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On The Concept Of Periapsis In Hill’s Problem

dc.contributor.authorVillac, Benjamin F.en_US
dc.contributor.authorScheeres, Daniel J.en_US
dc.date.accessioned2006-09-08T20:28:53Z
dc.date.available2006-09-08T20:28:53Z
dc.date.issued2004-09en_US
dc.identifier.citationVillac, B.F.; Scheeres, D.J.; (2004). "On The Concept Of Periapsis In Hill’s Problem." Celestial Mechanics and Dynamical Astronomy 90 (1-2): 165-178. <http://hdl.handle.net/2027.42/42568>en_US
dc.identifier.issn0923-2958en_US
dc.identifier.issn1572-9478en_US
dc.identifier.urihttps://hdl.handle.net/2027.42/42568
dc.description.abstractThe concept of closest approach is analyzed in Hill’s problem, resulting in a partitioning of the position space. The different behavior between the direct and retrograde motion is explained analytically, resulting in a simple estimate of the variation of Hill’s periodic and quasi-circular orbits as a function of the Jacobi constant. The local behavior of the orbits on the zero velocity surfaces and an analytical definition of local escape and capture in Hill’s problem are also given.en_US
dc.format.extent243864 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.otherCaptureen_US
dc.subject.otherEscapeen_US
dc.subject.otherHill’S Problemen_US
dc.subject.otherPeriapsisen_US
dc.subject.otherPeriodic Orbitsen_US
dc.titleOn The Concept Of Periapsis In Hill’s Problemen_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, , USA,en_US
dc.contributor.affiliationumDepartment of Aerospace Engineering, , The University of Michigan, , , Ann Arbor, , MI, , USA,en_US
dc.contributor.affiliationumcampusAnn Arboren_US
dc.description.bitstreamurlhttp://deepblue.lib.umich.edu/bitstream/2027.42/42568/1/10569_2004_Article_405.pdfen_US
dc.identifier.doihttp://dx.doi.org/10.1007/s10569-004-0405-9en_US
dc.identifier.sourceCelestial Mechanics and Dynamical Astronomyen_US
dc.owningcollnameInterdisciplinary and Peer-Reviewed


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