Some equilibrium of the restricted three-body problem with axial symmetric primaries and a gyrostat as infinitesimal mass

Tsogas, VG; Mavraganis, AG

dc.contributor.author	Tsogas, VG	en
dc.contributor.author	Mavraganis, AG	en
dc.date.accessioned	2014-03-01T01:19:33Z
dc.date.available	2014-03-01T01:19:33Z
dc.date.issued	2003	en
dc.identifier.issn	0923-2958	en
dc.identifier.uri	https://dspace.lib.ntua.gr/xmlui/handle/123456789/15563
dc.subject	Equilibrium states	en
dc.subject	Gyrostat	en
dc.subject	Three rigid body problem	en
dc.subject.classification	Astronomy & Astrophysics	en
dc.subject.classification	Mathematics, Interdisciplinary Applications	en
dc.title	Some equilibrium of the restricted three-body problem with axial symmetric primaries and a gyrostat as infinitesimal mass	en
heal.type	journalArticle	en
heal.identifier.primary	10.1023/A:1022922328755	en
heal.identifier.secondary	http://dx.doi.org/10.1023/A:1022922328755	en
heal.language	English	en
heal.publicationDate	2003	en
heal.abstract	The restricted three-body problem is reconsidered by replacing the point-like primaries of the classical problem by a pair of axisymmetric rigid bodies which have a plane of symmetry perpendicular to their axes, and the infinitesimal mass by a gyrostat. The conditions for the circular motion of the primaries around their center of mass are stated and they yield the classification of all possible orientations of these bodies into four groups according to the value of their angular velocity. Then the equations of motion of the gyrostat are derived and solved for the equilibrium configurations of the system.	en
heal.publisher	KLUWER ACADEMIC PUBL	en
heal.journalName	Celestial Mechanics and Dynamical Astronomy	en
dc.identifier.doi	10.1023/A:1022922328755	en
dc.identifier.isi	ISI:000181765200001	en
dc.identifier.volume	85	en
dc.identifier.issue	4	en
dc.identifier.spage	293	en
dc.identifier.epage	309	en