Ultraslow, slow, or fast spreading ridges: an interplay between plate tectonics and mantle convection
Abstract
Oceanic spreading rates are highly variable. These variations are known to correlate to a variety of surface observables,
like magmatic production, heat flow or bathymetry, which lead to classify ridges into fast and slow spreading
ridges, but also as the more peculiar ultraslow spreading regime. Here we explore the dynamic relationships between
spreading ridges, plate tectonics and mantle flow. For this, we first focus on the thermal signature at deeper
levels that we infer from the global S-wave seismic tomography model of Debayle and Ricard (2012). We show
that the thermal structure of ridges gradually departs from the half-space cooling model for slow, and above all
ultraslow spreading ridges. We also infer that the sub- lithospheric mantle temperature decreases by more than
180K from fast spreading to ultraslow spreading regimes. Both observations indicate that the mantle convection
pattern is increasingly altered underneath slow and ultraslow spreading ridges. We suggest that this is due to farfield
tectonics on the other ends of lithospheric plates. Not only it modulates the spreading rates but it also alters
the convection regime: collisions at active plate boundaries obstruct plate motion and decrease their velocities. We
then test this hypothesis using a thermo-mechanical model that represents a convection cell carrying a positively
buoyant continental lithosphere on top. The continent gradually drifts away from the spreading ridge, from which
the oceanic lithosphere grows and cools while the continent eventually collides at the opposite side. In turn, this
event drastically modifies the upper kinematic condition for the convecting mantle that evolves from a mobile lid
regime to an almost stagnant lid regime. Implications on spreading ridges are prominent: heat advection is slower
than thermal diffusion, which causes the oceanic lithosphere to thicken faster; the oceanic plates get compressed
and destabilized by a growing number of small scale transient plumes, which disrupts the structure of the oceanic
lithospheres, lowers the heat flow and may even starve ultraslow ridges from partial melting.