaker 1>at the stars and I'm gonna try to figure out

0:17:39.160 --> 0:17:41.359
<v Speaker 1>if I'm off. And this is what like a lot

0:17:41.400 --> 0:17:44.400
<v Speaker 1>of astronauts did, like Apollo eleven and follow their team.

0:17:44.560 --> 0:17:48.080
<v Speaker 1>They flew to the Moon by dead reckoning, but occasionally

0:17:48.119 --> 0:17:50.000
<v Speaker 1>they would check in and they would look at the

0:17:50.040 --> 0:17:52.560
<v Speaker 1>stars and try to get a more precise measurement for

0:17:52.600 --> 0:17:54.400
<v Speaker 1>where they were, and they would use that to correct

0:17:54.600 --> 0:17:57.720
<v Speaker 1>their flight path. Really, so I guess two questions. One

0:17:57.840 --> 0:18:00.480
<v Speaker 1>is why didn't they just use the moon as reference

0:18:00.800 --> 0:18:03.480
<v Speaker 1>because they were flying towards it, and they could tell

0:18:03.480 --> 0:18:06.399
<v Speaker 1>her they were going away from it or towards it.

0:18:06.560 --> 0:18:08.159
<v Speaker 1>And the size of it too, wouldn't it tell you

0:18:08.160 --> 0:18:10.399
<v Speaker 1>said of the distance? But and then my second question was,

0:18:11.000 --> 0:18:13.280
<v Speaker 1>you know, can you actually use the stars to tell

0:18:13.280 --> 0:18:16.280
<v Speaker 1>where you are? You can? So, yes, they were pointed

0:18:16.280 --> 0:18:18.320
<v Speaker 1>at the moon. But that's pretty rough, right, And what

0:18:18.359 --> 0:18:20.240
<v Speaker 1>you want to do was get to the Moon and

0:18:20.240 --> 0:18:22.879
<v Speaker 1>then enter into orbit around the Moon. And that was

0:18:22.880 --> 0:18:26.400
<v Speaker 1>a very precise maneuver. And just like with the spacecraft,

0:18:26.440 --> 0:18:28.400
<v Speaker 1>they had a limited amount of fuel, so if they

0:18:28.440 --> 0:18:30.480
<v Speaker 1>burnt their fuel the wrong time, they might not be

0:18:30.520 --> 0:18:32.680
<v Speaker 1>able to make it home. I said. The fuel is

0:18:32.760 --> 0:18:34.880
<v Speaker 1>very expensive to lift off the surface of the Earth,

0:18:34.960 --> 0:18:37.600
<v Speaker 1>and so everything was a very tight budget, so they

0:18:37.600 --> 0:18:41.240
<v Speaker 1>had to be really precise. There are no exactly you

0:18:41.280 --> 0:18:43.639
<v Speaker 1>can't just pull a eui in space. That costs a

0:18:43.680 --> 0:18:45.879
<v Speaker 1>lot of energy to pull ui. Like you missed the

0:18:45.920 --> 0:18:48.320
<v Speaker 1>snack shop. You missed the snack shop, man, you are

0:18:48.359 --> 0:18:51.280
<v Speaker 1>not going back. And yes, they did stellar navigation. They

0:18:51.359 --> 0:18:54.520
<v Speaker 1>looked by I to find stars, and they measured the

0:18:54.560 --> 0:18:58.920
<v Speaker 1>declination using gyroscopes and they use that to correct their calculations.

0:18:58.960 --> 0:19:01.240
<v Speaker 1>A huge fraction of the time they actually spent in

0:19:01.280 --> 0:19:05.359
<v Speaker 1>that module was typing data into that computer. You know,

0:19:05.480 --> 0:19:08.320
<v Speaker 1>it's a complicated system. And remember the whole program was

0:19:08.400 --> 0:19:11.320
<v Speaker 1>loaded into the computer before it launched, Like you didn't

0:19:11.359 --> 0:19:13.800
<v Speaker 1>have guys up there, like you know, tip tapping editing

0:19:13.800 --> 0:19:16.119
<v Speaker 1>the program being like I think we must change the

0:19:16.160 --> 0:19:18.639
<v Speaker 1>flight path or something. They had it all built in

0:19:18.840 --> 0:19:22.000
<v Speaker 1>with the opportunity for small corrections based on looking at

0:19:22.000 --> 0:19:24.640
<v Speaker 1>those stars. So what do you mean declination like where

0:19:24.680 --> 0:19:27.520
<v Speaker 1>the constellation was relative to the Earth or something like that. No,

0:19:27.680 --> 0:19:30.240
<v Speaker 1>relative to them, Right, they had an idea for where

0:19:30.240 --> 0:19:32.159
<v Speaker 1>they were, and they had an idea for if we

0:19:32.240 --> 0:19:35.440
<v Speaker 1>are here, the stars should appear at this angle relative

0:19:35.480 --> 0:19:38.200
<v Speaker 1>to the spaceship, and then they would measure where is

0:19:38.240 --> 0:19:41.240
<v Speaker 1>the star relative to where the spaceship is pointing because

0:19:41.240 --> 0:19:45.120
<v Speaker 1>I had careful gyroscopes and and those angles helped them

0:19:45.119 --> 0:19:48.320
<v Speaker 1>figure out exactly where they are. All right, Well that

0:19:48.359 --> 0:19:50.720
<v Speaker 1>sounds like, um it worked because they got to the

0:19:51.840 --> 0:19:55.359
<v Speaker 1>a few times, So I can't argue with that. All right, Well,

0:19:55.440 --> 0:19:57.320
<v Speaker 1>let's get into some of the other ways that we

0:19:57.400 --> 0:20:01.160
<v Speaker 1>can navigate in space and whether or not they could

0:20:01.160 --> 0:20:05.120
<v Speaker 1>help us explore the furthest switches of the Cosmos but first,

0:20:05.160 --> 0:20:19.879
<v Speaker 1>let's take a quick break, all right, Dina. We're talking

0:20:19.920 --> 0:20:24.520
<v Speaker 1>about navigating in space. Space, space, space, And I just

0:20:24.520 --> 0:20:27.200
<v Speaker 1>wonder why there's always an echo when people talk about space,

0:20:27.240 --> 0:20:30.760
<v Speaker 1>because there's no echoes in space. It's because it's cool, man,

0:20:31.240 --> 0:20:35.359
<v Speaker 1>It's so cool cool. It makes it sound mysterious. It

0:20:35.400 --> 0:20:38.640
<v Speaker 1>gives you a sense of literally space, right, echoes give

0:20:38.680 --> 0:20:40.960
<v Speaker 1>you a sense a big emptiness. But you know that's

0:20:40.960 --> 0:20:45.280
<v Speaker 1>just the um audio version of the artistic impression, which

0:20:45.359 --> 0:20:46.680
<v Speaker 1>you know, I'm not a fan. You not a fan

0:20:46.720 --> 0:20:50.040
<v Speaker 1>of the echoes in space. No, I'm a fan of

0:20:50.080 --> 0:20:52.720
<v Speaker 1>realistic science fiction. It should give us a cent or

0:20:52.800 --> 0:20:55.280
<v Speaker 1>what it's actually like to be out there. Though maybe

0:20:55.320 --> 0:20:57.240
<v Speaker 1>you know, if you're in a kind of little metal box,

0:20:57.280 --> 0:20:59.800
<v Speaker 1>maybe there are actually a lot of echoes, but inside

0:21:00.040 --> 0:21:03.280
<v Speaker 1>I see. Well, we're talking about how to navigating space,

0:21:03.359 --> 0:21:05.879
<v Speaker 1>which is a big question, you know. I feel like,

0:21:06.280 --> 0:21:08.080
<v Speaker 1>you know, whenever you watch a movie like Star Wars,

0:21:08.119 --> 0:21:09.679
<v Speaker 1>it's like how are they getting around? How do they

0:21:09.680 --> 0:21:11.320
<v Speaker 1>know where to go? And so we talked about it

0:21:11.440 --> 0:21:13.199
<v Speaker 1>one way, which is dead reckoning, Like if you know

0:21:13.240 --> 0:21:15.360
<v Speaker 1>you're an Earth and you leave Earth, you can sort

0:21:15.359 --> 0:21:17.600
<v Speaker 1>of track your progress, but then you also have to

0:21:17.680 --> 0:21:19.719
<v Speaker 1>kind of correct your errors as you go. That's right,

0:21:19.760 --> 0:21:22.320
<v Speaker 1>and a better way to do that is not just

0:21:22.440 --> 0:21:24.960
<v Speaker 1>be based on your initial calculation from Earth, but it

0:21:25.000 --> 0:21:29.080
<v Speaker 1>takes inspiration from how your smartphone gets you to your

0:21:29.080 --> 0:21:32.840
<v Speaker 1>friend's house, which is that it gets messages from satellites.

