Search Results - "Robutel, P."
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The resonant structure of Jupiter's Trojan asteroids – I. Long-term stability and diffusion
Published in Monthly notices of the Royal Astronomical Society (11-11-2006)“…We study the global dynamics of the jovian Trojan asteroids by means of the frequency map analysis. We find and classify the main resonant structures that…”
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Long term evolution and chaotic diffusion of the insolation quantities of Mars
Published in Icarus (New York, N.Y. 1962) (01-08-2004)“…As the obliquity of Mars is strongly chaotic, it is not possible to give a solution for its evolution over more than a few million years. Using the most recent…”
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On the coplanar eccentric non-restricted co-orbital dynamics
Published in Celestial mechanics and dynamical astronomy (01-03-2018)“…We study the phase space of eccentric coplanar co-orbitals in the non-restricted case. Departing from the quasi-circular case, we describe the evolution of the…”
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The resonant structure of Jupiter's Trojan asteroids – II. What happens for different configurations of the planetary system
Published in Monthly notices of the Royal Astronomical Society (11-10-2009)“…In a previous paper, we have found that the resonance structure of the present Jupiter Trojan swarms could be split up into four different families of…”
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Frozen orbits at high eccentricity and inclination: application to Mercury orbiter
Published in Celestial mechanics and dynamical astronomy (01-11-2010)“…We hereby study the stability of a massless probe orbiting around an oblate central body (planet or planetary satellite) perturbed by a third body, assumed to…”
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On the rotation of co-orbital bodies in eccentric orbits
Published in Celestial mechanics and dynamical astronomy (01-06-2016)“…We investigate the resonant rotation of co-orbital bodies in eccentric and planar orbits. We develop a simple analytical model to study the impact of the…”
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Frequency Map and Global Dynamics in the Solar System I: Short Period Dynamics of Massless Particles
Published in Icarus (New York, N.Y. 1962) (01-07-2001)“…Frequency map analysis (FMA) is a refined numerical method based on Fourier techniques that provides a clear representation of the global dynamics of…”
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The chaotic obliquity of the planets
Published in Nature (London) (18-02-1993)“…Numerical study of the obliquity of planets (the global stability of the spin-axis orientation of planets against secular orbital perturbations) shows that all…”
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Stabilization of the Earth's obliquity by the Moon
Published in Nature (London) (18-02-1993)“…By integrating the equations of precession of the Earth, all possible values of Earth's initial obliquity were investigated. The study shows the Moon to have…”
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The Influence of Giant Planets Near a Mean Motion Resonance on Earth-like Planets in the Habitable Zone of Sun-like Stars
Published in The Astrophysical journal (10-07-2008)“…We present a numerical study of several two-planet systems based on the motions of Jupiter and Saturn, in which the two giant planets move in low eccentric…”
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The Observed Trojans and the Global Dynamics Around The Lagrangian Points of the Sun–Jupiter System
Published in Celestial mechanics and dynamical astronomy (01-04-2005)“…In this paper, we make a systematic study of the global dynamical structure of the Sun-Jupiter L^sub 4^ tadpole region. The results are based on long-time…”
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On the stability of Earth-like planets in multi-planet systems
Published in Celestial mechanics and dynamical astronomy (01-09-2008)“…We present a continuation of our numerical study on planetary systems with similar characteristics to the Solar System. This time we examine the influence of…”
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Partial Reduction in the N-Body Planetary Problem using the Angular Momentum Integral
Published in Celestial mechanics and dynamical astronomy (01-11-2002)“…We present a new set of variables for the reduction of the planetary n-body problem, associated to the angular momentum integral, which can be of any use for…”
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High order symplectic integrators for perturbed Hamiltonian systems
Published in Celestial mechanics and dynamical astronomy (01-01-2001)“…A family of symplectic integrators adapted for the integration of perturbed Hamiltonian systems of the form H=A+εB was given in (McLachlan, 1995). We give here…”
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The resonant structure of Jupiter's Trojan asteroids - I. Long-term stability and diffusion
Published in Monthly notices of the Royal Astronomical Society (11-11-2006)Get full text
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The TROY project III. Exploring co-orbitals around low-mass stars
Published 05-07-2024“…Co-orbital objects, also known as trojans, are frequently found in simulations of planetary system formation. In these configurations, a planet shares its…”
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On the coplanar eccentric non restricted co-orbital dynamics
Published 20-11-2017“…We study the phase space of eccentric coplanar co-orbitals in the non-restricted case. Departing from the quasi-circular case, we describe the evolution of the…”
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Planetary system LHS 1140 revisited with ESPRESSO and TESS
Published 14-10-2020“…LHS 1140 is an M dwarf known to host two known transiting planets at orbital periods of 3.77 and 24.7 days. The external planet (LHS 1140 b) is a rocky…”
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Spin dynamics of close-in planets exhibiting large TTVs
Published 12-05-2017“…A&A 605, A37 (2017) We study the spin evolution of close-in planets in compact multi-planetary systems. The rotation period of these planets is often assumed…”
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