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Question #42274

Difficulty: 8/10 | 🟢 Free

The Question

A planet of initial mass m0m_0 is in a circular orbit of radius r0r_0 and period T0T_0 around a star of mass MM (M≫m0M \gg m_0). It moves through a uniform cosmic dust cloud, accreting dust at a constant rate dmdt=α\frac{dm}{dt} = \alpha. The dust is initially at rest relative to the star. Additionally, the cloud exerts a viscous drag force on the planet given by F⃗d=−βv⃗\vec{F}_d = -\beta \vec{v}, where v⃗\vec{v} is the planet's velocity and β\beta is a positive constant. Assuming the orbit remains quasi-circular, what is the orbital period TT of the planet when its mass reaches 2m02m_0?

Options

  • A.

    T02−3(1+β/α)T_0 2^{-3(1 + \beta/\alpha)}

  • B.

    T02−3(β/α)T_0 2^{-3(\beta/\alpha)}

  • C.

    T02−3(1+β/2α)T_0 2^{-3(1 + \beta/2\alpha)}

  • D.

    T02−32(1+β/α)T_0 2^{-\frac{3}{2}(1 + \beta/\alpha)}

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Correct Answer

Step-by-Step Solution

Explanation

How the Examiner Thinks

Multi-Concept_Bridge

Master problems that require linking physics and math concepts to solve complex competitive questions.

Concepts Behind This Question

Kepler’s Third Law (Time Period)|Viscosity and Stokes' Law|Integration

Why This Question Is Tricky

Common Mistakes

This question tests the application of Newton's Second Law and angular momentum in variable mass systems.

A common trap for JEE Advanced students is incorrectly assuming F⃗net=ma⃗\vec{F}_{net} = m\vec{a} applies to variable mass, leading to an incorrect torque equation dL⃗dt=α−βmL⃗\frac{d\vec{L}}{dt} = \frac{\alpha-\beta}{m}\vec{L}.

The correct fundamental law is F⃗net=dp⃗dt\vec{F}_{net} = \frac{d\vec{p}}{dt}.

Furthermore, students often forget that the accreted dust, being initially at rest, contributes zero momentum but increases the mass, effectively acting as an additional drag force (accretion drag).

Integrating the correct angular momentum decay with Kepler's Third Law for a shrinking quasi-circular orbit yields the true orbital period.

Quick Facts About This Question

Question Information

SubjectPhysics
ChapterGravitation - Class 11 Part 1
ConceptKepler’s Third Law (Time Period)
Difficulty8
Cognitive Load7
Target Solve Time160 sec
AccessFree