Step 1: Recall Kepler's area rule.
A planet sweeps out equal areas in equal times. So the areal velocity, the area swept per second, stays the same all along the orbit.
Step 2: Write the areal velocity.
The rate of sweeping area is \[ \frac{dA}{dt} = \frac{1}{2}\,r\,v, \] where $r$ is the distance from the Sun and $v$ is the speed at that point.
Step 3: Find where the speed is smallest.
Because the product $r\,v$ is fixed, the speed is least when the distance is greatest. So the minimum speed happens at the maximum distance.
Step 4: Put in the known values.
Use the maximum distance $r_{\max} = 4 \times 10^{12}$ m and the given areal velocity $4 \times 10^{16}$: \[ 4 \times 10^{16} = \frac{1}{2} \times (4 \times 10^{12}) \times v_{\min}. \]
Step 5: Solve for the minimum speed.
The right side is $2 \times 10^{12}\,v_{\min}$, so \[ v_{\min} = \frac{4 \times 10^{16}}{2 \times 10^{12}} = 2 \times 10^{4}. \]
Step 6: State the answer.
The slowest speed of the planet is found at the farthest point. \[ \boxed{2 \times 10^{4} \ \text{m s}^{-1}} \]