Escape velocity (\( v_e \)) is given by the formula: \[ v_e = \sqrt{2 g R} \] where \( g \) is the acceleration due to gravity and \( R \) is the radius of the planet.
For the given planet: \[ g_{{planet}} = 2.5 g_{{Earth}}, \quad R_{{planet}} = 10 R_{{Earth}} \] Now, computing the escape velocity ratio: \[ \frac{v_{e,{planet}}}{v_{e,{Earth}}} = \sqrt{\frac{2.5 g_{{Earth}} \times 10 R_{{Earth}}}{2 g_{{Earth}} R_{{Earth}}}} \] \[ = \sqrt{\frac{25}{5}} = \sqrt{5} \approx 5 \] Thus, the ratio of escape velocity on the planet to that on Earth is 5:1.
For the reaction:
\[ 2A + B \rightarrow 2C + D \]
The following kinetic data were obtained for three different experiments performed at the same temperature:
\[ \begin{array}{|c|c|c|c|} \hline \text{Experiment} & [A]_0 \, (\text{M}) & [B]_0 \, (\text{M}) & \text{Initial rate} \, (\text{M/s}) \\ \hline I & 0.10 & 0.10 & 0.10 \\ II & 0.20 & 0.10 & 0.40 \\ III & 0.20 & 0.20 & 0.40 \\ \hline \end{array} \]
The total order and order in [B] for the reaction are respectively: