"The ratio of the number of atoms in different energy states at thermal equilibrium can be calculated using the Boltzmann distribution law. The formula is:
N2/N1 = e-(E2-E1)/kT
where:
N2 and N1 are the number of atoms in the 5s and 3p states respectively,
E2 and E1 are the energies of the 5s and 3p states respectively,
k is the Boltzmann constant (8.6173 x 10-5 eV/K),
T is the temperature in Kelvin.
Substituting the given values:
N5s/N3p = e-(20.66 eV - 18.7 eV)/(8.6173 x 10-5 eV/K x 300 K)
N5s/N3p = e-1.96/0.02595
N5s/N3p = e-75.53
This ratio is extremely small, essentially zero for all practical purposes. Therefore, at 300 K, virtually all of the neon atoms will be in the 3p state, and almost none will be in the 5s state."
Found in less than 30 seconds using ck12.org/flexi (free access) :)