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Particle motions in Maxwell's ring dynamical systems

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dc.contributor.author Kalvouridis, TJ en
dc.date.accessioned 2014-03-01T02:45:43Z
dc.date.available 2014-03-01T02:45:43Z
dc.date.issued 2008 en
dc.identifier.issn 0923-2958 en
dc.identifier.uri https://dspace.lib.ntua.gr/xmlui/handle/123456789/32345
dc.subject Celestial mechanics en
dc.subject Particle dynamics in regular polygon configurations of (ν + 1) bodies en
dc.subject.classification Astronomy & Astrophysics en
dc.subject.classification Mathematics, Interdisciplinary Applications en
dc.subject.other CENTRAL CONFIGURATIONS en
dc.subject.other BODY PROBLEM en
dc.subject.other RELATIVE EQUILIBRIA en
dc.subject.other PERIODIC-SOLUTIONS en
dc.subject.other N BODIES en
dc.subject.other STABILITY en
dc.subject.other ORBITS en
dc.subject.other FAMILIES en
dc.title Particle motions in Maxwell's ring dynamical systems en
heal.type conferenceItem en
heal.identifier.primary 10.1007/s10569-008-9149-2 en
heal.identifier.secondary http://dx.doi.org/10.1007/s10569-008-9149-2 en
heal.language English en
heal.publicationDate 2008 en
heal.abstract The focus of this contribution is an effort to review and report the main results obtained so far, concerning the periodic motions of a small body in the combined gravitational field created by a regular ν-gon arrangement of ν big bodies with equal masses, where ν > 7, and another central primary with different mass. Various types of planar periodic motions are presented and networks of characteristic curves of families are depicted, in order to show their distribution in the space of the initial conditions, as well as the evolution of their members that are also examined under the variation of the parameters of the system. Furthermore, the regions of the allowed three-dimensional motions, as well as their variation, are illustrated by means of the zero-velocity surfaces. All this new material is added to the already existing data, and completes thus the profile of the dynamical behavior of the system. © 2008 Springer Science+Business Media B.V. en
heal.publisher SPRINGER en
heal.journalName Celestial Mechanics and Dynamical Astronomy en
dc.identifier.doi 10.1007/s10569-008-9149-2 en
dc.identifier.isi ISI:000260261300014 en
dc.identifier.volume 102 en
dc.identifier.issue 1-3 en
dc.identifier.spage 191 en
dc.identifier.epage 206 en


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