If you know calculus, you may quickly derive the most common equations of motion.
Suppose we have a constant acceleration a, an initial velocity vi, and an initial position xi. Denote the final velocity and final position as vf and xf respectively, and let ti and tf be the initial and final time, respectively.
From calculus, we know:
dtdv=a
Integrating,
dv=a⋅dt
∫titfdv=∫titfa⋅dt
[v]titf=[at]titf
vf−vi=a(tf−ti)
If we let the change in time equal t, then we get the familiar equation:
vf=vi+at
Now, we may apply the same process to solve for the position:
dtdx=v
dx=v⋅dt
∫titfdx=∫titfv⋅dt
∫titfdx=∫titf(vi+a(t−ti))⋅dt
[x]titf=[vit+21a(t−ti)2]titf
xf−xi=vi(tf−ti)+21a(tf−ti)2+0
If we let the change in time equal t, then we get the familiar equation:
xf=xi+vit+21at2
Now, let us evaluate this integral:
∫vivf2v⋅dv
A simple integration yields the result vf2−vi2.
On the other hand, we could evaluate this integral by substituting t as our variable instead of v.
Our new integral is:
∫titf2v(a⋅dt)
Clearly 2a is a constant, so we may move it out from the integral:
2a∫titfv⋅dt
But that integral is simply the displacement, xf−xi! Let us call this x.
Then, equating the two expressions:
vf2−vi2=2ax
This is our familiar time-excluding kinematics equation. Keep it in mind if you are not given time, but you are given much of the other information.