South-Central - 38th Annual Meeting (March 15–16, 2004)
Paper No. 11-9
Presentation Time: 4:20 PM-4:40 PM

THE INFLUENCE OF PRESSURE AND MINERALOGY ON SEISMIC VELOCITIES IN OCEANIC GABBROS: IMPLICATIONS FOR THE COMPOSITION AND STATE OF THE LOWER OCEANIC CRUST

CARLSON, R.L., Geology & Geophysics, Texas A&M Univ, 3115 TAMU, College Station, TX 77843-3115, carlson@geo.tamu.edu and MILLER, D.J., Ocean Drilling Program and Department of Geology & Geophysics, Texas A&M Univ, 3115 TAMU, College Station, TX 77843, miller@odpemail.tamu.edu

We have analyzed the relationship between P-wave velocities, measured at pressures of 40, 100, and 200 MPa, and modal mineralogy in oceanic gabbro samples from ODP Holes 735B, 894G, and 923A. At all pressures, velocities increase with increasing pyroxene content and decreasing alteration (phyllosilicate and amphibole content), but not with increasing olivine content. A Voigt-Reuss-Hill inverse model reveals that the effective bulk densities and elastic moduli of the plagioclase, pyroxene and amphibole phases are near their expected values, but the effective bulk density and elastic moduli of olivine in the gabbros are anomalously low, probably because the olivine is iron rich, and/or because the olivine grains contain ubiquitous networks of cracks. On average, gabbros with velocities typical of seismic layer 3 (6.7 to 7.0 km s-1) contain 5-15% alteration products, including 5-15% amphibole and 0-5% phyllosilicates. These results suggest that the lower crust is slightly to moderately altered. However, total alteration of the lower oceanic crust could be as low as 2%, if the lower crustal gabbros contain abundant olivine grains that have low densities and elastic moduli.

South-Central - 38th Annual Meeting (March 15–16, 2004)
General Information for this Meeting
Session No. 11
Topics in Tectonics and Structure
Texas A&M University: Geology Builiding, Room 101
1:00 PM-5:00 PM, Tuesday, March 16, 2004

Geological Society of America Abstracts with Programs, Vol. 36, No. 1, p. 28

© Copyright 2004 The Geological Society of America (GSA), all rights reserved. Permission is hereby granted to the author(s) of this abstract to reproduce and distribute it freely, for noncommercial purposes. Permission is hereby granted to any individual scientist to download a single copy of this electronic file and reproduce up to 20 paper copies for noncommercial purposes advancing science and education, including classroom use, providing all reproductions include the complete content shown here, including the author information. All other forms of reproduction and/or transmittal are prohibited without written permission from GSA Copyright Permissions.