Tidal dissipation by solid friction and the resulting orbital evolution

Dissipation of tidal energy in the earth's mantle and the moon was calculated assuming a dissipation factor 1/ Q constant throughout both bodies. In the mantle the dissipation varies from about 2 × 10 −6 / Q erg cm −3 sec −1 near the pole at the bottom of the mantle to about 0.02 × 10 −6 / Q erg …