To solve this problem, we will use the concept of the photoelectric effect and the associated equations.
The photoelectric effect is described by the equation:
K.E. = h\nu - \phiwhere:
Given data:
First, calculate the work function \phi using the threshold wavelength:
\phi = \frac{hc}{\lambda_0} = \frac{4.14 \times 10^{-15} \cdot 3 \times 10^{8}}{3250 \times 10^{-10}} \phi = \frac{12.42 \times 10^{-7}}{3250 \times 10^{-10}} = 3.821 \ \text{eV}Now, calculate the energy of the incident ultraviolet light:
E_{\text{incident}} = \frac{hc}{\lambda} = \frac{4.14 \times 10^{-15} \cdot 3 \times 10^{8}}{2536 \times 10^{-10}} E_{\text{incident}} = \frac{12.42 \times 10^{-7}}{2536 \times 10^{-10}} = 4.898 \ \text{eV}The kinetic energy of the ejected electron is:
K.E. = E_{\text{incident}} - \phi = 4.898 \ \text{eV} - 3.821 \ \text{eV} = 1.077 \ \text{eV}Convert this kinetic energy to joules (1 eV = 1.6 \times 10^{-19} \ \text{J}):
K.E. = 1.077 \times 1.6 \times 10^{-19} \ \text{J} = 1.7232 \times 10^{-19} \ \text{J}The kinetic energy is also related to velocity by the equation K.E. = \frac{1}{2}mv^2, where m is the mass of the electron (9.11 \times 10^{-31} \ \text{kg}).
Thus, solving for the velocity:
v = \sqrt{\frac{2 \cdot \text{K.E.}}{m}} = \sqrt{\frac{2 \cdot 1.7232 \times 10^{-19}}{9.11 \times 10^{-31}}} v = \sqrt{\frac{3.4464 \times 10^{-19}}{9.11 \times 10^{-31}}} = \sqrt{3.784 \times 10^{11}} v \approx 6.15 \times 10^{5} \ \text{ms}^{-1}Therefore, the velocity of the electron ejected from the silver surface is approximately 6 \times 10^{5} \ \text{ms}^{-1} or 0.6 \times 10^{6} \ \text{ms}^{-1}, which matches the given option ≃ 6 \times 10^5 \ \text{ms}^{-1} or ≃ 0.6 \times 10^6 \ \text{ms}^{-1}.