  In the present paper, we report on a study of the anisotropic strange stars
under Finsler geometry. Keeping in mind that Finsler spacetime is not merely a
generalization of Riemannian geometry rather the main idea is the projectivized
tangent bundle of the manifold $\mathpzc{M}$, we have developed the respective
field equations. Thereafter, we consider the strange quark distribution inside
the stellar system followed by the MIT bag model equation of state (EOS). To
find out the stability and also the physical acceptability of the stellar
configuration, we perform in detail some basic physical tests of the proposed
model. The results of the testing show that the system is consistent with the
Tolman-Oppenheimer-Volkoff (TOV) equation, Herrera cracking concept, different
energy conditions and adiabatic index. One important result that we observe is
that the anisotropic stress reaches to the maximum at the surface of the
stellar configuration. We calculate (i) the maximum mass as well as
corresponding radius, (ii) the central density of the strange stars for finite
values of bag constant $B_g$ and (iii) the fractional binding energy of the
system. This study shows that Finsler geometry is especially suitable to
explain massive stellar systems.
