Abstract

Deep-sea sediments have become an important new type of rare-earth element (REY) resources that have high potential to meet the increasing demand. However, the enrichment mechanisms of such deposits remain unclear. In this paper, we made a detailed discussion in bulk-sample geochemistry along the core profile of GC26 collected at the western Pacific Ocean. Elements are classified into lithophile-, phosphate-, and metal oxide elements, which have affinities to silicate, phosphate, and Fe–Mn (oxyhydr)oxide phases in sediments, respectively. Biophosphate is the major host of REY in deep-sea sediments. Its accumulation has a substantial effect on bulk-sample strontium isotopes, but a weak effect on bulk neodymium isotopes. Although the bulk neodymium isotopes imply there was a slight change in sedimentary provenances, it cannot explain the different behaviors of the three elemental groups simultaneously. Water-rock interactions at high temperature enlighten us that water–sediment interactions at low temperature, also known as early diagenesis, may be the answer of behaviors of the three element groups. Silicate dissolution during early diagenesis releases elements from the silicate lattice. When biophosphate accumulation occurs, the released phosphate elements (including REY) are preferentially incorporated into biophosphate rather than being released into seawater, which is the key to REY enrichment in deep-sea sediments. This is also the case for metal oxide elements (e.g., Mn, Co, and Ni) when oxygen fugacity is high enough to cause Fe–Mn (oxyhydr)oxide deposition as coatings or micro-nodules. Considerable amounts of silicate elements (e.g., Al, Ti, Fe, Cr, and V) are released into seawater to participate into global oceanic element cycle if they are less compatible in newly formed secondary silicate components (e.g., phillipsite). Our results provide new insights into the importance of early diagenesis of deep-sea sediments to REY enrichment and the global oceanic elemental budget.

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