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School of Engineering and Science - Jacobs University

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ABSTRACT<br />

The neodymium (Nd) isotopic composition <strong>of</strong> circa three billion-year-old (Ga)<br />

seawater is inferred from studies <strong>of</strong> b<strong>and</strong>ed iron-formations (IF) from South Africa.<br />

Iron-formations from the 2.9 Ga Pongola Supergroup display negative Є Nd values that<br />

are indistinguishable from local shale, suggesting that Nd derived from weathering <strong>of</strong><br />

continental crust dominated the Nd isotopic composition <strong>of</strong> shallow seawater. In<br />

contrast, Є Nd (t) in IF from the 2.95 Ga Pietersburg greenstone belt is clearly<br />

distinguishable from local clastic material, <strong>and</strong> indicates that where Nd was not sourced<br />

from local crust, seawater could possess more radiogenic Є Nd values <strong>of</strong> +1. The<br />

Pietersburg IF Є Nd (t) values are therefore interpreted to represent bulk Archean seawater<br />

not affected by local crustal Nd signatures. This Є Nd value <strong>of</strong> +1 is very similar to<br />

published Є Nd (t) estimates for Archean seawater, when only those IFs which display rare<br />

earth element ratios (REE) common to seawater are considered. Screening the data in<br />

such a manner clearly identifies seawater precipitates, <strong>and</strong> relatively constant Є Nd (t) <strong>of</strong><br />

+1 to +2 for Archean IFs suggest these values are a good average for 2.5-3.8 Ga<br />

seawater.<br />

If bulk Archean seawater typically displayed Є Nd (t) <strong>of</strong> +1, then hydrothermal<br />

alteration <strong>of</strong> mafic oceanic crust is considered the likely process for delivering relatively<br />

radiogenic Nd to seawater. Data from this study <strong>and</strong> previous work suggest significant<br />

high temperature (T) fluid input to seawater between 2.5-3.8 Ga, as supported by<br />

positive Eu anomalies in IFs, <strong>and</strong> the absence <strong>of</strong> negative Ce anomalies in any Archean<br />

IFs indicates that seawater was more reducing than modern seawater. Modern high-T<br />

fluids altering mafic oceanic crust possess both positive Є Nd values <strong>and</strong> Eu anomalies,<br />

<strong>and</strong> it is possible that these reducing, Fe-rich fluids exerted a greater control on Archean<br />

seawater chemistry than is observed today.<br />

However, the negative Є Nd (t) values for the Pongola IF data indicate that locally,<br />

shallow seawater could be isotopically distinct, <strong>and</strong> possess an Nd isotopic signature<br />

identical to local crust. If world seawater was isotopically homogenous with respect to<br />

Nd between 2.9-3.0 Ga, these data indicate a significant shift from positive Є Nd values in<br />

seawater during deposition <strong>of</strong> the Pietersburg IFs, to negative Є Nd values during<br />

deposition <strong>of</strong> the Pongola IFs. This is considered unlikely, <strong>and</strong> the Nd isotopic data are<br />

rather interpreted to reflect that, similar to modern oceans, ~3.0 Ga world oceans were<br />

composed <strong>of</strong> water masses that could be isotopically distinct with respect to Nd.<br />

i

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