Two families of simply symmetric orbits in E3

Katsiaris, G

dc.contributor.author	Katsiaris, G	en
dc.date.accessioned	2014-03-01T01:05:28Z
dc.date.available	2014-03-01T01:05:28Z
dc.date.issued	1971	en
dc.identifier.issn	0004640X	en
dc.identifier.uri	https://dspace.lib.ntua.gr/xmlui/handle/123456789/8851
dc.subject	Periodic Orbit	en
dc.title	Two families of simply symmetric orbits in E3	en
heal.type	journalArticle	en
heal.identifier.primary	10.1007/BF00654606	en
heal.identifier.secondary	http://dx.doi.org/10.1007/BF00654606	en
heal.publicationDate	1971	en
heal.abstract	Numerical processes are applied to the classical formulation of the restricted problem of three bodies in order to compute families of periodic orbits that exist in E3 and are symmetric with respect to a plane that contains the two primaries and their axis of angular velocity. Two such families are found and their stability numbers are computed. In general, the discovery of such families proves to be extremely difficult. © 1971 D. Reidel Publishing Company.	en
heal.publisher	Kluwer Academic Publishers	en
heal.journalName	Astrophysics and Space Science	en
dc.identifier.doi	10.1007/BF00654606	en
dc.identifier.volume	10	en
dc.identifier.issue	1	en
dc.identifier.spage	71	en
dc.identifier.epage	86	en