We compute the leading non-analytic correction to the baryon mass in t
he combined limits m(pi) --> O, N-c --> infinity with m(pi)N(c) held f
ixed. We reproduce the results of Cohen and Broniowski using semiclass
ical methods rather than heavy-baryon chiral perturbation theory. The
calculation is organized to demonstrate: 1 the model independence of o
ur results; and 2 the crucial role played by (iso)rotations of the hed
gehog pion cloud surrounding the baryon. Our rotationally improved lar
ge-N-c calculation yields results that naturally interpolate between o
rdinary chiral perturbation theory on the one hand, and large-N-c phys
ics on the other.