Step 1: Understanding the Concept:
A hot sphere in a cooler surrounding loses heat by radiation. By Stefan-Boltzmann law the net rate of heat loss is proportional to \(T^4 - T_0^4\), where \(T_0\) is the temperature of the surroundings.
Step 2: Set up the ratio:
Initial: \(R \propto 600^4 - 200^4\). Later: \(R' \propto 400^4 - 200^4\).
Take 200 as a common unit: \(600 = 3\), \(400 = 2\), \(200 = 1\).
Step 3: Compute:
\[ \frac{R'}{R} = \frac{2^4 - 1^4}{3^4 - 1^4} = \frac{16 - 1}{81 - 1} = \frac{15}{80} = \frac{3}{16} \]
Step 4: Why the other options are wrong.
\(\frac{16}{3}R\) and \(\frac{16}{9}R\) are larger than \(R\), but cooling slows as the sphere gets closer to the surrounding temperature. \(\frac{9}{16}R\) comes from taking \(\frac{3^2}{4^2}\), which is not the Stefan law.
Final Answer:
The new cooling rate is \(\frac{3}{16}R\), option (D).
\[ \boxed{\frac{3}{16}R} \]