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How Galaxies Are Disappearing From Our Universe

StartsWithABang writes: You've heard of dark energy before, and you know that it causes the expansion of our Universe to be accelerating. Instead of slowing down, distant galaxies are speeding up in their recession from us, rendering them unreachable from our point of view. But even though we can't see the light emitted from them today, we can still see the galaxies themselves! This article explains how this works, how no information gets lost, and what it means for the Big Bang.

19 of 174 comments (clear)

  1. Balloons by Intrepid+imaginaut · · Score: 4, Interesting

    What always bothered me about the balloon analogy was the implication that this expansion of space is mostly taking place where there's little actual matter, ie the space between galaxies. If it really was expanding like dots on a balloon, we'd see equivalent expansion within galaxies and as far as I'm aware we don't, at least not to any significant degree.

    Actually the whole thing is bothersome, if a galaxy was x light years away at some point in the past and it's now 2x light years away due to space expanding, doesn't that mean space has been created between the galaxies, and doesn't that violate some fairly fundamental laws of physics?

    1. Re:Balloons by wonkey_monkey · · Score: 4, Interesting

      As the AC's have said, gravity and other forces between particles completely swamp the "force" of expansion - for now. Imagine putting sheets of paper on a rubber sheet, and stretching the sheet. To an approximation, the centers of the pieces of paper would remain on the same spot on the sheet, while the rest of the paper would have the rubber sheet sliding out from under it, but the piece of paper would resist this "pull" on its edges easily.

      If the expansion of space is expanding, though, there will come at a time when this "force" (if it is a force, I'm the wrong person to ask) becomes more significant. First, gravity won't be able to hold galactic clusters together, then galaxies, then solar systems, then the forces between and within atoms won't be enough to keep them together.

      Sorry, bit of a downer to end on.

      --
      systemd is Roko's Basilisk.
    2. Re: Balloons by Immerman · · Score: 5, Interesting

      No. At least I don't think so. I'll admit my understanding is fuzzy, but a few points to think on:

      As I understand it (poorly), virtual particles appear to violate mass/energy conservation by their very nature - but they don't actually possess mass or energy themselves. Instead they sort of run on an "energy debt" for a few moments before either annihilating or capturing some "normal" energy so that they can persist. I think the energy is believed to be borrowed from the vacuum energy field - so that essentially you've temporarily lowered the energy of space itself in order to create some virtual particles, and there is no net energy change within the volume.

      Vacuum energy is *not* conserved - like dark energy it is created along with new space-time. Again this simply appears to be one of the fundamental laws of the universe - mass/energy conservation apparently doesn't apply to space-time itself, only to things *within* space-time.

      And finally there's a real possibility that matter can be created from whole cloth without violating conservation: In creating mass you also create a gravitational field, which in turn reduces the gravitational potential energy of everything else in the universe (gravitational energy is always negative). That reduction in the potential energy of the entire universe *may* perfectly balance the increase in mass-energy of the new matter. This is actually one of the theories about the big bang - it may be that the entire universe, taken as a whole, contains exactly zero net mass-energy: in essence everything really was created from nothing, and if you squeezed it all back together again you'd find there was still nothing there. It's just that the nothingness has been separated from itself in such a manner that things can be built out of the pieces.

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      --- Most topics have many sides worth arguing, allow me to take one opposite you.
    3. Re:Balloons by Immerman · · Score: 4, Interesting

      Not quite.

      The rate of dark-energy expansion is not actually changing - it's simply that as things drift apart you get more and more space between them, and since the space itself is expanding, the further apart you are, the more total expansion is occurring between you. Like stretching a rubber band with a couple marks near the middle - the ends will be getting further apart at a much faster rate than the marks near the middle, even though the entire rubber band is stretching at a constant rate.

      That means anything that is *already* drifting apart will accelerate apart indefinitely, but if the forces between two objects are currently holding them at a fixed distance from each other, then the amount of space (and dark energy) between them is not changing, and thus the repulsive "force" of expansion between them will likewise remain unchanged.

      Now for galaxies and even star systems - they're constantly shedding mass and energy, so *eventually* the gravitational bonds that hold them together may weaken to the point that they fly apart. And once that happens, and the space between objects begins to increase, only then can expansion begin to accelerate them apart even faster. For individual planets and stellar-remnants though, gravity is more than sufficient to keep the individual pieces in place.

