Equations of motion

The first two equations of motion are

vav=ΔdΔt(𝟏) and aav=ΔvΔt(𝟐).

If we substitute Δx=x2x1 for Δd and Δv, we get

d2=d1+vavΔt(𝟑) and v2=v1+aavΔt(𝟒).

If we take Δd=vavΔt and substitute the average of two velocities (initial and final) for vav, we get

Δd=v1+v22Δt(𝟓).

We can substitute equation (4) into this, yielding

Δd=v1+(v1+aavΔt)2Δt=2v1+aavΔt2Δt,

which simplifies to

Δd=v1Δt+12aav(Δt)2(𝟔).

If we rearrange equation (4) to isolate v1 and then substitute that into equation (5), we get

Δd=v2Δt12aav(Δt)2(𝟕).

We can derive one final equation, this time eliminating the one variable that has been present in all the others: time. We begin by rearranging equation (4) to isolate Δt, and then we substitute that into equation (5), giving us

Δd=(v1+v22)(v2v1aav).

By multiplying the denominators to the other side and recognizing the difference of squares, we get

2aavΔd=v22v12,

which we can rearrange to get our final equation,

v22=v12+2aavΔd(𝟖).

There might be a few more equations that we could have derived, but these eight (and rearranged versions of them) should take you a long way.