HEAL DSpace

Radiation effect on a particle's periodic orbits in a regular polygon configuration of N bodies

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dc.contributor.author Kalvouridis, TJ en
dc.contributor.author Bratsolis, E en
dc.contributor.author Kazazakis, D en
dc.date.accessioned 2014-03-01T01:29:04Z
dc.date.available 2014-03-01T01:29:04Z
dc.date.issued 2008 en
dc.identifier.issn 0167-9295 en
dc.identifier.uri https://dspace.lib.ntua.gr/xmlui/handle/123456789/19112
dc.subject Celestial mechanics en
dc.subject Photo-gravitational problem en
dc.subject Regular polygon (N + 1)-body problem en
dc.subject.classification Astronomy & Astrophysics en
dc.subject.classification Geosciences, Multidisciplinary en
dc.subject.other electromagnetic radiation en
dc.subject.other particle motion en
dc.subject.other polygon en
dc.title Radiation effect on a particle's periodic orbits in a regular polygon configuration of N bodies en
heal.type journalArticle en
heal.identifier.primary 10.1007/s11038-008-9241-3 en
heal.identifier.secondary http://dx.doi.org/10.1007/s11038-008-9241-3 en
heal.language English en
heal.publicationDate 2008 en
heal.abstract The photo-gravitational problems of two or more bodies have attracted much attention during the last decades. In this paper, radiation is considered as an additional factor influencing the particle motion in a regular polygon formation of N big bodies where the v = N - 1 primary bodies have equal masses and are located at the vertices of a regular polygon and the Nth primary has different mass and is located at the mass center of the system. We assume that some or all the primary bodies are radiation sources and we numerically explore various cases where symmetry of the resultant force field with respect to the same axis is preserved. For the purposes of our investigation we adopt Radzievski's theory and assumptions. The material gathered helps us to estimate the radiation effect on the evolution of periodic orbits and their characteristics, such as their periods and their stability. Figures and diagrams illustrate these alterations and document our conclusions. © Springer Science+Business Media B.V. 2008. en
heal.publisher SPRINGER en
heal.journalName Earth, Moon and Planets en
dc.identifier.doi 10.1007/s11038-008-9241-3 en
dc.identifier.isi ISI:000260219300005 en
dc.identifier.volume 103 en
dc.identifier.issue 3-4 en
dc.identifier.spage 143 en
dc.identifier.epage 159 en


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