Step 1: In the Bohr model the orbital frequency scales as \(f_n = \dfrac{f_1}{n^3}\), since \(v_n = v_1/n\) and \(r_n = n^2 r_1\), giving \(f_n = \dfrac{v_n}{2\pi r_n} = \dfrac{f_1}{n^3}\).
Step 2: For the ground state, \(v_1 = 2.19\times10^{6}\ \text{m/s}\) and \(r_1 = 0.529\times10^{-10}\ \text{m}\), so
\[f_1 = \frac{v_1}{2\pi r_1} = \frac{2.19\times10^{6}}{2\pi(0.529\times10^{-10})} \approx 6.59\times10^{15}\ \text{Hz}\]
Step 3: For \(n = 2\):
\[f_2 = \frac{f_1}{2^3} = \frac{6.59\times10^{15}}{8} \approx 8.24\times10^{14}\ \text{Hz}\]
Step 4: The number of revolutions in the lifetime \(\tau = 10^{-8}\ \text{s}\) is
\[N = f_2\,\tau = (8.24\times10^{14})(10^{-8}) \approx 8.2\times10^{6}\]
Step 5: Therefore
\[\boxed{N \approx 8.2\times10^{6}}\]