July 27, 2026
The Cosmic Q&A: Redshift, Dark Matter & the Shape of the Universe | Space Nuts: Astronomy...
WEBVTT
Kind: captions
Language: en
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Hello again. Thanks for joining us on
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Space Nuts. This is a Q&A edition. My
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name is Andrew Dunley. What's a Q&A
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edition? It's an edition where we get
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Q's and give you A's because you're so
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clever. Uh, something like that. Anyway,
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we're going to answer audience
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questions. That's what I'm getting at.
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We've got questions about Red Shift. We
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got questions about dark photons. What?
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Uh, we've got questions about deep space
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astronomy. And another one about the
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expansion of the universe. So, I think
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we talked about that last episode.
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Anyway, uh we'll see if we can solve all
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of that on this episode 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 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 with us again to kind of try to
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maybe answer some of that is Professor
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Fred Watson, astronomer at large. Hello,
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Fred.
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>> Hello, Andrew. Um, kind of is probably
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the best description really, isn't it?
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[laughter]
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>> Possibly. So, possibly so. Um, but you
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know, it's good to get questions. We've
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got a whole new batch. So, um, let's get
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stuck straight into it. Our first
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question comes from, um, uh, I I love
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the way he always ends his questions.
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I'm not going to reveal anything, but um
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let's hear from Roger.
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>> Hey there, space nuts. This is Roger the
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truck driver. Tonight I'm in uh Rutland,
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Vermont.
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Got a question about the red shift of
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galaxies.
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Um if the light that we're seeing from a
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far off galaxy is shifted to the red and
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it started out at a higher frequency,
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doesn't that mean energy's lost
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somewhere between here and there? And is
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that energy just transferred into space?
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And if it is, does that contribute to
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the expansion of space? And I'm not
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saying it's dark energy, but it is does
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it contribute to it or does that energy
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get dissipated in another way? All
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right. Always digging the show. You guys
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keep on trucking.
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[laughter] I love that. I love that. Uh
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we got train drivers that do that.
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Unfortunately, they do it at 3:00 in the
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morning. [gasps]
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Although today he did it at 10 to 7, I
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was pretty annoyed. Pretty annoyed.
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>> This is uh the one going past your
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place.
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>> Yeah, behind our place there's a rail
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line. It doesn't get used a heck of a
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lot, but when it does, um yes, the the
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glasses rattle. Uh the ones on my face,
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I mean. Uh thanks, Roger. Great
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question. Uh so um yeah the change in
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frequency with the um energy loss um
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where does the energy go and does it
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contribute to the expansion of the
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universe and could it possibly be maybe
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maybe not dark matter or dark energy
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>> or something.
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>> Yeah.
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>> Yeah. Um there's a lot he packed a lot
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into that question.
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>> He did and it's a great question too. Uh
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and you know I mean it's a um project is
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absolutely right the conservation of
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energy uh energy can't be created or
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destroyed. That's the the fundamental
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rule. Uh it's energy is always conserved
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[snorts] but
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uh the universe doesn't play by the
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ordinary rules.
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Uh and um it it's a it's an interesting
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answer here. Um and and I have to say
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it's changed my view of what this you
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know what the answer to this problem
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was.
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>> Okay.
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>> Uh because um when we've been asked this
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before been asked it for a long time I
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just assumed that the energy uh
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basically was absorbed by the universe
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by spacetime
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uh and maybe contributed to the
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expansion. Although there's it's a it's
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a you can't have it both ways because
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it's the expansion that's causing the
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the photon's energy to be to be lost. Uh
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and and just stepping back exactly as
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Roger said, uh you've got light going
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through the universe. It's uh the its
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wavelength is being stretched by the
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expansion of the universe. Therefore,
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the light is losing energy because the
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energy of a beam of light is all about
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the frequency of the light. In other
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words, or the wavelength, putting it
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another way.
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>> So, if you increase the wavelength, you
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lose energy and that's that's um a given
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already. Uh so, what I used to say was
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yes, it kind of goes into the universe,
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but um I've done a bit more reading on
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this and I was wrong. Oh.
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[sighs and gasps]
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Um because
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when you apply general relativity to the
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universe as a whole and that's the as
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we've talked about and we talked about
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it at length in the last episode it's uh
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the the kind of fundamental rule that
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governs everything that we understand in
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the universe. Um when you apply general
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relativity
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uh that conservation of energy that we
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expect to happen in the everyday world
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uh it doesn't hold good. So uh energy is
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not conserved in an expanding universe.
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>> Oh
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>> uh and so basically the energy simply
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disappears.
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It's just not there anymore because of
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the expansion of the universe. It's not
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causing the expansion of the universe.
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It's not create contributing to dark
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energy or dark matter, the energy loss.
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It just vanishes.
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>> Wow.
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>> So, work that one out.
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>> I can't. [snorts]
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>> No, I can't either. [laughter]
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>> Uh it's um it's I I kind of really need
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to look at the equations on this.
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>> Um you don't show them to me. I mean,
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I'm yeah I'm not that keen on looking at
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them myself either got too much else to
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do but uh but um uh but that's yes that
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is the thinking on this uh and I think
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the conservation rule does not work uh
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when it comes to
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um when it comes to consu to to to the
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universe on a whole.
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>> Yeah. Wow. Gee, that's um that's quite a
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revelation. And who who figured that
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out?
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>> Uh [sighs]
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uh it's on a number of uh different
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physics uh related.
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>> There's there there's the reason no one
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knows about it cuz it's physics and
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[laughter]
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who reads that stuff?
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>> Yeah. I think I think the relativistic
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bit of it
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>> uh comes from the fact that the energy
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of a particle which is what we're
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talking about it's an observer dependent
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quantity and so that's why relativity
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plays a part in this because you're the
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observer and and you're talking about
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something that's relative to another
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observer i.e. the photon.
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>> Yeah. Uh, and that's why you've got, you
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know, a relivist a relativistic uh,
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access to it.
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>> Wow. Okay. Um, great question, Roger.
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I'm not sure you were expecting that
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answer, but uh, there it is. Uh, the
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energy just
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gone,
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goes, vanishes, ceases to exist. It's a
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dead poly.
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So
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anyway, um, no one got that joke. I was,
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um, I was doing a Montipython skit for
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some reason.
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>> Yeah. Yeah, you were. That's right. I'm
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I'm Look, I'm pursuing this in a little
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bit more detail and, uh, and just trying
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to, you know, see whether we've got
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alternative alternative views of this.
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>> Generally speaking, you do get
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alternative views when it comes to this
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kind.
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>> That's right.
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>> Um, yes. So, so the the that's right. Uh
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I think I think the the standard
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explanation today is that energy is not
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is not conserved. Okay, we'll leave it
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at that until somebody throws another
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spanner into the
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>> Yeah, we might be giving a different
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answer next week.
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>> It could be. [laughter] Thanks, Roger.
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Great to hear from you. Toot toot. Uh
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we'll catch you next time. Our next
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question comes from Peter. He's from San
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Diego, California. While listening to
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another astrophysics podcast, I heard
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the term dark photon for the first time.
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Apparently, this is a particle
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astrophysicists are seeking in order to
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explain dark matter and/or dark energy.
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Could you please elaborate on what a
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dark photon could be? Um, dad joke for
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Andrew. A photon travels at the speed of
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light. Does that mean a dark photon
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travels at the speed of dark?
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>> [laughter]
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>> I like that. That's good.
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>> That's really good. Keep up the great
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work, he says. Uh, thank you, Peter.
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Hope all is well in San Diego,
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California.
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>> Uh, have you ever heard of a dark
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photon, Fred? Um, yes. I've probably got
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a few in this box here. [laughter]
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Um, your the speed of dark just just
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going back to that that quip. Uh there
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was a story I read uh probably a
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fortnight ago uh about exactly this in
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that darkness
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can move faster than the speed of light.
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>> No, [clears throat]
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it it's but it's a an illusory darkness.
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is when you've got um light beams
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interfering with one another so that
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you've that and interference
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light beams can cancel out. So if you've
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got two light waves and you add them up
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out of phase, they can cancel out and
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you get darkness.
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>> That's well-known principle of
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intererometry. I used to play with that
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when I was a student a lot. Uh but there
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are certain circumstances that those
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patterns of darkness can actually exceed
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the speed of light because they're not
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actually real. They're not real
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entities. They're not a thing that's
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carrying any sort of information or
00:10:26.480 --> 00:10:29.452
energy. They're just patterns in a in an
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[clears throat] interference pattern.
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They're just dark patches in it. And I
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think under certain circumstances, they
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could go faster than the speed of light.
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So, darkness might be not quite as uh
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you know as twe as you thought it was,
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>> I guess.
00:10:43.839 --> 00:10:47.590
>> Anyway, anyway, uh that's not the the
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question. Uh because dark photons are
00:10:50.079 --> 00:10:51.990
definitely something different and
00:10:52.000 --> 00:10:54.230
they're basically
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uh hypothetical. They've been
00:10:56.959 --> 00:10:59.269
hypothesized by physicists and
00:10:59.279 --> 00:11:00.790
cosmologists
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as being a force carrier similar to the
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ordinary photon but related to
00:11:09.760 --> 00:11:12.389
dark matter.
00:11:12.399 --> 00:11:15.430
In in other words, you might have Sorry,
00:11:15.440 --> 00:11:17.110
somebody's trying to phone me. I'm just
00:11:17.120 --> 00:11:18.790
going to kill that call.
00:11:18.800 --> 00:11:19.350
>> Yeah.
00:11:19.360 --> 00:11:21.190
>> Uh um
00:11:21.200 --> 00:11:24.472
>> that was me. That was me. No, it wasn't.
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[laughter]
00:11:25.792 --> 00:11:26.310
>> [sighs and gasps]
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>> They're they're you know they're part of
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the there may be when we discover
00:11:30.959 --> 00:11:34.150
finally what dark matter is there may be
00:11:34.160 --> 00:11:38.389
a suite of dark particles
00:11:38.399 --> 00:11:40.470
which could include dark photons. That's
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the line
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>> right?
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>> And and so you know we mentioned last
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week the or the last episode the uh the
00:11:48.320 --> 00:11:50.630
large hydrron collider being upgraded to
00:11:50.640 --> 00:11:52.470
be the high luminosity large hydrron
00:11:52.480 --> 00:11:55.670
collider. Um, that's one of the things
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they'd be looking for will be dark
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photons.
00:11:58.880 --> 00:12:04.230
Okay. Uh, yeah, I tried to do a um an AI
00:12:04.240 --> 00:12:07.509
search for an explanation on it and um
00:12:07.519 --> 00:12:09.670
it it it sort of gave me all this gobbly
00:12:09.680 --> 00:12:13.030
but um you know what would a dark
00:12:13.040 --> 00:12:16.150
proton photon do? It says it would carry
00:12:16.160 --> 00:12:19.269
a force within the dark sector.
00:12:19.279 --> 00:12:21.430
We call that the government. uh it might
00:12:21.440 --> 00:12:23.430
allow dark matter particles to interact
00:12:23.440 --> 00:12:25.430
with each other and it could very weakly
00:12:25.440 --> 00:12:27.910
mix with normal photons giving us a way
00:12:27.920 --> 00:12:30.710
to detect it. And the reason they reckon
00:12:30.720 --> 00:12:33.110
that scientists care about this is as
00:12:33.120 --> 00:12:35.350
you said could explain what dark matter
00:12:35.360 --> 00:12:38.230
is made of. So therefore solving some of
00:12:38.240 --> 00:12:40.310
those gaps in our current physics
00:12:40.320 --> 00:12:42.389
theories.
00:12:42.399 --> 00:12:44.550
So that's that's that's why people are
00:12:44.560 --> 00:12:45.750
interested in this and that's why
00:12:45.760 --> 00:12:47.350
they're upgrading the Large Hadron
00:12:47.360 --> 00:12:49.110
Collider and
00:12:49.120 --> 00:12:52.470
>> hopefully we will learn more in years to
00:12:52.480 --> 00:12:55.829
come. That's that's the that's the hope.
00:12:55.839 --> 00:12:57.590
That's the hope. Yeah. So we might you
00:12:57.600 --> 00:12:59.269
know we might be talking one day about
00:12:59.279 --> 00:13:01.829
dark photons um having been detected
00:13:01.839 --> 00:13:03.430
which would be
00:13:03.440 --> 00:13:05.910
>> a coup for space nukes.
