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dc.contributor.advisorJohn S. Lewis and Gordon H. Pettengill.en_US
dc.contributor.authorNozette, Stewart Daviden_US
dc.contributor.otherMassachusetts Institute of Technology. Dept. of Earth and Planetary Sciences.en_US
dc.date.accessioned2010-10-12T14:53:50Z
dc.date.available2010-10-12T14:53:50Z
dc.date.copyright1982en_US
dc.date.issued1983en_US
dc.identifier.urihttp://hdl.handle.net/1721.1/59033
dc.descriptionThesis (Ph.D.)--Massachusetts Institute of Technology, Dept. of Earth and Planetary Sciences, 1983.en_US
dc.descriptionMicrofiche copy available in Archives and Scienceen_US
dc.descriptionBibliography: leaves 164-188.en_US
dc.description.statementofresponsibilityby Stewart David Nozette.en_US
dc.format.extent[1], 188 leavesen_US
dc.language.isoengen_US
dc.publisherMassachusetts Institute of Technologyen_US
dc.rightsM.I.T. theses are protected by copyright. They may be viewed from this source for any purpose, but reproduction or distribution in any format is prohibited without written permission. See provided URL for inquiries about permission.en_US
dc.rights.urihttp://dspace.mit.edu/handle/1721.1/7582en_US
dc.subjectEarth and Planetary Sciences.en_US
dc.titleThe physical and chemical properties of the surface of Venusen_US
dc.typeThesisen_US
dc.description.degreePh.D.en_US
dc.contributor.departmentMassachusetts Institute of Technology. Department of Earth and Planetary Sciencesen_US
dc.contributor.departmentMassachusetts Institute of Technology. Department of Earth, Atmospheric, and Planetary Sciences
dc.identifier.oclc11126438en_US


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