The time taken for a ball to fall from a height $h$ under gravity is determined using the equation of motion $h = \frac{1}{2}gt^2$, where $g$ is the acceleration due to gravity and $t$ is the time.
- On Earth: Let the acceleration due to gravity be $g_{\text{earth}}$, the mass of Earth be $M$, and the radius of Earth be $R$. The time to fall height $h$ is $t$. Using the equation:
\[
\begin{align}
h = \frac{1}{2} g_{\text{earth}} t^2 \implies t^2 = \frac{2h}{g_{\text{earth}}} \implies t = \sqrt{\frac{2h}{g_{\text{earth}}}}
\]
- On the other planet: The planet has mass $M' = 100M$ and radius $R' = 10R$. The acceleration due to gravity $g$ is given by $g = \frac{GM}{R^2}$, where $G$ is the gravitational constant. For the planet:
\[
\begin{align}
g_{\text{planet}} = \frac{G M'}{(R')^2} = \frac{G (100M)}{(10R)^2} = \frac{100 G M}{100 R^2} = \frac{G M}{R^2} = g_{\text{earth}}
\]
The acceleration due to gravity on the planet is the same as on Earth, $g_{\text{planet}} = g_{\text{earth}}$. Now, calculate the time $t'$ to fall the same height $h$ on the planet:
\[
\begin{align}
h = \frac{1}{2} g_{\text{planet}} (t')^2 \implies (t')^2 = \frac{2h}{g_{\text{planet}}} = \frac{2h}{g_{\text{earth}}} \implies t' = \sqrt{\frac{2h}{g_{\text{earth}}}} = t
\]
Since $g_{\text{planet}} = g_{\text{earth}}$, the time $t'$ is equal to $t$. Thus, the time to fall the same height $h$ on the planet is $t$, which matches option (1).
Thus, the correct answer is (1).