  We consider static cosmological solutions along with their stability
properties in the framework of a recently proposed theory of massive gravity.
We show that the modifcation introduced in the cosmological equations leads to
several new solutions, only sourced by a perfect fluid, generalizing the
Einstein Static Universe found in General Relativity. Using dynamical system
techniques and numerical analysis, we show that the found solutions can be
either neutrally stable or unstable against spatially homogeneous and isotropic
perturbations.
