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

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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