We report the results of the first statistical analysis of colours (B - V,
V - R, V - I, and V - J) of the Trans-Neptunian and Centaur populations. Us
ing the same statistical techniques applied to define the current asteroid
taxonomy, we find a continuous spread of the objects between neutral colour
to very red. Pushing further the analysis, the TNOs may be split into four
groups. The differences in colour content are interpreted as a consequence
of the TNOs evolution (i.e. collisional history, space weathering, ...)