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<v Speaker 1>Hi there, thanks for joining us.

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<v Speaker 2>This is Space Nuts yet again. My name is Andrew Dunkley,

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<v Speaker 2>your host. It's so good to have your company. Coming

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<v Speaker 2>up on this episode. We've got a lot to get through.

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<v Speaker 2>As I tend to say, some clever work reveals where

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<v Speaker 2>most meteorites come from. Some space scientists have doubled down

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<v Speaker 2>on a brown dwarf mystery.

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<v Speaker 1>What does that mean? Snow white? Snow white and white?

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<v Speaker 1>Know the answer?

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<v Speaker 2>And some good news and some bad.

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<v Speaker 1>News for SpaceX.

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<v Speaker 2>That's all coming up on this episode of Space Nuts.

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<v Speaker 1>Fifteen second is in channel ten nine ignition sequence Space

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<v Speaker 1>Nuts or three two Space Nurts. Can I report it?

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<v Speaker 1>Neils Good?

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<v Speaker 2>Joining me again is Professor Fred what's an astronomer?

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<v Speaker 1>At La Tello? Fred?

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<v Speaker 3>Hi, Andrew, how are you going?

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<v Speaker 1>I'm going that way? Yeah, I'm good. I'm good. At

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<v Speaker 1>the moment, all is well. How are you?

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<v Speaker 3>I'm going that.

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<v Speaker 1>Way too, good thing. We're both going in the same

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<v Speaker 1>direction as it is.

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<v Speaker 2>Yes, you don't want to be going backwards at this

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<v Speaker 2>stage in our lives. It's that's absolutely right, very true,

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<v Speaker 2>unless you could wind back time and get younger and

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<v Speaker 2>yet take back all that knowledge you've got and you

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<v Speaker 2>know I've made the same mistakes over again.

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<v Speaker 3>No, I don't want to do that. Not enough for

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<v Speaker 3>making mistakes.

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<v Speaker 1>You just make different mistakes. I reckon, I think you do. Yeah,

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<v Speaker 1>it's usually the kind of mistakes you make. Is where

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<v Speaker 1>did I put my glasses? I can't remember? Oh yeah,

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<v Speaker 1>and yeah, I've done that. I can't find mine.

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<v Speaker 3>Now I give you a clue.

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<v Speaker 1>Let me just adjust my glasses. And what was the answer?

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<v Speaker 2>Yes, Judy and I have often talked about this and

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<v Speaker 2>look back at some of the mistakes we've made, mainly financial,

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<v Speaker 2>over the years, and we've both said, look, if we

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<v Speaker 2>didn't make those mistakes, other things wouldn't have happened that

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<v Speaker 2>have defined our lives. So, you know, you can't sort

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<v Speaker 2>of dismiss the mistakes because they made other good things happen.

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<v Speaker 1>You've got to think of it that way. So that's

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<v Speaker 1>the only way I could reconcile my past history with

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<v Speaker 1>any kind of satisfaction. Some of the mistakes have resulted

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<v Speaker 1>in some brilliant things.

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<v Speaker 2>Yes, Well, you know, to Err is human and that's

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<v Speaker 2>you know, that's the definition of a human being. We

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<v Speaker 2>make mistakes and hopefully learn from them. We've got to

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<v Speaker 2>learn something now, Fred from some very clever work that's

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<v Speaker 2>been done, and they reckon. They've nailed down around seventy

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<v Speaker 2>percent of the meteorites that we know of coming from

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<v Speaker 2>three basic events in recent history. So that's pretty exciting,

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<v Speaker 2>and I think they extrapolated some more information out they

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<v Speaker 2>can nearly account for ninety percent.

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<v Speaker 1>Of all meteorites. This is quite an amazing story, it is,

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<v Speaker 1>and it starts off with a kind of analysis of

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<v Speaker 1>meteorites because they're not all the same now, and you know,

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<v Speaker 1>the astronomers or planetary scientists, I guess classify them in

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<v Speaker 1>different ways, which is all about their composition. The stony

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<v Speaker 1>meteorites and metallic meteorites.

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<v Speaker 3>They are the two sort of basic.

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<v Speaker 1>Ones, but within those definitions there are different, you know,

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<v Speaker 1>different levels of how stoney they are or how not.

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<v Speaker 1>And I should just say at the outset that the

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<v Speaker 1>metallic ones are actually quite rare, so that the most

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<v Speaker 1>common meteorites that we found are something called well ordinary

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<v Speaker 1>chondrites chondrites C H O, N, D R I T

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<v Speaker 1>e S.

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<v Speaker 3>Looks like chong drites, but it's chondrites usually.

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<v Speaker 1>And they are what make up most of the it's

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<v Speaker 1>tens of thousands of meteorites that are in collections around

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<v Speaker 1>the world.

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<v Speaker 3>I can't remember the exact number, but it's a lot.

