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<v Speaker 1>Welcome back to another exciting episode of Space Nuts, the

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<v Speaker 1>podcast that is absolutely out of this world. I am

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<v Speaker 1>your host today, Heidi Compo, filling in for the regular

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<v Speaker 1>Andrew Dunkley. And here we have with us Professor Fred Watson,

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<v Speaker 1>astronomer at Large.

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<v Speaker 2>Fifteen shack and guide the Channel ten nine ignition.

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<v Speaker 1>Space Nuts SHY four three two one, space Nurse at

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<v Speaker 1>the NAT recorded fels good. Hi Fred, how are you

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<v Speaker 1>doing today?

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<v Speaker 2>I'm well, thanks handy and lovely to see you again.

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<v Speaker 2>And we have a beautiful sunny morning here in Sydney

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<v Speaker 2>where I'm recording at the moment, you're at the other

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<v Speaker 2>end of the world, at the other end.

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<v Speaker 1>Of the day, Space Center Houston.

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<v Speaker 2>It's evening.

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<v Speaker 1>It's been quite windy here, but the weather's been nice.

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<v Speaker 1>It's been warm, but not too warm. And this is

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<v Speaker 1>going to be this is going to be an I

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<v Speaker 1>think springtime in Houston is always just really fantastic. And

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<v Speaker 1>speaking of this month, I wanted to share with you

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<v Speaker 1>and our other listeners an exciting event that is happening

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<v Speaker 1>here in Space Center Houston. Well, yeah, sorry, it will

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<v Speaker 1>be at Space Center Houston, but it's happening in Houston

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<v Speaker 1>in general. Is the Spaceflight Human Optimization and Performance Summit,

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<v Speaker 1>so that will be happening at the end of the month,

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<v Speaker 1>and they are going to have all kinds of fantastic

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<v Speaker 1>speakers from NASA and other private organizations. They're giving educational

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<v Speaker 1>talks on the effects of spaceflight on the human body.

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<v Speaker 1>And it is such a fantastic opportunity to network, to

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<v Speaker 1>hear from people who are really at the cutting edge

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<v Speaker 1>of science, and to just kind of collaborate with some

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<v Speaker 1>really brilliant people. It's fun to sometimes be in those

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<v Speaker 1>places where you are pretty confident that you're not the

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<v Speaker 1>smartest person in the room.

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<v Speaker 2>I've spent my whole life feeling that, honestly, Well.

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<v Speaker 1>I feel like that sometimes when I'm looking at your

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<v Speaker 1>books and whatnot. So we've got some pretty fun articles

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<v Speaker 1>we're looking at today. We've got some things about stuff

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<v Speaker 1>going on on Mars. There's articles about space junk and

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<v Speaker 1>galaxy models. And I wanted to start this off by

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<v Speaker 1>asking you, Fred, have you ever been to Arizona.

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<v Speaker 2>Oh, yes, quite often, because for a long time the

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<v Speaker 2>center of the world's astronomy instrument development. What's the word

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<v Speaker 2>for it, frost, That's a good word. The center of

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<v Speaker 2>the world's Astronomy Instrument Development THRUST was in Tucson, and

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<v Speaker 2>of course the Kitpeak National Observatory is not very far

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<v Speaker 2>from Tucson, so I spent many many weeks there on

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<v Speaker 2>and off. And the other thing that Tucson's famous for

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<v Speaker 2>in that sense of the two of course are absolutely interlieved,

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<v Speaker 2>is that's where the basically the dark Sky movement started,

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<v Speaker 2>the idea that we can do something about light pollution,

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<v Speaker 2>because it was at that time the impact was mostly

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<v Speaker 2>on astronomers. But we now know that it's not just

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<v Speaker 2>astronomers who were impacted by bad light and light pollution,

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<v Speaker 2>it's the whole natural world and indeed ourselves. So that

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<v Speaker 2>has moved on since the early nineteen eighties when it

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<v Speaker 2>all got going in Tucson, Arizona. And yes, while I

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<v Speaker 2>was in TUCSONA I explored most of the rest of

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<v Speaker 2>Arizona's squat excellent.

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<v Speaker 1>Well, yeah, that's good. We're kind of building on what

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<v Speaker 1>we talked about last week with the pollution. But I

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<v Speaker 1>was going to say, if you've been to Arizona, well,

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<v Speaker 1>I guess in Sydney, Australia too. You've definitely seen some

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<v Speaker 1>dust storms.

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<v Speaker 2>Right, yeah, yeah, that's right, and absolutely I know where

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<v Speaker 2>this is going.

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<v Speaker 1>Do you get haboobs in Australia at all? You know?

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<v Speaker 2>Is that the name for what we call dust devils?

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<v Speaker 1>Oh, so the haboobs are the really really big ones.

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<v Speaker 1>I was living in Arizona. If you guys want to

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<v Speaker 1>google the twenty ten haboob in Arizona haboob. It's very

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<v Speaker 1>phonetic huboob. I believe or ha that it is a

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<v Speaker 1>Middle Eastern word because these normally happen in the Middle

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<v Speaker 1>East and with things like you've seen the movie Hill

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<v Speaker 1>Dalgo with the horse horses running things like that. So

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<v Speaker 1>if you see the twenty ten haboo Arizona pictures you'll

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<v Speaker 1>see what I'm talking about. Quite crazy, but yeah, dust

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<v Speaker 1>is something that you're going to be familiar with in

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<v Speaker 1>places like Australia and Arizona, but people may not be

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<v Speaker 1>as familiar with some of the dust storms on Mars,

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<v Speaker 1>which you're so smart. That's exactly where we were going

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<v Speaker 1>is they did see some dust devil activity on Mars,

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<v Speaker 1>and I think that's kind of cool and exciting. Can

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<v Speaker 1>you tell us a little bit about going out of that?

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<v Speaker 2>And it's for the this is a a topic I

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<v Speaker 2>really love, and it's because you've put your finger on it.

