The definition of the Hubble Constant implies the rate of expansion slows 
as time advances. I don't see that the two values contradict this 
conclusion. AG

On Friday, December 2, 2022 at 3:24:35 AM UTC-7 Lawrence Crowell wrote:

> Red shift data from supernovae SN1 give H = 74km/sec-Mpc. The velocity of 
> a region at distance d is v = Hd. Using the CMB data H = 70km/sec-Mpc. The 
> two data points appears distinct at a rather high sigma.
>
> LC
>
> On Friday, December 2, 2022 at 3:15:15 AM UTC-6 [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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