The equilibrium configurations of the restricted problem of 2+2 triaxial rigid bodies

Michalakis, DG; Mavraganis, AG

dc.contributor.author	Michalakis, DG	en
dc.contributor.author	Mavraganis, AG	en
dc.date.accessioned	2014-03-01T01:11:32Z
dc.date.available	2014-03-01T01:11:32Z
dc.date.issued	1995	en
dc.identifier.issn	0923-2958	en
dc.identifier.uri	https://dspace.lib.ntua.gr/xmlui/handle/123456789/11687
dc.subject	equilibrium solutions	en
dc.subject	Restricted 2+2 rigid body problem	en
dc.subject.classification	Astronomy & Astrophysics	en
dc.subject.classification	Mathematics, Interdisciplinary Applications	en
dc.title	The equilibrium configurations of the restricted problem of 2+2 triaxial rigid bodies	en
heal.type	journalArticle	en
heal.identifier.primary	10.1007/BF00691916	en
heal.identifier.secondary	http://dx.doi.org/10.1007/BF00691916	en
heal.language	English	en
heal.publicationDate	1995	en
heal.abstract	The restricted 2+2 body problem is considered. The infinitesimal masses are replaced by triaxial rigid bodies and the equations of motion are derived in Lagrange form. Subsequently, the equilibrium solutions for the rotational and translational motion of the bodies are detected. These solutions are conveniently classified in groups according to the several combinations which are possible between the translational equilibria and the constant orientations of the bodies. © 1995 Kluwer Academic Publishers.	en
heal.publisher	Kluwer Academic Publishers	en
heal.journalName	Celestial Mechanics & Dynamical Astronomy	en
dc.identifier.doi	10.1007/BF00691916	en
dc.identifier.isi	ISI:A1995UF84400005	en
dc.identifier.volume	63	en
dc.identifier.issue	1	en
dc.identifier.spage	81	en
dc.identifier.epage	100	en