Jerry X. Mitrovica

A resonance in the Earth's obliquity and precession over the past 20 Myr driven by mantle convection

The motion of the Solar System is chaotic to the extent that the precise positions of the planets are predictable for a period of only about 20 Myr (ref. 1). The Earths precession, obliquity and insolation parameters over this time period can be influenced by secular variations in the dynamic ellipticity of the planet which are driven by long-term geophysical processes, such as post-glacial rebound,. Here we investigate the influence of mantle convection on these parameters. We use viscous flow theory to compute time series of the Earths dynamic ellipticity for the past 20 Myr and then apply these perturbations to the nominal many-body orbital solution of Laskar et al.. We find that the convection-induced change in the Earths flattening perturbs the main frequency of the Earths precession into the resonance associated with a secular term in the orbits of Jupiter and Saturn, and thus significantly influences the Earths obliquity. We also conclude that updated time series of high-latitude summer solar insolation diverge from the nominal solution for periods greater than the past ∼5 Myr. Our results have implications both for obtaining precise solutions for precession and obliquity and for procedures that adopt astronomical calibrations to date sedimentary cycles and climatic proxy records.