Resumen: Asteroid 216-Kleopatra presents a ham-bone shape, that is to say, it is quite elongated body with two protuberances on its end-points, which makes of it the perfect candidate to model its shape and mass distribution by a Dipole-Segment, consisting on a massive segment with two spherical masses at the end-points of the rod and that is rotating about its center of mass with uniform velocity. Once obtained an approximation of the actual values of the involved parameters from recent results of Burov and coworkers, we obtain the complete map of families of symmetric periodic orbits, and describe the orbits of the different families, its parametric evolution, stability and also we compute the heteroclinic orbits connecting unstable isosceles equilibria. Idioma: Inglés DOI: 10.1016/j.asr.2024.10.017 Año: 2024 Publicado en: Advances in Space Research 74, 11 (2024), 5687-5697 ISSN: 0273-1177 Financiación: info:eu-repo/grantAgreement/ES/DGA/E24-23R Financiación: info:eu-repo/grantAgreement/ES/MICINN/PID2020-117066GB-I00 Tipo y forma: Article (Published version) Área (Departamento): Área Matemática Aplicada (Dpto. Matemática Aplicada)
Exportado de SIDERAL (2024-12-12-12:44:57)