derive, using W = Fs, the formula ∆EP = mg∆h for gravitational potential energy changes in a uniform gravitational field

Gravitational Potential Energy & Kinetic Energy

What is Work?

Work is the energy transferred when a force acts over a distance.

The basic formula is \$W = F\,s\$ (force times displacement).

⚡️ Think of pushing a shopping cart: the harder you push (larger \$F\$) and the farther you push (larger \$s\$), the more work you do.

Exam Tip

When you see a question about potential energy change, remember to start from the work done by the force.

Write down \$W = F\,s\$ and then replace \$F\$ with the appropriate force (e.g., \$mg\$ for gravity).

This shortcut often saves time in the exam.

Uniform Gravitational Field

In a uniform field near Earth’s surface, the weight of an object is constant:

\$F = mg\$, where \$m\$ is mass and \$g \approx 9.81\,\text{m/s}^2\$.

Deriving ΔEP = mgΔh

  1. Choose the direction of displacement.

    Let the object move upward by a distance Δh. The displacement vector is \$s = \Delta h\$ (positive upward).

  2. Write the work done by gravity.

    Gravity acts downward, opposite to the upward displacement, so the work done by gravity is negative:

    \$W_{\text{gravity}} = -mg\,\Delta h\$.

  3. Relate work to potential energy change.

    By definition, the change in gravitational potential energy is the negative of the work done by gravity:

    \$ΔEP = -W{\text{gravity}}\$.

  4. Substitute.

    Plugging in the expression for \$W_{\text{gravity}}\$ gives:

    \$ΔE_P = -(-mg\,\Delta h) = mg\,\Delta h.\$

So, when an object rises by Δh in a uniform field, its gravitational potential energy increases by \$mgΔh\$.

If it falls, Δh is negative and the potential energy decreases accordingly.

Example Problem

A 5 kg box is lifted 3 m above the ground.


ΔEP = \$5\,\text{kg} \times 9.81\,\text{m/s}^2 \times 3\,\text{m} = 147.15\,\text{J}\$ (≈147 J).

The box now has 147 J more gravitational potential energy than before.

Kinetic Energy Reminder

Kinetic energy (KE) is the energy of motion:

\$KE = \tfrac{1}{2}mv^2\$.

When an object falls, its potential energy converts to kinetic energy (ignoring air resistance).

Energy conservation: \$ΔE_P + ΔKE = 0\$.

Exam Tip

For questions involving both potential and kinetic energy, write the energy conservation equation:

\$E{\text{initial}} = E{\text{final}}\$.

Then substitute \$E = KE + EP\$ and solve for the unknown quantity.

Summary Table

QuantityFormulaUnits
Work\$W = F\,s\$J
Gravitational Potential Energy Change\$ΔE_P = mg\,Δh\$J
Kinetic Energy\$KE = \tfrac{1}{2}mv^2\$J