View Item 

Show simple item record

Stability in the Full Two-Body Problem
dc.contributor.authorScheeres, Daniel J.en_US
dc.date.accessioned2006-09-08T20:28:37Z
dc.date.available2006-09-08T20:28:37Z
dc.date.issued2002-05en_US
dc.identifier.citationScheeres, D. J.; (2002). "Stability in the Full Two-Body Problem." Celestial Mechanics and Dynamical Astronomy 83 (1-4): 155-169. <http://hdl.handle.net/2027.42/42564>en_US
dc.identifier.issn0923-2958en_US
dc.identifier.issn1572-9478en_US
dc.identifier.urihttps://hdl.handle.net/2027.42/42564
dc.description.abstractStability conditions are established in the problem of two gravitationally interacting rigid bodies, designated here as the full two-body problem. The stability conditions are derived using basic principles from the N -body problem which can be carried over to the full two-body problem. Sufficient conditions for Hill stability and instability, and for stability against impact are derived. The analysis is applicable to binary small-body systems such as have been found recently for asteroids and Kuiper belt objects.en_US
dc.format.extent127332 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.otherBinary Asteroidsen_US
dc.subject.otherStabilityen_US
dc.subject.otherN -Body Problemen_US
dc.titleStability in the Full Two-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, Ann Arbor, MI, 48109-2140, U.S.A.en_US
dc.contributor.affiliationumcampusAnn Arboren_US
dc.description.bitstreamurlhttp://deepblue.lib.umich.edu/bitstream/2027.42/42564/1/10569_2004_Article_5088381.pdfen_US
dc.identifier.doihttp://dx.doi.org/10.1023/A:1020143116091en_US
dc.identifier.sourceCelestial Mechanics and Dynamical Astronomyen_US
dc.owningcollnameInterdisciplinary and Peer-Reviewed


Files in this item

Name:
10569_2004_Article_5088381.pdf
Size:
124.3KB
Format:
PDF
View/Open

Show simple item record

Remediation of Harmful Language

The University of Michigan Library aims to describe library materials in a way that respects the people and communities who create, use, and are represented in our collections. Report harmful or offensive language in catalog records, finding aids, or elsewhere in our collections anonymously through our metadata feedback form. More information at Remediation of Harmful Language.

Accessibility

If you are unable to use this file in its current format, please select the Contact Us link and we can modify it to make it more accessible to you.