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<v Speaker 2>This is something we're familiar with here, not in Sydney certainly,

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<v Speaker 2>but in the western plains of New South Wales, and

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<v Speaker 2>I lived in that region for twenty five years. It

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<v Speaker 2>was very common to see these pillars of dust. Is

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<v Speaker 2>that what you mean by a haboob? Is it very much?

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<v Speaker 1>You know?

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<v Speaker 2>How does it relate to a tornado?

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<v Speaker 1>Bubes are much more extreme. It's an extreme dust storm

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<v Speaker 1>that's more like a wall of sand or by area.

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<v Speaker 1>So if you think of interstellar with the wave of water,

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<v Speaker 1>it's like that, but with sand.

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<v Speaker 2>We get that in Australia too, whether you know, the

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<v Speaker 2>top soil will blow off in one region and you

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<v Speaker 2>will literally get a wall of dust, brown dust, which

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<v Speaker 2>sometimes gives rise to the most spect tacular photographs. And

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<v Speaker 2>if the dust, you know, penetrates far enough, it does

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<v Speaker 2>actually reach the coast. There have been occasions of that

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<v Speaker 2>sort of dust storm in Sydney. The the whole color

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<v Speaker 2>of the landscape changes, not just because it's covered in dust,

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<v Speaker 2>but because the atmosphere filters out you know, all the

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<v Speaker 2>all the the blue light and you get this reddish

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<v Speaker 2>ethereal glow, which is in many ways etherea is probably

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<v Speaker 2>the wrong word. It's it's actually almost apocalyptic. It feels,

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<v Speaker 2>you know, that that you've got this wall of dust

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<v Speaker 2>and the colors afterwards, the cover of the peculiar colors.

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<v Speaker 2>But what I was going to talk about today though,

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<v Speaker 2>what are usually known as dust devils, which are quite

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<v Speaker 2>small areas of dust, and it's where you get a

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<v Speaker 2>little whirlwind that picks up a column of dust and

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<v Speaker 2>moves along the landscape. So you see these moving columns

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<v Speaker 2>of basically dust. Sometimes there's bits of debris being circulated around.

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<v Speaker 2>It's not a tornado, but it's you know, the sort

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<v Speaker 2>of perhaps the poor relative of a tornado. We do

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<v Speaker 2>get them in western New South Wales, and I've seen

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<v Speaker 2>a lot there, but I was surprised. It goes back

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<v Speaker 2>actually this story to probably about two thousand and three

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<v Speaker 2>or four, in the early days of the new generation

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<v Speaker 2>of Mars rovers. Spirit and Opportunity were the two that

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<v Speaker 2>really sort of put Mars rovers on the map. There

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<v Speaker 2>were other ones before that, but Spirit and Opportunity gave

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<v Speaker 2>us some stunning images of the planet's surface, and among

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<v Speaker 2>them were images from Spirit I think taken from the

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<v Speaker 2>top of a mountain range which was basically on the

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<v Speaker 2>edge of a crater. Actually it might have been Curiosity,

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<v Speaker 2>and I should have checked that. No, I think it's

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<v Speaker 2>Spirit Crater. I think it was its name if I

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<v Speaker 2>remember rightly, lovely images across the crater with a little

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<v Speaker 2>movie clips of these dust devils going across it, which

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<v Speaker 2>are relatively common on Mars, it turns out, and in

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<v Speaker 2>fact they were observed actually by the Viking orbiter back

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<v Speaker 2>in nineteen seventy six, so the spacecraft happened to be

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<v Speaker 2>looking down at a region where one of these was happening.

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<v Speaker 2>They're different from earthly ones in first of all, in

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<v Speaker 2>the sense that because the atmosphere on Mars is so dry,

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<v Speaker 2>it's virtually zero humidity, that means that static electricity can

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<v Speaker 2>build up, and so you often get flashes of lightning

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<v Speaker 2>in the base of Martian dust devils, and yeah, little

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<v Speaker 2>sparks of lightning caused by the static electricity build up.

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<v Speaker 2>And the other thing is they're much taller than the

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<v Speaker 2>ones we find here on Earth. The biggest one I

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<v Speaker 2>ever saw in South Wales here in Australia probably had

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<v Speaker 2>a height of about five hundred meters half a kilometer,

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<v Speaker 2>so what's that sort of you know, about about the

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<v Speaker 2>third of a mile basically, and that's you know, that

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<v Speaker 2>was pretty significant. On Mars they get up to eight kilometers,

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<v Speaker 2>which is like five miles, and I guess that's partly

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<v Speaker 2>due to the fact that the dust is very, very fine,

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<v Speaker 2>and also the fact that Mars of course only has

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<v Speaker 2>a third of the gravity that we have here on

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<v Speaker 2>planet Earth and just a quicker side. They're technically known

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<v Speaker 2>as dust devils. I think that's the correct term. It's

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<v Speaker 2>different from a haboob. A harboob's a wall of dust,

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<v Speaker 2>and that's something we also get. But in most of

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<v Speaker 2>Australia they have a first nation's name and aboriginal name.

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<v Speaker 2>They're called willy willies, and a willy Willie is a

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<v Speaker 2>little dust storm that going past on the horizon. One

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<v Speaker 2>of the little factoid about the Martian ones in particular

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<v Speaker 2>is that with both spirit and opportunity, which relied for

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<v Speaker 2>their power on solar panels, unlike curiosity and perseverance, which

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<v Speaker 2>have got thermoelectric nuclear generators, the dust panel, sorry, the

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<v Speaker 2>solar panels tended to get just covered by dust that is,

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<v Speaker 2>you know, present on Mars. Mars is a very very

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<v Speaker 2>dusty planet. So as you as you roam around the surface,

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<v Speaker 2>you're kicking up dust with the space with the rovers wheels,

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<v Speaker 2>and that dust eventually lands on the solar panels. I'm

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<v Speaker 2>going to have to clear my throat. Excuse me one minute, Yeah, yeah,

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<v Speaker 2>there we go. I hope that. Oh, I don't think.

