Fabry-Perot images of the HH 47 optical jet show that the velocity dec
reases from the center toward the edges which is interpreted as eviden
ce for entrainment. Those images can be used to investigate the rate o
f entrainment required to account for the observed luminosity. Entrain
ment along the jet can account for only small fractions of the jet mas
s and the molecular outflow seen in CO. We compare the density, excita
tion, and velocity structure of the jet with the predictions of viscou
s entrainment models and models of entrainment by expulsion of jet mat
erial by internal shocks, and find that either type of model can expla
in the general features of the observations.