Black Hole Temperatures, Cosmic Mapping & the Mystery of Dark Matter| Q&A | Space Nuts:...
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Temperature of Black Holes, Cosmic Mapping, and the Nature of Space
In this thought-provoking episode of Space Nuts , hosts Andrew Dunkley and Professor Fred Watson tackle some of the most intriguing questions from their audience. Join them as they delve into the chilling temperatures of black holes, the expansive mapping of the universe by cutting-edge telescopes, and the enigmatic nature of space itself.
Episode Highlights:
- The Temperature of Black Holes: Andrew and Fred discuss Casey's question regarding the temperature of black holes. They explore the stark contrast between the scorching accretion disks and the surprisingly frigid temperatures within the event horizons, shedding light on the complexities of black hole physics.
- Mapping the Universe: Eli's inquiry about the James Webb and Vera Rubin telescopes leads to a fascinating discussion on how much of the universe has been mapped and what we can expect in the coming decade. The hosts highlight the capabilities of these telescopes and the potential discoveries that await.
- The Emptiness of Space: Robert poses a thought-provoking question about the nature of space and the Higgs boson. Andrew and Fred unravel the concept of the Higgs field, discussing its implications for our understanding of the universe and whether space is truly empty or filled with these elusive particles.
- The Impact of Dark Matter and Energy: Rennie challenges the hosts to consider how discovering the true nature of dark matter and dark energy might affect life on Earth. Andrew and Fred reflect on the long-term benefits of such knowledge, drawing parallels to historical scientific advancements.
For more Space Nuts, including our continuously updating newsfeed and to listen to all our episodes, visit our website. (https://www.spacenutspodcast.com/) Follow us on social media at SpaceNutsPod on Facebook, Instagram, and more. We love engaging with our community, so be sure to drop us a message or comment on your favorite platform.
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Stay curious, keep looking up, and join us next time for more stellar insights and cosmic wonders. Until then, clear skies and happy stargazing.
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Episode link: https://play.headliner.app/episode/31318370?utm_source=youtube
Kind: captions
Language: en
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Hi there. Thanks for joining us again.
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This is a Q&A uh edition of Space Nuts,
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where we uh take audience questions and
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we pretend that we know what we're
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talking about in attempting to answer
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them or we get it right sometimes, too.
00:00:15.599 --> 00:00:18.790
Uh today we're going to be answering a
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question about uh the temperature of
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black holes. Uh I I'm not sure we've
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been there before. It may have come up,
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but um I can't remember when. uh and a
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question uh asking with the James Webb
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Space Telescope and the Vera Rubin
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telescope how much of the universe has
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been mapped. I can tell you this much uh
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and the emptiness of space is being
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questioned and what difference will it
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make to humanity uh if we find dark
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matter and dark energy? Um that's a
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really interesting question and Fred
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knows the answer. We'll ask him shortly
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on this edition of Space Nuts.
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>> 15 seconds. Guidance is internal. 10 9
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Ignition sequence start.
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>> Space nuts.
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>> 5 4 3 2
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>> 1 2 3 4 5 5 4 3 2 1
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>> Space Nuts.
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>> Astronauts report. It feels good.
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>> And he's back. And he has all the
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answers to all the questions of life,
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the universe, and everything. Professor
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Fred Watson, astronomer at large. Hello,
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Fred.
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No pressure there, Andrew.
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>> None at all. None at all.
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>> No pressure. That's right.
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>> Uh let's get straight into it, shall we?
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Um uh one of our regular contributors is
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Casey, who has a very interesting
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question about a subject we never
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discuss, black holes.
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>> Hi guys, this is Casey from Colorado and
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I was thinking about the temperature of
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black holes. I know that the accretion
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disc would be very hot, but I was
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wondering once you get past the event
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horizon if it would be hot or cold. Why
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do we think this? Thanks for the podcast
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and I hope you're both well. Thanks.
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>> Thank you, Casey. She's got me thinking
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about the temperature in Colorado
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because like we're facing some horrific
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temperatures around here at the moment,
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but I' i'd imagine it'd be quite the
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opposite in Colorado this time of the
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year.
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Yeah, I think that's that's absolutely
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right. Yes. But part of the world in
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winter.
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>> Absolutely. Um, now temperature of black
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holes. This this one's interesting
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because I suppose it varies on several
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factors. Um, where you are, what you're
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doing.
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I don't know what
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I would like. It's not like the not like
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the temperature of the sun, is it?
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>> No. No, it's not. Um, it's it's a re I'm
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I'm so glad Casey asked this question
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because it sent me down a rabbit hole I
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haven't been down before.
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>> Oh, wow.
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>> Uh, in and it leads you straight to
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quantum theory. Uh, uh, and um, it's,
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you know, it's a it really in a sense
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it's quite unexpected
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uh, what's what's happening. Uh so um
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the bottom line is whilst as Casey
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exactly as Casey says the accretion disc
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of the black hole is extremely hot uh
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and you know we're talking millions of
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degrees there because this that's where
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you get X-ray radiation from. It's the
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the stuff charging around the accretion
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disc uh that's uh swirling around the
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the black hole itself. But the black
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hole itself
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is the opposite. It's really really
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cold. Um, and basically, uh, it's
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because the the amount of radiation
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that they, uh, that they release is at a
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level uh, which means its temperature is
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measured in gazillionth of a degree.
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It's virtually absolute zero.
