Two fundamental empirical laws have been established in the analysis o
f galaxy space distribution. First, recent analyses have revealed that
the three-dimensional distribution of galaxies and clusters is charac
terized by large-scale structures and huge voids: such a distribution
shows fractal correlations up to the limits of the available samples.
This has confirmed the earlier de Vaucouleurs power-law density - dist
ance relation, now corresponding to a fractal structure with dimension
D approximate to 2, at least, in the range of scales similar to 1 div
ided by 200 Mpc (H-0 = 55 km/sec/Mpc). An eventual cut-off towards hom
ogenization has not been yet identified. Second, since Hubble's discov
ery, the linear redshift-distance law has been well established within
200 Mpc and also much deeper. The co-existence of these laws within t
he same scales is a challenge for the standard cosmology, where the li
near Hubble law is a strict consequence of homogeneity of the expandin
g universe. This puzzle is now sufficiently strong to raise doubts for
the standard cosmology.