This work explores the possibility of performing in-orbit particle collection for sampling and exploration missions towards asteroids. Ejecta is generated via a small kinetic impactor and two possible collection strategies are investigated: collecting the particle at the L2 Lagrangian point or collecting them while the orbit the asteroid and before they re-impact. Combining the dynamics of the particles in the Circular Restricted Three-Body Problem with realistic models for the ejecta generation, we evaluate the feasibility of the mission concept and characterised possible target asteroids given their physical properties.

Ejecta Dynamics Around Asteroids in View of In-Orbit Particle Collection Missions

Trisolini, M.;Colombo, C.;
2021-01-01

Abstract

This work explores the possibility of performing in-orbit particle collection for sampling and exploration missions towards asteroids. Ejecta is generated via a small kinetic impactor and two possible collection strategies are investigated: collecting the particle at the L2 Lagrangian point or collecting them while the orbit the asteroid and before they re-impact. Combining the dynamics of the particles in the Circular Restricted Three-Body Problem with realistic models for the ejecta generation, we evaluate the feasibility of the mission concept and characterised possible target asteroids given their physical properties.
2021
72nd International Astronautical Congress (IAC 2021)
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Utilizza questo identificativo per citare o creare un link a questo documento: https://hdl.handle.net/11311/1189549
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