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<v Speaker 1>Which have you know, they've been collected by meteorites hunters,

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<v Speaker 1>and of course they're free gifts from the universe, so

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<v Speaker 1>they're always valuable to have because they tell us about

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<v Speaker 1>the makeup of things. Anyway, the most common are these chondrites,

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<v Speaker 1>which are sort of carbonaceous. They're stony objects. But the

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<v Speaker 1>the conundrum is that the when you look at the asteroids,

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<v Speaker 1>and they sit in the asteroid belt principally, and we

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<v Speaker 1>believe that they are the main source of meteorites. So

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<v Speaker 1>there are one or two meteorites actually it's several hundred,

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<v Speaker 1>but a few that come that are known to come

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<v Speaker 1>from the Moon or Mars, or in fact the asteroid Vestor,

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<v Speaker 1>which is actually quite a large member of the asteroid belt,

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<v Speaker 1>the fourth one to be discovered. I think. I think

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<v Speaker 1>six percent of all meteorites come from either the Moon,

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<v Speaker 1>Mars or Vesta. However, as I said, most of them

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<v Speaker 1>are just chondrites. But here's the thing. The asteroid population,

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<v Speaker 1>the chondrites are actually quite rare. They don't dominate the

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<v Speaker 1>asteroid population, and so there is a puzzle there, why

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<v Speaker 1>should all ours be commoner garden chondrites whereas condracts are

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<v Speaker 1>relatively rare when you look at the asteroid belt in general.

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<v Speaker 1>And so what this team it's actually I think three

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<v Speaker 1>different teams of scientists who have produced I think there

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<v Speaker 1>are three papers involved here. And what they've done is

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<v Speaker 1>they've basically looked at the motion of the asteroids in

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<v Speaker 1>the asteroid belt. And you know, one of the wonderful

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<v Speaker 1>things that you and I talk about a lot is

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<v Speaker 1>how predicted predictable gravity is the fact that we can

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<v Speaker 1>we can actually get a really good idea of the

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<v Speaker 1>motions of objects through space tens of thousands or even

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<v Speaker 1>millions of years in the past and the future, because

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<v Speaker 1>gravitation is such a well understood phenomenon, at least at

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<v Speaker 1>the level of objects in the Solar System. And so

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<v Speaker 1>what they've done is they've studied the asteroid belt and

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<v Speaker 1>looked for events in the past that would have brought

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<v Speaker 1>asteroids together, that would have been collisions, and they've essentially

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<v Speaker 1>found some and there are collisions between chondrite asteroids. Ah.

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<v Speaker 1>You know, so it's making sense here that you've got

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<v Speaker 1>a relatively rare population within the asteroid belt, but they're

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<v Speaker 1>the ones that have collided, and they identify I think

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<v Speaker 1>three collisions over the last Actually they go back quite

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<v Speaker 1>a long way. There's one, the most distant one in

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<v Speaker 1>the past, a collision which I think we've talked about already.

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<v Speaker 1>Actually I think we talked about it in a different

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<v Speaker 1>context a few weeks ago. It's about four hundred and

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<v Speaker 1>sixty six million years ago, and we think that would

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<v Speaker 1>have that was a collision that absolutely showered the Earth

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<v Speaker 1>with meteorites and may even have formed a ring around

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<v Speaker 1>the Earth. And I think that's what we've talked about,

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<v Speaker 1>because there's a Massex, you know, there's an ice age

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<v Speaker 1>not long after that, and the thinking is that the

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<v Speaker 1>ring of asteroids around the Earth might have shaded in

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<v Speaker 1>the sun the planet a little bit to reduce the temperature.

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<v Speaker 1>So that's that's the furthest one. But there are other

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<v Speaker 1>collisions that have been identified which are more recently than that.

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<v Speaker 1>And I might read a paragraph, if I may, from

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<v Speaker 1>a very nice piece on this from Sky and Telescope,

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<v Speaker 1>one of the it is astronomy magazines in the world.

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<v Speaker 1>I was addicted to Sky of telescope when I was

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<v Speaker 1>a youngster, and what it says is two collisions involving

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<v Speaker 1>H chondrites. These are two different sorts of condrits H

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<v Speaker 1>and L chondrites, but they're all sort of common garden meteorites.

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<v Speaker 1>Two collisions involving H chondrites occurred so recently that the

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<v Speaker 1>researchers could trace their orbits well enough to date the

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<v Speaker 1>family's origin. This is the family of asteroids that resulted

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<v Speaker 1>from that collision. The older collision occurred seven point six

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<v Speaker 1>million years ago and yielded the family of objects with

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<v Speaker 1>orbits similar to one five eight Coronis. Now one five

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<v Speaker 1>eight Coronis is an asteroid. You remember that asteroids have

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<v Speaker 1>a number, which is the number in the order of discovery,

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<v Speaker 1>and Coronis is the name given by the discoverer, So

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<v Speaker 1>one five eight Coronis. They seem to have come from

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<v Speaker 1>a collision Coronis and it's similar family, a collision seven

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<v Speaker 1>point six million years ago. Reading back again from the

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<v Speaker 1>sky telescope, artic called a younger family dates back to

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<v Speaker 1>an event five point eight million years ago in which

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<v Speaker 1>Coronis underwent another major collision, splitting off the smaller asteroid

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<v Speaker 1>eight three two. Karen and its family, and so you know,

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<v Speaker 1>this is lovely detective work that gives you a picture

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<v Speaker 1>of the dynamics of the asteroid belt that we just

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<v Speaker 1>didn't have before, and gives us a really good understanding

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<v Speaker 1>that that some of this, you know, some of this

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<v Speaker 1>debris that we receive from space really comes from a

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<v Speaker 1>very small number of collisions in the asteroid belt.

