Physics Circle home Student Login

Home›Chapters›Heat Transfer and Radiation PYQs›Thermal Radiation: Black Body, Stefan & Wien›Question 10

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)

Q10MHT CET 2026 · 20 APR · SHIFT 2Easy

Thermal Radiation: Black Body, Stefan & Wien

Two stars A and B radiate maximum energy at wavelength 3.9×10−73.9 \times 10^{-7} m and 5.2×10−75.2 \times 10^{-7} m respectively. The ratio of the temperature of star A to that of star B will be

Show answer and solution

Answer: (d)

  1. Wien's law: λmT=b\lambda_m T = b, so T∝1λmT \propto \dfrac{1}{\lambda_m}.
  2. TATB=λBλA=5.2×10−73.9×10−7=43\dfrac{T_A}{T_B} = \dfrac{\lambda_B}{\lambda_A} = \dfrac{5.2 \times 10^{-7}}{3.9 \times 10^{-7}} = \dfrac{4}{3}
  3. So the answer is (d) 4:34 : 3.
Report a mistake

More questions on Thermal Radiation: Black Body, Stefan & Wien