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Journal of Petrology Advance Access originally published online on October 1, 2004
Journal of Petrology 2005 46(1):135-167; doi:10.1093/petrology/egh066
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Journal of Petrology vol. 46 issue 1 © Oxford University Press 2004; all rights reserved

An Experimental Investigation of the Influence of Water and Oxygen Fugacity on Differentiation of MORB at 200 MPa

JASPER BERNDT*, JÜRGEN KOEPKE and FRANÇOIS HOLTZ

INSTITUT FÜR MINERALOGIE, UNIVERSITÄT HANNOVER, WELFENGARTEN 1, D-30167 HANNOVER, GERMANY

RECEIVED APRIL 15, 2002; ACCEPTED JULY 28, 2004


    ABSTRACT
 TOP
 ABSTRACT
 INTRODUCTION
 EXPERIMENTAL TECHNIQUES
 RESULTS
 DISCUSSION
 CONCLUSIONS
 REFERENCES
 
Crystallization experiments were performed at 200 MPa in the temperature range 1150–950°C at oxygen fugacities corresponding to the quartz–fayalite–magnetite (QFM) and MnO–Mn3O4 buffers to assess the role of water and fO2 on phase relations and differentiation trends in mid-ocean ridge basalt (MORB) systems. Starting from a primitive (MgO 9·8 wt %) and an evolved MORB (MgO 6·49 wt %), crystallization paths with four different water contents (0·35–4·7 wt % H2O) have been investigated. In primitive MORB, olivine is the liquidus phase followed by plagioclase + clinopyroxene. Amphibole is present only at water-saturated conditions below 1000°C, but not all fluid-saturated runs contain amphibole. Magnetite and orthopyroxene are not stable at low fO2 (QFM buffer). Residual liquids obtained at low fO2 show a tholeiitic differentiation trend. The crystallization of magnetite at high fO2 (MnO–Mn3O4 buffer) results in a decrease of melt FeO*/MgO ratio, causing a calc-alkaline differentiation trend. Because the magnetite crystallization temperature is nearly independent of the H2O content, in contrast to silicate minerals, the calc-alkaline differentiation trend is more pronounced at high water contents. Residual melts at 950°C in a primitive MORB system have compositions approaching those of oceanic plagiogranites in terms of SiO2 and K2O, but have Ca/Na ratios and FeO* contents that are too high compared with the natural rocks, implying that fractionation processes are necessary to reach typical compositions of natural oceanic plagiogranites.

KEY WORDS: differentiation; MORB; oxygen fugacity; water activity; oceanic plagiogranite


    INTRODUCTION
 TOP
 ABSTRACT
 INTRODUCTION
 EXPERIMENTAL TECHNIQUES
 RESULTS
 DISCUSSION
 CONCLUSIONS
 REFERENCES
 
Since the late 1950s, many experimental studies have focused on the investigation of phase relations in natural basaltic systems for a better understanding of the differentiation mechanisms under crustal pressures and temperatures. Most of these experiments have been carried out at 1 atm (e.g. Osborn, 1959Go; Grove & Bryan, 1983Go; Grove & Baker, 1984Go; Juster et al., 1989Go; Snyder et al., 1993Go; Thy & Lofgren, 1994Go; Toplis & Carroll, 1995Go, 1996Go), assuming that the small pressure difference between shallow magma chambers and the surface does not influence significantly the results and implications drawn from these studies. It was considered that the low volatile content of basaltic melts (volatiles are incorporated in melts only under pressure) has little influence on phase relations. One of the benefits of these studies was to evaluate the role of fO2 (oxygen fugacity), which is a critical parameter controlling the crystallization of Fe–Ti oxides in iron-bearing systems.

Concerning the role of volatiles, especially H2O, the broad absence of amphibole as a primary cumulate phase in tholeiitic plutonic complexes (e.g. Skaergaard, Kiglapait, Pleasant Bay, typical oceanic crust) has been taken as evidence for very low water activities during the main stage of fractionation of these melts. However, the common presence of small amounts of interstitial amphibole within typical oceanic gabbros indicates that water may play a role, at least during the late differentiation stage of mid-ocean ridge basalt (MORB) (e.g. Gillis, 1996Go; Dick et al., 2000Go; Coogan et al., 2001Go). Studies on water contents in basalts by Sobolev & Chaussidon (1996)Go, Danyushevsky et al. (2000)Go and Kovalenko et al. (2000)Go showed that even for primitive MORB the H2O content varies from <0·1 up to 1·5 wt %. Assuming an initial water content for a primitive MORB liquid of 0·5 wt % at a pressure corresponding to shallow levels, the crystallization of 60 wt % of anhydrous minerals results in an increase of water activity (aH2O) up to about 0·23 [calculated after Burnham (1979)Go for MORB at 1100°C and 100 MPa; see below]. Thus, it can be expected that the water activity of MORB liquids increases with differentiation to values that influence phase relations in these systems (especially at high degrees of fractionation), even if the stability field of amphibole may not have been reached.

Few experimental data are available to understand the effect of aH2O on the differentiation trends of primitive MORBs at moderate pressure (e.g. ≤200 MPa). Spulber & Rutherford (1983)Go performed experiments using a primitive MORB from the Galapagos Spreading Centre to assess the origin of plagiogranites in oceanic ridges, but aH2O was not varied systematically. Further experimental investigations have been carried out in more alkali-rich compositions. The comparison of results from melting and crystallization experiments of Holloway & Burnham (1972)Go on the 1921 Kilauea tholeiite at aH2O ~ 0·6 with those of Yoder & Tilley (1962)Go and Helz (1973Go, 1976Go), at water-saturated conditions, shows that water influences phase relations and that the occurrence of amphibole influences the differentiation from andesitic to rhyolitic residual melts. Sisson & Grove (1993aGo, 1993b)Go investigated phase relations in calc-alkaline systems at water-saturated conditions, and Kawamoto (1996)Go carried out melting experiments at aH2O ≤ 1 in similar systems. Those workers emphasized the dramatic role of water and pointed out that the absence of amphibole in these systems does not necessarily mean that dry conditions are prevailing.

The lack of experiments in basaltic systems at moderate pressure (100–500 MPa) in the presence of volatiles is due to experimental problems. The formation of quench crystals is a serious problem when performing experiments with low-viscosity basaltic compositions, and often hampers the interpretation of results from phase equilibrium studies (e.g. Hamilton et al., 1964Go; Holloway & Burnham, 1972Go; Helz, 1973Go, 1976Go). In this study, all experiments were carried out in internally heated pressure vessels (IHPV) using a rapid-quench sample holder to avoid the formation of quench crystals during cooling of the experimental charge (Holloway et al., 1992Go; Roux & Lefevre, 1992Go; Berndt et al., 2002Go). A first series of experiments was undertaken to provide information on the influence of aH2O on phase relations in a primitive MORB system at 200 MPa and fO2 corresponding to the MnO–Mn3O4 buffer using both a primitive and a fractionated synthetic 10-component MORB glass (Table 1). As the fO2 of natural MORB lavas is found to vary generally between QFM – 2 and QFM + 1 (where QFM is the quartz–fayalite–magnetite buffer) (e.g. Carmichael & Ghiorso, 1986Go; Christie et al., 1986Go), we performed a second series of crystallization experiments under redox conditions corresponding to the QFM buffer. For these experiments, the sample holder was equipped with a hydrogen membrane to control and adjust fO2 (Berndt et al., 2002Go). All experiments were performed in the temperature range 1150–950°C and at 200 MPa, a typical pressure of MORB magma chambers under the mid-ocean ridge system at depths between 3 and 6 km (e.g. Fisk, 1984Go; Nicolas, 1989Go). For a better understanding of the role of water during differentiation of MORB, the initial water content of our experimental systems was varied systematically ranging from 0·35 wt % to 4·7 wt % H2O. The results are used to estimate the influence of H2O and fO2 on stability of Fe–Ti oxides and MORB liquid line of descent.


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Table 1: Composition of natural primitive MORB and synthetic MORB B1 and B2 (starting material)

 

    EXPERIMENTAL TECHNIQUES
 TOP
 ABSTRACT
 INTRODUCTION
 EXPERIMENTAL TECHNIQUES
 RESULTS
 DISCUSSION
 CONCLUSIONS
 REFERENCES
 
Apparatus
All experiments were performed in a large-volume IHPV working vertically with pure Ar or Ar–H2 mixtures as pressure medium. A detailed description of the apparatus has been given by Berndt et al. (2002)Go. Formation of quench crystals during cooling the experimental charge was avoided using a rapid-quench system [see experimental setup described by Berndt et al. (2002)Go] in which up to six capsules are fixed to a Pt-wire in the hot zone of the furnace. By fusing the Pt-wire, the capsules drop onto a cold copper block placed at the bottom of the sample holder (about 25°C). The intrinsic fO2 (pure Ar as pressure medium) of the IHPV has been measured at four temperatures (900–1200°C) using the Ni–Pd solid redox sensor technique after Taylor et al. (1992)Go and is equivalent to the MnO–Mn3O4 solid oxygen buffer (Fig. 1).



