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Bounds on Rotation Periods of Disrupted Binaries in the Full 2-Body Problem
dc.contributor.authorScheeres, Daniel J.en_US
dc.date.accessioned2006-09-08T20:28:49Z
dc.date.available2006-09-08T20:28:49Z
dc.date.issued2004-06en_US
dc.identifier.citationScheeres, D. J.; (2004). "Bounds on Rotation Periods of Disrupted Binaries in the Full 2-Body Problem." Celestial Mechanics and Dynamical Astronomy 89(2): 127-140. <http://hdl.handle.net/2027.42/42567>en_US
dc.identifier.issn0923-2958en_US
dc.identifier.issn1572-9478en_US
dc.identifier.urihttps://hdl.handle.net/2027.42/42567
dc.description.abstractConstraints on the final rotation rates of a Hill unstable binary in the full 2-body problem are derived and analyzed. Application of these constraints are made to the problem of a constant density body spun to disruption. This analysis has relevance to the evolution of asteroid spin rates.en_US
dc.format.extent103703 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.otherAsteroidsen_US
dc.subject.otherFull 2-body Problemen_US
dc.subject.otherGravitational Potentialsen_US
dc.subject.otherRotationen_US
dc.titleBounds on Rotation Periods of Disrupted Binaries in the Full 2-Body 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, 1320 Beal Avenue, 3048 FXB Building, Ann Arbor, MI, 48109-2140, U.S.A.en_US
dc.contributor.affiliationumcampusAnn Arboren_US
dc.description.bitstreamurlhttp://deepblue.lib.umich.edu/bitstream/2027.42/42567/1/10569_2004_Article_5268067.pdfen_US
dc.identifier.doihttp://dx.doi.org/10.1023/B:CELE.0000034503.44164.b5en_US
dc.identifier.sourceCelestial Mechanics and Dynamical Astronomyen_US
dc.owningcollnameInterdisciplinary and Peer-Reviewed


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