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A note on independent variables for restricted three-body problems

dc.contributor.authorHeppenheimer, T. A.en_US
dc.date.accessioned2006-09-08T20:28:14Z
dc.date.available2006-09-08T20:28:14Z
dc.date.issued1971-12en_US
dc.identifier.citationHeppenheimer, T. A.; (1971). "A note on independent variables for restricted three-body problems." Celestial Mechanics 4 (3-4): 326-328. <http://hdl.handle.net/2027.42/42558>en_US
dc.identifier.issn0008-8714en_US
dc.identifier.issn1572-9478en_US
dc.identifier.urihttps://hdl.handle.net/2027.42/42558
dc.description.abstractIn studies of the elliptic restricted three-body problem, the true anomaly of the motion of the primaries is often used as the independent variable. The equations of motion then show invariancy in form from the circular case. It is of interest whether other independent variables exist, such that the invariant form of the equations is maintained. It is found that true anomaly is the only such variable.en_US
dc.format.extent223414 bytes
dc.format.extent3115 bytes
dc.format.mimetypeapplication/pdf
dc.format.mimetypetext/plain
dc.language.isoen_US
dc.publisherKluwer Academic Publishers; D. Reidel Publishing Company ; Springer Science+Business Mediaen_US
dc.subject.otherPhysicsen_US
dc.subject.otherAstronomyen_US
dc.titleA note on independent variables for restricted three-body problemsen_US
dc.typeArticleen_US
dc.subject.hlbsecondlevelAstronomyen_US
dc.subject.hlbtoplevelScienceen_US
dc.description.peerreviewedPeer Revieweden_US
dc.contributor.affiliationumDept. of Aerospace Engineering, The University of Michigan, Ann Arbor, Mich., USAen_US
dc.contributor.affiliationumcampusAnn Arboren_US
dc.description.bitstreamurlhttp://deepblue.lib.umich.edu/bitstream/2027.42/42558/1/10569_2005_Article_BF01231394.pdfen_US
dc.identifier.doihttp://dx.doi.org/10.1007/BF01231394en_US
dc.identifier.sourceCelestial Mechanicsen_US
dc.owningcollnameInterdisciplinary and Peer-Reviewed


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