Skip to main content
All Reviews
Astronomy
intermediate

An exploration of the Kozai resonance in the Kuiper Belt

X.- S. Wan & T.- Y. Huang (2007)

Published
May 1, 2007
Journal
Monthly Notices of the Royal Astronomical Society · Vol. 377 · No. 1
DOI
10.1111/j.1365-2966.2007.11541.x

At a GlanceAI

Maps Kozai (Lidov–Kozai) resonance behavior for Kuiper Belt orbits, highlighting its role in long-term eccentricity–inclination exchange.

SummaryAI

The study examines how the Lidov–Kozai resonance can shape Kuiper Belt object dynamics through coupled oscillations of eccentricity and inclination with associated perihelion precession. By exploring where Kozai-type libration is expected in Kuiper Belt phase space, it clarifies when objects can maintain stable, long-lived configurations versus undergoing large orbital-element variations. This helps interpret the observed distribution of Kuiper Belt orbital architectures and informs dynamical pathways that can protect or destabilize distant small bodies.

Method SnapshotAI

Analytical and dynamical exploration of secular (Kozai) resonance structure in Kuiper Belt orbital parameter space.

BackgroundAI

Celestial mechanics of secular perturbations and Lidov–Kozai resonance applied to trans-Neptunian dynamics.