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<v Speaker 2>I don't think I muted that.

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<v Speaker 1>That's okay, we can edit that out.

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<v Speaker 2>That was meant to be muted out, and I'm sorry

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<v Speaker 2>I did. Sorry, Hugh, that probably went right in your ears,

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<v Speaker 2>as I can see from Heidie's face it went in

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<v Speaker 2>hers as well. Just to mention though, that the solar

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<v Speaker 2>panels themselves were cleared unlike my throat by dust devils.

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<v Speaker 2>They were actually cleared when these things passed over and

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<v Speaker 2>swept the dust off the solar panels. So Curiosity in particular,

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<v Speaker 2>which was in a sorry opportunity, was in a dusty

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<v Speaker 2>place that kept you know, the power kept dropping and

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<v Speaker 2>kept reappearing again because of these dust devils.

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<v Speaker 1>Quite quite extraordinary, and that's definitely going to be a

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<v Speaker 1>concern when we're trying to, you know, get humanity to

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<v Speaker 1>set up a colony on this planet. I'm just thinking

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<v Speaker 1>of the movie The Martian, as cliche as it is,

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<v Speaker 1>that was the big problem that got him stuck there

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<v Speaker 1>to begin with, was that big dust storm. So I

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<v Speaker 1>guess that was a bit scientifically accurate when they put

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<v Speaker 1>that into that movie.

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<v Speaker 2>And that's right, the dust storm was we now know

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<v Speaker 2>Martian dust is. It's toxic as well, in the sense

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<v Speaker 2>that it gets into your lungs. It does quite a

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<v Speaker 2>lot of damage. So in my view, not a place

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<v Speaker 2>to colonize, but that's my view.

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<v Speaker 1>Is the dust similar to the moon regolith, where it's

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<v Speaker 1>also kind of sticky?

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<v Speaker 2>Yeah, I think it's a bit like that, and probably

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<v Speaker 2>for the same sort of reason. Mars has such a

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<v Speaker 2>thin atmosphere that the erosion processes. Originally, erosion took place

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<v Speaker 2>with wind and water like like it did here on

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<v Speaker 2>Earth because of the fact that Mars had a warm

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<v Speaker 2>and wet climate. The thinness of the atmosphere means that

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<v Speaker 2>you've got a much higher level of bombardment by subatomic

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<v Speaker 2>particles from the Sun, and that's what gives you the sharp,

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<v Speaker 2>pointy edges of dust particles on the Moon. Now the

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<v Speaker 2>Moon's nearer to the Sun than Mars is, but I

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<v Speaker 2>think still the mechanism occurs that you've got bombardment, which

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<v Speaker 2>which actually further further breaks down the further breaks down

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<v Speaker 2>the dust.

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<v Speaker 1>Well, if if we do end up going to Mars

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<v Speaker 1>and we are successful with our endeavors there, we can

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<v Speaker 1>fill Twister three with Glenn Powell doing some twisters on Mars.

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<v Speaker 2>Space nuts to.

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<v Speaker 1>Get through the atmosphere. It seems like there is just

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<v Speaker 1>more and more issues with their atmosphere and all the

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<v Speaker 1>space trunk that's up there. And I even just saw

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<v Speaker 1>on I don't know if it was Prime or Netflix,

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<v Speaker 1>whatever streaming service I was on the other night, there's

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<v Speaker 1>a movie. There's a there's a movie out about space junk,

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<v Speaker 1>and in this sci fi movie they have people who

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<v Speaker 1>work in orbit constantly clearing space debris. But that might

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<v Speaker 1>not be something that's even a worry because it looks

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<v Speaker 1>like there's a new technology that can help us with

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<v Speaker 1>some of the space debris and junk. Can our orbit.

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<v Speaker 2>Absolutely, I mean, this is one of the major problems

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<v Speaker 2>of our era, the potential for space chunk. It's the

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<v Speaker 2>space junk already exists. There's a lot of stuff up

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<v Speaker 2>there that is now redundant and quite harmful, given that

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<v Speaker 2>the minimal orbital speed that you're going at is about

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<v Speaker 2>eight kilometers per second, about five miles per second, So

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<v Speaker 2>everything is charging around at very high speeds, and as

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<v Speaker 2>you will well know, even a fleck of paint can

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<v Speaker 2>take a chip out of the window of a space shuttle.

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<v Speaker 2>That very well known phenomenon from a few decades ago.

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<v Speaker 2>Actually so at the moment there are just over eleven

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<v Speaker 2>thousand active spacecraft in orbit around the Earth. Most of

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<v Speaker 2>them are Starlink satellites. But when you look at the

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<v Speaker 2>debris that is actually tracked, stuff that is redundant, I

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<v Speaker 2>don't have the exact figure out, but it's well over

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<v Speaker 2>thirty thousand items bigger than four inches sorry for it, yes,

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<v Speaker 2>four inches, one hundred millimeters, ten centimeters. And then when

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<v Speaker 2>you look at smaller stuff, you're in the millions. You're

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<v Speaker 2>really in the millions of bits of debris, and it's

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<v Speaker 2>all damaging. And that the main problem is that as

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<v Speaker 2>soon as you get a collision between two bits of

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<v Speaker 2>this stuff, especially if it's sizable in any way, then

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<v Speaker 2>you will get more debris being created, and that increases

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<v Speaker 2>the risk and that can lead to what's called the

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<v Speaker 2>Kessler syndrome, where everything's crashing into everything else and you

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<v Speaker 2>suddenly lose access to space. So it's a real problem

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<v Speaker 2>and one that needs attention, and indeed is getting attention

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<v Speaker 2>from the world's technologists. I just saw a tail walk

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<v Speaker 2>through the picture there behind.

