The equilibria of the translational-rotational motion of two gyrostats in a Newtonian central field of forces

Mavraganis, AG; Pangalos, CA

dc.contributor.author	Mavraganis, AG	en
dc.contributor.author	Pangalos, CA	en
dc.date.accessioned	2014-03-01T01:09:06Z
dc.date.available	2014-03-01T01:09:06Z
dc.date.issued	1992	en
dc.identifier.issn	0004-640X	en
dc.identifier.uri	https://dspace.lib.ntua.gr/xmlui/handle/123456789/10835
dc.subject.classification	Astronomy & Astrophysics	en
dc.subject.other	STABILITY	en
dc.title	The equilibria of the translational-rotational motion of two gyrostats in a Newtonian central field of forces	en
heal.type	journalArticle	en
heal.identifier.primary	10.1007/BF00645246	en
heal.identifier.secondary	http://dx.doi.org/10.1007/BF00645246	en
heal.language	English	en
heal.publicationDate	1992	en
heal.abstract	The motion of two mutually-attracting gyrostats in the Newtonian field of forces of a major body is considered. The equilibrium positions of the translational motions are found out and grouped, relative to the attractive body, in collinear and equilateral equilibria. The stationary orientations at these points are also detected and the stability of all equilibrium-configurations is investigated by means of the Routh-Hurwitz criterion © 1992 Kluwer Academic Publishers.	en
heal.publisher	Kluwer Academic Publishers	en
heal.journalName	Astrophysics and Space Science	en
dc.identifier.doi	10.1007/BF00645246	en
dc.identifier.isi	ISI:A1992JX27600010	en
dc.identifier.volume	196	en
dc.identifier.issue	1	en
dc.identifier.spage	125	en
dc.identifier.epage	142	en