Answer:
Option D
Explanation:
Photoemission will stop when the potential on silver sphere becomes equal to the stopping potential.
$\therefore$ $\frac{hc}{\lambda}-W=eV_{0}$
Here, $V_{0}=\frac{1}{4 \pi \epsilon_{0}} \frac{ne}{r}$
$\therefore$ $\left(\frac{1240}{1200}eV\right)-(4.7 eV)=\frac{9\times10^{9}\times n \times1.6 \times10^{-19}}{10^{-2}}$
$(6.2-4.7)=\frac{9\times10^{9}\times n \times1.6 \times10^{-19}}{10^{-2}}$
or $n=\frac{1.5\times10^{-2}}{9\times 1.6\times10^{-10}}=1.04\times10^{7}$
$\therefore$ Answer is 7