We present far-ultraviolet observations of IC 63, an emission/reflection nebula illuminated by the B0.5IV star γ Cassiopeia, located 1.3 pc from the nebula. Molecular hydrogen fluorescence was detected first in IC 63 by IU E and later at shorter wavelengths by ORF EU S. Here we present F ar U ltraviolet Spectroscopic Explorer (F U SE) observations towards three locations in the neb-ula, complem...