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<v Speaker 1>You, little dog speaking of little problems. Yes, always on

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<v Speaker 1>the parral. But yeah, I mean this is super interesting

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<v Speaker 1>because it's like every i mean almost every something going

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<v Speaker 1>wrong in space movie starts with this. So it's well

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<v Speaker 1>mel from the scientists down to the creatives. And so

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<v Speaker 1>it looks like this this this what do they call them,

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<v Speaker 1>the bold new weapon against space junk. It looks like

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<v Speaker 1>Percy p e r Sei Space Yep, that's right, is

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<v Speaker 1>a startup that's helping with these issues.

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<v Speaker 2>Yes, that's right. So that there is a backstory to

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<v Speaker 2>this in that there's been several experiments carried out by

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<v Speaker 2>both private companies and things, you know, body bodies like

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<v Speaker 2>the European Space Agency to try and see how you

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<v Speaker 2>could clean up space, and mostly it involves something like well,

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<v Speaker 2>one of them is sending up a spacecraft that centrally

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<v Speaker 2>rendevus with a satellite that's now redundant, whether it's a

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<v Speaker 2>rocket body or you know, a communication satellite, something that

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<v Speaker 2>switched off and is now dead. But he's a risk

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<v Speaker 2>because it's up there. And if you can then put

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<v Speaker 2>it through a grappling iron at it, you know, going

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<v Speaker 2>back to the technology that was used in the Middle Ages,

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<v Speaker 2>catch hold of it with your hydraulically propelled grappling iron

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<v Speaker 2>or whatever it is, you then can capture it. And

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<v Speaker 2>if you have a satellite that now has hold of

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<v Speaker 2>this Maverick object, you can basically apply braking rockets and

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<v Speaker 2>make it re enter so that it burns up and

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<v Speaker 2>is no longer a problem for collisions. But that's a

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<v Speaker 2>difficult that's quite a tricky problem and it needs, you know,

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<v Speaker 2>spacecraft equipped with quite large amounts of fuel to do that.

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<v Speaker 2>And so this new idea, the one that you've highlighted

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<v Speaker 2>from perse Iied Space, it's going to be tested actually

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<v Speaker 2>early next year. It's quite counterintuitive and takes it will

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<v Speaker 2>to get your head around how it works. It's called

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<v Speaker 2>an electrodynamic tether. It's a ribbon of aluminium maybe more

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<v Speaker 2>than that one hundreds of meters i e. Hundreds of

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<v Speaker 2>yards long and only a few inches or centimeters wide.

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<v Speaker 2>And what happens is that this thing gets a current

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<v Speaker 2>running up and down it from the plasma in the ionosphere.

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<v Speaker 2>And by that we mean charged particles charge sub atomic particles,

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<v Speaker 2>in other words, sub atomic particles that carry an electric charge,

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<v Speaker 2>so excuse me. So you get an electric current set

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<v Speaker 2>up in the tether, but that then interacts with the

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<v Speaker 2>asthmagnetic field. This is the really cunning bit and puts

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<v Speaker 2>a drag on the tether. It slows it down, it

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<v Speaker 2>starts breaking it. So if the tether is attached to

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<v Speaker 2>in fact, it can be attached to a cube sat.

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<v Speaker 2>They're small enough that you can do that. This is

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<v Speaker 2>the thing of size of a loaf of bread. But

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<v Speaker 2>you then have to attach the cube sat to whatever

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<v Speaker 2>spacecraft you want to whose orbit you want to change.

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<v Speaker 2>You can actually set things up so that you slow

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<v Speaker 2>down the Maverick spacecraft and essentially make it slow enough

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<v Speaker 2>that it will start to re enter the atmosphere and

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<v Speaker 2>be burned up and again got out of the way.

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<v Speaker 2>But this is the really coming bit. If you do

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<v Speaker 2>it in a slightly different way, you can also actually

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<v Speaker 2>push it into a higher orbit so that you can

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<v Speaker 2>refurbish a spacecraft one that has run out of its

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<v Speaker 2>maneuvering fuel, so it can't save itself from being swallowed

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<v Speaker 2>up by the atmosphere anymore. You can shove it up

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<v Speaker 2>to a higher orbits with the same electrodynamic tether and

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<v Speaker 2>give it a new lease of life. It's quite an

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<v Speaker 2>amazing promise. And this is the best bit. All of

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<v Speaker 2>this is free. It comes with no fuel expenditure. It's

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<v Speaker 2>because you're relying on the natural forces that' surround the

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<v Speaker 2>earth in order to do this. It's a very very

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<v Speaker 2>clever argument. The question is will it work.

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<v Speaker 1>Yeah, what you're sounding, what you're saying sounds truly just

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<v Speaker 1>like magic. And I think about that all the time.

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<v Speaker 1>If you were to tell ancient people about even just

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<v Speaker 1>the Internet or a phone, it would have founded like

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<v Speaker 1>magic for them. And oh, I'm talking to somebody around

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<v Speaker 1>the world. They would have thought I was a sorceress.

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<v Speaker 1>And this to me sounds just amazing. It's so cool

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<v Speaker 1>what humans have truly come up with. I mean, humanity,

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<v Speaker 1>I'm so proud of us. Sometimes sometimes I'm not so.

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<v Speaker 1>Sometimes Sometimes I look at what humanity is collectively doing

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<v Speaker 1>and it's just so awe inspiring and I just love

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<v Speaker 1>being around these people who are doing incredible things or

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<v Speaker 1>space nuts. But sometimes we mess it up, and sometimes

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<v Speaker 1>our models and predictions get it wrong, which looks like

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<v Speaker 1>that was the case with some models that they created

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<v Speaker 1>with these galaxies. There are models. Either the models got

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<v Speaker 1>it wrong or the galaxies got it wrong. But our

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<v Speaker 1>predictions is that they were going to continue growing, but

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<v Speaker 1>in reality the galaxies stopped growing sooner than the models predicted.