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<v Speaker 2>Yeah, it's fascinating, and I'm guessing after reading through the

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<v Speaker 2>article of this, this still has to be peer reviewed.

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<v Speaker 2>The paper is out there to be analyzed and chopped

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<v Speaker 2>up and debated, and uh, you know, others will probably

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<v Speaker 2>study the claims and say, well, hang on, men, but

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<v Speaker 2>they seem pretty confident.

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<v Speaker 1>Yeah they do.

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<v Speaker 3>I think these are pretty Yeah.

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<v Speaker 1>There are two Nature papers involved, so obviously one of

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<v Speaker 1>the leading scientific journals in the world. There's a lot

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<v Speaker 1>of detail to this. It's a story with many twists

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<v Speaker 1>and ins and outs, and what I've told you is

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<v Speaker 1>the you know, cod of the bottom line.

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<v Speaker 3>But it is worth a read.

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<v Speaker 1>It. It's very nicely put for astronomy enthusiasts in perhaps

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<v Speaker 1>one of the principal magazines for astronomy enthusiasts, going Telescope.

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<v Speaker 2>Yeah, I'm just amazed that you can look at a

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<v Speaker 2>situation and go okay, how did that happen and then

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<v Speaker 2>sort of work backwards to a source billions of years ago.

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<v Speaker 2>That just fascinates me. I think it's very clever, as

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<v Speaker 2>you said, very clever detective work. Yeah, and that's in

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<v Speaker 2>Sky and Telescope magazine if you want to read up.

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<v Speaker 2>While we're talking about meteorites, Fred, I read an article

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<v Speaker 2>or the other day which I think the BBC Science

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<v Speaker 2>website ran about Earth getting bombarded by micro meteorites, which

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<v Speaker 2>are tiny pieces of asteroid and they reckon. Between twenty

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<v Speaker 2>and sixty million kilograms falls on Earth every year in

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<v Speaker 2>micro meteorites. And if you were to I don't know

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<v Speaker 2>who worked this out, but if you were to stand

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<v Speaker 2>in the same spot for almost thirteen years, you would

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<v Speaker 2>get a micro meteorite caught in your hair. There you are,

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<v Speaker 2>there's a factoid if you like.

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<v Speaker 3>But of course, assuming that you have fard.

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<v Speaker 1>Well that's right.

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<v Speaker 2>If you don't, it would probably bounce off and land

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<v Speaker 2>in someone else's hair maybe the case.

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<v Speaker 1>That's an interesting article in it. It kind of sparks

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<v Speaker 1>memories for me of well, when I was in Edinburgh

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<v Speaker 1>decades ago. There are things called brown lea particles. Did

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<v Speaker 1>that crop up in the in the article you remember?

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<v Speaker 1>I can't see the word there.

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<v Speaker 2>I can see a couple of other interesting little tidbits,

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<v Speaker 2>like there's one in four thy six hundred chances of

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<v Speaker 2>being hit by a micro meteorite. If you stand in

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<v Speaker 2>the same spot for twenty four hours.

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<v Speaker 1>You probably you wouldn't know it. No, well, if you

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<v Speaker 1>stood in the same spot for twenty four hours, I

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<v Speaker 1>think you probably need therapy. Anyway, you're probably in line

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<v Speaker 1>for Taylor Swift tickets. That's probably where you'd be.

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<v Speaker 3>Oh, that could be it. That could yes, that could

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<v Speaker 3>be right.

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<v Speaker 1>Great, it's an interesting factoid. We should put that in

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<v Speaker 1>Friends Flip the Right.

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<v Speaker 2>Fled Fred's flippant Factoids, which we started doing on our

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<v Speaker 2>TikTok if you want to look at us and look

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<v Speaker 2>us up on TikTok when we do.

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<v Speaker 1>Little previews of the shows. So, yes, that's an interesting story,

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<v Speaker 1>as is this one. Fred. They've been studying a.

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<v Speaker 2>Brown dwarf for the last thirty years, but there's something

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<v Speaker 2>about it was off. So they've taken a closer look

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<v Speaker 2>and when bam, thank you ma'am, it's not one but

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<v Speaker 2>two brown dwarfs. They've only got five more defined.

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<v Speaker 1>Yeah, essentially this a good question what the population of

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<v Speaker 1>brown dwarf brown dwarf stars is.

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<v Speaker 3>It's very high.

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<v Speaker 1>It's subject that we haven't really talked about, no, Andrew,

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<v Speaker 1>and it's probably not a very good thing that we

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<v Speaker 1>haven't talked about it much because certainly one of my

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<v Speaker 1>former colleagues at the Australian Astronomical Observatory, Professor Christiny of

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<v Speaker 1>the University of New South Wales, he began his career

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<v Speaker 1>as one of the world's leading experts on brown dwarf stars.

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<v Speaker 1>He's now moved on to exoplanets, which I guess of

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<v Speaker 1>the next step down the series, because brown dwarfs in

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<v Speaker 1>a way they sit in size between the giant planets

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<v Speaker 1>of the Solar System, for example, or any other Solar

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<v Speaker 1>System and stars themselves. They're defined as having a mass

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<v Speaker 1>a lower mass limit of thirteen times the mass of Jupiter,

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<v Speaker 1>and that means that if Jupiter had grown to be

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<v Speaker 1>thirteen times its present size, it would have not been

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<v Speaker 1>a planet, it would have been a brown dwarf. And

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<v Speaker 1>the difference is that brown dwarfs have low level nuclear

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<v Speaker 1>processes going on in their interior, something called deuterium burning,

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<v Speaker 1>which gives them enough of a temperature that they're visible

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<v Speaker 1>in the infrared the redder than red waveband. So that's

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<v Speaker 1>how brown dwarfs are found using infrared telescopes. And back

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<v Speaker 1>in the day, it would be in the nineteen eighties

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<v Speaker 1>and nineties when brown dwarfs first started to be being discovered.