00:13:05.920 --> 00:13:08.389
>> Yes, it will. Uh but at this stage uh
00:13:08.399 --> 00:13:10.949
they are not proven. It's just a theory.
00:13:10.959 --> 00:13:13.030
So that's That's about as much as we
00:13:13.040 --> 00:13:15.030
know at this point in time.
00:13:15.040 --> 00:13:17.750
>> But uh very good question uh and thank
00:13:17.760 --> 00:13:19.990
you Peter for sending it in. This is
00:13:20.000 --> 00:13:22.069
Space Nuts with Andrew Dunley and
00:13:22.079 --> 00:13:25.590
Professor Fred Watson.
00:13:25.600 --> 00:13:27.350
Let's take a short break from the show
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>> And I feel
00:15:15.279 --> 00:15:17.430
>> Space Nuts. Okay, Fred, we'll move
00:15:17.440 --> 00:15:19.430
straight on to our next question, which
00:15:19.440 --> 00:15:23.430
is uh another audio question from Eli.
00:15:23.440 --> 00:15:27.829
Hello, this is Eli from sunny Coachella
00:15:27.839 --> 00:15:30.870
Valley in California.
00:15:30.880 --> 00:15:33.430
I'm embarrassed to admit it, but I still
00:15:33.440 --> 00:15:35.189
can't get my head around deep space
00:15:35.199 --> 00:15:38.230
astronomy. I get that the light from say
00:15:38.240 --> 00:15:41.910
a distant galaxy is a billion years old.
00:15:41.920 --> 00:15:44.550
But why that particular point in its
00:15:44.560 --> 00:15:47.189
time? Is it just a matter of whatever
00:15:47.199 --> 00:15:49.749
light is hitting us is the time we get
00:15:49.759 --> 00:15:51.749
to see?
00:15:51.759 --> 00:15:55.910
But for really early light, the JWST
00:15:55.920 --> 00:15:57.910
early universe stuff that's been
00:15:57.920 --> 00:16:01.269
traveling for 13 billion years and just
00:16:01.279 --> 00:16:04.310
hitting us now. Are we looking for the
00:16:04.320 --> 00:16:07.509
light that hasn't passed us by or hasn't
00:16:07.519 --> 00:16:10.710
made it here yet, but is from that one
00:16:10.720 --> 00:16:14.150
precise location long ago?
00:16:14.160 --> 00:16:16.550
This stuff is so difficult to get my
00:16:16.560 --> 00:16:19.829
head around. Love the show and hope you
00:16:19.839 --> 00:16:22.629
guys can clear this up for me.
00:16:22.639 --> 00:16:25.189
>> Uh, no we can't. We just thought we'd um
00:16:25.199 --> 00:16:27.990
put the question in there. Uh, thanks
00:16:28.000 --> 00:16:31.430
Eli. Uh it this is a deep um not only in
00:16:31.440 --> 00:16:33.509
deep space astronomy terms but it is a
00:16:33.519 --> 00:16:37.269
deep deep topic. Uh I mean when we look
00:16:37.279 --> 00:16:39.590
up into the sky at night and we see all
00:16:39.600 --> 00:16:42.389
those beautiful colored dots we are
00:16:42.399 --> 00:16:44.629
looking at history and it's variable
00:16:44.639 --> 00:16:47.829
history because some of it's 4.41 light
00:16:47.839 --> 00:16:51.269
years away and some of it's 400,000
00:16:51.279 --> 00:16:53.590
light years away. Some of it's further
00:16:53.600 --> 00:16:55.590
than that. It's um but then you've got
00:16:55.600 --> 00:16:58.069
the cosmic microwave background
00:16:58.079 --> 00:17:00.870
radiation which is kind of a leftover of
00:17:00.880 --> 00:17:03.430
of um [gasps]
00:17:03.440 --> 00:17:05.990
what happened after the big bang and
00:17:06.000 --> 00:17:08.470
that that's that's a different kettle to
00:17:08.480 --> 00:17:10.630
fish and I can understand why you got a
00:17:10.640 --> 00:17:13.591
headache Eli. Over to you Fred.
00:17:13.601 --> 00:17:14.470
[laughter]
00:17:14.480 --> 00:17:20.789
Thanks. Um so I guess you know that I I
00:17:20.799 --> 00:17:25.110
understand Eli's issue as well. um
00:17:25.120 --> 00:17:27.110
you you've got to be in the right place
00:17:27.120 --> 00:17:29.190
at the right time to see a photon from a
00:17:29.200 --> 00:17:32.789
distant galaxy. But I I guess the way to
00:17:32.799 --> 00:17:36.230
envisage this is if you think of the
00:17:36.240 --> 00:17:40.070
universe um and you've got to perhaps
00:17:40.080 --> 00:17:41.750
think of it as if you were looking at it
00:17:41.760 --> 00:17:43.590
from the outside, which we never can.
00:17:43.600 --> 00:17:46.150
But uh if you can think of it that way,
00:17:46.160 --> 00:17:48.950
then it's full of objects which are
00:17:48.960 --> 00:17:52.549
radiating light even in its infancy.
00:17:52.559 --> 00:17:54.150
when the universe was very young, the
00:17:54.160 --> 00:17:57.270
stuff in it was basically shining. Um
00:17:57.280 --> 00:17:59.350
once we got past the dark ages where no
00:17:59.360 --> 00:18:03.190
stars were shining, uh but um and those
00:18:03.200 --> 00:18:05.430
are the galaxies that we now see. So so
00:18:05.440 --> 00:18:08.310
they're constantly radiating light and
00:18:08.320 --> 00:18:10.310
that's like just like a river of light
00:18:10.320 --> 00:18:12.230
that's flowing
00:18:12.240 --> 00:18:15.350
down time, if I can put it that way. Uh
00:18:15.360 --> 00:18:19.669
and a long time in in the future, it
00:18:19.679 --> 00:18:22.630
reaches us. But it's not just, you know,
00:18:22.640 --> 00:18:25.110
an individual photon or something that's
00:18:25.120 --> 00:18:27.430
reaching us. It's this stream of stuff
00:18:27.440 --> 00:18:30.470
that is being radiated throughout the
00:18:30.480 --> 00:18:34.070
universe by these galaxies. So we um and
00:18:34.080 --> 00:18:37.270
and we we pick it up. We pick it up
00:18:37.280 --> 00:18:39.029
sometimes as exactly as you've said,
00:18:39.039 --> 00:18:40.870
well up to 10 billion years after it's
00:18:40.880 --> 00:18:43.350
been radiated. I think
00:18:43.360 --> 00:18:45.830
>> 12 billion years are the are the oldest
00:18:45.840 --> 00:18:47.830
or the earliest galaxies that we now
00:18:47.840 --> 00:18:49.510
see. We're looking back in time. 12
00:18:49.520 --> 00:18:51.750
billion years and seeing them as they
00:18:51.760 --> 00:18:54.470
were perhaps a billion and a half years
00:18:54.480 --> 00:18:57.190
after the big bang. Um, and they're they
00:18:57.200 --> 00:18:59.350
are shining. They're radiating light uh
00:18:59.360 --> 00:19:01.830
in the early universe and down the track
00:19:01.840 --> 00:19:03.830
that reaches us because that light's
00:19:03.840 --> 00:19:05.590
going in all directions. So, it wouldn't
00:19:05.600 --> 00:19:08.310
matter where in the universe we were, we
00:19:08.320 --> 00:19:10.870
would still see them. Uh, we'd just see
00:19:10.880 --> 00:19:12.549
them in a, you know, in a different
00:19:12.559 --> 00:19:14.630
position in the sky if we're a long way
00:19:14.640 --> 00:19:15.990
from where we are now.
00:19:16.000 --> 00:19:19.990
>> Yeah. Um but yeah so I I guess it's you
00:19:20.000 --> 00:19:22.549
know in a way one way of thinking about
00:19:22.559 --> 00:19:25.430
this is if you imagine us on planet
00:19:25.440 --> 00:19:28.390
earth here and imagine us being
00:19:28.400 --> 00:19:32.630
surrounded by a whole series of shells
00:19:32.640 --> 00:19:34.630
uh which we're at the center of and this
00:19:34.640 --> 00:19:36.310
is a bit like the crystalline spheres
00:19:36.320 --> 00:19:38.470
that people used to think uh the
00:19:38.480 --> 00:19:41.590
universe was made of. Uh but these these
00:19:41.600 --> 00:19:44.549
shells uh spherical shells all centered
00:19:44.559 --> 00:19:47.590
on the earth but each one clicks over to
00:19:47.600 --> 00:19:51.669
a to a a time further in the past. Uh
00:19:51.679 --> 00:19:53.510
because the lights coming to us from the
00:19:53.520 --> 00:19:55.990
whole the whole cosmos which is full of
00:19:56.000 --> 00:19:58.390
stuff. Uh and that's why we can see
00:19:58.400 --> 00:20:00.230
these these shells sort of being
00:20:00.240 --> 00:20:02.710
illuminated in a way by the objects that
00:20:02.720 --> 00:20:05.830
uh that radiated them at that time. uh
00:20:05.840 --> 00:20:09.270
that has um that we see them because of
00:20:09.280 --> 00:20:11.590
the the distance that they are away from
00:20:11.600 --> 00:20:13.909
us means that they've the light has
00:20:13.919 --> 00:20:15.990
taken that long to get to us. Whether
00:20:16.000 --> 00:20:17.990
that helps or not in fact I think I've
00:20:18.000 --> 00:20:20.924
just confused it completely but
00:20:20.934 --> 00:20:21.830
[snorts]
00:20:21.840 --> 00:20:25.029
um I
00:20:25.039 --> 00:20:27.750
just doing a little experimental search
00:20:27.760 --> 00:20:30.789
here for a sec.
00:20:30.799 --> 00:20:34.390
What what I I I agree with in terms of
00:20:34.400 --> 00:20:36.630
Eli's question and and getting your head
00:20:36.640 --> 00:20:40.230
around it is um if Beetlejuice or
00:20:40.240 --> 00:20:42.149
however you want to pronounce it went
00:20:42.159 --> 00:20:47.029
supernova right now as we were speaking
00:20:47.039 --> 00:20:50.230
>> we wouldn't see it for
00:20:50.240 --> 00:20:52.470
640 years.
00:20:52.480 --> 00:20:53.669
>> Yeah.
00:20:53.679 --> 00:20:57.350
So for it to have gone supernova in the
00:20:57.360 --> 00:21:00.230
past and us to witness it, it has to
00:21:00.240 --> 00:21:02.470
have happened
00:21:02.480 --> 00:21:06.230
pretty close to 640 years ago. Does that
00:21:06.240 --> 00:21:07.110
make sense?
00:21:07.120 --> 00:21:09.830
>> Yes. Um so you could think of that in
00:21:09.840 --> 00:21:13.909
another way. Um you know um anywhere
00:21:13.919 --> 00:21:16.630
between us and 640 light years away
00:21:16.640 --> 00:21:18.710
there could be this pulse of light
00:21:18.720 --> 00:21:20.789
that's on its way to us
00:21:20.799 --> 00:21:23.909
>> from Beetlejuice. uh it would spread out
00:21:23.919 --> 00:21:26.470
in a sphere uh and as that sphere
00:21:26.480 --> 00:21:28.549
expanded eventually it would wash over
00:21:28.559 --> 00:21:31.590
the earth and we'd see it um and perhaps
00:21:31.600 --> 00:21:33.350
see it during the day as well because it
00:21:33.360 --> 00:21:35.270
might get bright enough to do that.
00:21:35.280 --> 00:21:37.350
>> Uh and and I think that's a really good
00:21:37.360 --> 00:21:39.669
way of putting it, Andrew, because um
00:21:39.679 --> 00:21:41.029
thinking about the galaxies, they're
00:21:41.039 --> 00:21:43.029
just streaming light out all the time.
00:21:43.039 --> 00:21:45.750
But something like uh a supernova
00:21:45.760 --> 00:21:47.909
explosion which gives a big pulse of
00:21:47.919 --> 00:21:50.710
light um that's perhaps easier to get
00:21:50.720 --> 00:21:52.549
your head around because that's that's
00:21:52.559 --> 00:21:57.029
just got a um it'll take whatever
00:21:57.039 --> 00:21:59.029
whatever time is represented by the
00:21:59.039 --> 00:22:02.310
distance away. So 640 light years away.
