Published May 3, 2021 | Version v1
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Subduction-Driven Volatile Recycling: A Global Mass Balance

  • 1. Marine Chemistry and Geochemistry Department,Woods Hole Oceanographic Institution, Woods Hole, Massachusetts 02543
  • 2. Department of Geosciences, University of Massachusetts, Amherst, Massachusetts 01003, USA
  • 3. Centre de Recherches Pétrographiques et Géochimiques, CNRS UMR 7358, Université de Lorraine, F-54501 Vandoeuvre-lès-Nancy, France
  • 4. Department of Geological Sciences, Jackson School of Geosciences, The University of Texas at Austin, Austin, Texas 78712, USA
  • 5. Nordic Volcanological Center, Institute of Earth Sciences, University of Iceland, Reykjavik, Iceland 600169
  • 6. Géochimie des isotopes stables, Institut de Physique du Globe de Paris, 75238 Paris, France
  • 7. Department of Earth Sciences, University of Oxford, Oxford OX1 3AN, United Kingdom
  • 8. Department of Geology, Middlebury College, Middlebury, Vermont 05753, USA

Description

The model adopted here follows the box-model approach proposed by Barry & Hilton (2016), which considers two main mantle reservoirs represented by the primitive, deep mantle (PLM) sampled by primitive (high 3He/4He) mantle plumes (e.g., OIBs, Yellowstone, Iceland) and the depleted, convecting upper (DMM), notably sampled at mid-ocean ridges. In line with the mass-balance presented in this contribution, the PLM and DMM are taken to represent 10wt.% and 90wt.%, respectively, of the total mass of the mantle. The model is then built on the following assumptions: (1) the N ingassing flux commences at the onset of subduction and is constant through time; (2) a constant proportion of the total N ingassing flux (F) is subducted into each respective mantle reservoir (defined here as FPLM and FDMM) and instantaneously mixes with each reservoir during subduction; (3) the mantle outgassing fluxes from the PLM and DMM reservoirs are constant through time, but may be varied from one simulation to another; (4) the model must produce N contents ([N]) and isotope compositions (δ15N) of the PLM and DMM reservoirs that correspond to present-day observations; and (5) the initial mantle δ15N prior to the onset of subduction is common to the PLM and DMM reservoirs, with a value of either -6‰ (Labidi et al. 2020; Main Text) or -40 ‰ (Barry & Hilton 2016; Supplemental Figure 3). The DMM and PLM reservoirs are considered to have evolved to their current δ15N (-5‰ and +3‰, respectively) and [N] (Tables 1) compositions as a consequence of additions of different amounts of subducted sedimentary N (δ15N = +5 ‰).

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Working paper: 10.1146/annurev-earth-071620-055024 (DOI)