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Heat And Thermodynamics

MHT CET 2026 18th April Evening Shift

MCQ+1 / -02026
A black body radiates maximum energy at wavelength '$\lambda$' at temperature $T_1$ and its emissive power is E. When the temperature of the body is changed to $T_2$, it radiates maximum energy at wavelength $\dfrac{2\lambda}{3}$, then the emissive power will become

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