MHT CET · Physics · Thermal Properties of Matter

A black body radiates maximum energy at wavelength ' \(\lambda\) ' and its emissive power is ' \(E\) '. Now due to a change in temperature of that body, it radiates maximum energy at wavelength \(\frac{\lambda}{3}\). At that temperature emissive power is

A \(16: 1\)
B \(256: 1\)
C \(81: 1\)
D \(128: 1\)

Verified Solution

Answer & Solution

Correct Answer

(C) \(81: 1\)

Step-by-step Solution

Detailed explanation

\(\therefore\) Emissive power of black body is, From Wien's Law:
\(
\begin{aligned}
\mathrm{E} & =\sigma \mathrm{T}^4 \\
\lambda & =\frac{\mathrm{b}}{\mathrm{T}} \\
\therefore \quad \mathrm{E} & =\frac{\sigma \mathrm{b}^4}{\lambda^4} \\
\therefore \quad \frac{\mathrm{E}_2}{\mathrm{E}_1} & =\frac{\lambda_1^4}{\lambda_2^4}=\frac{\lambda^4}{\left(\frac{\lambda}{3}\right)^4}=\frac{81}{1}
\end{aligned}
\)

Apply the relevant identity from the chapter and substitute the values established in the previous step, keeping the original constraint in view.

Use the simplified expression to isolate the unknown, then plug the result back into the question setup to confirm the working is internally consistent.

Cross-check against a boundary or limiting case. Both the dimensional balance and the qualitative behaviour at the extreme should agree with the candidate answer.

Combine the steps above to identify the correct option. The remaining choices each fail at least one of the consistency, dimensional, or boundary checks.

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