0:21:33.240 --> 0:21:35.919
<v Speaker 1>Here on Earth, we have the GPS system, which is

0:21:36.200 --> 0:21:40.159
<v Speaker 1>constantly broadcasting messages. That's giving your phone an idea for

0:21:40.240 --> 0:21:43.240
<v Speaker 1>where it is, and your phone figures out where it

0:21:43.320 --> 0:21:45.760
<v Speaker 1>is by hearing these messages and knowing how long it

0:21:45.800 --> 0:21:48.560
<v Speaker 1>took the message to get here from the satellite, and

0:21:48.760 --> 0:21:51.080
<v Speaker 1>it uses that to figure out where the phone is

0:21:51.240 --> 0:21:53.520
<v Speaker 1>right and it also uses like a map, like your

0:21:53.560 --> 0:21:56.000
<v Speaker 1>phone knows where all the satellites should be at any time,

0:21:56.200 --> 0:21:57.960
<v Speaker 1>so once it gets a signal, it sort of knows

0:21:58.000 --> 0:22:01.200
<v Speaker 1>where it is, yeah, precisely in knows where the satellites are.

0:22:01.560 --> 0:22:03.359
<v Speaker 1>And then it gets these messages. And the messages have

0:22:03.359 --> 0:22:05.440
<v Speaker 1>a little time stamp on them. They say I sent

0:22:05.600 --> 0:22:08.320
<v Speaker 1>this message at exactly this time, and if you get

0:22:08.359 --> 0:22:11.840
<v Speaker 1>this message, you know, seventeen milliseconds later, then you know

0:22:11.960 --> 0:22:15.280
<v Speaker 1>how far the message flew because you knew it flew

0:22:15.359 --> 0:22:17.240
<v Speaker 1>at the speed of light. And you get enough of

0:22:17.280 --> 0:22:19.320
<v Speaker 1>these things and you can figure out where you are.

0:22:19.720 --> 0:22:23.040
<v Speaker 1>And there's an analogous system. There's GPS for deep space.

0:22:23.080 --> 0:22:26.800
<v Speaker 1>There is there's a space GPS. Yeah, there's a space GPS,

0:22:26.880 --> 0:22:30.120
<v Speaker 1>and it's called the Deep Space Network and NASA runs

0:22:30.160 --> 0:22:33.359
<v Speaker 1>it and it basically sends messages out in deep space

0:22:33.400 --> 0:22:37.000
<v Speaker 1>from three locations on the Earth, and satellites get those messages,

0:22:37.400 --> 0:22:39.560
<v Speaker 1>send them back and then we can use that to

0:22:39.600 --> 0:22:42.840
<v Speaker 1>figure out where the satellite is. It's like a reverse

0:22:43.160 --> 0:22:45.520
<v Speaker 1>Why are you seriously, it's like a reverse GPS. It's

0:22:45.520 --> 0:22:48.680
<v Speaker 1>like a reverse GPS. Yeah. What happens is you send

0:22:48.680 --> 0:22:51.359
<v Speaker 1>a message to a satellite and then it comes back

0:22:51.400 --> 0:22:53.679
<v Speaker 1>and you count, well, how long did it take for

0:22:53.720 --> 0:22:56.639
<v Speaker 1>the message to go there and come back, And that

0:22:56.720 --> 0:22:59.159
<v Speaker 1>gives you a sense for the distance. And then when

0:22:59.200 --> 0:23:02.119
<v Speaker 1>the message comes it's a little bit Doppler shifted based

0:23:02.119 --> 0:23:04.840
<v Speaker 1>on the speed of the satellite, and that tells you

0:23:05.000 --> 0:23:08.040
<v Speaker 1>how fast this satellite is moving away from you. So

0:23:08.080 --> 0:23:10.359
<v Speaker 1>it gives you a measure of the current position and

0:23:10.600 --> 0:23:13.800
<v Speaker 1>the velocity of the satellite. But I guess that only

0:23:13.840 --> 0:23:16.480
<v Speaker 1>works for satellites, right, like it doesn't work if from

0:23:16.520 --> 0:23:19.000
<v Speaker 1>in Jupiter or does it. Well, it works for anybody

0:23:19.040 --> 0:23:22.200
<v Speaker 1>that can receive these deep space messages and send them back.

0:23:22.960 --> 0:23:25.680
<v Speaker 1>So it doesn't give you your position relative to Jupiter. Note,

0:23:25.760 --> 0:23:29.359
<v Speaker 1>only gives you your position and velocity relative to Earth. Right,

0:23:29.560 --> 0:23:32.000
<v Speaker 1>But like if you know where Earth is, what this

0:23:32.080 --> 0:23:35.040
<v Speaker 1>signal help you know where you are in this solar system? No,

0:23:35.160 --> 0:23:37.640
<v Speaker 1>because you can't actually do the calculation yourself. And that's

0:23:37.640 --> 0:23:40.160
<v Speaker 1>one problem with this deep space network is that only

0:23:40.240 --> 0:23:43.080
<v Speaker 1>Earth gets to figure it out. Earth gets your message,

0:23:43.320 --> 0:23:46.000
<v Speaker 1>and then the second link gives Earth the information about

0:23:46.040 --> 0:23:48.280
<v Speaker 1>where you are, and then the folks on Earth have

0:23:48.320 --> 0:23:50.800
<v Speaker 1>to calculate Okay, turns out you were in this position

0:23:50.880 --> 0:23:53.000
<v Speaker 1>and send it to you. So it's kind of a

0:23:53.080 --> 0:23:55.000
<v Speaker 1>lot of back and forth. It's not that you can

0:23:55.000 --> 0:23:57.560
<v Speaker 1>just get this message from the deep space network and

0:23:57.560 --> 0:23:59.600
<v Speaker 1>figured it out yourself. The way your phone can from

0:24:00.160 --> 0:24:02.760
<v Speaker 1>s GPS is one directional, right, because it comes with

0:24:02.800 --> 0:24:05.960
<v Speaker 1>these time stamps. Right, So why why couldn't this work

0:24:06.000 --> 0:24:08.119
<v Speaker 1>the same way? The reason is the clock. The clock

0:24:08.160 --> 0:24:11.520
<v Speaker 1>on the satellite is not very good because really accurate

0:24:11.520 --> 0:24:14.160
<v Speaker 1>clocks are necessary to do these calculations. Is because it's

0:24:14.280 --> 0:24:17.040
<v Speaker 1>much more important to be super accurate more important than

0:24:17.080 --> 0:24:19.679
<v Speaker 1>your phone's GPS, and the clocks that are on the

0:24:19.680 --> 0:24:21.959
<v Speaker 1>satellites are not good enough to do this, so they

0:24:22.000 --> 0:24:24.360
<v Speaker 1>have to do the calculation back on Earth and then

0:24:24.480 --> 0:24:26.480
<v Speaker 1>send it to the satellite because on Earth to have

0:24:26.560 --> 0:24:30.760
<v Speaker 1>these super precise atomic clocks that keep everything in lockstep.

