On the origin of the high-perihelion scattered disk: the role of the Kozai mechanism and mean motion resonances

DOI10.1007/s10569-004-4623-yzbMath1092.70005OpenAlexW2040906192WikidataQ29396430 ScholiaQ29396430MaRDI QIDQ1776096

Tabaré Gallardo, Rodney S. Gomes, Julio A. Fernández, Adrián Brunini

Publication date: 20 May 2005

Published in: Celestial Mechanics and Dynamical Astronomy (Search for Journal in Brave)

Full work available at URL: https://doi.org/10.1007/s10569-004-4623-y

zbMATH Keywords

Edgeworth-Kuiper beltmigration modelobserved population model

Mathematics Subject Classification ID

Celestial mechanics (70F15)

Related Items (2)

The relativistic factor in the orbital dynamics of point masses ⋮ Long-term orbital dynamics of trans-Neptunian objects

Cites Work

• The Kozai resonance in the outer solar system and the dynamics of long-period comets
• A second fundamental model for resonance

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