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um they they
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basically they're
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it's quite a a nice way of putting it um
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which which I've uh summarized uh I
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think this comes from Wikipedia. It may
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come from AI actually. But the bottom
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line is even though black holes pull in
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matter and energy, their temperature is
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incredibly low because their large mass
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makes their event horizons effectively
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cold thermal emitters, absorbing energy
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faster than they radiate it at these
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scales. So that's the key to what's
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happening that like everything else,
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black holes suck stuff. it sucks stuff
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in uh and that stuff is matter which is
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equivalent to energy uh and because it's
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stuff that's going in and not radiating
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outwards uh even though there is what we
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call Hawking radiation which I'll get to
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in a second but that that um you know
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the uh what it means is that the the
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fact that there there's an energy input
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into the black hole it means that to the
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outside observer they look cold. They
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look very very cold. There is a
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relationship as you said uh we it might
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vary with some things and what it varies
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with uh is actually the mass of the
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black hole. Uh it's it's roughly uh an
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inverse proportionality proportionality
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the the temperature is inversely
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proportional to the mass. Um, and what
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that means is for super massive black
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holes, they are extremely cold. Uh, and
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that sort of figures because they're
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sucking in more energy and so the
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surface to an outside observer would
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look colder. Uh, they're talking about
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10 the minus14° Kelvin. U something with
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the mass of the sun um is a barmy 10us
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7° Kelvin. It's still virtually zero,
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but it's more uh more than the super
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massive black holes. So something the
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mass of the sun. So it's inversely
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proportional to the mass uh that inverse
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relationship. Uh and so so that's that's
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kind of what it's the Hawking radiation
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that gives the black hole a temperature
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essentially. It's because it's it's
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emitting radiation. Um, and we've talked
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about Hawking radiation before. Even
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though everything gets sucked into a
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black hole, there's this quantum
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situation where you can get um two
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virtual particles being created from
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nothing in empty space. One gets trapped
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by the black hole, the other doesn't.
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And so we see that as Hawking radiation
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uh suggested by Steven Hawking in the
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1970s now very well established. Uh but
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yeah to summarize the bottom line is
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Casey's uh question is a good one uh
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because it turns out that black holes
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are very very cold indeed despite the
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intense heat of the accretion disc. Work
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that one out. It's a really hard thing
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to to put your imagination around.
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>> I suppose you'd compare it to the heat
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on the It's got nothing to do with it at
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all, but by example the heat on the sun
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side of Mercury versus the cool on the
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shadow side. They're so extreme.
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>> Um.
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>> Yes. Yeah, that's right.
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>> For the same reason.
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>> Well, similar because the dark side of
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Mercury is cold uh because it's
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radiating energy into space.
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>> Um uh whereas uh and that that energy
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loss reduces the temperature. Whereas
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with a black hole, it's the other way
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around. The thing is the thing is
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sucking energy in at a greater rate than
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it's emitting energy. Uh so Mercury
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would Mercury's dark side would lose
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heat by infrared radiation. Um that
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radiation in the case of a black hole is
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is much smaller than the radiation that
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it's sucking in which is why it looks
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extremely cold. Uh so I'm trying to I'm
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trying to make sense of the parallel
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that you drew and I think it's I think
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it holds water Andrew. I think I think
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it's a good good answer.
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>> Well, actually the water will probably
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evaporate or freeze but anyway um
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>> freeze it.
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>> Uh I just thought of a question. Um so
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if a black hole sort of,
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you know, runs out of food, would that
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cause an alteration in its temperature?
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Um,
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I don't think so because I think once
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the I I get what you're saying and
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certainly in the argument that we've
00:08:45.760 --> 00:08:48.790
just been talking about, you'd think
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that if it's not sucking in energy
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anymore,
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>> uh, it it or sucking in matter anymore,
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it it would uh it would actually change
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its uh change its temperature. Um the
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reason why I think that might not happen
00:09:01.839 --> 00:09:04.389
is because the only thing that uh the
00:09:04.399 --> 00:09:06.550
temperature seems to be related to is
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the mass itself. So um there must be a
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mechanism and I'm sorry it's eluding me
00:09:12.000 --> 00:09:14.070
at the moment. Uh but there must be a
00:09:14.080 --> 00:09:16.070
mechanism that sort of locks once you've
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once you've got a a a black hole of
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sufficient mass um then uh its
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temperature is sort of locked in. Uh it
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must still be taking in energy in the
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form of radiation. So perhaps that's
00:09:31.040 --> 00:09:32.949
what's what's happening. you know, light
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light certainly gets sucked into a black
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hole that even even if it's not got an
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accretion disc of stuff to to feed on,
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uh the light certainly going in and
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perhaps that's enough to keep the
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temperature as low as we've described.
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Indeed. All right. Uh thanks Casey.
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Lovely to hear from you. Hope you're
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coping with the uh - 10^ the 15° Kelvin
00:09:54.800 --> 00:09:58.870
in Colorado. Uh our next question comes
00:09:58.880 --> 00:10:01.350
from Eli. Hello space fairers. I'm
00:10:01.360 --> 00:10:04.870
writing from the Coachella Valley desert
00:10:04.880 --> 00:10:07.350
here in Southern California. Uh, I've
00:10:07.360 --> 00:10:09.430
often thought some of the Google
00:10:09.440 --> 00:10:11.750
Earthlike software would be amazing to
00:10:11.760 --> 00:10:13.750
take into other galaxies throughout the
00:10:13.760 --> 00:10:17.030
universe. Intriguingly, I imagine you
00:10:17.040 --> 00:10:18.870
could take them back in time according
00:10:18.880 --> 00:10:21.350
to estimates of cosmic inflation, etc.
00:10:21.360 --> 00:10:24.470
all the way to the big bang in theory.