      As for atoms... the distances between subatomic particles are fundamental - you can't raise an electron further from the nucleus without adding an extremely precise amount of energy as a photon, and it will rapidly shed that photon to return to its stable base state. It's simply not possible for things to "drift apart" - they can only exist at very precise distances determined by their quantum wavefunctions. And since things can't get drift apart, expansion can't get it's foot in the door. Atoms have nothing to fear from expansion except loneliness.

      --
      --- Most topics have many sides worth arguing, allow me to take one opposite you.
    4. Re:Balloons by boristhespider · · Score: 4, Interesting

      "doesn't that violate some fairly fundamental laws of physics?"

      Do you not think that one of the many thousands of theoretical and observational physicists who've worked on this model for decades would perhaps have spotted this flaw at some point in the last eighty years...? Of course it doesn't violate fundamental laws of physics. The whole thing is based tightly on general relativity, so regardless of whether you believe that relativity is being applied accurately to cosmology or not (I don't, not entirely) there is no suggestion of it violating any fairly fundamental laws. Conservation of mass/energy is absolutely guaranteed in relativity. (In two tightly-coupled ways - directly, and via the Bianchi identities which are nothing more than geometric identities along the lines of, but more complicated than, the Pythagoras theorem. Which one you take as more fundamental depends on your philosophy but in relativity the one implies the other.)

      The balloon analogy is basically flawed. It's also flawed because it relies on one imagining (to the extent that one can, and no-one can actually do so since our brains didn't evolve to imagine 4d let alone 5d) a 3+1d balloon embedded in a 4+1d spacetime, through the analogy with a 2d balloon embedded in 3d space. This inevitably leads to people understandably querying where the centre is and wondering if it's in the middle of this 4+1d space. It also leads people to understandably ask why the galaxies aren't expanding.

      Basically, they're not expanding because the theory doesn't apply in them. There are two ways of viewing this - the simple (but inaccurate) and the headfuck. The simple way of looking at it is that the cosmological expansion is extremely weak and is very easily overpowered by other, more local, forces. So galaxies are easily held together because the gravitational pull between stars in a galaxy is overwhelmingly stronger than the pull of the cosmological expansion. This, unfortunately, does suggest there's some kind of balancing of forces and some kind of spatial expansion, which isn't strictly speaking true.

      The headfuck is something that's actually almost impossible to model but straightforward to understand in relativity. The theory that the balloon analogy is based on is Friedman-Lemaitre-Robertson-Walker (FLRW - we're probably missing a name or two in there, as well) cosmology, based on what's known as the FLRW metric, which does nothing more than give the Pythagoras theorem in a 3+1d universe made up of an inverted pyramid of flat 3d spatial surfaces stacked one on top of the other along some time direction. (They could also be a load of nested spheres, or more bewilderingly a pile of saddles, but the data supports the flat model and there's currently no real reason to favour the so called closed or open models.) The FLRW metric applies on scales at which the universe seems to look the same in every direction and wherever you move to. In the jargon, it's "homoegenous and isotropic". Things like the SDSS surveys demonstrate how this can happen quite well -- take a look at http://www.a.phys.nagoya-u.ac.... which is the collection of data from the first SDSS survey (which ended about a decade back, I think; we're on SDSSIII or thereabouts now but I like this figure). On small scales this is obviously really knotty and far from homogeneous, but if you zoom out and squint slightly (to give a form of smoothing) then everything looks the same. Doing this a bit more rigorously, which is notoriously model-dependent, gives the "homogeneity scale" at somewhere in the order of 100Mpc, or about a hundred times larger than a typical galaxy cluster. That's the scale at which the FLRW model applies -- and that's the scale at which every single consequence can be said to hold. Below that, nothing that it says should be taken without a massive pinch of salt. This is particularly true in clusters, which are what is known as 'virialised' and detached from the cosmological expansion -- t

    5. Re: Balloons by hackwrench · · Score: 2

      Over what seem to us as long periods of time all atoms are unstable.

  2. Balloons by Anonymous Coward · · Score: 5, Interesting

    What always bothered me about the balloon analogy was the implication that this expansion of space is mostly taking place where there's little actual matter, ie the space between galaxies. If it really was expanding like dots on a balloon, we'd see equivalent expansion within galaxies and as far as I'm aware we don't, at least not to any significant degree.

    At that scale, gravity massively dwarfs expansion. For any system which is gravitationally bound, you can assume the "force" of expansion is trivial.

