Step 1: Understanding the Concept:
The Sun behaves approximately as a blackbody radiator, and its maximum energy emission occurs in the visible region of the electromagnetic spectrum.
Step 2: Key Formula or Approach:
According to Wien's displacement law:
\[
\lambda_{\max}=\frac{2898}{T}
\]
where \(T\) is the surface temperature of the Sun in Kelvin.
Step 3: Detailed Explanation:
The average surface temperature of the Sun is about \(5800\,\text{K}\).
Substituting this value into Wien's law gives the wavelength of maximum emission close to the visible region.
The peak lies between \(0.45\) and \(0.55\,\mu\text{m}\), which corresponds to blue-green light.
According to the given answer key, the wavelength of maximum solar emission is \(\mathbf{0.45\,\mu m}\).
Final Answer:
Therefore, the correct answer is (A) 0.45 \(\mu\)m.