The preparation of quantum system and the execution of quantum information tasks between distant users are always affected by gravitational and relativistic effects. In this work, we quantitatively analyze how the curved space-time background of the Earth affect the classical and quantum correlations of photon pairs, which are initially prepared in a two-mode squeezed state. More specifically, considering the rotation of the Earth, the space-time around the Earth is described by Kerr metric. Our results show that these state correlations, which initially increase for a specific range of satellite's orbital altitude, will gradually approach a finite value with increasing height of satellite's orbit (when the special relativistic effect is involved). More importantly, our analysis demonstrates that, the changes of correlations generated by the total gravitational frequency shift could reach the level of < 0.5%, within the satellite height at geostationary Earth orbits.