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 |