Two spheres ‘S1’ and ‘S2’ have same radii but temperatures are ‘T1’ and ‘T2’ respectively. Their emissive power is same and emissivity is in the ratio 1 : 4. Then the ratio ‘T1’ to‘T2’ is
The emissive power can be represented by the Stefan-Boltzmann law:
E = σ * ε * T4
Given that the emissive power is the same for both spheres S1 and S2, and the emissivity ratio is 1:4, we can write:
E1 = E2
σ * ε1 * T14 = σ * ε2 * T24
ε1 * T14 = ε2 * T24
Since the ratio of emissivity (ε1 : ε2) is given as 1:4, we can substitute ε1 = x and ε2 = 4x, where x is a constant:
x * T14 = 4x * T24
Dividing both sides by x, we get:
T14 = 4T24
\(\frac {T_1^4}{T_2^4}\) = 4
Taking the fourth root of both sides, we have:
T1 = √2 * T2
Therefore, the ratio of T1 to T2 is (C) √2 : 1.
Given:
Emissive power \(E = \sigma \epsilon T^4\)
Emissivity ratio \(\epsilon_1 : \epsilon_2 = 1 : 4\)
Since the emissive power E is the same for both spheres:
\(\sigma \epsilon_1 T_1^4 = \sigma \epsilon_2 T_2^4\)
Canceling \(\sigma\) from both sides (since it's common):
\(\epsilon_1 T_1^4 = \epsilon_2 T_2^4\)
Given \(\epsilon_1 = x\) and \(\epsilon_2 = 4x\) (where x is a constant):
\(x T_1^4 = 4x T_2^4\)
Divide both sides by x:
\(T_1^4 = 4 T_2^4\)
Taking the fourth root of both sides:
\(T_1 = \sqrt[4]{4} \cdot T_2\)
\(T_1 = \sqrt{2} \cdot T_2\)
\(\frac{T_1}{T_2}=\) \(\frac{\sqrt{2}}{1}\)
So, the correct option is (C): \(\sqrt{2}:1\)
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