Speed of Body under Free Fall from Height
Theorem
Let an object $B$ be released above ground from a point near the Earth's surface and allowed to fall freely.
Let $B$ fall a distance $s$.
Then:
- $v = \sqrt {2 g s}$
where:
- $v$ is the speed of $B$ after having fallen a distance $s$
- $g$ is the Acceleration Due to Gravity at the height through which $B$ falls.
It is supposed that the distance $s$ is small enough that $g$ can be considered constant throughout.
Proof 1
From Body under Constant Acceleration: Velocity after Distance:
- $\mathbf v \cdot \mathbf v = \mathbf u \cdot \mathbf u + 2 \mathbf g \cdot \mathbf s$
All dot products are between pairs of parallel vectors.
Thus by Cosine Formula for Dot Product:
- $v^2 = u^2 + 2 g s$
Here the body falls from rest, so:
- $\mathbf u = \mathbf 0$
Thus:
- $v^2 = 2 g s$
and so:
- $v = \sqrt {2 g s}$
$\blacksquare$
Proof 2
From Acceleration is Second Derivative of Displacement with respect to Time:
- $\mathbf g = \dfrac {\d^2 \mathbf s} {\d t^2}$
Integrating with respect to $t$, and by definition of velocity:
- $\mathbf v = \dfrac {\d \mathbf s} {\d t} = \mathbf g t + \mathbf c_1$
When $t = 0$, we have that $\mathrm c_1$ is the initial velocity $\mathbf v_0$, and so:
- $\mathbf v = \dfrac {\d \mathbf s} {\d t} = \mathbf g t + \mathbf v_0$
Integrating with respect to $t$ again:
- $\mathbf s = \dfrac {\mathbf g t^2} 2 + \mathbf v_0 t + \mathbf c_2$
When $t = 0$, we have that $\mathrm c_2$ is the initial displacement $\mathbf s_0$, and so:
- $\mathbf s = \dfrac {\mathbf g t^2} 2 + \mathbf v_0 t + \mathbf s_0$
We have that $B$ is released at rest starting at $\mathbf s = \mathbf 0$.
Thus $\mathbf v_0 = \mathbf s_0 = \mathbf 0$ and so:
- $\mathbf s = \dfrac {\mathbf g t^2} 2$
- $\mathbf v = \mathbf g t$
By eliminating $t$ and taking the scalar quantities:
- $v = \sqrt {2 g s}$
$\blacksquare$
Proof 3
From the Principle of Conservation of Energy:
- $K + P = C$
where:
- $K$ is the kinetic energy of $B$
- $P$ is the potential energy of $B$
- $C$ is a constant.
Let the mass of $B$ be $m$.
From Kinetic Energy of Motion:
- $K = \dfrac {m v^2} 2$
where $v$ is the speed of $B$.
From Potential Energy of Position:
- $P = m g s$
where $s$ is the distance fallen by $B$.
Since $B$ falls from rest, its initial kinetic energy is zero.
Having fallen a distance $s$, $B$ has lost potential energy $m g s$.
Therefore:
- $\dfrac {m v^2} 2 = m g s$
from which the result follows by dividing both sides by $m$ and extracting the square root.
$\blacksquare$