Parametric evolution of periodic orbits in the restricted four-body problem with radiation pressure

Kalvouridis, TJ; Arribas, M; Elipe, A

dc.contributor.author	Kalvouridis, TJ	en
dc.contributor.author	Arribas, M	en
dc.contributor.author	Elipe, A	en
dc.date.accessioned	2014-03-01T01:26:52Z
dc.date.available	2014-03-01T01:26:52Z
dc.date.issued	2007	en
dc.identifier.issn	0032-0633	en
dc.identifier.uri	https://dspace.lib.ntua.gr/xmlui/handle/123456789/18264
dc.subject	Families of periodic orbits	en
dc.subject	Radiation pressure	en
dc.subject	Restricted four-body problem	en
dc.subject	Stability	en
dc.subject	Symmetric periodic orbits	en
dc.subject.classification	Astronomy & Astrophysics	en
dc.subject.other	Equations of motion	en
dc.subject.other	Gravitational effects	en
dc.subject.other	Problem solving	en
dc.subject.other	Radiation effects	en
dc.subject.other	Time varying systems	en
dc.subject.other	Periodic orbits	en
dc.subject.other	Radiation pressure	en
dc.subject.other	Restricted four-body problems	en
dc.subject.other	Symmetric periodic orbits	en
dc.subject.other	Orbits	en
dc.title	Parametric evolution of periodic orbits in the restricted four-body problem with radiation pressure	en
heal.type	journalArticle	en
heal.identifier.primary	10.1016/j.pss.2006.07.005	en
heal.identifier.secondary	http://dx.doi.org/10.1016/j.pss.2006.07.005	en
heal.language	English	en
heal.publicationDate	2007	en
heal.abstract	The backbone of the analysis in most dynamical systems is the study of periodic motions, since they greatly assist us to understand the structure of all possible motions. In this paper, we deal with the photogravitational version of the rectilinear restricted four-body problem and we investigate the dynamical behaviour of a small particle that is subjected to both the gravitational attraction and the radiation pressure of three bodies much bigger than the particle, the primaries. These bodies are always in syzygy and two of them have equal masses and are located at equal distances from the third primary. We study the effect of radiation on the distribution of the periodic orbits, their stability, as well as the evolution of the families and their main features. (c) 2006 Elsevier Ltd. All rights reserved.	en
heal.publisher	PERGAMON-ELSEVIER SCIENCE LTD	en
heal.journalName	Planetary and Space Science	en
dc.identifier.doi	10.1016/j.pss.2006.07.005	en
dc.identifier.isi	ISI:000244984600010	en
dc.identifier.volume	55	en
dc.identifier.issue	4	en
dc.identifier.spage	475	en
dc.identifier.epage	493	en