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<v Speaker 1>This new population of stars that didn't quite make it

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<v Speaker 1>because they're not big enough. I think they need to

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<v Speaker 1>be about ninety times one hundred times the mass in

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<v Speaker 1>Jupiter in order for you know, what we call hydrogen

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<v Speaker 1>fusion to take place and normal processes that make styles shine. Anyway,

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<v Speaker 1>that's the background. So this is a brown dwarf which

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<v Speaker 1>is called Gliza two to nine B. Gliza was an

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<v Speaker 1>astronomer who made a catalog of these things, and in

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<v Speaker 1>fact the discovery exactly as you said thirty years ago,

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<v Speaker 1>nearly discovered in nineteen ninety five and is one that

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<v Speaker 1>there is puzzle astronomers because they couldn't really work out

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<v Speaker 1>why it was so massive and so dim. It should

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<v Speaker 1>if it was the mass that we thought it was,

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<v Speaker 1>it should be a lot brighter. Now, school with a

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<v Speaker 1>couple of kids that fit that description.

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<v Speaker 3>Massive button dim Yeah, okay.

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<v Speaker 1>He didn't argue with them. He didn't argue with them,

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<v Speaker 1>so yeah, yeah, I can well imagine. I don't just

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<v Speaker 1>we probably shouldn't name them now that might get us

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<v Speaker 1>in talk. Never mentioned Paul's name. All right, let's move

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<v Speaker 1>on the brown dwarf gleaser to two nine B should

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<v Speaker 1>be more, should be brighter than it is given its

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<v Speaker 1>mass until now, and now we have had a paper

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<v Speaker 1>that's been lead authored by actually a graduate student, which

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<v Speaker 1>is you know, it's nice to see these post graduate

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<v Speaker 1>students doing their graduate students doing their basically cutting edge research.

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<v Speaker 1>And this gentleman Jerry Clan who is at the California

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<v Speaker 1>Institute of Technology, and Jerry can be either.

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<v Speaker 3>So I should just.

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<v Speaker 1>Qualify that by seeing saying this person, Jerry quann is

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<v Speaker 1>a graduate student at Caltech, the California Institute of Technology,

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<v Speaker 1>one of the leading organizations in the world for this

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<v Speaker 1>kind of work, and lots of other fields of studying too. Anyway,

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<v Speaker 1>he or she they have written a paper in Nature

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<v Speaker 1>which explains what the issue is and it's that Lisa

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<v Speaker 1>two to nine B isn't one, but is actually two

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<v Speaker 1>brown dwarfs thirty eight and thirty four times the US

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<v Speaker 1>of Jupiter, and they have a twelve day orbit around

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<v Speaker 1>each other and something close to our hearts here in Australia.

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<v Speaker 1>They were observed by using instruments at the very large

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<v Speaker 1>telescope in Chile run by the European Southern Observatory, which

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<v Speaker 1>we in Australia have a strategic partnership with. Now, so

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<v Speaker 1>the fact that this star is actually not a single star,

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<v Speaker 1>it's a binary, which is what we call two styles

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<v Speaker 1>orbiting around another is a great discoverer. Yeah, great discovery

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<v Speaker 1>and pushes forward our understanding of brown dwarfs. In fact,

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<v Speaker 1>it clearly solves a problem if this thing was more

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<v Speaker 1>massive than it should be for the amount of radiation

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<v Speaker 1>that it gives out.

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<v Speaker 3>So yes, really really.

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<v Speaker 1>Very nice, a very nice study. There's a nice quote

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<v Speaker 1>from one of the people who actually discovered Gleezer two

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<v Speaker 1>to nine B back in nineteen ninety five, Rebecca Oppenheimer,

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<v Speaker 1>who says, these two worlds whipping around each other are

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<v Speaker 1>actually smaller in radius than Jupiter. They look quite strange

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<v Speaker 1>in our night sky. If we had something like them

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<v Speaker 1>in our own solar system, they would indeed yeah.

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<v Speaker 2>Wow, No, that's a great discovery and it sorts out

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<v Speaker 2>a problem about this thing they've been looking at for

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<v Speaker 2>thirty years not being bright enough.

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<v Speaker 1>And yeah they've they've figured it out.

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<v Speaker 2>And Jerry is a bloke, so and look forgive me Fred,

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<v Speaker 2>but I think the Chinese pronounced their exes as ship

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<v Speaker 2>so Shun I would suggest his surname Jerry chu Anne

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<v Speaker 2>from the cultake yep, yes, originally from China and ultimately

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<v Speaker 2>in Canada. Yeah, yeah, very very good pick up by

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<v Speaker 2>him about the brown dwarf situation. How close is the

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<v Speaker 2>nearest one to us?

