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dc.contributor.author Yoder, C.F. en_US
dc.date.accessioned 2004-10-03T05:08:26Z
dc.date.available 2004-10-03T05:08:26Z
dc.date.issued 1995 en_US
dc.identifier.citation ICARUS en_US
dc.identifier.clearanceno 95-1119 en_US
dc.identifier.uri http://hdl.handle.net/2014/31439
dc.description.abstract The predicted orientation of Venus' rotation axis relative to its orbit can be uniquely determined given knowledge of its J2 gravity coefficient and polar moment of inertia C if its free obliquity is fully damped. This assumption seems warranted given the dominant damping mechanism: turbulent fluid friction at a core mantle boundary. The determination of the free obliquity is examined. en_US
dc.format.extent 3508522 bytes
dc.format.mimetype application/pdf
dc.language.iso en_US
dc.subject.other Venus free obliquity rotation axis planetary geophysics en_US
dc.title Venus' Free Obliquity en_US


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