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Question #43788

Difficulty: 8/10 | 🟢 Free

The Question

A spherical satellite of radius RR is in deep space where the ambient temperature is 0 K0 \text{ K}. Inside the satellite, a source contains a sample of He+He^+ ions. Exactly NN ions per second undergo an electronic transition from the first excited state to the ground state. All the emitted photon energy is completely absorbed by the satellite's interior. The satellite's outer surface has a latitude-dependent emissivity given by ϵ(θ)=ϵ0sin⁡2θ\epsilon(\theta) = \epsilon_0 \sin^2\theta, where θ\theta is the polar angle (0≤θ≤π0 \le \theta \le \pi) and ϵ0\epsilon_0 is a dimensionless constant. Assuming the satellite is highly thermally conductive so that its surface temperature TT is uniform, what is the steady-state temperature TT?

(Let E0E_0 be the ionization energy of a hydrogen atom in its ground state, and σ\sigma be the Stefan-Boltzmann constant.)

Options

  • A.

    (9NE08πR2σϵ0)14\left( \frac{9 N E_0}{8 \pi R^2 \sigma \epsilon_0} \right)^{\frac{1}{4}}

  • B.

    (3NE02πR2σϵ0)14\left( \frac{3 N E_0}{2 \pi R^2 \sigma \epsilon_0} \right)^{\frac{1}{4}}

  • C.

    (9NE032πR2σϵ0)14\left( \frac{9 N E_0}{32 \pi R^2 \sigma \epsilon_0} \right)^{\frac{1}{4}}

  • D.

    (3NE0π2R2σϵ0)14\left( \frac{3 N E_0}{\pi^2 R^2 \sigma \epsilon_0} \right)^{\frac{1}{4}}

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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

Energy Level Scaling|Stefan-Boltzmann Power Law|Emissivity and Absorptivity|Integration

Why This Question Is Tricky

Common Mistakes

This question tests the student's ability to bridge discrete quantum energy scaling with macroscopic continuous thermal radiation.

The primary trap lies in the calculation of the radiated power.

Students often incorrectly assume emissivity can be averaged linearly or forget the geometric weighting factor (sin⁡θ\sin\theta) in the differential area element dA=2πR2sin⁡θdθdA = 2\pi R^2 \sin\theta d\theta when integrating the Stefan-Boltzmann law over a spherical surface.

Furthermore, a secondary trap exists in the Bohr model scaling: students might forget the Z2Z^2 dependence for the He+He^+ ion, leading to an incorrect input power.

The problem demands rigorous application of surface integrals to non-uniform material properties in thermal equilibrium.

Quick Facts About This Question

Question Information

SubjectPhysics
ChapterAtoms - Class 12
ConceptEnergy Level Scaling
Difficulty8
Cognitive Load7
Target Solve Time160 sec
AccessFree