We report on the discovery of the He II Raman line lambda 485.1 nm in
the spectrum of the planetary nebula NGC 7027. This line is direct evi
dence for the presence of atomic hydrogen in the nebula. It is shown t
hat this Raman line can provide reliable pieces of information concern
ing both the velocity field of the He2+ region and the expansion veloc
ity of the surrounding H-0 shell. Detection of self-Raman scattering o
f Ly(gamma) is suspected.