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Heidi Campo: Welcome back to another fun episode, a Q

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and A episode of space nuts.

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Generic: 15 seconds. Guidance is internal.

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10, 9. Ignition

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sequence start. Space nuts. 5, 4, 3.

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2. 1, 2, 3, 4, 5, 5, 4,

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3, 2, 1. Space nuts. Astronauts

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report. It feels good.

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Heidi Campo: I'm your host, Heidi Campo, filling in for

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Andrew Dunkley. And joining us is Professor

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Fred Watson, astronomer at large.

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How are you doing, Fred? That was quite the

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smart, uh, little adjustment of your glasses.

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It made you look even more smart.

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Professor Fred Watson: Oh, thank. Thank

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you, Heidi. You can come again. Um,

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Luke, um, it's great to see you again and,

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uh, all going well here and lots, um,

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of exciting space stuff always to talk about,

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especially with the questions that we get

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from our listeners, which are always

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intriguing and often very

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insightful.

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Heidi Campo: Yeah.

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And so we do have. We have four questions

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today. Um, you know, two.

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Two audio questions, two

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written questions. Um, but we do want to say

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if you did not hear our announcement on the

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last episode, uh, we'll make that an episode

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and make that announcement again. We just

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want to say thank you to our listeners. We

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were declared, I guess you could say, the

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seventh, uh, top 20, top

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seven, uh, astronomy podcasts,

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wherever you listen to your podcast. So thank

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you so much. Fred, do you have anything you

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want to add to that?

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Professor Fred Watson: Only, um, uh, only that

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it's amazing how many people do

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listen to our podcasts. Um, I was in a

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medical waiting room on Monday, and a

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gentleman, I think his name was Stephen, came

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up and said, really enjoy the podcast.

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So, uh, it's quite nice.

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Heidi Campo: You're, like, at poverty.

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Professor Fred Watson: Well, you must be, too. I bet you find

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people, uh, and if you don't now, you will.

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You will do. Eventually, people who come up

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to you and say, yeah, I know your face, or, I

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know your. I know your voice.

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Heidi Campo: Well, I think I have to leave my house for

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that to happen. I. I'm. I'm too

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busy. I'm at the lab or I'm at home, so

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you don't see me in public unless you see me

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at the grocery store.

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Professor Fred Watson: There you go. That could be where it happens.

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You never know. So anyway, yeah,

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it's. Look, it's great to have that,

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um, seventh ranking in, uh, the

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world's top 50 astronomy

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podcasts. I'm thrilled to hear it.

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Heidi Campo: Well, I guess that makes our, uh, regular,

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um, people who write in their questions

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famous too, then, because we do have some

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regulars, a few of them today.

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Um, our first question today is from Mark

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Painter, and Mark has another

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black hole question. And then he has this

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funny emoji, uh, next to it that he, he

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made with text. It's not like a regular

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emoji. He did that with like special

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characters. Very clever. All right, so we

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have another, we have another black hole

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question from Mark. And Mark asks, as a

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singularity is formed with infinite mass,

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there must be a process of reduction,

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starting with electron degenerate matter,

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then collapsing to a neutron star. Then there

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is a quark, quark matter in

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massive neutron stars, where quarks are no

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longer confined to protons and

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neutrons. So my question is this. Can there

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be more stages of matter reduction to go

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through before a singularity or a Planck star

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is formed? That is, can

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quarks be composed of smaller units of

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matter and then these units break down

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to, to their constitutes

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and so on? Could there be many forms of

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matter we are yet to theorize

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and at some time possibly

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discover? Could it be elephants all

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the way down?

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Professor Fred Watson: Yeah, uh, oh, turtles all the way down. I

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think that was the other way of looking at

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the universe. Um, so it's a great

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question. Um, you know, if you think of. So

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we envisage the process of a black

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hole forming after a supernova explosion.

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You've got the uh, star which

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has run out of hydrogen fuel. Uh,

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this is one way of black hole formation.

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There's others. Uh, but anyway, it uh, runs

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out of hydrogen fuel, so there's no longer

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the outward radiation pressure to support the

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mass of the star, and it collapses. Uh, and

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if there's enough material there, the

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collapse doesn't just stop with

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uh, as, as Mark points out, electron

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degenerate matter. That's what we call a

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white dwarf star. Uh, or it doesn't

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stop with that, and it doesn't stop with

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neutron degenerate matter, which is what we

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call a neutron star. It just collapses down

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basically to uh, to, to a

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singularity, to this point of infinite

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density. Um, and it's not

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infinite mass, as Mark said, it's

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infinite density. But, um, that's not the

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point. The point is, um, you know, is there,

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uh, as you get to that

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singularity, are there

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other constituents of matter

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that the collapse goes through? And

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my understanding of this is that the answer

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is no. Uh, we understand

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the very well from particle physics

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what the, the most fundamental

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particles of matter are. Uh,

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uh, and it's what we call the standard model.

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There are 16 of them, plus something called

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the Higgs boson, which gives all, all the

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others their mass. Um,

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um, and ah, that these as far

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as we know, are ah, indivisible.

