On the growth and stability of Trojan planets

DOI10.1051/0004-6361:200810705zbMath1160.85301arXiv0811.4611OpenAlexW2091460103WikidataQ68674951 ScholiaQ68674951MaRDI QIDQ3618886

Richard P. Nelson, P. Cresswell

Publication date: 3 April 2009

Published in: Astronomy & Astrophysics (Search for Journal in Brave)

Full work available at URL: https://arxiv.org/abs/0811.4611

zbMATH Keywords

hydrodynamicsplanets and satellites: formation

Mathematics Subject Classification ID

Galactic and stellar dynamics (85A05) Hydrodynamic and hydromagnetic problems in astronomy and astrophysics (85A30)

Related Items (4)

New Hamiltonian expansions adapted to the Trojan problem ⋮ Secondary resonances and the boundary of effective stability of Trojan motions ⋮ Stability of Trojan planets in multi-planetary systems ⋮ Trojan resonant dynamics, stability, and chaotic diffusion, for parameters relevant to exoplanetary systems

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