
From the figure, the peak hemispherical emissivity occurs at: \[ \lambda_m = 6000\ \text{\AA} \] Convert the wavelength into micrometers:
Since \(1\ \text{\AA} = 10^{-10}\ \text{m}\), \[ 6000\ \text{\AA} = 6000 \times 10^{-10}\ \text{m} = 6 \times 10^{-7}\ \text{m} = 0.6\ \mu\text{m} \] Using Wien's law: \[ \lambda_m T = 2898\ \mu\text{mK} \] \[ T = \frac{2898}{0.6} = 4830\ \text{K} \] Thus, rounding to the nearest integer, \[ T \approx 4830\ \text{K} \] So, the temperature at which total hemispherical emissivity is highest is \(4830\) K.