Are the small neutrino oscillation parameters all related?

Neutrino oscillations reveal several small parameters, namely, ${\theta }_{13}$, the solar mass splitting {\em vis-`{a}-vis} the atmospheric one, and the deviation of ${\theta }_{23}$ from maximal mixing. Can these small quantities all be traced to a single source and, if so, how could that be tested? Here a see-saw model for neutrino masses is presented wherein a dominant term generates the atmospheric mass splitting with maximal mixing in this sector, keeping ${\theta }_{13}=0$ and zero solar splitting. A Type-I see-saw perturbative contribution results in non-zero values of ${\theta }_{13}$, $\Delta m^2_{solar}$,$\theta_{12}$,aswellasallows$\theta_{23}$todeviatefrom$\pi/4$ in consistency with the data while interrelating them all. CP-violation is a natural consequence and is large ($\delta \sim \pi \mathrm{/}2,3\pi \mathrm{/}2$) for inverted mass ordering. The model will be tested as precision on the neutrino parameters is sharpened.