You need: a metre stick (or any straight stick you measure), a tape measure, a sunny day (spring, summer or a clear winter day all work), a watch, and paper and pencil. Safety: never look directly at the Sun; look only at the shadow. On a summer day wear a hat and sunscreen and take breaks in the shade between readings.
- Stand the metre stick straight up on flat ground (a friend can hold it, or prop it with books). Measure its height h (1 m for a metre stick).
- Measure the shadow length L. Repeat every 30 minutes for two or three hours in the morning or afternoon.
- For each reading, the Sun's elevation angle θ satisfies tan θ = h/L. Compute θ = tan⁻¹(h/L) in degrees.
- The model is L = h cot θ = h cos θ/sin θ. Use the quotient rule to show dL/dθ = −h/sin² θ (θ in radians).
- For one of your angles, convert to the rate per degree by multiplying by π/180. Compare with how much your shadow actually changed between readings.
What to look for: with h = 1 m and θ = 40°, L ≈ 1.19 m and dL/dθ ≈ −1/sin² 40° ≈ −2.42 m per radian, or about −0.042 m (4.2 cm) shorter for each degree the Sun rises. Shadows change length fastest when the Sun is low (sin θ small), which is why evening shadows grow so quickly.