00:10:24.480 --> 00:10:26.870
um to his question with James Webb and
00:10:26.880 --> 00:10:29.509
the Vera Rubin coming online how much of
00:10:29.519 --> 00:10:32.389
the visible visible universe have we
00:10:32.399 --> 00:10:34.710
basically mapped and how much are we
00:10:34.720 --> 00:10:38.230
projected to map in say the next decade
00:10:38.240 --> 00:10:41.190
I think we've actually talked about how
00:10:41.200 --> 00:10:43.750
much that they're going to look at and
00:10:43.760 --> 00:10:45.750
how long it's going to take and I I I
00:10:45.760 --> 00:10:47.269
think Eli's going to be quite surprised
00:10:47.279 --> 00:10:50.550
by the answer
00:10:50.560 --> 00:10:53.269
well yes that's right I mean the the key
00:10:53.279 --> 00:10:55.670
words here are the Vera Vera Rubin
00:10:55.680 --> 00:10:59.269
Observatory uh because that will map the
00:10:59.279 --> 00:11:03.030
entire sky down to quite a significant
00:11:03.040 --> 00:11:08.389
depth not as deep as the web will um
00:11:08.399 --> 00:11:10.470
although it is an 8 m telescope the web
00:11:10.480 --> 00:11:12.790
is only 6 and a half mters so it's
00:11:12.800 --> 00:11:15.430
probably not far short of it uh the web
00:11:15.440 --> 00:11:17.350
of course looking in infrared and the
00:11:17.360 --> 00:11:19.670
Vera Rubin telescope looking in visible
00:11:19.680 --> 00:11:21.430
light but it's going to it's going to
00:11:21.440 --> 00:11:25.190
photograph the whole sky southern sky uh
00:11:25.200 --> 00:11:30.069
in uh every three three nights or so. So
00:11:30.079 --> 00:11:32.710
that will build up over the years a map
00:11:32.720 --> 00:11:34.310
of the things that don't change. I mean
00:11:34.320 --> 00:11:35.750
what it's looking for is things that do
00:11:35.760 --> 00:11:39.670
change but um as you integrate for all
00:11:39.680 --> 00:11:42.230
that time and by that I mean you you you
00:11:42.240 --> 00:11:44.710
know expose the detector to the sky so
00:11:44.720 --> 00:11:46.790
that you build up the image uh and you
00:11:46.800 --> 00:11:48.870
can add all those images together. We'll
00:11:48.880 --> 00:11:52.790
have we'll have a almost a complete map
00:11:52.800 --> 00:11:54.710
of the universe in the southern
00:11:54.720 --> 00:11:57.269
hemisphere because uh all the visible
00:11:57.279 --> 00:12:01.750
galaxies will show up. Uh the they we
00:12:01.760 --> 00:12:03.670
won't see the first galaxies. I don't
00:12:03.680 --> 00:12:05.910
think it's going to be powerful enough
00:12:05.920 --> 00:12:09.110
to see those. But uh and we're not sure
00:12:09.120 --> 00:12:10.790
even that the web has seen the first
00:12:10.800 --> 00:12:13.110
galaxies. Uh it's certainly seen some
00:12:13.120 --> 00:12:15.110
galaxies that we think are very early in
00:12:15.120 --> 00:12:16.949
the history of the universe. And I think
00:12:16.959 --> 00:12:19.670
the Verus Cy Rubin observatory will do
00:12:19.680 --> 00:12:22.949
the same thing. Uh but um you know so
00:12:22.959 --> 00:12:26.069
we're not in any sense getting a
00:12:26.079 --> 00:12:29.590
complete sense of the consens sorry a
00:12:29.600 --> 00:12:33.190
complete census of the universe. Uh but
00:12:33.200 --> 00:12:35.829
it's not going to be far off. Uh, and
00:12:35.839 --> 00:12:38.310
that's quite astonishing when you think
00:12:38.320 --> 00:12:40.230
of where we were, you know, well, just a
00:12:40.240 --> 00:12:42.790
few years ago, certainly when I was a a
00:12:42.800 --> 00:12:45.509
young working astronomer in the 1970s, I
00:12:45.519 --> 00:12:47.990
would have had my somebody It would have
00:12:48.000 --> 00:12:50.389
blown my mind to think that we could map
00:12:50.399 --> 00:12:54.230
all the galaxies uh in one hemisphere of
00:12:54.240 --> 00:12:55.750
the universe.
00:12:55.760 --> 00:12:57.509
>> Yeah. Uh, what about the northern
00:12:57.519 --> 00:13:00.389
hemisphere? Is there any
00:13:00.399 --> 00:13:05.990
>> work equivalent? uh the the there is I
00:13:06.000 --> 00:13:08.550
mean the Nancy Roman space telescope
00:13:08.560 --> 00:13:10.949
will look it's also a wide angle
00:13:10.959 --> 00:13:13.670
telescope like the the Ruben Observatory
00:13:13.680 --> 00:13:18.069
instrument is but um it's not as big
00:13:18.079 --> 00:13:22.069
it's a um it is a 2.3 meter telescope
00:13:22.079 --> 00:13:23.990
basically a Hubble Hubble telescope but
00:13:24.000 --> 00:13:26.710
with a wide field of view. Uh so we'll
00:13:26.720 --> 00:13:29.509
we'll certainly see uh pretty deep into
00:13:29.519 --> 00:13:30.949
the northern hemisphere. Whether it will
00:13:30.959 --> 00:13:32.949
go as deep as the Reuben Observatory,
00:13:32.959 --> 00:13:34.310
it's a different matter. I don't think
00:13:34.320 --> 00:13:35.750
it will because it's a much smaller
00:13:35.760 --> 00:13:37.829
telescope, but it is in space and that
00:13:37.839 --> 00:13:40.230
gives it excuse me that gives it
00:13:40.240 --> 00:13:42.389
advantages. There's no atmosphere to to
00:13:42.399 --> 00:13:45.190
get in the way. So that's perhaps the
