Optimization of asteroid capture missions using Earth resonant encounters

dc.contributor.authorNeves, Rita
dc.contributor.authorSanchez, Joan-Pau
dc.date.accessioned2018-10-31T11:34:11Z
dc.date.available2018-10-31T11:34:11Z
dc.date.issued2018-02-11
dc.description.abstractThis paper describes a robust methodology to design Earth-resonant asteroid capture trajectories leading to Libration Point Orbits (LPOs). These trajectories consider two impulsive manoeuvres; one occurring before the first Earth encounter and a final one that inserts the asteroid into a stable hyperbolic manifold trajectory leading to an LPO of the Sun-Earth system. The first manoeuvre is key to exploit the chaotic perturbative effects of the Earth and obtain important reductions on the cost of inserting the asteroid into a manifold trajectory. The perturbative effects caused by the Earth are here modelled by means of a Keplerian Map approximation, and these are a posteriori compared with the dynamics of the Circular Restricted Three-Body Problem. Savings in the order of 50% of total Δv are computed for four different asteroids.en_UK
dc.identifier.citationRita Neves, and Joan Pau Sánchez. Optimization of asteroid capture missions using Earth resonant encounters. In: Vasile M., Minisci E., Summerer L., McGinty P. (eds) Stardust Final Conference on Asteroids and Space Debris, Volume 52, 2018en_UK
dc.identifier.isbn978-3-319-69955-4
dc.identifier.issn1570-6591
dc.identifier.urihttps://doi.org/10.1007/978-3-319-69956-1_1
dc.identifier.urihttps://dspace.lib.cranfield.ac.uk/handle/1826/13597
dc.language.isoenen_UK
dc.publisherSpringeren_UK
dc.rightsAttribution-NonCommercial 4.0 International*
dc.rights.urihttp://creativecommons.org/licenses/by-nc/4.0/*
dc.titleOptimization of asteroid capture missions using Earth resonant encountersen_UK
dc.typeConference paperen_UK

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