    Actually the whole thing is bothersome, if a galaxy was x light years away at some point in the past and it's now 2x light years away due to space expanding, doesn't that mean space has been created between the galaxies, and doesn't that violate some fairly fundamental laws of physics?

    I think you understand. Yes, the hypothesis is that space itself is being created, and that this is a fundamental law of physics. There's no fundamental law for it to violate, there's conservation mass and energy, no conservation of space.

  3. Save the Galaxies! by vortex2.71 · · Score: 5, Funny

    I am personally doing my part to conserve galaxies and I hope that all of you are too. Please, please, please help do your part to conserve this valuable resource before it is too late. Not just for today because it's Universe Day, but for life.

    1. Re:Save the Galaxies! by Livius · · Score: 4, Funny

      100 000 000 000 should be enough galaxies for anyone.

  4. Re:Pretty simple, really by BarbaraHudson · · Score: 2

    It's more likely they can't stand the insufferable whiners on the internet who can't stop talking about how horrible the world is.

    The ping time would be horrendous,
    The energy required tremendous,
    But they don't want your stash of p0rn
    To them naked walrus are stupendous.
    Burma Shave

    What would happen if the expansion of our knowledge outpaced the expansion of the universe? Is there a cross-over point, so that we (or our robotic descendants) will be able to literally control the universe? And if so, should we?

    --
    "Transparent" is a shit show that trades on every stereotype going. A man in drag is NOT a transsexual.
  5. The long and short of it. by Chas · · Score: 4, Interesting

    The universe is expanding.
    As it expands, attractant forces (like gravity) hold less and less sway over things.
    Without that "drag", more distant objects are speeding up.
    We're starting to get to the point that certain objects are far enough away that, unless we find a BIG loophole in physics someplace, we'll never be able to reach them. And unless we find it SOON, we'll lose track of these objects, thus pretty much negating our ability to plot a course to them at all.

    --


    Chas - The one, the only.
    THANK GOD!!!
    1. Re:The long and short of it. by Immerman · · Score: 2

      Actually we're not "starting to" get to that point, I believe the article stated that 97% of observable galaxies have *already* crossed that threshold - we're just still seeing the light that was emitted (mostly) long before they did so. And, like watching something fall into a black hole, we will continue to see their fading, increasingly red-shifted image for as long as we can construct instruments sensitive enough to detect the photons emitted in the last instants before it crossed the "event horizon".

      --
      --- Most topics have many sides worth arguing, allow me to take one opposite you.
  6. Re:What? by pauljlucas · · Score: 4, Informative

    The photons can't reach us from those distances because the amount of space between the far-off galaxies and us is increasing faster than light can travel.

    --
    If you reply, do so only to what I explicitly wrote. If I didn't write it, don't assume or infer it.
  7. Re:How galaxies are disappearing from our universe by Concerned+Onlooker · · Score: 2

    Yep. From the article:

    "And while no galaxy has literally disappeared to the point where it's invisible, 97% of them have disappeared in the sense that they're unreachable to us, and that the light they're emitting today will never reach us. The galaxies are still visible, but only due to their old light."

    They're not disappearing from THE universe, they're disappearing from OUR universe.

    --
    http://www.rootstrikers.org/
  8. Re:Balloons speckled with paint... by taiwanjohn · · Score: 4, Interesting

    A spot of paint on your balloon would locally restrict expansion as it inflates, as galaxies seem to do in our expanding universe. My understanding of current hypotheses is that dark matter plays the role of "paint" in this analogy. However, there's an intriguing alternative explanation, which only becomes apparent when you think of space as a fluid.

    Ironically, I stumbled upon this notion after musing on the strong interaction. (And I confess I was a bit high at the time.) Something that repels at a distance but attracts in proximity... that reminds me of bubbles interacting in the surface tension of fluids. So I googled "space as a fluid" and found that there's a whole branch of inquiry in this direction. It doesn't get as much attention as String Theory, but it's not dismissed out of hand either. (Correct me if I'm wrong... IANA physicist.)

    Anyway, I'm curious to hear others' thoughts on this.

    --
    XML is like violence. If it doesn't solve your problem, you're not using enough of it. --AC
  9. Re:Pretty simple, really by Anonymous Coward · · Score: 2, Funny

    This should be modded funny not interesting, seriously people (who have mod points)

  10. Re:'Big Rip' better than Heat Death by Immerman · · Score: 2

    Well, either that, or the "Big Crunch", or infinite expansion at an ever-decelerating rate. The "Critical universe" you describe was always vaguely improbable - one atom more or less and you end up with one of the other two. You almost need a deity fine-tuning things for it to be a viable option. We discovered dark energy accidentally when trying to determine which of the three possible outcomes mandated by existing physics was most likely.

