Using the Stefan-Boltzmann Law: \[ P = \sigma A T^4 \] where \( P = 30 \, \text{kW} = 30 \times 10^3 \, \text{W} \), \( A \) is the surface area of the sphere, and \( T \) is the temperature. The surface area of a sphere is given by: \[ A = 4 \pi r^2 \] Substitute \( r = 0.03 \, \text{m} \): \[ A = 4 \pi (0.03)^2 \approx 0.0113 \, \text{m}^2 \] Now use the Stefan-Boltzmann equation to solve for \( T \): \[ 30 \times 10^3 = (5.67 \times 10^{-8}) \times 0.0113 \times T^4 \] Solving for \( T \): \[ T^4 \approx \frac{30 \times 10^3}{(5.67 \times 10^{-8}) \times 0.0113} \approx 4.6 \times 10^3 \] Thus, \( T \approx 4600 \, \text{K} \).
This question uses the Stefan-Boltzmann law for a small sphere acting as a perfect absorber and emitter. Rather than solving for temperature directly, each option can be checked by plugging it back into the law and comparing to the given 30 kW.
Testing each temperature against the actual formula shows the power radiated grows extremely fast with temperature, since it depends on the fourth power. Only 2600 K reproduces something close to the sphere's actual 30 kW.
So the correct answer is 2600 K.