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Comparison of Escape Velocities for Spherical Planets of Equal Density

Consider two spherical planets PP and QQ having uniform density ρ\rho, with masses MpM_p and MqM_q, and surface areas AA and 4A4A, respectively. Another spherical planet RR also possesses a uniform density ρ\rho, and its mass is equal to (Mp+Mq)(M_p + M_q). If the escape velocities from planets PP, QQ, and RR are VpV_p, VqV_q, and VrV_r, respectively, then:

Options

A

VQ>VR>VPV_Q > V_R > V_P

B

VR>VQ>VPV_R > V_Q > V_P

Correct
C

VR/VP=3V_R / V_P = 3

D

VP/VQ=12V_P / V_Q = \frac{1}{2}

Correct

Topics & Concepts

Step-by-Step Solution

To determine the correct options, we analyze the relationship between the surface area, mass, radius, density, and escape velocity for each spherical planet.

1. Determination of Radii

The surface area of a spherical planet of radius RR is given by: A=4πR2A = 4\pi R^2

For planets PP and QQ:

  • Surface area of planet PP: AP=A  ⟹  4πRP2=A  ⟹  RP=A4πA_P = A \implies 4\pi R_P^2 = A \implies R_P = \sqrt{\frac{A}{4\pi}}
  • Surface area of planet QQ: AQ=4A  ⟹  4πRQ2=4A  ⟹  RQ=2RPA_Q = 4A \implies 4\pi R_Q^2 = 4A \implies R_Q = 2 R_P

Thus, the relation between the radii of planets PP and QQ is: RQ=2RPR_Q = 2 R_P


2. Determination of Masses

The mass MM of a uniform sphere of radius RR and density ρ\rho is given by: M=43πR3ρM = \frac{4}{3}\pi R^3 \rho

Since all planets have the same uniform density ρ\rho, the mass of each planet is proportional to the cube of its radius (M∝R3M \propto R^3):

  • Mass of planet PP: MP=43πRP3ρM_P = \frac{4}{3}\pi R_P^3 \rho
  • Mass of planet QQ: MQ=43πRQ3ρ=43π(2RP)3ρ=8MPM_Q = \frac{4}{3}\pi R_Q^3 \rho = \frac{4}{3}\pi (2 R_P)^3 \rho = 8 M_P

For planet RR, its mass is given as: MR=MP+MQ=MP+8MP=9MPM_R = M_P + M_Q = M_P + 8 M_P = 9 M_P

Since MR=43πRR3ρ=9MPM_R = \frac{4}{3}\pi R_R^3 \rho = 9 M_P, we find the radius of planet RR: 43πRR3ρ=9(43πRP3ρ)  ⟹  RR3=9RP3  ⟹  RR=91/3RP\frac{4}{3}\pi R_R^3 \rho = 9 \left( \frac{4}{3}\pi R_P^3 \rho \right) \implies R_R^3 = 9 R_P^3 \implies R_R = 9^{1/3} R_P


3. Escape Velocity Derivation

The escape velocity VV from the surface of a spherical planet of mass MM, radius RR, and density ρ\rho is: V=2GMR=2G(43πR3ρ)R=8πGρ3⋅RV = \sqrt{\frac{2 GM}{R}} = \sqrt{\frac{2 G \left(\frac{4}{3}\pi R^3 \rho\right)}{R}} = \sqrt{\frac{8\pi G \rho}{3}} \cdot R

Since ρ\rho and GG are constant for all planets, the escape velocity is directly proportional to the radius of the planet (V∝RV \propto R): VP=8πGρ3RPV_P = \sqrt{\frac{8\pi G \rho}{3}} R_P VQ=8πGρ3RQ=2VPV_Q = \sqrt{\frac{8\pi G \rho}{3}} R_Q = 2 V_P VR=8πGρ3RR=91/3VPV_R = \sqrt{\frac{8\pi G \rho}{3}} R_R = 9^{1/3} V_P


4. Comparison of Escape Velocities

  • Ratio of VPV_P to VQV_Q: VPVQ=RPRQ=RP2RP=12\frac{V_P}{V_Q} = \frac{R_P}{R_Q} = \frac{R_P}{2 R_P} = \frac{1}{2} Therefore, Option (D) is correct.

  • Ratio of VRV_R to VPV_P: VRVP=RRRP=91/3≈2.08≠3\frac{V_R}{V_P} = \frac{R_R}{R_P} = 9^{1/3} \approx 2.08 \neq 3 Therefore, Option (C) is incorrect.

  • Ordering of Escape Velocities: Since 1<2<91/31 < 2 < 9^{1/3} (because 23=8<92^3 = 8 < 9), we have: RP<RQ<RR  ⟹  VP<VQ<VR  ⟹  VR>VQ>VPR_P < R_Q < R_R \implies V_P < V_Q < V_R \implies V_R > V_Q > V_P Therefore, Option (B) is correct.


Conclusion

The correct options are B and D.