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Question #43513

Difficulty: 8/10 | 🟢 Free

The Question

A spherically symmetric planet of radius RR has a non-uniform mass density given by ρ(r)=ρ0Rr\rho(r) = \frac{\rho_0 R}{r} for r≤Rr \le R, where ρ0\rho_0 is a positive constant and rr is the radial distance from the center. A satellite of mass mm is in a circular orbit around this planet at a radial distance of r=2Rr = 2R. A particle, also of mass mm, is projected from the center of the planet (r=0r=0) through a narrow, smooth radial tunnel. If the particle's speed when it reaches r=2Rr = 2R is exactly equal to the orbital speed of the satellite, what is the required projection speed v0v_0 at the center? (Assume no other celestial bodies are present and GG is the universal gravitational constant).

Options

  • A.

    R7πGρ0R \sqrt{7 \pi G \rho_0}

  • B.

    R5πGρ0R \sqrt{5 \pi G \rho_0}

  • C.

    R6πGρ0R \sqrt{6 \pi G \rho_0}

  • D.

    R103πGρ0R \sqrt{\frac{10}{3} \pi G \rho_0}

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Correct Answer

Step-by-Step Solution

Explanation

How the Examiner Thinks

Variable_Constraint

Develop pure symbolic logic skills by mastering algebraic constraints without relying on numerical data.

Concepts Behind This Question

Orbital Velocity Energy Balance|Electric Field Symmetry|Integration

Why This Question Is Tricky

Common Mistakes

This question tests the student's ability to derive gravitational potential from a non-uniform density distribution using Gauss's Law for gravitation, rather than blindly applying standard uniform-sphere formulas.

A common trap is calculating the correct total mass but incorrectly using the uniform solid sphere potential formula V(r)=−GM2R3(3R2−r2)V(r) = -\frac{GM}{2R^3}(3R^2 - r^2) for the interior, which leads to an incorrect potential difference (Option B).

Additionally, students might forget to account for the final kinetic energy required to match the satellite's orbital velocity, confusing the scenario with a simple escape velocity or maximum height problem (Option C).

Quick Facts About This Question

Question Information

SubjectPhysics
ChapterGravitation - Class 11 Part 1
ConceptOrbital Velocity Energy Balance
Difficulty8
Cognitive Load7
Target Solve Time160 sec
AccessFree