Abstract
The ultimate origin of water in the Earth’s hydrosphere is in the deep Earth—the mantle. Theory1 and experiments2,3,4 have shown that although the water storage capacity of olivine-dominated shallow mantle is limited, the Earth’s transition zone, at depths between 410 and 660 kilometres, could be a major repository for water, owing to the ability of the higher-pressure polymorphs of olivine—wadsleyite and ringwoodite—to host enough water to comprise up to around 2.5 per cent of their weight. A hydrous transition zone may have a key role in terrestrial magmatism and plate tectonics5,6,7, yet despite experimental demonstration of the water-bearing capacity of these phases, geophysical probes such as electrical conductivity have provided conflicting results8,9,10, and the issue of whether the transition zone contains abundant water remains highly controversial11. Here we report X-ray diffraction, Raman and infrared spectroscopic data that provide, to our knowledge, the first evidence for the terrestrial occurrence of any higher-pressure polymorph of olivine: we find ringwoodite included in a diamond from Juína, Brazil. The water-rich nature of this inclusion, indicated by infrared absorption, along with the preservation of the ringwoodite, is direct evidence that, at least locally, the transition zone is hydrous, to about 1 weight per cent. The finding also indicates that some kimberlites must have their primary sources in this deep mantle region.
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Acknowledgements
D.G.P. acknowledges CERC funding for this study. F.N. is supported by ERC Starting Grant 307322. Support from the Alfred P. Sloan Foundation’s Deep Carbon Observatory project created this research partnership. We thank T. Stachel for comments on the manuscript plus access to the FTIR instrument at the De Beers Laboratory of Diamond Research at the University of Alberta, and we thank J. Harris for discussions. Sample JUc29 was provided by Trigon GeoServices Ltd.
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Contributions
D.G.P. had the idea for the study, wrote the manuscript and helped perform the Raman and FTIR measurements. F.E.B. performed the Raman measurements and ion-milling and made compositional estimates. F.N. performed X-ray measurements. J.M. and L.N. first identified the inclusion as ringwoodite. M.T.H. selected the diamond for this study and assisted with manuscript preparation and geological background. S.M. performed the FTIR measurements and the water content estimate. K.M. assisted with manuscript preparation. G.S., S.S., B.V. and L.V. performed the synchrotron X-ray mapping measurements.
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Extended data figures and tables
Extended Data Figure 1 Image of JUc29 diamond and the ringwoodite-walstromite inclusion.
a, Monochrome image of diamond JUc29 taken under incident light, with the ringwoodite-walstromite inclusion pair highlighted by a red square. The irregular shape and hexagonal pits in the diamond are signs of significant resorption. b, Enlarged view of the area of the host diamond (rotated 90° relative to a) containing the ringwoodite-walstromite inclusion pair. The shadow behind the rectangular area outlining the inclusion pair is probably a stress fracture in the diamond.
Extended Data Figure 2 Three-dimensional confocal μXRF view of two-phase ringwoodite-walstromite inclusion.
Three-dimensional confocal μXRF view of two-phase inclusion within JUc29 diamond, showing Ca (red) and Fe (green) low-intensity isosurfaces for confocal μXRF, with blue representing the diamond host (derived from scatter intensity). Scale bar, 40 μm.
Extended Data Figure 3 Single-crystal X-ray diffraction image showing the main diffraction peaks of ringwoodite.
CCD image collected by a STOE STADI IV single-crystal diffractometer, using monochromatized MoKα radiation (λ = 0.71073 Å), working at 50 kV and 40 mA and with an exposure time of 60 s. The image shows the main four diffraction peaks of ringwoodite (outlined by blue circles and labelled “RINGW” for clarity), that is, the planes (113) at 2.44 Å, (440) at 1.40 Å, (220) at 2.81 Å and (115) at 1.51 Å, in their exact order of expected relative intensity, which is well determined by CCD. The expected fifth peak, at about 2.02 Å, was not found because it is covered by the very intense diamond peak, which occurs at the same d spacing (large and bright peaks in figure). In addition to the ringwoodite diffraction peaks, the main peaks of the host diamond are present as the most intense peaks (labelled ‘diamond’). The characteristic peaks of quartz are evident (labelled ‘quartz’). Secondary quartz crystals occur in resorption pits on the sample surface but quartz is not included within the diamond. The diffraction rings result from clay minerals again present on the surface of the diamond. Finally, at least one diffraction peak, that occurring at 3.03 Å, probably results from CaSiO3-walstromite (labelled ‘walstromite?’).
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Pearson, D., Brenker, F., Nestola, F. et al. Hydrous mantle transition zone indicated by ringwoodite included within diamond. Nature 507, 221–224 (2014). https://doi.org/10.1038/nature13080
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DOI: https://doi.org/10.1038/nature13080
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