  We construct a toy model for isothermal spheres in Horava gravity, which
includes Einstein's gravity if a parameter is appropriately chosen. The
equations for the isothermal spheres are derived from the partition function of
the gravitating particle system. We confirm that the Newtonian limit of the
system coincides with the model of the well-known isothermal sphere. The
stability of the isothermal sphere is found to be sensitive to the energy
density at the center of the sphere.