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<v Speaker 2>That's right. A fascinating story once again comes from I

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<v Speaker 2>guess the post a child of spacecraft at the moment,

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<v Speaker 2>at least for astronomers, the James Webspace Telescope, which has,

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<v Speaker 2>as you know, I think we talked about this a

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<v Speaker 2>week or so ago, has been concentrating on as well

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<v Speaker 2>as many other objects in space, but looking very much

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<v Speaker 2>at very distant galaxies, because that is our probe to

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<v Speaker 2>the early universe. Whenever we look into space, we're always

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<v Speaker 2>looking back in time. We are looking back, in this

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<v Speaker 2>case many many billions of years. We think the universe

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<v Speaker 2>is thirteen point eight billion years old, so nothing can

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<v Speaker 2>look back further than that. We do see something at

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<v Speaker 2>that age, but it's the flash of the Big Bang.

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<v Speaker 2>But those galaxies which came into being we think within

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<v Speaker 2>the first few hundred million years of the Big Bang.

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<v Speaker 2>The Big Bang generated hydrogen. Hydrogen form stars, stars form galaxies,

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<v Speaker 2>and so we basically have been looking for galaxies in

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<v Speaker 2>the early history of the universe kind of to try

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<v Speaker 2>and understand when these first stars occurred and when they

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<v Speaker 2>switched on. And the basically what's happened is we've uncovered

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<v Speaker 2>one after another puzzles, really quite serious puzzles for our

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<v Speaker 2>understanding of how galaxies work. And this new one, it's

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<v Speaker 2>another conundrum comes about because we see galaxies when the

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<v Speaker 2>universe was less than a billion years old, but we

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<v Speaker 2>see galaxies that look as though they should be several

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<v Speaker 2>billion years old, and that's because they've used up all

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<v Speaker 2>their hydrogen in forming forming the stars. Staff galaxies do

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<v Speaker 2>form stars because the hydrogen is the raw material of

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<v Speaker 2>the stars, and certainly our galaxy is actually still forming stars.

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<v Speaker 2>But some we know formed stars used up all their

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<v Speaker 2>hydrogen and became effectively dead galaxies. Now, we thought those

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<v Speaker 2>had to be going for billions of years in order

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<v Speaker 2>to get like that, but several have been found now

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<v Speaker 2>in the early universe, which looks as though they're much

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<v Speaker 2>older than they can be because they've you know, they've

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<v Speaker 2>only existed for a few hundred million few, yes, a

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<v Speaker 2>few hundred million years. There's some really nice nomenclature with this, Heidi,

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<v Speaker 2>because like you know, astronomers tend to light forming nice acronyms.

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<v Speaker 2>And there is a survey called which is called Red

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<v Speaker 2>Unknowns Bright Infrared Extra Galactic Survey, which abbreviates to RUBIES,

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<v Speaker 2>and I quite like that abbreviation. So one of these

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<v Speaker 2>galaxies is called Rubies udsqg Z seven. That's you know,

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<v Speaker 2>a nice yeah, just encapsulates everything about it. I guess

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<v Speaker 2>the Rubies is echoing what these galaxies look like. Galaxies

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<v Speaker 2>look like. They're redder than the star forming galaxies which

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<v Speaker 2>tendency who have the tendency to be blue. So another

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<v Speaker 2>puzzle in the early universe which we have to get

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<v Speaker 2>our heads around in order to understand really what's going

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<v Speaker 2>on in that distant era of our past.

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<v Speaker 1>Do you think and I almost like, you know, it's

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<v Speaker 1>almost scary to think this, but do you think that

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<v Speaker 1>we could discover so much in space with James Web

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<v Speaker 1>and looking deeper and deeper that it challenges everything that

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<v Speaker 1>we already know about the Solar System and sorry, the universe.

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<v Speaker 2>It's almost like that already. It's the Web telescope has

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<v Speaker 2>really caused a lot of heads scratching in terms of

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<v Speaker 2>how you make these observations fit with our models of

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<v Speaker 2>what the early universe was like. Some people and a

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<v Speaker 2>few of our question you know, when we've had Q

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<v Speaker 2>and A sessions in Space Notes, we occasionally get questions

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00:25:14.559 --> 00:25:17.799
<v Speaker 2>from listeners who've heard this sort of thing and say, well,

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<v Speaker 2>there's something wrong here because some of these galaxies must

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<v Speaker 2>have been formed before the Big Bang, and that can't

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<v Speaker 2>happen because there was nothing before the Big Bang, not

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<v Speaker 2>even space probably, And so what we're talking about is

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<v Speaker 2>not a conundrum that says, yes, we're seeing galaxies that

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<v Speaker 2>are too old for the universe. The conundrum is galaxies

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<v Speaker 2>evolved much more quickly than we expected them to. They

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<v Speaker 2>come into being, and as we've seen here, some of

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<v Speaker 2>them are almost enter old age when they're only a

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<v Speaker 2>few one hundred million years old, and that flies in

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<v Speaker 2>the face of conventional wisdom. It means that our models

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<v Speaker 2>of galaxy, for which we thought we had sort of

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<v Speaker 2>fairly well neat and tidied up or neatly and tidied up.

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<v Speaker 2>That didn't make sense either anyway. You know what I'm

419
00:26:09.200 --> 00:26:12.440
<v Speaker 2>trying to say. We thought we'd we thought we'd understood them,

420
00:26:13.079 --> 00:26:15.640
<v Speaker 2>and clearly we don't. There are gaps in our knowledge

421
00:26:15.680 --> 00:26:18.640
<v Speaker 2>that the James Webb Telescope is uncovering almost every day,

422
00:26:18.880 --> 00:26:22.519
<v Speaker 2>and it's a very stimulating time for astronomy and particularly

423
00:26:22.599 --> 00:26:25.039
<v Speaker 2>those theoretical astronomers who've got to get their head around

424
00:26:25.119 --> 00:26:27.079
<v Speaker 2>why it's like this and how this all works.