0:24:31.880 --> 0:24:36.600
<v Speaker 1>Interesting alright, So we we can't rely on the Earth

0:24:36.640 --> 0:24:38.520
<v Speaker 1>to tell us where we are, like if I'm out

0:24:38.520 --> 0:24:41.359
<v Speaker 1>in space, or can we can we rely on Earth

0:24:41.359 --> 0:24:43.440
<v Speaker 1>to tell me where I am. Earth can figure out

0:24:43.480 --> 0:24:45.800
<v Speaker 1>where you are, how far you are from the Earth,

0:24:45.840 --> 0:24:48.440
<v Speaker 1>and how fast you're going, but you know, it's kind

0:24:48.480 --> 0:24:51.679
<v Speaker 1>of limited. Like they can get really precise measurements of

0:24:51.720 --> 0:24:54.600
<v Speaker 1>where you are up to about one meter, which is

0:24:54.640 --> 0:24:57.920
<v Speaker 1>really pretty amazing, like you're out you know Jupiter distance,

0:24:57.960 --> 0:25:00.119
<v Speaker 1>and Earth can measure how far away you are to

0:25:00.280 --> 0:25:03.600
<v Speaker 1>within one meter based on the balance of the echo,

0:25:03.760 --> 0:25:06.560
<v Speaker 1>like the signal coming back and going there and back. Yeah,

0:25:06.640 --> 0:25:10.320
<v Speaker 1>just timing the echo because they have really precise atomic clocks.

0:25:10.359 --> 0:25:12.280
<v Speaker 1>But what they can't do is figure out like where

0:25:12.280 --> 0:25:16.119
<v Speaker 1>you are laterally, like your angle because there they don't

0:25:16.119 --> 0:25:19.439
<v Speaker 1>have an echo measurement, right, and so they're the uncertainties

0:25:19.480 --> 0:25:23.439
<v Speaker 1>more like four kilometers for every a U the distance

0:25:23.480 --> 0:25:27.760
<v Speaker 1>between the Earth and the Sun. I see, because you know,

0:25:28.040 --> 0:25:30.240
<v Speaker 1>if we're out by Jupiter, we don't shine like a star,

0:25:30.800 --> 0:25:33.240
<v Speaker 1>that's right, right, Like we're not visible to the Earth,

0:25:33.560 --> 0:25:35.159
<v Speaker 1>So they have no idea where we are. They just

0:25:35.200 --> 0:25:36.600
<v Speaker 1>know kind of how far we are. They know how

0:25:36.600 --> 0:25:38.200
<v Speaker 1>far you are, and they figure out where you are

0:25:38.280 --> 0:25:41.840
<v Speaker 1>laterally basically using dead reckoning and then correcting using these

0:25:41.920 --> 0:25:45.360
<v Speaker 1>radio measurements. But you know, that's a pretty big uncertainty.

0:25:45.359 --> 0:25:47.400
<v Speaker 1>If you get out to like the distance of Pluto,

0:25:47.800 --> 0:25:51.960
<v Speaker 1>then they're uncertainties two hundred kilometers, which is really big

0:25:52.040 --> 0:25:55.840
<v Speaker 1>if you're trying to enter into the orbit of Pluto. Yeah. Yeah,

0:25:55.880 --> 0:25:59.399
<v Speaker 1>that sounds like a pretty big error. Viewer off by

0:25:59.400 --> 0:26:04.040
<v Speaker 1>two meters in your phone GPS, you be in a

0:26:04.080 --> 0:26:06.920
<v Speaker 1>whole different state. Yeah. And so practically, what these folks

0:26:06.960 --> 0:26:09.679
<v Speaker 1>do is they use landmarks in the Solar system too

0:26:09.720 --> 0:26:12.320
<v Speaker 1>correct So if you're getting near Jupiter, it sund I

0:26:12.359 --> 0:26:14.639
<v Speaker 1>can be like, okay, I see where Jupiter is. It

0:26:14.680 --> 0:26:17.239
<v Speaker 1>can compare it to where thought Jupiter should be, and

0:26:17.240 --> 0:26:19.160
<v Speaker 1>you can use that to correct. So you're like you're

0:26:19.160 --> 0:26:21.880
<v Speaker 1>getting landmarks. You're like, oh, you're driving your friend's house

0:26:22.080 --> 0:26:24.320
<v Speaker 1>is supposed to be a hill there. Hoops, I must

0:26:24.320 --> 0:26:27.040
<v Speaker 1>be in the wrong spot passing to McDonald. I know

0:26:27.160 --> 0:26:30.240
<v Speaker 1>I'm halfway there kind of thing. Yeah, And so cameras

0:26:30.280 --> 0:26:33.720
<v Speaker 1>on board can give accurate measurements of nearby objects, not

0:26:33.840 --> 0:26:36.680
<v Speaker 1>very far away, only very nearby. You see a big,

0:26:36.720 --> 0:26:39.640
<v Speaker 1>well known asteroid, you pass the Moon or a planet,

0:26:39.800 --> 0:26:41.960
<v Speaker 1>then you can correct You're no longer reliant on the

0:26:42.000 --> 0:26:45.359
<v Speaker 1>messages from earthly interesting, but the satellite does that calculation

0:26:45.480 --> 0:26:47.399
<v Speaker 1>or like it has to send the picture bag and

0:26:47.400 --> 0:26:49.720
<v Speaker 1>then here on Earth were like, oh, it just pass Jupiter.

0:26:49.880 --> 0:26:51.720
<v Speaker 1>This is where you are. Yeah, that's all done on

0:26:51.800 --> 0:26:54.160
<v Speaker 1>Earth currently sends the data back and then we can

0:26:54.160 --> 0:26:56.840
<v Speaker 1>get corrections. And that's one of the problems is that

0:26:56.960 --> 0:26:59.359
<v Speaker 1>a lot of this stuff relies on calculations done on

0:26:59.400 --> 0:27:02.439
<v Speaker 1>Earth and then these back and forth communications with the

0:27:02.480 --> 0:27:05.399
<v Speaker 1>deep space network, which tie up the deep space network.

0:27:05.400 --> 0:27:07.439
<v Speaker 1>You know, you're only talking to one satellite. All the

0:27:07.480 --> 0:27:10.159
<v Speaker 1>other ones are waiting, so you can only talk to like,

0:27:10.320 --> 0:27:12.280
<v Speaker 1>you know, a few of them at a time. And

0:27:12.640 --> 0:27:14.959
<v Speaker 1>that's pretty serious because like GPS doesn't work that way.

0:27:15.040 --> 0:27:18.040
<v Speaker 1>GPS just sends out its messages and all the phones

0:27:18.080 --> 0:27:20.159
<v Speaker 1>in the world just kind of listen. It doesn't have

0:27:20.200 --> 0:27:22.119
<v Speaker 1>to be bothered by the fact that I'm using it

0:27:22.119 --> 0:27:24.000
<v Speaker 1>and somebody else is using it at the same time.

0:27:24.440 --> 0:27:26.840
<v Speaker 1>But deep space network gets tied up every time a

0:27:26.920 --> 0:27:30.040
<v Speaker 1>satellite needs to figure out its position. So they have

0:27:30.320 --> 0:27:32.639
<v Speaker 1>a new idea for how to improve this so that

0:27:32.640 --> 0:27:35.680
<v Speaker 1>it can be more like GPS. Well, how does that work?

0:27:35.800 --> 0:27:38.280
<v Speaker 1>Just put more clocks in it, or yes, build a

0:27:38.359 --> 0:27:41.480
<v Speaker 1>really precise clock and put it on the satellite. The

0:27:41.560 --> 0:27:44.679
<v Speaker 1>most precise clocks we have are atomic clocks. These are

0:27:44.720 --> 0:27:48.760
<v Speaker 1>clocks that measure little atoms doing very precise wiggles that

0:27:48.920 --> 0:27:52.040
<v Speaker 1>like vibrated very specific frequency. One of the most precise

0:27:52.080 --> 0:27:54.760
<v Speaker 1>things in the universe because it just happens over and

0:27:54.880 --> 0:27:58.760
<v Speaker 1>over and over again exactly the same time step. But

0:27:58.840 --> 0:28:02.560
<v Speaker 1>these atomic clocks are expensive and they're big, and so

0:28:02.600 --> 0:28:05.560
<v Speaker 1>the reason that we don't have good clocks on satellites

0:28:05.640 --> 0:28:09.639
<v Speaker 1>is because nobody's ever miniaturized them. So NASA spent a

0:28:09.640 --> 0:28:12.760
<v Speaker 1>lot of time building a deep space atomic clock, basically

0:28:12.880 --> 0:28:16.000
<v Speaker 1>a miniaturized version of atomic clock you can put on

0:28:16.080 --> 0:28:18.880
<v Speaker 1>the satellite. And is it a lot smaller or yeah,

0:28:18.960 --> 0:28:21.439
<v Speaker 1>it's a lot smaller, and it's a lot cheaper, and

0:28:21.480 --> 0:28:23.760
<v Speaker 1>it's about the size of a toaster. Wow. So you

0:28:23.840 --> 0:28:27.480
<v Speaker 1>wouldn't want to wear this atomic clock. It's not it's

0:28:27.480 --> 0:28:31.040
<v Speaker 1>not ready for wristwatch use. If you want to be

0:28:31.119 --> 0:28:34.680
<v Speaker 1>super untime to meetings and podcast recordings, I could wear

0:28:34.720 --> 0:28:37.320
<v Speaker 1>an atomic clock, but it might be a little inconvenient. No,

0:28:37.400 --> 0:28:39.520
<v Speaker 1>And these atomic clocks cost you know, enough fifty to

0:28:39.600 --> 0:28:42.840
<v Speaker 1>a hundred thousand dollars, which amazingly is actually cheaper than

0:28:42.920 --> 0:28:46.440
<v Speaker 1>some wristwatches you can buy for wearing. I never understood that.

