Parametric dependence of the stationary solutions in the restricted 2 + 2 body problem

Kalvouridis, TJ

dc.contributor.author	Kalvouridis, TJ	en
dc.date.accessioned	2014-03-01T01:13:59Z
dc.date.available	2014-03-01T01:13:59Z
dc.date.issued	1998	en
dc.identifier.issn	0004-640X	en
dc.identifier.uri	https://dspace.lib.ntua.gr/xmlui/handle/123456789/12827
dc.subject	Dynamic Behaviour	en
dc.subject	n-body problem	en
dc.subject	Stationary Solution	en
dc.subject.classification	Astronomy & Astrophysics	en
dc.subject.other	BODIES	en
dc.title	Parametric dependence of the stationary solutions in the restricted 2 + 2 body problem	en
heal.type	journalArticle	en
heal.identifier.primary	10.1023/A:1001571227509	en
heal.identifier.secondary	http://dx.doi.org/10.1023/A:1001571227509	en
heal.language	English	en
heal.publicationDate	1998	en
heal.abstract	The restricted gravitational 2 + 2 body problem, is a particular case of the N body problem and it may be used to approximate the dynamical behaviour of binary asteroids or dual sattelites moving in the gravitational field of two primaries P-i, i = 1, 2. By considering oblate primaries, five parameters are needed to describe the model, namely the reduced mass mu of the primary P-2, the reduced masses mu(1) and mu(2) of the minor bodies and the oblatenesses I-i, i = 1, 2 of the primaries. This work deals with the effect of those parameters on the location of the stationary solutions.	en
heal.publisher	KLUWER ACADEMIC PUBL	en
heal.journalName	Astrophysics and Space Science	en
dc.identifier.doi	10.1023/A:1001571227509	en
dc.identifier.isi	ISI:000078776500007	en
dc.identifier.volume	259	en
dc.identifier.issue	1	en
dc.identifier.spage	77	en
dc.identifier.epage	90	en