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Fig. 1. Intrinsic fO2 of the IHPV measured by solid sensor technique after Taylor et al. (1992)Go and calculated fO2 using coexisting magnetite–ilmenite pairs (Andersen et al., 1993Go) from runs at intrinsic conditions. Continuous lines show MnO–Mn3O4 and QFM buffer curve. Dashed line shows the shift of fO2 relative to the MnO–Mn3O4 buffer curve at lower water activities (aH2O = 0·3) and more reducing conditions in the experiments. NiPd sensor measurements after Taylor et al. (1992)Go were performed using both Pt and Au80Pd20 capsules.

 
Starting material
For experiments under oxidizing conditions (MnO–Mn3O4 buffer) two synthetic starting compositions (Table 1) were used for the crystallization experiments: a primitive MORB glass (B1) and a more evolved MORB glass (B2) corresponding to a residual glass composition obtained after 50% crystallization of B1 at 1100°C (run 42; Table 1). Only the B1 composition was used for experiments under reducing conditions (QFM buffer). Starting materials were made from synthetic oxide and carbonate powders. Oxide powder mixtures were placed into a Pt crucible and fused twice (grinding between fusions) at 1600°C, 1 atm, and a log fO2 corresponding to about –0·68 (air). To avoid alkali loss from the glass, melting duration was <1·5 h. Electron microprobe analyses of chips extracted from the top, middle and bottom of the glass showed that they are homogeneous. The glass B1 lies within the compositional range of natural primitive MORBs (Table 1).

Sample preparation and experimental procedure
First attempts were made by preparing the samples with dry powder of the starting glasses (grain size <50 µm) and a given amount of water added into Au80Pd20 capsules. After loading the capsules into the sample holder, they were held for about 1 h above the liquidus temperature at 200 MPa to obtain a homogeneous distribution of H2O in the melt and to allow redox equilibrium of the melt. In a second step, temperature was lowered to the desired run temperature. Resulting products clearly showed disequilibrium features such as complex zonation of minerals. Compositional variations for Al2O3 in clinopyroxene were as high as 5–9 wt % within a single crystal. To avoid these effects, charges with dry glass plus water were brought directly to the desired run temperature. Results at relatively high temperatures (1050–1150°C) did not show disequilibrium features, but mineral sizes and distributions were heterogeneous at lower temperatures and low water activity (aH2O). This is probably due to crystallization taking place before homogeneous distribution of water is achieved in the glass powder.

Therefore, the experimental strategy consisted in using pre-hydrated glass powder as starting materials (Gaetani & Grove, 1998Go; Müntener et al., 2001Go). Large amounts of dry glass powder were placed into Au80Pd20 capsules [internal diameter (i.d.) 0·5 cm; outer diameter (o.d.) 0·54 cm at 3 cm length] and stuffed with the help of a steel piston. Distilled water was added to the charge using a microsyringe in five steps to achieve homogeneous H2O distribution within the capsule. Sealed capsules were heated at 1250°C and 200 MPa (above the liquidus) at the desired fO2 (either MnO–Mn3O4 or QFM buffer conditions) for 24 h in an IHPV equipped with the rapid-quench hydrogen-membrane device described above. Homogeneous crystal- and bubble-free glasses were obtained and the water contents were determined by Karl–Fischer titration (KFT) (Table 2; for technique and precision see Behrens (1995)Go]. Final bulk water contents of the glasses vary between 0·35 and 4·7 wt % and are shown in Table 3.


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Table 2: Comparison between water solubility measured by Karl–Fischer titration (KFT) analysis and calculated by the thermodynamic model of Burnham (1979)Go assuming aH2O = 1 for MORB at 200 MPa

 
The pre-hydrated glasses were finally crushed in a steel mortar and sieved to fractions of 100–200 µm. About 50–80 mg of the hydrous glass powders were sealed in Au80Pd20 capsules (i.d. 0·3 cm; o.d. 0·34 cm at 1 cm length). A set of up to four capsules (corresponding to the four bulk H2O contents of B1 and B2) were fixed to the rapid-quench device and brought directly to run temperature. Phase relations were investigated at 200 MPa, at 50°C intervals in the temperature range 1150–950°C (Table 3). The run durations for oxidizing experiments were ~20 h, except for charges 62 and 61 (B1; 72 h) and 111 (B2; 96 h). The products of these longer experiments were compared with those of the 20 h runs conducted at the same pressure and temperature confirming identical results (runs 45, 42 and 104; see below and Table 3a and b). Experimental duration for runs under reducing conditions was limited by the diffusive Fe loss to the capsule material and varied with temperature from 2 to 9·2 h (Table 3c). After quenching each capsule was weighed to check for leaks and then punctured to determine if a fluid phase was present or not. A cross-section of each capsule (including the sample container) was prepared as a polished section for electron microprobe analysis of solid phases and the noble metal.


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Table 3a: Experimental conditions and results for composition B1 (MnO–Mn3O4 buffer)

 

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Table 3b: Experimental conditions and results for composition B2 (MnO–Mn3O4 buffer)

 

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Table 3c: Experimental conditions and results for composition B1 (QFM buffer)

 
Loss of iron
To avoid iron loss to the sample container (e.g. Johannes & Bode, 1978Go; Sisson & Grove, 1993aGo), Au80Pd20 capsules were used because Fe solubility is lower in Au80Pd20 than in Pt, and Au80Pd20 has a higher melting point than pure Au, which allowed us to perform experiments up to 1250°C (Kawamoto & Hirose, 1994Go). The glasses and capsule walls were analysed with the electron microprobe to check for iron loss or enrichment, respectively. No iron was detected in the capsule material of experiments performed under oxidizing conditions and the total Fe content of the hydrous glasses was equivalent to that of the dry starting material. Experiments performed under QFM buffer conditions showed significant iron loss as a result of Fe diffusion into the Au80Pd20 capsule material. Therefore, the Au80Pd20 capsules were pre-saturated in iron at fO2 corresponding to the QFM buffer at 200 MPa and 1200°C (conditions similar to the desired fO2 in the crystallization experiments at aH2O = 1) following the procedure described by Ford (1978)Go. Thus, iron loss could be limited in our study. A melt composition profile of run 130 (Table 3c), performed above the liquidus temperature at 1150°C and with about 4·58 wt % H2O melt water content, showed that iron has been lost mainly from the rim of the experimental charge, which is in direct contact with the capsule material. In the middle of the capsule the initial iron concentration of the glass was preserved. The average iron content along the profile was lowered by about 4·8% relative to the starting material. Iron loss from the other experiments performed at 1150°C was estimated to be between 6 and 8% relative by mass balance calculations. At temperatures below 1100°C, Spulber & Rutherford (1983)Go and Sisson & Grove (1993a)Go emphasized that no significant amount of iron was lost from their samples to the capsule material, which is in accordance with our results. Therefore, the iron content of the glasses analysed in the middle of the capsule is believed to be realistic. This is confirmed by Fe2+–Mg olivine–melt partition coefficients, which agree with published data for this mineral.

Calculations of aH2O and fO2
It has been shown that the thermodynamic model of Burnham (1979)Go is not always correct for the calculation of aH2O and melt water contents, especially at high pressures (e.g. water solubility can be underestimated by 20% relative at 500 MPa; Holtz et al., 1995Go). At 200 MPa, calculated H2O solubilities after Burnham (1979)Go for synthesized MORB glasses B1 and B2 agree well with the contents determined by KFT for these glasses (Table 2). Thus, we have used the model of Burnham (1979)Go to calculate melt water content at aH2O = 1. In addition, for runs in which aH2O was <1, water activities have also been calculated using the model of Burnham (1979)Go and the water contents of the melts determined by mass balance and electron microprobe (see below).

For runs performed under oxidizing conditions the fH2 was imposed by the vessel and corresponds to the MnO–Mn3O4 solid oxygen buffer [based on the equation of Chou (1978)Go]. For experiments at lower oxygen fugacities a proportion of H2 was added to the pressure medium (Ar) to reach a final pH2 at run conditions resulting in an fO2 corresponding to the QFM buffer at water-saturated conditions (Table 3c). It should be noted that in water-undersaturated experiments fH2O and thus fO2 decrease with aH2O (Scaillet et al., 1995Go), resulting in much more reducing fO2 conditions at low aH2O (Table 3).

Melt Fe2+/Fe3+ ratios were calculated using the method of Kress & Carmichael (1991)Go. As emphasized by Baker & Rutherford (1996)Go and Gaillard et al. (2001)Go, the expression of Kress & Carmichael (1991)Go has not been calibrated for hydrous glasses. For H2O-saturated rhyolitic melts Baker & Rutherford (1996)Go and Gaillard et al. (2001)Go showed that water has an oxidizing effect on the melt Fe2+/Fe3+ ratio relative to the Kress & Carmichael (1991)Go expression, especially at fO2 < NNO + 1·5 (where NNO is the nickel–nickel oxide buffer). For the hydrous experiments performed in this study at the QFM buffer (which is below the NNO buffer conditions), the calculated melt Fe2+/Fe3+ ratios were not corrected with respect to the melt water content, because the data of Baker & Rutherford (1996)Go and Gaillard et al. (2001)Go were obtained for water-saturated conditions in very silicic melts only. Thus, the effect of dissolved H2O on the Fe2+/Fe3+ ratio in basaltic melts, especially in runs at aH2O <1, is unknown.

