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Hello, thanks for joining us. This is Space Nuts where
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we talk astronomy, space science and all the problems of
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the world that we cannot solve, and a few other
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things as well. But coming up on this episode, in fact,
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we are going to look at some new information that's
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come from Yes, you're right, the James Web Space Telescope.
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It has found six new rogue planets. Rogue or orphan planets.
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They're out there floating around. They don't have a star,
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no mum, no dad, They're just hanging around on street
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corners smoking joints. But we're going to find out more
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about these ones. We're also looking at doubts that have
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been raised about the existence of dark matter itself. Well,
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if it's not dark matter, what is it? And if
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it's dark matter, I don't know. There's been a study
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done and they've gone nothing to see here. And we're
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going to look at some new ideas around the Fermi
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parad and life in the universe. It's all coming up
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on this edition of Space Nuts fifteen.
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In Channel ten nine ignition sequence Space Nuts or three two.
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One Space Nurse and I reported Neils Good and unraveling
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the ravelment that is astronomy and space science is professor Fred.
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What's a hello bread?
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Hello Andrew, good to see you, Good to see you.
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To you today, you're looking rather dapper, dapper pinstrop suit
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you Well, yes, yes it's the shirt you see that
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because I spent the morning in far more official meetings
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that were in I spent the morning on the golf course.
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Well there you go, yes, do share, because see I'm
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a bit red in the face.
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Got some sun. Yes, we had a beautiful day today.
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It's spring has just gone. It's like drop gone us,
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like a giant ball, and it just all the cold
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weather just suddenly vanished. Yes, very very enjoyable. I spoke.
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I've probably spoken too soon. Next week we'll have snow.
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Except it is coming back. The cool weather's coming back,
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of course it is. We've got twenty nine degrees here today. Yeah,
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we've been up in the ridiculous for winter.
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Yeah, we're expecting. I think we're sespecially get twenty five
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today and twenty eight on Friday. Yes, it's insane, and
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yeah we're still technically in winter. Yeah, I wonder what's
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caused all that. Let's not go there, but we have
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got a lot to talk about. Fred and the first
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thing is a story that's gained a bit of traction
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in several on several websites, and that is a new
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thing from the James Webb Space Telescope. Six Wandering rogue
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Planets is one headline. Another one says James web Spot's
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new rogue Worlds or Planets. I guess we could start
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off by explaining exactly what a roague planet is. I
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think most people have got it in their minds well
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and truly, but a few might be going, what what
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on Earth is that? It's Yes, it's some. There's all
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sorts of reasons for them, but they are out there.
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That's correct. And I mean I always think rogue planets
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is a it's not a good name for these things.
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The sound naughty, yes, that's right. It gives them a
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bad look. Whereas you know, if you call them orphan planets,
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then your sympathies are much.
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More with them. Just so sad.
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Sad planets. Yeah, there's an afterronym that I remember writing
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about a long time ago. They were called f flops.
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F flops was free floating low something, but I can't remember.
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I can't remember what it was. I'd have to look
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look it up. And I've got time to do that now.
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But I thought, yes, flops kind of. I think it
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gave them a you know, a sort of tick of
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failure across of failure. Really, didn't it that they just
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haven't made it? They're flops, Really, they're not. They haven't
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made it. And in a way, that is what this
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story is about. Because whilst we've known about roade planets
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or often planets for several decades now, some of the
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first were discovered actually using the Angle Australian telescope if
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I remember rightly here in Australia, in the Orion Nebula.
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So the irin Nebula is a place, it's a region
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of staff formation. It's a place which became sort of
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reasonably well known for its orphan planets. But the question
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about them is where they came from. And there are two,
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basically two possibilities. One is that they formed in the
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normal way that planets form, from the proto planetary disc
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around a young star. And so you know, rogue planets
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sorry often planets, would have formed along with their siblings
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in that protoplanetary disc and then something happened that basically
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kicked them out, sent them wandering off into interstellar space
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with no Sun to orbit around. Maybe we should call
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them banished planets planets looking in the school toilets.
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That's what it was.
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Yeah, well that's the I suppose that's the equivalent of
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a gravitational interaction with another planetary body, which as the
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same thing. Really you still get you still get kicked out.
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So did they form in the way that all planets
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formed the normal planetary formation, and then get kicked out
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by some gravitational interaction, or did they form as the
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bottom realm if I can put it that way of
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the star formation process. So when stars four in clouds
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of gas and dust, which is where we know they
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are formed, and you know they form by these blobs
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of this gas and dust collapsing under its own gravity,
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and eventually that collapse produces a high enough temperature because
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of compression that you will get nuclear reactions taking place. Now,
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the clouds of gas and dust where we know stars
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form are multi faceted, and there is a suspicion that
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perhaps some of them, you know, you get little globs
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of gas and dust which collapses as though it was
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going to form a stun a sun, not a stun
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a star or a sun, but it doesn't have enough
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mass in there, so the compression never reaches the temperatures
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that you need to click nuclear reactions into being. So
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that's what you might call the top down model, where
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you've got you start off forming a star, but there's
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not enough material to form that star, and what you
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get is something with the mess of a planet. And
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that is, you know, a perfectly reasonable explanation for why
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these orphan planets or roade planets exist, and in a
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way that gets rid of the orphan bit because they've
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never had a parent star. They've always been objects that
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have formed directly from the raw material of stars, that's
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gas and dust. So this new observation has shed some
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light on that and it comes, as you said, from
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the James Webspace telescope. About half a dozen of these
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orphan planets, road planets, flops, whatever you want to call them,
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have been found without a star to orbit, and they
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are in the perseous molecular cloud. It's a region of
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oll ocules, is that as the name implies, which is
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basically gas, cold gas and dust, and it's in the
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constellation of Persius, the Northern Hemisphere constellation. So the planets
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which have been found have ranged between five and ten
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times the mass of Jupiter. And this is a sort
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of critical measurement because there is thinking that suggests anything
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less than that than five times the mass of Jupiter
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would have to have been formed in a bigger planetary
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system and then kicked out. So there's a sort of
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lower limit there on the formation of these And so
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what you're saying is that, you know, if there were,
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if you were seeing them less than five times the
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mass of Jupiter, then you could point to them having
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been formed elsewhere in a solar system and then kicked.
