Astronomy and Astrophysics – Astronomy
Scientific paper
Oct 1993
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1993cemda..57...99m&link_type=abstract
Celestial Mechanics and Dynamical Astronomy (ISSN 0923-2958), vol. 57, no. 1-2, p. 99-108
Astronomy and Astrophysics
Astronomy
17
Asteroids, Circular Orbits, Elliptical Orbits, Jupiter (Planet), Long Term Effects, Orbit Calculation, Orbital Resonances (Celestial Mechanics), Solar Orbits, Sun, Three Body Problem, Eccentricity, Hamiltonian Functions, Orbit Perturbation
Scientific paper
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 nu5 and nu6 are located.
Moons Michele
Morbidelli Alessandro
No associations
LandOfFree
The main mean motion commensurabilities in the planar circular and elliptic problem does not yet have a rating. At this time, there are no reviews or comments for this scientific paper.
If you have personal experience with The main mean motion commensurabilities in the planar circular and elliptic problem, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and The main mean motion commensurabilities in the planar circular and elliptic problem will most certainly appreciate the feedback.
Profile ID: LFWR-SCP-O-1325654