0:28:46.600 --> 0:28:50.360
<v Speaker 1>But some people spend a ridiculous amount the gold plated iPhones, right, Yeah, Well,

0:28:50.400 --> 0:28:52.600
<v Speaker 1>I spent a few years in Switzerland where they have

0:28:52.640 --> 0:28:55.320
<v Speaker 1>these ridiculous watch shops. You can go in and spend

0:28:55.320 --> 0:28:58.600
<v Speaker 1>two hundred thousand dollars on a fancy watch. But it's

0:28:58.640 --> 0:29:01.920
<v Speaker 1>like hand built with all these little levers and gears thereby,

0:29:02.240 --> 0:29:04.600
<v Speaker 1>you know, dwarves underground or something I don't know, And

0:29:04.720 --> 0:29:08.440
<v Speaker 1>it's not even as accurate as a toaster exactly exactly.

0:29:08.440 --> 0:29:10.760
<v Speaker 1>I'll take a toaster's eye atomic watch from my wrist

0:29:11.040 --> 0:29:14.640
<v Speaker 1>any day. But the idea there is if you have

0:29:14.800 --> 0:29:18.120
<v Speaker 1>this atomic clock on the satellite, then it can get

0:29:18.240 --> 0:29:20.880
<v Speaker 1>messages from the Deep Space Network that have time stamps

0:29:20.920 --> 0:29:23.920
<v Speaker 1>on them to say we sent this message at whatever time,

0:29:24.280 --> 0:29:27.120
<v Speaker 1>and you can just compare that too. It's atomic clock

0:29:27.440 --> 0:29:29.600
<v Speaker 1>and they say, oh, it took x seconds to get here.

0:29:29.880 --> 0:29:32.440
<v Speaker 1>I can figure out where I am myself. And that's

0:29:32.440 --> 0:29:36.120
<v Speaker 1>a big step forward in what they call autonomous satellite navigation,

0:29:36.160 --> 0:29:38.959
<v Speaker 1>with the satellites are just sort of driving themselves, right then,

0:29:39.000 --> 0:29:41.840
<v Speaker 1>it's more like the GPS we have on our phones. Yeah, exactly,

0:29:42.080 --> 0:29:44.240
<v Speaker 1>and you can just be sort of passive. The folks

0:29:44.400 --> 0:29:47.360
<v Speaker 1>at home don't have to do these calculations themselves and

0:29:47.480 --> 0:29:50.240
<v Speaker 1>updated to the satellite. So there are fewer links because

0:29:50.240 --> 0:29:52.840
<v Speaker 1>the Deep space network is kind of sort of overburdened

0:29:52.920 --> 0:29:54.920
<v Speaker 1>right now. It's got like too many things to do,

0:29:55.040 --> 0:29:58.000
<v Speaker 1>is I mean time slice between too many projects. So

0:29:58.080 --> 0:30:00.400
<v Speaker 1>this would really free it up, all right. Well, it

0:30:00.400 --> 0:30:02.840
<v Speaker 1>sounds like things are looking good for navigating within the

0:30:02.920 --> 0:30:06.160
<v Speaker 1>Solar System. So we're getting better clocks on these satellites

0:30:06.160 --> 0:30:10.360
<v Speaker 1>and spacecraft, and we're also we can also use familiar

0:30:10.600 --> 0:30:13.640
<v Speaker 1>landmarks like Jupiter or other planets or the Sun to

0:30:13.720 --> 0:30:16.720
<v Speaker 1>sort of orient where we are within the Solar System.

0:30:16.760 --> 0:30:18.520
<v Speaker 1>That's right, but then it sort of gets trickier one

0:30:18.680 --> 0:30:21.160
<v Speaker 1>once we get out into space. Right, Yeah, all these

0:30:21.200 --> 0:30:24.240
<v Speaker 1>things still rely on being able to contact Earth. You're

0:30:24.240 --> 0:30:27.280
<v Speaker 1>getting these messages from the Deep Space Network, which is

0:30:27.360 --> 0:30:29.680
<v Speaker 1>on Earth, and if you want to navigate to like

0:30:29.720 --> 0:30:33.440
<v Speaker 1>Alpha Centauri or halfway across the galaxy, you don't want

0:30:33.480 --> 0:30:35.240
<v Speaker 1>to be getting messages from Earth. They're gonna be way

0:30:35.240 --> 0:30:37.240
<v Speaker 1>too faint. You're not gonna be able to pick remain.

0:30:37.520 --> 0:30:40.320
<v Speaker 1>So you need a broader system. You need a galaxy

0:30:40.480 --> 0:30:43.040
<v Speaker 1>spanning system. In order to get you out of the

0:30:43.080 --> 0:30:45.520
<v Speaker 1>Solar System and still make it to McDonald's. We need

0:30:45.560 --> 0:30:51.680
<v Speaker 1>like a like a capital GPS galactic positioning system. All right, Well,

0:30:51.720 --> 0:30:53.920
<v Speaker 1>let's get into how you would actually navigate if you

0:30:53.960 --> 0:30:56.160
<v Speaker 1>wanted to venture out from the Solar System or even

0:30:56.200 --> 0:30:59.040
<v Speaker 1>go to another galaxy. But first let's take a quick break.

0:31:10.800 --> 0:31:13.160
<v Speaker 1>All right. There we're talking about how did not get

0:31:13.200 --> 0:31:18.440
<v Speaker 1>lost in space? Although that's such a fun show, is it?

0:31:18.520 --> 0:31:19.920
<v Speaker 1>You like that show that, the new one or the

0:31:19.960 --> 0:31:21.320
<v Speaker 1>old one. I like the old one, but the new

0:31:21.360 --> 0:31:23.080
<v Speaker 1>one's fun watching with the whole family because you know,

0:31:23.120 --> 0:31:26.080
<v Speaker 1>it's a bit of a family adventure, some family tension there,

0:31:26.080 --> 0:31:29.080
<v Speaker 1>you know, you leave somebody behind. If you were frozen

0:31:29.200 --> 0:31:32.080
<v Speaker 1>underwater on some alien moon, would your family stop and

0:31:32.080 --> 0:31:34.600
<v Speaker 1>save you or not? Oh? Man, To me, it was

0:31:34.680 --> 0:31:36.840
<v Speaker 1>almost too much family drama. I'm like, where is the

0:31:36.880 --> 0:31:42.320
<v Speaker 1>space and they're getting lost in space they're like melting ice. Yeah, exactly.

