  We present the possibility that the gravitational growth of primordial
density fluctuations leads to what can be considered a week version of the
cosmological principle. The large scale mass distribution associated with this
principle must have the geometrical structures known as a regular honeycombs.
We give the most important parameters that characterize the honeycombs
associated with the closed, open, and flat FLRW models. These parameters can be
used to determine by means of observations which is the appropriate honeycomb.
For each of these honeycombs, and for a nearly flat universe, we have
calculated the probability that a randomly placed observer could detect the
honeycomb as a function of the density parameters.
