In this problem, we will model the effect of an atmosphere on Earth. Suppose that the Sun is a black body with temperature $T_1$ and radius $r_1$. The Earth is a sphere that is located at a distance $R$ from the Sun and has a radius $r_3$. The emissivity of the Earth is $\varepsilon_3$.
(1) If there is no atmosphere on Earth, determine the temperature of the Earth at equilibrium, $T_3$.
(2) Now, we consider the effects of an atmosphere. Model the atmosphere as a spherical shell of gas, with an emissivity $\varepsilon_2$ and outer radius $r_2>r_3$, surrounding the Earth. At thermal equilibrium, its absorptivity for both ultraviolet and infrared light is $\varepsilon_2$. The atmosphere transmits a fraction $t$ of ultraviolet light but is completely opaque to infrared. Assuming that the Sun emits ultraviolet light while the Earth emits and re-emits infrared, determine the temperature of the atmosphere $T_2$ and the Earth, $T_3$, at thermodynamic equilibrium. Assume that the atmosphere is a perfect thermal conductor such that all incident radiation is instantaneously evenly distributed across it.