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dc.contributor.authorBrenner, Norman Mitchell.en_US
dc.date.accessioned2010-02-09T16:25:54Z
dc.date.available2010-02-09T16:25:54Z
dc.date.copyright1975en_US
dc.date.issued1975en_US
dc.identifier.urihttp://hdl.handle.net/1721.1/51382en_US
dc.descriptionThesis: Ph. D., Massachusetts Institute of Technology, Department of Earth and Planetary Sciences, 1975en_US
dc.descriptionVita.en_US
dc.descriptionBibliography: leaves 53-55.en_US
dc.description.statementofresponsibilityby Norman Brenner.en_US
dc.format.extent92 leavesen_US
dc.publisherMassachusetts Institute of Technologyen_US
dc.rightsMIT theses may be protected by copyright. Please reuse MIT thesis content according to the MIT Libraries Permissions Policy, which is available through the URL provided.en_US
dc.rights.urihttp://dspace.mit.edu/handle/1721.1/7582en_US
dc.subjectEarth and Planetary Sciencesen_US
dc.subject.lcshPlanets Orbits.en_US
dc.subject.lcshCelestial mechanics.en_US
dc.titleThree-dimensional evolution of Mercury's spin-orbit resonanceen_US
dc.typeThesisen_US
dc.description.degreePh. D.en_US
dc.contributor.departmentMassachusetts Institute of Technology. Department of Earth, Atmospheric, and Planetary Sciencesen_US
dc.identifier.oclc02015549en_US
dc.description.collectionPh. D. Massachusetts Institute of Technology, Department of Earth and Planetary Sciencesen_US
dspace.imported2022-02-10T17:46:32Zen_US


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