Analytical techniques and determination of phase proportions
Electron microprobe analyses of glasses and minerals were performed with a Cameca Camebax and a Cameca SX 100 instrument and are listed in Table 4. Analytical conditions for minerals were 15 kV, 15 nA beam current, and counting times of 5 s for Na and K, and 10 s for all other elements. Glasses were analysed with a defocused beam of 20 µm with a 5 nA beam current and counting times of 2 s for Na and K, and 5 s for the other elements. In crystal-rich runs (glass < 30 wt %) the beam was defocused as much as possible, but loss of alkalis was observed for spot sizes <15 µm. In this case analyses were corrected by a loss factor using the B1 hydrous starting glasses as standards with known water contents.

Phase proportions (wt %) were determined by mass balance (glass analyses were normalized to 100 wt %). Melt water contents in runs with aH2O < 1 were calculated using the known melt fractions and bulk water content of the starting materials. No attempts were made to consider the water content in amphiboles, because runs within the amphibole stability field (Table 3; see Fig. 4) were water saturated.

The melt water content was also estimated for all runs with the ‘by-difference’ method (Devine et al., 1995Go; Koepke, 1997Go). Comparison of melt water contents obtained by mass balance (aH2O < 1) and from the ‘Burnham model’ (aH2O = 1) with the water contents determined with the ‘by-difference’ method show good agreement (Fig. 2).



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Fig. 2. Comparison of melt water contents for B1 and B2 calculated by mass balance (aH2O < 1; •, B1; {square}, B2) and by using the ‘Burnham model’ (aH2O = 1; {blacktriangleup}, B1; {triangleup}, B2) with the H2O contents obtained with the ‘by-difference’ method (Devine et al., 1995Go; Koepke, 1997Go). Error bars correspond to the average errors obtained for values using the ‘by-difference’ method (±1·23 wt %) and mass balance calculations (±0·74 wt %) assuming an error of 20% relative for phases with 1–10 wt % abundances.

 
In experiments with low melt fractions, in which water-saturated conditions mostly prevailed, melt water contents obtained by the ‘by-difference’ method were relatively higher than those from the ‘Burnham model’ (see triangles in Fig. 2 for runs with aH2O = 1). This is probably due to too low microprobe totals resulting from analyses of very small melt pools with a beam that could not be defocused. Analyses of glasses in runs with low melt fractions were possible because small batches of crystal-free residual liquid were located along the capsule rim. This was especially the case for run 151 containing about 8 wt % melt. However, for the near-solidus experiments 47 and 46 the remaining glass pools were too small to be analysed even with a focused beam. Hence, phase proportions (vol. %) have been estimated from back-scattered electron (BSE) images using analySIS© 3.0 software (Gardien et al., 1995Go; Koepke et al., 1996Go). The proportion in wt % (Table 3a) was recalculated assuming typical average densities for the solid phases and for the melt (melt density of 2·28 g/cm3 is estimated from glass composition of run 48 after Lange (1997)Go, Lange & Carmichael (1990)Go and Ochs & Lange (1999)Go]. For these two experiments the melt compositions were roughly determined by mass balance calculations.

Experimental limitations and general aspects on the effect of H2O on experimental results
It should be emphasized that there are different ways to understand the effect of H2O on mineral compositions and liquid lines of descent. The effect of bulk water content can be estimated by comparing experimental charges obtained at identical temperature with different bulk water content of the charge. However, comparison of such experiments shows that the crystal amount is not the same at different bulk water contents, especially for high-temperature runs (e.g. runs 42–45 at 1100°C; Table 3a; Fig. 3a). In these high-temperature experiments, residual melts have different water contents and therefore different aH2O. In contrast, for low-temperature runs (e.g. runs 34–37 at 1000°C, Table 3a) the crystal content is always high enough to attain fluid-saturated conditions (as a result of crystallization of mostly anhydrous phases). Thus, at high temperatures, a decrease of the bulk water content results in a strong decrease of aH2O in the experimental charge. In contrast, at low temperature, only small changes in aH2O with changing bulk water content are expected. In subsequent sections, results are discussed as a function of either bulk water content or aH2O. It is emphasized that these two parameters are not identical.



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Fig. 3. Back-scattered electron (BSE) images of run products obtained at 1100°C at MnO–Mn3O4 buffer conditions (a, B1; b, B2) and QFM buffer conditions (c, B1). gl, glass; ol, olivine; pl, plagioclase; cpx, clinopyroxene; mt, magnetite. Images show variation in modal proportion and phase stability in experiments with varying bulk water content and thus aH2O of the charge for a constant temperature. The absence of quench crystals should be noted.

 
From the discussion above, it could be expected that, at low temperatures (e.g. 950 and 1000°C), experimental conditions are always fluid saturated (water saturated), and all other parameters being equal (P, T, bulk composition, fO2), the phase assemblage and composition should be identical. The results in Fig. 4 show that this is not the case because the melt proportion, the relative proportions of minerals and, therefore, melt composition (see Figs 911) differ as a function of the bulk water content. An additional possible explanation is that despite the presence of a free fluid phase in these runs (Table 3) aH2O may be decreased by the presence of air in the capsules. Thus, aH2O slightly decreases with decreasing bulk water content because of the higher N2/H2O ratio in experiments with starting glasses containing low water contents. The XH2O [defined as XH2O/(XH2O + XN2)] in these charges was estimated to be 0·92 (for lowest bulk water contents). The small changes in aH2O for given bulk water contents at low temperature influence both composition and stability of experimental phases. For example, in B1 experiments at 1000°C, orthopyroxene is stable only at low bulk water contents (0·89 and 1·49 wt % H2O) and the stability of amphibole is reached only at the highest bulk water content of 4·70 wt % (Fig. 4a).



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Fig. 4. Phase relations of B1 (a) and B2 (b) compositions at MnO–Mn3O4 buffer conditions and B1 (c) at QFM buffer conditions as a function of temperature and bulk water content contoured for aH2O (dashed lines) at 200 MPa. gl, glass; ol, olivine; pl, plagioclase; cpx, clinopyroxene; mt, magnetite; ilm, ilmenite; am, amphibole. Continuous lines indicate beginning of crystallization of a phase. Dotted lines mark phase-out boundary. Contours of aH2O are based on aH2O calculated after Burnham (1979Go; Tables 2 and 3) and extrapolated between different runs.

 
A further point is that a change in the water content of the melt (and thus aH2O), while holding all other parameters constant, results in a change of fO2 (see above). Oxygen fugacity is identical in all runs with aH2O = 1 at isothermal conditions. In this case the fO2 corresponds to the adjusted fO2 conditions of the IHPV. In contrast, at higher temperatures, when H2O saturation has not been reached, fO2 depends also on the prevailing aH2O (Scaillet et al., 1995Go; Table 3). Hence, it is difficult to discriminate between the individual effects of aH2O and fO2, especially in the discussion on the evolution of iron-bearing phases.

Achievement of equilibrium
Crystallization experiments are known to be the best method to approach equilibrium conditions (Pichavant, 1987Go) when compared with melting experiments in which non-equilibrated residual minerals can remain for long run durations in the surrounding melt. The following observations are taken as evidence for near-equilibrium conditions. (1) All phases are typically homogeneous and their compositions change with the experimental conditions, following systematic compositional trends. (2) The crystal distribution is homogeneous in all experiments (Fig. 3a–c). (3) Phase relations and compositions were identical in runs performed at identical conditions and for different run duration (24 h and up to 96 h), at high and at low temperatures (for B1 compare runs 62 and 61 with 45 and 42, respectively, and for B2 compare run 111 with 104; Table 3a and b). (4) Mineral–melt and mineral–mineral partitioning coefficients (for olivine, plagioclase, amphibole and Fe–Ti oxides) are in good agreement with published data from other studies (see below). (5) The formation of quench crystals was avoided (Fig. 3a–c) so that there is no need to distinguish between quench and stable phases or to perform integrative measurements of glass and quench crystals, as has been done in previous studies (e.g. Helz, 1976Go).


    RESULTS
 TOP
 ABSTRACT
 INTRODUCTION
 EXPERIMENTAL TECHNIQUES
 RESULTS
 DISCUSSION
 CONCLUSIONS
 REFERENCES
 
Phase relations
Experimental results and phase proportions are listed in Table 3. Phase relations for compositions B1 and B2 are shown in T–H2O diagrams (Fig. 4). The influence of water on phase relations is presented in terms of both bulk water content and contours of equal aH2O in the melt. The relation between aH2O and water content of the melt is given in Table 3.

Primitive MORB system (B1) at MnO–Mn3O4 buffer conditions
Olivine is the liquidus phase for all bulk water contents (Fig. 4a). At aH2O = 1 and aH2O = 0·6 the saturation boundary is at about 1125°C and 1150°C, respectively. In runs below 1000°C olivine is no longer stable. This is in agreement with the decreasing calculated modal abundance of olivine at 1000°C compared with 1050°C (Table 3a) and with changes from euhedral to rounded olivine crystals at 1050°C and 1000°C. Plagioclase and clinopyroxene saturation curves are almost identical and the relative order of crystallization is unknown. Plagioclase and clinopyroxene start to crystallize between 1100°C and 1050°C at aH2O = 1 and at about 1150°C at aH2O = 0·2. Magnetite was found below 1050°C. Amphibole is stable under nearly water-saturated conditions only. It is present in all runs at 950°C and at 1000°C with 4·70 wt % bulk H2O content. Orthopyroxene is stable in runs with 0·89 and 1·49 wt % bulk H2O content at 1000°C and in all runs at 950°C. The ilmenite stability field is restricted to 950°C in charges with 0·89 and 1·49 wt % bulk H2O content.