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They are not able to fall

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into, into Pieces. They are,

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they are the ultimate, you know, the

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ultimate building blocks of matter.

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Um, there are six quarks, the up, down,

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charm, strange top and bottom quarks.

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Uh, that's the, you know, the,

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the, the, the quark component. So quarks

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themselves are, ah, have, have different

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varieties. Um, there are six

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leptons. The electron muon, tau,

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electron neutrino, muon neutrino and tau

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neutrino. And then the four fundamental

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forces of nature. What are called the gauge

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bosons, the gluon which

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uh, operates the strong atomic force,

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the photon, which we know is all about

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electromagnetic radiation, and the Z and W

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bosons, which uh, uh, dictate the weak

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nuclear force. So those are what, what

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everything is made of. And

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uh, the idea of separating them

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into smaller particles I think is

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uh, something that uh, the particle

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physicists rule out. They're telling us that

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that's the way it goes. And so yes, as

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the collapse takes place, um, these are

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probably the last things to you know, not

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to come into existence but to disappear, uh,

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down the singularity, if I can put it that

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way. But it's a great question, uh, Mark, and

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got me thinking about particle physics once

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again.

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Heidi Campo: Excellent.

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Well it looks like our next question is from

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one of those uh, famous regular

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listeners and it is a audio question,

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so we are going to play that for you now. You

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guys can all listen to Buddy from Oregon's

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question and Fred and I are going to listen

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to that right now. I'm just letting Fred get

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that queued up. All right everyone, we're

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going to play Buddy's question for you now.

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Buddy: This is Buddy from Ontario, Oregon again.

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Hey, I was listening to your latest episode

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and uh, where you m announced that

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there's a third object from outside our solar

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system passing through a comet I guess. And I

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know you said there was no point before in

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uh, trying to catch these objects because

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if you get that fast, you can sense something

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or that object in any direction. What if you

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were to just land like a spin launch on,

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on one of those objects with a few

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satellites. That way anytime it happen to get

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close enough to, to uh, something

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interesting, we could launch it with a spin

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launch and possibly maybe use that spin

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launch to counteract the speed that you're

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going at so that you could just kind of

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gently place a object in,

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in orbit around something. Seems like we

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should have eyes in any, every direction we

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can send one. But ah, anyways, what do you

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guys think? Thanks guys. Love this podcast.

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Professor Fred Watson: Um, intriguing stuff from Buddy as always.

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Um, so just uh, Filling

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in a few gaps in that SpinLaunch is indeed a

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technique for launching

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space vehicles. Uh, it's

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a company, I think they're called SpinLaunch,

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uh, and they've built this gigantic device

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that spins things up to a high level of

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rotation and that lets them go. Um,

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my understanding, although they've got um, I

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know there's an announcement recently they've

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got a large contract uh, for

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some possible uh, space vehicles. I don't

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think they've yet achieved um, a sufficient

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velocity as ah, you release it from the spin

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to get into orbit. That needs to go up to

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8km per second and I think they're much

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less than that. So um, M from Earth.

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Ah, that's not really a viable way

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of doing what Buddy's talking about, which is

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chasing after an interstellar object.

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Um, if you had one of these machines

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on board a spacecraft already, that

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might be a viable way of doing it because you

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only need to give it a smaller impulse. But

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you can still do that chemically. You can

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actually, you've got much more control over

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uh, what you're doing with chemical rockets.

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And the problem is, uh, as Buddy

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highlights the objects

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like these various,

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um, the three interstellar, um,

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objects that have passed through the solar

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system, Oumuamua, uh,

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Borisov, Comet Borisov, and the Current 1,

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uh, 3i Atlas, which is showing all the signs

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of being a comet. Um,

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that one's passing through the solar system

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at the moment. The problem is they're moving

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so fast. Um, uh, Atlas is

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moving at 60 ah, kilometers per second.

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It's a huge speed,

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bigger um, than anything that we've ever

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launched into space before, so we'd never

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chase it. Um, and

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this is the problem from our vantage point on

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uh, Earth. The idea is that one of these

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things comes in, you mount a space mission to

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go and rendezvous with it and check it out,

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which would be wonderful. But exactly as

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Buzzy says, you need eyes in all directions

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and more especially you need spacecra that

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are probably already out there, uh, just

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waiting to be deployed in particular

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directions. Now there's an interesting

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footnote though to this story because, um,

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within the last week we've had a

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proposal from our good

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friend Avi Loeb of the Harvard

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Smithsonian, uh, Center for Astrophysics.

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He has made the suggestion that

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uh, because uh, the ATLAS

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comet, uh, currently going through the solar

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system from some other solar system, it's

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probably older than our solar system because

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that passes relatively close to Jupiter. And

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I think it's either next year or the year

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after I Think it's probably next year,

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um, you could deploy

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a uh, spacecraft already in orbit around

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Jupiter. Uh, and he's thinking of the Juno

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spacecraft which is uh, already uh,

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orbiting Jupiter and telling us a lot about

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that planet. Um, you could change its

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orbit. It's in a very, uh, already in a

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highly elliptical or elongated

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orbit. Uh, uh, Loeb and his

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colleagues suggest that you could change that

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orbit, uh, make it

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elongated enough that you actually

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get uh, a closer look at uh, Comet

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3I Atlas as it passes by Jupiter.

