Although FNO has long been considered a computationally challenging mo
lecule, no thorough study of this species has been performed with meth
ods of electron correlation beyond second-order Moller-Plesset perturb
ation theory (MP2) and the singles and doubles configuration interacti
on (CISD) method. We have investigated the equilibrium structure, vibr
ational spectra, and relative energetics of FNO using high-levels of a
b initio theory. Methods include third and fourth-order Moller-Plesset
perturbation (MP3 and MP4), singles and doubles coupled-cluster (CCSD
) theory, and the CCSD(T) method, which incorporates a perturbational
estimate of the effects of connected triple excitations. The quadratic
configuration interaction method including single, double, and triple
excitations [QCISD(T)] method is also used. Computations using these
methods are performed with medium and large basis sets. Geometries cal
culated at the Hartree-Fock level are grossly in error, while going to
the CISD, MP3, MP4, and CCSD methods produces increasingly better res
ults. The CCSD(T) and QCISD(T) methods yield quite accurate structures
; surprisingly, the MP2 results are almost as good. The quality of the
calculated relative energetics closely follows that of the structure
predictions, except that the MP2 level of theory now performs slightly
worse than MP3, MP4, and CCSD methods.