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Mutual Potential of Homogeneous Polyhedra

dc.contributor.authorWerner, Robert A.en_US
dc.contributor.authorScheeres, Daniel J.en_US
dc.date.accessioned2006-09-08T20:29:01Z
dc.date.available2006-09-08T20:29:01Z
dc.date.issued2005-03en_US
dc.identifier.citationWerner, Robert A.; Scheeres, Daniel J.; (2005). "Mutual Potential of Homogeneous Polyhedra." Celestial Mechanics and Dynamical Astronomy 91 (3-4): 337-349. <http://hdl.handle.net/2027.42/42570>en_US
dc.identifier.issn0923-2958en_US
dc.identifier.issn1572-9478en_US
dc.identifier.urihttps://hdl.handle.net/2027.42/42570
dc.description.abstractThe mutual gravitational potential between a pair of homogeneous polyhedra is expressed using an infinite series. The nested volume integrals are evaluated analytically and result in simple tensor expressions containing no special functions. However, complexity increases as O (6 n ), where n is the term degree. An alternate formulation due to Liebenthal is also presented.en_US
dc.format.extent337696 bytes
dc.format.extent3115 bytes
dc.format.mimetypeapplication/pdf
dc.format.mimetypetext/plain
dc.language.isoen_US
dc.publisherKluwer Academic Publishers; Springeren_US
dc.subject.otherPhysicsen_US
dc.subject.otherAstronomyen_US
dc.subject.otherInertia Integralen_US
dc.subject.otherMutual Potentialen_US
dc.subject.otherPolyhedron Potentialen_US
dc.subject.otherTwo Rigid Bodies Problemen_US
dc.titleMutual Potential of Homogeneous Polyhedraen_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, , , 1320 Beal Avenue, , Ann Arbor, , MI, , 48109-2140, , USA,en_US
dc.contributor.affiliationotherJet Propulsion Laboratory, California Institute of Technology, , , 4800 Oak Grove Drive, , Pasadena, , CA, , 91109-8001, , USA,en_US
dc.contributor.affiliationumcampusAnn Arboren_US
dc.description.bitstreamurlhttp://deepblue.lib.umich.edu/bitstream/2027.42/42570/1/10569_2004_Article_4621.pdfen_US
dc.identifier.doihttp://dx.doi.org/10.1007/s10569-004-4621-0en_US
dc.identifier.sourceCelestial Mechanics and Dynamical Astronomyen_US
dc.owningcollnameInterdisciplinary and Peer-Reviewed


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