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School of Engineering and Science - Jacobs University

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

145<br />

However, the exact process <strong>of</strong> IF deposition is unclear, as it implies<br />

contradictory mechanisms in which seawater is reducing enough to<br />

transport large amounts <strong>of</strong> soluble Fe(II), yet oxidizing enough to<br />

episodically precipitate sediments that may contain N90% Fe (measured<br />

as Fe 2 O 3 ). Therefore, at least with respect to the marine Fe cycle,<br />

Archean seawater during IF deposition was clearly distinct from<br />

modern seawater, <strong>and</strong> several studies have attempted to quantify the<br />

importance <strong>of</strong> an Fe-rich hydrothermal flux by examining samarium–<br />

neodymium (Sm–Nd) isotopes in IFs (e.g., Miller <strong>and</strong> O'Nions, 1985;<br />

<strong>Jacobs</strong>en <strong>and</strong> Pimentel-Klose; 1988a, b; Derry <strong>and</strong> <strong>Jacobs</strong>en, 1990;<br />

Alibert <strong>and</strong> McCulloch; 1993; Bau et al., 1997a; Alex<strong>and</strong>er et al., 2008).<br />

This application <strong>of</strong> Sm–Nd isotopes is possible because fractionation<br />

during crustal differentiation produces different Sm/Nd ratios in<br />

oceanic <strong>and</strong> continental crust, resulting in unique 143 Nd/ 144 Nd ratios<br />

in these reservoirs due to the subsequent decay <strong>of</strong> 147 Sm to 143 Nd.<br />

Measured 143 Nd/ 144 Nd ratios are typically expressed using the Є Nd (t)<br />

notation (DePaolo <strong>and</strong> Wasserburg, 1976), which describes the deviation<br />

<strong>of</strong> 143 Nd/ 144 Nd in parts per 10 4 from CHUR (chondritic uniform<br />

reservoir, i.e., bulk silicate Earth) at time t. Continental crust, with a<br />

low Sm/Nd ratio <strong>and</strong> little radiogenic 143 Nd, displays negative Є Nd (t),<br />

whereas oceanic crust derived from a depleted mantle has a higher<br />

Sm/Nd ratio, more radiogenic 143 Nd, <strong>and</strong> positive Є Nd (t) values.<br />

Therefore, Sm–Nd isotope ratios in a sample <strong>of</strong> known age can distinguish<br />

whether Nd has been primarily derived from continental or<br />

oceanic crust.<br />

The purpose <strong>of</strong> this study is to screen IFs for seawater provenance<br />

on the basis <strong>of</strong> REE patterns, <strong>and</strong> then re-evaluate the isotopic evolution<br />

<strong>of</strong> Nd in Archean seawater. Though data between 3.0 <strong>and</strong> 3.5 Ga<br />

are few, it seems that seawater possessed relatively constant Є Nd (t)<strong>of</strong><br />

approximately +1 to +2 from 3.8 Ga until ~2.6 Ga. New Nd isotopic<br />

results for 2.95 Ga IF from the Pietersburg greenstone belt (PGB) in<br />

South Africa support this conclusion, <strong>and</strong> the PGB samples show strong<br />

evidence for mixing between a detrital sediment source with slightly<br />

negative Є Nd (t) <strong>and</strong> ambient seawater with positive Є Nd (t) equal to or<br />

greater than +1. It is concluded that, unlike modern seawater, the<br />

great majority <strong>of</strong> Nd in bulk seawater prior to 2.7 Ga originated from<br />

mantle-derived mafic source rocks. However, comparison <strong>of</strong> the<br />

