Interplanetary transfers in N-body systems

Trajectories existing in the complex N-body dynamical frameworks (CR3BP, ER3BP, ER4BP, etc.) are investigated to develop novel and effective solutions for the autonomous exploration of the solar system.

These studies led to: (i) the topological characterization of stable low-energy capture trajectories and (ii) of the osculating orbital elements at capture, and (iii) the development of minimum-energy/-propellant low-thrust guidance strategies to adjust the parameters of the low-energy trajectories or transferring a spacecraft from a high-energy trajectory to a low-energy one.

These solutions have been developed to (iv) respond to the constraints of actual on-board systems and verified modelling their real behaviour and high-fidelity orbit propagators, with particular focus on nano-/micro-satellite missions, characterized by limited performance of the guidance, navigation, attitude control and power systems and (v) the extensive use of rideshare launch opportunities.