scientific article
From MaRDI portal
Publication:3754929
zbMath0618.70006MaRDI QIDQ3754929
A. M. Nobili, Mario Carpino, Andrea Milani
Publication date: 1987
Title: zbMATH Open Web Interface contents unavailable due to conflicting licenses.
solar systemdynamical stabilitynumerical integrationsFourier analysis techniquessecular perturbation theory
Stability for nonlinear problems in mechanics (70K20) Computational methods for problems pertaining to mechanics of particles and systems (70-08) Celestial mechanics (70F15) Galactic and stellar dynamics (85A05)
Related Items (12)
Proper elements for resonant planet-crossing asteroids ⋮ Kolmogorov and Nekhoroshev theory for the problem of three bodies ⋮ Large scale chaos and marginal stability in the solar system ⋮ Review of the dynamics in the Kirkwood gaps ⋮ Old perturbative methods for a new problem in celestial mechanics: the space debris dynamics ⋮ Fitting a line to a sine ⋮ Monte Carlo modelling of cometary dynamics ⋮ The main secular resonances \(\nu{}_ 6,\nu{}_ 5\) and \(\nu{}_{16}\) in the asteroid belt ⋮ Are the analytical proper elements of asteroids still needed? ⋮ A semi-analytical model of the Galilean satellites' dynamics ⋮ Secular perturbation theory and computation of asteroid proper elements ⋮ Is the Solar System Stable?
This page was built for publication:
