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  • Springer  (40)
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  • Articles  (40)
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  • 1
    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.
    Type of Medium: Electronic Resource
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  • 2
    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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  • 3
    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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  • 4
    Electronic Resource
    Electronic Resource
    Springer
    Celestial mechanics and dynamical astronomy 57 (1993), S. 99-108 
    ISSN: 1572-9478
    Keywords: mean motion resonances ; secondary resonances ; secular resonances ; planar circular and elliptic restricted problem ; action-angle variables ; surfaces of section
    Source: Springer Online Journal Archives 1860-2000
    Topics: Physics
    Notes: Abstract We study the motion of asteroids in the main mean motion commensurabilities in the frame of the planar restricted three-body problem. No assumption is made about the size of the eccentricity of the asteroid. At small to moderate eccentricity, we recover existing results (shape of the phase space and location of secondary resonances). We also provide global pictures of the dynamics in the region of secondary resonances. At high eccentricity, the phase space portraits of the integrable part of the Hamiltonian show new families of stable orbits for the 3:2 and 2:1 cases and the secular resonances ν5 and ν6 are located.
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  • 5
    Electronic Resource
    Electronic Resource
    Springer
    Celestial mechanics and dynamical astronomy 57 (1993), S. 155-173 
    ISSN: 1572-9478
    Keywords: artificial satellite theory ; geosynchronous orbits ; critical inclination ; luni-solar effects ; surface of section
    Source: Springer Online Journal Archives 1860-2000
    Topics: Physics
    Notes: Abstract The luni-solar effects of a geosynchronous artificial satellite orbiting near the critical inclination is investigated. To tackle this four-degrees-of-freedom problem, a preliminary exploration separately analyzing each harmonic formed by a combination of the satellite longitude of the node and the Moon longitude of the node is opportune. This study demonstrates that the dynamics induced by these harmonics does not show resonance phenomena. In a second approach, the number of degrees of freedom is halved by averaging the total Hamiltonian over the two non-resonant angular variables. A semi-numerical method can now be applied as was done when considering solely the inhomogeneity of the geopotential (see Delhaise et Henrard, 1992). Approximate surfaces of section are constructed in the plane of the inclination and argument of perigee. The main effects of the Sun and Moon attractions compared to the terrestrial attraction alone are a strong increase in the amplitude of libration in inclination (from 0.6° to 3.2°) and a decrease of the corresponding libration period (from the order of 200 years to the order of 20 years).
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  • 6
    Electronic Resource
    Electronic Resource
    Springer
    Celestial mechanics and dynamical astronomy 66 (1996), S. 255-292 
    ISSN: 1572-9478
    Keywords: asteroids ; Nekhoroshev theorem ; degenerate systems
    Source: Springer Online Journal Archives 1860-2000
    Topics: Physics
    Notes: Abstract We investigate the possibility of obtaining a Nekhoroshev like result for the dynamical system describing the motion of an asteroid in the main belt, From the mathematical point of view this is a new result since the problem is degenerate and we want to control also the motion of degenerate actions, We find that there are regions, such as the resonances of low order among the fast angles (mean motion resonances), where a Nekhoroshev like result cannot be proved a priori, Conversely, we are able to confine the motions in the mean motion resonances of logarithmically large order in the perturbation parameters, as well as in the non-resonant region, We discuss also the connection with the existence of invariant tori.
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  • 7
    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.
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  • 8
    Electronic Resource
    Electronic Resource
    Springer
    Celestial mechanics and dynamical astronomy 47 (1989), S. 173-204 
    ISSN: 1572-9478
    Keywords: resonances ; perturbation method ; Kirkwood gaps ; periodic orbits
    Source: Springer Online Journal Archives 1860-2000
    Topics: Physics
    Notes: Abstract The general theory exposed in the first part of this paper is applied to the following resonances with Jupiter's motion : 3/2, 2/1, 5/2, 3/1, 7/2, 4/1; these are the most relevant resonances for the asteroids. The whole analysis is performed in the framework of the spatial problem of three bodies, both in the circular and in the elliptic case. The results are also compared with the observed distribution of the asteroids.
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  • 9
    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.
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  • 10
    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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