Pietersburg IF to similarly aged IF from South Africa indicates that<br />

where evolved local continental crust was present this mantle Nd<br />

signal was not discernible in shallow Archean seawater (Alex<strong>and</strong>er<br />

et al., 2008), implying that like modern oceans, the Archean ocean was<br />

not well-mixed with respect to its Nd isotopic composition.<br />

2. Nd in seawater <strong>and</strong> previous IF studies<br />

Seawater in modern oceans possesses negative Є Nd (0) between<br />

−1 <strong>and</strong> −20, though extreme values in this range are restricted to<br />

shallow waters (Frank, 2002; Goldstein <strong>and</strong> Hemming, 2003). There is<br />

no evidence that radiogenic Nd derived from hydrothermal alteration<br />

<strong>of</strong> mid-ocean ridge basalt contributes significantly to modern seawater,<br />

<strong>and</strong> in fact, efficient scavenging <strong>of</strong> REE by precipitating metal<br />

oxides near hydrothermal vent sites is considered to provide an<br />

ultimate sink for REE in seawater (German et al., 1990). As a result,<br />

Nd derived from continental crust dominates world seawater (e.g.,<br />

Piepgras <strong>and</strong> Wasserburg, 1980; Andersson et al., 2008, <strong>and</strong> references<br />

therein). The persistence <strong>of</strong> a ~20 Є Nd -unit variation between ocean<br />

basins indicates that the marine residence time <strong>of</strong> Nd (τ Nd ) is less than<br />

the mixing time <strong>of</strong> the oceans (~1500 yr, e.g., Broecker <strong>and</strong> Peng,<br />

1982), <strong>and</strong> estimates <strong>of</strong> τ Nd in modern oxic seawater based on isotopic<br />

studies typically range from ~500 yr (Tachikawa et al., 2003) to 1000–<br />

2000 yr (Je<strong>and</strong>el et al., 1995;). Temporal variability in seawater Є Nd (t)<br />

has also been noted, <strong>and</strong> Recent (b20 Ka) seawater Nd ratios appear to<br />

have fluctuated by 2–3 Є Nd -units on 1000–5000 yr time scales (e.g.,<br />

Piotrowski et al., 2005; Gutjahr et al., 2008).<br />

Early Nd isotopic studies <strong>of</strong> IFs attempted to constrain the source <strong>of</strong><br />

Fe to coeval seawater, based upon the premise that initial 143 Nd/ 144 Nd<br />

ratios in IFs would indicate if Fe was derived from hydrothermal fluids<br />

originating in ancient oceanic crust, or if the Fe was sourced from<br />

weathering <strong>of</strong> contemporaneous continental crust. However, this<br />

approach is problematic as recently discussed by Alex<strong>and</strong>er et al.<br />

(2008), as the different geochemical behaviors <strong>of</strong> Fe <strong>and</strong> Nd do not<br />

allow definitive statements to be made regarding the Fe source to IF<br />

based upon Nd isotopes.<br />

Regardless <strong>of</strong> the Fe source to IFs, the use <strong>of</strong> Sm–Nd isotopes for<br />

discerning the relative impact <strong>of</strong> oceanic crust-derived hydrothermal<br />

fluxes to Archean seawater should be possible. Neodymium isotopic<br />

data for IFs have varied, with Miller <strong>and</strong> O'Nions (1985) concluding<br />

that continental crust supplied much <strong>of</strong> the Nd to Archean oceans.<br />

However, later studies by <strong>Jacobs</strong>en <strong>and</strong> Pimentel-Klose (1988a, b),<br />

Alibert <strong>and</strong> McCulloch (1993), <strong>and</strong> Bau et al. (1997a) concluded that<br />

contemporaneous seawater Nd was primarily derived from hydrothermal<br />

alteration <strong>of</strong> mafic oceanic crust. A recent study <strong>of</strong> 2.9 Ga IF by<br />

Alex<strong>and</strong>er et al. (2008) indicates that shallow Archean seawater along<br />

cratonic margins was dominated by continentally-derived Nd, similar<br />

to coastal seawater in modern oceans. Whereas early studies have<br />

extrapolated data from relatively small numbers <strong>of</strong> samples <strong>and</strong> locations<br />

to be representative <strong>of</strong> the entire Archean ocean (e.g., Miller <strong>and</strong><br />

