A black coloured solid sphere of radius R and mass M is inside a cavity with a vacuum inside. The walls of the cavity are maintained at temperature T0. The initial temperature of the sphere is 3T0. If the specific heat o
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Concept: Stefan-Boltzmann Law, Heat Capacity
Question
A black coloured solid sphere of radius R and mass M is inside a cavity with a vacuum inside. The walls of the cavity are maintained at temperature T0. The initial temperature of the sphere is 3T0. If the specific heat of the material of the sphere varies as α T^3 per unit mass with the temperature T of the sphere, where α is a constant, then the time taken for the sphere to cool down to temperature 2T0 will be (σ is Stefan Boltzmann constant)
(A) Mα 16π R^2σ ((3)/(2) )
(B) Mα 16π R^2σ ((16)/(3) )
(C) Mα 4π R^2σ ((3)/(2) )
(D) Mα 4π R^2σ ((16)/(3) )
(A) Mα 16π R^2σ ((3)/(2) )
(B) Mα 16π R^2σ ((16)/(3) )
(C) Mα 4π R^2σ ((3)/(2) )
(D) Mα 4π R^2σ ((16)/(3) )
Try it yourself first
Hint: Pehle, aap Stefan-Boltzmann Law use karke rate of heat loss ka expression likho, aur phir usko specific heat ke term mein temperature change se relate karo.
Step-by-step solution
- 1
Given parameters
Sphere radius , mass , initial temperature , final temperature , cavity temperature . Specific heat . Stefan-Boltzmann constant . - 2
Rate of heat loss
Rate of heat loss by radiation from a black body is given by Stefan-Boltzmann Law. - 3
Relate heat loss to temperature change
Heat lost by sphere . Equate this with radiation heat loss and integrate. - 4
Substitute values
Substitute and into the equation. - 5
Rearrange for integration
Separate variables and for integration. - 6
Integrate both sides
Integrate from to and from to . - 7
Solve the integral
Use substitution , so . - 8
Evaluate definite integral
Substitute limits and simplify to find . - 9
Final time $\tau$
Simplify the logarithmic terms.\tau = \frac{M\alpha}{16\pi R^2\sigma} \ln\left(\frac{81T_0^4 - T_0^4}{16T_0^4 - T_0^4}\right) = \frac{M\alpha}{16\pi R^2\sigma} \ln\left(\frac{80T_0^4}{15T_0^4}\right) = \frac{M\alpha}{16\pi R^2\sigm
Final answer
(b)
Remember: Stefan-Boltzmann law aur variable specific heat ke integration ko yaad rakho.
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Ek object ka temperature hai aur surrounding ka temperature hai. Agar object ka temperature double ho jaye, toh uski net rate of heat loss by radiation kaise change hogi, assuming constant hai aur ?
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