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Question #43513
The Question
A spherically symmetric planet of radius has a non-uniform mass density given by for , where is a positive constant and is the radial distance from the center. A satellite of mass is in a circular orbit around this planet at a radial distance of . A particle, also of mass , is projected from the center of the planet () through a narrow, smooth radial tunnel. If the particle's speed when it reaches is exactly equal to the orbital speed of the satellite, what is the required projection speed at the center? (Assume no other celestial bodies are present and is the universal gravitational constant).
Options
- A.
- B.
- C.
- D.
Check Your Answer
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 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
| Subject | Physics |
| Chapter | Gravitation - Class 11 Part 1 |
| Concept | Orbital Velocity Energy Balance |
| Difficulty | 8 |
| Cognitive Load | 7 |
| Target Solve Time | 160 sec |
| Access | Free |