In an external environment of temperature (\(T\)) kelvin, a sphere at temperature (\(3T\)) kelvin has cooling rate \(R_1\). When the temperature of that sphere falls to (\(2T\)) kelvin, the cooling rate \(R_2\) of the sphere will become
Show Hint
Radiation rate \(\propto T^4-T_0^4\) for a body in surroundings at \(T_0\).