425
00:26:27.799 --> 00:26:30.720
<v Speaker 1>Ask me. Every semester of grad school, I finish up

426
00:26:30.720 --> 00:26:33.079
<v Speaker 1>the semester, I'm like, okay, finals, Well, I feel like

427
00:26:33.160 --> 00:26:36.240
<v Speaker 1>I know what I'm doing. Next semester should be a cakewalk.

428
00:26:36.440 --> 00:26:38.279
<v Speaker 1>And then I walk into next semester and I was like,

429
00:26:38.359 --> 00:26:42.240
<v Speaker 1>oh this is I feel completely inadequate again. And I

430
00:26:42.319 --> 00:26:47.519
<v Speaker 1>don't understand any of this, but I do. Astronomers and

431
00:26:47.720 --> 00:26:53.160
<v Speaker 1>cosmologists ever talk about the multiverse theory and how I

432
00:26:53.240 --> 00:26:58.240
<v Speaker 1>don't know if there could be you know, galaxies clashing

433
00:26:58.400 --> 00:27:04.359
<v Speaker 1>and colliding from other universes and the big bang of

434
00:27:04.559 --> 00:27:08.200
<v Speaker 1>our universe is timed differently than others. Is that something

435
00:27:08.279 --> 00:27:09.319
<v Speaker 1>that's been tossed around.

436
00:27:10.240 --> 00:27:15.279
<v Speaker 2>Yeah, there's a huge amount of activity in the what

437
00:27:15.440 --> 00:27:21.240
<v Speaker 2>you might call the the speculative sphere about the multiverse,

438
00:27:22.039 --> 00:27:27.599
<v Speaker 2>if I remember rightly, the term was coined by Martin Reece,

439
00:27:28.160 --> 00:27:33.079
<v Speaker 2>now Lord Reece, who's the astronomer oroyl in Britain, the

440
00:27:33.119 --> 00:27:35.839
<v Speaker 2>Astronomer Royal, I think, was the first person to point

441
00:27:35.920 --> 00:27:40.200
<v Speaker 2>out that the universe that we see around us is

442
00:27:40.440 --> 00:27:44.640
<v Speaker 2>very well tuned for things like stars and planets to form,

443
00:27:44.759 --> 00:27:47.960
<v Speaker 2>for galaxies to form, and for life to form, and

444
00:27:48.119 --> 00:27:51.759
<v Speaker 2>that you only have to change the fundamental consonants of

445
00:27:51.839 --> 00:27:54.240
<v Speaker 2>the universe a tiny bit either way and none of

446
00:27:54.319 --> 00:27:57.079
<v Speaker 2>that happens. And I think that was what led to

447
00:27:57.160 --> 00:28:01.160
<v Speaker 2>the idea that maybe our universe is just one of

448
00:28:01.359 --> 00:28:08.359
<v Speaker 2>many which have different physical constants, and we happen to

449
00:28:08.480 --> 00:28:11.359
<v Speaker 2>be the one that has the physical constants that allow

450
00:28:11.480 --> 00:28:14.359
<v Speaker 2>life to happen, which is, you know, it's kind of

451
00:28:14.519 --> 00:28:18.000
<v Speaker 2>self fulfilling almost. We're not in one of the other

452
00:28:18.079 --> 00:28:21.920
<v Speaker 2>ones because life wouldn't happen there. So that was the

453
00:28:22.039 --> 00:28:25.519
<v Speaker 2>start of it. There's been other ideas that speculate about

454
00:28:26.960 --> 00:28:29.720
<v Speaker 2>multiple universes, one of them and really neat one. Actually,

455
00:28:30.240 --> 00:28:34.240
<v Speaker 2>you may know, there's four fundamental forces in nature. There

456
00:28:34.319 --> 00:28:38.200
<v Speaker 2>strong and weak nuclear forces, the electromagnetic force, which is

457
00:28:38.319 --> 00:28:43.279
<v Speaker 2>light and radio and gravity. But gravity is hundreds of

458
00:28:43.440 --> 00:28:46.880
<v Speaker 2>it's actually billions upon billions upon billions upon billions of

459
00:28:47.000 --> 00:28:51.640
<v Speaker 2>times fainter, sorry, weaker than the other ones. It's not fainter,

460
00:28:51.759 --> 00:28:54.880
<v Speaker 2>it's weaker. So gravity is very very weak, even though

461
00:28:55.000 --> 00:28:57.519
<v Speaker 2>we feel it quite you know, noticeably if we fall

462
00:28:57.599 --> 00:29:00.440
<v Speaker 2>over and get pulled out to Earth with the bang.

463
00:29:01.119 --> 00:29:03.000
<v Speaker 2>But so gravity is very weak, and some people have

464
00:29:03.079 --> 00:29:06.359
<v Speaker 2>speculated that that might be because gravity leaks out into

465
00:29:06.440 --> 00:29:09.759
<v Speaker 2>other universes if we've got a multiverse. The problem is,

466
00:29:10.319 --> 00:29:12.680
<v Speaker 2>I mean, the word universe itself means all that we

467
00:29:12.759 --> 00:29:16.960
<v Speaker 2>can ever see or detect or measure, and as soon

468
00:29:17.000 --> 00:29:20.079
<v Speaker 2>as you start talking about other universes, you've thrown that

469
00:29:20.200 --> 00:29:23.559
<v Speaker 2>definition away, and it's hard to see where they would

470
00:29:23.640 --> 00:29:28.039
<v Speaker 2>exist unless there are higher dimensions that we do not

471
00:29:28.240 --> 00:29:31.759
<v Speaker 2>yet understand, and we might have, you know, a fifth

472
00:29:31.920 --> 00:29:36.119
<v Speaker 2>or a sixth or a twentieth dimension which contains other universes,

473
00:29:36.160 --> 00:29:38.400
<v Speaker 2>and then you have the idea of a multiverse. What's

474
00:29:38.519 --> 00:29:41.480
<v Speaker 2>difficult to see is how a galaxy from one of

475
00:29:41.519 --> 00:29:45.920
<v Speaker 2>those could stray into our universe, because otherwise it becomes