    It had been assumed that the universe was in a steady state primarily for historical, religious reasons: God created the Heavens and the Earth to last forever and ever amen, and that myth wound its way into our assumptions about the world. Had this latest burst of scientific advances originated within Hindu cultures rather than Christian ones, the idea of a steady-state universe would likely have been considered ridiculous - probably the "Big Crunch" (and subsequent Bang) would have been the default assumption. In fact that would probably have been the assumption of most religions - cyclicity is a rather fundamental theme in most religions that don't completely disregard the realities of the world.

    --
    --- Most topics have many sides worth arguing, allow me to take one opposite you.
  11. Re:Where is the center? by boristhespider · · Score: 4, Interesting

    Yes you are, and because you're not educated in the field.

    "The article assumes that planet earth is the center of the universe"

    No it doesn't. Cosmology does not assume that the Earth is in the centre of the universe. It assumes the exact opposite. It's even known as the "cosmological principle" -- and it's a fundamental axiom in cosmology. Without it we wouldn't have the model that we're talking about. Instead we'd have Lemaitre-Tolman-Bondi models, which are isotropic around the Earth but definitely not homogeneous.

    Basically, building the cosmological model goes like this:

    1) Observe the CMB. This is all around us, at 2.7K, and is absolutely the same in every direction. It is, in the jargon, isotropic around the Earth.
    2) Assume that gravity on large scales is accurately modelled by a geometric theory of gravity (such as, but not restricted to, general relativity). We now know that on average the universe should be described by a metric that is at least isotropic about a point near to Earth.
    3) Since this is obviously absurd, as you've picked up on, apply the cosmological principle. If the Earth is not in a special position in the universe, which it would be an astonishing act of hubris to assume it is, but the universe looks isotropic around the Earth, then there are only two choices. We can either dump the cosmological principle and assume the universe is centred on Earth -- which is... untenable, given the vast scale of the observations -- or we can assume that the universe looks isotropic around every point. This implies that it is homogeneous and isotropic: every point is the same in every way.
    4) We can now tighten our previous assumption and assume that the universe is modelled by a metric that is isotropic around every point. That means that it is composed of what are known in the jargon as "maximally-symmetric" 3d surfaces. This leads us naturally and inevitably to the Friedman-Lemaitre-Robertson-Walker metrics, which give rise to the "big bang" theory you dislike so strongly.

    There are obviously problems here. The phrase "on average" is used frequently and without rigour. That rigour cannot, as yet, be provided. We have assumed twice the nature of gravity - first that it is geometric in origin, and second that it is described by general relativity, which is basically the simplest geometric theory of gravity. Fitting to observation also leads us, naturally and inevitably -- unpleasantly so, if we're being honest -- to dark energy and dark matter. But there is a need to "create these terms", in that the theory demands them, and the theory is *astonishingly successful*. One of the main successes of FLRW cosmology is that it first predicted a characteristic wavelength of ripples on the cosmic microwave background, which was then observed (and which can be used to determine how much dark matter there is relative to normal matter), and that that same wavelength should also be imprinted on the large-scale distribution of galaxies. This was *also* observed, and is exactly where it was predicted by combining CMB and supernovae observations. This is amazing not least because the theory predicts the CMB forming when the universe is around 300,000 years old, while the large-scale distribution of galaxies is observed when the universe is pushing on a bit, probably around 10bn-12bn years old. The wavelength on the galaxy distribution is therefore extremely stretched compared to that seen on the CMB. And, as one might expect, the level to which it is stretched is extraordinarily sensitive to the cosmology - it doesn't take much of a change in the levels of matter, dark matter and dark energy to put it slap bang in the wrong place entirely.

    Doing this unfortunately means we need to put dark energy in the model. Unsurprisingly, this isn't as ad-hoc as it seems, since there are multiple candidates for a dark energy, but it's still a bit unfortunate since not many of them are profoundly appealing. (Perhaps the most appealing is also the original, proposed by Wetterich in 1987, s

  12. Re:Galaxies Moving Away? Really? by pedestrian+crossing · · Score: 2

    Because they are really close together (on a cosmological scale). Gravity rules at this scale.

    --
    A house divided against itself cannot stand.