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1 Instituto de Geología, Universidad Nacional Autónoma de México, 04510 México D.F., México
2 Departamento de Cristalografía y Mineralogía, Universidad Complutense de Madrid, 28040 Madrid, Spain
3 Departamento de Petrología y Geoquímica, Instituto de Geología Económica CSIC-UCM, Facultad de Ciencias Geológicas, Universidad Complutense, 28040 Madrid, Spain
Correspondence: * E-mail: liberto{at}servidor.unam.mx
| ABSTRACT |
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Key Words: Hydratable glass hydratable rhyolite glass hydratable tephra Malinche tephra Mexican Volcanic Belt
| INTRODUCTION |
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Water dissolved in magmas plays a significant role in volcanic eruptions in terms of the eruptive style, the evolution of magma properties such as viscosity, density, crystallization, mobilization of mineral components, the formation of mineral deposits, and the interaction between rocks and fluids among others. Water notably affects the physical and chemical behavior of volcanic glasses and characteristics such as chemical stability, crystal nucleation, and growth. The significance of glasses in magma characterization is increasingly important considering that glasses preserve the structural state of the melt at the bulk glass-transformation temperature (Dingwell and Webb 1990).
Volcanic glasses from lava domes and flows typically contain 0.2–0.8 wt% H2O. Pyroclastics may contain between 0.6–3.0 wt% H2O (Newman et al. 1986; Zhang et al. 1991; Zhang 1999). Water contents up to 10 wt% have been identified in rare opal, chalcedony, and agate (Newman et al. 1986; Zotov 2003). High water contents have been attributed to absorption by pumice glass, but generally contents above 0.5 wt% are due to entrapped molecular water (Frondel 1982; Stolper 1982; Stolper et al. 1982; Graetsch et al. 1985; Newman et al. 1986; Ihinger et al. 1994). Contents as high as 8.0 wt% H2O have been artificially incorporated into trachytic glasses at 850 °C and 20 to 200 mPa (Di Matteo et al. 2004) and of 10 wt% in rhyolitic glasses at 700 °C and 5000 bar PH2O (Zhang 1999).
The properties of glasses vary depending on the origin and association of water. Water may be primary water transferred from the magma or secondary water adsorbed by the glass. It may be in the form of molecular water, or as hydroxyls such as silanol (Si-OH) and aluminol (Al-OH), or as H+-bonded or hydronium ions H3O+. In the study of magmas and glasses, it is important to establish the origin of water, the mechanism of sorption, and how it affects the structural network, polymerization, stability, and reactivity of the glass (Stolper 1982; Dingwell and Webb 1990; Zhang et al. 1991; Keppler and Bagdassarov 1993; Zotov 2003).
Glasses with high contents of adsorbed water are not common. Hence, the present study focuses on a highly hydratable vitreous rhyolitic tephra from the stratovolcano La Malinche. This tephra is capable of adsorbing 12.63 wt% H2O. The goal of this work was to resolve the tephra geochemistry and to understand the origin and mechanisms of its unusual high water adsorption, glass framework, the influence of water on the glass, as well as its relationships to the precursor magma.
