Pages that link to "Item:Q4653466"
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The following pages link to Hamiltonian formulation of the secular theory for Trojan-type motion (Q4653466):
Displaying 11 items.
- Rigorous treatment of the averaging process for co-orbital motions in the planetary problem (Q338249) (← links)
- On the co-orbital motion of two planets in quasi-circular orbits (Q375148) (← links)
- Chaotic diffusion and effective stability of Jupiter Trojans (Q815684) (← links)
- On the coplanar eccentric non-restricted co-orbital dynamics (Q1637801) (← links)
- Secondary resonances and the boundary of effective stability of Trojan motions (Q1640683) (← links)
- On the co-orbital motion in the planar restricted three-body problem: the quasi-satellite motion revisited (Q1680315) (← links)
- Influence of the coorbital resonance on the rotation of the trojan satellites of saturn (Q1955977) (← links)
- A new perturbative solution to the motion around triangular Lagrangian points in the elliptic restricted three-body problem (Q2049208) (← links)
- Dynamics of ``jumping'' Trojans: a perturbative treatment (Q2203842) (← links)
- Trojan resonant dynamics, stability, and chaotic diffusion, for parameters relevant to exoplanetary systems (Q2348890) (← links)
- Secular evolution of co-orbital motion of two exoplanets: semi-analytical investigation (Q6573422) (← links)
