Abstract

The formation of new ocean crust at mid-ocean ridges is a fundamental component of the plate tectonic cycle and involves substantial transfer of heat and mass from the mantle. Hydrothermal circulation at mid-ocean ridges is critical for the advection of latent and sensible heat from the lower crust to enable the solidification of ocean crust near to the ridge axis. The sheeted dike complex (SDC) is the critical region between the eruptive lavas and the gabbros through which seawater-derived recharge fluids must transit to exchange heat with the magma chambers that form the lower ocean crust.ODP Hole 1256D in the eastern equatorial Pacific Ocean provides the only continuous sampling of in-situ intact upper ocean crust formed at a fast spreading rate, through the SDC into the dike–gabbro transition zone. Here we exploit a high sample density profile of the Sr-isotopic composition of Hole 1256D to quantify the time-integrated hydrothermal recharge fluid flux through the SDC. Assuming kinetically limited fluid–rock Sr exchange, a fluid flux of 1.5–3.2×106 kgm−2 is required to produce the observed Sr-isotopic shifts. Despite significant differences in the distribution and intensity of hydrothermal alteration and fluid/rock Sr-isotopic exchange between Hole 1256D and SDC sampled in other oceanic environments (ODP Hole 504B, Hess Deep and Pito Deep), the estimated recharge fluid fluxes at all sites are similar, suggesting that the heat flux extracted by the upper crustal axial hydrothermal system is relatively uniform at intermediate to fast spreading rates.The hydrothermal heat flux removed by fluid flow through the SDCs, is sufficient to remove only ∼20 to 60% of the available latent and sensible heat from the lower crust. Consequently, there must be additional thermal and chemical fluid–rock exchange deeper in the crust, at least of comparable size to the upper crustal hydrothermal system. Two scenarios are proposed for the potential geometry of this deeper hydrothermal system. The first requires the downward expansion of the upper crustal hydrothermal system ∼800 m into the lower crust in response to a downward migrating conductive boundary layer. The second scenario invokes a separate hydrothermal system in the lower crust for which fluid recharge bypasses reaction with the sheeted dikes, perhaps via flow down faults.

Highlights

  • Hydrothermal circulation is a key process in the formation and evolution of the ocean crust and impacts the broader Earth system through the modification of seawater chemistry and the subduction of altered ocean crust (Kelemen and Manning, 2015; Palmer and Edmond, 1989)

  • Our high sampling density allows us to evaluate the potential variability in the fluid flux and Damköhler number that are associated with the different alteration regimes (1.5–3.2 × 106 kg m−2 and N D = 0.16–0.44, respectively; Fig. 3; Table 2), confirming that fluid/rock reaction is heterogeneous within the Hole 1256D sheeted dikes, variations are relatively minor

  • We propose two possible scenarios for the geometry of this hydrothermal system that are thermally viable to make predictions of the anticipated 87Sr/86Sr profile of Hole 1256D when it is extended into cumulate gabbros: (1) a larger upper crustal hydrothermal system that extends down into the lower crust; and (2) the presence of a separate hydrothermal system in the lower crust for which recharge fluids have by-passed reaction with the sheeted dikes (Fig. 8)

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Summary

Introduction

Hydrothermal circulation is a key process in the formation and evolution of the ocean crust and impacts the broader Earth system through the modification of seawater chemistry and the subduction of altered ocean crust (Kelemen and Manning, 2015; Palmer and Edmond, 1989). Hydrothermal circulation is intimately involved in the magmatic accretion of new crust through the advection of sensible and latent heat (e.g., Kelemen et al, 1997). Knowledge of the hydrothermal fluid fluxes and pathways through the crust are crucial to understanding the size, shape and distribution of magma bodies, and the processes of magma emplacement during the accretion of the ocean crust in the axial region. ∼30% of the hydrothermal heat flux is advected from crust less than 1 million years old (Stein and Stein, 1994). In the axial region the magmatic heat released during the formation of the lower crust drives high-temperature (up to ∼400 ◦C)

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