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Equilibrium states of a gyrostat satellite in an annular configuration of N big bodies

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dc.contributor.author Tsogas, V en
dc.contributor.author Kalvouridis, TJ en
dc.contributor.author Mavraganis, AG en
dc.date.accessioned 2014-03-01T01:22:18Z
dc.date.available 2014-03-01T01:22:18Z
dc.date.issued 2005 en
dc.identifier.issn 0001-5970 en
dc.identifier.uri https://dspace.lib.ntua.gr/xmlui/handle/123456789/16518
dc.subject Equation of Motion en
dc.subject Equilibrium State en
dc.subject.classification Mechanics en
dc.subject.other Equations of motion en
dc.subject.other Force measurement en
dc.subject.other Gyroscopes en
dc.subject.other Integer programming en
dc.subject.other Loads (forces) en
dc.subject.other Mathematical models en
dc.subject.other Parameter estimation en
dc.subject.other Spacecraft en
dc.subject.other System stability en
dc.subject.other Equilibrium states en
dc.subject.other Gyrodynamics en
dc.subject.other Gyrostat satellite en
dc.subject.other Newtonian forces en
dc.subject.other Satellites en
dc.title Equilibrium states of a gyrostat satellite in an annular configuration of N big bodies en
heal.type journalArticle en
heal.identifier.primary 10.1007/s00707-004-0189-8 en
heal.identifier.secondary http://dx.doi.org/10.1007/s00707-004-0189-8 en
heal.language English en
heal.publicationDate 2005 en
heal.abstract The paper deals with the dynamics of a gyrostat satellite acted upon by the Newtonian forces of N coplanar big bodies, ν=N-1 of which are arranged at equal distances on the periphery of a circle, while the Nth body is located at the mass center of the system. The gyrostat's equations of motion are derived and its equilibrium states as well as their stability are studied. © Springer-Verlag 2005 Wien. en
heal.publisher SPRINGER WIEN en
heal.journalName Acta Mechanica en
dc.identifier.doi 10.1007/s00707-004-0189-8 en
dc.identifier.isi ISI:000228657400010 en
dc.identifier.volume 175 en
dc.identifier.issue 1-4 en
dc.identifier.spage 181 en
dc.identifier.epage 195 en


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