The dynamics of inclined Neptune Trojans
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Publication:1003179
DOI10.1007/S10569-008-9136-7zbMath1154.70316OpenAlexW2021219275MaRDI QIDQ1003179
Christoph Lhotka, Rudolf Dvorak, Richard I. Schwarz
Publication date: 27 February 2009
Published in: Celestial Mechanics and Dynamical Astronomy (Search for Journal in Brave)
Full work available at URL: https://doi.org/10.1007/s10569-008-9136-7
Related Items (7)
The 1/1 resonance in extrasolar planetary systems ⋮ Dynamic expansion points: an extension to Hadjidemetriou's mapping method ⋮ Long-term evolution of quasi-circular Trojan orbits ⋮ A parametric study of stability and resonances around \(L_4\) in the elliptic restricted three-body problem ⋮ Stability of Trojan planets in multi-planetary systems ⋮ Low-thrust propulsion in a coplanar circular restricted four body problem ⋮ Where are the Uranus Trojans?
Cites Work
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- The observed Trojans and the global dynamics around the Lagrangian points of the Sun-Jupiter system
- On the stability regions of the Trojan asteroids
- Symplectic mapping for Trojan-type motion in the elliptic restricted three-body problem
- On the stability of high inclined \(\mathbf L_4\) and \(\mathbf L_5\) Trojans
- Collisional velocities and rates in resonant planetesimal belts
- The dynamics of bodies with variable masses
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