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<v Speaker 1>Have we ever figured that out? Yes, we probably do

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<v Speaker 1>know that, and it's probably not that far, but I

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<v Speaker 1>don't know the answer to it. I'm sure while we're

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<v Speaker 1>talking about the next story, you can google closest.

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<v Speaker 3>Brown draft you know, I will, and.

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<v Speaker 1>I'm glad you do it, because, like, as we've just discovered,

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<v Speaker 1>it's very nice that, yeah, you can chill in these gaps.

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<v Speaker 2>The nearest Brown dwarfs are located in the Lumen sixteen system,

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<v Speaker 2>which is about six and a half light years away.

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<v Speaker 3>Yeah, I thought they would be quite close.

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<v Speaker 1>I mean, it's because we have a relatively nearby population

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<v Speaker 1>of brown dwarfs. So they're probably very common in the galaxy.

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<v Speaker 1>It's because they're not great distances that we know about

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<v Speaker 1>them at all, because they are so dim, they're kind

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<v Speaker 1>of broiled.

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<v Speaker 3>That's why they got that. Yeah.

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<v Speaker 2>Yeah, not weak enough to be plants, not strong enough

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<v Speaker 2>to be stars. They're just somewhere in between, wondering about

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<v Speaker 2>their identities.

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<v Speaker 3>Normally, they're probably very confused and very.

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<v Speaker 1>Confused spatial objects.

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<v Speaker 2>Yeah, if you want to read all about that, it's

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<v Speaker 2>in the Cosmos magazine website. This is Space Nuts with

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<v Speaker 2>Andrew Dunkley and Professor.

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<v Speaker 1>Fred Broad space Buds.

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<v Speaker 2>Okay, Fred, we've got a couple of stories involving SpaceX.

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<v Speaker 2>We've been talking about them a lot lately, and in

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<v Speaker 2>this case there's some good news and some not so

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<v Speaker 2>good news. Let's start off with the good news about

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<v Speaker 2>SpaceX making so many inroads in rocket technology.

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<v Speaker 3>It is.

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<v Speaker 1>It's really quite amazing what SpaceX has achieved so last

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<v Speaker 1>week as we stand at the moment. In late October,

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<v Speaker 1>SpaceX carried out it's ninety ninth operational flight of the year,

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<v Speaker 1>and that was styling another Starlink launch, So twenty Starlink

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<v Speaker 1>satellites launchtrom Cape Canaveral and basically a successful mission. The

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<v Speaker 1>booster had already flown sixteen lames beforehand and made after

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<v Speaker 1>the seventeenth flight, made a good recovery on the drone hip,

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<v Speaker 1>which is called just read the instructions. Yeah, that this great,

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<v Speaker 1>isn't it? So? You know, it's it's really quite remarkable.

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<v Speaker 1>So the Space Coast as it's called where Canaveral is

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<v Speaker 1>seventy one so far this year. Because SpaceX also launches

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<v Speaker 1>from other places as well, so seventy one from the

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<v Speaker 1>Space Coast, of which all but five of them have

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<v Speaker 1>been flown by SpaceX. It's quite an extraordinary track record.

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<v Speaker 1>In fact, one of them was one we saw where

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<v Speaker 1>we were in Florida back in May.

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<v Speaker 3>The others and.

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<v Speaker 1>The other five were flown by the United Launch Alliance.

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<v Speaker 1>But you know, that statistic in itself tells you how

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<v Speaker 1>much of a game changer being able to recover your

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<v Speaker 1>booster rocket is and that because that's what gives space

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<v Speaker 1>X the edge on this, that they can pull the

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<v Speaker 1>booster rocket back and launch it again. Yes, so, and

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<v Speaker 1>of course there's been other, you know, other other missions

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<v Speaker 1>that the breakdown is of the ninety nine launches is

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<v Speaker 1>ninety one Falcon and five Falcon Heavy missions. And I

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<v Speaker 1>don't think that includes the theybeating does the Starling Sorry

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<v Speaker 1>Starship launches? I can't remember how that fits into the

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<v Speaker 1>into the statistics the Starling launches, which of course culminated

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<v Speaker 1>in that extraordinary event a couple of weeks ago when

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<v Speaker 1>when the Starling Sorryes Starship boost of the Falcon Super

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<v Speaker 1>Heavy which are grabbed by the chopsticks. Yeah. Down there

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<v Speaker 1>a book a Chica in Texas. So, yes, that's the

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<v Speaker 1>good news. A lot of activity.

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<v Speaker 4>Yeah, they reckon Fred that they could reach around one

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<v Speaker 4>hundred and forty four launches by the end of this

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<v Speaker 4>calendar year, which would be an all time record.

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<v Speaker 2>That would, Yeah, an amazing achievement. I think they're launching

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<v Speaker 2>on average once every couple of weeks.

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<v Speaker 1>Well, yes, it's more than that. It's more than twice.

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<v Speaker 1>It's three times a week, basically three times a little. Yeah,

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<v Speaker 1>it's a lot. Yeah, it's kind of almost every day,

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<v Speaker 1>which is sort of what you know, what we It's

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<v Speaker 1>not quite that, but it's it's what we expected would

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<v Speaker 1>happen with all this. Now. Of course, most of those

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<v Speaker 1>launches were for styling satellites space butts.

