Elsevier

Lithos

Volume 152, 1 November 2012, Pages 56-65
Lithos

Trace element geochemistry of nyerereite and gregoryite phenocrysts from natrocarbonatite lava, Oldoinyo Lengai, Tanzania: Implications for magma mixing

https://doi.org/10.1016/j.lithos.2012.01.022Get rights and content

Abstract

The abundances of Li, P, Cl, V, Mn, Rb, Sr, Y, Cs, Ba, Pb, Th, U and REE, within and between, phenocrysts of nyerereite and gregoryite occurring in natrocarbonatite lavas erupted from the active volcano Oldoinyo Lengai (Tanzania) have been determined by electron microprobe, LA-ICP-MS and SIMS. These data show that, in general, nyerereite is enriched in Rb (71–137 ppm), Sr (14,485–23,240 ppm), Y (2.0–8.9 ppm), Cs (1.6–5.3 ppm), Ba (4000–11,510 ppm), but poorer in Li (21–91 ppm), P (820–1900 ppm) and V (5.1–47 ppm) relative to gregoryite (Rb = 43–106; Sr = 4255–7275; Y = 0.3–4.0; Cs = 0.6–5.1; Ba = 1125–7052; Li 84–489; P = 6790–15,860; V = 33–155 ppm). Nyerereite is highly enriched in REE (La = 236–973; Ce = 395–1044 ppm) relative to gregoryite (La = 59–309; Ce = 59–301 ppm). Chondrite normalized REE distribution patterns for nyerereite and gregoryite are parallel and linear with no Eu anomalies. They show extreme enrichment in light REE and depletion in heavy REE (nyerereite La/YbCN = 1759–7079; gregoryite La/YbCN = 1051–10,247). Significant differences exist in the abundances of trace elements within and between coexisting crystals occurring in diverse natrocarbonatite flows, although there do not appear to be any significant secular variations in phenocryst compositions in lavas erupted from a given vent. It is concluded that both major, minor and trace element compositional data for nyerereite and gregoryite phenocrysts occurring in natrocarbonatite lavas are derived by the crystallization of several different batches of magma in a continuously replenished fractionating magma chamber. Natrocarbonatite lavas are considered to be hybrids formed by the mixing of both crystals and melts formed from several batches of natrocarbonatite magma; thus bulk rock compositions cannot represent the compositions of the primary magma composition before the onset of fractionation. Differentiation of natrocarbonatite melts leads to enrichment of residua in Ba and Mg.

Highlights

► Determination of trace elements in nyerereite and gregoryite by LA-ICP-MS. ► Evidence for magma mixing for Oldoinyo Lengai natrocarbonatites. ► Evidence for secular variation in erupted natrocarbonatite.

Introduction

Oldoinyo Lengai, the world's only active carbonatite volcano, lies in the Gregory Rift Valley in northern Tanzania, Eastern Africa (2.764° S, 35.914° E). Various aspects of the geology, petrology, and mineralogy of the natrocarbonatite lavas have been described by Church and Jones (1995), Dawson et al., 1995, Dawson et al., 1996, Keller and Krafft (1990), Mitchell, 1997, Mitchell, 2006, Mitchell and Belton (2004), and Peterson (1990). The lavas exhibit a wide variety of textures reflecting the conditions of eruption and crystal–liquid fractionation during sub-aerial flow (Keller and Krafft, 1990). These can range from phenocryst-dominated vesicular spatter to aphyric cryptocrystalline filter-pressed residua containing skeletal nyerereite. The natrocarbonatites are composed dominantly of gregoryite [(Na,K,Ca)2CO3] and nyerereite [(Na,K)2Ca(CO3)2] phenocrysts set in a matrix of a Na-rich gregoryite-like phase, barian nyerereite, sodian sylvite , fluorite, potassian neighborite, and a Ba–Sr–Mg–Na–Cl–F-rich carbonate formerly known as phase X (Dawson et al., 1995), but now considered to be khanneshite (Mitchell, 2006, Zaitsev et al., 2008).

As of September 2007, the style of activity changed from the quiet effusive eruption of natrocarbonatite lavas to violent pyroclastic eruptions composed initially of hybrid peralkaline nepheline–melilite–combeite–(Na–Ca–phosphate–carbonate) ash and lapilli (Mitchell and Dawson, 2007) and ultimately to ash consisting of diverse combeite wollastonite nephelinites (Keller et al., 2010, Kervyn et al., 2010, Mattsson and Reusser, 2010, Mitchell and Dawson, 2011). Subsequent to the last major pyroclastic silicate eruption in 1967 the volcano remained dormant until 1983. Since July 2008 the volcano has exhibited intermittent minor activity confined to small natrocarbonatite flows at the bottom of an inaccessible deep pit crater. As a consequence of this change in volcanic style, samples of fresh natrocarbonatite lava can no longer be obtained. Hence, conservation and investigations of existing material becomes imperative.

Although the major element compositional variation of the minerals forming natrocarbonatite is relatively well known (Keller and Krafft, 1990, Mitchell and Belton, 2004, Peterson, 1990), there are few data on their minor and trace element contents (Zaitsev et al., 2009). These data are important in understanding the differentiation of carbonate melts, as trace elements which are typically incompatible with respect to phenocrysts in common silicate magmas, are compatible in the phenocrysts of natrocarbonatite. These magmas also are unusual in that differentiation leads to the concentration of Mg in residual melts, resulting in the formation of potassian neighborite and a Na–Mg-carbonate, possibly an eitelite-like phase (Gittins and Jago, 1998, Mitchell and Kjarsgaard, 2011).

