  Modified gravity models have been constantly proposed with the purpose of
evading some standard gravity shortcomings. Recently proposed by A.H.
Chamseddine and V. Mukhanov, the Mimetic Gravity arises as an optimistic
alternative. Our purpose in this work is to derive Tolman-Oppenheimer-Volkoff
equations and solutions for such a gravity theory. We solve them numerically
for quark star and neutron star cases. The results are carefully discussed.
