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A Correction to the Earth's Obliquity Rate

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dc.contributor.author Williams, J. en_US
dc.date.accessioned 2004-10-06T02:19:07Z
dc.date.available 2004-10-06T02:19:07Z
dc.date.issued 1993-05-13 en_US
dc.identifier.citation Santa Barbara, California, USA en_US
dc.identifier.clearanceno 93-0774 en_US
dc.identifier.uri http://hdl.handle.net/2014/35204
dc.description.abstract In the standard IAU theory for the orientation of the Earth's equator, the secular obliquity rate arises solely from the motiion of the ecliptic, not from the motion of the equator in space. en_US
dc.format.extent 65455 bytes
dc.format.mimetype application/pdf
dc.language.iso en_US
dc.subject.other secular obliquity rate Earth planetary perturbations en_US
dc.title A Correction to the Earth's Obliquity Rate en_US


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