00:13:45.200 --> 00:13:51.190
best bet. Um the excuse me, the other uh
00:13:51.200 --> 00:13:52.870
big instruments, I mean, there's a
00:13:52.880 --> 00:13:56.710
number of things going on. Um, in terms
00:13:56.720 --> 00:13:58.710
of the two kek telescopes which are in
00:13:58.720 --> 00:14:00.069
the northern hemisphere in Hawaii,
00:14:00.079 --> 00:14:02.550
they're 8 mclass telescopes, but they're
00:14:02.560 --> 00:14:04.310
not wide angle. These are telescopes
00:14:04.320 --> 00:14:07.430
that are built to home in in detail on
00:14:07.440 --> 00:14:09.990
individual objects rather than to do
00:14:10.000 --> 00:14:12.790
wide angle surveys. You need a specially
00:14:12.800 --> 00:14:14.310
designed telescope for that and the
00:14:14.320 --> 00:14:17.829
Reuben is exactly that. Um,
00:14:17.839 --> 00:14:21.430
there isn't really an equivalent. Uh
00:14:21.440 --> 00:14:23.990
there is a wide-angle telescope in La
00:14:24.000 --> 00:14:26.790
Palma which is um the basically the same
00:14:26.800 --> 00:14:28.629
as our UK Schmidt telescope here in
00:14:28.639 --> 00:14:30.150
Australia. It's called the Ocean Schmidt
00:14:30.160 --> 00:14:31.990
telescope. It's much older than our
00:14:32.000 --> 00:14:33.269
Schmidt. In fact, our Schmidt was
00:14:33.279 --> 00:14:35.030
modeled on it and that's a wide angle
00:14:35.040 --> 00:14:37.269
telescope that's surveying the sky, but
00:14:37.279 --> 00:14:39.030
that's looking for things like nearear
00:14:39.040 --> 00:14:40.790
asteroids and things of that sort rather
00:14:40.800 --> 00:14:43.189
than penetrating deep into the universe
00:14:43.199 --> 00:14:45.590
because it's only got a 1.2 2 meter
00:14:45.600 --> 00:14:48.550
aperture diameter much smaller than the
00:14:48.560 --> 00:14:50.389
eight meters that the Rubid telescope
00:14:50.399 --> 00:14:51.509
will have.
00:14:51.519 --> 00:14:53.189
>> Yeah.
00:14:53.199 --> 00:14:55.910
still um what we'll know in 10 years
00:14:55.920 --> 00:14:59.269
time will be extraordinary uh through
00:14:59.279 --> 00:15:01.590
through these two telescopes alone the
00:15:01.600 --> 00:15:05.430
James Webb and Vera Rubin um yeah who
00:15:05.440 --> 00:15:08.550
knows what they're going to un unveil uh
00:15:08.560 --> 00:15:11.430
and and what what have you know Vera
00:15:11.440 --> 00:15:12.949
Rubin's first photograph was a
00:15:12.959 --> 00:15:17.750
revelation uh and what James Webb is um
00:15:17.760 --> 00:15:20.230
is is shelling out is is extraordinary
00:15:20.240 --> 00:15:23.910
it It's It's like um I don't know,
00:15:23.920 --> 00:15:25.750
Taylor Swift. It's a hit record every
00:15:25.760 --> 00:15:27.910
time that every time they release a
00:15:27.920 --> 00:15:29.110
picture.
00:15:29.120 --> 00:15:31.990
>> It's uh it's incredible. So, Eli, the
00:15:32.000 --> 00:15:34.790
next decade will be extraordinary. Um
00:15:34.800 --> 00:15:37.509
so, just, you know, keep an eye on it
00:15:37.519 --> 00:15:39.750
would be my advice. And thanks for the
00:15:39.760 --> 00:15:42.310
question. This is Space Nuts with Andrew
00:15:42.320 --> 00:15:45.990
Dunley and Professor Fred Watson.
00:15:46.000 --> 00:15:47.509
Let's take a break from the show to tell
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>> 3 2 1
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>> Spacenuts.
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I think we have an audio question now.
00:17:37.360 --> 00:17:39.110
This one comes from one of our regulars
00:17:39.120 --> 00:17:40.150
as well.
00:17:40.160 --> 00:17:42.789
>> Hello Fred, Andrew, Jonty, and Heidi.
00:17:42.799 --> 00:17:45.669
This is Robert from the Netherlands.
00:17:45.679 --> 00:17:48.710
I have a question for you guys about the
00:17:48.720 --> 00:17:51.190
emptiness of space.
00:17:51.200 --> 00:17:54.230
Now, everybody is always saying that
00:17:54.240 --> 00:17:56.470
space is totally empty, right? One
00:17:56.480 --> 00:17:59.110
proton per square breeder, something
00:17:59.120 --> 00:18:03.510
like that. However, not that long ago,
00:18:03.520 --> 00:18:06.070
scientists did discover the Higs Bzon
00:18:06.080 --> 00:18:10.789
particle, the God particle, if you will.
00:18:10.799 --> 00:18:14.549
So apparently everything is on this grid
00:18:14.559 --> 00:18:18.789
of hex boss, but I'm not exactly an
00:18:18.799 --> 00:18:21.029
expert here. I'm just curious if you
00:18:21.039 --> 00:18:22.470
guys could shed some lights on this
00:18:22.480 --> 00:18:25.669
concept for me. So is it just an
00:18:25.679 --> 00:18:28.230
enormous field of these very regular
00:18:28.240 --> 00:18:31.430
hobbons everywhere in desal spaces or
00:18:31.440 --> 00:18:34.070
are they more numerous or less dense in
00:18:34.080 --> 00:18:37.270
certain parts? Is the void between
00:18:37.280 --> 00:18:40.310
galaxies actually a void? or is it an
00:18:40.320 --> 00:18:43.909
empty field of God particles?
00:18:43.919 --> 00:18:45.909
I really hope you can shed some lights.
00:18:45.919 --> 00:18:49.350
Thank you guys so much for answering.