Differentiated MORB system (B2) at MnO–Mn3O4 buffer conditions
In contrast to B1, olivine was not observed in experiments using the B2 starting composition. Magnetite crystallizes as the liquidus phase for all bulk water contents (Fig. 4b) and its liquidus temperature is below 1150°C for a bulk water content of 4·50 wt %. Clinopyroxene is observed between 1100°C and 1050°C at aH2O = 1 and 1150°C and 1100°C for aH2O < 0·3. The plagioclase saturation curve depends strongly on aH2O. At water-saturated conditions plagioclase is stable only below 1000°C. At lower water activities the saturation temperature of plagioclase rises to 1100°C (aH2O = 0·25). The ilmenite saturation curve depends also on aH2O and is approximately 50°C below that of plagioclase. In contrast to B1, orthopyroxene is observed in B2 at higher temperature for low bulk water contents. It crystallizes at 1050°C for an aH2O of 0·38 (run 96; Table 3b) but is not stable at 950°C and 4·5 wt % bulk H2O.

Primitive MORB system (B1) at QFM buffer conditions
Olivine is the liquidus phase for all bulk water contents and starts to crystallize between 1125°C and 1150°C at water-saturated conditions (Table 3c; Fig. 4c). At aH2O < 0·4 olivine crystallizes at temperatures higher than 1150°C. The plagioclase and clinopyroxene saturation temperature is about 50°C below that of olivine. Amphibole is stable only in experiments at 950°C in which water-saturated conditions have been reached even for low bulk water contents. Ilmenite crystallizes in runs 151 and 150 at 950°C (1·12 and 0·55 wt % bulk water content, respectively).

The solidus temperature was reached in run 150 and crystals were too small to be analysed correctly. Thus, ilmenite as well as all other phases were identified only qualitatively in this experiment by back-scattered electron images.

At a given temperature, the phase diagrams at both low and high fO2 (Fig. 4) show variations in the phase assemblages within the fluid-saturated field. This is attributed to the effect of the dilution of the fluid phase by air (see discussion above), resulting in a slight decrease of aH2O in capsules with low bulk water content (higher N2/Ar ratio).

Phase chemistry
Olivine
XFo of olivines obtained at MnO–Mn3O4 buffer conditions are generally higher (XFo between 92 and 83; Fig. 5a) than at QFM buffer conditions (XFo between 88 and 66; Fig. 5b). At constant temperature, XFo varies as a function of bulk water content (e.g. at 1100°C from XFo92 to XFo84 for a bulk water content of 4·7 and 0·89, respectively; Fig. 5a). At high fO2 XFo falls with falling temperature from 1150 to 1050°C to minimum values of XFo89 (4·70 wt % bulk H2O content) and XFo83 (0·89 wt % bulk H2O content), but rises again at temperatures <1050°C. This is a consequence of increasing magnetite crystallization leading to slightly higher MgO and lower FeO* (total iron) concentrations in the melt (Figs 5 and 9; Table 4a). At low fO2, the minimum XFo is observed in olivine crystallizing at 950°C and is identical, independent of bulk water content (XFo of 66). This is related to melt Mg-number, which is almost identical in all 950°C experiments (ranging from 38 to 35 for all bulk water contents).



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Fig. 5. Olivine composition in B1 as a function of temperature and bulk water content at MnO–Mn3O4 buffer conditions (a) and QFM (b). Error bars correspond to the standard deviation of average olivine compositions. For bulk water contents of 4·70 and 0·89 wt % numbers indicate the proportion of magnetite (wt % mt).

 

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Table 4a: Electron microprobe analyses of run products for composition B1 (MnO–Mn3O4 buffer conditions)

 
One of the most significant minor elements in olivine is calcium (Libourel, 1999Go), with concentrations depending on XFo ranging between 0·19 wt % and 0·47 wt % CaO (Table 4a and c). It is generally accepted that neither oxygen fugacity, nor temperature or pressure, directly influence Ca partitioning (Roeder, 1974Go; Longhi et al., 1978Go; Watson, 1979Go; Jurewicz & Watson, 1988Go; Libourel, 1999Go). As demonstrated by Libourel (1999)Go, Ca concentration in olivine depends on the olivine composition as well as on the alkali and alumina content of the melt. Generally, the partition coefficient (CaOOlivine/CaOMelt, in wt %) increases with decreasing XFo and increasing melt alkali and CaO content. Figure 6 shows vs XFo obtained in this study. As expected from the generally high XFo and low melt alkali content, Ca concentration in olivine is typically low in our system. Comparison with other data from experimental studies on more iron-rich, tholeiitic and other basaltic systems confirms values obtained in this study, suggesting equilibrium conditions with respect to Ca partitioning between olivine and melt.



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Fig. 6. vs the forsterite content of olivine. Additional data for various natural basaltic compositions from other studies as in Fig. 12. Error for is typically ±0·004 and has been obtained by error propagation calculating from the standard deviation of CaO concentrations in olivine and melt. Errors in olivine compositions are given in Fig. 5.

 
Pyroxene
Clinopyroxene and orthopyroxene obtained in runs with B1 at high fO2 vary only moderately with changing experimental conditions and have an average composition of En45Fs12Wo43 (±1·3 mol %) and En82Fs1Wo3 (±0·9 mol %), respectively (Table 4a). Clinopyroxene synthesized in experiments with composition B2 is characterized by a larger compositional variation (Table 4b). At water-saturated conditions clinopyroxene has an average composition of En42Fs12Wo46 (±2·3 mol %; 4·50 wt % bulk water content), which changes continuously with decreasing bulk water content to En48Fs13Wo39 (±1·4 mol %; 0·74 wt % bulk water content). B2 orthopyroxene in equilibrium with the most En-rich clinopyroxene crystallized at 0·74 wt % bulk water content has the highest Wo content (En71Fs20Wo9 ± 2·2 mol %). All other orthopyroxenes vary only little in their mole proportions (En79Fs16Wo5 ± 2 mol %), showing slight decreases in Fs and Wo contents with increasing bulk water content. At QFM buffer conditions clinopyroxene has an average composition of En44Fs14Wo42 ± 2 mol %. The average of clinopyroxene [defined as (XCpx–FeO/XCpx–MgO) x (XMelt–MgO/XMelt–FeO)] is 0·26 but generally increases with melt Mg-number. As reported by Hoover & Irvine (1977)Go and Toplis & Carroll (1995)Go, values increase independently of fO2 with increasing melt Mg-number up to 0·26 (for melt Mg-number of about 40). At QFM buffer conditions for relatively low melt Mg-number, the obtained values are in good agreement with published data (Table 4). For melt Mg-number above 50, the deviates from the linear trend with values up to 0·41. The same observation has been made for partitioning of Mg and Fe2+ between clinopyroxene and melt under MnO–Mn3O4 buffer conditions, which confirms that there is no dependence of on fO2 (Toplis & Carroll, 1995Go). It is noteworthy that the bulk water content has no influence on .


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Table 4b: Electron microprobe analyses of run products for composition B2 (MnO–Mn3O4 buffer conditions)

 
Plagioclase
The composition of plagioclase as a function of temperature and H2O is shown in Fig. 7. The anorthite (An) content decreases continuously by ~0·05 mol % per °C with falling temperature for all bulk water contents. Plagioclase synthesized at high fO2 is slightly more An-rich than that crystallized at similar T–H2O conditions and low fO2. Consequently, the highest An contents (An88, 1050°C; An79, 950°C) are obtained for B1 in runs with 4·70 wt % bulk H2O content (Fig. 7a). The most Ab-rich plagioclase for B1 (An66; Fig. 7b) is stable at 950°C with 1·12 wt % bulk water content. In agreement with previous studies (e.g. Turner & Verhoogen, 1960Go; Carmichael et al., 1974Go; Panjasawatwong et al., 1995Go; Martel et al., 1998Go; Scaillet & Evans, 1999Go; Berndt et al., 2001Go), at a given temperature the An content of plagioclase increases with increasing melt water content and therefore increasing aH2O. However, at fluid-saturated conditions, the plagioclase compositions are also systematically more Ca rich with increasing bulk water content, although the same melt water content (aH2O = 1) apparently has been reached in runs at lower temperatures. This is attributed to the presence of N2 in the capsules (as already discussed), resulting in a slight decrease of water activity with decreasing bulk water content and higher N2/H2O ratio.



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Fig. 7. Plagioclase composition in B1 as a function of temperature and bulk water content at MnO–Mn3O4 buffer conditions (a) and QFM (b). Errors bars correspond to the standard deviation of average plagioclase compositions. Water contents are given as bulk water contents. Numbers indicate aH2O of the melt.

