It seems that the kinematic equations can all be derived from some simple definitions.
We’ll begin with our symbols:
= position (or distance)
= initial velocity
= final velocity
= acceleration
= time (or duration)
We have the definitions:
so
so
Now, for our purposes, we will regard and
as constant, and
as a function
of
.
Since is constant, we have (abusing notation a little)
Thus we have our first kinematic equation:
[1]
We will now integrate this (w.r.t. ):
so .
Using the boundary condition if
, we have
.
Thus we have our second kinematic equation:
[2]
Now, if we substitute [1] into [2] at , we obtain
and so we have our third kinematic equation (one not normally given)
[3]
If we substitute [1] into [2] differently, at , we obtain
so
and so we have our fourth kinematic equation
[4]
Finally, substituting [4] into [1] at t, we have
so
and so we have our fifth kinematic equation
[5]
To review what we have:
[1] or [¬s]: ; an equation without
[2] or [¬v]: ; an equation without
[3] or [¬u]: ; an equation without
[4] or [¬a]: ; an equation without
[5] or [¬t]: ; an equation without
(See also my post on parabolic trajectories.)