derive, using the equations of motion, the formula for kinetic energy EK = 21mv2

Cambridge A-Level Physics 9702 – Gravitational Potential Energy and Kinetic Energy

Gravitational Potential Energy and Kinetic Energy

Learning Objective

Derive, using the equations of motion, the formula for kinetic energy $E_K = \frac{1}{2} m v^2$.

Key Concepts

  • Work–energy principle
  • Newton’s second law
  • Equations of motion for constant acceleration
  • Relationship between work done by gravity and change in kinetic energy

Derivation

Consider an object of mass $m$ moving vertically under the influence of gravity. Let upward be positive, so the weight is $-mg$.

  1. Start from Newton’s second law: $F = ma$. For gravity alone, $F = -mg$, therefore $$a = -g.$$
  2. Use the kinematic equation that relates velocity, displacement and acceleration for constant $a$: $$v^2 = u^2 + 2a s,$$ where $u$ is the initial velocity, $v$ the final velocity and $s$ the displacement.
  3. Multiply both sides by $m/2$: $$\frac{1}{2} m v^2 = \frac{1}{2} m u^2 + m a s.$$
  4. Recognise that $m a s = (ma)s = F s$, which is the definition of work done by a constant force over a displacement $s$. For gravity $F = -mg$, so the work done by gravity is $$W_{g}= (-mg)s = -mg s.$$
  5. Re‑arrange the previous equation: $$\frac{1}{2} m v^2 - \frac{1}{2} m u^2 = -mg s.$$ The left‑hand side is the change in kinetic energy $\Delta E_K$, and the right‑hand side is the work done by gravity $W_g$. This is the work–energy theorem: $$\Delta E_K = W_{g}.$$
  6. If the object starts from rest ($u=0$) and falls a distance $h$ (so $s = -h$), the equation becomes $$\frac{1}{2} m v^2 = mg h,$$ giving the familiar result $$v = \sqrt{2 g h}.$$ The expression $\frac{1}{2} m v^2$ is identified as the kinetic energy $E_K$ of the object.

Summary Table

Quantity Symbol Expression
Kinetic Energy $E_K$ $\displaystyle E_K = \frac{1}{2} m v^2$
Gravitational Potential Energy $E_P$ $\displaystyle E_P = m g h$
Work done by gravity $W_g$ $\displaystyle W_g = -mg s$
Suggested diagram: A mass $m$ falling a distance $h$ under gravity, showing initial velocity $u=0$, final velocity $v$, and the work done by the weight $mg$.

Practice Questions

  1. A 2.0 kg ball is dropped from rest from a height of 5.0 m. Calculate its kinetic energy just before it hits the ground. (Take $g = 9.8\ \text{m s}^{-2}$.)
  2. A 1500 kg car accelerates from 0 to 20 m s$^{-1}$ on a level road. Determine the change in its kinetic energy.
  3. Show that the work done by a constant horizontal force $F$ over a distance $d$ equals the increase in kinetic energy, using the same steps as in the derivation above.

Key Take‑aways

  • The kinetic energy of a body moving with speed $v$ is $E_K = \frac{1}{2} m v^2$.
  • The work–energy theorem links the work done by all forces to the change in kinetic energy.
  • Gravitational potential energy $E_P = m g h$ is converted into kinetic energy when an object falls, conserving the total mechanical energy (neglecting air resistance).