  We calculate the strange star properties in the framework of the Field
Correlator Method. We find that for the values of the gluon condensate
$G_2=0.006\;{\rm GeV}^4$ and $G_2=0.0068\;{\rm GeV}^4$, which give a critical
temperature $T_c\sim170\;{\rm MeV}$ at $\mu_c=0$, the sequences of strange
stars are compatible with some of the semi-empirical mass-radius relations and
data obtained from astrophysical observations.
