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MHT CET 2026 (19 May, Shift 1) · Thermal Radiation: Black Body, Stefan & Wien

Thermal Radiation: Black Body, Stefan & Wien question from MHT CET 2026 (19 May, Shift 1)

Q5MHT CET 2026 · 19 MAY · SHIFT 1Easy

Thermal Radiation: Black Body, Stefan & Wien

A perfectly black body radiates power at temperature T1T_1 K. If it is to radiate 16 times this power, its temperature should be increased by

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Answer: (d)

  1. Stefan's law: P∝T4P \propto T^4
  2. T2T1=161/4=2⇒T2=2T1\dfrac{T_2}{T_1} = 16^{1/4} = 2 \Rightarrow T_2 = 2T_1
  3. Increase =2T1−T1=T1= 2T_1 - T_1 = T_1
  4. So the answer is (d) (T1)(T_1) K.
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