The escape velocity is given by the formula: \[ v_{escape} = \sqrt{\frac{2GM}{R}} \]
Step 2: Given Mass and Radius RelationshipsWe are given the following mass and radius relationships: \[ \frac{M_{planet}}{M_{earth}} = \frac{1}{8}, \quad \frac{R_{planet}}{R_{earth}} = \frac{1}{2} \]
Step 3: Calculate the Ratio of Escape VelocitiesThe ratio of the escape velocities is: \[ \frac{v_{escape, planet}}{v_{escape, earth}} = \sqrt{\frac{M_{planet} R_{earth}}{M_{earth} R_{planet}}} = \frac{1}{2} \]
Step 4: Calculate the Escape Velocity from the PlanetTherefore, the escape velocity from the planet is: \[ v_{escape, planet} = \frac{1}{2} \times 11.2 = 5.6 \, \text{km/s} \]
Final Answer: \[ v_{escape, planet} = 5.6 \, \text{km/s} \]Which one of the following graphs accurately represents the plot of partial pressure of CS₂ vs its mole fraction in a mixture of acetone and CS₂ at constant temperature?
