Lesson 2 of 15

Free Fall

Free Fall Under Gravity

Near Earth's surface, gravity accelerates every object downward at:

g=9.81 m/s2g = 9.81 \ \text{m/s}^2

For an object with initial downward velocity v0v_0, the distance fallen after time tt is:

h(t)=v0t+12gt2h(t) = v_0 t + \frac{1}{2}g t^2

The first term is the constant-velocity contribution. The second term is the quadratic acceleration term — it grows as t2t^2.

Examples

v0v_0 (m/s)tt (s)hh (m)
014.905
0219.62
5229.62
10374.145

Galileo's Insight

Galileo showed that the distance fallen from rest is proportional to t2t^2. Doubling the fall time quadruples the distance fallen. Mass does not appear — all objects fall at the same rate (ignoring air resistance).

Your Task

Implement fallHeight(v0, t) returning the distance fallen in metres.

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