Photogravimagnetic assists of light sails: a mixed blessing for Breakthrough Starshot?

• Published in: arXiv.org
• Main Authors: gan, Duncan H, Heller, René, Hippke, Michael
• Format: Paper Journal Article
• Language: English
• Published: Ithaca Cornell University Library, arXiv.org 30.10.2017
• Subjects: Charging; Deceleration; Ejection; Lorentz force; Magnetic fields; Magnetism; Physics - Instrumentation and Methods for Astrophysics; Physics - Solar and Stellar Astrophysics; Radiation pressure; Red dwarf stars; Sails; Stellar magnetic fields; Trajectories
• ISSN: 2331-8422
• DOI: 10.48550/arxiv.1711.05856

Upon entering a star system, light sails are subject to both gravitational forces and radiation pressure, and can use both in concert to modify their trajectory. Moreover, stars possess significant magnetic fields, and if the sail is in any way charged, it will feel the Lorentz force also. We investigate the dynamics of so-called "photogravimagnetic assists" of sailcraft around \(\alpha\) Centauri A, a potential first destination en route to Proxima Centauri (the goal of the Breakthrough Starshot program). We find that a 10m\(^2\) sail with a charge-to-mass-ratio of around 10 \(\mu\)C/g or higher will need to take account of magnetic field effects during orbital maneouvres. The magnetic field can provide an extra source of deceleration and deflection, and allow capture onto closer orbits around a target star. However, flipping the sign of the sailcraft's charge can radically change resulting trajectories, resulting in complex loop-de-loops around magnetic field lines and essentially random ejection from the star system. Even on well-behaved trajectories, the field can generate off-axis deflections at \(\alpha\) Centauri that, while minor, can result in very poor targetting of the final destination (Proxima) post-assist. Fortunately for Breakthrough Starshot, nanosails are less prone to charging en route than their heavier counterparts, but can still accrue relatively high charge at both the origin and destination, when travelling at low speeds. Photogravimagnetic assists are highly non-trivial, and require careful course correction to mitigate against unwanted changes in trajectory.