Fluid flow through seamounts and implications for global mass fluxes

  1. Robert N. Harris1,
  2. Andrew T. Fisher2 and
  3. David S. Chapman3
  1. 1Department of Geology and Geophysics, University of Utah, Salt Lake City, Utah 84102, USA
  2. 2Earth Sciences Department, University of California, Santa Cruz, California 95064, USA
  3. 3Department of Geology and Geophysics, University of Utah, Salt Lake City, Utah 84102, USA

    Abstract

    Seamounts contribute to globally significant hydrothermal fluxes, but the dynamics and impacts of fluid flow through these features are poorly understood. Numerical models of coupled heat and fluid flow illustrate how seamounts induce local convection in the oceanic crust. We consider idealized axisymmetric seamounts and calculate mass and heat fluxes by using a coupled heat- and fluid-flow model. By using P. Wessel's global database of ∼15,000 seamounts identified through satellite gravimetry, we estimate that the mass flux associated with seamounts is ∼1014 kg/yr, a number comparable to estimated regional mass fluxes through mid-ocean ridges and flanks. In addition, the seamount-generated advective heat flux may be locally significant well beyond the 65 Ma average age at which advective lithospheric heat loss on ridge flanks ends. These flows may be important for facilitating geochemical exchange between the crust and ocean and may affect subseafloor microbial ecosystems.

    Footnotes

    • GSA Data Repository item 2004118, Figure DR1, normalized mass flux as a function of seamount aspect ratio and horizontal permeability, is available online at www.geosociety.org/pubs/ft2004.htm, or on request from editinggeosociety.org or Documents Secretary, GSA, P.O. Box 9140, Boulder, CO 80301-9140, USA.

      • Accepted May 4, 2004.
      • Received December 3, 2003.
      • Revision received April 29, 2004.
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