Interaction of sea water and lava during submarine eruptions at mid-ocean ridges

Michael R. Perfit (), Johnson R. Cann, Daniel J. Fornari, Jennifer Engels, Deborah K. Smith, W. Ian Ridley and Margo H. Edwards
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Michael R. Perfit: University of Florida
Johnson R. Cann: University of Leeds
Daniel J. Fornari: Woods Hole Oceanographic Institution, Geology and Geophysics Department
Jennifer Engels: University of Hawaii at Manoa
Deborah K. Smith: Woods Hole Oceanographic Institution, Geology and Geophysics Department
W. Ian Ridley: Mineral Resources Team
Margo H. Edwards: University of Hawaii at Manoa

Nature, 2003, vol. 426, issue 6962, 62-65

Abstract: Abstract Lava erupts into cold sea water on the ocean floor at mid-ocean ridges (at depths of 2,500 m and greater), and the resulting flows make up the upper part of the global oceanic crust1. Interactions between heated sea water and molten basaltic lava could exert significant control on the dynamics of lava flows and on their chemistry. But it has been thought that heating sea water at pressures of several hundred bars cannot produce significant amounts of vapour2,3,4,5 and that a thick crust of chilled glass on the exterior of lava flows minimizes the interaction of lava with sea water. Here we present evidence to the contrary, and show that bubbles of vaporized sea water often rise through the base of lava flows and collect beneath the chilled upper crust. These bubbles of steam at magmatic temperatures may interact both chemically and physically with flowing lava, which could influence our understanding of deep-sea volcanic processes and oceanic crustal construction more generally6. We infer that vapour formation plays an important role in creating the collapse features that characterize much of the upper oceanic crust and may accordingly contribute to the measured low seismic velocities in this layer.

Date: 2003
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DOI: 10.1038/nature02032

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