00:22:02.320 --> 00:22:04.549
It'll take 640 years to get here for
00:22:04.559 --> 00:22:06.470
that pulse to get here. But then it will
00:22:06.480 --> 00:22:09.190
sweep over us uh and we'll see the light
00:22:09.200 --> 00:22:11.110
the the light fading away.
00:22:11.120 --> 00:22:15.190
>> Yeah. And um the reason I chose that
00:22:15.200 --> 00:22:18.149
target is because there's a lot of
00:22:18.159 --> 00:22:20.710
conjecture about its future and the
00:22:20.720 --> 00:22:22.390
possibility that it's reaching that
00:22:22.400 --> 00:22:23.909
critical mass point.
00:22:23.919 --> 00:22:24.710
>> Yes.
00:22:24.720 --> 00:22:26.390
>> Um but it could have already happened.
00:22:26.400 --> 00:22:28.789
That's the other thing. [laughter]
00:22:28.799 --> 00:22:30.870
>> But we that's that's something we can
00:22:30.880 --> 00:22:33.029
have no knowledge of. That's the the key
00:22:33.039 --> 00:22:35.669
thing because um we are limited by the
00:22:35.679 --> 00:22:37.669
speed of light. That's the thing that
00:22:37.679 --> 00:22:39.350
always limits our view of the universe.
00:22:39.360 --> 00:22:41.830
And just to confuse Eli a little bit
00:22:41.840 --> 00:22:45.590
more, there are probably things in the
00:22:45.600 --> 00:22:47.430
universe we will never witness because
00:22:47.440 --> 00:22:49.590
the light is just too far away to reach
00:22:49.600 --> 00:22:51.909
us in any reasonable amount of time.
00:22:51.919 --> 00:22:53.350
Even even
00:22:53.360 --> 00:22:56.149
>> beyond the life of the earth itself or
00:22:56.159 --> 00:22:57.430
or our sun,
00:22:57.440 --> 00:23:01.110
>> we we we there are things we will never
00:23:01.120 --> 00:23:03.350
ever know about.
00:23:03.360 --> 00:23:04.390
>> Correct.
00:23:04.400 --> 00:23:06.870
>> It's um and that's where it just gives
00:23:06.880 --> 00:23:08.605
you um
00:23:08.615 --> 00:23:09.110
>> [snorts and laughter]
00:23:09.120 --> 00:23:11.110
>> one of those headaches that uh requires
00:23:11.120 --> 00:23:13.909
you to take paracetamol and ibuprofen at
00:23:13.919 --> 00:23:17.776
the same time. So,
00:23:17.786 --> 00:23:18.870
[laughter]
00:23:18.880 --> 00:23:21.350
>> um deep deep headaches. But Eli, great
00:23:21.360 --> 00:23:23.110
question. I'm not sure we solved your
00:23:23.120 --> 00:23:27.830
problem, but um anyway, uh it it I I try
00:23:27.840 --> 00:23:29.190
to explain this sort of stuff to my
00:23:29.200 --> 00:23:33.510
grandson uh and my granddaughters and
00:23:33.520 --> 00:23:36.230
you know, how do you explain time and
00:23:36.240 --> 00:23:40.549
distance to a to a a young child and um
00:23:40.559 --> 00:23:41.430
when you're trying to get through
00:23:41.440 --> 00:23:43.750
traffic, it's [laughter]
00:23:43.760 --> 00:23:45.190
>> that might not be the best time to do
00:23:45.200 --> 00:23:45.510
it.
00:23:45.520 --> 00:23:46.789
>> Probably not, but they're very
00:23:46.799 --> 00:23:47.990
interested.
00:23:48.000 --> 00:23:50.149
>> Very interested. Thanks, Eli. Great
00:23:50.159 --> 00:23:53.029
question.
00:23:53.039 --> 00:23:55.430
The crew of Artemis 2 now bound for the
00:23:55.440 --> 00:23:57.909
moon. Humanity's next great voyage
00:23:57.919 --> 00:23:59.270
begins.
00:23:59.280 --> 00:24:03.270
>> Space nuts. Our final question uh comes
00:24:03.280 --> 00:24:07.029
from Nova Scotia. It's from Ken. Uh
00:24:07.039 --> 00:24:08.470
look, this is an old chestnut. We've
00:24:08.480 --> 00:24:10.950
we've probably spoken about this many
00:24:10.960 --> 00:24:13.510
times, but it's always good to um to to
00:24:13.520 --> 00:24:15.990
revisit. If the universe is expanding,
00:24:16.000 --> 00:24:20.070
what is it expanding into? And also is
00:24:20.080 --> 00:24:23.269
the universe spherical?
00:24:23.279 --> 00:24:25.669
So um yes, what's it expanding into?
00:24:25.679 --> 00:24:29.350
Well, we don't know. And yes,
00:24:29.360 --> 00:24:32.230
>> that's yes. Uh it's actually we don't
00:24:32.240 --> 00:24:33.110
know and maybe
00:24:33.120 --> 00:24:35.110
>> and maybe maybe.
00:24:35.120 --> 00:24:39.669
>> So um the the universe is everything
00:24:39.679 --> 00:24:41.909
that we can detect. That's the
00:24:41.919 --> 00:24:43.269
definition of the universe. Everything
00:24:43.279 --> 00:24:46.870
we can measure or detect. And that means
00:24:46.880 --> 00:24:49.909
and we observe the expansion
00:24:49.919 --> 00:24:52.470
but we don't know whether there's an
00:24:52.480 --> 00:24:54.070
edge to the universe. We don't know
00:24:54.080 --> 00:24:55.990
whether it's infinite. We don't know
00:24:56.000 --> 00:24:58.390
anything beyond the horizons that we
00:24:58.400 --> 00:25:00.549
see. And the most obvious one is the
00:25:00.559 --> 00:25:03.350
cosmic microwave background radiation
00:25:03.360 --> 00:25:05.669
um which beyond which we can't see. But
00:25:05.679 --> 00:25:07.430
the universe almost certainly goes on be
00:25:07.440 --> 00:25:09.909
beyond that probably for a very long
00:25:09.919 --> 00:25:12.230
way. It may be very big. But we've got
00:25:12.240 --> 00:25:14.950
no knowledge of a boundary or or any
00:25:14.960 --> 00:25:17.029
other medium that it might be expanding
00:25:17.039 --> 00:25:18.310
into.
00:25:18.320 --> 00:25:22.470
>> So um one possibility is the idea of
00:25:22.480 --> 00:25:27.029
multiple universes and they might exist
00:25:27.039 --> 00:25:30.789
maybe in a higher dimensional
00:25:30.799 --> 00:25:34.630
uh arena if I can put it that way. you
00:25:34.640 --> 00:25:37.990
know, if you've if if you can um find
00:25:38.000 --> 00:25:40.789
that there are extra dimensions, we we
00:25:40.799 --> 00:25:42.789
know the three dimensions of space and
00:25:42.799 --> 00:25:45.830
one of time, that's what we've got now.
00:25:45.840 --> 00:25:49.750
Um but uh if there are hidden extra
00:25:49.760 --> 00:25:53.029
dimensions, maybe they provide a venue
00:25:53.039 --> 00:25:56.870
for the universe to expand into. Uh and
00:25:56.880 --> 00:25:59.350
there are various theories that accept
00:25:59.360 --> 00:26:02.630
that. um M theory is one of them where M
00:26:02.640 --> 00:26:04.470
is probably an abbreviation for
00:26:04.480 --> 00:26:06.310
membrane. The idea is that the universe
00:26:06.320 --> 00:26:08.390
is can be collapsed onto a
00:26:08.400 --> 00:26:10.470
two-dimensional membrane and there are
00:26:10.480 --> 00:26:12.870
lots of these membranes in the univer in
00:26:12.880 --> 00:26:15.110
the in the kind of higher dimensional
00:26:15.120 --> 00:26:17.190
universe but that's just conjecture and
00:26:17.200 --> 00:26:20.230
we've got no mechanism for proving that
00:26:20.240 --> 00:26:22.149
at the moment the only thing we know
00:26:22.159 --> 00:26:24.230
with certainty with absolute certainty
00:26:24.240 --> 00:26:26.230
is that the universe is expanding.
00:26:26.240 --> 00:26:28.230
>> Yes. uh at an accelerating rate,
00:26:28.240 --> 00:26:29.990
although the accelerating rate's not as
00:26:30.000 --> 00:26:32.390
accelerating as it once was. Possibly.
00:26:32.400 --> 00:26:33.110
>> Possibly.
00:26:33.120 --> 00:26:35.350
>> Um yeah, there there's there's three
00:26:35.360 --> 00:26:38.710
possible shapes of the universe. He asks
00:26:38.720 --> 00:26:41.909
it's if it's a a sphere. Um there's uh
00:26:41.919 --> 00:26:43.909
the flat universe theory. Oh, do we have
00:26:43.919 --> 00:26:46.310
to go there? Uh there's the closed
00:26:46.320 --> 00:26:49.190
universe theory, which is the positive
00:26:49.200 --> 00:26:52.390
curvature, so a sphere. or the open
00:26:52.400 --> 00:26:54.390
universe theory which is negative
00:26:54.400 --> 00:26:56.390
curvature. So it's more like the shape
00:26:56.400 --> 00:26:57.909
of a saddle.
00:26:57.919 --> 00:27:01.909
>> From what I'm reading, the most popular
00:27:01.919 --> 00:27:04.710
>> likelihood is the flat universe theory,
00:27:04.720 --> 00:27:07.350
>> but it but it's only flat in a ukidian
00:27:07.360 --> 00:27:10.230
sense. It doesn't mean it's shaped like
00:27:10.240 --> 00:27:11.830
a tabletop.
00:27:11.840 --> 00:27:14.149
>> Uh it means that parallel lines never
00:27:14.159 --> 00:27:16.549
meet. Basically, that's what we mean by
00:27:16.559 --> 00:27:17.909
flat. It's the the shape of the
00:27:17.919 --> 00:27:20.870
geometry. And the other thing that they
00:27:20.880 --> 00:27:23.750
suggest is that um you know it can be
00:27:23.760 --> 00:27:25.750
flat and still expanding as you said uh
00:27:25.760 --> 00:27:28.390
it might be infinite. We've we've talked
00:27:28.400 --> 00:27:30.630
about that before and there is likely no
00:27:30.640 --> 00:27:32.870
center and no edge.
00:27:32.880 --> 00:27:35.190
>> Correct. That's what we believe.
00:27:35.200 --> 00:27:40.310
>> Yeah. Now um to its shape so
00:27:40.320 --> 00:27:42.789
uh so
00:27:42.799 --> 00:27:45.029
basically I think Ken's question is is
00:27:45.039 --> 00:27:47.110
it spherical
00:27:47.120 --> 00:27:49.990
>> and we don't know the answer to that. We
00:27:50.000 --> 00:27:52.950
we know that the volume within which we
00:27:52.960 --> 00:27:56.950
can detect is spherical because the the
00:27:56.960 --> 00:27:59.350
cosmic microwave background radiation
00:27:59.360 --> 00:28:02.789
forms a an imaginary shell all around
00:28:02.799 --> 00:28:05.990
all around our galaxy. And it's the same
00:28:06.000 --> 00:28:08.149
distance in every direction. So in that
00:28:08.159 --> 00:28:10.549
regard, it's what we call isotropic, the
00:28:10.559 --> 00:28:12.710
same in all directions.
00:28:12.720 --> 00:28:15.110
Uh and that's really the only thing we
00:28:15.120 --> 00:28:18.149
can lay it down to. But there are ideas
00:28:18.159 --> 00:28:20.310
that if you looked at the universe on a
00:28:20.320 --> 00:28:21.990
bigger scale than we could see, it
00:28:22.000 --> 00:28:24.149
wouldn't be that it might be different
00:28:24.159 --> 00:28:26.389
in different directions.
00:28:26.399 --> 00:28:29.029
Um, and that in fact has been
00:28:29.039 --> 00:28:31.190
hypothesized as one of the sources of
00:28:31.200 --> 00:28:33.269
dark energy that we're just seeing a
00:28:33.279 --> 00:28:34.630
local bit of the universe that's
00:28:34.640 --> 00:28:37.590
expanding whose expansion is increasing
00:28:37.600 --> 00:28:40.630
whereas somewhere else it might be
00:28:40.640 --> 00:28:42.310
slowing down the expansion of the
00:28:42.320 --> 00:28:45.669
universe. Um,
00:28:45.679 --> 00:28:45.990
>> yeah,
00:28:46.000 --> 00:28:46.950
>> sorry. Go on.
