39 citations · 53 across the 4 of their papers we have counts for
9 papers
Secular evolution of resonant small bodies: semi-analytical approach for arbitrary eccentricities in the coplanar case
Juan Pons, Tabaré Gallardo
We study the secular evolution of a particle in deep mean motion resonance (MMR) with a planet in the planar elliptic restricted three body problem. We do not consider any restrict…
Semi-analytical model for planetary resonances: application to planets around single and binary stars
Tabaré Gallardo, Cristián Beaugé, Cristian A. Giuppone
In spite of planetary resonances being a common dynamical mechanism acting on planetary systems, no general model exists for describing their properties, particularly for commensur…
Three dimensional structure of mean motion resonances beyond Neptune
Tabare Gallardo
We propose a semianalytical method for the calculation of widths, libration centers and small amplitude libration periods of the mean motion resonances k_p:k in the framework of th…
Orbital stability in the Solar System for arbitrary inclinations and eccentricities: planetary perturbations versus resonances
Tabare Gallardo
Applying the technique of dynamical maps we study the orbital stability of test particles in the Solar System in the space (a,e,i) defined by 0.1<a<38 au, 0<e<0.9 and 0<i<180 ident…
The dynamical evolution of escaped Jupiter Trojan asteroids, link to other minor body populations
Romina P. Di Sisto, Ximena S. Ramos, Tabaré Gallardo
Jupiter Trojan asteroids are located around L4 and L5 Lagrangian points on relatively stable orbits, in 1:1 MMR with Jupiter. However, not all of them lie in orbits that remain sta…
Strength, stability and three dimensional structure of mean motion resonances in the Solar System
Tabare Gallardo
In the framework of the circular restricted three body problem we show that the numerically computed strength SR(e,i,w) is a good indicator of the strength and width of the mean-mo…