To solve this problem, we need to understand that the nucleus and the atom transition from their first excited states to ground states and emit photons of wavelengths \( \lambda_{N} \) and \( \lambda_{A} \) respectively.
The energy of the photon emitted during the transition can be given by the formula:
E = \frac{hc}{\lambda}
where \( h \) is Planck's constant, \( c \) is the speed of light, and \( \lambda \) is the wavelength of the emitted photon.
For the nucleus transitioning from its first excited state:
E_N = \frac{hc}{\lambda_N}
For the atom transitioning from its first excited state:
E_A = \frac{hc}{\lambda_A}
In general, the energy levels of a nucleus are far higher than those of an atom because nuclear forces are much stronger than electromagnetic forces. This implies:
E_N \gg E_A
Thus, we can say:
\frac{1}{\lambda_N} \approx 10^{6} \times \frac{1}{\lambda_A}
Simplifying the above expression for the ratio of wavelengths, we get:
\frac{\lambda_N}{\lambda_A} \approx 10^{-6}
Therefore, the ratio \(\frac{\lambda_{N}}{\lambda_{A}}\) is closest to 10^{-6}.
This matches with option 10^{-6}, confirming this as the correct answer.