11.2 eV
Step 1: Use the photoelectric equation: \( K_{{max}} = E - \phi \), where \(K_{{max}}\) is the maximum kinetic energy of the ejected electrons, \(E\) is the energy of the incident photons, and \(\phi\) is the work function.
Step 2: The maximum kinetic energy can also be expressed as \( K_{{max}} = e \cdot V \), where \(V\) is the stopping potential and \(e\) is the elementary charge.
Step 3: Setting \(e \cdot 6V = E - 5.2\) eV and solving for \(E\) gives \(E = 6 + 5.2 = 11.2\) eV.
Step 4: Therefore, the energy of the incident radiation is 11.2 eV.
Kepler's second law (law of areas) of planetary motion leads to law of conservation of
Kepler's second law (law of areas) of planetary motion leads to law of conservation of