Rotation Axis Variation Due To Spin Orbit Resonance

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dc.creatorGallavotti, Giovannni
dc.date1993-08-22
dc.date.accessioned2026-07-07T09:07:39Z
dc.date.available2026-07-07T09:07:39Z
dc.descriptionRotation axis variation due to spin orbit resonance: conference report; keywords: planetary precession, rigid body, chaos, KAM, Arnold diffusion, averaging, celestial mechanics, classical mechanics, large deviations
dc.description3 pages; e-mail gallavotti%40221.hepnet@lbl.gov
dc.identifierhttps://arxiv.org/abs/chao-dyn/9308006
dc.identifierhttp://arxiv.org/abs/chao-dyn/9308006
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/150448
dc.subjectChaotic Dynamics
dc.titleRotation Axis Variation Due To Spin Orbit Resonance
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