On 5/31/2025 9:00 PM, Alan Grayson wrote:


On Saturday, May 31, 2025 at 5:39:19 PM UTC-6 Brent Meeker wrote:



    On 5/31/2025 3:22 PM, Alan Grayson wrote:


    On Saturday, May 31, 2025 at 2:24:00 PM UTC-6 Brent Meeker wrote:

        And to be clear it was thought that the Hubble parameter was
        decreasing asymptotically to a constant value.  But /even
        with the Hubble parameter constant/ a receding galaxy is
        slower when it's close and recedes faster as it gets further
        away.  The recession speed is proportional to the distance;
        that's Hubble's law.

        Brent

    *
    *
    *This is confusing. Does Hubble's law hold in a universe where
    the expansion is speeding up? TY, AG
    *
    *Depends on what you mean by the speed of expansion. Hubble's
    parameter is the expansion speed per distance, so speed is
    proportional to distance.  Hubble's law assumed this to be a
    constant.  Then since every galaxy is moving to a greater distance
    then every galaxy is speeding up.

    Brent*

*
*
*Doesn't that imply that distant galaxies, at earlier times, were moving faster than nearby galaxies, *
More distant galaxies are always receding faster than less distant galaxies.   But in the past those more distant galaxies and the nearby galaxies were both closer than they are now and so were both receding more slowly than they are now.

*and thus contradicts the fairly recent finding that the rate of expansion is increasing, not decreasing? *
"Rate of expansion" is NOT the speed of galaxies.  It's the Hubble parameter, the constant of proportionality, H, in the equation (recession speed of galaxy at distance d) = H*d.  Note H has the dimension of 1/time, NOT length/time.  The recent discovery is that H is increasing.  Any value of H>0 implies that more distant galaxies are receding faster than less distant galaxies.

Brent

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