Smectite diagenesis, pore-water freshening, and fluid flow at the toe of the Nankai wedge
Earth and Planetary Science Letters
By: K. M. Brown, D.M. Saffer, and B.A. Bekins
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Abstract
The presence of low-chloride fluids in the lowermost sediments drilled at Ocean Drilling Program Site 808, at the Nankai accretionary wedge, has been considered as prime evidence for long-distance, lateral fluid flow from depth. Here, we re-evaluate the potential role of in situ reaction of smectite (S) to illite (I) in the genesis of this low chloride anomaly. This reaction is known to be occurring at Site 808, with both the S content and S to I ratio in the mixed layer clays decreasing substantially with depth. We show that the bulk of the chloride anomaly can generate by in situ clay dehydration, particularly if pre-reaction smectite abundances (Ai) approach ?? 10-15% of the bulk sediment. The Ai values, however, are not well constrained. At Ai values < 10-15%, an additional source of low-Cl fluid centered close to the de??collement could be required. Thus, there remains the important possibility that the observed low-Cl anomaly is a compound effect of both lateral flow and in situ smectite dehydration. ?? 2001 Elsevier Science B.V. All rights reserved.
Suggested Citation
Brown, K.M., Saffer, D., and Bekins, B., 2001, Smectite diagenesis, pore-water freshening, and fluid flow at the toe of the Nankai wedge: Earth and Planetary Science Letters, v. 194, no. 1-2, p. 97-109, https://doi.org/10.1016/S0012-821X(01)00546-5.
| Publication type | Article |
|---|---|
| Publication Subtype | Journal Article |
| Title | Smectite diagenesis, pore-water freshening, and fluid flow at the toe of the Nankai wedge |
| Series title | Earth and Planetary Science Letters |
| DOI | 10.1016/S0012-821X(01)00546-5 |
| Volume | 194 |
| Issue | 1-2 |
| Year Published | 2001 |
| Language | English |
| Larger Work Type | Article |
| Larger Work Subtype | Journal Article |
| Larger Work Title | Earth and Planetary Science Letters |
| First page | 97 |
| Last page | 109 |