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And that will be fabulous because it would be

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a way of getting up close and personal

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uh, with an interstellar object that might

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tell us a lot more about them, uh, about it

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than we, we know already. So um,

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so I think this is an exciting area that

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Buddy's highlighted. Uh, the idea of

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rendezvousing with uh, extraterrestrial

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or extrasolar, um,

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uh, extra

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extrasolar asteroids or comets,

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rendezvousing them with them, uh, with

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whatever we have at our disposal. And if

296
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we've got Juno at our disposal already

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hanging around in the vicinity of Jupiter,

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maybe it will be a good thing to do to bring

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the mission to an end by rendezvousing with

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Comet 3i Atlas. So I like that

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question.

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Heidi Campo: A lot of tongue twisters in this field.

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Professor Fred Watson: It's true.

304
00:13:15.200 --> 00:13:17.400
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00:15:02.100 --> 00:15:03.500
Generic: Roger in your labs right here.

345
00:15:03.500 --> 00:15:04.900
Professor Fred Watson: Also space nuts.

346
00:15:05.300 --> 00:15:07.540
Heidi Campo: Our next question starts, uh, off with a

347
00:15:07.540 --> 00:15:10.190
tongue twister. This is Lawrence from London

348
00:15:10.910 --> 00:15:13.910
says hi agents Lawrence from London. Lawrence

349
00:15:13.910 --> 00:15:16.190
from London here. I will jump straight to the

350
00:15:16.190 --> 00:15:18.710
point. Has there ever been any sort of

351
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proposal of space time being a super

352
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fluid? And if so, how did that play out?

353
00:15:24.750 --> 00:15:27.670
One of my biggest grievances are those space

354
00:15:27.670 --> 00:15:30.190
time diagrams that show a single plane with

355
00:15:30.190 --> 00:15:32.910
the planet on top causing curvature

356
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on said plane. For me it feels like

357
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it skews the four dimensional reality that

358
00:15:38.650 --> 00:15:41.610
truly exists as there is not just a single

359
00:15:41.610 --> 00:15:44.050
plane for everything to rest on. If we could

360
00:15:44.050 --> 00:15:46.650
find ways to visualize this more accurately,

361
00:15:46.970 --> 00:15:49.730
I feel like we would appeal to the

362
00:15:49.730 --> 00:15:52.530
fluid more often to describe the behavior

363
00:15:52.530 --> 00:15:55.130
of space time as it would allow for these

364
00:15:55.130 --> 00:15:57.610
extra dimensions rather than the typical two

365
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dimensional spacetime diagrams. As for

366
00:16:00.330 --> 00:16:03.000
time, perhaps it could be understood

367
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to be the flow rate of the superfluid.

368
00:16:06.600 --> 00:16:08.840
As for the elasticity and the structural

369
00:16:08.840 --> 00:16:11.640
integrity we see of space time, maybe

370
00:16:11.640 --> 00:16:14.640
quantized vortices. As for

371
00:16:14.640 --> 00:16:17.279
gravity, I have no idea. It is a good thing

372
00:16:17.279 --> 00:16:19.520
that I can ask this question to an

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astrophysicist. Many thanks gents. Looking

374
00:16:22.320 --> 00:16:24.440
forward to hearing your response.

375
00:16:25.560 --> 00:16:27.680
I'm interested too. That was quite an

376
00:16:27.680 --> 00:16:29.840
interesting, um, visual.

377
00:16:31.600 --> 00:16:34.040
Professor Fred Watson: Yeah, that's right. And his point's well

378
00:16:34.040 --> 00:16:36.480
made. Um, thanks. Thanks Lawrence for this.

379
00:16:36.560 --> 00:16:39.120
Your point's well made that we have no way of

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depicting space time being distorted by

