Loading…
Living dead slabs in 3-D: The dynamics of compositionally-stratified slabs entering a “slab graveyard” above the core-mantle boundary
► Slabs tend to rotate to basalt-side down as they sink. ► Slab-CMB interaction is characterised by heating up of the slab followed by separation of the basalt and harzburgite layers. ► Basalt–harzburgite segregation occurs in several different modes depending on the orientation and angle of the sla...
Saved in:
Published in: | Physics of the earth and planetary interiors 2011-10, Vol.188 (3), p.150-162 |
---|---|
Main Author: | |
Format: | Article |
Language: | English |
Subjects: | |
Citations: | Items that this one cites Items that cite this one |
Online Access: | Get full text |
Tags: |
Add Tag
No Tags, Be the first to tag this record!
|
Summary: | ► Slabs tend to rotate to basalt-side down as they sink. ► Slab-CMB interaction is characterised by heating up of the slab followed by separation of the basalt and harzburgite layers. ► Basalt–harzburgite segregation occurs in several different modes depending on the orientation and angle of the slab. ► A preexisting dense layer greatly increases the fraction of basalt that segregates from the slab; dimensionality also matters. ► Plumes form at the edges, sides and interiors of slabs, with depleted plume heads and basalt-entraining plume tails.
Segregation of subducted mid-ocean ridge basalt (MORB) at the CMB has been identified as a potentially important mechanism in the long-term evolution of the mantle and core. Here, three-dimensional (3-D) and two-dimensional (2-D) simulations of a compositionally-stratified slab reaching the CMB are presented, with the goals of characterising the resulting thermo-chemical structures for comparison with seismic studies, and of quantifying the fraction of MORB that is able to segregate and remain near the CMB. Compositional stratification of the slab results in a strong torque due to the relatively high density of basalt and low density of harzburgite, which tends to rotate the slab such that the basalt side faces down. Slab-CMB interaction is characterised by heating up of the slab followed by separation of the basalt and harzburgite layers, with harzburgite rising in vigorous plumes. Plumes form at the edges and sides of slabs at the CMB as well as in their interiors (as previously observed for purely thermal slabs) with plume heads dominated by depleted harzburgitic material (sometimes with small amounts of entrained basalt), while plume tails entrain basaltic material. Segregation of basalt depends strongly on the presence or absence of a preexisting dense layer at the CMB and by dimensionality. A preexisting dense layer greatly increases the fraction of basalt that segregates from the slab: in 3-D this fraction is in the range 0.5–0.7 with a layer present compared to 0.25–0.45 with no preexisting layer. Two modes of basalt segregation are observed for slabs that land basalt side-up (i) hot harzburgite extruding from the sides and edges and (ii) hot, harzburgite-rich plumes bursting through the basalt layer (as previously observed in laboratory experiments), whereas for a slab that lands basalt side down (iii) hot basalt can peel off from its underside, displaying fingering instabilities in 3-D. Furthermore, basalt |
---|---|
ISSN: | 0031-9201 1872-7395 |
DOI: | 10.1016/j.pepi.2011.04.013 |