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Question #42320
The Question
A non-uniform spherical planet of mass and radius has a radially dependent density profile , where is the distance from the center. A small payload of mass () is initially at rest at the exact center of the planet. The payload is then launched to infinity through a narrow radial shaft. Simultaneously, the planet undergoes a structural collapse under its own gravity, settling into a uniform sphere of radius . What is the total change in the gravitational potential energy of the system (planet + payload)?
Options
- A.
- B.
- C.
- D.
Check Your Answer
Correct Answer
Step-by-Step Solution
Explanation
How the Examiner Thinks
Intuition_Breaker
Train your brain to resist "obvious" answers that are designed to deceive your intuition.
Concepts Behind This Question
Potential Energy Reference|Gravitational Self-Energy|Center of Mass (COM) Frame
Why This Question Is Tricky
Common Mistakes
This question tests the rigorous definition of gravitational potential and self-energy for non-uniform mass distributions.
A common trap is assuming the potential at the center of a non-uniform body follows the uniform sphere formula () or simply using the surface potential ().
Furthermore, students often forget that the self-energy of the system is a dynamic quantity that changes during structural collapse.
By requiring the calculation of both the non-uniform self-energy integral and the internal potential field, the problem forces students to abandon point-mass approximations and evaluate the energy state relative to the object's own constituent parts.
Quick Facts About This Question
Question Information
| Subject | Physics |
| Chapter | Work, Energy, and Power - Class 11 Part 1 |
| Concept | Potential Energy Reference |
| Difficulty | 8 |
| Cognitive Load | 7 |
| Target Solve Time | 160 sec |
| Access | Free |