As temperature increases, atoms move faster, resulting in higher frequencies and shorter wavelengths of emitted radiation, but intensity does not simply correlate with a greater percentage of atoms emitting at these higher frequencies. Intensity refers to the total energy radiated across all wavelengths, which is proportional to the fourth power of temperature, as described by Stefan-Boltzmann's law. The peak wavelength of emission shifts to shorter wavelengths as temperature rises, illustrating that black bodies emit all wavelengths but have a maximum at a specific temperature. For example, heating an object changes its color from red to blue, indicating a shift in peak wavelength. Understanding these principles clarifies how temperature affects radiation intensity and frequency distribution.