Two families of simply symmetric orbits in E3

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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

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