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School of Engineering and Science - Jacobs University

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Chapter 1. Introduction<br />

1.1. Statement <strong>of</strong> research goal<br />

The research presented in this thesis relates to physical <strong>and</strong> chemical processes<br />

occurring in seawater during the first 2 billion years (2 Ga) <strong>of</strong> Earth’s history, <strong>and</strong><br />

particularly addresses seawater chemistry ca. 3.0 Ga. As samples <strong>of</strong> seawater from this<br />

time period are not available, except perhaps as microscopic fluid inclusions in some<br />

geologic samples, the research fundamentally rests upon archives <strong>of</strong> seawater chemistry<br />

that exist in the rock record. For studies <strong>of</strong> the Archean oceans (ca. 2.5-4.0 Ga) archives<br />

<strong>of</strong> seawater chemistry are limited due to the scarcity <strong>of</strong> the rock record. However,<br />

b<strong>and</strong>ed iron-formations (IFs) are common <strong>and</strong> extensive constituents <strong>of</strong> the Archean<br />

geologic record, <strong>and</strong> the work described here exclusively deals with IFs <strong>and</strong> Fe-rich<br />

sediments associated with IF deposition. Iron-formations were formally defined by<br />

James (1954) as “a chemical sediment, typically thin-bedded or laminated, containing<br />

15 per cent or more iron <strong>of</strong> sedimentary origin, commonly but not necessarily<br />

containing layers <strong>of</strong> chert”. These chemical sediments are clearly <strong>of</strong> marine origin (see<br />

Simonson, 2003, for details), <strong>and</strong> due to their ubiquitous occurrence during the<br />

Archean, IFs are likely one <strong>of</strong> the best seawater archives prior to ~2.7 Ga.<br />

One question regarding Archean oceans is the extent to which seawater chemistry<br />

was controlled by weathering <strong>of</strong> oceanic or continental crust. Different conclusions have<br />

been drawn, with some workers supporting weathering <strong>of</strong> continental crust as a<br />

dominant control on seawater chemistry (e.g., Miller <strong>and</strong> O’Nions, 1985), while others<br />

have supported hydrothermal alteration <strong>of</strong> oceanic crust as a primary control (<strong>Jacobs</strong>en<br />

<strong>and</strong> Pimentel-Klose, 1988a, 1988b; Veizer et al., 1989; Alibert <strong>and</strong> McCulloch, 1993;<br />

Bau et al. 1997a). The research presented here attempts to resolve these discrepant<br />

conclusions through new trace metal <strong>and</strong> isotopic data for ca. 3.0 Ga IFs. A secondary<br />

1

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