00:28:46.960 --> 00:28:49.029
>> No, that that would be a a universe
00:28:49.039 --> 00:28:50.789
that's not isotropic. It's not the same
00:28:50.799 --> 00:28:52.630
in all directions, but we assume it's
00:28:52.640 --> 00:28:55.190
isotropic. That's all we can do in our
00:28:55.200 --> 00:28:56.870
assumptions in cosmology.
00:28:56.880 --> 00:28:59.190
>> We just can't see
00:28:59.200 --> 00:29:01.269
beyond what we can see, which sounds
00:29:01.279 --> 00:29:02.789
stupid, but that's that's the way the
00:29:02.799 --> 00:29:03.909
universe is.
00:29:03.919 --> 00:29:04.310
>> Yeah.
00:29:04.320 --> 00:29:06.630
>> Um Yeah. We've got the known universe
00:29:06.640 --> 00:29:08.389
and then the rest.
00:29:08.399 --> 00:29:09.190
>> That's right.
00:29:09.200 --> 00:29:09.909
>> Basically,
00:29:09.919 --> 00:29:11.350
>> and the rest might be a lot bigger than
00:29:11.360 --> 00:29:12.230
the known universe.
00:29:12.240 --> 00:29:14.470
>> We just Yeah. But we just don't know. Um
00:29:14.480 --> 00:29:16.389
I I [clears throat] the only thing I
00:29:16.399 --> 00:29:18.070
thought of is like you look at Earth's
00:29:18.080 --> 00:29:20.310
atmosphere and as you go out it fins and
00:29:20.320 --> 00:29:24.630
so there's no defined line between space
00:29:24.640 --> 00:29:28.310
and the earth proper. Could the universe
00:29:28.320 --> 00:29:30.870
be of the same ilk?
00:29:30.880 --> 00:29:32.950
Yes. But that would imply that the
00:29:32.960 --> 00:29:35.669
spacetime just sort of keeps keeps on
00:29:35.679 --> 00:29:37.990
going. It just might be empty.
00:29:38.000 --> 00:29:39.590
>> Uh
00:29:39.600 --> 00:29:41.029
>> yeah. Don't know.
00:29:41.039 --> 00:29:41.909
>> Don't know more.
00:29:41.919 --> 00:29:44.149
>> We don't know. We don't know.
00:29:44.159 --> 00:29:46.850
>> Why are you asking us? We don't know.
00:29:46.860 --> 00:29:49.350
[laughter]
00:29:49.360 --> 00:29:52.149
>> Oh dear. Um, thank you, Ken. Uh, very
00:29:52.159 --> 00:29:54.070
thoughtprovoking question and thanks for
00:29:54.080 --> 00:29:55.590
sending it in. If you have questions for
00:29:55.600 --> 00:29:58.310
us, please send them to us via our
00:29:58.320 --> 00:30:00.389
website, spacenutspodcast.com,
00:30:00.399 --> 00:30:01.909
spacenuts.io.
00:30:01.919 --> 00:30:03.269
There's a little button at the top
00:30:03.279 --> 00:30:06.149
called AMA, and that's what you click on
00:30:06.159 --> 00:30:08.470
to send us text and audio questions. If
00:30:08.480 --> 00:30:10.149
you've got a device with a microphone,
00:30:10.159 --> 00:30:12.470
you're all set. Uh most smartphones and
00:30:12.480 --> 00:30:14.950
smart devices have that and you can send
00:30:14.960 --> 00:30:17.669
it to us in audio form. Don't forget to
00:30:17.679 --> 00:30:18.789
tell us who you are and where you're
00:30:18.799 --> 00:30:20.470
from or you can send us a text question.
00:30:20.480 --> 00:30:23.110
Just fill in the blanks. And while
00:30:23.120 --> 00:30:24.310
you're there, have a look around, visit
00:30:24.320 --> 00:30:26.710
the shop, get something from yourself.
00:30:26.720 --> 00:30:29.750
Um you know, whatever you like. And
00:30:29.760 --> 00:30:31.430
we're done. Fred, thank you so much.
00:30:31.440 --> 00:30:34.549
That was a tough one. [laughter]
00:30:34.559 --> 00:30:37.510
Well, we you know, uh Space Nuts always
00:30:37.520 --> 00:30:40.070
probes the limits of knowledge. We does.
00:30:40.080 --> 00:30:40.630
That's what we do.
00:30:40.640 --> 00:30:42.789
>> Unfortunately, I have such limited
00:30:42.799 --> 00:30:44.710
knowledge. I'm not very helpful, but um
00:30:44.720 --> 00:30:45.990
glad you're here.
00:30:46.000 --> 00:30:48.310
>> No, you are very helpful and um so are
00:30:48.320 --> 00:30:50.230
our listeners because they keep on
00:30:50.240 --> 00:30:51.029
probing which
00:30:51.039 --> 00:30:53.350
>> they do indeed. All right, Fred. Thanks
00:30:53.360 --> 00:30:54.549
very much. We'll catch you on the next
00:30:54.559 --> 00:30:55.350
episode.
00:30:55.360 --> 00:30:56.789
>> Sounds great. Thanks, Andrew.
00:30:56.799 --> 00:30:58.310
>> Professor Fred Watson, astronomer at
00:30:58.320 --> 00:31:00.310
large. And thanks to Hugh in the studio,
00:31:00.320 --> 00:31:01.590
who couldn't be with us today because
00:31:01.600 --> 00:31:03.510
he's been expanding at an accelerating
00:31:03.520 --> 00:31:05.510
rate, so he went to the gym. And from
00:31:05.520 --> 00:31:07.110
me, Andrew Dunley, thanks for your
00:31:07.120 --> 00:31:08.310
company. We'll see you on the next
00:31:08.320 --> 00:31:10.549
episode of Space Nuts. Bye-bye.
00:31:10.559 --> 00:31:11.510
>> Space nuts.
00:31:11.520 --> 00:31:13.669
>> You've been listening to the Space Nuts
00:31:13.679 --> 00:31:15.909
podcast
00:31:15.919 --> 00:31:18.070
>> available at [music] Apple Podcasts,
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[music] from byes.com.
Kind: captions
Language: en
00:00:00.080 --> 00:00:01.829
Hello again. Thanks for joining us on
00:00:01.839 --> 00:00:04.230
Space Nuts. This is a Q&A edition. My
00:00:04.240 --> 00:00:06.390
name is Andrew Dunley. What's a Q&A
00:00:06.400 --> 00:00:08.710
edition? It's an edition where we get
00:00:08.720 --> 00:00:12.150
Q's and give you A's because you're so
00:00:12.160 --> 00:00:14.070
clever. Uh, something like that. Anyway,
00:00:14.080 --> 00:00:15.270
we're going to answer audience
00:00:15.280 --> 00:00:16.630
questions. That's what I'm getting at.
00:00:16.640 --> 00:00:18.710
We've got questions about Red Shift. We
00:00:18.720 --> 00:00:21.670
got questions about dark photons. What?
00:00:21.680 --> 00:00:24.230
Uh, we've got questions about deep space
00:00:24.240 --> 00:00:26.390
astronomy. And another one about the
00:00:26.400 --> 00:00:28.310
expansion of the universe. So, I think
00:00:28.320 --> 00:00:30.070
we talked about that last episode.
00:00:30.080 --> 00:00:31.910
Anyway, uh we'll see if we can solve all
00:00:31.920 --> 00:00:34.790
of that on this episode of Space Nuts.
00:00:34.800 --> 00:00:39.590
>> 15 seconds. Guidance is internal. 10 9
00:00:39.600 --> 00:00:41.350
Ignition sequence start.
00:00:41.360 --> 00:00:42.310
>> Space Nuts.
00:00:42.320 --> 00:00:47.190
>> 5 4 3 2 1 2 3 4 5 5 4 3 2 1
00:00:47.200 --> 00:00:48.389
>> Space Nuts.
00:00:48.399 --> 00:00:51.430
>> Astronauts report. It feels good.
00:00:51.440 --> 00:00:55.029
And with us again to kind of try to
00:00:55.039 --> 00:00:57.270
maybe answer some of that is Professor
00:00:57.280 --> 00:00:59.270
Fred Watson, astronomer at large. Hello,
00:00:59.280 --> 00:00:59.990
Fred.
00:01:00.000 --> 00:01:02.709
>> Hello, Andrew. Um, kind of is probably
00:01:02.719 --> 00:01:04.835
the best description really, isn't it?
00:01:04.845 --> 00:01:05.750
[laughter]
00:01:05.760 --> 00:01:09.030
>> Possibly. So, possibly so. Um, but you
00:01:09.040 --> 00:01:10.469
know, it's good to get questions. We've
00:01:10.479 --> 00:01:13.590
got a whole new batch. So, um, let's get
00:01:13.600 --> 00:01:15.510
stuck straight into it. Our first
00:01:15.520 --> 00:01:18.710
question comes from, um, uh, I I love
00:01:18.720 --> 00:01:20.630
the way he always ends his questions.
00:01:20.640 --> 00:01:23.030
I'm not going to reveal anything, but um
00:01:23.040 --> 00:01:24.710
let's hear from Roger.
00:01:24.720 --> 00:01:27.749
>> Hey there, space nuts. This is Roger the
00:01:27.759 --> 00:01:31.270
truck driver. Tonight I'm in uh Rutland,
00:01:31.280 --> 00:01:32.789
Vermont.
00:01:32.799 --> 00:01:34.550
Got a question about the red shift of
00:01:34.560 --> 00:01:36.149
galaxies.
00:01:36.159 --> 00:01:38.710
Um if the light that we're seeing from a
00:01:38.720 --> 00:01:41.510
far off galaxy is shifted to the red and
00:01:41.520 --> 00:01:44.550
it started out at a higher frequency,
00:01:44.560 --> 00:01:46.550
doesn't that mean energy's lost
00:01:46.560 --> 00:01:49.190
somewhere between here and there? And is
00:01:49.200 --> 00:01:52.149
that energy just transferred into space?
00:01:52.159 --> 00:01:54.950
And if it is, does that contribute to
00:01:54.960 --> 00:01:56.950
the expansion of space? And I'm not
00:01:56.960 --> 00:01:59.749
saying it's dark energy, but it is does
00:01:59.759 --> 00:02:03.350
it contribute to it or does that energy
00:02:03.360 --> 00:02:06.630
get dissipated in another way? All
00:02:06.640 --> 00:02:08.790
right. Always digging the show. You guys
00:02:08.800 --> 00:02:10.991
keep on trucking.
00:02:11.001 --> 00:02:13.830
[laughter] I love that. I love that. Uh
00:02:13.840 --> 00:02:15.430
we got train drivers that do that.
00:02:15.440 --> 00:02:17.190
Unfortunately, they do it at 3:00 in the
00:02:17.200 --> 00:02:18.790
morning. [gasps]
00:02:18.800 --> 00:02:21.270
Although today he did it at 10 to 7, I
00:02:21.280 --> 00:02:23.430
was pretty annoyed. Pretty annoyed.
00:02:23.440 --> 00:02:25.030
>> This is uh the one going past your
00:02:25.040 --> 00:02:25.430
place.
00:02:25.440 --> 00:02:27.110
>> Yeah, behind our place there's a rail
00:02:27.120 --> 00:02:28.630
line. It doesn't get used a heck of a
00:02:28.640 --> 00:02:31.350
lot, but when it does, um yes, the the
00:02:31.360 --> 00:02:33.990
glasses rattle. Uh the ones on my face,
00:02:34.000 --> 00:02:35.990
I mean. Uh thanks, Roger. Great
00:02:36.000 --> 00:02:39.830
question. Uh so um yeah the change in
00:02:39.840 --> 00:02:44.790
frequency with the um energy loss um
00:02:44.800 --> 00:02:46.550
where does the energy go and does it
00:02:46.560 --> 00:02:48.470
contribute to the expansion of the
00:02:48.480 --> 00:02:51.910
universe and could it possibly be maybe
00:02:51.920 --> 00:02:55.990
maybe not dark matter or dark energy
00:02:56.000 --> 00:02:56.710
>> or something.
00:02:56.720 --> 00:02:57.030
>> Yeah.
