Step 1: Use the photoelectric equation
The photoelectric effect is described by the equation:
\[
E_{\text{photon}} = W + E_{\text{kinetic}}
\]
where:
- \( E_{\text{photon}} \) is the energy of the incident photon,
- \( W \) is the work function of the metal,
- \( E_{\text{kinetic}} \) is the kinetic energy of the emitted photoelectron.
The energy of a photon is given by the equation:
\[
E_{\text{photon}} = \frac{hc}{\lambda}
\]
where:
- \( h \) is Planck’s constant (\( h = 6.626 \times 10^{-34} \, \text{J} \cdot \text{s} \)),
- \( c \) is the speed of light (\( c = 3.0 \times 10^8 \, \text{m/s} \)),
- \( \lambda \) is the wavelength of the light.
The work function \( W \) is given as 1.0 eV, which we need to convert into joules:
\[
W = 1.0 \, \text{eV} = 1.0 \times 1.602 \times 10^{-19} \, \text{J} = 1.602 \times 10^{-19} \, \text{J}
\]
Step 2: Calculate the energy of the incident photon
The wavelength of the ultraviolet light is \( \lambda = 99 \, \text{nm} = 99 \times 10^{-9} \, \text{m} \). Using the formula for photon energy:
\[
E_{\text{photon}} = \frac{(6.626 \times 10^{-34} \, \text{J} \cdot \text{s})(3.0 \times 10^8 \, \text{m/s})}{99 \times 10^{-9} \, \text{m}}
\]
Simplifying:
\[
E_{\text{photon}} = \frac{1.9878 \times 10^{-25}}{99 \times 10^{-9}} = 2.01 \times 10^{-18} \, \text{J}
\]
Step 3: Find the kinetic energy of the emitted photoelectron
From the photoelectric equation:
\[
E_{\text{kinetic}} = E_{\text{photon}} - W
\]
Substituting the values:
\[
E_{\text{kinetic}} = 2.01 \times 10^{-18} \, \text{J} - 1.602 \times 10^{-19} \, \text{J} = 1.85 \times 10^{-18} \, \text{J}
\]
Step 4: Calculate the wavelength of the fastest photoelectron
The kinetic energy of the photoelectron is related to its momentum by:
\[
E_{\text{kinetic}} = \frac{p^2}{2m}
\]
where \( p \) is the momentum of the photoelectron and \( m \) is the mass of the electron (\( m = 9.1 \times 10^{-31} \, \text{kg} \)).
Solving for \( p \):
\[
p = \sqrt{2mE_{\text{kinetic}}}
\]
Substituting the values:
\[
p = \sqrt{2(9.1 \times 10^{-31} \, \text{kg})(1.85 \times 10^{-18} \, \text{J})}
\]
\[
p = \sqrt{3.37 \times 10^{-48}} = 5.81 \times 10^{-24} \, \text{kg} \cdot \text{m/s}
\]
The wavelength \( \lambda_{\text{electron}} \) of the fastest photoelectron is related to its momentum by the de Broglie relation:
\[
\lambda_{\text{electron}} = \frac{h}{p}
\]
Substituting the values:
\[
\lambda_{\text{electron}} = \frac{6.626 \times 10^{-34}}{5.81 \times 10^{-24}} = 1.14 \times 10^{-10} \, \text{m} = 0.114 \, \text{nm}
\]
Final Answer:
The wavelength of the fastest photoelectron emitted is \( \boxed{0.114 \, \text{nm}} \).