| GEOLOGIC SETTING |
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| ANALYTICAL METHODS |
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radiation on bulk and clay-sized fractions scanned at 1 °2
min–1. Whole-rock, major, and trace element analyses were performed by X-ray fluorescence (XRF) on bulk powders fused as glass beads. Total Fe was analyzed by XRF and calculated as FeO. Accuracy was monitored according to international standards and was better than ±2%. Loss on ignition and adsorbed water H2O+ were determined by wet chemistry and DGA. Infrared spectra (IR) in the mid-IR region of 4000–400 cm–1 and near-IR to 5500 cm–1 were recorded, using a Varian spectrometer, from powdered material mixed with KBr and pressed into disks. The magic angle spinning nuclear magnetic resonance (MAS NMR) spectrum of 27Al was recorded using a Varian 300 MHz spectrometer equipped with a 7 mm rotor magic angle spinning (MAS) probe. Samples were spun at 6 KHz. Signals of 27Al were recorded at 78 Hz with a 1–2 µs pulse width, a spectral width of 100 KHz, and 1 s relaxation delay between pulses. Calibration was performed with saturated aqueous AlNO3·6H2O and resonance was reported in parts per million. The morphology, microtexture, and compositions of glasses and minerals were initially determined by scanning electron microscopy (SEM) at 20 kV operating voltage, coupled with energy dispersive X-ray (EDX) analyses on unpolished carbon-coated fragments. More complete studies were performed using SEM and lattice imaging techniques by electron diffraction on fine material separated from ultrasonically dispersed, gently crushed bulk tephra. Analyses were done using a JEOL 2000FX scanning electron microscope operating with an acceleration voltage of 200 kV, a resolution of 3.1 Å, and equipped with a double inclined sample holder and an EDX Oxford ISIS spectrometer with a resolution of 136 eV at 5.39 keV. Lattice imaging by electron diffraction was useful in selecting glass fragments free of crystallization. Transmission electron microscopy (TEM) studies at higher resolutions were performed on very fine material centrifuged from aqueous suspension after removal of coarse material, using a JEOL 3000FX metallographic electronic microscope operated at an acceleration voltage of 300 kV. Analytical data were matrix-corrected by established procedures (Electronic Microscopy Laboratory of the Universidad Complutense de Madrid) (Bence and Albee 1968; Albee and Ray 1970). | RESULTS |
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range exhibit an intense halo of predominantly glass, Ca-plagioclase, augite, hypersthene, ferrosilite, calcite, and cristobalite (Fig. 2
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B(H2O) at 1630.97 and 1663.54 cm–1 and their first overtones 2
B(H2O) at 3275.00 and 3391.37 cm–1. They are associated with molecular water (H2Om) Type I(A) molecules vibrating essentially free in interstitial sites and with H2Om Type I(B) molecules H-bonded to silanol groups in the glass network. In the OH region, the strong shoulder at 3624.83 cm–1 corresponds to the
S(OH) stretching motion of silanol groups and the
S(H2O)III stretching of silanols H-bonded to oxygen of neighboring H2Om Type III. The band could also represent hydrogen bonding between silanols and the silica network of the type
SiOH· · ·O= displaced from the known 3672 cm–1 frequency by intense hydration and H-bonding (Davis and Tomozawa 1996).
The 3472.94 cm–1 band assigned to
S(H2O)I and II is a combination band that includes asymmetric stretching
AS(H2O)II from molecular water H2Om Type II molecules bound to the silica network and symmetric stretching
SS(H2O)I from free H2Om/hydrogen bonded H2Om Type I(A) molecules inside the glass. These are expected at 3450 and 3425 cm–1 in silica glasses (Davis and Tomozawa 1996). In La Malinche tephra, the 3472.94 frequency suggests a dominant contribution from Type II molecules. The absorbance of the 3472.94 cm–1 band caused by H2Om motions is higher than the absorbance of the 3624.83 cm–1 shoulder from OH motions hence pointing to low-temperature hydration of the glass (Davis and Tomozawa 1996). Hydration at high temperatures and partial water pressures would have incorporated less H2Om and more OHs (hydroxyls) in the glass. The low-absorbance band at 5230.22 cm–1 bending (Fig. 7
) is a combination band that adds contributions from stretching motions
B(H2O) +
S(H2O) of H2Om. It sustains the predominance in tephra of molecular water H2Om over hydroxyls OH.
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AS(O1SiOH· · ·HO) of SiO in silanols H-bonded to O atoms of neighboring silanol groups at low H2Om contents or to oxygen of H2O molecules at high H2Om contents (Davis and Tomozawa 1996), the 3510 cm–1 OH stretching
S(OH· · ·HOSi) of silanols H-bonded to the oxygen of neighboring silanols, and the ~4566 cm–1 band from silanol groups hydrogen bonded to H2O molecules. Also absent are the 964 cm–1 SiO asymmetric stretching of
AS(O3SiOH) and
AS(O1SiO) and the 2820–2810 cm–1 stretching
S(OH· · ·X) corresponding to OH stretching of silanols H-bonded to non-bridging O atoms (NBOs).
