Warm and Oxidizing Slabs Limit Ingassing Efficiency of Nitrogen to the Mantle

Nitrogen is a major and essential component of Earth’s atmosphere, yet relative to other volatile elements, there are relatively few experimental constraints on the pathways by which nitrogen cycles between Earth’s interior and exterior. We report mineral-melt and mineral-fluid partitioning experiments to constrain the behavior of nitrogen during slab dehydration and sediment melting processes. Experiments reacted rhyolitic melts with silicate and oxide minerals, in the presence of excess aqueous fluid, over temperatures between 725-925 °C and pressures between 0.2 and 2.3 GPa. Oxygen fugacity ranged between iron metal saturation (∼NNO-5) to that in excess of primitive arc basalts (∼NNO+2). Our experiments demonstrate that hydrous fluid is the preferred phase for nitrogen over minerals (biotite, K-feldspar, and amphibole) and rhyolitic melts across all conditions explored. Relatively large effects of pressure (Δlog(DN melt-fluid)/Δ(GPa/K) = 761 ± 68 (1σ), Δlog(DN biolite-fluid)/Δ(GPa/K) = 462 ± 169) and moderate effects of oxygen fugacity (DN melt-fluid)/ΔNNO = -0.20 ± 0.04, Δlog DN biolite-fluid/ΔNNO = -0.10 ± 0.04) modulate partitioning of nitrogen. We further document negligible partitioning effects related to mineral composition or Cl content of hydrous fluid. Of the minerals investigated, biotite has the largest affinity for N and should control the retention of N in slabs where present. Application of partitioning data to slab dehydration PT paths highlights the potential for highly incompatible behavior (DN biolite-fluid 0.1). We find that slab melting is less effective at extracting N from slabs than fluid loss, at least under oxidized conditions (NNO+1). Ultimately, the conditions under which slabs lose fluid strongly affect the distribution of nitrogen between Earth’s interior and exterior.

Colin R.M. Jackson, Elizabeth Cottrell, Ben Andrews, Warm and oxidizing slabs limit ingassing efficiency of nitrogen to the mantle, Earth and Planetary Science Letters, Volume 553, 2021, 116615 abstract

Representative backscatter electron images of (a) CS series experiments (CS_NK_EXP34, P = 0.2 GPa, T = 725 °C, ƒO2 = ΔNNO+0) and (b) PC series experiments (PC_NK_EXP9, P = 0.95 GPa, T = 775 °C, ƒO2 = ΔNNO-0.08). CS series experiments (a) contain a quenched melt (dark), feldspar that grades from Na-rich core to K-rich rims, and relatively small laths of biotite. PC series experiments run with HY3 starting materials (b) contain a quenched melt, laths of biotite, and, in this example, pyroxene. Vesicles of varying size are present throughout all run products. Pt capsule is present in the bottom of the image.