In Classical mechanics (that is, when the velocities involved are significantly less than the speed of light) the average velocity of an object moving a distance d during a time interval t is described by the simple formula:
v = d/t.
Acceleration is the change of an object's velocity over time. It is defined as:
a = (vf - vi)/t
The final velocity of an object after accelerating at acceleration a for a period of time t is:
vf = vi + at
The average velocity of an accelerating object is (vf + vi)/2. To find the displacement of an accelerating objuect during a time interval, substitute this expression into the first formula to get:
d = t(vf + vi)/2
When only the object's initial velocity is known, the expression
d = vit + (at2)/2
can be used. The basic equations for final velocity and displacement can be combined to form an equation that is independent of time:
vf2 = vi2 + 2ad
These simple equations become more complicated as velocities approach the speed of light, where the effects of general relativity starts to become significant.