00:18:49.360 --> 00:18:51.029
Thank you, Robert. Good to hear from
00:18:51.039 --> 00:18:55.350
you. Uh the emptiness of space. So he
00:18:55.360 --> 00:18:58.230
said one proton per square meter. Is
00:18:58.240 --> 00:19:01.350
that um a reasonable
00:19:01.360 --> 00:19:04.070
>> uh yeah per cubic meter? something
00:19:04.080 --> 00:19:06.070
something like that. Um
00:19:06.080 --> 00:19:09.990
>> yeah um it's uh it's of that order I
00:19:10.000 --> 00:19:14.630
think in in intergalactic space. Um
00:19:14.640 --> 00:19:18.870
uh but uh Robert's right in the sense
00:19:18.880 --> 00:19:24.070
that the Higs field which is the other
00:19:24.080 --> 00:19:28.390
way of looking at the Higs Bzon
00:19:28.400 --> 00:19:31.669
permeates basically permeates empty
00:19:31.679 --> 00:19:36.470
space. Um so
00:19:36.480 --> 00:19:39.669
uh this is all about the duality of
00:19:39.679 --> 00:19:41.510
particles
00:19:41.520 --> 00:19:44.789
uh with waves and with what we call
00:19:44.799 --> 00:19:48.070
fields. Um and we I mean we imagine
00:19:48.080 --> 00:19:49.990
fields when we think of gravitation
00:19:50.000 --> 00:19:52.230
because we think of a a gravitational
00:19:52.240 --> 00:19:55.909
field as a as a as a a
00:19:55.919 --> 00:19:59.110
sort of a a well if I can put it that
00:19:59.120 --> 00:20:01.750
way in a in a trampoline. Uh the
00:20:01.760 --> 00:20:03.029
trampolines, the field, you put
00:20:03.039 --> 00:20:05.190
something in it and it it distorts it.
00:20:05.200 --> 00:20:05.510
>> Yeah.
00:20:05.520 --> 00:20:10.070
>> Uh so with the Higs uh Bzon, the Higs
00:20:10.080 --> 00:20:14.470
field uh is this sort of invisible. It's
00:20:14.480 --> 00:20:16.470
been described as a something like
00:20:16.480 --> 00:20:21.110
molasses or syrup. Uh that what actually
00:20:21.120 --> 00:20:23.830
give particles their mass because um
00:20:23.840 --> 00:20:25.750
they move slowly through it because they
00:20:25.760 --> 00:20:28.549
get sticky. Uh that's one way of looking
00:20:28.559 --> 00:20:32.390
at it. Um but uh the Higs Bzon is
00:20:32.400 --> 00:20:36.470
essentially a um in in a in a sense uh a
00:20:36.480 --> 00:20:39.830
ripple in the Higs field. The Higs field
00:20:39.840 --> 00:20:43.270
fills space and the Higs Bzons uh are
00:20:43.280 --> 00:20:45.990
ripples in it. That's one way uh to look
00:20:46.000 --> 00:20:52.070
at it. Um it's it's uh
00:20:52.080 --> 00:20:54.470
the I think what Robert's interested in
00:20:54.480 --> 00:20:58.789
is the density of these Bzons.
00:20:58.799 --> 00:21:02.070
uh whether they are uniformly
00:21:02.080 --> 00:21:05.029
uh distributed through space or whether
00:21:05.039 --> 00:21:10.470
we're talking about um you know uh Bzons
00:21:10.480 --> 00:21:14.789
uh that are
00:21:14.799 --> 00:21:16.950
more dense in some places than than
00:21:16.960 --> 00:21:21.510
others. uh and I I guess the the bottom
00:21:21.520 --> 00:21:22.950
line is that you would expect there to
00:21:22.960 --> 00:21:27.350
be more Bzons where there is more uh
00:21:27.360 --> 00:21:30.549
more uh what you might call normal
00:21:30.559 --> 00:21:32.710
matter the the quarks and normal
00:21:32.720 --> 00:21:34.950
particles but that might not be the
00:21:34.960 --> 00:21:36.950
case. Uh I need to look at that a little
00:21:36.960 --> 00:21:38.549
bit more carefully Andrew as you can
00:21:38.559 --> 00:21:41.430
probably tell uh to to find out what the
00:21:41.440 --> 00:21:44.470
distribution of Higs Bzons are. If you
00:21:44.480 --> 00:21:46.070
assume the Higs field is uniform
00:21:46.080 --> 00:21:47.669
throughout space, which I think it might
00:21:47.679 --> 00:21:48.950
be.
00:21:48.960 --> 00:21:50.630
>> Yeah, I suppose so. I mean, it's a
00:21:50.640 --> 00:21:52.390
complicated area. You're talking about
00:21:52.400 --> 00:21:54.230
particle physics, aren't you? Really?
00:21:54.240 --> 00:21:55.510
It's um it's not
00:21:55.520 --> 00:21:57.029
>> I believe so. Yes.
00:21:57.039 --> 00:22:00.789
>> It's not it's not basic maths. So, um
00:22:00.799 --> 00:22:02.230
>> yeah, it's particle physics we're
00:22:02.240 --> 00:22:04.310
talking about. And um as as I've said
00:22:04.320 --> 00:22:05.830
before, the disclaimer is I'm not a
00:22:05.840 --> 00:22:09.430
particle physicist. I've been to been to
00:22:09.440 --> 00:22:12.470
CERN a few times and had my mind blown
00:22:12.480 --> 00:22:13.830
by what they do there at the Large
00:22:13.840 --> 00:22:15.669
Hadron Collider. In fact, I've been
00:22:15.679 --> 00:22:17.909
underground in the Ladron Collider, but
00:22:17.919 --> 00:22:19.750
I'm still not a physicist, a particle
00:22:19.760 --> 00:22:23.270
physicist. I uh learn what they they
00:22:23.280 --> 00:22:25.990
tell me and kind of hope for the best.