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<v Speaker 2>Therein though, lies a problem, and this is where we

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<v Speaker 2>get onto the not so good news for SpaceX because

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<v Speaker 2>people have been analyzing their activity, and it's not just them,

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<v Speaker 2>there's a lot of organizations that use similar technology. And

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<v Speaker 2>the concerns have been raised about pollution in our atmosphere.

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<v Speaker 1>That's right, and this is something that's been growing in

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<v Speaker 1>I guess attention over the past well a few months

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<v Speaker 1>perhaps the past year. Is what happens when the spacecraft

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<v Speaker 1>re enters the atmosphere, so it burns up if you know,

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<v Speaker 1>less bits of it actually get down to the Earth,

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<v Speaker 1>which we do know happens from time to time.

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00:25:50.519 --> 00:25:51.759
<v Speaker 3>We've talked about that as well.

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<v Speaker 1>But fac the spacecraft burns up. If you've got a

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<v Speaker 1>like a Starlink satellite, which way is about a quarter

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<v Speaker 1>of a ton about three meters by one meter, they

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<v Speaker 1>basically are completely burned up in the atmosphere, and that

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<v Speaker 1>means there's a quarter of a ton of stuff gone

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<v Speaker 1>into the atmosphere, and the stuff is mostly aliminium oxide

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<v Speaker 1>because they're must be made of aluminium. They burned up

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<v Speaker 1>and generate aliminium oxide. And that is well, it's one

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<v Speaker 1>of these gases that contributes to the hole in the

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<v Speaker 1>ozone there and so it is not that and gentle

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<v Speaker 1>on the atmosphere. There's an estimate which is that at

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<v Speaker 1>the moment, about half a ton of burned up satellite

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<v Speaker 1>trash as it's called, you know, by some of the

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00:26:46.920 --> 00:26:49.480
<v Speaker 1>authors who are written about this, and I'm looking at

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00:26:49.480 --> 00:26:54.039
<v Speaker 1>the space dot com website. At the moment satellite trash

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<v Speaker 1>half a ton comes in per day. And that's because

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<v Speaker 1>you've got you know, a lot of Starlink satellites burning

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<v Speaker 1>up their they're a quarter of a talent. But you've

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<v Speaker 1>also got the upper stage of the Starlink launch vehicles.

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<v Speaker 1>So it's the top part of a Falcon heavy, the

422
00:27:15.440 --> 00:27:19.319
<v Speaker 1>bit that does not get returned to Earth, the cheaper bit.

423
00:27:20.640 --> 00:27:22.720
<v Speaker 1>I think it weighs about four tons when all the

424
00:27:22.720 --> 00:27:26.200
<v Speaker 1>fuels out of it, and so that's they're coming down

425
00:27:26.240 --> 00:27:29.319
<v Speaker 1>as well. So if Starlink are launching twenty at a time,

426
00:27:29.400 --> 00:27:33.200
<v Speaker 1>which is about the standard number at the moment, then

427
00:27:33.480 --> 00:27:37.000
<v Speaker 1>that every twenty satellites you get another four tons of debris,

428
00:27:37.079 --> 00:27:40.880
<v Speaker 1>which is the aluminium oxide that comes from the upper

429
00:27:40.880 --> 00:27:47.039
<v Speaker 1>stage of your rocket. That's it's a concern. It's starting

430
00:27:47.039 --> 00:27:52.599
<v Speaker 1>to worry people. As I said, in particular, particularly it

431
00:27:52.640 --> 00:27:56.480
<v Speaker 1>is in regards to its effect on the ozone lare.

432
00:27:57.119 --> 00:28:01.400
<v Speaker 1>Now you and I have to before about the lifetime

433
00:28:01.440 --> 00:28:04.920
<v Speaker 1>of Stalink satellites. They are about five years and you

434
00:28:04.960 --> 00:28:08.160
<v Speaker 1>will recall probably that the first tranch of Starlink satellites

435
00:28:08.240 --> 00:28:12.200
<v Speaker 1>was launched in May twenty nineteen. That's five years ago,

436
00:28:12.359 --> 00:28:14.240
<v Speaker 1>more than five years ago. So they are starting to

437
00:28:14.279 --> 00:28:15.039
<v Speaker 1>come back.

438
00:28:15.480 --> 00:28:19.960
<v Speaker 2>And this is going to constantly rotate over time. They

439
00:28:20.839 --> 00:28:22.759
<v Speaker 2>launching more.

440
00:28:22.559 --> 00:28:25.359
<v Speaker 1>Than the getting back that have past.

441
00:28:25.400 --> 00:28:27.440
<v Speaker 2>They use by date, so they come back and burn up.

442
00:28:27.480 --> 00:28:30.240
<v Speaker 2>They put a bunch more up there. They ultimately want

443
00:28:30.240 --> 00:28:32.680
<v Speaker 2>to put like what one hundred thousand of these things

444
00:28:32.720 --> 00:28:34.279
<v Speaker 2>in orbit, and I.

445
00:28:34.319 --> 00:28:36.119
<v Speaker 1>Think it could be one hundred thousand when you added

446
00:28:36.200 --> 00:28:40.359
<v Speaker 1>all the different constellations. At the moment, Starlink's twelve thousand

447
00:28:41.279 --> 00:28:46.960
<v Speaker 1>aiming at but with possible extension of another thirty thousand

448
00:28:47.000 --> 00:28:48.759
<v Speaker 1>spacecraft in case two.

