Step 1: Recall the formula for gravitational acceleration.
At the surface of a planet, the acceleration due to gravity is:
\[
g = \frac{GM}{R^2}
\]
where $G$ is the gravitational constant, $M$ is the planet's mass, and $R$ is its radius.
Step 2: Write the ratio of gravitational accelerations.
For the new planet: $M' = 100M$ and $R' = 10R$.
\[
\frac{g'}{g} = \frac{M'/R'^2}{M/R^2} = \frac{100M / (10R)^2}{M/R^2} = \frac{100M}{100R^2} \cdot \frac{R^2}{M} = 1
\]
Step 3: Interpret the result.
Since $g' = g$, the gravitational pull at the surface of the new planet is exactly the same as on Earth.
Step 4: Use kinematics for the fall.
For a ball dropped from rest through height $h$:
\[
h = \frac{1}{2}g t^2
\]
Step 5: Compare times on both planets.
Since $h$ is the same and $g' = g$, the time to fall must also be the same:
\[
t' = t
\]
Step 6: State the answer.
The ball takes the same time $t$ seconds on the new planet.
\[
\boxed{t \text{ s}}
\]