00:22:26.000 --> 00:22:28.390
>> Yeah. Aren't they making a larger Hedron
00:22:28.400 --> 00:22:30.549
collider?
00:22:30.559 --> 00:22:34.950
uh they are planning one um something
00:22:34.960 --> 00:22:36.950
called
00:22:36.960 --> 00:22:38.470
uh
00:22:38.480 --> 00:22:40.230
I can't remember it's something like the
00:22:40.240 --> 00:22:42.470
large you know the future large collider
00:22:42.480 --> 00:22:44.870
I think something like that uh which
00:22:44.880 --> 00:22:46.870
whereas the large hydron collider has a
00:22:46.880 --> 00:22:49.110
diameter or a circumference of 27
00:22:49.120 --> 00:22:52.789
kilometers this is 100 kilometers
00:22:52.799 --> 00:22:55.110
um if they ever get the money for it
00:22:55.120 --> 00:22:57.029
they are planning an opening ceremony
00:22:57.039 --> 00:23:00.470
for it in 2070
00:23:00.480 --> 00:23:03.350
It's called the uh future circular
00:23:03.360 --> 00:23:03.750
collider.
00:23:03.760 --> 00:23:05.430
>> Future circular collider. That's it.
00:23:05.440 --> 00:23:08.630
>> Um 91 km ring successor to the large
00:23:08.640 --> 00:23:11.029
hedron collider.
00:23:11.039 --> 00:23:15.350
>> And they expect it to be approved.
00:23:15.360 --> 00:23:18.470
Then the 2728 financial year by the look
00:23:18.480 --> 00:23:19.909
of it. Construction starting in the
00:23:19.919 --> 00:23:22.789
2030s. So it's a little way off.
00:23:22.799 --> 00:23:25.029
>> Completion 2070.
00:23:25.039 --> 00:23:26.549
>> 2070.
00:23:26.559 --> 00:23:27.029
Lime.
00:23:27.039 --> 00:23:28.630
>> Yeah.
00:23:28.640 --> 00:23:31.990
That's where the last let's not hold it
00:23:32.000 --> 00:23:35.590
is what I saw. Yeah. So I don't think um
00:23:35.600 --> 00:23:37.590
I I you know even with the best will in
00:23:37.600 --> 00:23:40.230
the world space will probably have
00:23:40.240 --> 00:23:42.149
dwindled to an audience measured in
00:23:42.159 --> 00:23:44.230
single digits by then. So
00:23:44.240 --> 00:23:47.909
>> possibly possibly so yes uh more could
00:23:47.919 --> 00:23:49.430
pick up new listeners along the way but
00:23:49.440 --> 00:23:51.990
we won't know about it. But um I I
00:23:52.000 --> 00:23:53.750
suppose the other side to this question
00:23:53.760 --> 00:23:56.710
though is that we do see concentrations
00:23:56.720 --> 00:23:59.909
of particles in some parts of the
00:23:59.919 --> 00:24:02.310
universe uh like dark matter seems to
00:24:02.320 --> 00:24:05.350
concentrate around galaxies
00:24:05.360 --> 00:24:06.310
kind of thing. Is that
00:24:06.320 --> 00:24:07.110
>> Yeah,
00:24:07.120 --> 00:24:09.510
>> that a different kettle of fish.
00:24:09.520 --> 00:24:11.830
>> I I think so because we're talking about
00:24:11.840 --> 00:24:14.950
something that is um a property of the
00:24:14.960 --> 00:24:19.669
universe itself almost. Um,
00:24:19.679 --> 00:24:24.149
so that the Higs field is everywhere.
00:24:24.159 --> 00:24:26.390
>> Okay. Gotcha. I understand. No, I get
00:24:26.400 --> 00:24:27.909
it. I get it. Yeah. All right.
00:24:27.919 --> 00:24:28.549
>> Yeah.
00:24:28.559 --> 00:24:31.590
>> So, Robert, the answer is um maybe
00:24:31.600 --> 00:24:33.830
possibly could be. Uh, we need to do a
00:24:33.840 --> 00:24:36.390
bit more homework by the sound of it.
00:24:36.400 --> 00:24:37.830
>> We might be able to get back to you on
00:24:37.840 --> 00:24:39.350
that.
00:24:39.360 --> 00:24:41.909
>> Just Fred's writing a note so he doesn't
00:24:41.919 --> 00:24:43.990
forget. Except he'll forget where the
00:24:44.000 --> 00:24:45.510
note is. Shh.
00:24:45.520 --> 00:24:47.029
>> All right.
00:24:47.039 --> 00:24:49.430
It's in this book.
00:24:49.440 --> 00:24:52.710
Thanks, Robert.
00:24:52.720 --> 00:24:55.590
>> Okay, we checked all four systems and
00:24:55.600 --> 00:24:57.029
>> Space Nets.
00:24:57.039 --> 00:25:00.390
>> And our final question comes from Renie.
00:25:00.400 --> 00:25:02.789
Uh, this is a really interesting
00:25:02.799 --> 00:25:04.230
question because he says, I'm going to
00:25:04.240 --> 00:25:06.149
play devil's advocate with this
00:25:06.159 --> 00:25:09.830
question. How will finding out what dark
00:25:09.840 --> 00:25:12.710
matter and dark energy really are help
00:25:12.720 --> 00:25:16.789
the earth and all uh of its life now and
00:25:16.799 --> 00:25:19.269
in the future? Renie from California.
00:25:19.279 --> 00:25:21.510
We've had a few US questions this week.
00:25:21.520 --> 00:25:24.710
That's nice. Two from Cali. Uh so yeah,
00:25:24.720 --> 00:25:26.230
what difference will it make if we find
00:25:26.240 --> 00:25:30.070
this stuff to Earth and life as it is
00:25:30.080 --> 00:25:33.510
now and in the future?
