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| Woops. Yes, galaxies. Too late to edit.
> Anyway, given the number of galaxies in the ring, being at different distances but their projections just happening to form a rough circle would be even more astonishing than the galaxies in fact sharing a causal history due to some unknown early-universe mechanism. I don't understand what you mean by this. Why would it be "more astonishing" than an actual causal connection? Surely astronomers are more interested in causal connections than observational coincidences? To illustrate: the stars making up the constellation of Norma [1] form a rough square when seen from earth, but as their distances from Earth vary greatly this is just an illusion caused by Earth's relative orientation to them. Given the Copernican principle (which I accept is not a physical law) I'm struggling to see why a group of galaxies that form a circle only when seen from "near" earth [2] are actually cosmologically significant. I accept that the ring contains more than four galaxies, and this makes the ring more statistically significant than a square of galaxies. But it still implies a privileged viewpoint in order for it to be actually significant. I still have the gut feeling that this potential significance is more than offset by the enormously greater observational scale. tl/dr: why is this more than just naming a new constellation? (Just to re-iterate: I'm interested in understanding the errors in my mental model - and I'm not trying to poke holes in the work of scientists more qualified them me.) [1] https://en.wikipedia.org/wiki/Norma_(constellation) [2] And also, I guess, from a similar point on the other "side" of the ring |
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| which, to be clear, is the exact point the parent comment is making.
Randomness only favors something over noise if there is a non random process determining the structure |
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| When the entire class of things are unlikely given the number of observations. The odds that I personally may win the Jackpot are low but the odds that someone at sometime wins is very high. So me winning would surprise me but someone winning wouldn’t. Applying that rule to research and a lot of people are looking for something interesting in many domains not just this particular one.
Similarly finding any shape in a random set of points is much more likely than the odds of any one shape. So you need to adjust for both things people are looked for correlations and the entire class of things that would notice not just the odds of what you happened to see. A random process you run spitting out a famous quote would be low, but you would also be surprised Pi is 3,14 or Pi is 3.14 etc etc. Thus someone else hitting a random process and getting “To be or knot to be” is now looking at the odds that anyone anywhere would get something that’s close to something memorable which should actually be quite high. TLDR; https://xkcd.com/882/ |
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| Actually I do have a plausible mechanism whose numbers have been sanity checked by a couple of cosmologists, but has never been published.
Here's the idea. The expansion of the universe is currently accelerating. If this continues indefinitely, we get the https://en.wikipedia.org/wiki/Big_Rip model. What happens if the Big Rip proceeds to the point where a lot of https://en.wikipedia.org/wiki/Vacuum_energy gets released, and that release stops the Rip by creating the next Big Bang? This could form a cycle since the next Bang creates cosmos that in turn will Rip. It doesn't sound entirely crazy to me. The Casimir effect shows that you should release vacuum energy when you constrain the volume that a particularly bit of space can interact with. The incredible expansion of a Rip should constrain such interactions. So a large release of vacuum energy seems expected. And who knows how releasing vacuum energy interacts with the acceleration of the expansion of the universe? Let's do a back of the envelope estimate. Theory estimates vacuum energy at something like 10^113 joules per cubic meter of vacuum energy. For comparison the visible universe is estimated at 10^53 kg. Using Einstein's E = mc^2, that's around 10^70 joules. Current cosmological models say that at the hottest part of the Big Bang, the universe must have already been larger than a cubic meter. Yes, there is a lot of energy not in the form of visible matter. Even so, there's a lot of room for a release of vacuum energy to explain the energy density needed at the beginning of a Big Bang. We at least pass the most basic sanity check. This would offer interesting answers to some key cosmological questions. Current Big Bang models struggle with how a large volume started out very uniform. Inflation has been proposed for this, but it has some problems. But in this model, extreme uniformity over a large volume is predicted. If you add in quantum fluctuations starting the vacuum release, that have spread out before we go from Rip to Bang, then you can also explain arbitrarily large structures in the universe. This also explains the arrow of time. How could we start off with such low entropy when entropy is always increasing? Well as the universe expands, entropy increases. But volume increases faster. We wind up with a giant universe filled with very low entropy/volume. When a small piece of that forms a new Big Bang, it again starts with very low entropy. Unfortunately, this involves an insane lack of conservation of energy. But GR provides no easy way to even state what conservation of energy means. At least not outside of limited classes of models. Which this is not one of. So the idea of energy not being conserved at cosmological scales is at least not entirely unprecedented by current theory. |
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| Carl Sagan would agree. In his book The Demon Haunted World he explains science in very similar terms as you. He also gives examples of primitive humans doing science. |
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| from Figure 1 (page 5 of the PDF) https://arxiv.org/pdf/2402.07591:
> The tangent-plane distribution of Mg II absorbers in the redshift slice z = 0.802 ± 0.060. the ring is visible in the slice, which corresponds to a distance range based on those redshift values and cosmological parameters. I think this is effectively a spherical shell of a certain thickness. |
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| It absolutely does not. "Interact with each other only gravitationally" has its plain and ordinary meaning: we're ignoring other interactions. No charge, no collisions, no radiation, etc. |
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| Ah, good, we've finally found Boulder's Ring. Weird that it's not in the middle of the Great Attractor, but maybe this was just the Xeelee's prototype. |
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| Wild speculation: It's the result of another universe poking into our own, forcing a bunch of galaxies near the center point to spread out in a circular fashion. |
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| Cool insight. Anyone with more knowledge care to weigh in? Some supermassive dark matter there? Also, on what timeframe might this change if so? Note to self to Google this topic in a year. |
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| The Cosmological Principle has been suspect for a long time. It just adds so little value and costs so much to our understanding of the universe. Best to stick to provable things. |
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| Too bad a ring is still too easy to get created naturally. If it would have had the shape of a square, or a dogecoin, that'd get really interesting |
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| The big bang was everywhere. Space itself was created by the big bang. It's not like a bomb going off in space somewhere even though that's more intuitive to imagine. |
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| Something so key to the news, and yet not mentioned in this article.
The ring we see is how it looked 9 billion years ago. The universe is 14 billion years old. So, when the universe was still a baby. |
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| Context, as it seems to have been missed:
>For reasons*, there's a soft limit on the scale that you'd expect structures** to scale to. The content you cited acknowledges the premise of the Cosmological Principle, but it does not say anything about what these "reasons" could be. So, nope, that's not an adequate argument. Again, I could waste my time on a PhD in Cosmology to come back and actually make a good argument for why homogeneity in structure is favored at large cosmological scales ... but why should I? I didn't bring that particular argument into the conversation [1]. 1: https://en.wikipedia.org/wiki/Burden_of_proof_(philosophy) |
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| I'm not an astronomer either, but pretty sure if I generated uniformly random points on the scale of number of visible galaxys, I could find a circle in there |
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| > 9.2 billion light-years from Earth
> cosmological neighbours These structures are more than halfway across the observable Universe. It's ludicrous to claim that they are neighbours. |
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| They're saying the Big Ring is a neighbor not of earth, but of the "giant arc of galaxies" which "appears in the same region of sky at the same distance from Earth as the Big Ring". |
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| If you've got two structures of size X, with a distance of X between them as well, that's relatively close.
That's as if Paris had a second Eiffel tower three blocks away. |
That last video, at about 3:55, shows the ring as a bunch of red balls surrounded by a bunch of blue balls. All the balls seem randomly distributed, but a small subset are colored red. I wonder what makes those balls different? There doesn't seem to be anything unusual about their arrangement, other than they chose to color them red.