The influence of a chemical boundary layer on the fixity, spacing and lifetime of mantle plumes

Abstract

Seismological observations provide evidence that the lowermost mantle contains superposed thermal and compositional boundary layers¹ that are laterally heterogeneous^2,3. Whereas the thermal boundary layer forms as a consequence of the heat flux from the Earth's outer core, the origin of an (intrinsically dense) chemical boundary layer remains uncertain⁴. Observed zones of ‘ultra-low’ seismic velocity⁵ suggest that this dense layer may contain metals^6,7 or partial melt⁸, and thus it is reasonable to expect the dense layer to have a relatively low viscosity. Also, it is thought that instabilities in the thermal boundary layer could lead to the intermittent formation and rise of mantle plumes. Flow into ascending plumes can deform the dense layer, leading, in turn, to its gradual entrainment^{9,10,11,12,13,14}. Here we use analogue experiments to show that the presence of a dense layer at the bottom of the mantle induces lateral variations in temperature and viscosity that, in turn, determine the location and dynamics of mantle plumes. A dense layer causes mantle plumes to become spatially fixed, and the entrainment of low-viscosity fluid enables plumes to persist within the Earth for hundreds of millions of years.