476
00:29:46.240 --> 00:29:49.000
<v Speaker 2>part of the universe and probably would have formed with

477
00:29:49.920 --> 00:29:54.680
<v Speaker 2>you know, with our universe and our galaxies. The one

478
00:29:54.759 --> 00:29:58.880
<v Speaker 2>thing that people point to as an observational tool is

479
00:29:59.000 --> 00:30:02.759
<v Speaker 2>this my co wave background, this background of radiation that

480
00:30:02.839 --> 00:30:05.519
<v Speaker 2>we see and understand as being the flash of the

481
00:30:05.559 --> 00:30:08.160
<v Speaker 2>Big Bang, that we're seeing so far in look back

482
00:30:08.279 --> 00:30:10.240
<v Speaker 2>time that we can still see it because that has

483
00:30:10.279 --> 00:30:13.839
<v Speaker 2>a pattern imprinted on it, which are hot, slightly warmer,

484
00:30:13.880 --> 00:30:17.200
<v Speaker 2>and cooler zones of temperature. And some people think they

485
00:30:17.240 --> 00:30:19.680
<v Speaker 2>can see patterns in that that they think might have

486
00:30:19.839 --> 00:30:23.759
<v Speaker 2>come from a different universe. But that is very very speculative,

487
00:30:24.319 --> 00:30:25.279
<v Speaker 2>very speculative.

488
00:30:25.319 --> 00:30:29.640
<v Speaker 1>Indeed, that's more of the mathematicians' realm is to go

489
00:30:29.759 --> 00:30:32.440
<v Speaker 1>in to find some of these things mathematically before we

490
00:30:32.519 --> 00:30:36.359
<v Speaker 1>can even really define it theoretically, and then you know,

491
00:30:36.720 --> 00:30:39.960
<v Speaker 1>maybe a thousand years from now will have the technology

492
00:30:40.079 --> 00:30:44.880
<v Speaker 1>to better understand this. But in the meantime, I guess

493
00:30:44.960 --> 00:30:47.599
<v Speaker 1>the only way that I think this could theoretically make sense,

494
00:30:47.680 --> 00:30:51.039
<v Speaker 1>and this is just fun little brain candy, is you

495
00:30:51.119 --> 00:30:55.960
<v Speaker 1>know my pencil leaves behind it's in three D. My

496
00:30:56.079 --> 00:30:58.599
<v Speaker 1>three dimensional pencil leaves behind its mark on a piece

497
00:30:58.599 --> 00:31:02.440
<v Speaker 1>of paper. That's only because the lead is that crossover

498
00:31:02.759 --> 00:31:06.160
<v Speaker 1>and so there could be I don't know, crossover bits

499
00:31:06.279 --> 00:31:10.559
<v Speaker 1>of matter that can bleed in two different dimensions.

500
00:31:10.839 --> 00:31:13.680
<v Speaker 2>Yeah. The nice thing about your analogy is that you're

501
00:31:13.720 --> 00:31:16.359
<v Speaker 2>quite right. Your pencil is it's not a pencil, but

502
00:31:16.440 --> 00:31:19.480
<v Speaker 2>it looks a bit like that. It's a three dimensional object.

503
00:31:20.079 --> 00:31:22.920
<v Speaker 2>You're right on paper, which is a two dimensional object.

504
00:31:23.440 --> 00:31:26.759
<v Speaker 2>And so you've got a three dimensional object interacting with

505
00:31:26.839 --> 00:31:31.599
<v Speaker 2>a two dimensional object. And that could be a nice

506
00:31:31.720 --> 00:31:35.839
<v Speaker 2>model for what the you know, what the multiverse is like.

507
00:31:37.720 --> 00:31:41.480
<v Speaker 2>And in fact, it's not too far out. We can

508
00:31:41.640 --> 00:31:44.680
<v Speaker 2>sort of almost extend it as well, because excuse me,

509
00:31:45.759 --> 00:31:47.000
<v Speaker 2>we have a piece of paper.

510
00:31:49.000 --> 00:31:50.960
<v Speaker 1>Oh fantastic, now I'm in the demos.

511
00:31:51.400 --> 00:31:54.319
<v Speaker 2>Yeah, so I don't know whether anybody else can see this.

512
00:31:54.599 --> 00:31:56.640
<v Speaker 2>If you're listening, I'm sorry about this, but I'm holding

513
00:31:56.680 --> 00:31:59.599
<v Speaker 2>up a sheet of paper. We can all envision a

514
00:31:59.640 --> 00:32:02.000
<v Speaker 2>piece of it actually turns out to be two pieces

515
00:32:02.039 --> 00:32:05.880
<v Speaker 2>of paper. And that's the idea of something called M theory.

516
00:32:06.640 --> 00:32:10.480
<v Speaker 2>M theory is membrane, and so we think one sheet

517
00:32:10.519 --> 00:32:13.880
<v Speaker 2>of paper is a membrane on which our universe is imprinted,

518
00:32:14.640 --> 00:32:17.160
<v Speaker 2>and another sheet of paper might be a membrane with

519
00:32:17.279 --> 00:32:20.240
<v Speaker 2>another universe on it, and the idea is that it's

520
00:32:20.279 --> 00:32:25.039
<v Speaker 2>collisions between these membranes that cause big bangs. This is

521
00:32:25.200 --> 00:32:28.480
<v Speaker 2>known as the ech pyrotic theory of the universe, to

522
00:32:28.559 --> 00:32:32.480
<v Speaker 2>give it a name. What's freaky about that is, if

523
00:32:32.559 --> 00:32:36.559
<v Speaker 2>it's true these membranes are only a few millimeters apart, and.

524
00:32:36.759 --> 00:32:40.160
<v Speaker 1>So things happening all then.

525
00:32:40.200 --> 00:32:43.000
<v Speaker 2>Maybe there are yes. Yes, that's right. So take that

526
00:32:43.079 --> 00:32:47.240
<v Speaker 2>one away and think about it. But what a good analogy? Though?

