Concept:
The photoelectric effect explains the emission of electrons from a metal surface when electromagnetic radiation of sufficiently high frequency falls on it.
According to Einstein’s photoelectric equation:
:contentReference[oaicite:0]{index=0}
where:
• \(K.E.\) = maximum kinetic energy of emitted photoelectron
• \(h\) = Planck’s constant
• \(\nu\) = frequency of incident radiation
• \(\phi\) = work function of metal
Step 1: Write all the given quantities clearly.
The given values are:
\[
\phi = 9.53 \times 10^{-19}\ \text{J}
\]
\[
\nu = 3.5 \times 10^{16}\ \text{Hz}
\]
\[
h = 6.62 \times 10^{-34}\ \text{Js}
\]
We are required to calculate the kinetic energy of the emitted photoelectron.
Step 2: Calculate the energy of the incident photon.
Using:
\[
E = h\nu
\]
Substituting the values:
\[
E = (6.62 \times 10^{-34})(3.5 \times 10^{16})
\]
Now multiply the numerical values:
\[
6.62 \times 3.5 = 23.17
\]
and combine the powers of ten:
\[
10^{-34} \times 10^{16} = 10^{-18}
\]
Therefore:
\[
E = 23.17 \times 10^{-18}\ \text{J}
\]
Rewriting in standard scientific notation:
\[
E = 2.317 \times 10^{-17}\ \text{J}
\]
Step 3: Apply Einstein’s photoelectric equation.
Using:
\[
K.E. = h\nu - \phi
\]
Substitute the calculated values:
\[
K.E. = 2.317 \times 10^{-17} - 9.53 \times 10^{-19}
\]
Convert both quantities to same power:
\[
9.53 \times 10^{-19}
=
0.0953 \times 10^{-17}
\]
Hence:
\[
K.E.
=
2.317 \times 10^{-17}
-
0.0953 \times 10^{-17}
\]
\[
K.E.
=
2.2217 \times 10^{-17}\ \text{J}
\]
Approximating:
\[
K.E. \approx 2.2 \times 10^{-17}\ \text{J}
\]
Step 4: Write the final answer.
Therefore, the kinetic energy of the emitted photoelectron is:
\[
\boxed{2.2 \times 10^{-17}\ \text{J}}
\]
Hence, the correct option is:
\[
\boxed{(C)}
\]