Einstein's Cat said:
How does proper distance change with time?
If ##D## is the (now) proper distance between us and a distant galaxy, then
$$D \left( t \right) = R \left( t \right) \chi,$$
where ##R \left( t \right)## is the scale factor for the universe (a solution to Friedmann's equation), ##\chi## is the constant comoving coordinate difference between us and the galaxy, and ##t## is cosmological time.
Einstein's Cat, are you familiar with calculus? Assuming you are, the rate of change of proper distance is given by
$$\frac{dD}{dt} = \frac{dR}{dt} \chi.$$
If the scale factor is known, then so is its rate of change ##dR/dt## , thus giving the rate change of proper distance, ##dD/dt##.
Multiplying the left side of the above equation by one in the form ##1=R/R##, and using ##D = R \chi## gives the Hubble relation
$$\frac{dD}{dt} = \frac{dR}{dt} \frac{R}{R} \chi = H D,$$
where the Hubble parameter (a function of time) is give by
$$H = R \frac{dR}{dt}. $$