Le mer. 11 sept. 2024, 18:15, Alan Grayson <[email protected]> a
écrit :

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> On Wednesday, September 11, 2024 at 10:08:42 AM UTC-6 Quentin Anciaux
> wrote:
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> Le mer. 11 sept. 2024, 18:04, Alan Grayson <[email protected]> a écrit :
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> On Wednesday, September 11, 2024 at 4:33:51 AM UTC-6 Quentin Anciaux wrote:
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> Le mer. 11 sept. 2024, 11:49, Alan Grayson <[email protected]> a écrit :
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> On Wednesday, September 11, 2024 at 3:26:01 AM UTC-6 Quentin Anciaux wrote:
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> Le mer. 11 sept. 2024, 11:23, Alan Grayson <[email protected]> a écrit :
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> On Tuesday, September 10, 2024 at 3:50:08 PM UTC-6 Quentin Anciaux wrote:
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> Le mar. 10 sept. 2024, 23:19, Alan Grayson <[email protected]> a écrit :
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> On Tuesday, September 10, 2024 at 2:19:42 PM UTC-6 John Clark wrote:
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> On Tue, Sep 10, 2024 at 3:57 PM Alan Grayson <[email protected]> wrote:
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>
> *>> Even if you ignore Dark Energy and postulate that the Hubble constant
> really is constant, every object a megaparsec away (3.26 million
> light-years) is moving away from us at about 70 kilometers per second. So
> if you try to look at objects a sufficiently large number of megaparsec
> away you will fail to find any because they are moving away from us faster
> than the speed of light.*
>
>
> >* That was in the past. At present, the universe is expanding at about
> 70 km/sec.*
>
>
> *Galaxies are receding from the Earth at 70 km/sec for EACH megaparsec
> distant from Earth they are. The further from Earth they are, the faster
> they are moving away from us, so if they are far enough away they will be
> moving faster than the speed of light away from us. *
>
> *> You're assuming the universe today is infinite,*
>
>
> *NO! I said IF the entire universe is infinite today then it was always
> infinite, and IF it was finite 10^-35 seconds after the Big Bang then it's
> still finite today. I also said nobody knows if the entire universe is
> infinite or finite. *
>
>
> *>* *Hubble's law applies to the past, not to the future,*
>
>
> *What the hell?!  *
>
>
> *How about an intelligent reply? Obviously, if the universe is infinite
> today, it was always infinite. But that's what I am questioning. For
> galaxies to fall out of view, they have to moving at greater than c. Now
> they aren't receding that fast. How will they start moving that fast?
> You're applying Hubble's law without thinking what it says. Just because a
> galaxy is now receding at less than c, how will continued expansion
> increase that speed to greater than c? AG *
>
>
> The farther they are the faster they are receding from you, so as they
> continue to get farther away they receed faster from you till the point
> they receed faster than c and go out of your horizon.
>
> Quentin
>
>
> Instead of preaching the Gospel, why don't you try to justify Brent's
> equation to prove your point, if you can. I see the distance separation
> along the equator for two separated galaxies as linear as the radius of the
> sphere expands. Brent uses Hubble's law, but the proof of what you claim
> shouldn't depend on Hubble, but just the geometry. AG
>
>
> I did multiple times with the balloon analogy which is purely geometrical,
> see previous answers.
>
>
> I don't think so. You just asserted it. AG
>
>
> The equation that links distance and recession velocity in both cases
> comes from the same geometric principles of uniform expansion in space. The
> proportionality between distance and velocity is a natural consequence of
> how expansion works, whether it’s on a 2D surface like a balloon or in 3D
> space like our universe.
>
> The expansion of the balloon and the universe follow similar dynamics
> because, in both cases, the expansion is homogeneous (the same everywhere)
> and isotropic (the same in all directions).
>
> If you mark two points close to each other on the balloon and start
> inflating it, those two points will move apart slowly. However, if you mark
> two points farther apart, they will move away from each other much more
> quickly as the balloon expands.
>
>
> This is what you keep claiming, but have yet to offer a *mathematical
> proof*. Try this; two galaxies on the equator of a sphere, with a
> separation distance s, and the equator expanding as a function of its
> radius r to simulate expansion. The recessional velocity is ds/dt, which
> depends on dr/dt. If dr/dt is constant, so will be ds/dt, and the
> recessional velocity is constant and cannot reach c or greater. What is
> wrong with this proof, falsifying Hubble's law and your model? AG
>
>
> I did multiple times and gave an example with points... up to you to read
> it.
>
>
> *You and Clark have no clue what a mathematical proof is. You're just
> stating what you believe, which might be true, but hardly qualifies as a
> proof of concept. AG *
>

🤣🤣🤣 ok figure out by yourself then... you're doing religion, not trying
to understand your mistake.

>
> In the same way, in the universe, the farther away a galaxy is, the more
> space there is between us and that galaxy. Since each portion of space is
> expanding, more distant galaxies experience the cumulative effect of the
> expansion over several portions of space. This means that for a galaxy at a
> great distance, the total expansion of space is larger, which results in a
> higher recession velocity.
>
> * John* K Clark    See what's on my new list at  Extropolis
> <https://groups.google.com/g/extropolis>
>
> hwt
>
>
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