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Secular Motion in a 2nd Degree and Order-Gravity Field with no Rotation
dc.contributor.authorScheeres, Daniel J.en_US
dc.contributor.authorHu, W.en_US
dc.date.accessioned2006-09-08T20:28:29Z
dc.date.available2006-09-08T20:28:29Z
dc.date.issued2001-03en_US
dc.identifier.citationScheeres, D. J.; Hu, W.; (2001). "Secular Motion in a 2nd Degree and Order-Gravity Field with no Rotation." Celestial Mechanics and Dynamical Astronomy 79(3): 183-200. <http://hdl.handle.net/2027.42/42562>en_US
dc.identifier.issn0923-2958en_US
dc.identifier.issn1572-9478en_US
dc.identifier.urihttps://hdl.handle.net/2027.42/42562
dc.description.abstractThe motion of a particle about a non-rotating 2nd degree and order-gravity field is investigated. Averaging conditions are applied to the particle motion and a qualitative analysis which reveals the general character of motion in this system is given. It is shown that the orbit plane will either be stationary or precess about the body's axis of minimum or maximum moment of inertia. It is also shown that the secular equations for this system can be integrated in terms of trigonometric, hyperbolic or elliptic functions. The explicit solutions are derived in all cases of interest.en_US
dc.format.extent140994 bytes
dc.format.extent3115 bytes
dc.format.mimetypeapplication/pdf
dc.format.mimetypetext/plain
dc.language.isoen_US
dc.publisherKluwer Academic Publishers; Springer Science+Business Mediaen_US
dc.subject.otherPhysicsen_US
dc.subject.otherAstronomyen_US
dc.subject.otherDipole Gravityen_US
dc.subject.otherSecular Motionen_US
dc.subject.otherAveraging Methodsen_US
dc.subject.otherAnalytical Solutionen_US
dc.titleSecular Motion in a 2nd Degree and Order-Gravity Field with no Rotationen_US
dc.typeArticleen_US
dc.subject.hlbsecondlevelAstronomyen_US
dc.subject.hlbtoplevelScienceen_US
dc.description.peerreviewedPeer Revieweden_US
dc.contributor.affiliationumDepartment of Aerospace Engineering, The University of Michigan, Ann Arbor, MI, 48109-2140en_US
dc.contributor.affiliationumDepartment of Aerospace Engineering, The University of Michigan, Ann Arbor, MI, 48109-2140en_US
dc.contributor.affiliationumcampusAnn Arboren_US
dc.description.bitstreamurlhttp://deepblue.lib.umich.edu/bitstream/2027.42/42562/1/10569_2004_Article_332232.pdfen_US
dc.identifier.doihttp://dx.doi.org/10.1023/A:1017555005699en_US
dc.identifier.sourceCelestial Mechanics and Dynamical Astronomyen_US
dc.owningcollnameInterdisciplinary and Peer-Reviewed


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