 
The direct influence of H2O on plagioclase–liquid equilibrium compositions is shown in Fig. 8. For a constant Ca/Na ratio in the melt, the An content of plagioclase obtained at nearly water-saturated conditions (4·55–5·25 wt % H2O in melt) is noticeably higher when compared with An contents in plagioclases in equilibrium with melts containing about 2 wt % H2O. Consequently, [defined as molar (Ca/Na)Plag/(Ca/Na)Liq] increases with increasing aH2O of the melt. Continuous lines in Fig. 8 indicate values given by Sisson & Grove (1993a)Go for plagioclase–melt pairs obtained in high-alumina basalts with 4 wt % H2O in the melt at 100 MPa (; Sisson & Grove, 1993bGo) and 2 wt % H2O in the melt at 200 and 500 MPa (; Baker & Eggler, 1987Go). This indicates that the effect of pressure variations between 100 and 500 MPa on is negligible. As emphasized by Sisson & Grove (1993aGo,) the pressure dependence of in dry systems in the range 1 atm to 20 kbar is always significantly lower than the influence of water. values obtained in this study for given melt water contents in primitive and differentiated MORB compositions agree well with the data of Sisson & Grove (1993aGo, 1993bGo) and Baker & Eggler (1987)Go for high-alumina basalts. This confirms that plagioclase composition mainly depends on aH2O and melt Ca/Na.



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Fig. 8. Ca/Na ratios for plagioclase–melt pairs in B1 obtained at water-saturated conditions [aH2O = 1; melt water contents calculated after Burnham (1979)Go; Table 3] and c. 2 wt % H2O in the melt. Continuous lines show, after Sisson & Grove (1993a)Go for plagioclase–melt pairs in high-alumina basalt (Sisson & Grove, 1993b)Go at 100 MPa and about 4 wt % H2O in melt (), and about 2 wt % H2O in melt at 200 and 500 MPa (Baker & Eggler, 1987Go; KD ~ 1·7).

 
Compared with experimental studies in dry systems (e.g. Toplis & Carroll, 1995Go), the An content of plagioclase obtained in our study decreases only by about 0·05 mol % per °C [compared with 0·5 mol % per °C in the study of Toplis & Carroll (1995)Go for a given bulk water content with falling temperature (Fig. 7)]. As discussed above, in water-bearing systems, for a given bulk water content, increasing crystal fraction (as a result of falling temperature) results in an increase of melt water content. Thus, the effect of decreasing Ca/Na in the melt with progressive crystallization, resulting in a strong decrease of An content in dry systems, is compensated by increasing melt water content.

Amphibole
According to the classification of Leake et al. (1997)Go the synthesized amphibole is pargasite. The Mg-number of amphibole (calculated with all iron as FeO*) increases with increasing bulk water content (Table 4). The number of Si atoms in the tetrahedral position of the amphibole synthesized at 1000°C is lower than that of amphibole obtained at 950°C, whereas AlIV increases with rising temperature. This is in agreement with previous experimental studies (Helz, 1981Go; Sisson & Grove, 1993aGo). At 950°C, Si and Al remain constant for all bulk water contents. Sisson & Grove (1993a)Go showed that the tetrahedral Al/Si ratio of amphibole is linearly related to the Al/Si ratio of the melt and can be described as . An average of 1·01 (±0·08) from coexisting liquid–amphibole pairs obtained in B1 and B2 agrees well with the value of 0·94 (±0·06) given by Sisson & Grove (1993a)Go for liquid–amphibole couples in compositions ranging from high-alumina basalt to high-silica rhyolite.

The occurrence of amphibole in natural systems is often used to argue whether magmas were ‘dry’ or hydrous in a broadly qualitative sense. Our results support previous experimental findings in hydrous basaltic and calc-alkaline systems (e.g. Holloway & Burnham, 1972Go; Helz, 1973Go; Spulber & Rutherford, 1983Go; Sisson & Grove, 1993aGo; Johnson et al., 1994Go) showing that a relatively high amount of H2O in the melt is necessary to stabilize amphibole (~5 wt % in our study). In our study the stability field of amphibole is always restricted to runs under nearly water-saturated conditions (Fig. 4); however, not all experiments containing a free fluid phase contain amphibole, probably because of higher N2/H2O ratio in charges with low bulk water contents and thus slightly lower aH2O (see above). This indicates that very small variations in aH2O may influence amphibole stability. However, the absence of amphibole is clearly not evidence for ‘dry’ conditions.

Fe–Ti oxides
Owing to the small size of magnetite and ilmenite crystals, analyses of these phases are often contaminated by the surrounding glass as indicated by variable SiO2 contents (Table 4a and b). However, no attempt was made to correct the analyses.

Magnetite in B1 and B2, which is stable only at high fO2, is characterized by relatively low ulvöspinel contents [XUsp; calculated after Andersen et al. (1993)Go] ranging from 5 to 19 mol %, depending mainly on the bulk water content and, to a lesser extent, on temperature. XUsp systematically increases with decreasing bulk water content for all temperatures (Table 4a and b).

For a given temperature, XUsp in B1 experiments with different bulk water contents remains relatively constant (e.g. 8 and 9·5 mol % at 1050°C and 950°C, respectively, in runs with between 4·70 and 0·89 wt % bulk H2O content). In contrast to B1, magnetite from B2 shows a stronger XUsp variation as a function of temperature. At 1050°C and 950°C, the difference in XUsp between experiments with 4·50 and 0·74 wt % bulk water content is 14 and 4 mol %, respectively. MgO contents of B1 and B2 magnetite decrease with falling temperature for constant bulk water contents and with decreasing bulk water content for a given temperature. This evolution of MgO content in magnetite is related to the Mg-number of the melt. Al2O3 content also decreases with falling temperature for a constant bulk water content.

The ilmenite content [XIlm; calculated after Andersen et al. (1993)Go] of rhombohedral oxides synthesized in B2 decreases regularly with falling temperature (from XIlm = 43 mol % at 1050°C to XIlm = 33 mol% at 950°C for 0·74 wt % bulk water content; Table 4b) and increases systematically at constant temperature with decreasing bulk water content. The same effect of water is observed for B1 ilmenite crystallized in runs with 0·89 and 1·49 wt % bulk water content at 950°C, which have generally higher XIlm than those obtained at similar conditions in B2. Compared with magnetite, MgO, Al2O3, and MnO contents in ilmenite are generally lower. As for magnetite, MgO content falls with decreasing bulk water content and falling temperature.

The results of Bacon & Hirschmann (1988)Go can be used as a test for coexisting Fe–Ti oxide equilibrium using Mg/Mn partitioning between magnetite and ilmenite. Fe–Ti oxide pairs from B1 and B2 experiments (Table 4a and b) satisfy the Mg/Mn partitioning criterion of Bacon & Hirschmann (1988)Go, having an average magnetite log(Mg/Mn) of 1·26 (± 0·13) and ilmenite log(Mg/Mn) of 1·40 (± 0·08).

Glass composition at MnO–Mn3O4 buffer conditions
Compositions of glasses obtained in B1 and B2 experiments are given in Table 4a and b and the concentrations of SiO2 and FeO* are plotted against temperature in Figs 9 and 10. Depending on experimental conditions, glass compositions range from basaltic through dacitic to rhyolitic (run 106; classification using the total alkalis–silica (TAS) diagram after, for example, Le Bas et al. (1986)Go] and follow a calc-alkaline differentiation trend. SiO2, Na2O, and K2O concentrations continuously increase for B1 and B2 with falling temperature and decreasing bulk water content. However, compared with B2, SiO2 contents of B1 vary only slightly for a given temperature with changing bulk water content (Figs 9a and 10a). The maximum SiO2 concentration is about 64 wt % in B1 and 70 wt % in B2. Despite different initial Na2O contents of B1 and B2 the same maximum Na2O concentration of about 5·5 wt % to 4 wt % is reached in both systems for the lowest and highest bulk water contents, respectively (at 950°C).



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Fig. 9. B1 (MnO–Mn3O4 buffer) melt oxide concentrations of SiO2 (a) and FeO* (b) (normalized to 100 wt %) as a function of bulk water content and temperature. Errors bars correspond to the standard deviation of multiple electron microprobe analyses (Table 4). All analyses are normalized to 100 wt %. Dashed lines indicate calculated melt compositions of experiments 47 and 46 (see comments in ‘Analytical techniques’ section).

 
The MgO and CaO concentrations in glasses from B1 and B2 decrease with falling temperature. In runs with high bulk water contents (4·70 and 4·50 wt % H2O in B1 and B2, respectively), the CaO remains constant (B1) or rises slightly (B2), but decreases once clinopyroxene begins to crystallize. At constant temperature, MgO and CaO contents fall with decreasing bulk water content, in contrast to SiO2, Na2O and K2O. MgO contents decrease from their initial values of 9·77 wt % (B1) and 6·49 wt % (B2) to a minimum of approximately 2·5 wt % (highest bulk water contents) and 1·2 wt % (lowest bulk water content).

The TiO2 concentrations in B1 glasses decrease with increasing bulk water contents, which can be correlated with the increasing XUsp in magnetite with increasing bulk water content (see above). For a given bulk water content TiO2 concentrations first increase and then decrease with falling temperature. The maximum value is reached at 1100°C for 0·89 and 1·49 wt % bulk water content and at 1000°C for 2·53 and 4·70 wt % bulk water content. In B2, TiO2 concentrations at low temperatures are mainly controlled by the crystallization of ilmenite. In all experiments containing ilmenite, the TiO2 concentration in the glass is below 1·3 wt %. In addition, TiO2 contents show a general decrease with falling bulk water content and temperature.