00:25:33.520 --> 00:25:37.430
Um so um yeah if if we magically did
00:25:37.440 --> 00:25:40.070
find the answer to these things and we
00:25:40.080 --> 00:25:43.430
will eventually uh over a period of time
00:25:43.440 --> 00:25:45.510
I hope it's not till not be I hope it's
00:25:45.520 --> 00:25:49.350
before 2070 because I want to know um it
00:25:49.360 --> 00:25:51.990
it what it will do will be complete our
00:25:52.000 --> 00:25:54.950
understanding of the universe in a way
00:25:54.960 --> 00:25:58.630
that it it's not the case at the moment.
00:25:58.640 --> 00:26:03.190
So um it it basically refineses our
00:26:03.200 --> 00:26:04.789
understanding
00:26:04.799 --> 00:26:07.269
uh in a if I can put it this way in a
00:26:07.279 --> 00:26:11.510
way that's similar to the way general
00:26:11.520 --> 00:26:13.190
relativity
00:26:13.200 --> 00:26:17.830
refined it back in 1915.
00:26:17.840 --> 00:26:21.029
Um, so the fact that we suddenly
00:26:21.039 --> 00:26:23.669
understood gravity, the way gravity
00:26:23.679 --> 00:26:26.870
works in a new light, which is what
00:26:26.880 --> 00:26:32.870
general relativity did um meant that uh
00:26:32.880 --> 00:26:35.750
yes, the physicists could go away happy
00:26:35.760 --> 00:26:38.630
because they solved a problem. There
00:26:38.640 --> 00:26:41.269
were a number of problems that Newtonian
00:26:41.279 --> 00:26:43.430
gravity couldn't couldn't help with
00:26:43.440 --> 00:26:46.470
which were solved by Einsteinian
00:26:46.480 --> 00:26:47.830
gravity.
00:26:47.840 --> 00:26:51.909
So um but that didn't seem to offer any
00:26:51.919 --> 00:26:55.029
future benefits for humankind. But here
00:26:55.039 --> 00:26:57.830
we are rather more than 100 years later,
00:26:57.840 --> 00:27:03.590
110 years later and we have um tools
00:27:03.600 --> 00:27:06.950
which rely absolutely on general
00:27:06.960 --> 00:27:08.549
relativity. And the one I'm thinking of
00:27:08.559 --> 00:27:12.310
most commonly is uh GPS
00:27:12.320 --> 00:27:15.750
uh because our position finding um
00:27:15.760 --> 00:27:18.549
software simply would not work without
00:27:18.559 --> 00:27:20.950
general relativity. you'd have errors in
00:27:20.960 --> 00:27:23.750
the region of 10 kilometers which is not
00:27:23.760 --> 00:27:26.789
kind of what you want with GPS but that
00:27:26.799 --> 00:27:31.350
took a 100 years and so Renie that's the
00:27:31.360 --> 00:27:33.190
sort of time scale I think on which you
00:27:33.200 --> 00:27:34.950
have to be optimistic about the way it
00:27:34.960 --> 00:27:37.590
might help humankind or life on earth
00:27:37.600 --> 00:27:40.390
generally because if we become
00:27:40.400 --> 00:27:43.590
responsible um a responsible species on
00:27:43.600 --> 00:27:44.870
our planet we're going to help the whole
00:27:44.880 --> 00:27:48.230
planet if we if we live sustainably and
00:27:48.240 --> 00:27:50.870
um live alongside inside uh all our
00:27:50.880 --> 00:27:54.149
companion organisms on on this planet.
00:27:54.159 --> 00:27:56.870
So uh yeah, so I I think um what you
00:27:56.880 --> 00:27:59.190
can't say is that it won't help them.
00:27:59.200 --> 00:28:01.590
That's the thing. You can't say that it
00:28:01.600 --> 00:28:04.549
will either. Uh but there's a good
00:28:04.559 --> 00:28:07.510
chance that in the same way that um
00:28:07.520 --> 00:28:09.750
something as obstruuse as general
00:28:09.760 --> 00:28:11.750
relativity actually comes into
00:28:11.760 --> 00:28:14.630
everybody's everyday lifeund odd years
00:28:14.640 --> 00:28:17.510
later. I think that's the the model and
00:28:17.520 --> 00:28:21.110
it's one reason why why deep research
00:28:21.120 --> 00:28:22.630
like this is funded. It's why
00:28:22.640 --> 00:28:24.789
fundamental research that is just
00:28:24.799 --> 00:28:27.190
knowledge for its own sake at the moment
00:28:27.200 --> 00:28:28.710
why it's funded because you never know
00:28:28.720 --> 00:28:30.710
what the spin-offs might be.
00:28:30.720 --> 00:28:33.029
>> Absolutely. Uh and you can look back in
00:28:33.039 --> 00:28:34.710
history at some of the great discoveries
00:28:34.720 --> 00:28:37.830
and how they've they've changed things
00:28:37.840 --> 00:28:42.149
on Earth and have changed human life. Um
00:28:42.159 --> 00:28:44.710
>> I'm just trying to think of one. Well,
00:28:44.720 --> 00:28:45.909
electricity for a start.
00:28:45.919 --> 00:28:48.149
>> Yeah. Well, they, you know, it was just
00:28:48.159 --> 00:28:50.470
physicists playing around in the early
00:28:50.480 --> 00:28:52.230
19th century. Oh, this is really
00:28:52.240 --> 00:28:53.269
interesting.
00:28:53.279 --> 00:28:55.909
>> Um, nobody ever thought we'd use it like
00:28:55.919 --> 00:28:57.510
we do today.
