Step 1: The escape velocity \( v_e \) is the minimum velocity required for an object to escape the gravitational pull of the planet.
The formula for escape velocity is: \[ v_e = \sqrt{\frac{2GM}{R}} \] where: - \( G \) is the gravitational constant,
- \( M \) is the mass of the planet,
- \( R \) is the radius of the planet.
Step 2: The escape velocity does not depend on the mass of the object being thrown, but depends on the mass \( M \) and radius \( R \) of the planet. Thus, the correct answer is that escape velocity depends on the mass, density, and radius of the planet.
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: