The role of the nucleon resonances (N*) in omega photoproduction is investi
gated by using the resonance parameters predicted by Capstick and Roberts [
Phys. Rev. D 46, 2864 (1992): 49, 4570 (1994)]. In contrast with the previo
us investigations based on the SU(6)xO(3) limit of the constituent quark mo
del, the employed N*-->gammaN and N*-->omegaN amplitudes include the config
uration mixing effects due to the residual quark-quark interactions. The co
ntributions from the nucleon resonances are found to be significant relativ
e to the nonresonant amplitudes in changing the differential cross sections
at large scattering angles and various spin observables. In particular, we
suggest that a crucial test of our predictions can be made by measuring th
e parity asymmetry and beam-target double asymmetry at forward scattering a
ngles. The dominant contributions are found to be from N3/2(divided by)(191
0), a missing resonance, and N3/2(-)(1960) which is identified as the D-13(
2080) of the Particle Data Group.