00:02:57.040 --> 00:02:59.270
>> Yeah. Um there's a lot he packed a lot
00:02:59.280 --> 00:03:00.229
into that question.
00:03:00.239 --> 00:03:02.390
>> He did and it's a great question too. Uh
00:03:02.400 --> 00:03:06.470
and you know I mean it's a um project is
00:03:06.480 --> 00:03:08.149
absolutely right the conservation of
00:03:08.159 --> 00:03:11.430
energy uh energy can't be created or
00:03:11.440 --> 00:03:13.589
destroyed. That's the the fundamental
00:03:13.599 --> 00:03:18.457
rule. Uh it's energy is always conserved
00:03:18.467 --> 00:03:20.470
[snorts] but
00:03:20.480 --> 00:03:22.630
uh the universe doesn't play by the
00:03:22.640 --> 00:03:24.869
ordinary rules.
00:03:24.879 --> 00:03:30.470
Uh and um it it's a it's an interesting
00:03:30.480 --> 00:03:33.670
answer here. Um and and I have to say
00:03:33.680 --> 00:03:37.110
it's changed my view of what this you
00:03:37.120 --> 00:03:38.550
know what the answer to this problem
00:03:38.560 --> 00:03:39.430
was.
00:03:39.440 --> 00:03:39.750
>> Okay.
00:03:39.760 --> 00:03:43.110
>> Uh because um when we've been asked this
00:03:43.120 --> 00:03:46.470
before been asked it for a long time I
00:03:46.480 --> 00:03:49.270
just assumed that the energy uh
00:03:49.280 --> 00:03:51.589
basically was absorbed by the universe
00:03:51.599 --> 00:03:53.830
by spacetime
00:03:53.840 --> 00:03:56.710
uh and maybe contributed to the
00:03:56.720 --> 00:04:00.789
expansion. Although there's it's a it's
00:04:00.799 --> 00:04:02.630
a you can't have it both ways because
00:04:02.640 --> 00:04:04.710
it's the expansion that's causing the
00:04:04.720 --> 00:04:08.390
the photon's energy to be to be lost. Uh
00:04:08.400 --> 00:04:11.429
and and just stepping back exactly as
00:04:11.439 --> 00:04:13.670
Roger said, uh you've got light going
00:04:13.680 --> 00:04:17.189
through the universe. It's uh the its
00:04:17.199 --> 00:04:18.789
wavelength is being stretched by the
00:04:18.799 --> 00:04:21.349
expansion of the universe. Therefore,
00:04:21.359 --> 00:04:24.150
the light is losing energy because the
00:04:24.160 --> 00:04:26.629
energy of a beam of light is all about
00:04:26.639 --> 00:04:28.469
the frequency of the light. In other
00:04:28.479 --> 00:04:30.230
words, or the wavelength, putting it
00:04:30.240 --> 00:04:31.189
another way.
00:04:31.199 --> 00:04:34.310
>> So, if you increase the wavelength, you
00:04:34.320 --> 00:04:38.390
lose energy and that's that's um a given
00:04:38.400 --> 00:04:41.270
already. Uh so, what I used to say was
00:04:41.280 --> 00:04:43.030
yes, it kind of goes into the universe,
00:04:43.040 --> 00:04:45.110
but um I've done a bit more reading on
00:04:45.120 --> 00:04:48.193
this and I was wrong. Oh.
00:04:48.203 --> 00:04:48.870
[sighs and gasps]
00:04:48.880 --> 00:04:51.510
Um because
00:04:51.520 --> 00:04:54.950
when you apply general relativity to the
00:04:54.960 --> 00:04:57.830
universe as a whole and that's the as
00:04:57.840 --> 00:04:59.270
we've talked about and we talked about
00:04:59.280 --> 00:05:01.830
it at length in the last episode it's uh
00:05:01.840 --> 00:05:04.150
the the kind of fundamental rule that
00:05:04.160 --> 00:05:06.710
governs everything that we understand in
00:05:06.720 --> 00:05:10.390
the universe. Um when you apply general
00:05:10.400 --> 00:05:11.990
relativity
00:05:12.000 --> 00:05:18.070
uh that conservation of energy that we
00:05:18.080 --> 00:05:21.510
expect to happen in the everyday world
00:05:21.520 --> 00:05:25.590
uh it doesn't hold good. So uh energy is
00:05:25.600 --> 00:05:28.550
not conserved in an expanding universe.
00:05:28.560 --> 00:05:29.590
>> Oh
00:05:29.600 --> 00:05:34.710
>> uh and so basically the energy simply
00:05:34.720 --> 00:05:36.310
disappears.
00:05:36.320 --> 00:05:39.270
It's just not there anymore because of
00:05:39.280 --> 00:05:41.510
the expansion of the universe. It's not
00:05:41.520 --> 00:05:43.110
causing the expansion of the universe.
00:05:43.120 --> 00:05:45.110
It's not create contributing to dark
00:05:45.120 --> 00:05:47.590
energy or dark matter, the energy loss.
00:05:47.600 --> 00:05:49.590
It just vanishes.
00:05:49.600 --> 00:05:50.310
>> Wow.
00:05:50.320 --> 00:05:51.749
>> So, work that one out.
00:05:51.759 --> 00:05:53.189
>> I can't. [snorts]
00:05:53.199 --> 00:05:55.670
>> No, I can't either. [laughter]
00:05:55.680 --> 00:05:59.670
>> Uh it's um it's I I kind of really need
00:05:59.680 --> 00:06:02.390
to look at the equations on this.
00:06:02.400 --> 00:06:05.909
>> Um you don't show them to me. I mean,
00:06:05.919 --> 00:06:07.990
I'm yeah I'm not that keen on looking at
00:06:08.000 --> 00:06:09.990
them myself either got too much else to
00:06:10.000 --> 00:06:13.990
do but uh but um uh but that's yes that
00:06:14.000 --> 00:06:18.950
is the thinking on this uh and I think
00:06:18.960 --> 00:06:22.550
the conservation rule does not work uh
00:06:22.560 --> 00:06:25.110
when it comes to
00:06:25.120 --> 00:06:28.309
um when it comes to consu to to to the
00:06:28.319 --> 00:06:30.309
universe on a whole.
00:06:30.319 --> 00:06:33.670
>> Yeah. Wow. Gee, that's um that's quite a
00:06:33.680 --> 00:06:35.189
revelation. And who who figured that
00:06:35.199 --> 00:06:37.189
out?
00:06:37.199 --> 00:06:38.309
>> Uh [sighs]
00:06:38.319 --> 00:06:40.870
uh it's on a number of uh different
00:06:40.880 --> 00:06:43.350
physics uh related.
00:06:43.360 --> 00:06:45.350
>> There's there there's the reason no one
00:06:45.360 --> 00:06:48.059
knows about it cuz it's physics and
00:06:48.069 --> 00:06:48.870
[laughter]
00:06:48.880 --> 00:06:51.029
who reads that stuff?
00:06:51.039 --> 00:06:53.350
>> Yeah. I think I think the relativistic
00:06:53.360 --> 00:06:55.350
bit of it
00:06:55.360 --> 00:06:59.189
>> uh comes from the fact that the energy
00:06:59.199 --> 00:07:00.790
of a particle which is what we're
00:07:00.800 --> 00:07:04.390
talking about it's an observer dependent
00:07:04.400 --> 00:07:07.670
quantity and so that's why relativity
00:07:07.680 --> 00:07:09.589
plays a part in this because you're the
00:07:09.599 --> 00:07:12.390
observer and and you're talking about
00:07:12.400 --> 00:07:14.710
something that's relative to another
00:07:14.720 --> 00:07:16.629
observer i.e. the photon.
00:07:16.639 --> 00:07:19.749
>> Yeah. Uh, and that's why you've got, you
00:07:19.759 --> 00:07:22.309
know, a relivist a relativistic uh,
00:07:22.319 --> 00:07:24.150
access to it.
00:07:24.160 --> 00:07:27.670
>> Wow. Okay. Um, great question, Roger.
00:07:27.680 --> 00:07:29.189
I'm not sure you were expecting that
00:07:29.199 --> 00:07:31.589
answer, but uh, there it is. Uh, the
00:07:31.599 --> 00:07:33.909
energy just
00:07:33.919 --> 00:07:35.510
gone,
00:07:35.520 --> 00:07:39.589
goes, vanishes, ceases to exist. It's a
00:07:39.599 --> 00:07:41.670
dead poly.
00:07:41.680 --> 00:07:43.589
So
00:07:43.599 --> 00:07:47.350
anyway, um, no one got that joke. I was,
00:07:47.360 --> 00:07:50.070
um, I was doing a Montipython skit for
00:07:50.080 --> 00:07:50.629
some reason.
00:07:50.639 --> 00:07:52.629
>> Yeah. Yeah, you were. That's right. I'm
00:07:52.639 --> 00:07:55.189
I'm Look, I'm pursuing this in a little
00:07:55.199 --> 00:07:57.510
bit more detail and, uh, and just trying
00:07:57.520 --> 00:07:59.029
to, you know, see whether we've got
00:07:59.039 --> 00:08:03.189
alternative alternative views of this.
00:08:03.199 --> 00:08:04.869
>> Generally speaking, you do get
00:08:04.879 --> 00:08:06.469
alternative views when it comes to this
00:08:06.479 --> 00:08:06.869
kind.
00:08:06.879 --> 00:08:08.550
>> That's right.
00:08:08.560 --> 00:08:15.270
>> Um, yes. So, so the the that's right. Uh
00:08:15.280 --> 00:08:17.110
I think I think the the standard
00:08:17.120 --> 00:08:20.070
explanation today is that energy is not
00:08:20.080 --> 00:08:23.589
is not conserved. Okay, we'll leave it
00:08:23.599 --> 00:08:25.189
at that until somebody throws another
00:08:25.199 --> 00:08:26.309
spanner into the
00:08:26.319 --> 00:08:27.670
>> Yeah, we might be giving a different
00:08:27.680 --> 00:08:28.710
answer next week.
00:08:28.720 --> 00:08:30.710
>> It could be. [laughter] Thanks, Roger.
00:08:30.720 --> 00:08:32.550
Great to hear from you. Toot toot. Uh
00:08:32.560 --> 00:08:34.550
we'll catch you next time. Our next
00:08:34.560 --> 00:08:38.070
question comes from Peter. He's from San
00:08:38.080 --> 00:08:40.070
Diego, California. While listening to
00:08:40.080 --> 00:08:42.389
another astrophysics podcast, I heard
00:08:42.399 --> 00:08:45.590
the term dark photon for the first time.
00:08:45.600 --> 00:08:47.110
Apparently, this is a particle
00:08:47.120 --> 00:08:49.829
astrophysicists are seeking in order to
00:08:49.839 --> 00:08:52.310
explain dark matter and/or dark energy.
00:08:52.320 --> 00:08:54.389
Could you please elaborate on what a
00:08:54.399 --> 00:08:58.550
dark photon could be? Um, dad joke for
00:08:58.560 --> 00:09:01.110
Andrew. A photon travels at the speed of
00:09:01.120 --> 00:09:03.509
light. Does that mean a dark photon
00:09:03.519 --> 00:09:06.266
travels at the speed of dark?
00:09:06.276 --> 00:09:06.870
>> [laughter]
00:09:06.880 --> 00:09:08.949
>> I like that. That's good.
00:09:08.959 --> 00:09:10.630
>> That's really good. Keep up the great
00:09:10.640 --> 00:09:12.790
work, he says. Uh, thank you, Peter.
00:09:12.800 --> 00:09:15.030
Hope all is well in San Diego,
00:09:15.040 --> 00:09:16.230
California.
00:09:16.240 --> 00:09:17.910
>> Uh, have you ever heard of a dark
00:09:17.920 --> 00:09:20.710
photon, Fred? Um, yes. I've probably got
00:09:20.720 --> 00:09:22.870
a few in this box here. [laughter]
00:09:22.880 --> 00:09:25.750
Um, your the speed of dark just just
00:09:25.760 --> 00:09:29.430
going back to that that quip. Uh there
00:09:29.440 --> 00:09:33.430
was a story I read uh probably a
00:09:33.440 --> 00:09:37.829
fortnight ago uh about exactly this in
00:09:37.839 --> 00:09:40.710
that darkness
00:09:40.720 --> 00:09:43.350
can move faster than the speed of light.
