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A crystallizing dense magma ocean at the base of the Earth’s mantle


The distribution of geochemical species in the Earth’s interior is largely controlled by fractional melting and crystallization processes that are intimately linked to the thermal state and evolution of the mantle. The existence of patches of dense partial melt at the base of the Earth’s mantle1, together with estimates of melting temperatures for deep mantle phases2 and the amount of cooling of the underlying core required to maintain a geodynamo throughout much of the Earth’s history3, suggest that more extensive deep melting occurred in the past. Here we show that a stable layer of dense melt formed at the base of the mantle early in the Earth’s history would have undergone slow fractional crystallization, and would be an ideal candidate for an unsampled geochemical reservoir hosting a variety of incompatible species (most notably the missing budget of heat-producing elements) for an initial basal magma ocean thickness of about 1,000 km. Differences in 142Nd/144Nd ratios between chondrites and terrestrial rocks4 can be explained by fractional crystallization with a decay timescale of the order of 1 Gyr. These combined constraints yield thermal evolution models in which radiogenic heat production and latent heat exchange prevent early cooling of the core and possibly delay the onset of the geodynamo to 3.4–4 Gyr ago5.

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Figure 1: Schematic illustration of the formation and evolution of a dense basal magma ocean.
Figure 2: Sketch of the idealized model.
Figure 3: Evolution of the preferred model as a function of time.
Figure 4: Predicted element concentrations in the present-day basal magma ocean and solid mantle.


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We thank D. Stevenson for comments that helped us to considerably sharpen this paper. M. Moreira, C. Jaupart and M. Jellinek also provided valuable feedback. This research was supported by the SEDIT programme of INSU, the French Ministry of Research and a CIAR postdoctoral fellowship.

Author Contributions All authors contributed equally to the manuscript.

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Correspondence to S. Labrosse.

Supplementary information

Supplementary Notes

The file contains Supplementary Notes with additional explanations, and in particular the equations for the Sm-Nd evolution, a figure representing the trade-offs between parameters to satisfy the constraints from Nd and a table of parameters used for the model evolution. (PDF 338 kb)

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Labrosse, S., Hernlund, J. & Coltice, N. A crystallizing dense magma ocean at the base of the Earth’s mantle. Nature 450, 866–869 (2007).

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