Correct answer: 110 km s⁻¹
The escape velocity is determined by the formula v = √(2GM/R), where G is the gravitational constant, M is the mass of the planet, and R is its radius. In this case, since the planet is 10 times more massive and has a radius that is 10 times smaller, the escape velocity increases by a factor of √(10/0.1) = √100 = 10, resulting in an escape velocity of 110 km s⁻¹.