Full length ArticleInfluence of temperature, pressure, and fluid salinity on the distribution of chlorine into serpentine minerals
Introduction
Serpentinization, a hydrothermal alteration of ultramafic rocks (typically peridotite and komatiite) at relatively low temperatures (≤500 °C), produces serpentine minerals, (±) brucite, (±) talc, and (±) magnetite. Serpentinization occurs at various geological settings, including the ocean floor, mid-ocean ridges, and subduction zones (e.g., Charlou et al., 1996, Charlou et al., 2000, Maekawa et al., 2001, Hyndman and Peacock, 2003, Mével, 2003, Evans et al., 2013). Serpentinization greatly modifies chemical and physical properties of the oceanic lithosphere (e.g., Escartín et al., 1997, Escartín et al., 2001, Scambelluri et al., 1995, Mével, 2003, Guillot and Hattori, 2013). Serpentinites (with >90% serpentine) have a dramatically lower density compared to primary peridotites, whereas serpentinites have magnetic susceptibility around one to two orders of magnitude higher (Mével, 2003, Evans et al., 2013). As suggested by deformation experiments, a very low degree of serpentinization can greatly decrease the strength of olivine (Escartín et al., 1997, Escartín et al., 2001). Analyses of natural serpentinites show that serpentine minerals can incorporate not only water (up to 13.5 wt%) but also chlorine and fluid-mobile elements, such as Cs, Ba, and Sr (Scambelluri et al., 1995, Hattori and Guillot, 2003, Deschamps et al., 2012, Guillot and Hattori, 2013). Compared to fresh peridotite (with <30 ppm Cl), serpentinites have around one to two orders of magnitude higher chlorine (e.g., Bonifacie et al., 2008, Barnes and Straub, 2010). Thermodynamic and experimental studies suggest that serpentine minerals can be stable at depths of greater than 200 km (Ulmer and Trommsdorff, 1995, Schmidt and Poli, 1998). Therefore, serpentinization may play a significant role for the transfer of H2O, chlorine, and fluid-mobile elements into the mantle.
In spite of the importance, the mechanisms that control the incorporation of chlorine into serpentine minerals still remain poorly understood (Rucklidge, 1972, Rucklidge and Patterson, 1977, Anselmi et al., 2000, Scambelluri et al., 2004, Sharp and Barnes, 2004, Barnes and Sharp, 2006, Bonifacie et al., 2008). Chlorine can be hosted in a structurally-bound site, i.e., substitute for the hydroxyl group in serpentine (e.g., Anselmi et al., 2000) or in a water-soluble site (e.g., Rucklidge and Patterson, 1977, Sharp and Barnes, 2004, Barnes and Sharp, 2006). Hydrothermal experiments show that chlorine in the water-soluble site is readily leached by water (Sharp and Barnes, 2004, Barnes and Sharp, 2006). Fluid inclusions of natural serpentinites commonly have salinities with great variations (e.g., Philippot et al., 1998, Scambelluri et al., 1997, Scambelluri et al., 2004). As a consequence, chlorine in serpentine may vary greatly even under the same T-P conditions. Analyses of natural serpentinites show that oceanic serpentinites, possibly formed at ∼250 °C, had abundant chlorine, up to 0.62 wt%, whereas antigorite serpentinites with the experience of eclogite-facies metamorphic grade contained much less chlorine (Scambelluri et al., 2004). However, natural serpentinites commonly experience multistage metamorphic history, and consequently the chlorine may not necessarily represent a single T-P condition. In particular, chlorine in natural serpentinites may be greatly influenced by lateral metamorphic fluids. Therefore, it is necessary to experimentally investigate the influence of temperature, pressure, and salinity of starting fluids on the incorporation of chlorine into serpentine minerals.
In this study, we performed experiments at 80–500 °C and pressures ranging from vapor saturated pressures to 20 kbar with peridotite, orthopyroxene, and olivine with <5% pyroxene as starting materials. The objectives are to (1) quantify the concentrations of chlorine in serpentine formed under different conditions, (2) investigate influence of temperature, pressure, fluid salinity, and water/rock ratios on chlorine distribution into serpentine minerals, and (3) assess the importance of serpentinization for the recycling of chlorine in subduction zones.
Section snippets
Preparation of starting materials
An unaltered peridotite, sampled at Panshishan (Jiangsu Province, China) where it occurs as xenoliths in alkaline basalts (Chen et al., 1994, Sun et al., 1998, Xu et al., 2008, Yang, 2008), was taken as the starting material. Peridotite is composed of ∼65 vol% olivine, 20 vol% orthopyroxene, 15 vol% clinopyroxene and ∼2 vol% spinel. Chemical compositions of primary minerals in peridotite were described in a previous experimental study (Huang et al., 2015a). The peridotite is fresh, as evidenced by
Identification of secondary hydrous minerals
As revealed by SEM imaging and Fourier transform infrared spectroscopy analyses (Fig. 1), the main secondary hydrous mineral produced at 311 °C and 3.0 kbar was fibrous chrysotile, and tabular shaped lizardite was formed in experiments at 80–200 °C and vapor saturated pressures, and at 400 °C and 3.0 kbar. Infrared spectra of solid products show typical infrared bands of serpentine at 954 cm−1, 1087 cm−1, and 3686 cm−1. The bands at 954 cm−1 and 1087 cm−1 were assigned to the SiO group of serpentine, and
Conclusions
Hydrothermal experiments were performed at 80–500 °C and pressures ranging from vapor saturated pressures to 20 kbar to study influence of temperature, fluid salinity, water/rock ratios, and pressure on chlorine distribution into serpentine minerals. The results show that chlorine is hosted in a structurally-bound site of serpentine, and it strongly depends on the mobility of iron, aluminum and silica during serpentinization. Chlorine concentrations of serpentine formed at 80 °C were very low,
Acknowledgements
This research was financially supported by the Natural Science Foundation of China (91328204, 41603060), postdoctoral Science Foundation of China (2015M570735, 2016T90805), the Strategic Priority Research Program of Chinese Academy of Sciences (XDB06030100), and the scientific research fund of the Second Institute of Oceanography, SOA (JG1405). We thank S. Jiang at South China University of Technology for the help during FTIR analyses.
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