Target selection for Near-Earth Asteroids in-orbit sample collection missions
arXiv:2212.09497 · doi:10.1016/j.actaastro.2022.12.012
Abstract
This work presents a mission concept for in-orbit particle collection for sampling and exploration missions towards Near-Earth asteroids. Ejecta is generated via a small kinetic impactor and two possible collection strategies are investigated: collecting the particle along the anti-solar direction, exploiting the dynamical features of the L Lagrangian point or collecting them while the spacecraft orbits the asteroid and before they re-impact onto the asteroid surface. Combining the dynamics of the particles in the Circular Restricted Three-Body Problem perturbed by Solar Radiation Pressure with models for the ejecta generation, we identify possible target asteroids as a function of their physical properties, by evaluating the potential for particle collection.
References in corpus (7)
- OSIRIS-REx: Sample Return from Asteroid (101955) Bennu
- Density of asteroids
- Ejecta Cloud from a Kinetic Impact on the Secondary of a Binary Asteroid: I. Mechanical Environment and Dynamic Model
- Ejecta cloud from the AIDA space project kinetic impact on the secondary of a binary asteroid: II. fates and evolutionary dependencies
- Physical properties of near-Earth asteroids with a low delta-: Survey of target candidates for the Hayabusa2 mission
- Predicting the vulnerability of spacecraft components: modelling debris impact effects through vulnerable-zones
- Ejecta cloud distributions for the statistical analysis of impact cratering events onto asteroids' surfaces: a sensitivity analysis