An initial investigation by Keller and Spettel (1995) of bulk single samples of each of nyerereite and gregoryite demonstrated that the former is richer in rare earth elements (REE) than the latter. Bulk analysis of gregoryite is not desirable as this mineral typically contains inclusions of nyerereite, ferroan alabandite, and quenched groundmass material. Recently, Mitchell and Kamenetsky (2008) and Zaitsev et al. (2009) using laser ablation ICP-MS have both demonstrated significant differences in the contents of Li, P, V, Mn, Rb, Sr, Y, Cs, Ba and REE and other trace elements within and between nyerereite and gregoryite phenocrysts. Zaitsev et al. (2009) provided only 12 compositions for REE from one sample collected in 2000. In this work we significantly extend these initial data by presenting trace element data obtained on phenocrysts of nyerereite and gregoryite occurring in several natrocarbonatite samples collected between 1996 and 2005. Major element data are also given for Ba-rich nyerereite and khanneshite occurring in the groundmass of the natrocarbonatites that erupted in July 2000.

Section snippets

Analytical techniques

All minerals were identified by back-scattered electron imagery and energy dispersive X-ray spectrometry. Major (Ca, Na, K) and minor (Sr, Ca, P, Cl, S, Mn, Fe) compositions were determined by quantitative energy dispersive X-ray spectrometry using a JEOL-JSM5900 scanning electron microscope equipped with a LINK ISIS 300 analytical system incorporating a Super ATW light element detector (133 eV FwHm MnK). Raw EDS spectra were acquired for 120 s (live time) with an accelerating voltage of 20 kV and

Nyerereite phenocrysts: Sr and Ba compositional variations

Fig. 1 illustrates a typical partially-resorbed nyerereite phenocryst occurring in the 23rd July 2000 natrocarbonatite flow emanating from vent T37B, and shows the locations of the EMP analytical points for the major and minor element contents given in Table 1. The core and margin of this crystal were also analyzed by SIMS (Table 4, anal. 1c and 1r). Table 1 shows that there is very little compositional variation within this crystal with respect to the major elements (Ca, Na, K). Other crystals

Gregoryite phenocrysts: Sr and Ba compositional variation

Table 7 and Fig. 5 demonstrate that gregoryite is poor in Ba and Sr (4255–7275 ppm Sr; 1125–7855 ppm Ba) relative to nyerereite (17,645–25,249 ppm Sr; 4783–11,598 ppm Ba) within and between samples of natrocarbonatite. The Sr variation is relatively limited but is positively correlated with increasing Ba content (Fig. 5). As both Sr and Ba can be expected to substitute for Ca in these carbonates, the lower Sr and Ba contents of gregoryite undoubtedly reflect the lower Ca content of this mineral

Rare earth elements

Table 6, Table 8 show that nyerereites have greater rare earth element (REE) contents than gregoryite. Rims of nyerereite phenocrysts are enriched in REE relative to cores, whereas no trend is evident for the gregoryites. Fig. 6 shows that nyerereite contains greater amounts of Ce than gregoryite. In common with Sr–Ba variations, nyerereite phenocrysts in different flows show particular ranges in REE contents. Apart from phenocrysts in the 2004 flow from T58 there is no correlation between Ce

Alkali elements: Li, Rb, Cs

Li is concentrated in gregoryite, whereas Rb is preferentially concentrated in nyerereite (Fig. 8; Table 4, Table 5, Table 7); a distribution also observed by Zaitsev et al. (2009). There are significant secular variations in abundances; in particular both carbonates from the T58-2000 flow are poor in Li and Rb relative to those in other flows. The enrichment of Rb in nyerereite is unexpected as Rb might be considered to enter preferentially the larger Na-site available in gregoryite. However,

Other trace elements

Table 4 presents data for P2O5, B, F, and Cl determined by SIMS in nyerereite phenocrysts. P2O5 contents range from 0.16 to 1.34 wt.% and are similar to data (0.31–0.72 wt.%) given by Zaitsev et al.(2009). These data are considered not to represent the presence of nanometer-size inclusions of apatite. Boron contents range from 7 to 57 ppm with no systematic core to margin variations evident. There are no previously published data for B in nyerereite. Chlorine contents as determined by SIMS range

Discussion

Our data for trace elements in alkali carbonate phenocrysts clearly shows significant differences in the abundances of trace elements between coexisting crystals occurring in a single natrocarbonatite flow. These differences are unlikely to be related to in situ small scale compositional heterogeneity in the melt as natrocarbonatites have extremely low viscosity (Dawson et al., 1995, Mattsson and Caricchi, 2009) and, unlike silicate melts, cannot sustain such heterogeneity. These observations

Conclusions

We have in this study determined the abundances of Li, B, F, Cl, P, S, V, Mn, Rb, Sr, Y, Cs, Ba, Pb, Th and U and REE within and between nyerereite and gregoryite phenocrysts. Their compositional variation is listed in Table 1, Table 2, Table 3, Table 4, Table 5, Table 6, Table 7, Table 8. Our data show that, in general, nyerereite is enriched in Rb, Sr, Y, Cs, Ba, and REE but poorer in Li, P and V relative to gregoryite.

Individual nyerereite and gregoryite crystals within and between

Acknowledgments

Mitchell's research at Oldoinyo Lengai is supported by the Natural Sciences and Engineering Research Council of Canada and Lakehead University. Kamenetsky is supported by an Australian Research Council Professorial Fellowship and Discovery grant. The assistance of L. Danyushevsky, S. Gilbert, and S. Meffre with the LA-ICP-MS analysis is greatly appreciated. Roger Mitchell and Dima Kamentsky thank the Alexander von Humboldt Stiftung for providing travel and accommodation costs to attend the

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