This article gives the results of an analytical and numerical study of a two‐gyro, gravity‐oriented communications satellite. The principal purpose of the study was to uncover and solve the analytical problems arising in the design of passive gravity‐gradient altitude control systems. Although the study was directed at satellite orientation, it is felt that many of the techniques developed have general use in the investigation of dynamical systems.
We consider both small and large motions about the desired earth‐pointing orientation. In the small‐motion study, the goal is simultaneous optimization of the transient response and the forced response to perturbations caused by orbital eccentricity, magnetic torques, solar torques, thermal rod bending, and micrometeorite impact. In the large‐motion study, we enumerate all possible equilibrium positions of the satellite and then consider initial despin after injection into orbit, inversion of the satellite from one stable equilibrium position to another by switching of gyro bias torques, and the decay of transient motions resulting from large initial angular rates.
As a specific numerical example, we have treated a 300‐lb satellite in a 6000‐nm orbit, stabilized by a 60‐ft extensible rod with a 20‐lb tip mass, and by two single‐degree‐of‐freedmn gyros, each with an angular momentum of 106 cgs units. Without a detailed discussion of hardware, it is concluded that such a system, having a total weight of 50 to 75 pounds including power supply, will provide a settling time for small disturbances of less than one orbit and will hold the antenna pointing error within a few degrees.