Le mer. 11 sept. 2024, 09:14, Alan Grayson <[email protected]> a
écrit :

>
>
> On Wednesday, September 11, 2024 at 12:41:56 AM UTC-6 Quentin Anciaux
> wrote:
>
> To be clearer, imagine you have points drawn on the surface of a balloon.
> As you inflate the balloon, the distance between two points increases, even
> though the points themselves aren't moving across the surface of the
> balloon. The farther apart the points are initially, the faster they seem
> to be moving away from each other as the balloon inflates. Similarly, in
> the universe, the farther away a galaxy is, the faster its recession
> velocity, but this velocity is due to the expansion of space itself, not
> because the galaxy is moving through space.
>
> Quentin
>
>
> *If we imagine two separated galaxies on the equator of an expanding
> sphere, the distance between them increases as the sphere expands. But the
> light from either will reach the other, unless the distance is increasing
> faster than c. How does your model guarantee that the distance is
> increasing faster than c? AG *
>

Because the expansion is continuous  as long as expansion rate is > 0,
sooner or later distant object will receed faster than c.

>
> Le mer. 11 sept. 2024, 08:37, Quentin Anciaux <[email protected]> a
> écrit :
>
>
>
> Le mer. 11 sept. 2024, 07:39, Alan Grayson <[email protected]> a écrit :
>
>
>
> On Tuesday, September 10, 2024 at 10:51:22 PM UTC-6 Quentin Anciaux wrote:
>
>
>
> Le mer. 11 sept. 2024, 00:06, Alan Grayson <[email protected]> a écrit :
>
>
>
> On Tuesday, September 10, 2024 at 3:50:08 PM UTC-6 Quentin Anciaux wrote:
>
>
>
> Le mar. 10 sept. 2024, 23:19, Alan Grayson <[email protected]> a écrit :
>
>
>
> On Tuesday, September 10, 2024 at 2:19:42 PM UTC-6 John Clark wrote:
>
> On Tue, Sep 10, 2024 at 3:57 PM Alan Grayson <[email protected]> wrote:
>
>
> *>> 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
>
>
> *That's the conventional wisdom but what is the physical mechanism? Hubble
> discovered that the universe was expanding faster in the past, than in the
> present.  Now its rate of expansion is much slower, allowing us to see many
> distant galaxies. What is the physical mechanism that will cause its
> present expansion rate to increase to greater than c*
>
>
> The expansion rate can still be the same or even slow down that my
> explanationis still valid,  no need for the *expansion rate* to change for
> current objects near the horizon to soon recess at more than c.
>
>
> *You haven't explained anything. You're just repeating what you've heard
> or read. A long time ago Brent explained it as a purely geometric result of
> the expansion, but now I tend to doubt that explanation. Specifically, if a
> galaxy now relatively close and visible but due to the expansion moves,
> say, into a region where the recessional velocity HAD BEEN some multiple of
> its recessional velocity when relatively near the Milky Way, why does its
> recessional velocity increase? AG *
>
>
> Because expansion is everywhere the same, take the inflated balloon
> example, any two points are receeding faster from each other as the balloon
> inflate at a constant rate, and again it's not the objects that are going
> at +c, but the space between those objects that expand.
>
>
> *, so distant galaxies will be beyond our field of view? AG*
>
> * John* K Clark    See what's on my new list at  Extropolis
> <https://groups.google.com/g/extropolis>
>
> hwt
>
>
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