Skip Navigation



Journal of Petrology Advance Access published online on May 28, 2007

Journal of Petrology, doi:10.1093/petrology/egm021
This Article
Right arrow Full Text Freely available
Right arrow FREE Full Text (PDF) Freely available
Right arrowOA All Versions of this Article:
48/7/1351    most recent
egm021v1
Right arrow Alert me when this article is cited
Right arrow Alert me if a correction is posted
Services
Right arrow Email this article to a friend
Right arrow Similar articles in this journal
Right arrow Alert me to new issues of the journal
Right arrow Add to My Personal Archive
Right arrow Download to citation manager
Google Scholar
Right arrow Articles by Frost, B. R.
Right arrow Articles by Beard, J. S.
Right arrow Search for Related Content
GeoRef
Right arrow GeoRef Citation
Social Bookmarking
 Add to CiteULike   Add to Connotea   Add to Del.icio.us  
What's this?

© 2007 The Author(s)
This is an Open Access article distributed under the terms of the Creative Commons Attribution Non-Commercial License (http://creativecommons.org/licenses/by-nc/2.0/uk/) which permits unrestricted non-commercial use, distribution, and reproduction in any medium, provided the original work is properly cited.

On Silica Activity and Serpentinization

B. Ronald Frost1,* and James S. Beard2

1Department of Geology and Geophysics, University of Wyoming, Laramie, WY 82072, USA
2Virginia Museum of Natural History, 21 Starling Avenue, Martinsville, VA 24112, USA

Received October 3, 2006; Revised typescript accepted March 29, 2007


   Abstract

Serpentinites have the lowest silica activity of common crustal rocks. At the serpentinization front, where olivine, serpentine, and brucite are present, silica activities (relative to quartz) are of the order of 10–2·5 to 10–5, depending on the temperature. Here we argue that this low silica activity is the critical property that produces the unusual geochemical environments characteristic of serpentinization. The formation of magnetite is driven by the extraction of silica from the Fe3Si2O5(OH)4 component of serpentine, producing extremely reducing conditions as evinced by the rare iron alloys that partially serpentinized peridotites contain. The incongruent dissolution of diopside to form Ca2+, serpentine, and silica becomes increasingly favored at lower T, producing the alkalic fluids characteristic of serpentinites. The interaction of these fluids with adjacent rocks produces rodingites, and we argue that desilication is also part of the rodingite-forming process. The low silica activity also explains the occurrence of low-silica minerals such as hydrogrossular, andradite, jadeite, diaspore, and corundum in serpentinites or rocks adjacent to serpentinites. The tendency for silica activity to decrease with decreasing temperature means that the presence of certain minerals in serpentinites can be used as indicators of the temperature of serpentinization. These include, with decreasing temperature, diopside, andradite and diaspore. Because the assemblage serpentine + brucite marks the lowest silica activity reached in most serpentinites, the presence and distribution of brucite, which commonly is a cryptic phase in serpentinites, is critical to interpreting the processes that lead to the hydration of any given serpentinite.

KEY WORDS: serpentinization; serpentinites; silica activity; oxygen fugacity; rodingites; magnetization of serpentinites


*Corresponding author. 307-766-4290. 307-766-6679. rfrost{at}uwyo.edu


Add to CiteULike CiteULike   Add to Connotea Connotea   Add to Del.icio.us Del.icio.us    What's this?


This article has been cited by other articles:


Home page
American MineralogistHome page
B. W. Evans, S. M. Kuehner, and A. Chopelas
Magnetite-free, yellow lizardite serpentinization of olivine websterite, Canyon Mountain complex, N.E. Oregon
American Mineralogist, November 1, 2009; 94(11-12): 1731 - 1734.
[Abstract] [Full Text] [PDF]


Home page
J PetrologyHome page
T. Morishita, K. Hara, K. Nakamura, T. Sawaguchi, A. Tamura, S. Arai, K. Okino, K. Takai, and H. Kumagai
Igneous, Alteration and Exhumation Processes Recorded in Abyssal Peridotites and Related Fault Rocks from an Oceanic Core Complex along the Central Indian Ridge
J. Petrology, July 1, 2009; 50(7): 1299 - 1325.
[Abstract] [Full Text] [PDF]


Home page
Economic GeologyHome page
A. H. Ahmed, S. Arai, and M. Ikenne
Mineralogy and Paragenesis of the Co-Ni Arsenide Ores of Bou Azzer, Anti-Atlas, Morocco
Economic Geology, March 1, 2009; 104(2): 249 - 266.
[Abstract] [Full Text] [PDF]


Home page
J PetrologyHome page
J. S. Beard, B. R. Frost, P. Fryer, A. McCaig, R. Searle, B. Ildefonse, P. Zinin, and S. K. Sharma
Onset and Progression of Serpentinization and Magnetite Formation in Olivine-rich Troctolite from IODP Hole U1309D
J. Petrology, March 1, 2009; 50(3): 387 - 403.
[Abstract] [Full Text] [PDF]


Home page
J PetrologyHome page
F. Klein and W. Bach
Fe-Ni-Co-O-S Phase Relations in Peridotite-Seawater Interactions
J. Petrology, January 1, 2009; 50(1): 37 - 59.
[Abstract] [Full Text] [PDF]


Home page
J PetrologyHome page
L. Pelletier, F. Vils, A. KALT, and K. Gmeling
Li, B and Be Contents of Harzburgites from the Dramala Complex (Pindos Ophiolite, Greece): Evidence for a MOR-type Mantle in a Supra-subduction Zone Environment
J. Petrology, December 4, 2008; (2008) egn057v1.
[Abstract] [Full Text] [PDF]


Home page
J PetrologyHome page
B. W. Evans
Control of the Products of Serpentinization by the Fe2+Mg-1 Exchange Potential of Olivine and Orthopyroxene
J. Petrology, October 16, 2008; (2008) egn050v1.
[Abstract] [Full Text] [PDF]


Home page
J PetrologyHome page
B. R. Frost, J. S. Beard, A. McCaig, and E. Condliffe
The Formation of Micro-Rodingites from IODP Hole U1309D: Key To Understanding the Process of Serpentinization
J. Petrology, September 1, 2008; 49(9): 1579 - 1588.
[Abstract] [Full Text] [PDF]



Disclaimer: Please note that abstracts for content published before 1996 were created through digital scanning and may therefore not exactly replicate the text of the original print issues. All efforts have been made to ensure accuracy, but the Publisher will not be held responsible for any remaining inaccuracies. If you require any further clarification, please contact our Customer Services Department.