Concept:
Blackbody radiation laws describe how objects emit radiation based on their temperature.
Step 1: Understanding the relationship.
The law that connects the
wavelength of maximum emission with temperature is:
\[
\lambda_{\max} T = \text{constant}
\]
Step 2: Identifying the law.
This relationship is given by
Wien’s Displacement Law.
Step 3: Eliminating incorrect options.
- Stefan-Boltzmann Law relates total energy to \(T^4\).
- Planck’s Law gives full radiation distribution.
- Kirchhoff’s Law relates emission and absorption.
Conclusion:
Thus, the correct answer is
Wien’s Displacement Law.