To solve this question, we need to understand the comparison of projectile motion on Earth and another planet. The key concept here is that the trajectory of a projectile depends on two parameters: the initial velocity and the gravitational acceleration where the projectile is fired.
Let us define the symbols:
The formula for the range R of a projectile is given by:
R = \frac{v^2 \sin(2\theta)}{g}
Since both projectiles follow identical trajectories, their ranges must be equal:
\frac{v_1^2 \sin(2\theta)}{g_1} = \frac{v_2^2 \sin(2\theta)}{g_2}
The terms \sin(2\theta) cancel out from both sides:
\frac{v_1^2}{g_1} = \frac{v_2^2}{g_2}
Rearranging for g_2 gives:
g_2 = \frac{v_2^2 \cdot g_1}{v_1^2}
Substituting the values:
g_2 = \frac{(3\, m/s)^2 \cdot 9.8\, m/s^2}{(5\, m/s)^2}
= \frac{9 \cdot 9.8}{25}
= \frac{88.2}{25}
= 3.528\, m/s^2
Therefore, the acceleration due to gravity on the other planet is approximately 3.5\, m/s^2.
The correct answer is 3.5.