0:31:42.520 --> 0:31:45.680
<v Speaker 1>I thought it was good anyway, A lot of fun anyway. So, yeah,

0:31:45.760 --> 0:31:48.440
<v Speaker 1>it's a problem if you go out into space, especially

0:31:48.480 --> 0:31:50.400
<v Speaker 1>you can like in another part of the galaxy where

0:31:50.400 --> 0:31:52.480
<v Speaker 1>the stars are in a totally different arrangement. How do

0:31:52.520 --> 0:31:53.800
<v Speaker 1>you get around, how do you know where you are,

0:31:53.840 --> 0:31:56.240
<v Speaker 1>and how do you know where to go? So what

0:31:56.320 --> 0:31:58.080
<v Speaker 1>can we do then, Daniel? Yeah, well, what you need

0:31:58.120 --> 0:32:00.880
<v Speaker 1>is some other source of signals. Either have a very

0:32:00.960 --> 0:32:03.560
<v Speaker 1>accurate galactive map of where all the stars are, but

0:32:03.600 --> 0:32:06.040
<v Speaker 1>as you say, these things are changing in time and

0:32:06.160 --> 0:32:09.160
<v Speaker 1>we have only measurements from Earth and those positions are

0:32:09.200 --> 0:32:11.680
<v Speaker 1>not that accurate. Which you really need is some sort

0:32:11.720 --> 0:32:16.040
<v Speaker 1>of network of signals from all over the galaxy sending

0:32:16.080 --> 0:32:18.400
<v Speaker 1>you time stamped messages. I mean, if you could design

0:32:18.440 --> 0:32:21.720
<v Speaker 1>it yourself, you would have a bunch of sources around

0:32:21.760 --> 0:32:25.680
<v Speaker 1>the galaxy sending you messages saying time equals one time

0:32:25.680 --> 0:32:28.760
<v Speaker 1>equals two time equals three, right, and from those like

0:32:28.800 --> 0:32:31.880
<v Speaker 1>the like the GPS satellites we have just now on Earth,

0:32:32.080 --> 0:32:34.160
<v Speaker 1>you just have If you could just have GPS satellites

0:32:34.200 --> 0:32:37.400
<v Speaker 1>all the way through the galaxy super powerful, that would

0:32:37.440 --> 0:32:39.800
<v Speaker 1>be enough because you could use the nearest satellites to

0:32:39.840 --> 0:32:42.240
<v Speaker 1>figure out how far you are from each one, and

0:32:42.320 --> 0:32:44.560
<v Speaker 1>you need three of them to triangulate your position in

0:32:44.640 --> 0:32:47.800
<v Speaker 1>three D space and then you be golden. But you

0:32:47.840 --> 0:32:50.040
<v Speaker 1>know that's a trillion dollar program, right, could could you

0:32:50.160 --> 0:32:52.920
<v Speaker 1>use like galaxies to orienter cell? Like you know, like

0:32:52.960 --> 0:32:55.000
<v Speaker 1>if I'm in somewhere in the Milky Way, I could

0:32:55.080 --> 0:32:57.400
<v Speaker 1>tell where the center of the Milky Way was maybe,

0:32:57.880 --> 0:33:01.080
<v Speaker 1>and I could look for other galaxy ease out there,

0:33:01.480 --> 0:33:03.760
<v Speaker 1>and so can I use that to orient myself? Yeah,

0:33:03.800 --> 0:33:05.880
<v Speaker 1>And you can get a rough orientation that way, right,

0:33:05.920 --> 0:33:08.600
<v Speaker 1>you can tell you know where Andrameda is relative to

0:33:08.600 --> 0:33:11.560
<v Speaker 1>the Milky Way, So you can spin yourself around and

0:33:11.560 --> 0:33:14.080
<v Speaker 1>tell where and Drameda is. But it's very rough, I mean,

0:33:14.080 --> 0:33:16.959
<v Speaker 1>and Drameda is really far away, and so measuring its

0:33:17.040 --> 0:33:20.720
<v Speaker 1>location precisely is not that helpful. We need much more

0:33:20.760 --> 0:33:23.360
<v Speaker 1>precision than you can get from just like fixing the

0:33:23.440 --> 0:33:26.240
<v Speaker 1>positions of other galaxies, like, yeah, that will tell you roughly.

0:33:26.600 --> 0:33:28.520
<v Speaker 1>But if you want to navigate and you want to

0:33:28.520 --> 0:33:30.520
<v Speaker 1>save fuel and you want to make it with your

0:33:30.720 --> 0:33:34.760
<v Speaker 1>thousand frozen human bodies to Alpha Centauri or whatever, then

0:33:35.080 --> 0:33:36.560
<v Speaker 1>you've got to be more precise than that. You don't

0:33:36.560 --> 0:33:39.440
<v Speaker 1>want to miss by a few million kilometers, You got it,

0:33:39.840 --> 0:33:41.959
<v Speaker 1>You do not, And then they start to warm up

0:33:41.960 --> 0:33:44.920
<v Speaker 1>and there, you know, expecting the land in Alpha Centauri

0:33:45.000 --> 0:33:48.040
<v Speaker 1>and have breakfast, and you didn't bring any months and

0:33:48.040 --> 0:33:50.400
<v Speaker 1>so and so you're saying that one idea could could be,

0:33:50.440 --> 0:33:53.520
<v Speaker 1>like to make these GPS satellites and put them all

0:33:53.520 --> 0:33:56.440
<v Speaker 1>over the galaxy. But that's really expensive. Yeah, that's ridiculous,

0:33:56.440 --> 0:33:58.560
<v Speaker 1>Like we didn't even know how to get them there, right,

0:33:58.560 --> 0:34:03.680
<v Speaker 1>that's the whole problem. You're right, How would the satellites

0:34:03.720 --> 0:34:06.520
<v Speaker 1>know where to go or where they are? How would

0:34:06.560 --> 0:34:09.280
<v Speaker 1>we know where they are? We'd have to bootstrap them somehow.

0:34:09.719 --> 0:34:11.520
<v Speaker 1>If you don't know where the satellites are, then they're

0:34:11.520 --> 0:34:13.960
<v Speaker 1>not very useful right there, Like here's a signal from

0:34:14.000 --> 0:34:17.319
<v Speaker 1>someplace we don't know, thank you very much. That's useless.

0:34:17.400 --> 0:34:20.720
<v Speaker 1>So what you need to do is find some naturally

0:34:20.800 --> 0:34:24.920
<v Speaker 1>occurring equivalent something in the galaxy that operates similar to

0:34:25.040 --> 0:34:27.600
<v Speaker 1>GPS that lets you figure out where you are. And

0:34:27.640 --> 0:34:32.880
<v Speaker 1>it turns out the galaxy provides is it alien satellites? Daniel,

0:34:32.880 --> 0:34:35.479
<v Speaker 1>are you going for the alien button? I didn't even

0:34:35.560 --> 0:34:38.200
<v Speaker 1>think about the alien button, but now I am. Now

0:34:38.200 --> 0:34:41.600
<v Speaker 1>I'm wondering if aliens are using our GPS system to

0:34:41.680 --> 0:34:45.680
<v Speaker 1>navigate our solar system right to us. Yes, well, if

0:34:45.719 --> 0:34:49.160
<v Speaker 1>you enter the solar system that already had alien civilization

0:34:49.200 --> 0:34:51.600
<v Speaker 1>and have GPS signals, then yeah, you could use it

0:34:51.800 --> 0:34:54.919
<v Speaker 1>without them even noticing, because it's a passive system, right right,

0:34:55.040 --> 0:34:59.920
<v Speaker 1>then maybe they're using us as a GPS exactly exactly,

0:35:00.360 --> 0:35:04.360
<v Speaker 1>that's the concerned. But even without aliens, there are naturally occurring,

0:35:04.840 --> 0:35:07.799
<v Speaker 1>very regular clocks in our galaxy interesting and they are

0:35:07.800 --> 0:35:10.919
<v Speaker 1>called pulsars. You don't have to build them, they're already there.

0:35:11.000 --> 0:35:13.719
<v Speaker 1>They are already there. We talked on the podcast before

0:35:13.760 --> 0:35:17.480
<v Speaker 1>about what happens when really massive stars collapse that they

0:35:17.520 --> 0:35:20.320
<v Speaker 1>blow up, there's a supernova, and then if there's enough

0:35:20.400 --> 0:35:22.719
<v Speaker 1>stuff in the center of it, in the core, but

0:35:22.760 --> 0:35:24.640
<v Speaker 1>not enough to make a black hole, they can form

0:35:24.680 --> 0:35:28.400
<v Speaker 1>this thing called a neutron star, which is a ridiculously

0:35:28.520 --> 0:35:31.759
<v Speaker 1>dense ball of matter. It's called like the mass of

0:35:31.760 --> 0:35:34.920
<v Speaker 1>the Sun, but it's the size of a city. Right,

0:35:34.960 --> 0:35:37.400
<v Speaker 1>It's it's like almost a black hole. It's almost a

0:35:37.440 --> 0:35:40.439
<v Speaker 1>black hole. Yeah, if your star was like eighty two

0:35:40.480 --> 0:35:42.960
<v Speaker 1>thirty masses of the Sun, then you're probably going to

0:35:43.040 --> 0:35:45.120
<v Speaker 1>turn into a neutron star. If it was heavier than

0:35:45.160 --> 0:35:47.640
<v Speaker 1>you probably get into a black hole. But some of

0:35:47.680 --> 0:35:51.239
<v Speaker 1>these neutron stars are amazing because they have a magnetic

0:35:51.320 --> 0:35:55.719
<v Speaker 1>field which is really intense, and the magnetic field means

0:35:55.760 --> 0:35:59.040
<v Speaker 1>that there's a huge column of radiation that's spewed out

0:35:59.120 --> 0:36:01.840
<v Speaker 1>from the north magnetic field and the south magnetic field.