00:09:43.360 --> 00:09:45.670
>> No, [clears throat]
00:09:45.680 --> 00:09:48.790
it it's but it's a an illusory darkness.
00:09:48.800 --> 00:09:52.630
is when you've got um light beams
00:09:52.640 --> 00:09:55.430
interfering with one another so that
00:09:55.440 --> 00:09:58.550
you've that and interference
00:09:58.560 --> 00:10:00.630
light beams can cancel out. So if you've
00:10:00.640 --> 00:10:02.710
got two light waves and you add them up
00:10:02.720 --> 00:10:04.470
out of phase, they can cancel out and
00:10:04.480 --> 00:10:06.550
you get darkness.
00:10:06.560 --> 00:10:07.829
>> That's well-known principle of
00:10:07.839 --> 00:10:09.750
intererometry. I used to play with that
00:10:09.760 --> 00:10:13.190
when I was a student a lot. Uh but there
00:10:13.200 --> 00:10:14.870
are certain circumstances that those
00:10:14.880 --> 00:10:18.630
patterns of darkness can actually exceed
00:10:18.640 --> 00:10:21.190
the speed of light because they're not
00:10:21.200 --> 00:10:22.949
actually real. They're not real
00:10:22.959 --> 00:10:24.790
entities. They're not a thing that's
00:10:24.800 --> 00:10:26.470
carrying any sort of information or
00:10:26.480 --> 00:10:29.452
energy. They're just patterns in a in an
00:10:29.462 --> 00:10:30.470
[clears throat] interference pattern.
00:10:30.480 --> 00:10:32.230
They're just dark patches in it. And I
00:10:32.240 --> 00:10:33.990
think under certain circumstances, they
00:10:34.000 --> 00:10:36.949
could go faster than the speed of light.
00:10:36.959 --> 00:10:40.069
So, darkness might be not quite as uh
00:10:40.079 --> 00:10:43.190
you know as twe as you thought it was,
00:10:43.200 --> 00:10:43.829
>> I guess.
00:10:43.839 --> 00:10:47.590
>> Anyway, anyway, uh that's not the the
00:10:47.600 --> 00:10:50.069
question. Uh because dark photons are
00:10:50.079 --> 00:10:51.990
definitely something different and
00:10:52.000 --> 00:10:54.230
they're basically
00:10:54.240 --> 00:10:56.949
uh hypothetical. They've been
00:10:56.959 --> 00:10:59.269
hypothesized by physicists and
00:10:59.279 --> 00:11:00.790
cosmologists
00:11:00.800 --> 00:11:05.590
as being a force carrier similar to the
00:11:05.600 --> 00:11:09.750
ordinary photon but related to
00:11:09.760 --> 00:11:12.389
dark matter.
00:11:12.399 --> 00:11:15.430
In in other words, you might have Sorry,
00:11:15.440 --> 00:11:17.110
somebody's trying to phone me. I'm just
00:11:17.120 --> 00:11:18.790
going to kill that call.
00:11:18.800 --> 00:11:19.350
>> Yeah.
00:11:19.360 --> 00:11:21.190
>> Uh um
00:11:21.200 --> 00:11:24.472
>> that was me. That was me. No, it wasn't.
00:11:24.482 --> 00:11:25.782
[laughter]
00:11:25.792 --> 00:11:26.310
>> [sighs and gasps]
00:11:26.320 --> 00:11:27.990
>> They're they're you know they're part of
00:11:28.000 --> 00:11:30.949
the there may be when we discover
00:11:30.959 --> 00:11:34.150
finally what dark matter is there may be
00:11:34.160 --> 00:11:38.389
a suite of dark particles
00:11:38.399 --> 00:11:40.470
which could include dark photons. That's
00:11:40.480 --> 00:11:41.990
the line
00:11:42.000 --> 00:11:43.110
>> right?
00:11:43.120 --> 00:11:45.269
>> And and so you know we mentioned last
00:11:45.279 --> 00:11:48.310
week the or the last episode the uh the
00:11:48.320 --> 00:11:50.630
large hydrron collider being upgraded to
00:11:50.640 --> 00:11:52.470
be the high luminosity large hydrron
00:11:52.480 --> 00:11:55.670
collider. Um, that's one of the things
00:11:55.680 --> 00:11:57.110
they'd be looking for will be dark
00:11:57.120 --> 00:11:58.870
photons.
00:11:58.880 --> 00:12:04.230
Okay. Uh, yeah, I tried to do a um an AI
00:12:04.240 --> 00:12:07.509
search for an explanation on it and um
00:12:07.519 --> 00:12:09.670
it it it sort of gave me all this gobbly
00:12:09.680 --> 00:12:13.030
but um you know what would a dark
00:12:13.040 --> 00:12:16.150
proton photon do? It says it would carry
00:12:16.160 --> 00:12:19.269
a force within the dark sector.
00:12:19.279 --> 00:12:21.430
We call that the government. uh it might
00:12:21.440 --> 00:12:23.430
allow dark matter particles to interact
00:12:23.440 --> 00:12:25.430
with each other and it could very weakly
00:12:25.440 --> 00:12:27.910
mix with normal photons giving us a way
00:12:27.920 --> 00:12:30.710
to detect it. And the reason they reckon
00:12:30.720 --> 00:12:33.110
that scientists care about this is as
00:12:33.120 --> 00:12:35.350
you said could explain what dark matter
00:12:35.360 --> 00:12:38.230
is made of. So therefore solving some of
00:12:38.240 --> 00:12:40.310
those gaps in our current physics
00:12:40.320 --> 00:12:42.389
theories.
00:12:42.399 --> 00:12:44.550
So that's that's that's why people are
00:12:44.560 --> 00:12:45.750
interested in this and that's why
00:12:45.760 --> 00:12:47.350
they're upgrading the Large Hadron
00:12:47.360 --> 00:12:49.110
Collider and
00:12:49.120 --> 00:12:52.470
>> hopefully we will learn more in years to
00:12:52.480 --> 00:12:55.829
come. That's that's the that's the hope.
00:12:55.839 --> 00:12:57.590
That's the hope. Yeah. So we might you
00:12:57.600 --> 00:12:59.269
know we might be talking one day about
00:12:59.279 --> 00:13:01.829
dark photons um having been detected
00:13:01.839 --> 00:13:03.430
which would be
00:13:03.440 --> 00:13:05.910
>> a coup for space nukes.
00:13:05.920 --> 00:13:08.389
>> Yes, it will. Uh but at this stage uh
00:13:08.399 --> 00:13:10.949
they are not proven. It's just a theory.
00:13:10.959 --> 00:13:13.030
So that's That's about as much as we
00:13:13.040 --> 00:13:15.030
know at this point in time.
00:13:15.040 --> 00:13:17.750
>> But uh very good question uh and thank
00:13:17.760 --> 00:13:19.990
you Peter for sending it in. This is
00:13:20.000 --> 00:13:22.069
Space Nuts with Andrew Dunley and
00:13:22.079 --> 00:13:25.590
Professor Fred Watson.
00:13:25.600 --> 00:13:27.350
Let's take a short break from the show
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>> And I feel
00:15:15.279 --> 00:15:17.430
>> Space Nuts. Okay, Fred, we'll move
00:15:17.440 --> 00:15:19.430
straight on to our next question, which
00:15:19.440 --> 00:15:23.430
is uh another audio question from Eli.
00:15:23.440 --> 00:15:27.829
Hello, this is Eli from sunny Coachella
00:15:27.839 --> 00:15:30.870
Valley in California.
00:15:30.880 --> 00:15:33.430
I'm embarrassed to admit it, but I still
00:15:33.440 --> 00:15:35.189
can't get my head around deep space
00:15:35.199 --> 00:15:38.230
astronomy. I get that the light from say
00:15:38.240 --> 00:15:41.910
a distant galaxy is a billion years old.
00:15:41.920 --> 00:15:44.550
But why that particular point in its
00:15:44.560 --> 00:15:47.189
time? Is it just a matter of whatever
00:15:47.199 --> 00:15:49.749
light is hitting us is the time we get
00:15:49.759 --> 00:15:51.749
to see?
00:15:51.759 --> 00:15:55.910
But for really early light, the JWST
00:15:55.920 --> 00:15:57.910
early universe stuff that's been
00:15:57.920 --> 00:16:01.269
traveling for 13 billion years and just
00:16:01.279 --> 00:16:04.310
hitting us now. Are we looking for the
00:16:04.320 --> 00:16:07.509
light that hasn't passed us by or hasn't
00:16:07.519 --> 00:16:10.710
made it here yet, but is from that one
00:16:10.720 --> 00:16:14.150
precise location long ago?
00:16:14.160 --> 00:16:16.550
This stuff is so difficult to get my
00:16:16.560 --> 00:16:19.829
head around. Love the show and hope you
00:16:19.839 --> 00:16:22.629
guys can clear this up for me.
00:16:22.639 --> 00:16:25.189
>> Uh, no we can't. We just thought we'd um
00:16:25.199 --> 00:16:27.990
put the question in there. Uh, thanks
00:16:28.000 --> 00:16:31.430
Eli. Uh it this is a deep um not only in
00:16:31.440 --> 00:16:33.509
deep space astronomy terms but it is a
00:16:33.519 --> 00:16:37.269
deep deep topic. Uh I mean when we look
00:16:37.279 --> 00:16:39.590
up into the sky at night and we see all
00:16:39.600 --> 00:16:42.389
those beautiful colored dots we are
00:16:42.399 --> 00:16:44.629
looking at history and it's variable
00:16:44.639 --> 00:16:47.829
history because some of it's 4.41 light
00:16:47.839 --> 00:16:51.269
years away and some of it's 400,000
00:16:51.279 --> 00:16:53.590
light years away. Some of it's further
00:16:53.600 --> 00:16:55.590
than that. It's um but then you've got
00:16:55.600 --> 00:16:58.069
the cosmic microwave background
00:16:58.079 --> 00:17:00.870
radiation which is kind of a leftover of
00:17:00.880 --> 00:17:03.430
of um [gasps]
00:17:03.440 --> 00:17:05.990
what happened after the big bang and
00:17:06.000 --> 00:17:08.470
that that's that's a different kettle to
00:17:08.480 --> 00:17:10.630
fish and I can understand why you got a
00:17:10.640 --> 00:17:13.591
headache Eli. Over to you Fred.
00:17:13.601 --> 00:17:14.470
[laughter]
00:17:14.480 --> 00:17:20.789
Thanks. Um so I guess you know that I I
00:17:20.799 --> 00:17:25.110
understand Eli's issue as well. um
00:17:25.120 --> 00:17:27.110
you you've got to be in the right place
00:17:27.120 --> 00:17:29.190
at the right time to see a photon from a
00:17:29.200 --> 00:17:32.789
distant galaxy. But I I guess the way to
00:17:32.799 --> 00:17:36.230
envisage this is if you think of the
00:17:36.240 --> 00:17:40.070
universe um and you've got to perhaps
00:17:40.080 --> 00:17:41.750
think of it as if you were looking at it
00:17:41.760 --> 00:17:43.590
from the outside, which we never can.
00:17:43.600 --> 00:17:46.150
But uh if you can think of it that way,
00:17:46.160 --> 00:17:48.950
then it's full of objects which are
00:17:48.960 --> 00:17:52.549
radiating light even in its infancy.