381
00:16:42.560 --> 00:16:45.280
matter, which is what happens other than,

382
00:16:45.360 --> 00:16:47.640
you know, this picture that we all are

383
00:16:47.640 --> 00:16:49.640
familiar with of a planet sitting on a

384
00:16:49.640 --> 00:16:52.000
trampoline, uh, with the

385
00:16:52.080 --> 00:16:54.760
trampoline map being distorted by the, by the

386
00:16:54.760 --> 00:16:56.520
gravity of the planet. That's because we have

387
00:16:56.520 --> 00:16:58.550
to reduce it to two dimensions. It's because,

388
00:16:58.620 --> 00:17:00.140
because it's the only way we can really

389
00:17:00.140 --> 00:17:02.300
envisage it. But

390
00:17:02.760 --> 00:17:05.740
um, the notion underlying

391
00:17:06.080 --> 00:17:08.940
uh, Lawrence's question is

392
00:17:09.020 --> 00:17:11.780
that, uh, he's sort of in a

393
00:17:11.780 --> 00:17:14.460
sense ahead of the game. And that is because,

394
00:17:14.700 --> 00:17:17.460
well, uh, he talks about superfluids. A

395
00:17:17.460 --> 00:17:19.660
superfluid is a fluid with zero

396
00:17:19.660 --> 00:17:22.060
viscosity and that is what

397
00:17:22.060 --> 00:17:25.030
spacetime is. Uh, it is already

398
00:17:25.750 --> 00:17:28.310
effectively a superfluid. Uh, our

399
00:17:28.310 --> 00:17:31.110
Understanding of space time comes from

400
00:17:31.350 --> 00:17:34.190
general relativity, Einstein's general theory

401
00:17:34.190 --> 00:17:36.470
of relativity. And he was,

402
00:17:37.430 --> 00:17:40.230
he understood the idea that

403
00:17:40.710 --> 00:17:43.470
matter would distort

404
00:17:43.470 --> 00:17:45.940
space, uh,

405
00:17:46.310 --> 00:17:48.310
because he was basically trying to understand

406
00:17:48.470 --> 00:17:50.870
gravity. Uh, and he

407
00:17:53.890 --> 00:17:55.690
basically what he did was propose that

408
00:17:55.690 --> 00:17:58.570
gravity, so that gravity was the way he was

409
00:17:58.570 --> 00:18:01.250
approaching this. Gravity is the same as

410
00:18:01.250 --> 00:18:04.170
acceleration. Um, so if

411
00:18:04.170 --> 00:18:06.930
you were in a spacecraft, uh, with

412
00:18:06.930 --> 00:18:09.410
no windows, uh, and

413
00:18:09.490 --> 00:18:12.410
somebody lit the fuse and put the

414
00:18:12.410 --> 00:18:14.450
rocket underneath the spacecraft and sent it

415
00:18:14.450 --> 00:18:17.210
accelerating on its way from within that

416
00:18:17.210 --> 00:18:19.740
spacecraft, you would not know whether you're

417
00:18:19.740 --> 00:18:22.580
feeling the effect of the acceleration or the

418
00:18:22.580 --> 00:18:24.940
pull of gravity. They are indistinguishable.

419
00:18:24.940 --> 00:18:27.740
It's something that technically is

420
00:18:27.980 --> 00:18:29.980
known by the equivalence principle, which

421
00:18:30.060 --> 00:18:32.860
holds up incredibly strongly.

422
00:18:33.820 --> 00:18:35.380
So what you're saying is gravity and

423
00:18:35.380 --> 00:18:37.420
acceleration are effectively the same thing.

424
00:18:37.660 --> 00:18:40.020
That allowed Einstein to build a

425
00:18:40.020 --> 00:18:42.540
geometrical model of how gravity works.

426
00:18:42.700 --> 00:18:45.300
And that's what led to our

427
00:18:45.300 --> 00:18:47.300
understanding of space time. Something that

428
00:18:47.300 --> 00:18:49.580
is distorted by the presence of matter.

429
00:18:50.840 --> 00:18:52.980
Uh, it's got a uh,

430
00:18:52.980 --> 00:18:55.130
gobbledygook description, the

431
00:18:55.130 --> 00:18:58.090
mathematical uh, description

432
00:18:58.090 --> 00:19:01.090
or the mathematical structure if you

433
00:19:01.090 --> 00:19:03.890
like, that we see a

434
00:19:03.890 --> 00:19:06.770
space time, um, it is based

435
00:19:06.770 --> 00:19:08.450
on geometry developed by

436
00:19:09.730 --> 00:19:12.050
a uh, German mathematician who's can't

437
00:19:12.050 --> 00:19:13.610
remember his first name. His second name was

438
00:19:13.610 --> 00:19:16.170
Riemann. Riemann in the

439
00:19:16.170 --> 00:19:19.000
1850s proposed the idea

440
00:19:19.000 --> 00:19:21.200
of spaces that could be

441
00:19:21.200 --> 00:19:23.960
distorted by things within them.

442
00:19:25.000 --> 00:19:27.960
And that turns out that that's exactly what

443
00:19:27.960 --> 00:19:30.800
space time is. Uh, in the

444
00:19:30.800 --> 00:19:33.520
relativistic view it's something a

445
00:19:33.520 --> 00:19:35.280
mathematical construct that we call a

446
00:19:35.280 --> 00:19:38.160
Riemannian manifold. And it is a

447
00:19:38.160 --> 00:19:40.640
superfluid. It basically behaves just like a

448
00:19:40.640 --> 00:19:43.480
superfluid. Uh, and uh, you

449
00:19:43.480 --> 00:19:46.120
know, the quantized vortices that Lawrence

450
00:19:46.120 --> 00:19:49.000
mentions, that puts a different slant

451
00:19:49.000 --> 00:19:51.800
on it because you're suddenly into

452
00:19:51.980 --> 00:19:54.840
um, uh, um, quantum ah,

453
00:19:55.280 --> 00:19:58.080
theory, uh, rather than

454
00:19:58.080 --> 00:20:00.880
relativity theory. So we'll just leave that

455
00:20:00.880 --> 00:20:03.600
to one side. But as far as relativity is

456
00:20:03.600 --> 00:20:06.440
concerned, space is a superfluid. And the way

457
00:20:06.440 --> 00:20:08.960
gravity emerges. Lawrence says, as for

458
00:20:08.960 --> 00:20:10.560
gravity, I have no idea. It's a good thing I

459
00:20:10.560 --> 00:20:12.400
can ask this question to an astrophysicist.

