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MHT CET 2026 (20 Apr, Shift 2) · Thermal Radiation: Black Body, Stefan & Wien

Thermal Radiation: Black Body, Stefan & Wien question from MHT CET 2026 (20 Apr, Shift 2)

Q27MHT CET 2026 · 20 APR · SHIFT 2Medium

Thermal Radiation: Black Body, Stefan & Wien

A black body is at temperature of 5780 K. The energy of radiation emitted by the body at wavelength 300 nm is U1U_1, at wavelength 500 nm is U2U_2 and that at 900 nm is U3U_3 respectively. Wien's constant b=2.89×106b = 2.89 \times 10^{6} nmK. This shows that

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Answer: (c)

  1. Wien's law: λm=bT=2.89×1065780=500 nm\lambda_m = \frac{b}{T} = \frac{2.89 \times 10^6}{5780} = 500\text{ nm}.
  2. Energy is maximum at 500 nm and falls on either side.
  3. So U2U_2 is the largest: U1<U2>U3U_1 < U_2 > U_3, answer (c).
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