00:17:52.559 --> 00:17:54.150
when the universe was very young, the
00:17:54.160 --> 00:17:57.270
stuff in it was basically shining. Um
00:17:57.280 --> 00:17:59.350
once we got past the dark ages where no
00:17:59.360 --> 00:18:03.190
stars were shining, uh but um and those
00:18:03.200 --> 00:18:05.430
are the galaxies that we now see. So so
00:18:05.440 --> 00:18:08.310
they're constantly radiating light and
00:18:08.320 --> 00:18:10.310
that's like just like a river of light
00:18:10.320 --> 00:18:12.230
that's flowing
00:18:12.240 --> 00:18:15.350
down time, if I can put it that way. Uh
00:18:15.360 --> 00:18:19.669
and a long time in in the future, it
00:18:19.679 --> 00:18:22.630
reaches us. But it's not just, you know,
00:18:22.640 --> 00:18:25.110
an individual photon or something that's
00:18:25.120 --> 00:18:27.430
reaching us. It's this stream of stuff
00:18:27.440 --> 00:18:30.470
that is being radiated throughout the
00:18:30.480 --> 00:18:34.070
universe by these galaxies. So we um and
00:18:34.080 --> 00:18:37.270
and we we pick it up. We pick it up
00:18:37.280 --> 00:18:39.029
sometimes as exactly as you've said,
00:18:39.039 --> 00:18:40.870
well up to 10 billion years after it's
00:18:40.880 --> 00:18:43.350
been radiated. I think
00:18:43.360 --> 00:18:45.830
>> 12 billion years are the are the oldest
00:18:45.840 --> 00:18:47.830
or the earliest galaxies that we now
00:18:47.840 --> 00:18:49.510
see. We're looking back in time. 12
00:18:49.520 --> 00:18:51.750
billion years and seeing them as they
00:18:51.760 --> 00:18:54.470
were perhaps a billion and a half years
00:18:54.480 --> 00:18:57.190
after the big bang. Um, and they're they
00:18:57.200 --> 00:18:59.350
are shining. They're radiating light uh
00:18:59.360 --> 00:19:01.830
in the early universe and down the track
00:19:01.840 --> 00:19:03.830
that reaches us because that light's
00:19:03.840 --> 00:19:05.590
going in all directions. So, it wouldn't
00:19:05.600 --> 00:19:08.310
matter where in the universe we were, we
00:19:08.320 --> 00:19:10.870
would still see them. Uh, we'd just see
00:19:10.880 --> 00:19:12.549
them in a, you know, in a different
00:19:12.559 --> 00:19:14.630
position in the sky if we're a long way
00:19:14.640 --> 00:19:15.990
from where we are now.
00:19:16.000 --> 00:19:19.990
>> Yeah. Um but yeah so I I guess it's you
00:19:20.000 --> 00:19:22.549
know in a way one way of thinking about
00:19:22.559 --> 00:19:25.430
this is if you imagine us on planet
00:19:25.440 --> 00:19:28.390
earth here and imagine us being
00:19:28.400 --> 00:19:32.630
surrounded by a whole series of shells
00:19:32.640 --> 00:19:34.630
uh which we're at the center of and this
00:19:34.640 --> 00:19:36.310
is a bit like the crystalline spheres
00:19:36.320 --> 00:19:38.470
that people used to think uh the
00:19:38.480 --> 00:19:41.590
universe was made of. Uh but these these
00:19:41.600 --> 00:19:44.549
shells uh spherical shells all centered
00:19:44.559 --> 00:19:47.590
on the earth but each one clicks over to
00:19:47.600 --> 00:19:51.669
a to a a time further in the past. Uh
00:19:51.679 --> 00:19:53.510
because the lights coming to us from the
00:19:53.520 --> 00:19:55.990
whole the whole cosmos which is full of
00:19:56.000 --> 00:19:58.390
stuff. Uh and that's why we can see
00:19:58.400 --> 00:20:00.230
these these shells sort of being
00:20:00.240 --> 00:20:02.710
illuminated in a way by the objects that
00:20:02.720 --> 00:20:05.830
uh that radiated them at that time. uh
00:20:05.840 --> 00:20:09.270
that has um that we see them because of
00:20:09.280 --> 00:20:11.590
the the distance that they are away from
00:20:11.600 --> 00:20:13.909
us means that they've the light has
00:20:13.919 --> 00:20:15.990
taken that long to get to us. Whether
00:20:16.000 --> 00:20:17.990
that helps or not in fact I think I've
00:20:18.000 --> 00:20:20.924
just confused it completely but
00:20:20.934 --> 00:20:21.830
[snorts]
00:20:21.840 --> 00:20:25.029
um I
00:20:25.039 --> 00:20:27.750
just doing a little experimental search
00:20:27.760 --> 00:20:30.789
here for a sec.
00:20:30.799 --> 00:20:34.390
What what I I I agree with in terms of
00:20:34.400 --> 00:20:36.630
Eli's question and and getting your head
00:20:36.640 --> 00:20:40.230
around it is um if Beetlejuice or
00:20:40.240 --> 00:20:42.149
however you want to pronounce it went
00:20:42.159 --> 00:20:47.029
supernova right now as we were speaking
00:20:47.039 --> 00:20:50.230
>> we wouldn't see it for
00:20:50.240 --> 00:20:52.470
640 years.
00:20:52.480 --> 00:20:53.669
>> Yeah.
00:20:53.679 --> 00:20:57.350
So for it to have gone supernova in the
00:20:57.360 --> 00:21:00.230
past and us to witness it, it has to
00:21:00.240 --> 00:21:02.470
have happened
00:21:02.480 --> 00:21:06.230
pretty close to 640 years ago. Does that
00:21:06.240 --> 00:21:07.110
make sense?
00:21:07.120 --> 00:21:09.830
>> Yes. Um so you could think of that in
00:21:09.840 --> 00:21:13.909
another way. Um you know um anywhere
00:21:13.919 --> 00:21:16.630
between us and 640 light years away
00:21:16.640 --> 00:21:18.710
there could be this pulse of light
00:21:18.720 --> 00:21:20.789
that's on its way to us
00:21:20.799 --> 00:21:23.909
>> from Beetlejuice. uh it would spread out
00:21:23.919 --> 00:21:26.470
in a sphere uh and as that sphere
00:21:26.480 --> 00:21:28.549
expanded eventually it would wash over
00:21:28.559 --> 00:21:31.590
the earth and we'd see it um and perhaps
00:21:31.600 --> 00:21:33.350
see it during the day as well because it
00:21:33.360 --> 00:21:35.270
might get bright enough to do that.
00:21:35.280 --> 00:21:37.350
>> Uh and and I think that's a really good
00:21:37.360 --> 00:21:39.669
way of putting it, Andrew, because um
00:21:39.679 --> 00:21:41.029
thinking about the galaxies, they're
00:21:41.039 --> 00:21:43.029
just streaming light out all the time.
00:21:43.039 --> 00:21:45.750
But something like uh a supernova
00:21:45.760 --> 00:21:47.909
explosion which gives a big pulse of
00:21:47.919 --> 00:21:50.710
light um that's perhaps easier to get
00:21:50.720 --> 00:21:52.549
your head around because that's that's
00:21:52.559 --> 00:21:57.029
just got a um it'll take whatever
00:21:57.039 --> 00:21:59.029
whatever time is represented by the
00:21:59.039 --> 00:22:02.310
distance away. So 640 light years away.
00:22:02.320 --> 00:22:04.549
It'll take 640 years to get here for
00:22:04.559 --> 00:22:06.470
that pulse to get here. But then it will
00:22:06.480 --> 00:22:09.190
sweep over us uh and we'll see the light
00:22:09.200 --> 00:22:11.110
the the light fading away.
00:22:11.120 --> 00:22:15.190
>> Yeah. And um the reason I chose that
00:22:15.200 --> 00:22:18.149
target is because there's a lot of
00:22:18.159 --> 00:22:20.710
conjecture about its future and the
00:22:20.720 --> 00:22:22.390
possibility that it's reaching that
00:22:22.400 --> 00:22:23.909
critical mass point.
00:22:23.919 --> 00:22:24.710
>> Yes.
00:22:24.720 --> 00:22:26.390
>> Um but it could have already happened.
00:22:26.400 --> 00:22:28.789
That's the other thing. [laughter]
00:22:28.799 --> 00:22:30.870
>> But we that's that's something we can
00:22:30.880 --> 00:22:33.029
have no knowledge of. That's the the key
00:22:33.039 --> 00:22:35.669
thing because um we are limited by the
00:22:35.679 --> 00:22:37.669
speed of light. That's the thing that
00:22:37.679 --> 00:22:39.350
always limits our view of the universe.
00:22:39.360 --> 00:22:41.830
And just to confuse Eli a little bit
00:22:41.840 --> 00:22:45.590
more, there are probably things in the
00:22:45.600 --> 00:22:47.430
universe we will never witness because
00:22:47.440 --> 00:22:49.590
the light is just too far away to reach
00:22:49.600 --> 00:22:51.909
us in any reasonable amount of time.
00:22:51.919 --> 00:22:53.350
Even even
00:22:53.360 --> 00:22:56.149
>> beyond the life of the earth itself or
00:22:56.159 --> 00:22:57.430
or our sun,
00:22:57.440 --> 00:23:01.110
>> we we we there are things we will never
00:23:01.120 --> 00:23:03.350
ever know about.
00:23:03.360 --> 00:23:04.390
>> Correct.
00:23:04.400 --> 00:23:06.870
>> It's um and that's where it just gives
00:23:06.880 --> 00:23:08.605
you um
00:23:08.615 --> 00:23:09.110
>> [snorts and laughter]
00:23:09.120 --> 00:23:11.110
>> one of those headaches that uh requires
00:23:11.120 --> 00:23:13.909
you to take paracetamol and ibuprofen at
00:23:13.919 --> 00:23:17.776
the same time. So,
00:23:17.786 --> 00:23:18.870
[laughter]
00:23:18.880 --> 00:23:21.350
>> um deep deep headaches. But Eli, great
00:23:21.360 --> 00:23:23.110
question. I'm not sure we solved your
00:23:23.120 --> 00:23:27.830
problem, but um anyway, uh it it I I try
00:23:27.840 --> 00:23:29.190
to explain this sort of stuff to my
00:23:29.200 --> 00:23:33.510
grandson uh and my granddaughters and
00:23:33.520 --> 00:23:36.230
you know, how do you explain time and
00:23:36.240 --> 00:23:40.549
distance to a to a a young child and um
00:23:40.559 --> 00:23:41.430
when you're trying to get through
00:23:41.440 --> 00:23:43.750
traffic, it's [laughter]
00:23:43.760 --> 00:23:45.190
>> that might not be the best time to do
00:23:45.200 --> 00:23:45.510
it.
00:23:45.520 --> 00:23:46.789
>> Probably not, but they're very
00:23:46.799 --> 00:23:47.990
interested.
00:23:48.000 --> 00:23:50.149
>> Very interested. Thanks, Eli. Great
00:23:50.159 --> 00:23:53.029
question.
00:23:53.039 --> 00:23:55.430
The crew of Artemis 2 now bound for the
00:23:55.440 --> 00:23:57.909
moon. Humanity's next great voyage
00:23:57.919 --> 00:23:59.270
begins.
00:23:59.280 --> 00:24:03.270
>> Space nuts. Our final question uh comes
00:24:03.280 --> 00:24:07.029
from Nova Scotia. It's from Ken. Uh
00:24:07.039 --> 00:24:08.470
look, this is an old chestnut. We've
00:24:08.480 --> 00:24:10.950
we've probably spoken about this many
00:24:10.960 --> 00:24:13.510
times, but it's always good to um to to
00:24:13.520 --> 00:24:15.990
revisit. If the universe is expanding,
00:24:16.000 --> 00:24:20.070
what is it expanding into? And also is
00:24:20.080 --> 00:24:23.269
the universe spherical?
00:24:23.279 --> 00:24:25.669
So um yes, what's it expanding into?
00:24:25.679 --> 00:24:29.350
Well, we don't know. And yes,
00:24:29.360 --> 00:24:32.230
>> that's yes. Uh it's actually we don't
00:24:32.240 --> 00:24:33.110
know and maybe
00:24:33.120 --> 00:24:35.110
>> and maybe maybe.
00:24:35.120 --> 00:24:39.669
>> So um the the universe is everything
00:24:39.679 --> 00:24:41.909
that we can detect. That's the
00:24:41.919 --> 00:24:43.269
definition of the universe. Everything
00:24:43.279 --> 00:24:46.870
we can measure or detect. And that means
00:24:46.880 --> 00:24:49.909
and we observe the expansion
00:24:49.919 --> 00:24:52.470
but we don't know whether there's an
00:24:52.480 --> 00:24:54.070
edge to the universe. We don't know
00:24:54.080 --> 00:24:55.990
whether it's infinite. We don't know
00:24:56.000 --> 00:24:58.390
anything beyond the horizons that we
00:24:58.400 --> 00:25:00.549
see. And the most obvious one is the
00:25:00.559 --> 00:25:03.350
cosmic microwave background radiation
00:25:03.360 --> 00:25:05.669
um which beyond which we can't see. But
00:25:05.679 --> 00:25:07.430
the universe almost certainly goes on be
00:25:07.440 --> 00:25:09.909
beyond that probably for a very long
00:25:09.919 --> 00:25:12.230
way. It may be very big. But we've got
00:25:12.240 --> 00:25:14.950
no knowledge of a boundary or or any
00:25:14.960 --> 00:25:17.029
other medium that it might be expanding
00:25:17.039 --> 00:25:18.310
into.