460
00:20:12.400 --> 00:20:14.665
Well, I'm glad you did. Uh, because grav,

461
00:20:14.665 --> 00:20:16.500
gravity is the acceleration. It's the

462
00:20:16.980 --> 00:20:18.980
distortion of space causing

463
00:20:19.860 --> 00:20:22.860
us to feel an acceleration which we see as

464
00:20:22.860 --> 00:20:25.740
gravity. I hope that answers Lawrence's

465
00:20:25.740 --> 00:20:26.100
question.

466
00:20:27.460 --> 00:20:28.740
Heidi Campo: That was fantastic.

467
00:20:31.700 --> 00:20:33.940
Generic: Three, two, one.

468
00:20:34.500 --> 00:20:35.700
Heidi Campo: Space nuts.

469
00:20:35.860 --> 00:20:38.660
Our very last question of this episode

470
00:20:38.740 --> 00:20:40.830
is from Dan,

471
00:20:41.420 --> 00:20:44.310
um, on the Gold coast. And this is also an

472
00:20:44.310 --> 00:20:46.150
audio question. So I'm going to give Fred

473
00:20:46.150 --> 00:20:49.030
just a second to cue that up and we are going

474
00:20:49.030 --> 00:20:50.110
to play that for you now.

475
00:20:50.750 --> 00:20:52.830
Martin Berman Gorvine: Hey, guys. Dan here from the Gold Coast.

476
00:20:53.230 --> 00:20:54.670
Quick, um, question. Thought it might be a

477
00:20:54.670 --> 00:20:57.590
bit different for you. Got a friend who a

478
00:20:57.590 --> 00:21:00.190
couple of years ago we were discussing space

479
00:21:00.190 --> 00:21:02.310
exploration, that kind of stuff, and his view

480
00:21:02.310 --> 00:21:04.670
was that he'd understand why the human race

481
00:21:05.630 --> 00:21:07.870
puts, uh, time into exploring space

482
00:21:08.540 --> 00:21:10.780
when we still don't quite understand Earth.

483
00:21:11.100 --> 00:21:13.900
And I couldn't, you know, I couldn't put into

484
00:21:13.900 --> 00:21:16.660
words myself why it's so important, which I

485
00:21:16.660 --> 00:21:19.500
understand it is. I was hoping you could put

486
00:21:19.500 --> 00:21:22.140
into your own words why is it so important

487
00:21:22.140 --> 00:21:24.960
that we also put time into, uh,

488
00:21:25.100 --> 00:21:27.770
exploring space? Thanks for that. Um,

489
00:21:27.980 --> 00:21:30.860
also, Heidi, with your sci fi brain,

490
00:21:30.860 --> 00:21:32.780
I'm wondering, have you read Project Hail

491
00:21:32.780 --> 00:21:35.540
Mary? Do you love it like I do? And are you

492
00:21:35.540 --> 00:21:37.860
excited for the movie? All right, cheers.

493
00:21:38.020 --> 00:21:38.500
Bye.

494
00:21:39.940 --> 00:21:42.300
Heidi Campo: Oh my goodness. I'm so excited that you

495
00:21:42.300 --> 00:21:45.060
brought up Project Hail Mary. Um, that is

496
00:21:45.060 --> 00:21:47.980
next on my list. Um, it

497
00:21:47.980 --> 00:21:49.900
is next on my list. I have read other books

498
00:21:49.900 --> 00:21:52.900
from that author and I'm very excited to

499
00:21:52.900 --> 00:21:55.780
read it, but I have not yet. Um, and I

500
00:21:55.780 --> 00:21:58.260
feel a little bit like a hypocrite because

501
00:21:58.740 --> 00:22:01.580
I pride myself on often reading the

502
00:22:01.580 --> 00:22:03.580
books before the movies. But now I feel like

503
00:22:03.580 --> 00:22:05.300
a hipster because I'm reading it before the

504
00:22:05.300 --> 00:22:06.100
movie comes out.

505
00:22:09.140 --> 00:22:11.220
Professor Fred Watson: That's good. No, that's. You're ahead of the

506
00:22:11.220 --> 00:22:14.140
game, Heidi. That's the great thing. Um, when

507
00:22:14.140 --> 00:22:16.060
you've read it, I'd love to hear what it's

508
00:22:16.060 --> 00:22:16.340
about.

509
00:22:18.340 --> 00:22:18.740
Heidi Campo: Facebook.

510
00:22:20.340 --> 00:22:22.820
Professor Fred Watson: Yeah. Yep, sounds great.