527
00:32:47.279 --> 00:32:49.279
<v Speaker 2>You did? You did? You hit on the right.

528
00:32:49.559 --> 00:32:51.960
<v Speaker 1>I watch a lot of sci fi. They drain and

529
00:32:52.039 --> 00:32:58.319
<v Speaker 1>dumb it down for their their watchers, their viewers. You know,

530
00:32:58.519 --> 00:33:01.119
<v Speaker 1>I've always thought of this ever since I was a

531
00:33:01.160 --> 00:33:04.400
<v Speaker 1>little kid with the Men in Black the original movie,

532
00:33:05.039 --> 00:33:08.640
<v Speaker 1>the very end scene where they zoom all the way

533
00:33:08.720 --> 00:33:11.039
<v Speaker 1>out of our Earth and our gay and our soul

534
00:33:11.160 --> 00:33:13.559
<v Speaker 1>system and galaxy and universe, and it keeps zooming out,

535
00:33:13.680 --> 00:33:15.559
<v Speaker 1>and it keeps zooming out, and it keeps zooming out,

536
00:33:15.599 --> 00:33:19.480
<v Speaker 1>and then eventually everything that we could conceptualize in our

537
00:33:19.759 --> 00:33:23.240
<v Speaker 1>known universe was just a marble in an alien's hand

538
00:33:23.440 --> 00:33:26.720
<v Speaker 1>and they were just playing with marvels. And it's just,

539
00:33:26.920 --> 00:33:31.000
<v Speaker 1>you know, the idea that it just continually exponentially if

540
00:33:31.039 --> 00:33:33.759
<v Speaker 1>you just could open up the aperture infinitely, there would

541
00:33:33.799 --> 00:33:37.680
<v Speaker 1>always be something bigger and bigger and bigger. And I

542
00:33:37.759 --> 00:33:41.119
<v Speaker 1>think that mathematically, they've I've just heard this. I have

543
00:33:41.200 --> 00:33:44.079
<v Speaker 1>no idea, but I think mathematically, some of the formulas

544
00:33:44.119 --> 00:33:47.680
<v Speaker 1>to look at some of the smallest known things and

545
00:33:47.759 --> 00:33:51.200
<v Speaker 1>the biggest things are similar. And I think that falls

546
00:33:51.200 --> 00:33:52.119
<v Speaker 1>into quantum theory.

547
00:33:53.000 --> 00:33:58.160
<v Speaker 2>Yeah, that's why. Well, yes, that's correct quantum. I mean,

548
00:33:58.200 --> 00:34:00.839
<v Speaker 2>when you look at the mathematics of relative quantum theory,

549
00:34:00.880 --> 00:34:03.440
<v Speaker 2>which are the two sort of theories that you know,

550
00:34:04.799 --> 00:34:07.519
<v Speaker 2>one governs are very small, one governs are very large,

551
00:34:08.960 --> 00:34:11.800
<v Speaker 2>some of those equations do look similar. They're all horrendous.

552
00:34:11.880 --> 00:34:15.079
<v Speaker 2>Mathematics was not my strong point at university. I'm afraid,

553
00:34:15.599 --> 00:34:16.320
<v Speaker 2>oh me neither.

554
00:34:16.639 --> 00:34:19.920
<v Speaker 1>But now, oh but what if? And you know, I

555
00:34:19.960 --> 00:34:21.960
<v Speaker 1>don't think these are the questions will ever answer. But

556
00:34:22.079 --> 00:34:25.360
<v Speaker 1>what if it was just a big circle? How craazy

557
00:34:25.360 --> 00:34:27.880
<v Speaker 1>would that be? Those are the things we may never

558
00:34:28.000 --> 00:34:31.920
<v Speaker 1>find out though, but we will continue to explore and

559
00:34:32.079 --> 00:34:35.679
<v Speaker 1>answer those questions every week here on Space Nuts. Fred,

560
00:34:35.760 --> 00:34:38.679
<v Speaker 1>did you have anything else you wanted to add to

561
00:34:38.800 --> 00:34:40.320
<v Speaker 1>our conversation today.

562
00:34:41.639 --> 00:34:45.519
<v Speaker 2>Not only that we have a very exciting time at

563
00:34:45.519 --> 00:34:48.480
<v Speaker 2>the moment in human space flight. We've just seen the

564
00:34:49.360 --> 00:34:53.280
<v Speaker 2>orbital flight, sorry orbital flight of the FRAM two mission,

565
00:34:53.320 --> 00:34:58.000
<v Speaker 2>the privately operated space mission that took humans into a

566
00:34:58.079 --> 00:35:00.519
<v Speaker 2>polar orbit for the first time, one that is both

567
00:35:00.559 --> 00:35:04.000
<v Speaker 2>the north and the South pole. Those astronauts returned a

568
00:35:04.079 --> 00:35:06.639
<v Speaker 2>few days ago with lots of tales to tell. We

569
00:35:06.760 --> 00:35:09.599
<v Speaker 2>might cover that in a future is edition of Space Nuts.

570
00:35:10.320 --> 00:35:12.400
<v Speaker 1>It's very exciting. Thank you so much, Fred, It was

571
00:35:12.440 --> 00:35:13.400
<v Speaker 1>great talking to you today.

572
00:35:14.119 --> 00:35:16.159
<v Speaker 2>Always a pleasure, Hidi, thank you very much for your

573
00:35:16.239 --> 00:35:23.159
<v Speaker 2>time to space to the Space Nuts podcast available at

574
00:35:23.199 --> 00:35:28.440
<v Speaker 2>Apple Podcasts, Spotify, iHeart Radio, or your favorite podcast player.

575
00:35:28.679 --> 00:35:31.440
<v Speaker 1>You can also stream on demand at bides dot com.

576
00:35:32.000 --> 00:35:35.920
<v Speaker 2>This has been another quality podcast production from nights dot com.
