Physics
Scientific paper
Oct 2011
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2011epsc.conf.1882w&link_type=abstract
EPSC-DPS Joint Meeting 2011, held 2-7 October 2011 in Nantes, France. http://meetings.copernicus.org/epsc-dps2011, p.1882
Physics
Scientific paper
This talk will review our ideas concerning the origin and evolution of planetary obliquities, i.e. the tilt of a planet's spin axis to it's orbit pole. Processes that affect the obliquity include impacts during planet formation, tidal dissipation, atmospheric torques, spin axis precession, orbital variations and spin-orbit resonances. Each planet has a unique history involving how these various mechanisms come into play. I will attempt to outline the main elements of these histories for each planet in the solar system.
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