TY. I think I get it, but I must devote more time to fully appreciate your 
comment. AG

On Friday, December 2, 2022 at 5:50:26 PM UTC-7 jessem wrote:

> The wiki page on the Hubble parameter also says in the section at 
> https://en.wikipedia.org/wiki/Hubble%27s_law#Time-dependence_of_Hubble_parameter
>  
> that the expansion seems to be accelerating in such a way that the first 
> derivative of the scale factor a(t) is increasing over time but the Hubble 
> parameter H(t) is decreasing, and that this has the implication "The 
> recession velocity of one chosen galaxy does increase, but different 
> galaxies passing a sphere of fixed radius cross the sphere more slowly at 
> later times". There's a more technical discussion of how these parameters 
> are defined at 
> https://en.wikipedia.org/wiki/Accelerating_expansion_of_the_universe#Technical_definition
>  
> which mentions that physicists define "accelerating expansion" specifically 
> in terms of the second derivative of the scale factor being positive, it 
> doesn't require an increasing Hubble parameter.
>
> On Fri, Dec 2, 2022 at 4:15 AM Alan Grayson <[email protected]> wrote:
>
>> It's measured about 70 km/sec/megaparsec. This is a direct measurement 
>> using red shift to measure recessional velocity, and different standard 
>> candles depending on the distance. So, at a distance of one megaparsec, the 
>> expansion rate is 70 km/sec; at two megaparsecs the expansion rate is 140 
>> km/sec; and so on. This suggests the rate of expansion is greater as we go 
>> back in time; or conversely, that the rate of expansion is slower as we go 
>> forward in time. How is this reconciled with the 1998 measurements that the 
>> rate of expansion is actually speeding up? AG 
>>
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