Direct low-energy trajectories to Near-Earth Objects

TL;DR

This paper introduces a novel trajectory design method for low-energy transfers from Earth to Near-Earth Objects using invariant manifolds in the circular restricted three-body problem, enabling cost-effective space missions.

Contribution

The work develops a new trajectory design approach leveraging invariant structures in the CR3BP to connect Earth and NEOs efficiently, improving upon traditional mission planning techniques.

Findings

Trajectory paths follow hyperbolic invariant manifolds.

Method reduces transfer energy and time compared to conventional methods.

Applicable to various departure points near Earth or libration points.

Abstract

Near-Earth Objects (NEOs) are asteroids, comets and meteoroids in heliocentric orbits with perihelion below 1.3 au. Similarly to the population of the Main Asteroid Belt, NEOs are primordial bodies and their study can improve our understanding of the origins of the Solar System. With a catalog of over 30~000 known asteroids and approximately 100 listed short-period comets, the NEO population represents an inventory of exploration targets reachable with significantly lower cost than the objects of the Main Asteroid Belt. In addition, the materials present in these bodies could be used to resupply spacecraft en route to other destinations. The trajectories of past missions to NEOs have been designed with the patched-conics technique supplemented by impulsive and/or low-thrust maneuvers and planetary gravity assist. The transfer times range from some months to a few years, and the close-approach speeds relative to the target have been as high as 10 km/s. The design technique described in this work leverages the invariant structures of the circular restricted three-body problem (CR3BP) to connect the vicinity of the Earth with NEOs in low-eccentricity, low-inclination orbits. The fundamental building blocks are periodic orbits around the collinear points L$_1$ and L$_2$ of the Sun-Earth CR3BP. These orbits are used to generate paths that follow the associated hyperbolic invariant manifolds, exit the sphere of influence of the Earth and reach NEOs on nearby orbits. The strategy is simple, can be applied to depart either a libration point orbit or the vicinity of the Earth, and offers attractive performance features.