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

Croustalloudi, MN; Kalvouridis, TJ

dc.contributor.author	Croustalloudi, MN	en
dc.contributor.author	Kalvouridis, TJ	en
dc.date.accessioned	2014-03-01T11:46:25Z
dc.date.available	2014-03-01T11:46:25Z
dc.date.issued	2010	en
dc.identifier.issn	0004640X	en
dc.identifier.uri	https://dspace.lib.ntua.gr/xmlui/handle/123456789/37893
dc.subject	Regular polygon problem of (N+1) bodies	en
dc.subject	Ring problem of (N+1) bodies	en
dc.subject	Trapping regions of motion	en
dc.subject	Zero velocity surfaces	en
dc.title	Regions of a satellite's motion in a Maxwell's ring system of N bodies	en
heal.type	other	en
heal.identifier.primary	10.1007/s10509-010-0462-3	en
heal.identifier.secondary	http://dx.doi.org/10.1007/s10509-010-0462-3	en
heal.publicationDate	2010	en
heal.abstract	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. © 2010 Springer Science+Business Media B.V.	en
heal.journalName	Astrophysics and Space Science	en
dc.identifier.doi	10.1007/s10509-010-0462-3	en
dc.identifier.spage	1	en
dc.identifier.epage	14	en