511
00:22:24.580 --> 00:22:27.220
Very quickly, uh, why do we

512
00:22:27.780 --> 00:22:30.580
explore space? Why explore the universe, uh,

513
00:22:30.580 --> 00:22:33.180
when there's so much on Earth that's left to

514
00:22:33.180 --> 00:22:36.100
understand? Uh, and I guess we. One way

515
00:22:36.100 --> 00:22:39.060
of. There's many, many, many reasons why. And

516
00:22:39.060 --> 00:22:41.620
it's principally governments that support the

517
00:22:41.620 --> 00:22:44.300
exploration of space, certainly by

518
00:22:44.300 --> 00:22:47.060
astronomers, and um, to some extent the

519
00:22:47.060 --> 00:22:49.660
exploration of space by space probes as well.

520
00:22:49.820 --> 00:22:51.660
Although there's a, certainly, uh, a

521
00:22:52.140 --> 00:22:54.520
commercial sector moving into that, uh,

522
00:22:54.520 --> 00:22:56.420
trying to send spacecraft to the moon and

523
00:22:56.420 --> 00:22:58.880
things of that sort. But why do we do it? Um,

524
00:22:58.880 --> 00:23:00.940
well, we wouldn't be able to understand Earth

525
00:23:00.940 --> 00:23:02.940
fully if we didn't know about space.

526
00:23:03.680 --> 00:23:06.630
Um, so, uh, the two are

527
00:23:06.630 --> 00:23:08.390
really part and parcel of the same thing.

528
00:23:08.390 --> 00:23:11.270
It's trying to understand our environment on

529
00:23:11.270 --> 00:23:13.150
the biggest possible scale.

530
00:23:13.840 --> 00:23:16.750
Uh, and you know, uh, if you

531
00:23:16.750 --> 00:23:19.630
didn't, um, understand how planets form,

532
00:23:20.430 --> 00:23:23.350
then it wouldn't really tell you, um, how the

533
00:23:23.350 --> 00:23:25.870
Earth has formed. Uh, and that's an important

534
00:23:25.950 --> 00:23:28.670
part of the Earth's history. So that's.

535
00:23:29.150 --> 00:23:31.350
And of course the other thing is that we as a

536
00:23:31.350 --> 00:23:34.150
species are curious we want to know about

537
00:23:34.150 --> 00:23:35.950
our environment in space, we want to know

538
00:23:35.950 --> 00:23:37.990
about the origin of space, we want to know

539
00:23:37.990 --> 00:23:39.910
about where everything came from. It's

540
00:23:39.910 --> 00:23:42.790
fundamental science that may not have an

541
00:23:42.790 --> 00:23:45.470
immediate commercial benefit, but it

542
00:23:45.470 --> 00:23:48.290
tells us about ourselves, uh,

543
00:23:48.350 --> 00:23:49.450
and um,

544
00:23:51.950 --> 00:23:54.190
satisfies our uh, curiosity,

545
00:23:54.670 --> 00:23:57.650
our yearning to understand uh,

546
00:23:57.650 --> 00:23:59.950
the scale of space and

547
00:24:00.580 --> 00:24:03.420
how it all works. That's the, I

548
00:24:03.420 --> 00:24:05.700
guess the fundamental reason for doing it.

549
00:24:05.700 --> 00:24:07.700
But there are many other reasons.

550
00:24:08.820 --> 00:24:11.100
One uh, reason why governments invest in

551
00:24:11.100 --> 00:24:13.700
space and astronomy is to

552
00:24:13.700 --> 00:24:15.460
inspire upcoming generations

553
00:24:16.420 --> 00:24:19.140
because we know that there's nothing like

554
00:24:19.860 --> 00:24:22.820
black holes or killer asteroids or whatever

555
00:24:22.820 --> 00:24:25.660
for getting kids switched on to science.

556
00:24:25.660 --> 00:24:27.540
And it's a great way. Even if they don't

557
00:24:27.540 --> 00:24:30.100
become astronomers or space scientists, they

558
00:24:30.100 --> 00:24:31.930
at least understand the scientific methods.

