  Is it actually possible to interpret gravitation as space's property in a
pure classical way. Then, we note that extended self-gravitating system
equilibrium depends directly on the number of dimension of the space in which
it evolves. Given those precisions, we review the principal thermodynamical
knowledge in the context of classical gravity with arbitrary dimension of
space. Stability analyses for bounded 3D systems, namely the Antonov
instability paradigm, are then rapproched to some amazing properties of
globular clusters and galaxies.