449
00:28:49.119 --> 00:28:50.920
<v Speaker 3>I don't think it's called that anymore, but it was

450
00:28:51.000 --> 00:28:51.319
<v Speaker 3>called that.

451
00:28:52.119 --> 00:28:54.400
<v Speaker 1>But then on top of that, you've got one Web

452
00:28:54.440 --> 00:28:57.079
<v Speaker 1>which has something like six hundred spacecraft in orbit. You've

453
00:28:57.079 --> 00:29:02.359
<v Speaker 1>got Koiper which is another another of these constellations fun

454
00:29:02.519 --> 00:29:07.000
<v Speaker 1>which is the Chinese answer to starlink. That's fourteen to

455
00:29:07.079 --> 00:29:09.880
<v Speaker 1>fifteen thousand such a lites. When you add all these up,

456
00:29:10.440 --> 00:29:12.319
<v Speaker 1>it could be that by the end of the decade

457
00:29:12.319 --> 00:29:15.079
<v Speaker 1>we have one hundred thousand satellites in orbit, which would

458
00:29:15.119 --> 00:29:19.559
<v Speaker 1>actually impact on the sky very significantly. Well, that's the problem.

459
00:29:19.680 --> 00:29:24.920
<v Speaker 2>One problem for observational astronomers is the pollution that creates

460
00:29:25.000 --> 00:29:28.599
<v Speaker 2>for observations. But all of these things are going to

461
00:29:28.599 --> 00:29:31.200
<v Speaker 2>come back down, They're designed to come back down and

462
00:29:31.279 --> 00:29:33.440
<v Speaker 2>burn up on re entry, and we're putting all that

463
00:29:34.960 --> 00:29:39.200
<v Speaker 2>aluminium oxide into the atmosphere. And I read the word

464
00:29:39.240 --> 00:29:43.200
<v Speaker 2>but it's escaped me. But it basically means that with

465
00:29:43.279 --> 00:29:47.160
<v Speaker 2>the effect this could have on the ozone layer, it

466
00:29:47.200 --> 00:29:52.319
<v Speaker 2>would affect here. It is the albedo, the ability for

467
00:29:52.440 --> 00:29:57.559
<v Speaker 2>our planet to reflect sunlight. So this is yet another

468
00:29:57.640 --> 00:30:01.319
<v Speaker 2>potential greenhouse effect problem.

469
00:30:02.000 --> 00:30:09.000
<v Speaker 1>Yes, that's right. Indeed, that's right. It's clearly shaping up

470
00:30:09.039 --> 00:30:13.319
<v Speaker 1>to be an environmental problem that is a direct result

471
00:30:13.359 --> 00:30:16.400
<v Speaker 1>of the space age. And there's not many of those

472
00:30:16.400 --> 00:30:19.200
<v Speaker 1>that you can point to. You know, a lot of

473
00:30:19.200 --> 00:30:25.000
<v Speaker 1>people think it's the exhaust gases from the rockets, which

474
00:30:25.759 --> 00:30:29.599
<v Speaker 1>in a particular way it is because solid rocket fuel

475
00:30:29.960 --> 00:30:34.799
<v Speaker 1>is very bad for ozone depletion, and apparently the solid

476
00:30:34.839 --> 00:30:38.799
<v Speaker 1>rockets that are used for some of the launchers United

477
00:30:39.519 --> 00:30:44.000
<v Speaker 1>United Launch Alliances Atlas five uses strap on solid rocket boosters.

478
00:30:45.240 --> 00:30:48.519
<v Speaker 1>China's Long March eleven has solid rocket fuel boosters, and

479
00:30:48.599 --> 00:30:52.599
<v Speaker 1>actually the new Ariana six, the European one, also has

480
00:30:52.640 --> 00:30:56.119
<v Speaker 1>these strap on boosters and they give out chemicals that

481
00:30:56.119 --> 00:30:59.920
<v Speaker 1>are pretty horrible. There's chlorine in there, and the low

482
00:31:00.039 --> 00:31:04.799
<v Speaker 1>with all sorts of stuff, and the worst of it

483
00:31:04.839 --> 00:31:09.440
<v Speaker 1>is that they are putting these exhaust plumes into the

484
00:31:09.480 --> 00:31:13.880
<v Speaker 1>stratosphere just basically where the ozone is. So it's a

485
00:31:13.960 --> 00:31:17.160
<v Speaker 1>really bad effect of those on depletion, more so actually

486
00:31:17.200 --> 00:31:20.559
<v Speaker 1>than the burning up of re entering satellite. So this

487
00:31:20.720 --> 00:31:24.200
<v Speaker 1>is all looking like a pretty gloomy story for space,

488
00:31:24.279 --> 00:31:27.960
<v Speaker 1>that we're putting all this stuff into the atmosphere that

489
00:31:28.039 --> 00:31:29.759
<v Speaker 1>we could probably do without.

490
00:31:30.240 --> 00:31:34.279
<v Speaker 2>Well, unless somebody in authority acts quickly and says, okay,

491
00:31:34.319 --> 00:31:36.960
<v Speaker 2>you can't do that anymore. We know what could happen.

492
00:31:37.119 --> 00:31:39.200
<v Speaker 2>We don't want that to happen. You're going to have

493
00:31:39.200 --> 00:31:43.920
<v Speaker 2>to find another way. It sounds like a simple answer.

