  This contribution is the affirmative side of a debate held with Dr. L.
Pietronero at Princeton in June, 1996. I present the observational evidence
that the fractal behavior which characterizes the small scale galaxy
distribution does not continue to arbitarily large scale, but has a well
defined cutoff with an outer length scale of order 30h$^{-1}$ Mpc. For example,
plots of the IRAS 1.2 Jy survey exhibit a very clear approach to homogeneity on
large scale, in complete contradiction to the endless fractal model.