O'Nions, 1985; <strong>Jacobs</strong>en <strong>and</strong> Pimentel-Klose, 1988b), the conflicting<br />

interpretations could reflect spatial <strong>and</strong> temporal heterogeneity with<br />

respect to 143 Nd/ 144 Nd ratios in Earth's early oceans. This study<br />

addresses the possibility that Nd isotopic heterogeneity existed in the<br />

Archean ocean, similar to what is observed in modern oceans.<br />

It is necessary to examine the possibility that primary Nd isotopic<br />

signals recorded in IFs may be reset by post-depositional processes;<br />

however, the Sm–Nd isotopic system is resistant to metamorphism<br />

<strong>and</strong> consistent Nd isotopic results are obtained for IFs that have experienced<br />

a wide range <strong>of</strong> metamorphic overprint. Bau et al. (1997a)<br />

reported Sm–Nd data for the stratigraphically equivalent Kuruman<br />

<strong>and</strong> Penge IFs <strong>of</strong> the Transvaal Supergroup in South Africa (Beukes,<br />

1983). Whereas the Kuruman IFs were weakly metamorphosed<br />

(b200 °C) <strong>and</strong> the Penge IFs suffered intense metamorphic overprint<br />

(N500 °C), both IFs yield very similar Sm–Nd isotopic ratios, <strong>and</strong> REE<br />

patterns are indistinguishable between the two. Moreover, 2.5–3.7 Ga<br />

IFs from a number <strong>of</strong> locations <strong>and</strong> with very different metamorphic<br />

histories display remarkably similar, seawater-like REE distributions<br />

(e.g., Alibert <strong>and</strong> McCulloch, 1993; Bolhar et al., 2004), <strong>and</strong> in a<br />

detailed study <strong>of</strong> worldwide IFs Bau (1993) concluded that postdepositional<br />

REE mobility in IFs is negligible.<br />

3. Geologic setting<br />

The Pietersburg greenstone belt outcrops over a 150 km long by<br />

70 km wide area located in northeast South Africa (Fig. 1). The<br />

northeastern portion <strong>of</strong> the PGB consists <strong>of</strong> schists, is bounded by the<br />

Limpopo metamorphic province, <strong>and</strong> experienced the highest degrees<br />

<strong>of</strong> deformation <strong>and</strong> lower to upper amphibolite grade metamorphism<br />

(De Wit et al., 1992). The southwestern portion <strong>of</strong> the belt is<br />

surrounded by igneous intrusives <strong>and</strong> younger cover <strong>of</strong> the Traansvaal<br />

Supergroup, <strong>and</strong> experienced less tectonic deformation <strong>and</strong> lower<br />

degrees <strong>of</strong> metamorphism (De Wit et al., 1992). The PGB contains two<br />

major tectonic units separated by a distinct unconformity, above<br />

which lies the sedimentary Uitkyk Formation (De Wit et al., 1992).<br />

Below the unconformity, the South African Committee for Stratigraphy<br />

(SACS, 1980) recognized five formations, from oldest to youngest,<br />

the Mothiba, Ysterberg, Eersteling, Z<strong>and</strong>rivierspoort, <strong>and</strong> the Vrischgewaagd.<br />

Only the lowermost Mothiba <strong>and</strong> Ysterberg Formations<br />

contain IF. However, De Wit (1991) observed significant structural<br />

repetition in the southwestern portion <strong>of</strong> the PGB, where the IF<br />

samples for this study originated, <strong>and</strong> concluded that a strict<br />

SACS stratigraphy was not applicable. Therefore, we adopt the stratigraphy<br />

<strong>of</strong> De Wit (1991) for this area, which labels all units below<br />

the unconformity as simatic basement, due to the silica-magnesia

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