Pages that link to "Item:Q1976072"
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The following pages link to A symplectic mapping model as a tool to understand the dynamics of 2/1 resonant asteroid motion (Q1976072):
Displaying 16 items.
- The dynamical structure of the MEO region: long-term stability, chaos, and transport (Q285125) (← links)
- Asteroids: 2/1 resonance and high eccentricity (Q687257) (← links)
- A hyperbolic twist mapping model for the study of asteroid orbits near the 3:1 resonance (Q1091159) (← links)
- Asteroid motion near the 3:1 resonance (Q1308751) (← links)
- Fast Lyapunov indicators. Application to asteroidal motion (Q1373175) (← links)
- Phase space transport in a map of asteroid motion (Q1570378) (← links)
- Comparative study of the \(2:3\) and \(3:4\) resonant motion with Neptune: an application of symplectic mappings and low frequency analysis (Q1766785) (← links)
- A symplectic mapping model for the study of 2:3 resonant trans-Neptunian motion (Q1870187) (← links)
- Symplectic mappings of co-orbital motion in the restricted problem of three bodies (Q1870201) (← links)
- A symplectic mapping for the synchronous spin-orbit problem (Q1955517) (← links)
- Identification of asteroid groups in the \(z_1\) and \(z_2\) nonlinear secular resonances through genetic algorithms (Q2049211) (← links)
- An analytically treatable model of long-term dynamics in a mean motion resonance with coexisting resonant modes (Q2210852) (← links)
- Dynamic expansion points: an extension to Hadjidemetriou's mapping method (Q2389400) (← links)
- Formal solution of the asteroid motion near the 2:1 commensurability (Q2466370) (← links)
- ON THE BIFURCATION AND CONTINUATION OF PERIODIC ORBITS IN THE THREE BODY PROBLEM (Q3165830) (← links)
- Symbolic computation of the averaged Hamiltonian describing the motion of asteroids under the influence of major planets. (Q5959718) (← links)