27Al MAS NMR
The predominant form of 27Al in tephra is tetrahedral coordinated IVAl characterized by the intense broad shift at 56.241 ppm and slightly skewed toward more shielded positions (Fig. 8
). Octahedral VIAl is defined by the weak broad shift at –0.937 ppm, whereas low-intensity shoulders at 38.8, 33.3, and 28.3 ppm indicate minor association of VAl. The 3.7 intensity ratio between shifts of IVAl and VIAl establishes the dominance of tetrahedral IVAl.
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The VIAl shift at –0.937 ppm occurs within the 15 to –10 ppm known range for silicoaluminate glasses (Kirkpatrick 1988; Stebbins 1995; Petrini et al. 1999; Stebbins et al. 2000; Slejko et al. 2003; Allwardt et al. 2005a, 2005b, 2007) and silicates (Dirken et al. 1992; Rehak et al. 1998; Kelsey et al. 2008). The VAl shifts at 38.8, 33.3, and 28.3 ppm are within the known range of 25–35 ppm (Kirkpatrick 1988; Stebbins 1995; Wang et al. 2002b; Allwardt et al. 2007), of 34.9–44.2 ppm for polyhedral AlO5 in SiO2-Al2O3-CaO glasses (Neuville et al. 2004), and of 38.7–33.6 ppm for Al2O3-CaO glasses (Neuville et al. 2007). The intense motion at 108.732 ppm (Fig. 8
) corresponds to a static peak or to a satellite transition caused by a first-order quadrupolar interaction exceeding the sample rotation frequency.
Electron microscopy
Less than 2% of the tephra is comprised of well-developed crystals (~10 µm in size) of pigeonite oriented along their z axis in a flow pattern (Figs. 9b and 9d
; compositions 2 and 3 in Table 3
), tabular augite (Fig. 9c
; composition 1 in Table 3
), and prismatic ferrosilite (Figs. 9e, 9f, and 9g
; compositions 4, 5, and 6 in Table 3
). Laumontite occurs as a few thin tabular oriented crystals in glass (Figs. 9h and 9i
; compositions 7 and 8 in Table 3
) and as an authigenic replacement of plagioclase (Fig. 9e
; composition 9 in Table 3
) associated with authigenic calcite (Fig. 9j
). Mazzite appears as thin hexagonal prisms in glass (Figs. 9a and 9f
; compositions 10 and 12 in Table 3
).
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Major element variation diagrams for the sodic glasses, indicated in Figure 12
, show that Al2O3 and Na2O decrease, MgO and FeO increase, and that there is little change in CaO and K2O as SiO2 increases from 71.80 to 77.77 wt%. Similarly, the non-sodic glasses show decreasing Al2O3 and increasing MgO. However, the non-sodic glasses differ from the sodic glasses in terms of decreasing FeO and K2O as SiO2 increases from 74.84 to 83.88 wt%. Variation diagrams for alkalis vs. SiO2 indicate a steeper depletion of alkalis in sodic glasses than in the non-sodic, peraluminous glasses (Fig. 13
).
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| DISCUSSION |
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The compositions of crystals and glasses were determined using SEM and EDX of selected fragments with the difficulties in precision related to crystal size and association with glass. To better visualize the compositional variation of glasses and to ascertain crystallization paths, we refer to their normative compositions (Table 5
) calculated from the CIPW norm (Best 1982). Tephra and glasses show highly evolved compositions with differentiation indices (DI) higher than 50. Among the sodic glasses (M1 to M4), M1 has 57.8% normative plagioclase (An13Ab87) that evolves to 18.1% (An22Ab78) in glass M4. Normative hypersthene increases from 3.4% (En50Fe50) to 9.9% (En62Fe38). The liquidus temperature descends from 814 to 704 °C, suggesting crystallization of Ca-plagioclase to Na-plagioclase and increasingly ferrous pyroxene in progressively more siliceous glass. Glasses M7 and M12 are siliceous, with composition M12 corresponding to 11.0% normative plagioclase (An54Ab46) and 14% hypersthene (En75Fe25). Glasses M5 and M6 are sodium-free glasses with normative hypersthene (En65Fe35) and anorthite. These glasses are characterized by low viscosity, a liquidus temperature of 739 °C (within the same range as sodic glass M2), and a differentiation index of 71. Glasses M8 to M11 and M13 correspond to sodium free glasses of normative 9.1 to 6.9% anorthite and hypersthene (En67Fe33, En71Fe29, En72Fe28, En66Fe34, and En82Fe18, respectively) in increasingly more siliceous melts with the liquidus temperature descending from 739 to 575 °C and differentiation index ascending from 78 to a highly evolved 85. In the systems albite-orthoclase-anorthite and albite-anorthite-hypersthene, sodic glasses have albitic compositions different from those of non-sodic glasses that are richer in normative hypersthene, anorthite, and orthoclase (Fig. 14
).