The evolution of FeO* content in B1 and B2 glasses is similar to that of TiO2. In B1, the maximum FeO* values are observed at 1100°C (10·19 wt % for 1·49 wt % bulk water content; 10·98 wt % for 0·89 wt % bulk water content; Fig. 9b). The FeO* concentration in melts from experiments with 2·05 and 4·70 wt % bulk water content show only little variation down to 1050°C (about 8·9 wt %). In B2, FeO* contents of all glasses in experiments containing ilmenite are below 5·8 wt % (Fig. 10b). In addition to the effect of ilmenite, FeO* also decreases with falling temperature (for aH2O = 1, 4·5 wt % bulk water) and with increasing water content of the melt (compare runs at 1100°C; Fig. 10b).



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Fig. 10. B2 (MnO–Mn3O4 buffer) melt oxide concentrations of SiO2 (a) and FeO* (b) (normalized to 100 wt %) as a function of bulk water content and temperature. Further details are given in the caption of Fig. 9.

 
Glass composition at QFM buffer conditions
Experimental melt compositions are given in Table 4c. The evolutions of melt SiO2 and FeO* with temperature as a function of bulk water content are shown in Fig. 11. In contrast to oxidizing conditions, melts follow a tholeiitic differentiation trend (see Figs 14 and 15;Irvine & Baragar, 1971Go; Miyashiro, 1974Go), ranging from basaltic to andesitic compositions. SiO2 content of the melt (Fig. 11a) increases with falling temperature and bulk water content up to 61 wt % (run 151). FeO* concentration generally increases with falling temperature, but shows significant variations with changing bulk water content (Fig. 11b). For water-saturated melts, FeO* content increases slightly from 1150°C to 950°C (8·24 wt % at 1150°C and 8·97 wt % at 950°C). For lower bulk water contents, FeO* first increases with falling temperature and decreases at temperatures below 1050°C. The highest FeO* is observed for about 0·5 wt % bulk water content with 10·95 wt % FeO* at 1050°C (run 143). The FeO* content in water-saturated melts at 950°C is identical in runs 153 and 152 (no ilmenite present). However, the melt FeO* content is significantly lower in run 151 containing ilmenite. With falling temperature and decreasing bulk water content, the melt MgO and CaO concentrations also decrease. In contrast, Na2O and K2O rise in concentration with falling temperature and bulk water content. A maximum TiO2 content is reached at 1000°C and decreases generally in all experiments at 950°C.



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Fig. 11. B1 (QFM buffer) melt oxide concentrations of SiO2 (a) and FeO* (b) (normalized to 100 wt %) as a function of bulk water content and temperature. Further details are given in the caption of Fig. 9.

 

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Table 4c: Electron microprobe analyses of run products for composition B1 (QFM buffer conditions)

 

    DISCUSSION
 TOP
 ABSTRACT
 INTRODUCTION
 EXPERIMENTAL TECHNIQUES
 RESULTS
 DISCUSSION
 CONCLUSIONS
 REFERENCES
 
Comparison of phase relations at high and low fO2
Phase relations obtained for the B1 starting composition at oxidizing and reducing oxygen fugacities can be compared to estimate the effect of fO2, as all other parameters are equal (pressure, temperature, bulk water content). For both high and low oxygen fugacities olivine is the liquidus phase crystallizing at similar temperatures between 1150°C and 1100°C, depending on bulk water content. In contrast to B1 phase relations at oxidizing conditions, orthopyroxene is not stable at low fO2. This is in agreement with previous studies (e.g. Grove & Juster, 1989Go), which show that decreasing melt Mg-number (as a result of decreasing fO2) strongly confines the low-Ca pyroxene stability. Because orthopyroxene is not stable at reducing conditions (melt Mg-number of about 35 at 950°C; Table 4c), olivine is present in the low-temperature runs at 950°C, in contrast to oxidizing conditions (melt Mg-number of 61–68). Magnetite did not crystallize at low fO2 because of the lower melt Fe3+/Fe2+ ratio. Ilmenite stability is known to be less dependent on the oxidation state of the melt (e.g. Toplis & Carroll, 1995Go), and this mineral is observed at the same temperature and bulk water contents in both reducing and oxidizing conditions. The clinopyroxene and plagioclase saturation is also widely independent of fO2, as both phases crystallize between 1150°C and 1050°C.

Mg/Fe partitioning between olivine and melt
Partitioning of Fe and Mg between olivine and melt, expressed as (Roeder & Emslie, 1970Go) is known to show only a small dependence on melt composition, temperature and fO2, with a value of about 0·3 (± 0·02). The determined in this study is slightly higher with an average value of 0·33 (± 0·01). This higher value is in agreement with the results of Ulmer (1989)Go, who showed a slight positive pressure dependence of , thus suggesting that equilibrium conditions between olivine and melt have been reached in our experiments. Although is generally assumed to be constant, implying a linear relationship between XFo and melt Mg-number, it is emphasized that small but significant deviations occur as a function of the melt Mg-number. This is illustrated in Fig. 12, which shows that XFo decreases with the melt Mg-number over a wide range of bulk compositions, temperatures and oxygen fugacities. Toplis & Carroll (1995)Go observed, in agreement with the data of Longhi & Pan (1988)Go and Shi (1993)Go, that values increase up to 0·4 for melt Mg-number <30. This has been interpreted as due to the non-ideality of Fe2+–Mg mixing either in the olivine (Wiser & Wood, 1991Go; Toplis & Carroll, 1995Go) or in the melt (Hoover & Irvine, 1977Go), which leads to relatively lower Mg/Fe2+ in olivine than in the coexisting melt (Fig. 12). Our data extend the available database towards high melt Mg-number. Using this database (obtained at various P, T, aH2O, fO2 and bulk compositions), we show that the equilibrium composition of olivine–liquid pairs can be described as a logarithmic function of the melt Mg-number in the pressure range 0·1–200 MPa for both dry and hydrous systems at various fO2:

(1)
The curve in Fig. 12 represents the calculated XFo as a function of the liquid Mg-number using equation (1).



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Fig. 12. Variation of forsterite content (mol % Fo) as a function of melt Mg-number (Mg#). Olivine compositions and corresponding melt Mg-number from the following studies have been added: Toplis & Carroll (1995)Go: 1 atm, QFM + 1 to QFM – 2, 1170–1050°C, ferrobasaltic composition representing the parental liquid of the Skaergard intrusion; Tormey et al. (1987)Go: only 1 atm experiments were considered, QFM, 1240–1152°C, MORB composition dredged near the Kane Fracture Zone; Yang et al. (1996)Go: 1 atm, QFM, 1251–1110°C, six MORB glasses; Sisson & Grove (1993a)Go: 200 MPa, NNO, H2O saturated, 1050–925°C, high-alumina basalts; Snyder et al. (1993)Go: 1 atm, QFM to 0·5 log units above iron–wüstite (IW), 1192–1061°C, ferrobasaltic compositions representing parental liquids, Newark Island layered intrusion, Kiglapait intrusion, Skaergard intrusion and a tholeiitic composition from Langjökull, Iceland; Grove & Bryan (1983)Go: 1 atm, QFM, 1245–1131°C, four basaltic compositions (primitive basalts from the FAMOUS area, one primitive basalt characterized by ‘plume-type’ geochemistry and one basalt with typical parental composition near the Kane Fracture Zone). The curve is a logarithmic fit to the data for anhydrous to water-saturated basaltic systems crystallizing under low pressure (1 atm–200 MPa).

 
Effect of H2O and fO2 on olivine and orthopyroxene stability
H2O is known to depolymerize melts and thus enhance the stability field of depolymerized phases such as olivine (e.g. Kushiro, 1975Go; Ulmer, 1989Go). The highest proportion of olivine in B1 at high fO2, calculated by mass balance, is reached at 1050°C for all bulk water contents (Table 4a). This is confirmed by the shape of the olivines. At this temperature and below, olivine textures change from euhedral to rounded crystals, indicating a partial resorption during the experiment (partial resorption of olivine is probably the result of a rapid growth of this mineral in the first minutes of the experiment when compared with the other mineral phases). Toplis & Carroll (1995)Go made similar observations for olivine in a dry ferrobasaltic system at slightly higher temperatures (1070–1130°C) for fO2 in the range QFM + 1 to QFM – 2. Toplis & Carroll (1995)Go observed a falling onset temperature of olivine resorption with decreasing fO2. However, the onset of olivine resorption in our study is observed at lower temperatures despite the fact that fO2 is higher in B1 runs at MnO–Mn3O4 buffer conditions than in the study of Toplis & Carroll (1995)Go. A possible explanation is that the higher depolymerization of our hydrous melts leads to increasing stability and activity of olivine (e.g. Kushiro, 1975Go). This is supported by the study of Spulber & Rutherford (1983)Go showing that olivine is stable in a MORB composition until the solidus is reached at low fO2 (graphite–methane buffer) and hydrous conditions (aH2O ~ 0·6), suggesting that the olivine stability field is extended to lower temperatures with decreasing fO2 and increasing aH2O in basaltic systems. This is also confirmed by the experiments from this study at low fO2 in which olivine is always a stable phase (Fig. 4c).

