Mostrando ítems 1-8 de 8
Jorba, A.; Nicolás, B.; Rodríguez, O. (2024-12-03)
The Hilda group is a set of asteroids whose mean motion is in a 3:2 orbital resonance with Jupiter. In this paper, we use the planar Circular Restricted Three-Body Problem (CRTBP) as a dynamical model and we show that there ...
Duarte, G.; Jorba, Angel (2024-10-26)
Comet 39P/Oterma is known to make fast transitions between heliocentric orbits outside the orbit of Jupiter and heliocentric orbits inside that of Jupiter. In this paper, the dynamics of comet Oterma is modelled and fitted ...
Alessi, E. M.; Baldomá, I.; Giralt, M.; Guardia, M. (2024-11-05)
Space debris mitigation guidelines represent the most effective method to preserve the circumterrestrial environment. Among them, end-of-life disposal solutions play a key role. In this regard, effective strategies should ...
Alessi, Elisa Maria; Baldomá Barraca, Inmaculada; Giralt, Mar; Guardia, Marcel; Pousse, Alexandre (2025-03-01)
Motivated by the practical interest in the third-body perturbation as a natural cleaning mechanism for high-altitude Earth orbits, we investigate the dynamics stemming from the secular Hamiltonian associated with the lunar ...
Lamas, J.; Guardia, M.; Sea, T. M. (2025-04-10)
In this paper we consider the planar circular restricted three body problem (PCRTBP), which models the motion of a massless body under the attraction of other two bodies, the primaries, which describe circular orbits around ...
Gidea, Marian; Llibre i Saló, Jaume (2009-11)
We study planar central configurations of the five-body problem where three of the bodies are collinear, forming an Euler central configuration of the three-body problem, and the two other bodies together with the collinear ...
Jorba, À.; Jorba-Cuscó, M.; Rosales, J.J. (2020-02-07)
The bicircular model is a periodic time-dependent perturbation of the Earth–Moon restricted three-body problem that includes the direct gravitational effect of the Sun on the infinitesimal particle. In this paper, we focus ...
Clarke, M.; Fejoz, J.; Guàrdia, M. (2024-09-19)
Poincaré's work more than one century ago, or Laskar's numerical simulations from the 1990's on, have irrevocably impaired the long-held belief that the Solar System should be stable. But mathematical mechanisms explaining ...