Step 1: Understand Stefan-Boltzmann Law.
The energy radiated per unit time (power) by a black body is given by the Stefan-Boltzmann Law: \(P = \sigma A T^4\) where \(\sigma\) is the Stefan-Boltzmann constant, A is the surface area, and T is the temperature.
Step 2: Calculate the surface areas. The surface area of a sphere is given by \(A = 4\pi r^2\). For the smaller body, \(r_1 = 0.2\) m. \(A_1 = 4\pi (0.2)^2 = 4\pi (0.04) = 0.16\pi\) m\(^2\) For the bigger body, \(r_2 = 0.8\) m. \(A_2 = 4\pi (0.8)^2 = 4\pi (0.64) = 2.56\pi\) m\(^2\)
Step 3: Calculate the radiated energies. For the smaller body, \(T_1 = 800\) K. \(E = P_1 = \sigma A_1 T_1^4 = \sigma (0.16\pi) (800)^4\) For the bigger body, \(T_2 = 400\) K. \(P_2 = \sigma A_2 T_2^4 = \sigma (2.56\pi) (400)^4\)
Step 4: Find the ratio of radiated energies. \(\frac{P_2}{P_1} = \frac{\sigma (2.56\pi) (400)^4}{\sigma (0.16\pi) (800)^4} = \frac{2.56}{0.16} \times \left(\frac{400}{800}\right)^4\) \(\frac{P_2}{P_1} = 16 \times \left(\frac{1}{2}\right)^4 = 16 \times \frac{1}{16} = 1\) So, \(P_2 = P_1 = E\).
Three conductors of same length having thermal conductivity \(k_1\), \(k_2\), and \(k_3\) are connected as shown in figure. Area of cross sections of 1st and 2nd conductor are same and for 3rd conductor it is double of the 1st conductor. The temperatures are given in the figure. In steady state condition, the value of θ is ________ °C. (Given: \(k_1\) = 60 Js⁻¹m⁻¹K⁻¹,\(k_2\) = 120 Js⁻¹m⁻¹K⁻¹, \(k_3\) = 135 Js⁻¹m⁻¹K⁻¹)