As emphasized by Juster et al. (1989)Go and Toplis & Carroll (1995)Go, high silica activities of the melt promote resorption of olivine involving a reaction of the type Mg2SiO4ol + SiO2glass = 2MgSiO3pig. At high fO2, in B1 the orthopyroxene saturation curve (opx-in curve; Fig. 4a) and olivine-out curve are not identical, but overlap at 1000°C and 0·89 and 1·49 wt % bulk water content. Because the resorption of olivine roughly parallels the crystallization of orthopyroxene, we suggest that the occurrence of orthopyroxene is related to the reaction described above. Furthermore, orthopyroxene crystallizes first in runs with lower bulk water contents and thus higher crystal fraction and higher silica activity of the melts. In the fractionated B2 composition, olivine is absent. Therefore, the generally higher melt SiO2 contents of the B2 compositions expand the stability field of orthopyroxene, particularly at low aH2O up to 1050°C.

Effect of H2O and fO2 on Fe–Ti oxide stability
The stability of Fe–Ti oxides in basaltic systems has been widely investigated because of its important influence on differentiation paths. Generally, it is difficult to discriminate between the individual effects of H2O, fO2 and melt composition (and thus activities of critical components) on the stability of ilmenite and magnetite, because aH2O also influences the prevailing fO2, which in turns controls the Fe2O3 content in the melt. As shown by, for example, Snyder et al. (1993)Go and Toplis & Carroll (1995)Go, for dry basaltic systems the magnetite stability field expands to high temperature with increasing fO2 (as a result of the increasing ferric iron content of the melt). In contrast, ilmenite is stable at lower fO2 and is rather a function of melt TiO2 content than of melt oxidation state (Thy & Lofgren, 1994Go; Toplis & Carroll, 1995Go). In this study, for B1 the stability field of ilmenite is identical for reducing and oxidizing conditions (Fig. 4a and c). This supports the hypothesis of Toplis & Carroll (1995)Go that ilmenite is nearly independent of melt oxidation state but depends mainly on melt TiO2 content. As mentioned above, runs with low bulk water content at low temperatures have water activities less than unity despite fluid saturation having been reached in these experiments. Thus, melt fraction decreases with decreasing bulk water contents, resulting in higher TiO2 concentrations. Therefore, at a given temperature, ilmenite stability is enhanced with decreasing bulk water content, independently of fO2. This is illustrated in Fig. 4a and c, showing that ilmenite is stable at 950°C in samples with bulk water contents between 0·55 and 1·5 wt %, but not at higher bulk water contents.

Magnetite is stable in B1 runs performed at high fO2, but not in the experiments conducted at the QFM buffer. At high fO2, magnetite crystallizes between 1100°C and 1050°C, but is not the liquidus phase as olivine, plagioclase and clinopyroxene are stable at higher temperatures (Fig. 4a). This is in contrast to studies performed under dry conditions in basaltic systems at high fO2, in which magnetite is usually the liquidus phase, or at least a near-liquidus phase (Roeder, 1974Go; Grove & Juster, 1989Go; Juster et al., 1989Go) with a crystallization temperature of about 1100°C (e.g. Thy & Lofgren 1994Go), independent of bulk composition. A possible explanation for the lower saturation temperature in hydrous MORB systems is that the solubility of magnetite is higher in hydrous melts than in dry systems. Toplis & Carroll (1995)Go showed [with additional data of Juster et al. (1989)Go, Snyder & Carmichael (1992)Go and Thy & Lofgren (1994)Go] that the ferric iron content of magnetite-saturated liquids is a linear function of the inverse temperature for a variety of dry basaltic compositions, independently of fO2 (Fig. 13). The results at high fO2 show that magnetite saturation is reached at lower temperatures for a given melt Fe2O3 content compared with dry systems. This suggests that the activity of Fe2O3 in the melt is probably lowered by H2O compared with dry systems. The absence of magnetite in B1 at the QFM buffer can be explained by the lower melt Fe2O3 concentration (because of the low fO2) in combination with the effect of dissolved water (Fig. 13; note that the FeO* contents are generally higher in B1 melts obtained at low fO2 than those from experiments performed under oxidizing conditions).



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Fig. 13. Ln Fe2O3 content of melts as a function of the inverse temperature. Only experiments with the highest (between 4·7 and 4·5 wt %) and lowest (between ~0·5 and 0·89 wt %) bulk water contents are considered. Continuous line indicate experiments conducted at high fO2 (MnO–Mn3O4 buffer) in which magnetite was a stable phase. Dashed line shows in Fe2O3 contents of magnetite-saturated dry melts from Toplis & Carroll (1995)Go for various compositions.

 
Differentiation trend at high and low oxygen fugacities
Residual melt compositions obtained in runs at high and low fO2 allow us to estimate the influence of H2O and fO2 on the liquid line of descent, as all other parameters (bulk composition, bulk water content, temperature and pressure) were similar. The residual liquids obtained at fO2 conditions corresponding to the QFM buffer show a general increase in melt FeO*/MgO ratio with falling temperature as a result of the absence of magnetite among the crystallizing phases. These melts follow, independently of bulk water content, a tholeiitic differentiation trend [Figs 14 and 15; classification after Irvine & Baragar (1971)Go and Miyashiro (1974)Go]. This is in agreement with previous studies performed in basaltic systems at lower fO2, in which Fe–Ti oxides are not stable until a significant amount of silicates crystallized and the melt is enriched in FeO* (Spulber & Rutherford, 1983Go; Juster et al., 1989Go; Snyder et al., 1993Go) following a tholeiitic differentiation trend. Residual B1 melts from experiments at high fO2 coexist widely with magnetite and are consequently depleted in FeO* following a calc-alkaline differentiation trend (Figs 14 and 15). At high fO2, for the lowest bulk water contents in B1, magnetite appears 100°C or more below the liquidus (Fig. 4a). With increasing bulk water content, the magnetite appearance temperature is unaffected, but the liquidus, defined by silicates, is depressed by about 50°C (highest bulk water content). Thus, higher water contents cause magnetite to appear closer to the liquidus, as described by Sisson & Grove (1993a)Go. Consequently, at MnO–Mn3O4 buffer conditions the liquid line of descent enters the calc-alkaline field at an earlier stage of differentiation for high bulk water contents compared with low bulk water contents (Fig. 15). At these high fO2 values the potential for changing the differentiation trend with water is low, as magnetite crystallizes early and in relatively high proportions for all bulk water contents, preventing a change from a calc-alkaline to a tholeiitic trend in primitive MORBs. However, it could be expected that for oxygen fugacities corresponding to the Ni–NiO buffer, the addition of only water can change MORB differentiation path from tholeiitic (dry conditions) to calc-alkalic (water-saturated) by the early stabilization of Fe–Ti oxides under hydrous conditions, as observed for calc-alkaline systems by Sisson & Grove (1993a)Go.



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Fig. 14. FeO*/MgO ratio of residual melts vs melt SiO2 content. TH (tholeiitic)–CA (calc-alkaline) dividing line is from Miyashiro (1974)Go. Water contents are given as bulk water contents.

 


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Fig. 15. Experimental residual liquids projected into the AFM, total alkali (Na2O + K2O)–total iron (FeO*)–MgO ternary diagram (calculated from melt composition in wt %). Only experiments with the highest (between 4·7 and 4·5 wt %) and lowest (between ~0·5 and 0·89 wt %) bulk water contents are shown. TH (tholeiitic)–CA (calc-alkaline) dividing line is from Irvine & Baragar (1971)Go.

 
Mechanisms of melt FeO* enrichment during early stages of differentiation
At low as well as at high fO2, the melt FeO* content increases with falling temperature in the initial differentiation stages (Figs 9b, 10b and 11b). When comparing the melt FeO* content at a given temperature as a function of the bulk water content, the greatest differences can be observed at 1050°C at reducing conditions. At these temperatures the highest melt FeO* is obtained for the lowest bulk water content. This cannot be an effect of enhanced Fe–Ti oxide stability at high melt water contents, as magnetite is not stable under these conditions (Fig. 4c).

An important factor that may control the melt FeO* enrichment during initial differentiation stages is the proportion of plagioclase and Fe–Mg silicates. As shown by, for example, Yoder (1965)Go, Gaetani et al. (1993)Go and Sisson & Grove (1993a)Go, H2O suppresses the proportion of plagioclase as a highly polymerized phase relative to mafic Fe–Mg silicates (e.g. olivine, pyroxene, amphibole). Thus, crystallization of higher proportions of Fe–Mg silicates and destabilization of plagioclase at high water contents depletes the melt in Fe and Mg. The plagioclase/Fe–Mg-silicate ratio is shown in Fig. 16 for the highest and lowest bulk water contents at oxidizing and reducing conditions, respectively. As expected, the plagioclase/Fe–Mg-silicate ratio is significantly higher in runs with low bulk water content and independent of the fO2. Consequently, residual melts obtained from experiments performed at low water contents should show systematically higher melt FeO* concentrations than more hydrous liquids. However, this is the case only for those runs conducted at high temperatures; it is not observed for the low-temperature runs, as melt FeO* concentrations are almost similar at a temperature of 1000°C (Figs 9b, 10b and 11b). It should be noted that the composition of the melt, and thus its FeO* content, is not only dependent on the ratio of plagioclase/mafic minerals in combination with Fe–Ti-oxide crystallization, as magnetite is not stable in the low-fO2 runs (Fig. 4c), but is also a complex function of the proportion and composition of clinopyroxene and olivine, which vary with water content. At 950°C the FeO* enrichment process is even reversed compared with the high-temperature situation: the residual melt obtained from experiments performed at low bulk water content (1 wt % H2O) shows the lowest FeO* concentration. This is obviously due to the presence of ilmenite in combination with a very low melt fraction (7·9 wt %) in this run driving the FeO* content in the melt to lower values (Table 3c, Fig. 11b).



