It has been suggested that if the Universe satisfies a flat, multiply conne
cted, perturbed Friedmann-Lemaitre model, then cosmic microwave background
data from the COBE satellite implies that the minimum size of the injectivi
ty diameter (shortest closed spatial geodesic) must be larger than about a
of the horizon diameter. To show that this claim is misleading, a simple T-
2 X R universe model of injectivity diameter a quarter of this size, i.e. a
tenth of the horizon diameter, is shown to be consistent with COBE four-ye
ar observational maps of the cosmic microwave background. This is done usin
g the identified circles principle.