Abstract

Water content plays a vital role in determining mantle rheology and thus mantle convection and plate tectonics. Most parameterised convection models predict that Earth initially underwent a period of rapid degassing and heating, followed by a slow and sustained period of regassing and cooling. However, these models assume water is instantaneously mixed and homogeneously distributed into the mantle. This is a limitation because the mixing time for water entering and leaving the mantle is a function of the Rayleigh number which varies dramatically with water content, temperature, and through time. Here we present an adapted parametrised model (Crowley et al., 2011) to include the coupled effects of the time scale of mixing with a water-dependent viscosity. We consider two mixing types: first, where the mixing time is constant throughout the model and second, where mixing time varies as a response to an evolving Rayleigh number. We find that, facilitated by the effects of water content in the melt region at mid-ocean ridges, a constant mixing time can induce long periods of degassing. The inclusion of a variable mixing time dependent on the Rayleigh number acts to limit the period of degassing and also results in more water being stored in the mantle and less at the surface than in both the constant and instantaneous mixing cases. Mixing time cannot be more than ∼2 billion years as large mixing times trap water in the mantle, leaving a dry surface. Even small changes in the surface ocean induced by mixing times on the order of 0.1 Gyrs can cause changes in the global-mean sea level on the order of 10's of metres. These changes in sea level could easily uncover topographic highs in the bathymetry, potentially aiding sub-aerial erosion a process thought to be important in early Earth evolution. Even in this relatively simple model, the inclusion of a mixing time between water entering and leaving the mantle creates a more dynamic water cycle.

Highlights

  • Viscosity is the determinant physical property in the thermal evolution of the mantle, dependent on many parameters including temperature, pressure and grain size but the effect of water is currently undergoing investigation

  • Running models to 9 Gyrs ensures that we capture behaviour of the system until it reaches a steady state. Both the thermal evolution and water cycle can be in two states, depending on whether the input or output of the system is dominant

  • The water cycle can be in a state of net regassing where R > D or net degassing where R < D

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Summary

Introduction

Viscosity is the determinant physical property in the thermal evolution of the mantle, dependent on many parameters including temperature, pressure and grain size but the effect of water is currently undergoing investigation. Parametrised studies have shown a water-dependent viscosity initially produces a period of heating and a state of net degassing (where degassing at mid-ocean ridges, MORs, exceeds regassing at subduction zones), followed by a long and sustained period of cooling and a state of net regassing (Crowley et al, 2011; Sandu et al, 2011). This is due to the rapidly decreasing water content increasing the viscosity, trapping heat and causing the temperature to build up.

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