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tokens: ACKNOWLEDGEMENTS We have used NASA’s ADS Bibliographic Services. Most of the computations that made possible this work were performed with NASA NAIF SPICE Software (Acton 1996 and Jon D. Giorgini), Python 2.7 , and their related tools and libraries, iPython (Pérez Granger 2007 ), Matplotlib (Hunter et al. 2007 ), scipy , and numpy (Van Der Walt, Colbert Varoquaux 2011 ). Special thanks to the reviewers that through their criticism significantly contributed to improve the paper. In particular, we thank Steve Chesley for his in-depth initial review of this work; his comments and observations contributed to improve significantly the quality of the manuscript with respect to its initial versions. We appreciate the assistance of Jon D. Giorgini, senior analyst of the JPL Solar system Dynamics Group. We also thank Professor Ignacio Ferrin and Professor David Asher for useful comments and insightful discussions about this topic. We also thank the organizers of Meteoroid 2016 conference for allowing us to present the initial versions of this work to the meteor and asteroid scientific community. This work is supported by Vicerrectoria de Docencia-UdeA and the Estrategia de Sostenibilidad 2014-2015 de la Universidad de Antioquia . MS is supported by Colciencias, Doctorado Nacional - 647 programme. We thank Universidad Pontificia Bolivariana (UPB-Medellin) and DELL for allowing us to run most of our simulations in their data centres.