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.