Utilizing Deep Reinforcement Learning to Effect Autonomous Orbit Transfers and Intercepts Via Electromagnetic Propulsion

Utilizing Deep Reinforcement Learning to Effect Autonomous Orbit Transfers and Intercepts Via Electromagnetic Propulsion

Problem Utilizing Deep Reinforcement Learning to Effect Autonomous Results The growth in space-capable entities has caused a rapid rise in Orbit Transfers and Intercepts via Electromagnetic Propulsion ➢ Analysis the number of derelict satellites and space debris in orbit Gabriel Sutherland ([email protected]), Oregon State University, Corvallis, OR, USA ❖ The data suggests spacecraft highly capable of around Earth, which pose a significant navigation hazard. Frank Soboczenski ([email protected]), King’s College London, London, UK neutralizing/capturing small to intermediate debris Athanasios Vlontzos ([email protected]), Imperial College London, London, UK ❖ In simulations, spacecraft was able to capture and/or Objectives neutralize debris ranging in mass from 1g to 100g ❖ Satellites suffered damage in some Develop a system that is capable of autonomously neutralizing simulations multiple pieces of space debris in various orbits. Software & Simulations ❖ Simulations show that damaged segments of satellite were vaporized, which means Background that no additional debris was added to orbit ➢ Dangerous amounts of space debris in orbit, estimates vary ❖ Neural Network based on Deep Deterministic Policy ➢20,000+ tracked objects larger Gradient (DDPG) effective at low-thrust orbit transfers in than 10 cm diameter 2D Hohmann transfer problem ➢Est 500,000 objects larger ❖ Using ASTOS simulation software, mission-representative than 1 cm in diameter model of spacecraft and experimental propulsion system ➢Est 100 million objects ❖ Interfaced with DRL to train the Neural smaller than 1cm in diameter ➢ Orbital speeds of these objects Network with realistic data vary from 100+ kph to 28,100 kph ➢ Future Studies ➢ Spacecraft collisions due to space ❖ Train DDPG for 3 dimensional orbit transfer problems debris have been sparse so far Tracked spacecraft in Earth orbit. Generated using Celestia Software. Earth’s magnetic lines and Van Allen radiation belts. Generated using ❖ Incorporate European Space Agency’s Space Debris ➢1985 – US Anti-satellite missile destroys aging weather satellite. Celestia Software. Software Suite Decayed orbit resulted in minimal additional debris ❖ Collision and intercept probability analysis ➢1996 - French satellite damaged by debris from French rocket launched in 1980’s with DRAMA software ➢2007 - China destroyed a old weather satellite via a missile ❖ Train Neural Network for safe deorbit of ➢Added 3,000+ trackable debris to orbit debris using Oriundo model ➢2009 - derelict Russian satellite collided with and destroyed ❖ Manufacture CubeSat prototype Iridium communication satellite ❖ Multi-electrodynamic tether ➢Added 2,000+ trackable debris to orbit ❖ Onboard AI via next-gen VPU ➢ Kessler Syndrome remains an increased possibility ➢Cascade of debris collisions in orbit creating more debris in chaotic orbits ➢Would lead to many orbits becoming inaccessible due to debris Force vectors for a Lorentz Force propelled spacecraft in Earth’s geomagnetic field danger ➢ The Earth has a geomagnetic field surrounding it ➢Extends more than Applications 600,000km above the surface ➢ Deep Reinforcement Learning for Orbit Transfer Equivalence graph of the total intensity (unit: nT) ➢Produced by currents ➢ Useful for effecting intercepts between in Earth’s core primary spacecraft and target orbit ➢Interactions between Solar storms and the ➢ Highly efficient for low-thrust maneuvers Geomagnetic field ➢ Magnetic propulsion system cause it to expand or ➢ Propellant-less propulsion system could be Shrink used in future spacecraft design for long General design for Deep Reinforcement Learning architecture mission life Cross-section of Geomagnetic field. (NASA) Equivalence graph of the declination angle (unit: deg) Equivalence graph of the inclination angle (unit: deg) ➢ Provides potential for satellite ➢ Lorentz Force constellations in close formation Spacecraft Design ➢ Could be used for planetary orbit insertion ➢ Lifetime >6 months for deep space missions ➢ Orbit: 2,000km – 36,000km Onboard capabilities: ➢ Real-time Operating System Conclusions ➢ Lorentz equation describes the force exerted on a charged ➢ Autonomous target selection filter particle B by electrical field E and magnetic field v ➢ Capable of ignoring active spacecraft ➢ In materials, particles also generate forces described in Lorentz ➢ Carbon-fiber composite net sections Results indicate a system similar in design to that of equation ➢ Net deployment and actuation system spacecraft outlined in this study has the potential to ➢ Powered by Electroactive polymers (EAPs) ➢ Systems of equations involving conductive properties, ➢ Telemetry uplink/downlink drastically reduce amount of space debris and derelicts in specific heat, insolation, and density of a material must be Earth orbit, thus reducing the risk of a Kessler syndrome solved to accurately predict magnetic forces exerted on it Key Capabilities scenario happening. ➢ Electro-dynamic tethers exploit changes in earth’s magnetic ➢ Low-power onboard Neural Network for propulsion system control and target selection field across different orbital areas to generate electricity ➢ Radiation-resistant software ➢ Neural Networks have been shown to be effective for continuous Acknowledgements low-thrust orbit changes, and resilient to missed thrust events Anatomy of an Electroactive Polymer (EAP). These fibers contract 300% when a current is run through them at high voltage. Photo courtesy of Jet Propulsion ➢Oregon NASA Space Grant Consortium Rendering of current debris capture spacecraft design. Lab. ➢Valarie Dr. Nancy Squires, Oregon State University. .

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