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Journal ArticleDOI

The serpentinite multisystem revisited : chrysotile is metastable

Bernard W. Evans
- 01 Jun 2004 - 
- Vol. 46, Iss: 6, pp 479-506
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TLDR
The two polymorphs of serpentine Mg3Si2O5(OH)4, lizardite and chrysotile, occur in nature in virtually identical ranges of temperature and pressure, from surficial or near-surficial environments to temperatures perhaps as high as 400°C.
Abstract
The two rock-forming polymorphs of serpentine Mg3Si2O5(OH)4, lizardite and chrysotile, occur in nature in virtually identical ranges of temperature and pressure, from surficial or near-surficial environments to temperatures perhaps as high as 400°C. Laboratory evidence indicates that lizardite is the more stable at low temperatures, but the difference in their Gibbs free energies is not more than about 2 kJ in the 300-400°C range. Above about 300°C, antigorite + brucite is more stable than both; in other words, chrysotile is nowhere the most stable. The crystal structures of lizardite and chrysotile give rise to contrasting crystallization behaviors and hence modes of occurrence. The hydration of peridotite at low temperature results in the growth of lizardite from olivine, and (commonly topotactically) from chain and sheet silicates, although the MgO-SiO2-H2O (MSH) phase diagram predicts antigorite + talc in bastite. The activity of H2O during serpentinization may be buffered to low values by the solids,...

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Citations
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An improved and extended internally consistent thermodynamic dataset for phases of petrological interest, involving a new equation of state for solids

TL;DR: In this paper, the Tait equation of state (TEOS) was used to model the temperature dependence of both the thermal expansion and bulk modulus in a consistent way, which has led to improved fitting of the phase equilibrium experiments.
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H2-rich fluids from serpentinization: Geochemical and biotic implications

TL;DR: The catalytic properties of FeNi3 allow complex organic compounds to form within serpentinite and, when mixed with atmospherically produced complex organic matter and waters that circulated through basalts, constitutes an attractive prebiotic substrate.
Journal ArticleDOI

On Silica Activity and Serpentinization

TL;DR: 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 this paper.
Journal ArticleDOI

Common depth of slab-mantle decoupling: Reconciling diversity and uniformity of subduction zones

TL;DR: In this article, the authors developed numerical thermal models with a nonlinear mantle rheology for seventeen subduction zones, spanning a large range of slab age, descent rate, and geometry.
Journal ArticleDOI

Unraveling the sequence of serpentinization reactions: petrography, mineral chemistry, and petrophysics of serpentinites from MAR 15°N (ODP Leg 209, Site 1274)

TL;DR: Bach et al. as discussed by the authors proposed that low-fluid-flux serpentinization of olivine to serpentine and ferroan brucite is followed by later stages of serpentinisation under more open-system conditions and formation of magnetite by the breakdown of ferro-an Brucite.
References
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Book

The techniques of modern structural geology

TL;DR: In this paper, Geologie and Analyse des contraintes were used to analyze the fissuration reference record of the Fissuration Reference Record created on 2004-09-07, modified on 2016-08-08.
Journal ArticleDOI

Coesite and pure pyrope in high-grade blueschists of the Western Alps: a first record and some consequences

TL;DR: A pyrope-quartzite originally described by Vialon (1966) from the Dora Maira massif was resampled and reinvestigated in this article, showing that the whole matrix has once been coesite.
Journal ArticleDOI

Serpentine Stability to Mantle Depths and Subduction-Related Magmatism

Peter Ulmer, +1 more
- 12 May 1995 - 
TL;DR: Results of high-pressure experiments on samples of hydrated mantle rocks show that the serpentine mineral antigorite is stable to ∼720�C at 2 gigapascals, to ∼690 �C at 3 gigapascalals, and to ∼620�C to 5 gigapASCals.
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