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A second Na-free magma, represented by glasses M5 and M6, evolves upon cooling, through compositions M7 to M13, to a highly siliceous glass with 83.88 wt% SiO2 and normative liquidus temperature 575 °C (Table 4
). Glasses M5 and M6 have liquidus temperatures and contents of SiO2 and Al2O3 approximately equal to those of sodic glasses M2 and M3, suggesting possible simultaneous crystallization of both magmas starting at around 739 °C. Crystallization of the Na-free magma—as estimated from the normative calculations—began with high-Mg, low-Fe pyroxene and ended with low-Mg, high-Fe pyroxene+Ca-plagioclase. The Na-free magma crystallized a comparatively larger amount of pyroxene with a dominant ferrosilite component and a lower amount of labradorite (from samples M7 and M12) in highly siliceous glass than the Na glasses. The latter crystallized more sodic plagioclase and less pyroxene in less siliceous glass.
Analyzed phenocrysts have compositions of aluminous labradorite, augite (En41Fe59), pigeonite (En47Fe59 and En58Fe42), and ferrosilite (En9Fe81 and En24Fe76) (Table 3
) similar to those estimated from the CIPW norm in predominantly Na-free glasses. The cooling path and crystallization were likely in equilibrium (Osborn and Muan 1960; Morse 1980). Glasses M12 and M13 correspond to the lowest temperature residual melt with 83.88 wt% SiO2. Limited formation of pyroxene and plagioclase in amounts less than those anticipated from the normative calculations could indicate rapid cooling and solidification of magma, associated with a fast reduction in pressure, temperature, and water vapor and poor development of the glass framework.
Analyzed and normative data have indicated that solidification and crystallization of sodic and non-sodic magmas started ~739 °C or above and ended ~575 °C. Sodic residual magma M4 solidified at the normative liquidus temperature of 704 °C, whereas non-sodic magma M13 did so at 575 °C. Both temperatures are above the stability limits of the zeolites laumontite and mazzite recognized in tephra in amounts <1 vol%. Compositional data for crystalline minerals and glasses (Tables 3
and 4
; Figs. 12
and 13
) indicate that the two magmatic processes of crystal fractionation were overlapped by a later process of secondary low-grade metamorphism on the glasses by fluids, leading to crystallization of mazzite from the less siliceous sodic glasses, laumontite from the more silicic non-sodic glasses, and authigenic laumontite from Ca-plagioclase and calcite. In the presence of abundant water, water diffused into the glass would have forced cations outward, modified Al-O bonds, and de-polymerized the glass structural network, forming SiOH, AlOH, and Si-O-T bonds (Mungall and Martin 1994; Slejko et al. 2004).
SEM and TEM studies allowed for the recognition of glasses of distinct compositions and fluidity and their devitrification to fine-grained, well-formed crystallites (<5 nm in size) of plagioclase and pyroxene. These crystallites are not hydratable, nor are the larger ~10 µm crystals of plagioclase and pyroxenes observed by SEM at 20 kV. Only a minor fraction (less than 2%, of ~10 µm size crystals) of low-grade metamorphic laumontite and mazzite adsorb water. Crystallization of magmatic laumontite is not evident from the SEM studies. The minor abundance of laumontite and mazzite does not justify the intense dehydration shown by tephra.
