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 *


*, 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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