0:36:01.840 --> 0:36:05.040
<v Speaker 1>So they're like shining a really bright light of radiation

0:36:05.400 --> 0:36:08.880
<v Speaker 1>in two directions in space. Right, Because the stars themselves

0:36:08.880 --> 0:36:11.719
<v Speaker 1>don't shine that much, but like the chaos they cause

0:36:11.800 --> 0:36:14.640
<v Speaker 1>around them with the magnetic field and all the stuff

0:36:14.680 --> 0:36:17.440
<v Speaker 1>around them, then that is what glows and points in

0:36:17.480 --> 0:36:20.759
<v Speaker 1>a particular direction. Exactly. There's no fusion happening inside a

0:36:20.800 --> 0:36:23.399
<v Speaker 1>neutron star, but there's still an intense amount of other

0:36:23.480 --> 0:36:26.879
<v Speaker 1>radiation produced, and the magnetic field funnels it into these

0:36:26.920 --> 0:36:30.560
<v Speaker 1>type beams. And then if the magnetic north pole is

0:36:30.600 --> 0:36:33.920
<v Speaker 1>not aligned with the spinning of the star, right, it's

0:36:33.960 --> 0:36:36.480
<v Speaker 1>not perfectly aligned like on Earth. Then what you get

0:36:36.560 --> 0:36:40.400
<v Speaker 1>is this neutron star that's sweeping around. It's rotating, but

0:36:40.480 --> 0:36:44.680
<v Speaker 1>the direction in which its signal is beaming keeps scanning

0:36:44.680 --> 0:36:48.880
<v Speaker 1>through the galg like a galactic lighthouse, you know, like

0:36:48.920 --> 0:36:52.120
<v Speaker 1>a spotlight that just miss just like that, yeah, Or

0:36:52.160 --> 0:36:54.239
<v Speaker 1>like just like on the top of a police car,

0:36:54.360 --> 0:36:57.680
<v Speaker 1>you have this rotating red light and it never turns

0:36:57.680 --> 0:36:59.840
<v Speaker 1>on or off, but it looks to you like it's flashing.

0:37:00.200 --> 0:37:02.400
<v Speaker 1>So from Earth, if you look at a pulsar, it

0:37:02.480 --> 0:37:06.640
<v Speaker 1>goes on off, on off, on off, on off very regularly,

0:37:07.000 --> 0:37:09.880
<v Speaker 1>just like a lighthouse would or a police light, and

0:37:09.920 --> 0:37:11.759
<v Speaker 1>it's not actually turning on off, it's just sort of

0:37:11.800 --> 0:37:14.759
<v Speaker 1>sweeping past you. Right. So if we can use these

0:37:14.800 --> 0:37:17.040
<v Speaker 1>to kind of tell where we are, like as as

0:37:17.120 --> 0:37:20.960
<v Speaker 1>literally like lighthouses in space, sort of like lighthouses in space,

0:37:21.160 --> 0:37:24.520
<v Speaker 1>And the reason is that they're incredibly accurate. They have

0:37:24.880 --> 0:37:28.160
<v Speaker 1>about as much regularity as an atomic clock. Really, like

0:37:28.239 --> 0:37:32.040
<v Speaker 1>these little particles in very special conditions and cold climates

0:37:32.040 --> 0:37:36.280
<v Speaker 1>and special laboratories are very regular. But these enormous, massive

0:37:36.360 --> 0:37:40.560
<v Speaker 1>spinning hunks of neutrons are also regular, and so they're

0:37:40.560 --> 0:37:45.280
<v Speaker 1>basically like a very powerful galactic clock that's constantly descending

0:37:45.280 --> 0:37:50.439
<v Speaker 1>out a pulse like tick tick tick. Suddenly that makes

0:37:50.440 --> 0:37:53.120
<v Speaker 1>a nice guy a little more stressful. It's full of

0:37:53.200 --> 0:37:57.040
<v Speaker 1>ticking clocks. But it's it's like crazy periods to right,

0:37:57.080 --> 0:37:59.080
<v Speaker 1>it's not like tick tack tick. Take. It's like every

0:37:59.120 --> 0:38:02.480
<v Speaker 1>twenty millis like and they're shining. There's a big variety

0:38:02.480 --> 0:38:05.640
<v Speaker 1>of them, from radio pulsars down to X ray pulsars.

0:38:05.640 --> 0:38:08.759
<v Speaker 1>It depends, as you say, on their period. And these

0:38:08.760 --> 0:38:11.640
<v Speaker 1>ones that are very fast and like twenty milliseconds, these

0:38:11.640 --> 0:38:14.200
<v Speaker 1>are the best ones to use for timing. And it's

0:38:14.200 --> 0:38:18.560
<v Speaker 1>hard to imagine, like an enormous, super dense star boiled

0:38:18.640 --> 0:38:22.640
<v Speaker 1>down into a tiny object that spins every twenty milliseconds. Right,

0:38:22.680 --> 0:38:25.480
<v Speaker 1>It's like, hey, thousands and thousands of times a second,

0:38:25.880 --> 0:38:28.720
<v Speaker 1>this huge thing is spinning. It's it's an incredible amount

0:38:28.719 --> 0:38:31.000
<v Speaker 1>of energy. It's mind blowing. So we can use these

0:38:31.239 --> 0:38:34.239
<v Speaker 1>because we know from Earth where they are, and so

0:38:34.280 --> 0:38:37.280
<v Speaker 1>if you're out there in space, you could maybe find

0:38:37.320 --> 0:38:40.960
<v Speaker 1>them by looking out, and then you can tell kind

0:38:40.960 --> 0:38:42.759
<v Speaker 1>of where you are because you could recognize them. Buy

0:38:42.840 --> 0:38:45.959
<v Speaker 1>what their period. Each one has its own fingerprint because

0:38:45.960 --> 0:38:48.120
<v Speaker 1>of its period, and you already know where they are,

0:38:48.200 --> 0:38:50.880
<v Speaker 1>so you find them, you identified and you're like, okay,

0:38:50.880 --> 0:38:53.600
<v Speaker 1>this is pulsar x J seventeen or whatever. And then

0:38:53.600 --> 0:38:57.040
<v Speaker 1>you listen to the pulses, you know, tick tick tick,

0:38:57.600 --> 0:39:00.680
<v Speaker 1>and based on the pulses that you hear, you can

0:39:00.680 --> 0:39:03.520
<v Speaker 1>tell where in the wave form you are. Now, the

0:39:03.560 --> 0:39:06.480
<v Speaker 1>problem is they don't send messages like the GPS satellites.

0:39:06.520 --> 0:39:09.600
<v Speaker 1>The GPS satellite say okay, it's time equals seven, it's

0:39:09.640 --> 0:39:11.879
<v Speaker 1>time equals eight, and then when it gets to you,

0:39:11.880 --> 0:39:13.840
<v Speaker 1>you can compare against your own clock they have. You

0:39:13.880 --> 0:39:16.640
<v Speaker 1>have like synchronized clocks on each side, so you can

0:39:16.680 --> 0:39:19.120
<v Speaker 1>measure how long it takes the signal to get there.