00:25:18.320 --> 00:25:22.470
>> So um one possibility is the idea of
00:25:22.480 --> 00:25:27.029
multiple universes and they might exist
00:25:27.039 --> 00:25:30.789
maybe in a higher dimensional
00:25:30.799 --> 00:25:34.630
uh arena if I can put it that way. you
00:25:34.640 --> 00:25:37.990
know, if you've if if you can um find
00:25:38.000 --> 00:25:40.789
that there are extra dimensions, we we
00:25:40.799 --> 00:25:42.789
know the three dimensions of space and
00:25:42.799 --> 00:25:45.830
one of time, that's what we've got now.
00:25:45.840 --> 00:25:49.750
Um but uh if there are hidden extra
00:25:49.760 --> 00:25:53.029
dimensions, maybe they provide a venue
00:25:53.039 --> 00:25:56.870
for the universe to expand into. Uh and
00:25:56.880 --> 00:25:59.350
there are various theories that accept
00:25:59.360 --> 00:26:02.630
that. um M theory is one of them where M
00:26:02.640 --> 00:26:04.470
is probably an abbreviation for
00:26:04.480 --> 00:26:06.310
membrane. The idea is that the universe
00:26:06.320 --> 00:26:08.390
is can be collapsed onto a
00:26:08.400 --> 00:26:10.470
two-dimensional membrane and there are
00:26:10.480 --> 00:26:12.870
lots of these membranes in the univer in
00:26:12.880 --> 00:26:15.110
the in the kind of higher dimensional
00:26:15.120 --> 00:26:17.190
universe but that's just conjecture and
00:26:17.200 --> 00:26:20.230
we've got no mechanism for proving that
00:26:20.240 --> 00:26:22.149
at the moment the only thing we know
00:26:22.159 --> 00:26:24.230
with certainty with absolute certainty
00:26:24.240 --> 00:26:26.230
is that the universe is expanding.
00:26:26.240 --> 00:26:28.230
>> Yes. uh at an accelerating rate,
00:26:28.240 --> 00:26:29.990
although the accelerating rate's not as
00:26:30.000 --> 00:26:32.390
accelerating as it once was. Possibly.
00:26:32.400 --> 00:26:33.110
>> Possibly.
00:26:33.120 --> 00:26:35.350
>> Um yeah, there there's there's three
00:26:35.360 --> 00:26:38.710
possible shapes of the universe. He asks
00:26:38.720 --> 00:26:41.909
it's if it's a a sphere. Um there's uh
00:26:41.919 --> 00:26:43.909
the flat universe theory. Oh, do we have
00:26:43.919 --> 00:26:46.310
to go there? Uh there's the closed
00:26:46.320 --> 00:26:49.190
universe theory, which is the positive
00:26:49.200 --> 00:26:52.390
curvature, so a sphere. or the open
00:26:52.400 --> 00:26:54.390
universe theory which is negative
00:26:54.400 --> 00:26:56.390
curvature. So it's more like the shape
00:26:56.400 --> 00:26:57.909
of a saddle.
00:26:57.919 --> 00:27:01.909
>> From what I'm reading, the most popular
00:27:01.919 --> 00:27:04.710
>> likelihood is the flat universe theory,
00:27:04.720 --> 00:27:07.350
>> but it but it's only flat in a ukidian
00:27:07.360 --> 00:27:10.230
sense. It doesn't mean it's shaped like
00:27:10.240 --> 00:27:11.830
a tabletop.
00:27:11.840 --> 00:27:14.149
>> Uh it means that parallel lines never
00:27:14.159 --> 00:27:16.549
meet. Basically, that's what we mean by
00:27:16.559 --> 00:27:17.909
flat. It's the the shape of the
00:27:17.919 --> 00:27:20.870
geometry. And the other thing that they
00:27:20.880 --> 00:27:23.750
suggest is that um you know it can be
00:27:23.760 --> 00:27:25.750
flat and still expanding as you said uh
00:27:25.760 --> 00:27:28.390
it might be infinite. We've we've talked
00:27:28.400 --> 00:27:30.630
about that before and there is likely no
00:27:30.640 --> 00:27:32.870
center and no edge.
00:27:32.880 --> 00:27:35.190
>> Correct. That's what we believe.
00:27:35.200 --> 00:27:40.310
>> Yeah. Now um to its shape so
00:27:40.320 --> 00:27:42.789
uh so
00:27:42.799 --> 00:27:45.029
basically I think Ken's question is is
00:27:45.039 --> 00:27:47.110
it spherical
00:27:47.120 --> 00:27:49.990
>> and we don't know the answer to that. We
00:27:50.000 --> 00:27:52.950
we know that the volume within which we
00:27:52.960 --> 00:27:56.950
can detect is spherical because the the
00:27:56.960 --> 00:27:59.350
cosmic microwave background radiation
00:27:59.360 --> 00:28:02.789
forms a an imaginary shell all around
00:28:02.799 --> 00:28:05.990
all around our galaxy. And it's the same
00:28:06.000 --> 00:28:08.149
distance in every direction. So in that
00:28:08.159 --> 00:28:10.549
regard, it's what we call isotropic, the
00:28:10.559 --> 00:28:12.710
same in all directions.
00:28:12.720 --> 00:28:15.110
Uh and that's really the only thing we
00:28:15.120 --> 00:28:18.149
can lay it down to. But there are ideas
00:28:18.159 --> 00:28:20.310
that if you looked at the universe on a
00:28:20.320 --> 00:28:21.990
bigger scale than we could see, it
00:28:22.000 --> 00:28:24.149
wouldn't be that it might be different
00:28:24.159 --> 00:28:26.389
in different directions.
00:28:26.399 --> 00:28:29.029
Um, and that in fact has been
00:28:29.039 --> 00:28:31.190
hypothesized as one of the sources of
00:28:31.200 --> 00:28:33.269
dark energy that we're just seeing a
00:28:33.279 --> 00:28:34.630
local bit of the universe that's
00:28:34.640 --> 00:28:37.590
expanding whose expansion is increasing
00:28:37.600 --> 00:28:40.630
whereas somewhere else it might be
00:28:40.640 --> 00:28:42.310
slowing down the expansion of the
00:28:42.320 --> 00:28:45.669
universe. Um,
00:28:45.679 --> 00:28:45.990
>> yeah,
00:28:46.000 --> 00:28:46.950
>> sorry. Go on.
00:28:46.960 --> 00:28:49.029
>> No, that that would be a a universe
00:28:49.039 --> 00:28:50.789
that's not isotropic. It's not the same
00:28:50.799 --> 00:28:52.630
in all directions, but we assume it's
00:28:52.640 --> 00:28:55.190
isotropic. That's all we can do in our
00:28:55.200 --> 00:28:56.870
assumptions in cosmology.
00:28:56.880 --> 00:28:59.190
>> We just can't see
00:28:59.200 --> 00:29:01.269
beyond what we can see, which sounds
00:29:01.279 --> 00:29:02.789
stupid, but that's that's the way the
00:29:02.799 --> 00:29:03.909
universe is.
00:29:03.919 --> 00:29:04.310
>> Yeah.
00:29:04.320 --> 00:29:06.630
>> Um Yeah. We've got the known universe
00:29:06.640 --> 00:29:08.389
and then the rest.
00:29:08.399 --> 00:29:09.190
>> That's right.
00:29:09.200 --> 00:29:09.909
>> Basically,
00:29:09.919 --> 00:29:11.350
>> and the rest might be a lot bigger than
00:29:11.360 --> 00:29:12.230
the known universe.
00:29:12.240 --> 00:29:14.470
>> We just Yeah. But we just don't know. Um
00:29:14.480 --> 00:29:16.389
I I [clears throat] the only thing I
00:29:16.399 --> 00:29:18.070
thought of is like you look at Earth's
00:29:18.080 --> 00:29:20.310
atmosphere and as you go out it fins and
00:29:20.320 --> 00:29:24.630
so there's no defined line between space
00:29:24.640 --> 00:29:28.310
and the earth proper. Could the universe
00:29:28.320 --> 00:29:30.870
be of the same ilk?
00:29:30.880 --> 00:29:32.950
Yes. But that would imply that the
00:29:32.960 --> 00:29:35.669
spacetime just sort of keeps keeps on
00:29:35.679 --> 00:29:37.990
going. It just might be empty.
00:29:38.000 --> 00:29:39.590
>> Uh
00:29:39.600 --> 00:29:41.029
>> yeah. Don't know.
00:29:41.039 --> 00:29:41.909
>> Don't know more.
00:29:41.919 --> 00:29:44.149
>> We don't know. We don't know.
00:29:44.159 --> 00:29:46.850
>> Why are you asking us? We don't know.
00:29:46.860 --> 00:29:49.350
[laughter]
00:29:49.360 --> 00:29:52.149
>> Oh dear. Um, thank you, Ken. Uh, very
00:29:52.159 --> 00:29:54.070
thoughtprovoking question and thanks for
00:29:54.080 --> 00:29:55.590
sending it in. If you have questions for
00:29:55.600 --> 00:29:58.310
us, please send them to us via our
00:29:58.320 --> 00:30:00.389
website, spacenutspodcast.com,
00:30:00.399 --> 00:30:01.909
spacenuts.io.
00:30:01.919 --> 00:30:03.269
There's a little button at the top
00:30:03.279 --> 00:30:06.149
called AMA, and that's what you click on
00:30:06.159 --> 00:30:08.470
to send us text and audio questions. If
00:30:08.480 --> 00:30:10.149
you've got a device with a microphone,
00:30:10.159 --> 00:30:12.470
you're all set. Uh most smartphones and
00:30:12.480 --> 00:30:14.950
smart devices have that and you can send
00:30:14.960 --> 00:30:17.669
it to us in audio form. Don't forget to
00:30:17.679 --> 00:30:18.789
tell us who you are and where you're
00:30:18.799 --> 00:30:20.470
from or you can send us a text question.
00:30:20.480 --> 00:30:23.110
Just fill in the blanks. And while
00:30:23.120 --> 00:30:24.310
you're there, have a look around, visit
00:30:24.320 --> 00:30:26.710
the shop, get something from yourself.
00:30:26.720 --> 00:30:29.750
Um you know, whatever you like. And
00:30:29.760 --> 00:30:31.430
we're done. Fred, thank you so much.
00:30:31.440 --> 00:30:34.549
That was a tough one. [laughter]
00:30:34.559 --> 00:30:37.510
Well, we you know, uh Space Nuts always
00:30:37.520 --> 00:30:40.070
probes the limits of knowledge. We does.
00:30:40.080 --> 00:30:40.630
That's what we do.
00:30:40.640 --> 00:30:42.789
>> Unfortunately, I have such limited
00:30:42.799 --> 00:30:44.710
knowledge. I'm not very helpful, but um
00:30:44.720 --> 00:30:45.990
glad you're here.
00:30:46.000 --> 00:30:48.310
>> No, you are very helpful and um so are
00:30:48.320 --> 00:30:50.230
our listeners because they keep on
00:30:50.240 --> 00:30:51.029
probing which
00:30:51.039 --> 00:30:53.350
>> they do indeed. All right, Fred. Thanks
00:30:53.360 --> 00:30:54.549
very much. We'll catch you on the next
00:30:54.559 --> 00:30:55.350
episode.
00:30:55.360 --> 00:30:56.789
>> Sounds great. Thanks, Andrew.
00:30:56.799 --> 00:30:58.310
>> Professor Fred Watson, astronomer at
00:30:58.320 --> 00:31:00.310
large. And thanks to Hugh in the studio,
00:31:00.320 --> 00:31:01.590
who couldn't be with us today because
00:31:01.600 --> 00:31:03.510
he's been expanding at an accelerating
00:31:03.520 --> 00:31:05.510
rate, so he went to the gym. And from
00:31:05.520 --> 00:31:07.110
me, Andrew Dunley, thanks for your
00:31:07.120 --> 00:31:08.310
company. We'll see you on the next
00:31:08.320 --> 00:31:10.549
episode of Space Nuts. Bye-bye.
00:31:10.559 --> 00:31:11.510
>> Space nuts.
00:31:11.520 --> 00:31:13.669
>> You've been listening to the Space Nuts
00:31:13.679 --> 00:31:15.909
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