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Out, but there were the rants of the litter.
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Yeah, in that sense, that's right. Although five times the
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mass of Jupiter is pretty big, it is, I wouldn't
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call it that towards space, No, No, you rather, you
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certainly wouldn't want to do that. You could get into
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all kinds of trouble. So this observation tends to favor
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the idea that these things have formed as though there
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were going to be stars but haven't got that far.
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There is another limit.
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That that that applies to these objects, because anything that's
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more than thirteen times the mass of Jupiter becomes something else.
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That is what we call a brown dwarf star, because
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that is the mass in which what you might call
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low level nuclear processes kicking. It's basically deuterium burning. They
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call it fusion of deuteria. So anything above thirteen times
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the massive Jupiter will be a brown dwarf star.
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Speaking of woage trade, for those who are watching us,
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I've got a brown dwarf.
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Hang on, turn my Oh so you do.
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Yes, it's a terra Cotta warrior from China.
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Yes, that's right, there you go.
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But it fits in the palm of my hand, brown dwarf.
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Is it less than it must be more than thirteen
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times a massive Jupiter then if it's that, but just
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watch out for that deuterium fusion in the interior.
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I hope there's none in there.
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At the risk of wondering, if you and I are
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talking across purposes here, I'll carry on, yes and so yeah,
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So more than thirteen times a massive Jupiter, you've got
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a brown dwarf. More than ninety three times the mass
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of Jupiter, you've got a star. Yeah, because then you
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get the you've got enough mass to create hydrogen fusion.
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Fusion of hydrogen. It's to helium the normal nuclear process,
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so that it's it's an interesting set of observations that
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we've got that might draw a line under the question
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as to whether rogue planets often planets, whether they form
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alone in a top down process in other words, collapsing
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star cloud clouds of raw material of stars, or whether
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they're kicked out of their solar systems. And it looks
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as though it is the former rather than the latter.
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Yeah, so they're independently created and then then just float
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off into the into the ether. And then I guess
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what will likely happen to them is I'll just keep
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floating around out there doing not much.
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Yes, that's right. They'll indeed, they will, they'll, you know,
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they will evolve in a slow sort of way. They
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they're almost certainly gas giants. There is just one other
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sneaky input into this debate that came from these new observations,
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and that is that one of these rogue planets looks
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as though it has its own protoplanetary disk, in other words,
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a miniature version of what the Solar system would have
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looked like in its early history where the planets were formed,
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or what a solar system looks like it looks as
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though there's a sort of tiny replica of a solar
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system being formed around one of these rogue planets, which
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again points to the top down formation mechanism. In other words,
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they're formed by the collapse of small clouds of gas
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in a molecular cloud.
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That's fascinating. I also think during this study they found
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a brown dwarf that had its own planet, So that
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what would you call that? That's not a they're not
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rogue planets.
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That's a no, no, that's it might you might almost
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call it a binary system because the brown dwarf is
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low mass, the planet's probably quite high mass. The difference
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between one and the other is one's burning deuterium and.
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The other isn't. Yeah, wow, there's so much you know, this,
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James web Tap the space Telescope is starting to reveal
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to us. And even though it's which I've mentioned before,
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opening up so many more questions, it's also managing to
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answer some questions. And yeah, and we're only in the
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early phases of its role. It's mission. Who knows what
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else we'll discover. But if you're interested in reading that
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story about rogue planets, just do a search for it.
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There are so many platforms. Space dot com has done
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something on a Cosmos magazine, or if you want to
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put yourself to sleep and read the whole thing, it's
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in the Astronomical Journal. That's where they published the official paper. Yes,
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this is space Nut's Andrew Dunkley here with Professor Fred
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what's a.
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Murder you here? Space butts?
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Now, for doubts have been raised about the existence of
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dark matter. We get a lot of questions, surprisingly about
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dark matter, people wanting to know what it is, how
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we've managed to find it. You know, we haven't actually
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identified it. We just sort of know it's there because
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it has to be, otherwise things wouldn't add up. But
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now a new study has been published that's basically said, hey,
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we've looked for this stuff and no, I find it
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can't exist.
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Yeah, nobody's saying it can't exist.
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I just threw that in there for topical humor.
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Well yes, yeah, yes, don't misquote anybody though, So yes,
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So it's some results from a dark matter particle detector
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which is looking specifically for one candidate particle for the
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dark matter problem. So quick recap without there being something
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called dark matter galaxies wouldn't hold together. They'd rotate too
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fast to hold themselves together. And that's you know, that's
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one of the main reasons why we think dark matter
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is present, plus the fact that we see evidence for
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it with gravitational lensing and things of that sort. But
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it's not detectable by normal means because it doesn't seem
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to interact with normal particles in any way other than
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by gravity. It doesn't interact, you know, from a nuclear standpoint,
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it doesn't interact from any kind of electromagnetic interaction, in
241
00:15:53.799 --> 00:15:56.440
other words, interact with photons, none of that. Doesn't want
242
00:15:56.480 --> 00:16:01.759
to know, but it seems to exist. Now, multiple candidates
243
00:16:01.759 --> 00:16:04.559
have been proposed for what that particle might be, and