Equations of motion

The first two equations of motion are

v→av=Δd→Δt(𝟏) and a→av=Δv→Δt(𝟐).

If we substitute Δx=x2−x1 for Δd→ and Δv→, we get

d→2=d→1+v→avΔt(𝟑) and v→2=v→1+a→avΔt(𝟒).

If we take Δd→=v→avΔt and substitute the average of two velocities (initial and final) for v→av, we get

Δd→=v→1+v→22Δt(𝟓).

We can substitute equation (4) into this, yielding

Δd→=v→1+(v→1+a→avΔt)2Δt=2v→1+a→avΔt2Δt,

which simplifies to

Δd→=v→1Δt+12a→av(Δt)2(𝟔).

If we rearrange equation (4) to isolate v→1 and then substitute that into equation (5), we get

Δd→=v→2Δt−12a→av(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→=(v→1+v→22)(v→2−v→1a→av).

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

2a→avΔd→=v→22−v→12,

which we can rearrange to get our final equation,

v→22=v→12+2a→avΔd→(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.