As described above, tephra loses 12.63 wt% adsorbed water reversibly by heating to 72 °C and 0.57 wt% is lost from hydroxyls and water by heating to 454 °C. Weak endothermic reactions at 645 and 952 °C are caused by structural accommodations or by additional minor losses of water and hydroxyls. Although strong dehydration and thermal behavior resemble characterisitics of zeolite minerals, their presence is further discounted by the fact that a dehydration loss of 12.63 wt% H2O would correspond to an estimated content of 78 wt% fully hydrated laumontite CaAl2Si4O12·4.5H2O in the tephra (Fridriksson et al. 2003a). Such amounts would have been unmistakably recognized by XRD. However, the XRD data does not record the presence of laumontite or any other zeolite. The dehydration/hydration of the tephra at 72 °C is fully reversible even after heating to 500 °C. Laumontite, when heated from 25 to 270 °C, loses water from sites W1, W5, and W2 and between 300 and 400 °C, loses half of the water in W8 sites, collapsing its structure irreversibly (Fridriksson et al. 2003a, 2003b; van Reeuwijk 1974; Armbruster and Kohler 1992; Stahl et al. 1996; Bish and Carey 2001).
The intense hydration/dehydration of the tephra is attributed to the glass, which is its principal component. Vibrational spectra have shown that molecular water H2Om is the principal adsorbate, predominating over hydroxyls OH. Molecular H2Om occurs as Type I(A) molecules vibrating freely in interstitial sites, Type I(B) molecules H-bonded to silanol groups in the glass network, silanols H-bonded to oxygen of neighboring Type III H2Om molecules, Type II molecules bound to the silica network, and free H2Om hydrogen bonded to H2Om Type I(A) molecules inside the glass. The higher absorbance of the 3472.94 cm–1 band caused by motions of Type II H2Om molecules bound to the silica network, relative to the lower absorbance 3624.83 cm–1 shoulder from OH motions, establishes the predominance of molecular H2Om and low-temperature hydration of glass. Hydration at high temperatures and partial water pressures would have incorporated less H2Om and more hydroxyls OH in the glass. The low-absorbance band at 5230.22 cm–1 (Fig. 7
) that adds contributions from HOH motions
B(H2O) +
S(H2O) of molecular water H2Om (Stolper 1982; Davis and Tomozawa 1996), and the absence of the ~4520 cm–1 signal due to XOH bending plus stretching, confirms the predominance of molecular water H2Om over hydroxyls OH associated with the glass.
Adsorption by the glass is linked to its surface activity. NMR studies have indicated that 27Al is predominantly in the form of IVAl and some is present as VAl, possibly developed by reactions between polymerized tetrahedral and single tetrahedra terminating in NBOs (Topliss et al. 1997a, 1997b, 2000; Neuville et al. 2004, 2007; Allwardt et al. 2005a, 2005b, 2007). IVAl and VAl contribute to the surface activity of the glass by generating NBOs from reaction of AlO4 to configurations of AlO6 and AlO5 or VAl-O-IVSi and VIAl-O-IVSi in the magma at extreme conditions of 2500 K and 2–8 GPa (Poe et al. 1994; Stebbins 1995; Lee 2004; Allwardt et al. 2005a, 2005b, 2007), and from the replacement of VIAl by Mg2+ and Fe2+ of high electrostatic charge and field strength (Cormier et al. 2003; Neuville et al. 2007).
Non-bridging oxygens could additionally result from low concentrations of Na in the sodic glasses and Ca in the non-sodic glasses, which are insufficient to charge balance Al, develop Al-O-Na and Al-O-Ca bonds, polymerize the glass, and impart chemical and physical stability (Cormier et al. 2003; Angeli et al. 2007). Their limited availability to compensate Al would develop Al-O bonds and NBO activity. Molecular dynamic studies and experimental data on the SiO2-Al2O3-CaO system have shown that low-SiO2, high-CaO glasses, which do not contain VAl, may have abundant NBOs and highly polymerized stable networks (Neuville et al. 2007), whereas glasses with over 40 mol% SiO2 and very low Al2O3 develop IVAl in Q4 sites with the formation of VAl and large NBO capacity (Kirkpatrick et al. 1986; Oestrike et al. 1987; Poe et al. 1994).
| ACKNOWLEDGMENTS |
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| Footnotes |
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E-mail: mdoval{at}geo.ucm.es MANUSCRIPT HANDLED BY AARON CELESTIAN
MANUSCRIPT RECEIVED December 20, 2008; MANUSCRIPT ACCEPTED June 19, 2009
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