Periodic Reporting for period 1 - FAAST (Facilitating Autonomy in Astrodynamics for Spacecraft Technology)
Periodo di rendicontazione: 2023-07-16 al 2025-07-15
An important bottleneck in the current state-of-the-art for spaceflight is that the onboard computational capabilities in spacecraft are still quite limited, due to the need for radiation-hardened onboard computers to survive the harsh deep space environment. As a result, deep-space spacecraft must still be cautiously controlled remotely from the ground by teams of engineers, using dedicated deep-space communications infrastructure of limited capacity. Thus, despite the falling cost-to-orbit and the advancement of space technology, operation costs stemming from such activities remain stubbornly high. To propel a scalable future for space exploration, there is a strong need for autonomous capability that can operate with limited computational resources and at a level of safety and reliability worthy for use on invaluable spacecraft.
The main goal of FAAST is to develop robust and computationally efficient algorithms for autonomous orbit guidance and control for low-cost space vehicles which must plan and re-plan their trajectories in an uncertain environment. This is achieved by the following four objectives:
1. Develop and validate a new approach that facilitates computationally feasible onboard techniques.
2. Ensure that the new formulation can be applied to the highly uncertain space environment.
3. Apply the new implementation to develop an algorithm for autonomous orbit guidance in a relevant test problem. A successful algorithm should be computationally lean and robust, facilitating on-board planning and re-planning.
4. High-fidelity testing of the algorithm and study of high-fidelity modeling of the space environment.
The second year focused mainly on generalization of the monomial method, its applications in a range of onboard optimization problems of relevance in astrodynamics and spaceflight, and the improvement of the method leveraging techniques for reducing the complexity of the representation of a given optimization problem without compromising solution accuracy. Also performed in the end of the first and much of the second year were high-fidelity studies of the dynamics at work in binary asteroid systems, which are popular targets for deep space spacecraft. In this capacity the project interfaced with the ERC TRACES project and made use of software developed in the GRAINS MSCA project (Grant IDs 101077758 and 800060, respectively).
Overall the work resulted in 3 journal articles (1 published, 2 submitted), 5 conference works, and 3 software prototypes (one related to dynamical modeling and two related to spacecraft guidance).