559
00:24:32.160 --> 00:24:34.400
They understand the evidence based method

560
00:24:34.720 --> 00:24:37.640
that is fundamental to all signs. Um, and

561
00:24:37.640 --> 00:24:40.600
so that's another reason we've got of course

562
00:24:40.600 --> 00:24:43.300
spin offs, we've got all kinds of uh,

563
00:24:43.520 --> 00:24:46.080
things. There are three different things

564
00:24:46.080 --> 00:24:48.840
inside this mobile phone that I'm holding up

565
00:24:48.840 --> 00:24:51.360
for those of you who don't have, don't have

566
00:24:51.440 --> 00:24:54.430
YouTube Music version of this podcast. Uh,

567
00:24:54.560 --> 00:24:57.040
three things of that that came from astronomy

568
00:24:57.200 --> 00:25:00.120
and understanding physics. Uh, you know

569
00:25:00.120 --> 00:25:02.160
the GPS system relies on general

570
00:25:02.480 --> 00:25:04.380
relativity which was test by

571
00:25:04.860 --> 00:25:07.500
astronomical observations. The camera in it

572
00:25:07.820 --> 00:25:09.830
was essentially um,

573
00:25:10.310 --> 00:25:13.180
uh, evolved from cameras that were

574
00:25:13.180 --> 00:25:15.010
developed from uh,

575
00:25:15.820 --> 00:25:18.220
astronomical cameras that we were bringing

576
00:25:18.460 --> 00:25:21.180
to fruition in the 1980s. These

577
00:25:21.420 --> 00:25:24.220
silicon devices that let us see very faint

578
00:25:24.220 --> 00:25:26.900
light levels and WI fi, the WI fi, uh,

579
00:25:27.020 --> 00:25:29.820
that um, lets us use our phones actually

580
00:25:29.900 --> 00:25:32.500
started off in the head of an astrophysicist

581
00:25:32.500 --> 00:25:35.230
working in radio astronomy. How do you send

582
00:25:35.230 --> 00:25:37.470
signals backwards and forwards in your

583
00:25:37.470 --> 00:25:39.190
laboratories? And he was an Australian. Well

584
00:25:39.190 --> 00:25:41.390
he still is. His name is John o' Sullivan and

585
00:25:41.390 --> 00:25:43.390
I've had a number of

586
00:25:44.270 --> 00:25:47.090
pleasant chats with him over the years. Uh,

587
00:25:47.090 --> 00:25:49.990
very well known astrophysicist. So um,

588
00:25:49.990 --> 00:25:52.630
lots of reasons why we do space, uh,

589
00:25:52.670 --> 00:25:55.670
not just because we are curious

590
00:25:55.670 --> 00:25:57.470
about it, but that's the main

591
00:25:58.510 --> 00:25:59.790
underlying reason.

592
00:26:01.230 --> 00:26:03.230
Heidi Campo: Fred, what got you interested in space?

593
00:26:04.110 --> 00:26:05.790
Why did you choose this as a career?

594
00:26:06.670 --> 00:26:09.550
Professor Fred Watson: Yeah, look, in

595
00:26:09.550 --> 00:26:12.230
a sense, um, I'm a product of exactly what

596
00:26:12.230 --> 00:26:14.760
I've just been talking about. Um,

597
00:26:15.270 --> 00:26:17.630
ah, although things were a little bit

598
00:26:17.630 --> 00:26:20.470
different when I was a youngster because I

599
00:26:20.470 --> 00:26:23.310
was at school in the late 1950s, early 1960s

600
00:26:23.310 --> 00:26:26.240
at the dawn of the space age. Uh, so

601
00:26:26.240 --> 00:26:28.880
it was in our faces all the time. Uh,

602
00:26:28.920 --> 00:26:31.760
and plus the fact that there had

603
00:26:31.760 --> 00:26:34.320
recently been a world war and a lot of people

604
00:26:34.320 --> 00:26:35.640
thought there was going to be another one

605
00:26:35.640 --> 00:26:37.200
which will be fought on the grounds of

606
00:26:37.200 --> 00:26:39.560
Science. So science was

607
00:26:39.960 --> 00:26:42.960
absolutely hammered into us. Um, the school

608
00:26:42.960 --> 00:26:45.560
I was at had four streams.

609
00:26:45.720 --> 00:26:47.920
Uh, three of them were science streams, one

610
00:26:47.920 --> 00:26:50.840
was an art stream. And that is not the case

611
00:26:50.840 --> 00:26:53.640
now. Um, so, um, in a sense

612
00:26:53.640 --> 00:26:55.870
I was a product of my time. But

613
00:26:56.510 --> 00:26:58.990
I was inspired, um, by,

614
00:26:59.500 --> 00:27:02.030
uh, in fact, an astronomer who. I was only

615
00:27:02.030 --> 00:27:04.310
thinking about him this morning. Sadly now no

616
00:27:04.310 --> 00:27:06.510
longer with us, a gentleman by the name of

617
00:27:06.510 --> 00:27:09.150
Patrick Moore, who, uh, was

618
00:27:10.030 --> 00:27:12.910
the most famous astronomer in Britain for

619
00:27:13.390 --> 00:27:16.270
40, maybe even 50 years. He

620
00:27:16.270 --> 00:27:18.870
had a TV program which, uh, started in

621
00:27:18.870 --> 00:27:21.110
1957. It's still running. He's not in

622
00:27:21.110 --> 00:27:23.630
Britain. Does it anymore. Uh, the sky at

623
00:27:23.630 --> 00:27:26.150
night. So the sky at night was one of the

624
00:27:26.150 --> 00:27:28.350
things that inspired me and got me interested

625
00:27:28.350 --> 00:27:31.230
in space. And I never really grew up. I

626
00:27:31.230 --> 00:27:33.630
just, um, carried on being interested and

627
00:27:33.630 --> 00:27:35.110
have been all my life. So.

628
00:27:35.350 --> 00:27:38.310
Heidi Campo: So I love that. That's a really fun story.

