Question

Difficulty: HardGravitational Field and Orbits

Planet PP has a mean uniform density that is twice that of Planet QQ, and a radius that is half that of Planet QQ. What is the ratio of the escape velocity at the surface of Planet PP to the escape velocity at the surface of Planet QQ?

  1. 12\frac{1}{\sqrt{2}}Answer
  2. B
    12\frac{1}{2}
  3. C
    11
  4. D
    2\sqrt{2}

Answer

12\frac{1}{\sqrt{2}}
The correct answer is derived by substituting the planet's mass in terms of radius and density (M=43πR3ρM = \frac{4}{3}\pi R^3 \rho) into the escape velocity equation ve=2GMRv_e = \sqrt{\frac{2GM}{R}}. Simplifying gives ve=R83πGρv_e = R\sqrt{\frac{8}{3}\pi G \rho}, which means escape velocity is proportional to RρR\sqrt{\rho}. Halving the radius and doubling the density yields a factor of 12×2=22=12\frac{1}{2} \times \sqrt{2} = \frac{\sqrt{2}}{2} = \frac{1}{\sqrt{2}}.

Step-by-Step Solution

1
Express the mass of a uniform spherical planet in terms of its radius RR and density ρ\rho.
M=43πR3ρM = \frac{4}{3}\pi R^3 \rho
Mass equals volume multiplied by mean density.
2
Substitute mass into the escape velocity formula ve=2GMRv_e = \sqrt{\frac{2GM}{R}}.
ve=2G(43πR3ρ)R=R83πGρv_e = \sqrt{\frac{2G \left(\frac{4}{3}\pi R^3 \rho\right)}{R}} = R\sqrt{\frac{8}{3}\pi G \rho}
This establishes the proportionality veRρv_e \propto R\sqrt{\rho}.
3
Set up the ratio of escape velocity for Planet PP to Planet QQ using RP=12RQR_P = \frac{1}{2}R_Q and ρP=2ρQ\rho_P = 2\rho_Q.
\frac{v_{e,P}}{v_{e,Q}} = \frac{R_P\sqrt{\rho_P}}{R_Q\sqrt{\rho_Q}} = \frac{\left(\frac{1}{2}R_Q\right)\sqrt{2\rho_Q}}{R_Q\sqrt{\rho_Q}} = \frac{1}{2}\sqrt{2} = \frac{1}{\sqrt{2}}
Evaluating the ratio of proportional quantities yields the final scale factor.

Key Concept

Dependence of Escape Velocity on Planet Density and Radius
Estimated Time:2m 0s
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