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Regions of a satellite's motion in a Maxwell's ring system of N bodies

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Regions of a satellite's motion in a Maxwell's ring system of N bodies (EN)
Kalvouridis, TJ (EN)
Croustalloudi, MN (EN)
journalArticle (EN)
2014-03-01T01:36:42Z
2011 (EN)
The study of a dynamical system comprises a variety of processes, each one of which requires careful analysis. A fundamental preliminary step is to detect and limit the regions where solutions may exist. In the case of the ring problem of (N+1)-bodies or, otherwise, the regular polygon problem of (N+1) bodies, the existence of a Jacobian-type integral of motion constitutes the key for the investigation of the areas where the motions of the small particle are realized. Based on the aforementioned integral, we present an extended study of the parametric evolution of the regions where 3-D particle motions may exist. (EN)
Astronomy & Astrophysics (EN)
Ring problem of (N+1) bodies (EN)
Zero velocity surfaces (EN)
Trapping regions of motion (EN)
EQUILIBRIA (EN)
ORBITS (EN)
DYNAMICS (EN)
LINEAR-STABILITY (EN)
BODY PROBLEM (EN)
Regular polygon problem of (N+1) bodies (EN)
CONFIGURATIONS (EN)
ASTROPHYSICS AND SPACE SCIENCE (EN)
English
SPRINGER (EN)
National Technical University of Athens
Digital Library of National Technical University of Athens | Dspace@NTUA
Κεντρική Βιβλιοθήκη Ε.Μ.Π.
Ιδρυματικό Αποθετήριο
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