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School of Engineering and Science - Jacobs University

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Author's personal copy<br />

150 B.W. Alex<strong>and</strong>er et al. / Earth <strong>and</strong> Planetary <strong>Science</strong> Letters 283 (2009) 144–155<br />

REY abundances decrease. However, when comparing samples <strong>of</strong><br />

similar REY content the relative size <strong>of</strong> the anomalies varies. For<br />

example, IF5 possesses a REY distribution <strong>and</strong> positive La <strong>and</strong> Y<br />

anomalies almost identical to samples <strong>of</strong> similar concentration, yet IF5<br />

displays a significantly larger Eu anomaly.<br />

The possibility <strong>of</strong> significant alteration <strong>of</strong> the primary REY distributions<br />

is considered unlikely. Mobility <strong>of</strong> the REY has not been observed<br />

in Archean IFs (Bau, 1993), <strong>and</strong> concentrations <strong>of</strong> REY may vary<br />

considerably between adjacent Fe- <strong>and</strong> Si-rich b<strong>and</strong>s in Archean–<br />

Paleoproterozoic IFs (Bau <strong>and</strong> Dulski, 1992). This behavior is also<br />

observed in samples IF5 <strong>and</strong> IF5a, which were obtained from adjacent<br />

layers in a ~4 cm section <strong>of</strong> drill core <strong>and</strong> yet possess distinct REY<br />

patterns <strong>and</strong> very different REY concentrations (Fig. 3). We emphasize<br />

that the lack <strong>of</strong> significant diagenetic or metamorphic alteration is<br />

further supported by the excellent correlation <strong>of</strong> relatively mobile Rb<br />

compared to highly immobile elements such as Ti <strong>and</strong> Th (Fig. 2).<br />

Similarly to immobile trace elements, Є Nd (2.95 Ga) <strong>of</strong> the IF<br />

samples varies as a function <strong>of</strong> Al content (Fig. 4), with samples containing<br />

more than 0.5% Al 2 O 3 displaying relatively uniform negative<br />

Є Nd (2.95 Ga) between −0.35 <strong>and</strong> −0.66. Samples containing less<br />

than 0.5% Al 2 O 3 are significantly more radiogenic, displaying positive<br />

Є Nd (2.95 Ga) between +0.29 <strong>and</strong> +0.99. The difference between the<br />

two groups <strong>of</strong> Є Nd (2.95 Ga) values exceeds the analytical error <strong>of</strong> the<br />

measurements. The correlation between increasing immobile element<br />

contents (e.g., Al, Th, Zr, Rb, <strong>and</strong> Hf) <strong>and</strong> decreasing Є Nd (t) suggests<br />

that crustal sources contributing detritus to the Pietersburg IF depositional<br />

basin possessed Є Nd (2.95 Ga) <strong>of</strong> approximately −0.5, <strong>and</strong><br />

seawater responsible for precipitating the IF was more radiogenic with<br />

Є Nd (2.95 Ga) similar to or greater than +1.<br />

6. Discussion<br />

6.1. Nature <strong>of</strong> the detrital aluminosilicate source<br />

The higher Al 2 O 3 content (≥1.5%) <strong>of</strong> some IF samples indicates<br />

contamination with detrital aluminosilicates, <strong>and</strong> c<strong>and</strong>idates for a<br />

detrital source(s) to the iron-formation include lithologies in the<br />

simatic basement. Published data from the Eersteling area are primarily<br />

for major elements <strong>and</strong> transition metals, <strong>and</strong> 80 analyses have<br />

characterized metagabbros, metabasalts, amphibolites, serpentinites,<br />

as well as quartz porphyrys (Saager <strong>and</strong> Meyer, 1982; Jones, 1990;<br />

Byron <strong>and</strong> Barton, 1990). Aluminum averaged 9.7% in these samples<br />

<strong>and</strong> only four contained more than 15% Al 2 O 3 (maximum 16.4%),<br />

suggesting that if the aluminosilicate fraction in the iron-formation<br />

was derived from pre-existing simatic basement then 15% Al 2 O 3 is the<br />

likely upper limit for this material, which agrees well with estimates<br />

for Archean mafic rocks (Condie, 1993). The strong correlations<br />

between immobile trace elements <strong>and</strong> Al allows reasonable estimates<br />

to be made regarding the trace metal distribution in the detrital source,<br />

<strong>and</strong> by comparing this estimated distribution with trace element data<br />

from the literature it may be possible to restrict the provenance <strong>of</strong> the<br />

detrital component. Estimated trace metal data (Fig. 5) for the most Alrich<br />

sample (IF7) at higher Al 2 O 3 contents <strong>of</strong> 10–15% match reasonably<br />

well with a mixture <strong>of</strong> Archean felsic volcanics <strong>and</strong> komatiites possessing<br />

compositions as proposed by Condie (1993), <strong>and</strong> komatiites in<br />

the PGB have been described previously (Saager <strong>and</strong> Mayer, 1982).<br />

However, few trace element data exist for PGB mafic rocks, making it<br />

difficult to characterize the nature <strong>of</strong> this aluminosilicate source,<br />

except to state that physical weathering <strong>of</strong> serpentinized material is an<br />

unlikely c<strong>and</strong>idate for any detritus present in the Pietersburg IF.<br />

The relatively high Al 2 O 3 content in some samples (e.g., IF3, IF4, <strong>and</strong><br />

IF7) renders them unsuitable as archives for the marine fluid that<br />

precipitated the Pietersburg IF, but these samples do provide Nd isotopic<br />

information regarding the clastic detrital source during deposition<br />

<strong>of</strong> the IF. Samples with Al 2 O 3 greater than ~0.5% possess very<br />

consistent Є Nd (t) close to −0.5 (Fig. 4), which is considered to reflect<br />

the Nd isotopic composition <strong>of</strong> the detrital aluminosilicate source. Close<br />

examination <strong>of</strong> the Al–Є Nd (t) relationships (Fig. 4) suggeststhattwocomponent<br />

conservative mixing between a detrital aluminosilicate<br />

source <strong>and</strong> the pure chemical precipitate that formed the IFs might<br />

adequately model the Nd isotopic data. However, two-component<br />

mixing models that attempt to account for detrital contamination<br />

Fig. 5. Trace element discrimination diagrams for simatic basement samples from the southwest region <strong>of</strong> the PGB. The grey area in both diagrams represents the range <strong>of</strong> predicted<br />

element concentrations in sample IF7, <strong>and</strong> was calculated from linear regressions <strong>of</strong> the metal contents as a function <strong>of</strong> Al. The lower border <strong>of</strong> the grey area represents 10% Al 2 O 3 <strong>and</strong><br />

the upper border represents 15% Al 2 O 3 , which is a reasonable range for the detrital source (see Section 6). Diagram a contains literature data for possible source lithologies (Jones,<br />

1990; Byron <strong>and</strong> Barton, 1990), <strong>of</strong> which pillow lavas <strong>and</strong> amphibolites are broadly consistent with the predicted distribution pattern. Diagram b shows the distribution patterns for<br />

model Archean komatiites <strong>and</strong> felsic volcanics <strong>of</strong> Condie (1993), a mixture <strong>of</strong> which could reasonably produce the pattern observed in the detrital fraction <strong>of</strong> the iron-formation<br />

samples, <strong>and</strong> komatiites are present within the oldest sections <strong>of</strong> the PGB (Saager <strong>and</strong> Meyer, 1982).

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