  In this work, we made an extensive study about the possible presence of
anisotropies in strange stars. To accomplish this task, we use three different
configurations for the strange matter: the unpaired matter, a two-flavor
super-conducting (2SC) strange matter, and a fully three-flavor
super-conducting strange matter (CFL). For each configuration, we calculate the
relevant quantities for the strange stars, such as the mass-radius relation,
the dimensionless tidal parameter, the moment of inertia, and the surface
curvature for different degrees of anisotropies. Whenever possible, we compare
our results with constraints found in the literature, especially focusing on
the existence of very massive pulsars (PSR J0952-0607), as well as very light
compact objects (HESS J1731-347).
