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  • 1
    Electronic Resource
    Electronic Resource
    Springer
    Celestial mechanics and dynamical astronomy 72 (1998), S. 129-156 
    ISSN: 1572-9478
    Source: Springer Online Journal Archives 1860-2000
    Topics: Physics
    Notes: Abstract The present paper reviews our current understanding of the dynamical structure of the Kuiper belt and of the origin of Jupiter-family comets. It also discusses the evolutionary scenarios that have been proposed so far to explain the observed structure of the Kuiper belt population.
    Type of Medium: Electronic Resource
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  • 2
    Electronic Resource
    Electronic Resource
    Springer
    Celestial mechanics and dynamical astronomy 63 (1995), S. 227-239 
    ISSN: 1572-9478
    Keywords: Invariant tori ; overlapping of resonances ; Lyapunov exponents ; diffusion times ; random walk
    Source: Springer Online Journal Archives 1860-2000
    Topics: Physics
    Notes: Abstract On the basis of the general theory of Hamiltonian systems, we consider the relationship between Lyapunov times and macroscopic diffusion times. We find out that there are two regimes: the Nekhoroshev regime and the resonant overlapping regime. In the first case the diffusion time is exponentially long with respect to Lyapunov times. In the second case, the relationship is polynomial although we do not find any theoretical reason for the existence of a ‘universal’ power law. We show numerical evidences which confirm our theoretical considerations.
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  • 3
    Electronic Resource
    Electronic Resource
    Springer
    Celestial mechanics and dynamical astronomy 47 (1989), S. 145-172 
    ISSN: 1572-9478
    Keywords: resonance ; perturbation method ; Kirkwood gaps ; periodic orbits
    Source: Springer Online Journal Archives 1860-2000
    Topics: Physics
    Notes: Abstract The classical problem of the dynamics in the asteroids belt is revisited in the light of recently developed perturbation methods. We consider the spatial problem of three bodies both in the circular and in the elliptic case, looking for families of periodic or quasi periodic orbits. Some criteria for deciding the stability of these families are also indicated.
    Type of Medium: Electronic Resource
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  • 4
    Electronic Resource
    Electronic Resource
    Springer
    Celestial mechanics and dynamical astronomy 51 (1991), S. 169-197 
    ISSN: 1572-9478
    Keywords: asteroid belt ; secular resonance ; action angle variables ; surface of section ; numerical simulation
    Source: Springer Online Journal Archives 1860-2000
    Topics: Physics
    Notes: Abstract In this paper an analytical model, suitable for a global description of the dynamics in a secular resonance of order 1, is derived from the general perturbation study developed in a previous paper (Morbidelli and Henrard (1991)). Such a model is then used to study the secular resonances ν6, ν5 and ν16, and pictures illustrating the secular motion are obtained. The peculiarities of the ν5 resonances are discussed in detail. The results are compared with those obtained by the theories of Yoshikawa and Nakai-Kinoshita. Some numerical simulations performed by Ch. Froeschlé and H. Scholl are discussed in the light of the new theoretical results. New numerical experiments on the ν6 resonance are also presented.
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  • 5
    Electronic Resource
    Electronic Resource
    Springer
    Celestial mechanics and dynamical astronomy 56 (1993), S. 273-276 
    ISSN: 1572-9478
    Source: Springer Online Journal Archives 1860-2000
    Topics: Physics
    Type of Medium: Electronic Resource
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  • 6
    Electronic Resource
    Electronic Resource
    Springer
    Celestial mechanics and dynamical astronomy 55 (1993), S. 131-159 
    ISSN: 1572-9478
    Keywords: Perturbation methods ; KAM theorem ; Nekhoroshev theorem ; action-angle variables
    Source: Springer Online Journal Archives 1860-2000
    Topics: Physics
    Notes: Abstract We revisit some results of perturbation theories by a method of successive elimination of harmonics inspired by some ideas of Delaunay. On the one hand, we give a connection between the KAM theorem and the Nekhoroshev theorem. On the other hand, we support in a quantitative fashion a semi-numerical method of analysis of a perturbed system recently introduced by one of the authors.
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  • 7
    Electronic Resource
    Electronic Resource
    Springer
    Celestial mechanics and dynamical astronomy 60 (1994), S. 29-56 
    ISSN: 1572-9478
    Keywords: asteroids ; proper elements ; averaging method
    Source: Springer Online Journal Archives 1860-2000
    Topics: Physics
    Notes: Abstract Based on Williams' work and rewritten in action angle variables, a method for the calculation of proper elements is here presented. The averaging over the long periodic terms is performed by the semi numerical method developed by Henrard (1990); no series expansion in eccentricity or inclination of the asteroid is used which allows calculating proper elements for highly inclined orbits. Conversely, the theory is truncated at the first degree in the eccentricity and the inclination of the perturbing planets. A few tests about accuracy and consistency are presented.
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  • 8
    Electronic Resource
    Electronic Resource
    Springer
    Celestial mechanics and dynamical astronomy 65 (1996), S. 107-136 
    ISSN: 1572-9478
    Keywords: Nekhoroshev theorem ; frequency analysis ; Lyapunov exponents ; asteroids ; degenerate systems
    Source: Springer Online Journal Archives 1860-2000
    Topics: Physics
    Notes: Abstract The present paper reviews the Nekhoroshev theorem from the point of view of physicists and astronomers. We point out that Nekhoroshev result is strictly connected with the existence of a specific structure of the phase space, the existence of which can be checked with several numerical tools. This is true also for a degenerate system such as the one describing the motion of an asteroid in the so called main belt. The main difference is that in some parts of the belt, the Nekhoroshev result cannot apply a priori. Mean motion resonances of order smaller than the logarithm of the mass of Jupiter and first order secular resonances must be excluded. In the remaining parts, conversely, the Nekhoroshev theorem can be proved, provided someparameters, such as the masses, the eccentricities and the inclinations of the planets are small enough. At the light of this result, a massive campaign of numerical integrations of real and fictitious asteroids should allow to understand which is the real dynamical structure of the asteroid belt.
    Type of Medium: Electronic Resource
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  • 9
    Electronic Resource
    Electronic Resource
    Springer
    Celestial mechanics and dynamical astronomy 68 (1998), S. 199-204 
    ISSN: 1572-9478
    Source: Springer Online Journal Archives 1860-2000
    Topics: Physics
    Type of Medium: Electronic Resource
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  • 10
    Electronic Resource
    Electronic Resource
    Springer
    Celestial mechanics and dynamical astronomy 55 (1993), S. 101-130 
    ISSN: 1572-9478
    Keywords: action-angle variables ; resonances ; chaotic motion ; perturbation theories ; KAM theorem
    Source: Springer Online Journal Archives 1860-2000
    Topics: Physics
    Notes: Abstract A practical method for the detailed exploration of two degrees of freedom dynamical systems is presented in this paper. This method is made up of several steps, in each of which we eliminate, via the introduction of suitable action-angle variables, the most relevant harmonic present in the Fourier expansion of the perturbation. In this way, at the end, one obtains a satisfactory description of the fine structure of secondary resonances, as well as detailed information about the size of chaotic layers and about the localization of regions filled up with invariant tori.
    Type of Medium: Electronic Resource
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