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Fig. 16. Plagioclase/mafic phase ratios in B1 vs melt fraction (in wt %; both calculated by mass balance). Only experiments with the highest (between 4·7 and 4·5 wt %) and lowest (between ~0·5 and 0·89 wt %) bulk water contents are plotted.

 
Fractionation effects
A perfect fractional crystallization path requires a continuous removal of solids from the system. In our study we have investigated two compositions at high fO2, B1 and B2, where B2 corresponds to the composition of the residual melt of a run in the B1 system after 50 wt % crystallization and a bulk water content of 0·89 wt % (run 42, Table 3a). Thus, only one fractionation step has been carried out. This fractionation event is far from being representative of natural fractionation steps but illustrates the influence of fractionation on liquid line of descent and phase relations.

Experimental results from the evolved B2 composition show that phase relations are different from B1 (Fig. 4a and b). Magnetite is the liquidus phase in B2 because of the high fO2 and the melt Fe2O3 content, which is higher than in B1. Stability fields of both orthopyroxene and ilmenite are enhanced as a result of the higher aSiO2 and of generally higher melt TiO2 concentration, respectively. The curves of equal aH2O are shifted to lower temperatures because of the generally lower crystal fraction in B2 (Fig. 4b). Mineral and melt compositions produced in B2 are different from those in B1 and are consistent with equilibrium compositions in more evolved systems. Our results also show that starting with a primitive MORB, a quartz andesitic melt can be obtained without any fractionation step (e.g. B1, 12·6% melt, run 48), and a rhyolitic–trondhjemitic melt can already be obtained after one fractionation step (B2, 14% melt, run 106).

Implications for the origin of SiO2-rich residual melts in MORB systems
Always included in the MORB-derived gabbroic section of the oceanic crust are small, but ubiquitous, amounts of felsic, evolved rocks, the so-called oceanic plagiogranites (e.g. Dick et al., 1991Go). Such rocks are commonly found in ophiolites (e.g. Coleman & Peterman, 1975Go; Malpas, 1979Go; Jenner et al., 1991Go). The processes discussed to generate these SiO2-rich melts are: (1) crystal–liquid differentiation from a basaltic magma (e.g. Arth et al., 1978Go; Pedersen & Malpas, 1984Go; Martin, 1987Go; Niu et al., 2002Go); (2) partial melting of gabbro, basalt, or amphibolite (e.g. Flagler & Spray, 1991Go; Springer & Seck, 1997Go); (3) immiscibility between an Fe-enriched and a silicic residual liquid (Dixon & Rutherford, 1979Go). There is, however, no evidence in the experiments that residual melts become immiscible at later stages of differentiation. SiO2-rich residual melts containing more than 60 wt % SiO2 are produced in the B1 crystallization experiments under oxidizing and reducing fO2 conditions at 950°C (Fig. 14). As expected, the B1 residual liquids obtained under high fO2 are more SiO2 rich than those at reducing conditions, as a result of the crystallization of magnetite at high fO2, which causes a stronger SiO2 enrichment of the melt (e.g. Toplis & Carroll, 1995Go; about 64 wt % SiO2 in residual melts at the MnO–Mn3O4 buffer and about 60 wt % SiO2 in melts at the QFM buffer at 950°C). Thus, residual melts at 950°C are plagiogranitic in terms of SiO2 and K2O, as natural plagiogranites have bulk SiO2 contents between 60 and 75 wt % (e.g. Coleman & Peterman, 1975Go; Fig. 17). Compared with natural plagiogranite compositions (see Koepke et al., 2004Go, table 4) the Ca-numbers [100 x XCaO/(XCaO + XNaO0·5)] of the experimental melts of primitive B1 are very high, implying that potential plagioclase crystallizing in these liquids would be too An rich. The Ca-number values of the plagiogranitic melts of the more fractionated B2 starting composition match those found in natural plagiogranite compositions, indicating that fractionation processes need to be involved to reach the typical Ab-rich plagioclases of natural plagiogranites and also the high bulk SiO2 contents (>70 wt %) of some natural rocks.



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Fig. 17. Liquid lines of descent in log K2O vs SiO2 (wt %) (normalized to a total of 100 wt %; all bulk water contents are included) for B1 and B2 at QFM and MnO–Mn3O4 buffer conditions. +, natural plagiogranites from different tectonic settings (see Koepke et al. 2004Go, table 4). Included is the field for oceanic plagiogranites after Coleman & Donato (1979)Go.

 
However, typical bulk FeO* contents in plagiogranites are in the range of 1–7 wt %, which does not match values for the liquids obtained under QFM buffer conditions as a result of the tholeiitic differentiation trend caused by the absence of magnetite (with about 9 wt % melt FeO* content in the most evolved melts of B1; Fig. 11b). In contrast, residual liquids produced under oxidizing conditions show melt FeO* contents of about 5 wt %, corresponding to common bulk iron contents found in natural plagiogranites. This does, however, not mean that generation of plagiogranites takes place at such high fO2. Fractionation of B1 at the QFM buffer would also result in FeO* depletion and SiO2 enrichment of the melt as soon as the crystallization temperature of magnetite is reached. It can be noted that this temperature is significantly lower at QFM than at MnO–Mn3O4 buffer conditions. As reported by Dick et al. (2000)Go and Desmurs et al. (2002)Go, there is indeed evidence for Fe–Ti-oxide fractionation in natural MORB systems, which is apparently required to produce plagiogranites with typical FeO* contents of about 5 wt %.


    CONCLUSIONS
 TOP
 ABSTRACT
 INTRODUCTION
 EXPERIMENTAL TECHNIQUES
 RESULTS
 DISCUSSION
 CONCLUSIONS
 REFERENCES
 
H2O and fO2 are found to be important factors in controlling solid phase compositions and stability in a MORB system. It has been demonstrated that changing aH2O influences significantly the Mg/Fe ratio in iron-bearing phases such as olivine as a result of changing fO2. Furthermore, increasing aH2O influences Fe–Ti oxide compositions by raising the fO2 of the charge. values for plagioclase obtained in this study for a given melt water content agree well with previous studies (e.g. Sisson & Grove, 1993a)Go, confirming that plagioclase composition mainly depends on the melt water content and the Ca/Na ratio of the system.

At QFM buffer conditions the residual melt FeO*/MgO ratio generally increases with falling temperature following a tholeiitic differentiation trend. A calc-alkaline differentiation trend is observed at high fO2 (MnO–Mn3O4 buffer), as magnetite crystallizes between 1100°C and 1050°C, independently of bulk water content. However, the crystallization temperature of silicates is depressed with increasing bulk water content. Thus, residual melts of runs with high bulk water contents show a more distinct calc-alkaline differentiation trend, even though the effect is small at these high oxygen fugacities and no change from calc-alkaline to tholeiitic trend can be produced by lowering the water content. This is probably the case in the investigated MORB system at oxygen fugacities relevant to arc magmas (Ni–NiO), as proposed by Sisson & Grove (1993a)Go for calc-alkaline systems, in which the addition of H2O favours a calc-alkaline differentiation trend by early stabilization of Fe–Ti oxides. In addition to fO2 and H2O, which influence melt FeO* evolution by stabilization of Fe–Ti oxides, water controls melt iron content also by the plagioclase/Fe–Mg-silicate ratio in the main crystallization interval.

Phase relations, crystallization sequence and mineral compositions obtained from evolved melt compositions of MORB systems after 50 wt % crystallization are different from the primitive MORB composition. In detail, the liquid lines of descent differ slightly (higher SiO2 contents of melts are reached at identical P, T and aH2O). However, the general compositional trends of residual melts obtained in both compositions are very similar. SiO2-rich residual melts can be obtained under both oxidizing and reducing conditions but at least one fractionation step is required to reach plagiogranitic residual melt compositions.


    ACKNOWLEDGEMENTS
 
We thank Otto Dietrich for preparing the samples, and Bettina Aichinger and Willi Hurkuck for technical assistance. Harald Behrens and Marcus Nowak are thanked for many helpful discussions. Reviews by Othmar Müntener, Fidel Costa, Tom Sisson and Leonid Danyushevsky have significantly improved the manuscript. The authors also thank Colin W. Devey for editorial handling. This study was supported by Deutsche Forschungsgemeinschaft grant (project no. KO 1723/1).


* Corresponding author. Present address: Institut für Mineralogie, Westfälische Wilhelms-Universität Münster, Corrensstrasse 24, D-48149 Münster, Germany. Telephone: +49 (0)251 83 33049. Fax: +49 (0)251 83 38397. E-mail: jberndt{at}uni-muenster.de


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