The deformational properties of a terrestrial planetary mantle including mantle elastic moduli and viscosity determine planetary deformation in response to forcings. A forcing can have vastly different sets of time-scales ranging from seconds as in seismic wave propagation (e.g., Dziewonski & Anderson, 1981) to a day as for tides (e.g., Longman, 1966). In addition, there are even longer relevant time scales such as months or years as for post-seismic deformation (e.g., Nur & Mavko, 1974), tens of thousands of years as for glacial isostatic adjustment (GIA) (e.g., Peltier, 1976),millions of years as for long-term tectonic and mantle dynamic forcing of volcanic building (e.g., Watts, 2001) and mantle convection (e.g., Schubert et al., 2001), and possibly billions of years of tidal-rotational forcing due to planetary orbit changes (e.g., Qin et al., 2018). Depending on the time-scale of a forcing, the mantle may respond differently and display purely elastic, viscoelastic, and purely viscous