Chaotic motion of comets in near-parabolic orbit: Mapping approaches
type: Item
instance of: scholarly article
title: Chaotic motion of comets in near-parabolic orbit: Mapping approaches
zbMATH Open document ID: 0838.70014
DOI: 10.1007/BF00693090
author: Jie Liu
author: Yisui Sun
published in: Celestial Mechanics and Dynamical Astronomy
publication date: 1996-06-09T00:00:00Z
review text: Mapping techniques are used to investigate the chaotic character and stability near some resonant zones. Three-dimensional measure preserving mapping with ``slice-cutting'' and LCN's are used to study the system in detail. Stability of 2/1, 4/3, and 3/2 resonant zones increases successively according to this theoretical analysis. This investigation contributes to the hypothesis that parabolic orbit comets come from the Oort cloud. However, the role of the Kuiper belt is ignored in this study.
Mathematics Subject Classification ID: 70F15
Mathematics Subject Classification ID: 37B99
zbMATH DE Number: 754600
zbMATH Keywords: three-dimensional measure preserving mapping
zbMATH Keywords: stability
zbMATH Keywords: resonant zones
zbMATH Keywords: Oort cloud
MaRDI profile type: Publication
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description: scientific article; zbMATH DE number 754600