0:39:19.440 --> 0:39:22.600
<v Speaker 1>That's from the GPS. Pulsars aren't as convenient. They don't

0:39:22.600 --> 0:39:26.080
<v Speaker 1>have a clock built in that labels each pulse separately,

0:39:26.320 --> 0:39:28.799
<v Speaker 1>so it's harder to tell exactly how long it took

0:39:29.000 --> 0:39:30.680
<v Speaker 1>the pulse to get there. Right, But why do you

0:39:30.680 --> 0:39:32.799
<v Speaker 1>need to know that? Couldn't you just kind of look

0:39:32.880 --> 0:39:35.200
<v Speaker 1>where they are and you know the angle to you,

0:39:35.480 --> 0:39:37.239
<v Speaker 1>and then use like three or four of them to

0:39:37.320 --> 0:39:39.600
<v Speaker 1>kind of triangulate where you are. What you really want

0:39:39.640 --> 0:39:42.919
<v Speaker 1>to know is your distance to an individual pulsar, because

0:39:42.960 --> 0:39:45.880
<v Speaker 1>that defines your position on the surface of a sphere

0:39:45.920 --> 0:39:48.720
<v Speaker 1>that surrounds that pulsar. And you do it for another pulsar,

0:39:48.920 --> 0:39:51.840
<v Speaker 1>and then your distance is defined by where those spheres intersect,

0:39:52.080 --> 0:39:54.160
<v Speaker 1>and we do it for three pulsars. Then you can

0:39:54.160 --> 0:39:56.960
<v Speaker 1>figure out where your distance is exactly in three D space.

0:39:57.120 --> 0:39:58.839
<v Speaker 1>You're right there. You can tell roughly where you are

0:39:58.920 --> 0:40:01.239
<v Speaker 1>by the angles, but that's not precise enough. Which you

0:40:01.280 --> 0:40:03.880
<v Speaker 1>really want to know is the distance to these things? Really?

0:40:03.920 --> 0:40:06.239
<v Speaker 1>Why is the angle not precise enough? Because these things

0:40:06.239 --> 0:40:09.240
<v Speaker 1>are really really far away, right, and so a pretty

0:40:09.239 --> 0:40:11.640
<v Speaker 1>big change in the location of the pulse are relative

0:40:11.640 --> 0:40:14.640
<v Speaker 1>to you corresponds to a really small change in the angle.

0:40:14.960 --> 0:40:17.120
<v Speaker 1>So what you really want to know is the radial distance,

0:40:17.360 --> 0:40:19.799
<v Speaker 1>not just the angle. Oh, I see, it works if

0:40:19.840 --> 0:40:22.560
<v Speaker 1>you're moving a huge distances, but like you couldn't tell

0:40:22.600 --> 0:40:24.600
<v Speaker 1>you like by the meter where you are, yeah, or

0:40:24.640 --> 0:40:26.480
<v Speaker 1>if you're really close to something, like if you're really

0:40:26.520 --> 0:40:29.680
<v Speaker 1>close to Jupiter, then it's angle relative to you has

0:40:29.719 --> 0:40:32.520
<v Speaker 1>a lot of powerful information about your location. But if

0:40:32.600 --> 0:40:35.960
<v Speaker 1>Jupiter is really far away, then that information loses value

0:40:36.000 --> 0:40:38.879
<v Speaker 1>and all these pulsars are pretty far away. But there's

0:40:38.880 --> 0:40:42.520
<v Speaker 1>actually a really cool trick to overcoming this problem of

0:40:42.880 --> 0:40:47.200
<v Speaker 1>pulsars not being like GPS statelines just using because great,

0:40:47.200 --> 0:40:49.319
<v Speaker 1>because I don't have the time stamp. They just have

0:40:49.360 --> 0:40:51.560
<v Speaker 1>a pulse. Yeah, so all you know is where you

0:40:51.600 --> 0:40:54.799
<v Speaker 1>are on the pulse. And so say these pulses are like,

0:40:55.200 --> 0:40:58.680
<v Speaker 1>you know, a kilometer long, for example, So if you

0:40:58.880 --> 0:41:01.399
<v Speaker 1>listen to a specific pulse, are that you could tell

0:41:01.440 --> 0:41:05.000
<v Speaker 1>where you are within that one kilometer long pulse. You're like, oh,

0:41:05.040 --> 0:41:06.279
<v Speaker 1>I'm at the top of it, or I'm at the

0:41:06.320 --> 0:41:08.080
<v Speaker 1>bottom of it, or I mean the quiet part of

0:41:08.080 --> 0:41:10.360
<v Speaker 1>it or the loud part of it. That doesn't actually

0:41:10.360 --> 0:41:12.600
<v Speaker 1>tell you how far you are from the pulse are.

0:41:12.680 --> 0:41:15.680
<v Speaker 1>What you know is how far you are through one

0:41:15.920 --> 0:41:19.000
<v Speaker 1>pulse length, but you don't know how many more pulse

0:41:19.120 --> 0:41:22.120
<v Speaker 1>lengths there are between you and the pulse are. If

0:41:22.160 --> 0:41:24.919
<v Speaker 1>you know you're halfway through its pulse, then you could

0:41:24.920 --> 0:41:27.760
<v Speaker 1>be half a pulse length away from the original pulsar,

0:41:28.280 --> 0:41:31.080
<v Speaker 1>or you could be one and a half pulse lengths away,

0:41:31.200 --> 0:41:34.800
<v Speaker 1>or three hundred forty two and a half pulse lengths away.

0:41:35.040 --> 0:41:39.400
<v Speaker 1>There's an infinite number of possibilities. So instead of locating

0:41:39.400 --> 0:41:42.040
<v Speaker 1>you onto a single sphere when you know the distance,

0:41:42.320 --> 0:41:46.000
<v Speaker 1>it's actually given you an infinite number of spheres, each

0:41:46.040 --> 0:41:49.080
<v Speaker 1>one one pulse length away, because all of those are

0:41:49.120 --> 0:41:53.000
<v Speaker 1>consistent with what you're seeing. That's not as good as GPS,

0:41:53.040 --> 0:41:55.880
<v Speaker 1>but you know it can still work because you can

0:41:55.920 --> 0:41:58.840
<v Speaker 1>do the same thing for another pulsar and get another

0:41:58.920 --> 0:42:02.000
<v Speaker 1>set of spheres, and then find a third pulsar and

0:42:02.040 --> 0:42:05.000
<v Speaker 1>get a third set of spheres, And where those spheares

0:42:05.080 --> 0:42:07.880
<v Speaker 1>intersect is the number of places that you could be

0:42:08.280 --> 0:42:11.399
<v Speaker 1>places that are consistent with the signals you're seeing. Now

0:42:11.440 --> 0:42:14.280
<v Speaker 1>that's not just one place, it's not a unique solution.

0:42:14.280 --> 0:42:18.040
<v Speaker 1>There's still a few ambiguities. There's more than one possible

0:42:18.080 --> 0:42:21.239
<v Speaker 1>location that's consistent with those signals, and then you have

0:42:21.239 --> 0:42:23.640
<v Speaker 1>to figure out which one is yours based on where

0:42:23.640 --> 0:42:26.640
<v Speaker 1>you thought you were recently, and you know other clues.

0:42:27.040 --> 0:42:29.440
<v Speaker 1>I see, you're sort of converting the time stamp of

0:42:29.480 --> 0:42:32.000
<v Speaker 1>these pulses to like using the speed of light to

0:42:32.080 --> 0:42:36.680
<v Speaker 1>kind of tell where you are in terms of space. Yeah, exactly,

0:42:36.920 --> 0:42:39.000
<v Speaker 1>and you don't know exactly how far your way you

0:42:39.000 --> 0:42:41.520
<v Speaker 1>are from the pulsar, you know, like, I'm a certain

0:42:41.600 --> 0:42:46.239
<v Speaker 1>number of beats of this pulsar's pulse away plus a

0:42:46.280 --> 0:42:48.920
<v Speaker 1>little bit, you know, only that extra little bit. And

0:42:48.960 --> 0:42:52.760
<v Speaker 1>so there's lots of different solutions, lots of different possibilities

0:42:52.760 --> 0:42:54.840
<v Speaker 1>for how far you might be away from one pulsar.

0:42:55.160 --> 0:42:57.160
<v Speaker 1>But if you have two or three or four, then

0:42:57.200 --> 0:42:59.560
<v Speaker 1>you can narrow it down. You can say I'm a

0:42:59.560 --> 0:43:01.759
<v Speaker 1>certain from this one, a certain distance from that one.