494
00:31:43.920 --> 00:31:44.599
<v Speaker 2>I'm sure it's not.

495
00:31:46.200 --> 00:31:46.720
<v Speaker 3>No, it's not.

496
00:31:46.920 --> 00:31:49.640
<v Speaker 1>I mean you're kind of reduced to something like the

497
00:31:49.680 --> 00:31:51.559
<v Speaker 1>space Elevator, which is probably.

498
00:31:51.319 --> 00:31:52.640
<v Speaker 3>A non starter anyway.

499
00:31:52.839 --> 00:31:58.359
<v Speaker 1>Yeah, so yeah, yeah, interesting, really interesting analysis.

500
00:31:58.960 --> 00:32:02.240
<v Speaker 2>Indeed, it's not good to finish on a down I

501
00:32:02.359 --> 00:32:06.200
<v Speaker 2>like that. But for all their achievements, there is a

502
00:32:06.200 --> 00:32:08.680
<v Speaker 2>price to pay, and it sounds like our atmosphere is

503
00:32:08.720 --> 00:32:12.000
<v Speaker 2>paying that price and we'll do for some time to

504
00:32:12.039 --> 00:32:14.440
<v Speaker 2>come unless something can be done about it. And there's

505
00:32:14.720 --> 00:32:17.920
<v Speaker 2>an alternative on the horizon, but it doesn't appear to

506
00:32:17.960 --> 00:32:19.720
<v Speaker 2>be the case. If you want to read that story,

507
00:32:20.039 --> 00:32:23.960
<v Speaker 2>as Fred said, it's on the space dot com website,

508
00:32:24.000 --> 00:32:28.279
<v Speaker 2>and that story about the SpaceX launchers is at fizz

509
00:32:28.319 --> 00:32:33.160
<v Speaker 2>phys fizz dot org. And don't forget if you would

510
00:32:33.200 --> 00:32:36.680
<v Speaker 2>like to contact us or visit our website, you can

511
00:32:36.759 --> 00:32:39.799
<v Speaker 2>do that. That's space Nuts podcast dot com or space

512
00:32:39.960 --> 00:32:45.000
<v Speaker 2>nuts dot io. And have a look around. Christmas isn't

513
00:32:45.039 --> 00:32:47.880
<v Speaker 2>far away. Maybe you want to get somebody a nice

514
00:32:48.039 --> 00:32:53.319
<v Speaker 2>space related gifty pooh, we've got them at our shop.

515
00:32:53.519 --> 00:32:56.519
<v Speaker 2>And if you want to be a supporter of space Nuts,

516
00:32:56.759 --> 00:33:00.759
<v Speaker 2>don't forget to click on the supporter tab and maybe

517
00:33:00.799 --> 00:33:03.440
<v Speaker 2>become a patron. We're not telling you to we would

518
00:33:03.480 --> 00:33:05.519
<v Speaker 2>never tell you to do that, but it's an option

519
00:33:05.759 --> 00:33:10.480
<v Speaker 2>and we certainly send our thanks out to the several

520
00:33:10.599 --> 00:33:12.119
<v Speaker 2>hundred members of.

521
00:33:12.279 --> 00:33:18.880
<v Speaker 1>Various patron based organized website who support Space Nuts.

522
00:33:18.880 --> 00:33:21.440
<v Speaker 2>We really do appreciate it. Thank you so very much.

523
00:33:21.480 --> 00:33:25.839
<v Speaker 2>Lots of benefits come with being a patron, which Hugh

524
00:33:26.200 --> 00:33:30.160
<v Speaker 2>looks after. So that's all on our website, Spacenuts podcast

525
00:33:30.240 --> 00:33:32.960
<v Speaker 2>dot com. Fred, We're all done, Thank you so much,

526
00:33:33.160 --> 00:33:34.279
<v Speaker 2>so nice to talk to.

527
00:33:34.279 --> 00:33:39.279
<v Speaker 3>You again, and I will speak again. I'm sure we will.

528
00:33:39.599 --> 00:33:41.640
<v Speaker 2>Could be a few minutes, could be a few days,

529
00:33:42.079 --> 00:33:45.279
<v Speaker 2>you never know. Professor Fred Wat's an astronomer at large.

530
00:33:45.279 --> 00:33:50.440
<v Speaker 1>And thanks to Hu in the studio for I'll get

531
00:33:50.480 --> 00:33:51.160
<v Speaker 1>back to you on that.

532
00:33:51.319 --> 00:33:54.119
<v Speaker 2>And from me Andrew Dunkley, thanks for your company. We'll

533
00:33:54.119 --> 00:33:56.359
<v Speaker 2>catch you again on the next episode.

534
00:33:55.960 --> 00:34:01.079
<v Speaker 1>Of Space Nuts. Bye bye, Sauts. Listening to the Space

535
00:34:01.200 --> 00:34:02.720
<v Speaker 1>Nuts podcast.

536
00:34:03.799 --> 00:34:09.800
<v Speaker 4>Available at Apple Podcasts, Spotify, iHeartRadio, or your favorite podcast player.

537
00:34:10.000 --> 00:34:13.119
<v Speaker 1>You can also stream on demand at bites dot com.

538
00:34:13.320 --> 00:34:19.000
<v Speaker 2>This has been another quality podcast production from nights dot com.
