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Classical Mechanics

Acceleration

The vector rate of change of velocity with respect to time.

Governing formula a = dv/dt = d²r/dt²
SI unit m/s²

In depth

Acceleration occurs whenever an object speeds up, slows down (deceleration), or changes direction. Net force and acceleration are always collinear.

Examples in the real world

A dragster accelerating from 0 to 100 km/h in 1.5 seconds, or a planet accelerating toward the Sun in orbit.