Low-energy capture of asteroids onto KAM tori
arXiv:1501.03193 · doi:10.2514/1.G000797
Abstract
We present a new method for engineering the artificial capture of asteroids. Based on theories of the chaos-assisted capture of natural satellites of the giant planets, we show how an unbound asteroid that passes close to a regular region of phase space can be easily moved onto the nearby KAM tori and essentially permanently captured with the Earth's Hill sphere without closing the zero velocity curves. The method has the advantages of a relatively low delta-v requirement and no need for control strategies. An illustration of the method is given for an example asteroid trajectory, demonstrating that it is a viable strategy for the final capture stage of asteroids in the Earth's neighbourhood.
arXiv comment13 pages, 3 figures, accepted by the Journal of Guidance, Control, and Dynamics
References in corpus (7)
- Formation of Kuiper-belt binaries through multiple chaotic scattering encounters with low-mass intruders
- Easily Retrievable Objects among the NEO Population
- Capturing Near Earth Objects
- Three-Body Capture of Irregular Satellites: Application to Jupiter
- Capture and escape in the elliptic restricted three-body problem
- A Symplectic Integrator for Hill's Equations
- Periodic orbits for 3 and 4 co-orbital bodies