00:28:57.520 --> 00:28:59.350
>> And I suppose one of the this is
00:28:59.360 --> 00:29:03.029
probably a a fundamental example. Uh, as
00:29:03.039 --> 00:29:07.350
we learn things, we learn things. So it
00:29:07.360 --> 00:29:09.350
expands our minds. It expands our
00:29:09.360 --> 00:29:11.190
inquisitiveness. It expands our
00:29:11.200 --> 00:29:13.830
intelligence. It it it it enables
00:29:13.840 --> 00:29:17.669
humanity to understand more about itself
00:29:17.679 --> 00:29:19.350
and its place in the universe. You know,
00:29:19.360 --> 00:29:22.389
you go back to 1543
00:29:22.399 --> 00:29:23.990
when Capernicus
00:29:24.000 --> 00:29:26.149
>> found that the earth was not the center
00:29:26.159 --> 00:29:29.029
of the universe. I think he got shouted
00:29:29.039 --> 00:29:31.430
down pretty heavily for that. But that's
00:29:31.440 --> 00:29:33.750
the truth. We know that now. Uh there
00:29:33.760 --> 00:29:36.789
was I can't remember who it was but um
00:29:36.799 --> 00:29:38.549
another thing that goes back quite a way
00:29:38.559 --> 00:29:41.830
when the discovery was made that our son
00:29:41.840 --> 00:29:43.909
is actually a star. I mean for a long
00:29:43.919 --> 00:29:46.310
time we didn't know that.
00:29:46.320 --> 00:29:48.230
>> You know it's it's about knowledge as
00:29:48.240 --> 00:29:50.149
much as anything. I think
00:29:50.159 --> 00:29:51.510
>> Yeah. Yep.
00:29:51.520 --> 00:29:52.549
>> I love that one though.
00:29:52.559 --> 00:29:54.230
>> That's right. Yeah.
00:29:54.240 --> 00:29:54.630
>> The sun.
00:29:54.640 --> 00:29:55.430
>> It's great.
00:29:55.440 --> 00:29:56.149
>> Yeah.
00:29:56.159 --> 00:29:56.710
>> I think
00:29:56.720 --> 00:29:57.830
>> you can look it up. It's online
00:29:57.840 --> 00:29:59.350
somewhere. I did it as a quiz question
00:29:59.360 --> 00:30:01.990
once on the radio and um got a great
00:30:02.000 --> 00:30:04.310
response to that cuz people just in the
00:30:04.320 --> 00:30:06.470
modern era never thought that there
00:30:06.480 --> 00:30:08.149
would have been a time where people look
00:30:08.159 --> 00:30:12.149
at this this hot ball in the sky and go
00:30:12.159 --> 00:30:15.190
what is that? Um and you know looking at
00:30:15.200 --> 00:30:16.789
all the other stars not making the
00:30:16.799 --> 00:30:19.269
correlation they just didn't know. It's
00:30:19.279 --> 00:30:22.149
um it was incredible. So I suppose Renie
00:30:22.159 --> 00:30:24.389
it's it's it's about knowledge. It's
00:30:24.399 --> 00:30:26.630
about expanding our understanding of
00:30:26.640 --> 00:30:28.789
life, the universe, and everything and
00:30:28.799 --> 00:30:31.110
not stopping at 42.
00:30:31.120 --> 00:30:34.710
Um, that's the way I look at it.
00:30:34.720 --> 00:30:36.470
I think you're and I think you're
00:30:36.480 --> 00:30:38.549
absolutely right. I think um, you know,
00:30:38.559 --> 00:30:40.389
both that's two sides of the same thing.
00:30:40.399 --> 00:30:43.350
We're we're we but it's why we why we do
00:30:43.360 --> 00:30:45.029
this sort of thing. It's why it's we're
00:30:45.039 --> 00:30:46.630
a curious species and
00:30:46.640 --> 00:30:47.190
>> absolutely
00:30:47.200 --> 00:30:48.630
>> knowledge is power. Yeah.
00:30:48.640 --> 00:30:50.789
>> Yeah. Yeah. That's another thing. Yeah.
00:30:50.799 --> 00:30:53.110
Absolutely true, Renie. Great question.
00:30:53.120 --> 00:30:55.590
good one for discussion and debate and
00:30:55.600 --> 00:30:57.029
keep them coming. If you'd like to send
00:30:57.039 --> 00:30:59.990
questions into us, um you can do so
00:31:00.000 --> 00:31:01.590
through our website,
00:31:01.600 --> 00:31:03.430
spacenutspodcast.com,
00:31:03.440 --> 00:31:06.870
spacenuts.io, they're the two URLs. And
00:31:06.880 --> 00:31:08.389
while you're there, have a look around.
00:31:08.399 --> 00:31:10.870
The AMA button at the top, ask me
00:31:10.880 --> 00:31:12.710
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00:31:12.720 --> 00:31:15.029
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00:31:51.200 --> 00:31:53.669
Always a pleasure.
00:31:53.679 --> 00:31:55.430
>> Good to talk, Andrew. And um I'm sure
00:31:55.440 --> 00:31:57.430
we'll do it again soon.
00:31:57.440 --> 00:31:59.909
>> Yes, I'm sure we will. Uh could be a few
00:31:59.919 --> 00:32:01.909
minutes, could be a week, who knows. Uh
00:32:01.919 --> 00:32:03.590
and Hugh in the studio, thanks to him
00:32:03.600 --> 00:32:05.269
for doing everything he does. We don't
00:32:05.279 --> 00:32:07.350
know what that is, but we appreciate it.
00:32:07.360 --> 00:32:09.110
And from me, Andrew Dunley, thanks for
00:32:09.120 --> 00:32:10.710
your company. See you on the next
00:32:10.720 --> 00:32:13.029
episode of Space Nuts. Bye-bye.
00:32:13.039 --> 00:32:15.430
>> Space Nuts. You'll be listening to the
00:32:15.440 --> 00:32:18.389
Space Nuts podcast
00:32:18.399 --> 00:32:21.430
>> available at Apple Podcasts, Spotify,
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