629
00:27:40.310 --> 00:27:43.070
Professor Fred Watson: Yes. You know, I, I just

630
00:27:43.070 --> 00:27:45.830
feel very fortunate to have had

631
00:27:45.910 --> 00:27:48.800
a job throughout my life that I probably

632
00:27:48.800 --> 00:27:51.320
would have done even if they hadn't paid me

633
00:27:51.320 --> 00:27:53.760
for it because it was my passion.

634
00:27:54.080 --> 00:27:56.160
Not sure how I would have lived had that been

635
00:27:56.160 --> 00:27:57.680
the case. But anyway.

636
00:27:57.680 --> 00:27:58.400
Heidi Campo: That's wonderful.

637
00:27:58.400 --> 00:27:59.120
Professor Fred Watson: It's been great.

638
00:27:59.200 --> 00:28:02.080
Heidi Campo: Well, on, um, that positive note, um, keep,

639
00:28:02.080 --> 00:28:04.120
keep dreaming, everyone. Keep looking at the

640
00:28:04.120 --> 00:28:06.720
stars and keep sending us your questions.

641
00:28:07.200 --> 00:28:09.080
Especially if you're one of our female

642
00:28:09.080 --> 00:28:11.320
listeners. I have been here all summer and we

643
00:28:11.320 --> 00:28:13.680
have not gotten one question from the ladies.

644
00:28:13.840 --> 00:28:16.720
So if you're a female listener and you

645
00:28:16.720 --> 00:28:19.440
have been wondering if your question's good

646
00:28:19.440 --> 00:28:21.080
enough. It's good enough. Just send it in.

647
00:28:21.960 --> 00:28:24.400
We, um, love our fellas, but if there are, I

648
00:28:24.400 --> 00:28:26.000
mean, we've got to have female listeners.

649
00:28:26.000 --> 00:28:28.440
This can't be 100% guys who are interested in

650
00:28:28.440 --> 00:28:31.360
space. Uh, so send in your questions. We

651
00:28:31.360 --> 00:28:34.040
want to hear from you. Fred, do you have any

652
00:28:34.040 --> 00:28:35.000
closing remarks?

653
00:28:35.880 --> 00:28:38.840
Professor Fred Watson: No, just to, to say, uh, absolutely, I agree

654
00:28:38.840 --> 00:28:40.680
with that. We do know we've, we've got some

655
00:28:40.680 --> 00:28:42.720
female listeners. We've occasionally had

656
00:28:42.720 --> 00:28:45.580
questions in the past. We have, uh,

657
00:28:45.760 --> 00:28:48.160
one, uh, person who is a pilot.

658
00:28:48.560 --> 00:28:50.800
She flies across the Atlantic and looks at

659
00:28:50.800 --> 00:28:53.080
the stars and sends us notes, uh, about what

660
00:28:53.080 --> 00:28:53.600
she see.

661
00:28:53.840 --> 00:28:55.840
Heidi Campo: That's such a beautiful picture.

662
00:28:56.800 --> 00:28:59.640
Professor Fred Watson: Yeah, isn't it great? And so, uh, yeah, I

663
00:28:59.640 --> 00:29:02.440
agree we should shout out to our female space

664
00:29:02.440 --> 00:29:04.640
nuts listeners. Get your questions in. We'd

665
00:29:04.640 --> 00:29:06.260
love to hear from you all.

666
00:29:06.260 --> 00:29:08.520
Heidi Campo: Ah, righty then. Well, you heard it from the

667
00:29:08.520 --> 00:29:11.040
man himself. Um, and you probably only

668
00:29:11.200 --> 00:29:13.280
maybe, maybe only a few more weeks with me.

669
00:29:13.280 --> 00:29:15.880
So send in your questions. Um, if you have

670
00:29:15.880 --> 00:29:18.660
any sci fi related questions about favorite

671
00:29:18.660 --> 00:29:21.100
sci fi books and whatnot. Because Andrew is

672
00:29:21.100 --> 00:29:23.660
going to be back soon. We're not quite sure

673
00:29:23.660 --> 00:29:26.020
when, but we've got a few more weeks left of

674
00:29:26.020 --> 00:29:28.460
me, and then, um, Andrew will be back as your

675
00:29:28.460 --> 00:29:31.260
host. But till then, you're stuck with me and

676
00:29:31.260 --> 00:29:33.940
I thank you all for listening. Till next

677
00:29:33.940 --> 00:29:35.180
time. See you later.

678
00:29:36.380 --> 00:29:38.540
Generic: You've been listening to the Space Nuts

679
00:29:38.540 --> 00:29:41.100
podcast, available

680
00:29:41.260 --> 00:29:43.170
at Apple podcasts, Spotify,

681
00:29:43.250 --> 00:29:46.010
iHeartRadio, or your favorite podcast

682
00:29:46.010 --> 00:29:47.770
player. You can also stream on

683
00:29:47.770 --> 00:29:50.490
demand at bitesz.com This  has been

684
00:29:50.490 --> 00:29:52.770
another quality podcast production from

685
00:29:52.770 --> 00:29:53.970
bitesz.com