0:43:01.880 --> 0:43:06.400
<v Speaker 1>It's a harder problem because these pulsars aren't nicely time stamped,

0:43:06.520 --> 0:43:08.799
<v Speaker 1>but people have figured it out, and if you do

0:43:08.880 --> 0:43:11.440
<v Speaker 1>all the mathematics, you can figure out where you are

0:43:11.480 --> 0:43:14.759
<v Speaker 1>in the Solar system to within five kilometers. Wow, that's

0:43:14.760 --> 0:43:17.200
<v Speaker 1>pretty good. That's pretty good. That's better than the two

0:43:17.719 --> 0:43:20.480
<v Speaker 1>from before. Yeah, exactly, it's pretty good. And it works

0:43:20.520 --> 0:43:23.319
<v Speaker 1>all the way across the galaxy, not just within our

0:43:23.360 --> 0:43:26.080
<v Speaker 1>Solar system, so you can be far from even if

0:43:26.160 --> 0:43:29.320
<v Speaker 1>Earth in blodes the nuclear war, you can still figure

0:43:29.360 --> 0:43:32.600
<v Speaker 1>out where you are from these pulsars. Are the pulsars

0:43:32.760 --> 0:43:35.960
<v Speaker 1>distributed all over the galaxy or are we only looking

0:43:36.000 --> 0:43:38.760
<v Speaker 1>at the ones around us. They're distributed across the galaxy.

0:43:38.840 --> 0:43:40.840
<v Speaker 1>People have done a study and they found like fifty

0:43:40.920 --> 0:43:44.560
<v Speaker 1>or sixty good X ray pulsars that are distributed well

0:43:44.680 --> 0:43:46.799
<v Speaker 1>enough across the galaxy that you could use them as

0:43:46.880 --> 0:43:50.680
<v Speaker 1>reference points. And they've actually tried this. They've done it.

0:43:50.680 --> 0:43:53.000
<v Speaker 1>They've built a little one and they fluid on the

0:43:53.040 --> 0:43:56.160
<v Speaker 1>International Space Station and they tried it and it worked. Wow.

0:43:56.200 --> 0:43:58.520
<v Speaker 1>Pretty cool, all right, So it sounds like we do

0:43:58.600 --> 0:44:01.400
<v Speaker 1>have a GPS for the Alexy. We have a galactic

0:44:01.480 --> 0:44:04.719
<v Speaker 1>Pulse source system. You should also call it GPS. It's

0:44:04.760 --> 0:44:07.759
<v Speaker 1>pretty awesome. It's pretty awesome. I love this idea of like,

0:44:08.280 --> 0:44:10.800
<v Speaker 1>you know, astronomers don't get to build what they want.

0:44:10.960 --> 0:44:13.200
<v Speaker 1>They just get to look out there and find stuff

0:44:13.239 --> 0:44:16.080
<v Speaker 1>and use it to be clever to extract the information

0:44:16.120 --> 0:44:18.759
<v Speaker 1>they need. And here's another great example of just like

0:44:18.880 --> 0:44:21.319
<v Speaker 1>making do with what you have. Right, it's almost like

0:44:21.360 --> 0:44:24.480
<v Speaker 1>a nature and the universe made these lighthouses and put

0:44:24.520 --> 0:44:27.040
<v Speaker 1>them all over the galaxy just for us to kind

0:44:27.040 --> 0:44:29.960
<v Speaker 1>of used to get around. Yeah, probably not just for us,

0:44:30.120 --> 0:44:32.120
<v Speaker 1>but it would be a cool science fiction universe where

0:44:32.160 --> 0:44:34.840
<v Speaker 1>we actually visit one of these pulsars and discover, oh,

0:44:34.880 --> 0:44:38.960
<v Speaker 1>they're artificial. Maybe they're part of some billion global positions. Oh,

0:44:38.960 --> 0:44:42.759
<v Speaker 1>it is a lighthouse. It didn't occur naturally, that would

0:44:42.760 --> 0:44:45.560
<v Speaker 1>be pretty awesome. That would be worth some echoes in space.

0:44:45.680 --> 0:44:50.880
<v Speaker 1>Space space space space space cool cool cool. All right, Well,

0:44:51.239 --> 0:44:53.440
<v Speaker 1>I feel a lot better now about Star Wars and

0:44:53.520 --> 0:44:57.520
<v Speaker 1>about other science fiction movies and books. It sounds like

0:44:58.160 --> 0:45:00.920
<v Speaker 1>in the future we could be using these pulsars to

0:45:01.040 --> 0:45:02.600
<v Speaker 1>kind of know where we are in the galaxy and

0:45:02.640 --> 0:45:05.279
<v Speaker 1>to kind of build a map of the entire place. Yeah,

0:45:05.440 --> 0:45:08.560
<v Speaker 1>and as we venture out further and further beyond our

0:45:08.560 --> 0:45:11.400
<v Speaker 1>solar system and try to explore other solar systems, this

0:45:11.440 --> 0:45:13.440
<v Speaker 1>will be a critical way to know where we are

0:45:13.560 --> 0:45:16.720
<v Speaker 1>and hopefully how to come home. Yeah, And so future

0:45:16.800 --> 0:45:20.719
<v Speaker 1>space explorers flying around with their partners and spouses can

0:45:21.000 --> 0:45:24.399
<v Speaker 1>not argue about where they are getting lost, which would

0:45:24.400 --> 0:45:26.719
<v Speaker 1>probably make for a messy divorce out in space. Well,

0:45:26.719 --> 0:45:28.920
<v Speaker 1>they'll probably still argue, like, let's not use that pulsar.

0:45:29.000 --> 0:45:34.560
<v Speaker 1>That one's not reliable. Everybody's using that pulsar. You sound

0:45:34.640 --> 0:45:37.480
<v Speaker 1>like you, You sound like your father. All right. Well,

0:45:37.520 --> 0:45:40.439
<v Speaker 1>I hope that was interesting and gives you a little

0:45:40.480 --> 0:45:42.319
<v Speaker 1>bit more of a sense that we kind of know

0:45:42.360 --> 0:45:45.279
<v Speaker 1>where we are in the universe and the galaxy, and

0:45:45.400 --> 0:45:46.839
<v Speaker 1>that it would be a little bit hard to get

0:45:46.880 --> 0:45:49.280
<v Speaker 1>lost in space. That's right. And this idea of pulsars

0:45:49.360 --> 0:45:52.040
<v Speaker 1>took decades to figure out to narrow down to make

0:45:52.080 --> 0:45:55.239
<v Speaker 1>it work, and it only gives us five kilometer uncertainty.

0:45:55.440 --> 0:45:58.520
<v Speaker 1>Probably somebody out there will have an even better idea

0:45:58.760 --> 0:46:00.960
<v Speaker 1>for how to narrow down our edition. So have that

0:46:01.080 --> 0:46:03.359
<v Speaker 1>idea today so that it's ready for us to use

0:46:03.480 --> 0:46:05.560
<v Speaker 1>in twenty or thirty years. That's right. You don't want

0:46:05.560 --> 0:46:07.719
<v Speaker 1>to miss those snacks, you know. If you miss that

0:46:07.800 --> 0:46:11.200
<v Speaker 1>snack by five kilometers, that's that's not good eating. If

0:46:11.239 --> 0:46:13.520
<v Speaker 1>you learn nothing else today. Remember there are no U

0:46:13.600 --> 0:46:17.320
<v Speaker 1>turns in space or echoes, but there probably are snacks,

0:46:18.200 --> 0:46:20.759
<v Speaker 1>all right. Thanks for joining us, See you next time.

0:46:28.960 --> 0:46:31.760
<v Speaker 1>Thanks for listening, and remember that Daniel and Jorge Explain

0:46:31.840 --> 0:46:34.719
<v Speaker 1>the Universe is a production of I Heart Radio. For

0:46:34.840 --> 0:46:37.759
<v Speaker 1>more podcast for my Heart Radio, visit the I Heart

0:46:37.840 --> 0:46:41.480
<v Speaker 1>Radio Apple Apple Podcasts, or wherever you listen to your

0:46:41.520 --> 0:46:42.240
<v Speaker 1>favorite shows.